'Yellow Star' images and/or videos results page 181 of 5

Type # for projects,to access projects, > for users, and ? for help.

Your ongoing selection

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4572671","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"s_numazawa","item_category5":"not_balown","item_list_name":"search_results","item_name":"artist_s_view_of_the_double_star_epsilon_aurigae_almaaz_binary_star_epsilon_aurigae_artwork_almaaz_i","item_variant":"undefined"},{"item_id":"GBW3246144","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"stanislaw_jacobson_presides_over_the_ghetto_court_lodz_poland_1942_photo","item_variant":"undefined"},{"item_id":"GBW3246121","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hans_biebow_left_chief_of_the_german_nazi_administration_of_the_lodz_ghetto_at_a_street_market_lodz_","item_variant":"undefined"},{"item_id":"PIX4568311","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"open_cluster_ngc_6242_in_scorpio_open_star_cluster_ngc_6242_in_scorpius_this_cluster_is_about_3500_y","item_variant":"undefined"},{"item_id":"NFM315096","item_category":"illustration","item_category2":"undetermined_copyright","item_category3":"standard","item_category4":"english_school_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"chadderton_colour_litho","item_variant":"undefined"},{"item_id":"PIX4610295","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_2997_in_the_pneumatic_machine_spiral_galaxy_ngc_2997_in_antlia_ngc_2997_is_a_spira","item_variant":"undefined"},{"item_id":"PIX4650930","item_category":"illustration","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"august_24_2016_the_three_stars_that_make_up_the_centaur_alpha_system_are_the_closest_stars_to_the_su","item_variant":"undefined"},{"item_id":"PIX4610276","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_2997_in_the_pneumatic_machine_spiral_galaxy_ngc_2997_in_antlia_ngc_2997_is_a_spira","item_variant":"undefined"},{"item_id":"PIX4619447","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_trifide_m20_in_the_constellation_sagittarius_trifid_nebula_m20_in_sagittarius_view_of_the_tri","item_variant":"undefined"},{"item_id":"PIX4619490","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_trifide_m20_in_the_constellation_sagittarius_trifid_nebula_m20_in_sagittarius_view_of_the_tri","item_variant":"undefined"},{"item_id":"GBW3246146","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"material_warehouse_in_the_shoemaking_workshop_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"MEP1266789","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"luca_mozzati","item_category5":"not_balown","item_list_name":"search_results","item_name":"western_ivan_s_vault_in_the_friday_mosque_masijd_i_jami_xii_century_isfahan_iran_mixed_technique","item_variant":"undefined"},{"item_id":"GBW3246138","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jewish_workers_in_the_saddle_workshop_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"PIX4650886","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"august_24_2016_the_three_stars_that_make_up_the_centaur_alpha_system_are_the_closest_stars_to_the_su","item_variant":"undefined"},{"item_id":"PIX4620599","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_7129_in_cephee_nebula_by_reflexion_located_3300_light_years_from_earth_this_nebula_houses","item_variant":"undefined"},{"item_id":"PIX4572374","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"m_carroll","item_category5":"not_balown","item_list_name":"search_results","item_name":"comparison_of_sun_sizes_sirius_and_rigel_size_comparison_sun_sirius_and_rigel_the_sun_yellow_star_at","item_variant":"undefined"},{"item_id":"PIX4573950","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"detection_of_an_exoplanet_transit_method_detection_of_an_exoplanet_transit_method_this_method_of_ind","item_variant":"undefined"},{"item_id":"GBW3246129","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jews_in_the_ghetto_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"GBW3246157","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"two_bearded_jewish_men_in_the_ghetto_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"GBW3246171","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"book_sale_in_the_ghetto_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"PIX4618093","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_m43_in_orion_m43_nebula_in_orion_nebula_m43_ngc_1982_is_part_of_the_great_nebula_of_orion_m42","item_variant":"undefined"},{"item_id":"PIX4620597","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"tom_davis","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_7129_in_cephee_grand_champ_nebula_ngc_7129_in_cepheus_wide_field_nebula_reflexion_located","item_variant":"undefined"},{"item_id":"MEP1266755","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"luca_mozzati","item_category5":"not_balown","item_list_name":"search_results","item_name":"friday_mosque_1349_14th_century_kerman_iran_mosaic","item_variant":"undefined"},{"item_id":"CH1197957","item_category":"illustration","item_category2":"undetermined_copyright","item_category3":"standard","item_category4":"english_school_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"white_star_line_world_famous_liners_colour_lithograph","item_variant":"undefined"},{"item_id":"PIX4564845","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_ngc_6522_in_sagittarius_globular_cluster_ngc_6522_in_sagittarius_this_cluster_of_st","item_variant":"undefined"},{"item_id":"PIX4621322","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebuleuse_barnard_86_open_cluster_ngc_6520_dark_nebula_barnard_86_and_open_cluster_ngc_6520_ngc_6520","item_variant":"undefined"},{"item_id":"PIX4569048","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cluster_of_stars_south_serpent_the_serpens_south_star_cluster_cluster_of_fifty_very_young_stars_35_o","item_variant":"undefined"},{"item_id":"GBW3246135","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_man_selling_goods_in_a_ghetto_street_lodz_poland_1942_photo","item_variant":"undefined"},{"item_id":"PIX4564844","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_clusters_ngc_6522_and_ngc_6528_in_sagittarius_baade_s_window_around_ngc_6522_ngc_6522_right","item_variant":"undefined"},{"item_id":"PIX4618845","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_in_the_nebula_ngc_2467_star_forming_region_ngc_2467_star_formation_in_the_nebula_ngc_","item_variant":"undefined"},{"item_id":"PIX4610442","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_m82_view_in_different_wavelength_galaxy_m82_in_multi_wavelength_composite_of_different_images","item_variant":"undefined"},{"item_id":"PIX4617791","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"orion_nebula_m42_m43_the_great_nebula_in_orion_located_1500_years_light_the_orion_nebula_is_the_clos","item_variant":"undefined"},{"item_id":"PIX4617824","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"orion_nebula_m42_m43_the_great_nebula_in_orion_located_1500_years_light_the_orion_nebula_is_the_clos","item_variant":"undefined"},{"item_id":"PIX4610028","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_2397_galaxy_spiral_ngc_2397_the_galaxy_ngc_2397_is_a_classic_spiral_galaxy_located","item_variant":"undefined"},{"item_id":"PIX4572591","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nova_de_l_eagle_nova_aquilae_artwork_artist_s_view_of_a_nova_a_white_dwarf_star_that_attracts_the_ma","item_variant":"undefined"},{"item_id":"PIX4610013","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_2397_galaxy_spiral_ngc_2397_the_galaxy_ngc_2397_is_a_classic_spiral_galaxy_located","item_variant":"undefined"},{"item_id":"FFF8771881","item_category":"footage","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"glitter_and_colorful_marbleized_liquid_motion_art_2024","item_variant":"undefined"},{"item_id":"KCP395964","item_category":"illustration","item_category2":"in_copyright","item_category3":"premium","item_category4":"campbell_pedersen_kathrine","item_category5":"not_balown","item_list_name":"search_results","item_name":"night_and_day_star_2009_acrylic_on_canvas","item_variant":"undefined"},{"item_id":"PIX4612481","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m83_in_hydra_spiral_galaxy_m83_in_hydra_the_galaxy_m83_ngc_5236_is_located_about_15_mi","item_variant":"undefined"},{"item_id":"PIX4564878","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"around_baade_s_window_around_baade_s_window_stars_field_to_the_center_of_our_galaxy_the_bright_star_","item_variant":"undefined"},{"item_id":"PIX4609189","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"central_region_of_the_spiral_galaxy_ngc_300_in_the_sculptor_nucleus_of_spiral_galaxy_ngc_300_in_scul","item_variant":"undefined"},{"item_id":"PIX4612513","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m83_in_hydra_spiral_galaxy_m83_in_hydra_the_galaxy_m83_ngc_5236_is_located_about_15_mi","item_variant":"undefined"},{"item_id":"PIX4564265","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"blue_stragglers_in_cluster_47_toucan_blue_stragglers_in_globular_cluster_47_tucanae_this_image_obtai","item_variant":"undefined"},{"item_id":"PIX4610385","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_infrared_