'ETOILE' images et/ou videos résultats

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

Votre Sélection en cours

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4573012","item_category2":"no_copyright","item_category3":"standard","item_category4":"p_carril","item_category5":"not_balown","item_list_name":"search_results","item_name":"hertzsprung_russell_the_hertzsprung_russell_diagram_hertzsprung_russell_hr_diagram_displaying_stars_","item_variant":"undefined"},{"item_id":"PIX4572996","item_category2":"no_copyright","item_category3":"standard","item_category4":"p_carril","item_category5":"not_balown","item_list_name":"search_results","item_name":"hertzsprung_russell_the_hertzsprung_russell_diagram_hr_diagram_hertzsprung_russell_displaying_stars_","item_variant":"undefined"},{"item_id":"PIX4573006","item_category2":"no_copyright","item_category3":"standard","item_category4":"p_carril","item_category5":"not_balown","item_list_name":"search_results","item_name":"hertzsprung_russell_the_hertzsprung_russell_diagram_hr_diagram_hertzsprung_russell_displaying_stars_","item_variant":"undefined"},{"item_id":"PIX5619655","item_category2":"no_copyright","item_category3":"standard","item_category4":"s_numazawa","item_category5":"not_balown","item_list_name":"search_results","item_name":"polaris_artwork","item_variant":"undefined"},{"item_id":"PIX4571743","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"capella_star_in_the_coach_star_capella_in_auriga_the_brightest_star_in_the_constellation_of_the_coac","item_variant":"undefined"},{"item_id":"PIX4572039","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"polaris_illustration_polaris_system_illustration_polaris_is_a_triple_system_composed_of_a_supergiant","item_variant":"undefined"},{"item_id":"PIX4572139","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"contact_binary_star_vfts_352_illustration_binary_contact_star_vfts_352_vfts_352_is_a_contact_binary_","item_variant":"undefined"},{"item_id":"PIX4621903","item_category2":"no_copyright","item_category3":"standard","item_category4":"adam_block","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ic_405_star_ae_aurigae_in_the_coach_nebula_ic_405_and_runaway_star_ae_aurigae_ic_405_is_a_neb","item_variant":"undefined"},{"item_id":"PIX4650930","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":"PIX4620765","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_n11_in_the_great_magellan_cloud_n11_star_forming_region_in_large_magellanic_cloud_lmc_n11_hen","item_variant":"undefined"},{"item_id":"LAL319223","item_category2":"no_copyright","item_category3":"standard","item_category4":"english_school_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"starfish","item_variant":"undefined"},{"item_id":"PIX4571830","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_three_stars_that_make_up_the_centaur_alpha_system_are_the_closest_stars_to_the_sun_the_image_on_","item_variant":"undefined"},{"item_id":"FGL6203359","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cinema_playbill_for_the_film_the_canary_murder_case_directed_by_malcolm_st_clair_in_a_silent_version","item_variant":"undefined"},{"item_id":"PIX4650886","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":"PIX4571719","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_sirius_in_the_great_dog_sirius_in_canis_major_sirius_is_the_main_star_in_the_constellation_big_","item_variant":"undefined"},{"item_id":"EHT6948166","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"york_minster_minster_yard_york_uk_b_w_photo","item_variant":"undefined"},{"item_id":"PIX6333926","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"rain_of_shooting_stars_perseides_photo","item_variant":"undefined"},{"item_id":"PIX4635927","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"lactee_route_in_sagittarius_and_scorpio_milky_way_in_sagittarius_and_scorpiu","item_variant":"undefined"},{"item_id":"PIX4621141","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_in_the_southern_cross_star_formation_in_the_southern_cross_part_of_the_lactee_route_i","item_variant":"undefined"},{"item_id":"PIX4598770","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_rain_leonid_meteor_storm_leonides_november_18_2001_radiant_in_the_constellation_leo_no","item_variant":"undefined"},{"item_id":"PIX4598877","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_perseide_perseid_meteor_trainee_left_by_the_passage_of_a_shooting_star_on_august_8_199","item_variant":"undefined"},{"item_id":"PIX4598695","item_category2":"no_copyright","item_category3":"standard","item_category4":"s_numazawa","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_rain_leonides_11_2001_leonid_meteor_storm_nov_19_200","item_variant":"undefined"},{"item_id":"PIX4660660","item_category2":"no_copyright","item_category3":"standard","item_category4":"oshin_zakarian","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_sky_on_the_castle_of_shavaz_starry_sky_above_shavaz_castle_star_sky_on_the_castle_of_shavaz_in_","item_variant":"undefined"},{"item_id":"PIX4599310","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_star_a_fireball_artwor","item_variant":"undefined"},{"item_id":"PIX4598786","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_rain_leonid_meteor_storm_leonides_in_front_of_the_constellation_orion_november_2001_le","item_variant":"undefined"},{"item_id":"PIX4598766","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_rain_leonid_meteor_storm_leonides_near_betelgeuse_in_orion_18_november_2001_3_meteors_","item_variant":"undefined"},{"item_id":"PIX4620956","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_in_the_galaxy_ngc_6822_bubble_nebulae_in_ngc_6822_nebula_in_the_irregular_galaxy_ngc_6822_adj","item_variant":"undefined"},{"item_id":"PIX4571864","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barnard_s_star_movement_the_proper_motion_of_barnard_s_star_barnard_s_star_is_a_red_dwarf_less_than_","item_variant":"undefined"},{"item_id":"PRX1109874","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"german_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"echinoderms_c_1860_colour_litho","item_variant":"undefined"},{"item_id":"PIX4571790","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"red_dwarf_star_proxima_of_centauri_proxima_centauri_in_x_ray_proxima_of_centaur_in_the_center_of_the","item_variant":"undefined"},{"item_id":"PIX4636564","item_category2":"no_copyright","item_category3":"standard","item_category4":"stephane_guisard","item_category5":"not_balown","item_list_name":"search_results","item_name":"chimborazo_chimborazo_and_milky_way_the_lactee_road_over_the_chimborazo_volcano_6268_metres_in_ecuad","item_variant":"undefined"},{"item_id":"UIG3524469","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"sunflower_sea_star_pycnopodia_helianthoides","item_variant":"undefined"},{"item_id":"PIX4599279","item_category2":"no_copyright","item_category3":"standard","item_category4":"s_numazawa","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_illustration_meteor_with_milky_way_artwork_artist_s_view_of_a_shooting_star_and_lactee","item_variant":"undefined"},{"item_id":"PIX4599231","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_meteor_a_shooting_star_passes_through_the_star_sky_september_28_2011_a_meteor_seen_on_","item_variant":"undefined"},{"item_id":"PIX4599222","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_orionide_orionid_meteor_an_orionid_swarm_car_seen_on_october_27_2011_orionid_meteor_se","item_variant":"undefined"},{"item_id":"PIX4620890","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_n81_in_the_small_magellan_cloud_celestial_maternity_ward_n81_in_the_small_magellanic_cloud_a_","item_variant":"undefined"},{"item_id":"PIX4645603","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"space_telescope_spitzer_artist_view_the_spitzer_space_telescope_artwork_the_spitzer_space_telescope_","item_variant":"undefined"},{"item_id":"STC4071282","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_17th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"asterias_aurantiaca_and_comatula_carinata_from_the_mollusca_and_radiata_pub_1833_hand_coloured_engra","item_variant":"undefined"},{"item_id":"PIX4621390","item_category2":"no_copyright","item_category3":"standard","item_category4":"stephane_guisard","item_category5":"not_balown","item_list_name":"search_results","item_name":"around_the_baade_window_the_baade_s_window_region_the_baade_window_at_the_bottom_right_of_the_gamma_","item_variant":"undefined"},{"item_id":"PIX4567770","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"double_cluster_of_persee_double_cluster_in_perseus_ngc_884_on_the_left_and_h_persei_ngc_869_on_the_r","item_variant":"undefined"},{"item_id":"XRD1710804","item_category2":"no_copyright","item_category3":"standard","item_category5":"balown","item_list_name":"search_results","item_name":"affiche_du_film_dark_star_l_etoile_noire_de_johncarpenter_1974","item_variant":"undefined"},{"item