view_spiral_galaxy_m81_seen_in_infrared_view_obtained_by_spitzer_space_te","item_variant":"undefined"},{"item_id":"PIX4613001","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_6744_in_the_constellation_peacock_spiral_galaxy_ngc_6744_in_pavo_the_galaxy_ngc_67","item_variant":"undefined"},{"item_id":"PIX4594275","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"triangle_constellation_and_andromede_galaxy_constellation_of_triangulum_with_andromeda_galaxy_the_co","item_variant":"undefined"},{"item_id":"PIX4610337","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"jim_misti","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4621422","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebulae_lbn_552_and_cohen_129_nebulae_lbn_552_and_cohen_129_in_cepheus_nebulae_in_the_constellation_","item_variant":"undefined"},{"item_id":"PIX4669608","item_category2":"no_copyright","item_category3":"standard","item_category4":"miller_ron_b_1947","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_end_of_oceans_on_earth_artist_s_view_earth_s_oceans_end_artist_view_when_the_sun_swells_to_becom","item_variant":"undefined"},{"item_id":"FFF8771894","item_category":"footage","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"glitter_and_colorful_marbleized_liquid_motion_art_2024","item_variant":"undefined"},{"item_id":"PIX4570101","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"b_s_fletcher","item_category5":"not_balown","item_list_name":"search_results","item_name":"comete_hyakutake_comet_hyakutake_comete_hyakutake_march_1996_this_is_the_spectacular_comet_hyakutake","item_variant":"undefined"},{"item_id":"PIX4621371","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dark_stars_and_nebulae_in_sagittarius_the_star_clouds_of_sagittarius_star_field_towards_the_center_o","item_variant":"undefined"},{"item_id":"PIX4564866","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_clusters_ngc_6522_and_ngc_6528_in_sagittarius_baade_s_window_around_ngc_6522_ngc_6522_right","item_variant":"undefined"},{"item_id":"PIX4608987","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"andromede_galaxy_m31_infrared_view_the_andromeda_galaxy_seen_in_infrared_this_image_shows_the_differ","item_variant":"undefined"},{"item_id":"CH987012","item_category":"illustration","item_category2":"in_copyright","item_category3":"standard","item_category4":"indiana_robert_1928_2018","item_category5":"not_balown","item_list_name":"search_results","item_name":"one_indiana_square_1970_acrylic_on_canvas","item_variant":"undefined"},{"item_id":"PIX4588148","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"luc_perrot","item_category5":"not_balown","item_list_name":"search_results","item_name":"spica_saturn_and_mars_astral_trio_in_the_sky_of_the_reunion_on_the_left_the_blue_star_spica_from_the","item_variant":"undefined"},{"item_id":"UDK845857","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"leeward_islands_saba_saba_flag_and_dutch_flag_flying_side_by_side","item_variant":"undefined"},{"item_id":"PIX4564266","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_globular_cluster_47_toucan_starfield_in_the_globular_cluster_47_tucanae_ngc_104_the_gl","item_variant":"undefined"},{"item_id":"PIX4564863","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_clusters_ngc_6522_and_ngc_6528_in_sagittarius_baade_s_window_around_ngc_6522_ngc_6522_right","item_variant":"undefined"},{"item_id":"PIX4660037","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"alex_tudorica","item_category5":"not_balown","item_list_name":"search_results","item_name":"huangshan_china_the_huang_mountains_or_huangshan_or_yellow_mountains_or_yellow_mountain_are_a_mounta","item_variant":"undefined"},{"item_id":"FFF8771893","item_category":"footage","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"glitter_and_colorful_marbleized_liquid_motion_art_2024","item_variant":"undefined"},{"item_id":"PIX4564283","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_47_toucan_the_globular_cluster_47_tucanae_ngc_104_the_globular_cluster_47_toucan_or","item_variant":"undefined"},{"item_id":"FFF8770121","item_category":"footage","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"glitter_and_colorful_marbleized_liquid_motion_art_2024","item_variant":"undefined"},{"item_id":"PIX4564306","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_47_toucan_the_globular_cluster_47_tucanae_ngc_104_the_globular_cluster_47_toucan_or","item_variant":"undefined"},{"item_id":"PIX4564310","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_47_toucan_the_globular_cluster_47_tucanae_ngc_104_the_globular_cluster_47_toucan_or","item_variant":"undefined"},{"item_id":"PIX4564335","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_ngc_1806_in_dorado_globular_cluster_ngc_1806_in_dorado_image_of_the_globular_cluste","item_variant":"undefined"},{"item_id":"PIX4594320","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"triangle_constellation_and_andromede_galaxy_constellation_of_triangulum_with_andromeda_galaxy_the_co","item_variant":"undefined"},{"item_id":"PIX4564424","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"centaur_omega_globular_cluster_ngc_5139_omega_centauri_globular_cluster_visible_to_the_naked_eye_in_","item_variant":"undefined"},{"item_id":"PIX4565011","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_m54_in_sagittarius_globular_cluster_m54_in_sagittarius_the_globular_cluster_m54_pho","item_variant":"undefined"},{"item_id":"PIX4610325","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4573338","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanets_around_a_red_dwarf_star_exoplanets_around_a_red_dwarf_star_artist_s_view_of_extrasolar_pl","item_variant":"undefined"},{"item_id":"OSN3916579","item_category":"illustration","item_category2":"in_copyright","item_category3":"premium","item_category4":"osborne_neale","item_category5":"not_balown","item_list_name":"search_results","item_name":"signs_of_the_zodiac_capricorn_pullover_from_a_series_of_fashion_caricatures_one_for_each_sign_of_the","item_variant":"undefined"},{"item_id":"PIX4610379","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4610340","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_seen_by_the_hubble_space_telescope_spiral_galaxy_m81_in_ursa_major_the_spiral_gala","item_variant":"undefined"},{"item_id":"PIX4590674","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"constellations_of_gemels_and_little_dog_constellations_of_gemini_and_canis_minor_constellation_of_ge","item_variant":"undefined"},{"item_id":"GDG492933","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"gerard_degeorge","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_friday_mosque_vault_of_the_east_madrasa_decorative_tilework_detail_photo","item_variant":"undefined"},{"item_id":"RMY8617701","item_category":"illustration","item_category2":"in_copyright","item_category3":"premium","item_category4":"murray_roberta","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_sheriff_2022_digital","item_variant":"undefined"},{"item_id":"FFF8771900","item_category":"footage","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"colorful_marbleized_liquid_motion_art_2024","item_variant":"undefined"},{"item_id":"PIX4564450","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"stars_in_the_globular_cluster_omega_centauri_omega_centauri_seen_by_hubble_space_telescope_located_1","item_variant":"undefined"},{"item_id":"GBW3246161","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jewish_fire_fighters_in_the_ghetto_lodz_poland_1940_photo","item_variant":"undefined"},{"item_id":"ETE4911473","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"simon_trampetter_of_amsterdam_decouts_the_yellow_star_from_the_jacket_of_his_friend_joseph_keller_of","item_variant":"undefined"},{"item_id":"PIX4610335","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4583130","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"visible_crab_nebula_infrared_and_x_the_crab_nebula_m1_the_crab_nebula_is_the_rest_of_a_supernova_tha","item_variant":"undefined"},{"item_id":"PIX4610399","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4610741","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_3521_in_the_lion_spiral_galaxy_ngc_3521_in_leo_ngc_3521_is_a_spiral_galaxy_located","item_variant":"undefined"},{"item_id":"SZT2980722","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jewish_citizen_in_berlin_b_w_photo","item_variant":"undefined"},{"item_id":"PIX4627172","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"le_soleil_vu_by_sdo_on_may_23_2010_the_sun_seen_by_sdo_may_23_2010_le_soleil_vu_en_ultraviolet_by_sd","item_variant":"undefined"},{"item_id":"PIX4623779","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_of_the_red_rectangle_in_the_unicorn_the_red_rectangle_afgl_915_this_planetary_nebul","item_variant":"undefined"},{"item_id":"PIX4569954","item_category":"photo","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"comete_of_halley_halley_s_comet_view_on_april_10_1986","item_variant":"undefined"},{"item_id":"LLM8663608","item_category":"illustration","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"german_school_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"arcs_of_colour_in_the_sky_after_sunset_colour_litho","item_variant":"undefined"}]}}

Type # for projects,to access projects, > for users, and ? for help.

Advanced Search Search Tips

Images of 'Yellow Star' found, 430

«
1
…
2
3
4
…
5
»

Artist's view of the double star Epsilon Aurigae (Almaaz) - Binary star Epsilon Aurigae. Artwork - Almaaz is a binary star with a strange eclipse; it is eclipsed by a gigantic companion for two years. It is believed that this companion could be composed of one or two stars surrounded by a large disc of dust. The visible companion is a yellow supergiant type F, one of the brightest stars in the sky. Epsilon Aurigae (Almaaz) is an eclipsing binary star

Artist's view of the double star Epsilon Aurigae (Almaaz) - Binary star Epsilon Aurigae. Artwork - Almaaz is a binary star with a strange eclipse; it is eclipsed by a gigantic companion for two years. It is believed that this companion could be composed of one or two stars surrounded by a large disc of dust. The visible companion is a yellow supergiant type F, one of the brightest stars in the sky. Epsilon Aurigae (Almaaz) is an eclipsing binary star

S. Numazawa

PIX4572671

Stanislaw Jacobson presides over the ghetto court, Lodz, Poland, 1942 (photo)

Stanislaw Jacobson presides over the ghetto court, Lodz, Poland, 1942 (photo)

GBW3246144

Hans Biebow (left), chief of the German Nazi administration of the Lodz ghetto at a street market, Lodz, Poland, 1942 (photo)

Hans Biebow (left), chief of the German Nazi administration of the Lodz ghetto at a street market, Lodz, Poland, 1942 (photo)

GBW3246121

Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

Open cluster NGC 6242 in Scorpio - Open star cluster NGC 6242 in Scorpius - This cluster is about 3500 years old - light from the Sun and is about 50 million years old. A bright yellow star is in the foreground. This cluster is one of many in the sparkling southern constellation of Scorpius. It is marked by a bright yellow star (spectral type K5) which happens to be in the foreground at a distance of about 1000 light years. The cluster itself is about 3,500 light years from the sun. The cluster is slightly dimmed by foreground dust. This so - called interstellar extinction is common with object close to the Galactic plane. Despite this, it is possible to estimate the age of the cluster by measuring the color and relative brightness of its stars. The age turns out to be about 50 million years, which is quite mature for an open cluster of this type. By now, most of the brightest stars will have turned into supernovae and vanished, leaving this quite modest group to compete with the many

PIX4568311

Chadderton (colour litho)

Chadderton (colour litho)

English School, (20th century)

NFM315096

Spiral galaxy NGC 2997 in the Pneumatic Machine - Spiral galaxy NGC 2997 in Antlia - NGC 2997 is a spiral galaxy distant about 55 million years - light. NGC 2997 seems to be a galaxy seen from the front but in reality is inclined by about 45 degrees. Its arms are home to large star-forming regions while its core is surrounded by much older yellow stars. The disc of NGC 2997 is inclined at about 45 degrees to our line of sight, revealing its internal structure and giving the galaxy an oval appearance. Like most spirals, the galaxy has two prominent spiral arms, which appear to originate in the yellow nucleus, are peppered with bright red blobs of ionised hydrogen which are similar to regions of star formation in our own Milky Way. Within these gas clouds are produced the hot blue stars which generate most of the light in the arms of the galaxy. A much older population of yellowish stars are concentrated around the nucleus. NGC 2997 is located about 55 million light year from us

Spiral galaxy NGC 2997 in the Pneumatic Machine - Spiral galaxy NGC 2997 in Antlia - NGC 2997 is a spiral galaxy distant about 55 million years - light. NGC 2997 seems to be a galaxy seen from the front but in reality is inclined by about 45 degrees. Its arms are home to large star-forming regions while its core is surrounded by much older yellow stars. The disc of NGC 2997 is inclined at about 45 degrees to our line of sight, revealing its internal structure and giving the galaxy an oval appearance. Like most spirals, the galaxy has two prominent spiral arms, which appear to originate in the yellow nucleus, are peppered with bright red blobs of ionised hydrogen which are similar to regions of star formation in our own Milky Way. Within these gas clouds are produced the hot blue stars which generate most of the light in the arms of the galaxy. A much older population of yellowish stars are concentrated around the nucleus. NGC 2997 is located about 55 million light year from us

PIX4610295

August 24, 2016: The three stars that make up the Centaur Alpha system are the closest stars to the Sun. Proxima du Centaur is located at a distance of 4.22 light years from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 light years from the Sun. These two stars are relatively similar to the Sun. Although Proxima of Centauri is distant from the Alpha couple of Centauri, its movement seems to link it to this system and is sometimes called Alpha Centauri C - This image of the sky around the bright star Alpha Centauri AB also shows the much fainter red dwarf star, Proxima Centauri, the closest star to the Solar System. The picture was created from pictures forming part of the Digitized Sky Survey 2. The blue halo around Alpha Centauri AB is an artifact of the photographic process, the star is really pale yellow in colour like the Sun

August 24, 2016: The three stars that make up the Centaur Alpha system are the closest stars to the Sun. Proxima du Centaur is located at a distance of 4.22 light years from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 light years from the Sun. These two stars are relatively similar to the Sun. Although Proxima of Centauri is distant from the Alpha couple of Centauri, its movement seems to link it to this system and is sometimes called Alpha Centauri C - This image of the sky around the bright star Alpha Centauri AB also shows the much fainter red dwarf star, Proxima Centauri, the closest star to the Solar System. The picture was created from pictures forming part of the Digitized Sky Survey 2. The blue halo around Alpha Centauri AB is an artifact of the photographic process, the star is really pale yellow in colour like the Sun

PIX4650930

Spiral galaxy NGC 2997 in the Pneumatic Machine - Spiral galaxy NGC 2997 in Antlia - NGC 2997 is a spiral galaxy distant about 55 million years - light. NGC 2997 seems to be a galaxy seen from the front but in reality is inclined by about 45 degrees. Its arms are home to large star-forming regions while its core is surrounded by much older yellow stars. The disc of NGC 2997 is inclined at about 45 degrees to our line of sight, revealing its internal structure and giving the galaxy an oval appearance. Like most spirals, the galaxy has two prominent spiral arms, which appear to originate in the yellow nucleus, are peppered with bright red blobs of ionised hydrogen which are similar to regions of star formation in our own Milky Way. Within these gas clouds are produced the hot blue stars which generate most of the light in the arms of the galaxy. A much older population of yellowish stars are concentrated around the nucleus. NGC 2997 is located in the southern constellation of Antlia, abo

Spiral galaxy NGC 2997 in the Pneumatic Machine - Spiral galaxy NGC 2997 in Antlia - NGC 2997 is a spiral galaxy distant about 55 million years - light. NGC 2997 seems to be a galaxy seen from the front but in reality is inclined by about 45 degrees. Its arms are home to large star-forming regions while its core is surrounded by much older yellow stars. The disc of NGC 2997 is inclined at about 45 degrees to our line of sight, revealing its internal structure and giving the galaxy an oval appearance. Like most spirals, the galaxy has two prominent spiral arms, which appear to originate in the yellow nucleus, are peppered with bright red blobs of ionised hydrogen which are similar to regions of star formation in our own Milky Way. Within these gas clouds are produced the hot blue stars which generate most of the light in the arms of the galaxy. A much older population of yellowish stars are concentrated around the nucleus. NGC 2997 is located in the southern constellation of Antlia, abo

PIX4610276

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

PIX4619447

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. The spectacular Trifid nebula (Messier 20) is one of the best known in the sky. It is a striking mixture of brilliant red light emitted from excited hydrogen gas and the soft blue glow of a reflection nebula. The blue arises from starlight, scattered by dust particles between the stars. The size of the particles is minute, similar to those of smoke, which also has a bluish hue. However, the scattered light is not a pure blue, and if we see it through a medium that is yellow (i.e. absorbs blue light) some green colouration remains. This effect can be seen in some of the darker parts of the faint reflection nebula that surrounds the Trifid, where partial absorption of light by foreground dust provides a yellow 'filte

PIX4619490

Material warehouse in the shoemaking workshop, Lodz, Poland, 1940 (photo)

Material warehouse in the shoemaking workshop, Lodz, Poland, 1940 (photo)

GBW3246146

Western Ivan's Vault in the Friday Mosque (Masijd-i jami), XII century, Isfahan, Iran (mixed technique)

Western Ivan's Vault in the Friday Mosque (Masijd-i jami), XII century, Isfahan, Iran (mixed technique)

Luca Mozzati

MEP1266789

Jewish workers in the saddle workshop, Lodz, Poland, 1940 (photo)

Jewish workers in the saddle workshop, Lodz, Poland, 1940 (photo)

GBW3246138

August 24, 2016: The three stars that make up the Centaur Alpha system are the closest stars to the Sun. Proxima du Centaur is located at a distance of 4.22 light years from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 light years from the Sun. These two stars are relatively similar to the Sun. Although Proxima of Centauri is distant from the Alpha couple of Centauri, its movement seems to link it to this system and is sometimes called Alpha Centauri C - This image of the sky around the bright star Alpha Centauri AB also shows the much fainter red dwarf star, Proxima Centauri, the closest star to the Solar System. The picture was created from pictures forming part of the Digitized Sky Survey 2. The blue halo around Alpha Centauri AB is an artifact of the photographic process, the star is really pale yellow in colour like the Sun. Proxima Centauri appears as a faint red star towards the lower-right of the picture