_id":"PIX4572025","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"polaris_system_polaris_is_a_triple_system_consisting_of_a_supergiant_star_and_two_dwarf_stars_it_is_","item_variant":"undefined"},{"item_id":"PIX4599254","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_meteor_a_shooting_star_passes_through_the_star_sky_september_28_2011_a_meteor_seen_on_","item_variant":"undefined"},{"item_id":"PIX4598975","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_perseide_perseid_meteor_a_car_seen_during_the_rain_of_shooting_stars_from_august_12_13","item_variant":"undefined"},{"item_id":"PIX4621658","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_rcw38_in_the_constellation_of_sails_seen_in_infrared_by_the_vlt_three_colour_composite_image_","item_variant":"undefined"},{"item_id":"PIX4572668","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_a_pulsating_variable_star_a_pulsating_variable_star_artwor","item_variant":"undefined"},{"item_id":"PIX4620981","item_category2":"no_copyright","item_category3":"standard","item_category4":"d_de_martin","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_sh2_101_sharpless_101_in_the_swan_looking_towards_the_constellation_cygnus_a_stunning_and_com","item_variant":"undefined"},{"item_id":"PIX4645602","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"space_telescope_spitzer_artist_view_the_spitzer_space_telescope_artwork_the_spitzer_space_telescope_","item_variant":"undefined"},{"item_id":"PIX4652865","item_category2":"no_copyright","item_category3":"standard","item_category4":"alex_tudorica","item_category5":"not_balown","item_list_name":"search_results","item_name":"cerro_tololo_observatory_cerro_tololo_observatory_lactee_road_above_cerro_tololo_observatory_chile_m","item_variant":"undefined"},{"item_id":"PIX4598719","item_category2":"no_copyright","item_category3":"standard","item_category4":"oshin_zakarian","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_stars_meteor","item_variant":"undefined"},{"item_id":"PIX4598681","item_category2":"no_copyright","item_category3":"standard","item_category4":"s_numazawa","item_category5":"not_balown","item_list_name":"search_results","item_name":"shooting_star_rain_leonides_leonid_meteor_storm_nov_19_2001_nov_19_2001","item_variant":"undefined"},{"item_id":"PIX4571865","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"alpha_centauri_alpha_centauri_alpha_centauri_is_a_double_star_alpha_centauri_a_and_b_near_the_sun_4_","item_variant":"undefined"},{"item_id":"PIX4620599","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":"PIX4652859","item_category2":"no_copyright","item_category3":"standard","item_category4":"alex_tudorica","item_category5":"not_balown","item_list_name":"search_results","item_name":"cerro_tololo_observatory_cerro_tololo_observatory_lactee_road_above_cerro_tololo_observatory_chile_t","item_variant":"undefined"},{"item_id":"PIX4567707","item_category2":"no_copyright","item_category3":"standard","item_category4":"jerry_lodriguss","item_category5":"not_balown","item_list_name":"search_results","item_name":"double_cluster_of_persee_double_cluster_in_perseus_ngc884_on_the_left_and_h_persei_ngc869_on_the_rig","item_variant":"undefined"},{"item_id":"PIX4567708","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"double_cluster_of_persee_double_cluster_in_perseus_ngc884_on_the_left_and_h_persei_ngc869_on_the_rig","item_variant":"undefined"},{"item_id":"PIX4567773","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"double_cluster_of_persee_double_cluster_in_perseus_chi_persei_ngc_884_on_the_left_and_h_persei_ngc_8","item_variant":"undefined"},{"item_id":"PIX4620812","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebuleuse_n44_in_the_great_magellan_cloud_this_photo_shows_the_southern_part_of_the_spectacular_n44_","item_variant":"undefined"},{"item_id":"PIX4636832","item_category2":"no_copyright","item_category3":"standard","item_category4":"laurent_laveder","item_category5":"not_balown","item_list_name":"search_results","item_name":"summer_milky_way_the_lactee_route_from_sagittarius_to_the_constellation_of_swan_obtained_august_13_2","item_variant":"undefined"},{"item_id":"PIX4636848","item_category2":"no_copyright","item_category3":"standard","item_category4":"laurent_laveder","item_category5":"not_balown","item_list_name":"search_results","item_name":"summer_lactee_route_summer_sky_with_the_milky_way_above_south_horizon_august_13_2006_treguennec_fini","item_variant":"undefined"}]}}