August 24, 2016: The three stars that make up the Centaur Alpha system are the closest stars to the Sun. Proxima du Centaur is located at a distance of 4.22 light years from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 light years from the Sun. These two stars are relatively similar to the Sun. Although Proxima of Centauri is distant from the Alpha couple of Centauri, its movement seems to link it to this system and is sometimes called Alpha Centauri C - This image of the sky around the bright star Alpha Centauri AB also shows the much fainter red dwarf star, Proxima Centauri, the closest star to the Solar System. The picture was created from pictures forming part of the Digitized Sky Survey 2. The blue halo around Alpha Centauri AB is an artifact of the photographic process, the star is really pale yellow in colour like the Sun. Proxima Centauri appears as a faint red star towards the lower-right of the picture

PIX4650886

Nebula NGC 7129 in Cephee: Nebula by reflexion located 3300 light years from Earth. This nebula houses very young stars, aged less than a million years old. - NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN497. Also conspicuous in the field are several bright Herbig-Haro objects, the signatures of young stellar objects soon to emerge in the main sequence. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B-type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity

Nebula NGC 7129 in Cephee: Nebula by reflexion located 3300 light years from Earth. This nebula houses very young stars, aged less than a million years old. - NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN497. Also conspicuous in the field are several bright Herbig-Haro objects, the signatures of young stellar objects soon to emerge in the main sequence. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B-type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity

PIX4620599

Comparison of Sun Sizes, Sirius and Rigel - Size comparison: Sun, Sirius and Rigel - The Sun (yellow star at the top), and the star Sirius A, (the brightest star in the sky) compared to the huge star Rigel, a supergeant blue star in the constellation of Orion. The brightest star in Earth's sky, Sirius, is seen here next to our Sun and the blue giant Rigel. Sirius has a small companion star, Sirius B. Rigel forms the left foot in the constellation Orion, and its light is equal to 40,000 suns

Comparison of Sun Sizes, Sirius and Rigel - Size comparison: Sun, Sirius and Rigel - The Sun (yellow star at the top), and the star Sirius A, (the brightest star in the sky) compared to the huge star Rigel, a supergeant blue star in the constellation of Orion. The brightest star in Earth's sky, Sirius, is seen here next to our Sun and the blue giant Rigel. Sirius has a small companion star, Sirius B. Rigel forms the left foot in the constellation Orion, and its light is equal to 40,000 suns

M. Carroll

PIX4572374

Detection of an exoplanet: transit method - Detection of an exoplanet: transit method - This method of indirect detection is based on the study of star luminosite (yellow line). If the latter varies periodically, it may indicate the passage of a planet in front of its star. If a planet crosses in front of its star, then the observed brightness of the star (yellow line) is modified

Detection of an exoplanet: transit method - Detection of an exoplanet: transit method - This method of indirect detection is based on the study of star luminosite (yellow line). If the latter varies periodically, it may indicate the passage of a planet in front of its star. If a planet crosses in front of its star, then the observed brightness of the star (yellow line) is modified

PIX4573950

Jews in the Ghetto, Lodz, Poland, 1940 (photo)

Jews in the Ghetto, Lodz, Poland, 1940 (photo)

GBW3246129

Two bearded Jewish men in the ghetto, Lodz, Poland, 1940 (photo)

Two bearded Jewish men in the ghetto, Lodz, Poland, 1940 (photo)

GBW3246157

Book sale in the ghetto, Lodz, Poland, 1940 (photo)

Book sale in the ghetto, Lodz, Poland, 1940 (photo)

GBW3246171

Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger st

Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger st

PIX4618093

Nebula NGC 7129 in Cephee - Grand Champ - Nebula NGC 7129 in Cepheus - Wide field - Nebula reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN 497. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B - type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity

Nebula NGC 7129 in Cephee - Grand Champ - Nebula NGC 7129 in Cepheus - Wide field - Nebula reflexion located 3300 years - light of the Earth. This nebula houses very young stars, aged less than a million years old. NGC 7129 is a young compact star forming region which displays an unusual patchwork of colorful nebulosity and bright stars contrasted against the dust clouds of the Milky Way. NGC 7129 contains several bright reflection nebulae including the large blue reflection cloud NGC 7133 and the unusual small yellow reflection cloud LBN 497. The dominant blue reflection nebula, NGC 7133 is illuminated by two young B - type stars BD+65* 1637 and BD+65* 1638. Both stars are less than one million years old and represent the core of NGC 7129, a small cluster of low mass stars which populate the 36 light year wide cavity

Tom Davis

PIX4620597

Friday Mosque, 1349, 14th century, Kerman, Iran (mosaic)

Friday Mosque, 1349, 14th century, Kerman, Iran (mosaic)

Luca Mozzati

MEP1266755

White Star Line, World Famous Liners, (colour lithograph)

White Star Line, World Famous Liners, (colour lithograph)

English School, (20th century)

CH1197957

Globular cluster NGC 6522 in Sagittarius - Globular cluster NGC 6522 in Sagittarius - This cluster of stars is located about 25,000 years - light from Earth towards the center of our galaxy

Globular cluster NGC 6522 in Sagittarius - Globular cluster NGC 6522 in Sagittarius - This cluster of stars is located about 25,000 years - light from Earth towards the center of our galaxy

PIX4564845

Nebuleuse Barnard 86 & open cluster NGC 6520 - Dark nebula Barnard 86 and open cluster NGC 6520 - NGC 6520, in the center of the image, is a cluster of young stars, aged a few million years. To its right is the dark nebula, Barnard 86, a cloud of molecular gas and dust, very cold, in which stars form. In the background, the billions of years old stars of Sagittarius. NGC 6520 is a young star cluster formed only millions of years ago. Besides, the dark nebula Barnard 86, a molecular cloud, very cold, from which the stars of NGC 6520 surely formed. All around them, oldest stars, which are billions of years old, form the star clouds of Sagittarius in the southern Milky Way and are in orbit around the inner part of the Galaxy. They are cool and yellow

Nebuleuse Barnard 86 & open cluster NGC 6520 - Dark nebula Barnard 86 and open cluster NGC 6520 - NGC 6520, in the center of the image, is a cluster of young stars, aged a few million years. To its right is the dark nebula, Barnard 86, a cloud of molecular gas and dust, very cold, in which stars form. In the background, the billions of years old stars of Sagittarius. NGC 6520 is a young star cluster formed only millions of years ago. Besides, the dark nebula Barnard 86, a molecular cloud, very cold, from which the stars of NGC 6520 surely formed. All around them, oldest stars, which are billions of years old, form the star clouds of Sagittarius in the southern Milky Way and are in orbit around the inner part of the Galaxy. They are cool and yellow

PIX4621322

Cluster of stars South Serpent - The Serpens South star cluster - Cluster of fifty very young stars (35 of which are still only proto - stars, stars in formation) observed by the Spitzer space telescope on 27 October 2006 in the constellation of the Serpent. Located only 848 years from Earth, this cluster of stars is completely masked by interstellar dust and is only revealed in infrared light. Red filaments in the background are organic molecules, PAH (aromatic polycyclic hydrocarbons composed of carbon atoms and hydrogen. In this image, Nasa's Spitzer Space Telescope spots the Serpens South star cluster, which consists of a relatively dense group of 50 young stars - - 35 of which are protostars, or stellar infants, that are just beginning to form. Stellar members of Serpens South star cluster can be seen as the green, yellow, and orange tinted specks sitting atop the black dust lane running down the center of the image. Like raindrops, stars form when thick patches of cosmic clouds c

Cluster of stars South Serpent - The Serpens South star cluster - Cluster of fifty very young stars (35 of which are still only proto - stars, stars in formation) observed by the Spitzer space telescope on 27 October 2006 in the constellation of the Serpent. Located only 848 years from Earth, this cluster of stars is completely masked by interstellar dust and is only revealed in infrared light. Red filaments in the background are organic molecules, PAH (aromatic polycyclic hydrocarbons composed of carbon atoms and hydrogen. In this image, Nasa's Spitzer Space Telescope spots the Serpens South star cluster, which consists of a relatively dense group of 50 young stars - - 35 of which are protostars, or stellar infants, that are just beginning to form. Stellar members of Serpens South star cluster can be seen as the green, yellow, and orange tinted specks sitting atop the black dust lane running down the center of the image. Like raindrops, stars form when thick patches of cosmic clouds c

PIX4569048

A man selling goods in a ghetto street, Lodz, Poland, 1942 (photo)

A man selling goods in a ghetto street, Lodz, Poland, 1942 (photo)

GBW3246135

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window, around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window, around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564844