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

Recherche avancée Astuces de recherche

Images de 'ETOILE' médias trouvés, 14,014

«
1
2
3
…
234
»

Hertzsprung - Russell - The Hertzsprung - Russell diagram - Hertzsprung - Russell (HR) diagram displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

Hertzsprung - Russell - The Hertzsprung - Russell diagram - Hertzsprung - Russell (HR) diagram displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

P. Carril

PIX4573012

Hertzsprung - Russell - The Hertzsprung - Russell diagram - HR diagram (Hertzsprung - Russell) displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

Hertzsprung - Russell - The Hertzsprung - Russell diagram - HR diagram (Hertzsprung - Russell) displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

P. Carril

PIX4572996

Hertzsprung - Russell - The Hertzsprung - Russell diagram - HR diagram (Hertzsprung - Russell) displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

Hertzsprung - Russell - The Hertzsprung - Russell diagram - HR diagram (Hertzsprung - Russell) displaying stars according to their surface temperature and luminosite. The Hertzsprung - Russell diagram is named after the Danish astronomer Einar Hertzsprung (1873 - 1967) and the American astronomer Henry Norris Russell (1877 - 1957). At the beginning of the 20th century they independently noticed that red stars come in very different sizes, pioneering subsequent studies of stellar parameters (e.g., temperature, size and mass). In its basic version, this diagram plots stellar temperature (or colour) against brightness (or magnitude) and is therefore also referred to as the “” colour - magnitude diagram””. The position of a particular star in the diagram also provides information about its evolutionary stage (and age)

P. Carril

PIX4573006

Polaris. Artwork

Polaris. Artwork

S. Numazawa

PIX5619655

Capella Star in the Coach - Star Capella in Auriga - The brightest star in the constellation of the Coach, Capella (Aur), is a yellow giant star with an apparent magnitude of 0.08 and the sixth brightest star in the sky. Located 42 years of light from us, it is one of the 100 closest stars on Earth. Star Capella in Auriga constellation is the 6th brightest star in the night sky. It is located 42 light years from the earth

Capella Star in the Coach - Star Capella in Auriga - The brightest star in the constellation of the Coach, Capella (Aur), is a yellow giant star with an apparent magnitude of 0.08 and the sixth brightest star in the sky. Located 42 years of light from us, it is one of the 100 closest stars on Earth. Star Capella in Auriga constellation is the 6th brightest star in the night sky. It is located 42 light years from the earth

Jerry Lodriguss

PIX4571743

Polaris - Illustration - Polaris System - Illustration - Polaris is a triple system composed of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This illustration shows the triple system of this star, Polaris A and Polaris Ab, and further on, his companion Polaris B. This is a view from within the Polaris triple star system. The North Star, Polaris A is a bright supergiant variable star.Just above Polaris is a small companion, Polaris Ab, which is 2 billion miles from Polaris. Much farther away, near the top of the illustration, is the wide companion Polaris B. Polaris B is located approximately 240 billion miles from Polaris A. The two companion stars are the same temperature as Polaris A, but are dwarf stars. The wide companion star is visible in small telescopes. It was first noticed by William Herschel in 1780. The close companion, Polaris Ab was known to exist from measurements of a wobble in Polaris, caused by the gravitational tu

Polaris - Illustration - Polaris System - Illustration - Polaris is a triple system composed of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This illustration shows the triple system of this star, Polaris A and Polaris Ab, and further on, his companion Polaris B. This is a view from within the Polaris triple star system. The North Star, Polaris A is a bright supergiant variable star.Just above Polaris is a small companion, Polaris Ab, which is 2 billion miles from Polaris. Much farther away, near the top of the illustration, is the wide companion Polaris B. Polaris B is located approximately 240 billion miles from Polaris A. The two companion stars are the same temperature as Polaris A, but are dwarf stars. The wide companion star is visible in small telescopes. It was first noticed by William Herschel in 1780. The close companion, Polaris Ab was known to exist from measurements of a wobble in Polaris, caused by the gravitational tu

PIX4572039

Contact Binary Star VFTS 352 - Illustration - Binary Contact Star VFTS 352: VFTS 352 is a contact binary star composed of two O stars located in the Nebula of the Tarantula in the Great Magellan Cloud 160,000 light years from Earth. It's the most massive contact binary ever seen. It is composed of two stars orbiting each other in just over a day, the stars being so close that their surfaces touch each other. This artist's impression shows VFTS 352, the hottest and most massive double star system to date where the two components are in contact and sharing material. The two stars in this extreme system lie about 160,000 light-years from Earth in the Large Magellanic Cloud. This intriguing system could be heading for a dramatic end, either with the formation of a single giant star or as a future binary black hole

Contact Binary Star VFTS 352 - Illustration - Binary Contact Star VFTS 352: VFTS 352 is a contact binary star composed of two O stars located in the Nebula of the Tarantula in the Great Magellan Cloud 160,000 light years from Earth. It's the most massive contact binary ever seen. It is composed of two stars orbiting each other in just over a day, the stars being so close that their surfaces touch each other. This artist's impression shows VFTS 352, the hottest and most massive double star system to date where the two components are in contact and sharing material. The two stars in this extreme system lie about 160,000 light-years from Earth in the Large Magellanic Cloud. This intriguing system could be heading for a dramatic end, either with the formation of a single giant star or as a future binary black hole

PIX4572139

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 and runaway star AE Aurigae - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. The Flaming Star Nebula, IC 405, surrounds the variable star AE Aurigae. AE Aurigae is normally a 5.96 magnitude star of spectral class O. The star AE Aurigae itself is very bright, young, blue, and known as a runaway star since it appears to have been ejected from the Orion Nebula region about 2.5 million years ago

Nebula IC 405, star AE Aurigae in the Coach - Nebula IC 405 and runaway star AE Aurigae - IC 405, is a nebula illuminated by the massive star AE Aurigae. This type O star is a “” fleeing star”, a star ejected from the Orion nebula about 2.5 million years ago and continues its race at a speed of 200 km per second. The Flaming Star Nebula, IC 405, surrounds the variable star AE Aurigae. AE Aurigae is normally a 5.96 magnitude star of spectral class O. The star AE Aurigae itself is very bright, young, blue, and known as a runaway star since it appears to have been ejected from the Orion Nebula region about 2.5 million years ago

Adam Block

PIX4621903

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

Nebula N11 in the Great Magellan Cloud - N11 star forming region in Large Magellanic Cloud (LMC) - N11 (Henize 11) is a vast star-forming region located in the Great Magellan Cloud galaxy. It is home to a cluster of hot young stars, NGC 1760. This glowing complex of rings, shells, and powerful young stars lies in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The overall complex of glowing gas and stars is known as N11 while the central cluster of hot young blue stars is know as NGC 1760. The complex expanding shells of gas have likely formed from multiple generations of hot O and B type stars and their supernovae. N11 spans over 1000 light years across