Star formation in the nebula NGC 2467 - Star - forming region NGC 2467 - Star formation in the nebula NGC 2467, located approximately 17,000 years ago - light from Earth in the southern constellation of Stern. Image obtained by the Hubble Space Telescope in 2004. A colourful star - forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas - - mostly hydrogen - - that serves as an incubator for new stars. It is located about 17,000 light years away in the southern constellation of Puppis. This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys through three different filters (F550M, F6

Star formation in the nebula NGC 2467 - Star - forming region NGC 2467 - Star formation in the nebula NGC 2467, located approximately 17,000 years ago - light from Earth in the southern constellation of Stern. Image obtained by the Hubble Space Telescope in 2004. A colourful star - forming region is featured in this stunning new NASA/ESA Hubble Space Telescope image of NGC 2467. Looking like a roiling cauldron of some exotic cosmic brew, huge clouds of gas and dust are sprinkled with bright blue, hot young stars. Strangely shaped dust clouds, resembling spilled liquids, are silhouetted against a colourful background of glowing. Like the familiar Orion Nebula, NGC 2467 is a huge cloud of gas - - mostly hydrogen - - that serves as an incubator for new stars. It is located about 17,000 light years away in the southern constellation of Puppis. This picture was created from images taken with the Wide Field Channel of the Advanced Camera for Surveys through three different filters (F550M, F6

PIX4618845

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

Galaxy M82 view in different wavelength - Galaxy M82 in multi - wavelength - Composite of different images: in blue the image obtained by Chandra in X-rays, in red the infrared image obtained by Spitzer, in yellow, orange, green, the image of Hubble. M82 is an irregular galaxy distant about 12 million years - light from Earth. Its nucleus, which appears to have suffered from the passage of the neighbouring galaxy M81, is in a phase of violent star activity. Its central regions are rich in star formation. These hot stars blow a stellar wind that becomes a very violent galactic wind. Composite of multi - wavelength images of the active galaxy M82 from the three Great Observatories. X - ray data recorded by Chandra appears here in blue; infrared light recorded by Spitzer appears in red; Hubble's observations of hydrogen emission appears in orange, and the bluest visible light appears in yellow - green. Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange

PIX4610442

Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light fr

Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light fr

PIX4617791

Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light fr

Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained from the 2.2 meter MPG/ESO telescope of the La Silla Observatory. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun. This new image of the Orion Nebula was captured using the Wide Field Imager camera on the MPG/ESO 2.2 - metre telescope at the La Silla Observatory, Chile. This image is a composite of several exposures taken through a total of five different filters. Light that passed through a red filter, as well as light fr

PIX4617824

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its eclat was decreasing (box). Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its br

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its eclat was decreasing (box). Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its br

PIX4610028

Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star

Nova de l'Eagle - Nova Aquilae. Artwork - Artist's view of a nova, a white dwarf star that attracts the material of a companion star at the end of life, a red giant, and compresses these gases and then unleash a nuclear fusion reaction releasing a huge amount of energy in the form of a brief, extremely bright light. Here the artist showed the binary system just before the explosion of the nova. The artist's illustration depicts a classical nova binary system just before an explosion on the surface of the white dwarf. Classical novas occur in a system where a white dwarf closely orbits a normal, companion star. In this illustration, gas is flowing from the large red, companion star into a disk and then onto the white dwarf that is hidden inside the white area. As the gas flows ever closer to the white dwarf, it gets increasingly hotter, as indicated by the change in colors from yellow to white. When the explosion occurs, it engulfs the disk of gas and the red companion star

PIX4572591

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

PIX4610013

Glitter and Colorful Marbleized Liquid Motion Art, 2024

Glitter and Colorful Marbleized Liquid Motion Art, 2024

FFF8771881

Night and Day Star, 2009 (acrylic on canvas)

premium — Night and Day Star, 2009 (acrylic on canvas)

Night and Day Star, 2009 (acrylic on canvas)

Campbell Pedersen, Kathrine

KCP395964

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

PIX4612481

Around Baade's window - Around Baade's window - Stars field to the center of our galaxy. The bright star at the bottom of the image is Gamma of Sagittarius. The globular cluster in the center of the image is NGC 6522. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The German - American astronomer Walter Baade selected for study a region of the crowded star fields in Sagittarius where he believed the Galactic dust obscuration was both uniform and minimal. He used this line of sight to establish the distance of the unseen Galactic centre, using variable stars as his yardstick. He found it to be about 30,000 light years away. This part of the sky, around the globular cluster NGC 6522, is now known as Baade's window. The brightest star in the photograph is gamma Sagittarii, a deep yellow, naked eye star of about third magnitude. It is in the foreground at a distance of about 100 light years

Around Baade's window - Around Baade's window - Stars field to the center of our galaxy. The bright star at the bottom of the image is Gamma of Sagittarius. The globular cluster in the center of the image is NGC 6522. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. The German - American astronomer Walter Baade selected for study a region of the crowded star fields in Sagittarius where he believed the Galactic dust obscuration was both uniform and minimal. He used this line of sight to establish the distance of the unseen Galactic centre, using variable stars as his yardstick. He found it to be about 30,000 light years away. This part of the sky, around the globular cluster NGC 6522, is now known as Baade's window. The brightest star in the photograph is gamma Sagittarii, a deep yellow, naked eye star of about third magnitude. It is in the foreground at a distance of about 100 light years

PIX4564878

Central region of the spiral galaxy NGC 300 in the Sculptor - Nucleus of spiral galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. The photo taken by Siding Spring's 3.9m telescope highlights the nucleus of this galaxy. At the centre of the spiral arms of NGC 300 is an unusually compact, star - like nucleus. It is surrounded by a faint but extensive yellow haze, consisting of millions of faint, cool stars. This is the older population, or 'bulge' of NGC 300, a distant equivalent to the (much more numerous) stars that we see in our own galaxy as the brightest part of the Milky Way in Sagittarius

Central region of the spiral galaxy NGC 300 in the Sculptor - Nucleus of spiral galaxy NGC 300 in Sculptor - Located about 7 million years ago - light from Earth, the spiral galaxy NGC 300 belongs to the Sculptor's group. The photo taken by Siding Spring's 3.9m telescope highlights the nucleus of this galaxy. At the centre of the spiral arms of NGC 300 is an unusually compact, star - like nucleus. It is surrounded by a faint but extensive yellow haze, consisting of millions of faint, cool stars. This is the older population, or 'bulge' of NGC 300, a distant equivalent to the (much more numerous) stars that we see in our own galaxy as the brightest part of the Milky Way in Sagittarius

PIX4609189

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained from the 3.9m telescope of Siding Spring, Australia. M83 is thought to be very like our own Galaxy, the Milky Way, but seen from above one of its poles and at a distance of about 15 million light years. Composed of billions of stars and huge clouds of dust and gas, this object is one of the finest examples of a spiral galaxy and shows a concentration of older, yellow stars in its central nucleus with younger, blue stars and patchy red clouds of glowing gas and dark dust lanes in the trailing spiral arms. The massive blue stars occasionally explode as supernovae; at least eight have been seen in Messier 83 in the last 70 years

PIX4612513

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

Blue stragglers in cluster 47 Toucan - Blue stragglers in globular cluster 47 Tucanae - This image obtained by the Hubble space telescope shows a detail of the 47 Toucan cluster near its center (the field is indicated on the left image taken from the ground). The yellow circles on the right image indicate the position of stars identified by the telescope as blue trainers. Because of the high density of stars within a globular cluster, a collision between two stars sometimes occurs, merging into a single young, bright and warm star called a blue straggler. The core of globular cluster 47 Tucanae is home to many blue stragglers, rejuvenated stars that glow with the blue light of young stars. A ground - based telescope image (on the left) shows the entire crowded core of 47 Tucanae, located 15,000 light - years away in the constellation Tucana. Peering into the heart of the globular cluster's bright core, the Hubble Space Telescope's Wide Field and Planetary Camera 2 separated the dense c

PIX4564265

Spiral galaxy M81 infrared view - Spiral galaxy M81 seen in infrared - View obtained by Spitzer space telescope in different wavelengths. In infrared, Spitzer sees dust rather than stars, thus improving our understanding of star formation. The M81 spiral galaxy is located 12 million light years away from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. Located in the northern constellation of Ursa Major (which also includes the Big Dipper), this galaxy is easily visible through binoculars or a small telescope. M81 is located at a distance of 12 million light - years. These infrared images were obtained by Spitzer's infrared array camera. At these wavelengths, Spitzer sees the dust, rather than the stars, within the disc of silicates and carbonaceous grains. It is well - mixed with gas, which is best seen at radio wavelengths, to form the essential ingredients for future star formation