Nebula N11 in the Great Magellan Cloud - N11 star forming region in Large Magellanic Cloud (LMC) - N11 (Henize 11) is a vast star-forming region located in the Great Magellan Cloud galaxy. It is home to a cluster of hot young stars, NGC 1760. This glowing complex of rings, shells, and powerful young stars lies in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The overall complex of glowing gas and stars is known as N11 while the central cluster of hot young blue stars is know as NGC 1760. The complex expanding shells of gas have likely formed from multiple generations of hot O and B type stars and their supernovae. N11 spans over 1000 light years across

R. Gendler

PIX4620765

Starfish

Starfish

English School, (20th century)

LAL319223

The three stars that make up the Centaur Alpha System are the closest stars to the Sun. The image on the left shows the double alpha star of the Centauri (Alpha Centauri A and B) overexposed to the red dwarf star Proxima of the Centaurus (indicated by the arrow). Proxima du Centaur is located at a distance of 4.22 years - light from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 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. Location of the Alpha Centauri triple stellar system in the sky. The brighter stars (Alpha Centauri A and B) are strongly overexposed, with the outlying member, Proxima lying approx. 2.2* to the south - west (arrow). Smaller areas around the stars are shown in the inserts to the right. The photo has been reproduced from a blue - sen

The three stars that make up the Centaur Alpha System are the closest stars to the Sun. The image on the left shows the double alpha star of the Centauri (Alpha Centauri A and B) overexposed to the red dwarf star Proxima of the Centaurus (indicated by the arrow). Proxima du Centaur is located at a distance of 4.22 years - light from the Sun but is invisible to the naked eye. Alpha Centauri A and B are a little further away, 4.36 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. Location of the Alpha Centauri triple stellar system in the sky. The brighter stars (Alpha Centauri A and B) are strongly overexposed, with the outlying member, Proxima lying approx. 2.2* to the south - west (arrow). Smaller areas around the stars are shown in the inserts to the right. The photo has been reproduced from a blue - sen

PIX4571830

CINEMA Playbill for the film “The Canary Murder Case” directed by Malcolm St. Clair in a silent version and then sonorized with the direction of Frank Tuttle

CINEMA Playbill for the film “The Canary Murder Case” directed by Malcolm St. Clair in a silent version and then sonorized with the direction of Frank Tuttle

FGL6203359

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

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Jerry Lodriguss

PIX4571719

York Minster, Minster Yard, York, UK (b/w photo)

York Minster, Minster Yard, York, UK (b/w photo)

EHT6948166

Rain of shooting stars, Perseides (photo)

Rain of shooting stars, Perseides (photo)

Sebastian Voltmer

PIX6333926

Lactee route in Sagittarius and Scorpio - Milky way in Sagittarius and Scorpiu

Lactee route in Sagittarius and Scorpio - Milky way in Sagittarius and Scorpiu

Sebastian Voltmer

PIX4635927

Star Formation in the Southern Cross - Star Formation in the Southern Cross - Part of the lactee route in the constellation of the Southern Cross seen in infrared by the Herschel space telescope. The hottest dust appears in blue, the coldest ones appear in red, the new stars will be born. Composite images obtained by SPIRE and PACS instruments on September 3, 2009. Some of the coldest and darkest dust in space shines brightly in this infrared image from the Herschel Observatory, a European Space Agency mission with important participation from NASA. The image is a composite of light captured simultaneously by two of Herschel's three instruments - - the photodetector array camera and spectrometer, and its spectral and photometric imaging receiver. The image reveals a cold and turbulent region where material is just beginning to condense into new stars. It is located in the plane of our Milky Way galaxy, 60 degrees from the center. Blue shows warmer material, red the coolest. The red fil

Star Formation in the Southern Cross - Star Formation in the Southern Cross - Part of the lactee route in the constellation of the Southern Cross seen in infrared by the Herschel space telescope. The hottest dust appears in blue, the coldest ones appear in red, the new stars will be born. Composite images obtained by SPIRE and PACS instruments on September 3, 2009. Some of the coldest and darkest dust in space shines brightly in this infrared image from the Herschel Observatory, a European Space Agency mission with important participation from NASA. The image is a composite of light captured simultaneously by two of Herschel's three instruments - - the photodetector array camera and spectrometer, and its spectral and photometric imaging receiver. The image reveals a cold and turbulent region where material is just beginning to condense into new stars. It is located in the plane of our Milky Way galaxy, 60 degrees from the center. Blue shows warmer material, red the coolest. The red fil