Spiral galaxy M81 infrared view - Spiral galaxy M81 seen in infrared - View obtained by Spitzer space telescope in different wavelengths. In infrared, Spitzer sees dust rather than stars, thus improving our understanding of star formation. The M81 spiral galaxy is located 12 million light years away from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. Located in the northern constellation of Ursa Major (which also includes the Big Dipper), this galaxy is easily visible through binoculars or a small telescope. M81 is located at a distance of 12 million light - years. These infrared images were obtained by Spitzer's infrared array camera. At these wavelengths, Spitzer sees the dust, rather than the stars, within the disc of silicates and carbonaceous grains. It is well - mixed with gas, which is best seen at radio wavelengths, to form the essential ingredients for future star formation

PIX4610385

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 30 million years away - light from Earth. This galaxy is very similar to our galaxy, the lactee path. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This picture of the nearby galaxy NGC 6744 was taken with the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla. The large spiral galaxy is similar to the Milky Way, making this image look like a picture postcard of our own galaxy sent from extragalactic space. The picture was created from exposures taken through four different filters that passed blue, yellow - green, red light, and the glow coming from hydrogen gas. These are shown in this picture as blue, green, orange and red, respectively

Spiral galaxy NGC 6744 in the constellation Peacock - Spiral galaxy NGC 6744 in Pavo - The galaxy NGC 6744 is about 30 million years away - light from Earth. This galaxy is very similar to our galaxy, the lactee path. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This picture of the nearby galaxy NGC 6744 was taken with the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla. The large spiral galaxy is similar to the Milky Way, making this image look like a picture postcard of our own galaxy sent from extragalactic space. The picture was created from exposures taken through four different filters that passed blue, yellow - green, red light, and the glow coming from hydrogen gas. These are shown in this picture as blue, green, orange and red, respectively

PIX4613001

Triangle Constellation and Andromede Galaxy - Constellation of Triangulum with Andromeda galaxy - The constellation Triangle is a small constellation in the northern hemisphere, not far from the Andromede galaxy. Triangulum is one of the 48 constellations noted by Ptolemy and is one of the smallest of the modern star groupings codified in the 1930s. However, the most obvious triangle in this image joins the surrounding trio of yellow - orange stars, Almak, Mirach and Hamal, in which Triangulum is nicely placed. Of course almost any three stars can form a triangle but these two, one inside the other, make quite a distinctive asterism

Triangle Constellation and Andromede Galaxy - Constellation of Triangulum with Andromeda galaxy - The constellation Triangle is a small constellation in the northern hemisphere, not far from the Andromede galaxy. Triangulum is one of the 48 constellations noted by Ptolemy and is one of the smallest of the modern star groupings codified in the 1930s. However, the most obvious triangle in this image joins the surrounding trio of yellow - orange stars, Almak, Mirach and Hamal, in which Triangulum is nicely placed. Of course almost any three stars can form a triangle but these two, one inside the other, make quite a distinctive asterism

PIX4594275

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. A black hole resides in the center of the galaxy. The M81 galaxy is about 12 million light - years away. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The galaxy's central bulge contains much older, redder stars. It is significantly larger than the Milky Way's bulge. A black hole of 70 million solar masses resides at the center of M81. The black hole is about 15 times the mass of the Milky Way's black hole

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. A black hole resides in the center of the galaxy. The M81 galaxy is about 12 million light - years away. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The galaxy's central bulge contains much older, redder stars. It is significantly larger than the Milky Way's bulge. A black hole of 70 million solar masses resides at the center of M81. The black hole is about 15 times the mass of the Milky Way's black hole

Jim Misti

PIX4610337

Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center

Nebulae LBN 552 and Cohen 129 - Nebulae LBN 552 and Cohen 129 in Cepheus - Nebulae in the constellation Cephee. This region in Cepheus does offer delicate reflection nebulae that have been cataloged by Beverly T. Lynds, University of Arizona, in 1965. This catalog was made from studying the red and blue plates taken by the 48 - inch Palomar Sky Survey. Cohen 129 is the small yellow nebula just slightly up of center

PIX4621422

The End of Oceans on Earth - Artist's View - Earth's oceans end - Artist view: When the Sun swells to become a giant yellow star, the heat on Earth will evaporate the oceans. As the sun gets older, it begins to swell. As it enters the yellow giant stage, the earth becomes so warm that the oceans dry up

The End of Oceans on Earth - Artist's View - Earth's oceans end - Artist view: When the Sun swells to become a giant yellow star, the heat on Earth will evaporate the oceans. As the sun gets older, it begins to swell. As it enters the yellow giant stage, the earth becomes so warm that the oceans dry up

Miller, Ron (b.1947)

PIX4669608

Glitter and Colorful Marbleized Liquid Motion Art, 2024

Glitter and Colorful Marbleized Liquid Motion Art, 2024

FFF8771894

Comete Hyakutake - Comet Hyakutake - Comete Hyakutake March 1996. This is the spectacular Comet Hyakutake as it passed closest to Earth in March of 1996. The solid portion or nucleus of a comet is made up of ice, frozen gases, dust and small rock. And it is relatively small - less than 15 miles in diameter. As its orbit takes it closer to the sun, this frozen mass begins to melt and a coma, which is a gaseous cloud, develops around the nucleus. This coma can grow to be tens of thousands of miles in diameter. Finally a tail also develops which can become millions of miles long. This color photo reveals the blue - green glow around the coma, the yellow - red shroud of a dust tail, and the many long blue streamers of the ion tail

Comete Hyakutake - Comet Hyakutake - Comete Hyakutake March 1996. This is the spectacular Comet Hyakutake as it passed closest to Earth in March of 1996. The solid portion or nucleus of a comet is made up of ice, frozen gases, dust and small rock. And it is relatively small - less than 15 miles in diameter. As its orbit takes it closer to the sun, this frozen mass begins to melt and a coma, which is a gaseous cloud, develops around the nucleus. This coma can grow to be tens of thousands of miles in diameter. Finally a tail also develops which can become millions of miles long. This color photo reveals the blue - green glow around the coma, the yellow - red shroud of a dust tail, and the many long blue streamers of the ion tail

B&S.Fletcher

PIX4570101

Dark Stars and Nebulae in Sagittarius - The Star Clouds of Sagittarius - Star Field towards the center of our galaxy. The bright star towards the center of the image is Gamma of Sagittarius. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Orbiting round the centre of our Galaxy are found huge numbers of stars which are mostly faint, cool and often billions of years old. They are as ancient as the Galaxy itself. These stars are seen with the unaided eye as the hazy star clouds of the southern Milky Way, especially rich in Sagittarius. Our line of sight in this direction is strongly affected by dust, which reveals itself by both dimming the starlight passing through it and by selectively removing the blue light, changing the apparent colour to a deeper yellow. Though the colour change is only seen in photographs such as this, the dustiness of the Milky Way is obvious to the unaided eye. Near the centre of the picture is a region known as Baade's Window after the astro

Dark Stars and Nebulae in Sagittarius - The Star Clouds of Sagittarius - Star Field towards the center of our galaxy. The bright star towards the center of the image is Gamma of Sagittarius. Image obtained from the 1.2m Schmidt UK telescope of Siding Spring. Orbiting round the centre of our Galaxy are found huge numbers of stars which are mostly faint, cool and often billions of years old. They are as ancient as the Galaxy itself. These stars are seen with the unaided eye as the hazy star clouds of the southern Milky Way, especially rich in Sagittarius. Our line of sight in this direction is strongly affected by dust, which reveals itself by both dimming the starlight passing through it and by selectively removing the blue light, changing the apparent colour to a deeper yellow. Though the colour change is only seen in photographs such as this, the dustiness of the Milky Way is obvious to the unaided eye. Near the centre of the picture is a region known as Baade's Window after the astro

PIX4621371

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564866

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

Andromede Galaxy (M31) infrared view - The Andromeda galaxy seen in infrared - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, yellow and red). This image obtained by the WISE satellite also distinguishes the two Andromede satellite galaxies, M32 (above the nucleus of the Andromede galaxy) and NGC 205 (M110) below. Infrared composite at the following wavelengths: 3.4 and 4.6 microns (blue), 12 microns (green), and 22 microns dust sensitive, red. M31, is captured in full in this new image from Nasa's Wide - field Infrared Survey Explorer, or WISE. The mosaic covers an area equivalent to more than 100 full moons, or five degrees across the sky. WISE used all four of its infrared detectors to capture this picture (3.4 - and 4.6 - micron light is colored blue; 12 - micron light is green; and 22 - micron light is red). Blue highlights mature stars, while yellow and red show dust heated

PIX4608987

One Indiana Square, 1970 (acrylic on canvas)

One Indiana Square, 1970 (acrylic on canvas)

Indiana, Robert (1928-2018)

CH987012

Spica Saturn and Mars - Astral trio in the sky of the Reunion On the left, the blue star Spica (from the constellation of the Virgin), on his right Saturn (yellowish) and below Mars (reddish). August 9, 2012 Trio in the sky of Reunion Island At left, the blue star Spica (in Virgo), Saturn to its right (yellow) and below Mars (reddish). August 9 2012

Spica Saturn and Mars - Astral trio in the sky of the Reunion On the left, the blue star Spica (from the constellation of the Virgin), on his right Saturn (yellowish) and below Mars (reddish). August 9, 2012 Trio in the sky of Reunion Island At left, the blue star Spica (in Virgo), Saturn to its right (yellow) and below Mars (reddish). August 9 2012

Luc Perrot

PIX4588148

Leeward Islands, Saba, Saba flag and Dutch flag flying side by side

Leeward Islands, Saba, Saba flag and Dutch flag flying side by side

UDK845857

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

Globular clusters NGC 6522 and NGC 6528 in Sagittarius - Baade's Window around NGC 6522 - NGC 6522 (right) and NGC 6528 (left) are two clusters located about 25,000 years ago - light from Earth towards the center of our galaxy

PIX4564863

Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Huangshan - China: The Huang Mountains (or Huangshan or Yellow Mountains or Yellow Mountain) are a mountainous massif in Anui meridional, eastern province of China. The region is known for its beauty, which is based on the shape of granite peaks, the tormented coniferes, and the clouds that frequently surround the massif. 15 December 2016. Huangshan is a mountain range in southern Anui province in eastern China. The area is well known for its scenery, sunsets, peculiarly-shaped granite peaks, Huangshan pine trees, hot springs, winter snow, and views of the clouds from above. December 15 2016

Alex Tudorica

PIX4660037

Glitter and Colorful Marbleized Liquid Motion Art, 2024

Glitter and Colorful Marbleized Liquid Motion Art, 2024

FFF8771893

Globular cluster 47 Toucan - The globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clus

Globular cluster 47 Toucan - The globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clus

PIX4564283

Glitter and Colorful Marbleized Liquid Motion Art, 2024

Glitter and Colorful Marbleized Liquid Motion Art, 2024

FFF8770121

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

PIX4564306

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the oldest stars known today. Image obtained from the 3.9m telescope of Siding Spring, Australia. Among the many spectacular objects in the southern skies are two magnificent naked - eye globular clusters, omega Centauri and 47 Tucanae. These ancient cities of stars are captives of the Milky Way but were formed long before our Galaxy assumed its present shape, indeed these clusters have some of the oldest known stars. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies. The crowded central region leads to occasional stellar encounters and it is in 47 Tuc that rapidly - spinning pulsars have been discovered by radio astronomers. Although the light of globular clust

PIX4564310

Globular cluster NGC 1806 in Dorado - Globular cluster NGC 1806 in Dorado - Image of the globular cluster NGC 1806 located in the southern constellation of Dorado. NGC 1806 belongs to the galaxy of the Great Magellan Cloud, a galaxy adjacent to our lactee path. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has turned its sharp eye towards a tight collection of stars, first seen 174 years ago. The result is a sparkling image of NGC 1806, tens of thousands of stars gravitationally bound into a rich cluster. Commonly called globular clusters, most of these objects are very old, having formed in the distant past when the Universe was only a fraction of its current age. NGC 1806 lies within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. It can be observed within the constellation of Dorado (the dolphin - fish), an area of the sky best seen from the Earth's southern hemisphere. NGC 1806 was discovered in 1836 by the British astr

Globular cluster NGC 1806 in Dorado - Globular cluster NGC 1806 in Dorado - Image of the globular cluster NGC 1806 located in the southern constellation of Dorado. NGC 1806 belongs to the galaxy of the Great Magellan Cloud, a galaxy adjacent to our lactee path. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has turned its sharp eye towards a tight collection of stars, first seen 174 years ago. The result is a sparkling image of NGC 1806, tens of thousands of stars gravitationally bound into a rich cluster. Commonly called globular clusters, most of these objects are very old, having formed in the distant past when the Universe was only a fraction of its current age. NGC 1806 lies within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. It can be observed within the constellation of Dorado (the dolphin - fish), an area of the sky best seen from the Earth's southern hemisphere. NGC 1806 was discovered in 1836 by the British astr

PIX4564335

Triangle Constellation and Andromede Galaxy - Constellation of Triangulum with Andromeda galaxy - The constellation Triangle is a small constellation in the northern hemisphere, not far from the Andromede galaxy. Triangulum is one of the 48 constellations noted by Ptolemy and is one of the smallest of the modern star groupings codified in the 1930s. However, the most obvious triangle in this image joins the surrounding trio of yellow - orange stars, Almak, Mirach and Hamal, in which Triangulum is nicely placed. Of course almost any three stars can form a triangle but these two, one inside the other, make quite a distinctive asterism

Triangle Constellation and Andromede Galaxy - Constellation of Triangulum with Andromeda galaxy - The constellation Triangle is a small constellation in the northern hemisphere, not far from the Andromede galaxy. Triangulum is one of the 48 constellations noted by Ptolemy and is one of the smallest of the modern star groupings codified in the 1930s. However, the most obvious triangle in this image joins the surrounding trio of yellow - orange stars, Almak, Mirach and Hamal, in which Triangulum is nicely placed. Of course almost any three stars can form a triangle but these two, one inside the other, make quite a distinctive asterism

PIX4594320

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

Centaur Omega globular cluster - NGC 5139 Omega Centauri globular cluster - Visible to the naked eye in the southern hemisphere, Centaurus Omega is the most massive globular cluster in the galaxy. About 17,000 light years ago, millions of stars nearly 12 billion years old are concentrated here. This image obtained by the Spitzer space telescope reveals in yellow and red the big red stars, whose dust radiates infrared, and in blue the smaller and less evoluted stars. Omega Centauri is the biggest and brightest of the more than 150 similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. While the visible - light observations highlight the cluster's millions of jam - packed stars, Spitzer's infrared eyes reveal the dustier, more evolved stars tossed throughout the region. Globular clusters are some of the oldest objects in our universe. The

PIX4564424

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

Globular cluster M54 in Sagittarius - Globular cluster M54 in Sagittarius - The globular cluster M54 photographed by the Hubble space telescope (HST). M54 resides about 90,000 light years from Earth, in the dwarf galaxy of Sagittarius. The object shown in this beautiful Hubble image, dubbed Messier 54, could be just another globular cluster, but this dense and faint group of stars was in fact the first globular cluster found that is outside our galaxy. Discovered by the famous astronomer Charles Messier in 1778, Messier 54 belongs to a satellite of the Milky Way called the Sagittarius Dwarf Elliptical Galaxy. Messier had no idea of the significance of his discovery at the time, and it wasn't until over two centuries later, in 1994, that astronomers found Messier 54 to be part of the miniature galaxy and not our own. Current estimates indicate that the Sagittarius dwarf, and hence the cluster, is situated almost 90 000 light - years away - - more than three times as far from the centre

PIX4565011

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. In the background at the top, an irregular dwarf galaxy, Holmberg IX. Image obtained by an amateur telescope of 50 cm, composting different poses. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (

R. Jay GaBany

PIX4610325

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

Exoplanets around a red dwarf star - Exoplanets around a red dwarf star - Artist's view of extrasolar planets orbiting a red dwarf star. This artist's concept illustrates a young, red dwarf star surrounded by three planets. Such stars are dimmer and smaller than yellow stars like our sun, which makes them ideal targets for astronomers wishing to take images of planets outside our solar system, called exoplanets

PIX4573338

Signs of the Zodiac: 'Capricorn pullover' from a series of fashion caricatures, one for each sign of the zodiac

premium — Signs of the Zodiac: 'Capricorn pullover' from a series of fashion caricatures, one for each sign of the zodiac

Signs of the Zodiac: 'Capricorn pullover' from a series of fashion caricatures, one for each sign of the zodiac

OSN3916579

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate

R. Gendler

PIX4610379

Spiral galaxy M81 seen by the Hubble space telescope - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions, while its core is surrounded by much older yellow stars and a black hole. Image obtained by the Hubble space telescope with the ACS camera in 2006. Although the M81 galaxy is 11.6 million light - years away, this image taken by the Hubble space telescope is so sharp that it can resolve individual stars, along with open star clusters, globular star clusters, and even glowing regions of fluorescent gas. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The greenish regions are dense areas of bright star formation. The ultraviolet light from hot young stars are fluorescing the surr

Spiral galaxy M81 seen by the Hubble space telescope - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions, while its core is surrounded by much older yellow stars and a black hole. Image obtained by the Hubble space telescope with the ACS camera in 2006. Although the M81 galaxy is 11.6 million light - years away, this image taken by the Hubble space telescope is so sharp that it can resolve individual stars, along with open star clusters, globular star clusters, and even glowing regions of fluorescent gas. The spiral arms, which wind all the way down into the nucleus, are made up of young, bluish, hot stars formed in the past few million years. They also host a population of stars formed in an episode of star formation that started about 600 million years ago. The greenish regions are dense areas of bright star formation. The ultraviolet light from hot young stars are fluorescing the surr

PIX4610340

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

Constellations of Gemels and Little Dog - Constellations of Gemini and Canis Minor - Constellation of Gemels with bright stars Castor and Pollux. Below is the small constellation of the Little Dog, with the bright star Procyon. Canis Minor (the Lesser Dog) is sometimes regarded as the smaller of the two dogs of Orion the hunter. It is minor indeed, just 185 degrees square, and 71st in size of the 88 modern constellations. The most obvious and interesting object Canis Minor is its main star, the pale yellow Procyon. Its name is from the Greek, meaning 'before the dog', since it rises before the Sirius, the Dog Star. Gemini (the Twins) is a much more interesting collection of stars, easily visualised as two figures holding hands, their heads represented by the stars Castor and Pollux. The constellation is an ancient zodiacal construction, with a rich mythology vanishing in the mists of time. It is from the direction of Gemini (near Castor) that annual Geminid meteor showers radiate, arou

PIX4590674

The Friday Mosque, vault of the East madrasa, decorative tilework (detail) (photo)

The Friday Mosque, vault of the East madrasa, decorative tilework (detail) (photo)

Gerard Degeorge

GDG492933

The Sheriff, 2022 (digital)

premium — The Sheriff, 2022 (digital)

The Sheriff, 2022 (digital)

Murray, Roberta

RMY8617701

Colorful Marbleized Liquid Motion Art, 2024

Colorful Marbleized Liquid Motion Art, 2024

FFF8771900

Stars in the globular cluster Omega Centauri - Omega Centauri seen by Hubble space telescope - Located 16,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the most ancient objects in our galaxy. This image obtained by the Hubble Space Telescope in July 2009 shows only a small part of this cluster, where 100,000 stars are visible. Hubble Space Telescope snapped this panoramic view of a colorful assortment of 100,000 stars residing in the crowded core of a giant star cluster. The image reveals a small region inside the massive globular cluster Omega Centauri, which boasts nearly 10 million stars. The stars in Omega Centauri are between 10 billion and 12 billion years old. The cluster lies about 16,000 light - years from Earth. This is one of the first images taken by the new Wide Field Camera 3 (WFC3), installed aboard Hubble in May 2009, during Servicing Mission 4. The majority of the stars in the imag

Stars in the globular cluster Omega Centauri - Omega Centauri seen by Hubble space telescope - Located 16,000 years ago - light from Earth in the southern constellation of Centaur, Omega Centauri contains several million stars and is one of the most ancient objects in our galaxy. This image obtained by the Hubble Space Telescope in July 2009 shows only a small part of this cluster, where 100,000 stars are visible. Hubble Space Telescope snapped this panoramic view of a colorful assortment of 100,000 stars residing in the crowded core of a giant star cluster. The image reveals a small region inside the massive globular cluster Omega Centauri, which boasts nearly 10 million stars. The stars in Omega Centauri are between 10 billion and 12 billion years old. The cluster lies about 16,000 light - years from Earth. This is one of the first images taken by the new Wide Field Camera 3 (WFC3), installed aboard Hubble in May 2009, during Servicing Mission 4. The majority of the stars in the imag

PIX4564450

Jewish fire-fighters in the ghetto, Lodz, Poland, 1940 (photo)

Jewish fire-fighters in the ghetto, Lodz, Poland, 1940 (photo)

GBW3246161

Simon Trampetter of Amsterdam decouts the Yellow Star from the jacket of his friend Joseph Keller of Brussels, 1945 (b/w photo)

Simon Trampetter of Amsterdam decouts the Yellow Star from the jacket of his friend Joseph Keller of Brussels, 1945 (b/w photo)

ETE4911473

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major - The spiral galaxy M81 is located 12 million years ago - light from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. Image obtained with a 50 cm telescope through different filters, total of different poses: 20h. M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral gala

R. Gendler

PIX4610335

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

Spiral galaxy M81 in the Great Bear - Spiral galaxy M81 in Ursa Major: The spiral galaxy M81 is located 12 million light years from Earth. Its arms are home to star-forming regions while its core is surrounded by much older yellow stars. An irregular dwarf galaxy, PGC 28757 (Holmberg IX), is visible at the top of the picture. - M81 is the brightest member of the nearby galactic group called the M81 group. This group contains at least 25 other members including the peculiar starburst galaxy M82, the peculiar galaxy NGC 3077 and many dwarfs galaxies. The core galaxies of the group (M81, M82, NGC 3077, NGC 2976) are strongly interacting and are all imbedded within a large and extended molecular gas cloud. The Dwarf irregular Holmberg IX (seen above M81 in the image) most likely condensed from tidal debri existing between M81 and M82. M81 has the distinction of being the nearest spiral galaxy to have an active galactic nucleus (AGN). AGN galaxies are luminous galaxies that demonstrate much

PIX4610399

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. Image obtained with the VLT in Chile. This picture of the nearby galaxy NGC 3521 was taken using the FORS1 instrument on Eso's Very Large Telescope, at the Paranal Observatory in Chile. The large spiral galaxy lies in the constellation of Leo (The Lion), and is only 35 million light - years distant. This picture was created from exposures taken through three different filters that passed blue light, yellow/green light, and near - infrared light. These are shown in this picture as blue, green, and red, respectively

Spiral Galaxy NGC 3521 in the Lion - Spiral galaxy NGC 3521 in Leo - NGC 3521 is a spiral galaxy located about 35 million years ago - light from Earth. Image obtained with the VLT in Chile. This picture of the nearby galaxy NGC 3521 was taken using the FORS1 instrument on Eso's Very Large Telescope, at the Paranal Observatory in Chile. The large spiral galaxy lies in the constellation of Leo (The Lion), and is only 35 million light - years distant. This picture was created from exposures taken through three different filters that passed blue light, yellow/green light, and near - infrared light. These are shown in this picture as blue, green, and red, respectively

PIX4610741

Jewish citizen in Berlin (b/w photo)

Jewish citizen in Berlin (b/w photo)

SZT2980722

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

Le Soleil vu by SDO on May 23, 2010 - The Sun seen by SDO. May 23, 2010 - Le Soleil vu en ultraviolet by SDO (Solar Dynamics Observatory) on May 23, 2010. This image taken by SDO (Solar Dynamics Observatory) is a composite of three extreme ultraviolet wavelengths: 211 A (false - color yellow) 193 A (green) and 171 A (blue), each tracing a different gas temperature ranging from 1 to 2 million degrees K

PIX4627172

Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

Planetary Nebula of the Red Rectangle in the Unicorn - The Red Rectangle, AFGL 915 - This planetary nebula is located about 2300 years ago - light. Image from Siding Spring 3.9m Telescope This surprising object is one of an unusual class of nebulae surrounding mature, sun - like stars that are about to turn into planetary nebulae. Not all pre - planetary nebulae have outbursts like this, and in those that do, the nebula lasts only a few thousand years, hence the rarity. The central star has a thick belt of dust like a girdle around its equator which restricts outflow in that direction. Instead, the star ejects material in a kind of cone from each of its poles. The spectrum of the nebula shows unusual, strong red lines from hydrogen bonded to grains of carbon, however there is sufficient light reflected from the embedded star to dilute the strong red spectrum to the deep yellow we see here

PIX4623779

Comete of Halley - Halley's comet - View on April 10, 1986

Comete of Halley - Halley's comet - View on April 10, 1986

PIX4569954

Arcs of colour in the sky after sunset (colour litho)

Arcs of colour in the sky after sunset (colour litho)

German School, (20th century)

LLM8663608

«
1
…
2
3
4
…
5
»

Why choose Bridgeman Images

Art. Culture. History.

We partner with the world's leading museums, galleries and artists, so you have access to the highest-quality imagery.

Discover our collection Browse FAQs

Simple. Fast. Reliable.

Our teams can help you find the perfect content and take care of all of the copyright and licensing requirements.

Contact us

Discover millions of images and videos for your creative projects.

Start your search

© Copyright 2024 Bridgeman Art Library Limited. Registered in England and Wales as company number 01056394.