PIX4621141

Shooting Star Rain - Leonid Meteor Storm - Leonides, November 18, 2001. Radiant in the constellation Leo. Nov 18 2001

Shooting Star Rain - Leonid Meteor Storm - Leonides, November 18, 2001. Radiant in the constellation Leo. Nov 18 2001

Jerry Lodriguss

PIX4598770

Shooting star -Perseide - Perseid meteor - Trainee left by the passage of a shooting star on August 8, 1997. Trail left by a bright Perseid meteor. August 8, 1997

Shooting star -Perseide - Perseid meteor - Trainee left by the passage of a shooting star on August 8, 1997. Trail left by a bright Perseid meteor. August 8, 1997

Sebastian Voltmer

PIX4598877

Shooting star rain -Leonides 11/2001 - Leonid meteor storm Nov 19 200

Shooting star rain -Leonides 11/2001 - Leonid meteor storm Nov 19 200

S. Numazawa

PIX4598695

Star sky on the castle of Shavaz - Starry sky above Shavaz castle - Star sky on the castle of Shavaz in the desert of Yazd in Iran. Shavaz castle, desert of Yazd, Ira

Star sky on the castle of Shavaz - Starry sky above Shavaz castle - Star sky on the castle of Shavaz in the desert of Yazd in Iran. Shavaz castle, desert of Yazd, Ira

Oshin Zakarian

PIX4660660

Artist's View Star - A Fireball. Artwor

Artist's View Star - A Fireball. Artwor

S. Numazawa

PIX4599310

Shooting star rain - Leonid Meteor Storm - Leonides in front of the constellation Orion, November 2001. Leonid meteor storm. November 200

Shooting star rain - Leonid Meteor Storm - Leonides in front of the constellation Orion, November 2001. Leonid meteor storm. November 200

Sebastian Voltmer

PIX4598786

Shooting star rain - Leonid Meteor Storm - Leonides, near Betelgeuse in Orion. 18 November 2001. 3 meteors near Betelgeuse in Orion. Nov 18, 2001

Shooting star rain - Leonid Meteor Storm - Leonides, near Betelgeuse in Orion. 18 November 2001. 3 meteors near Betelgeuse in Orion. Nov 18, 2001

Jerry Lodriguss

PIX4598766

Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar

Nebula in the galaxy NGC 6822 - Bubble nebulae in NGC 6822 - Nebula in the irregular galaxy NGC 6822, adjacent to our galaxy. This gas bubble houses massive stars known as Wolf - Rayet. NGC 6822 is a nearby irregular galaxy reminiscent of the Large Magellanic Cloud (LMC). Like the LMC it contains many, extremely hot stars of the Wolf - Rayet type, stars which often have intense stellar winds blasting from their surfaces. Small groups of such stars are found at the centres of the bubble nebulae seen here, which are the result of the stellar winds colliding with the more or less stationary interstellar medium in NGC 6822. At the interface of the collision, the interstellar medium glows, producing a thin, luminous bubble. Such bubbles are rare in the more turbulent Milky Way galaxy, but Henize 70 in the Large Magellanic Cloud is similar

PIX4620956

Barnard's Star Movement - The proper motion of Barnard's star - Barnard's Star is a red dwarf less than six years from Earth in the constellation Ophiuchus. Its proximity makes it move quickly ahead of the other stars. Barnard's star is known for having the most important clean movement. This composite image made from three images taken in 1988 (blue), 1991 (red) and 1993 (green) shows the shift of the star in 15 years. Barnard's Star is red dwarf star approximately 6 light - years away from Earth in the constellation of Ophiuchus Its proper motion is 10.3 arcseconds per year, which remains the largest known proper motion of any star relative to the Sun. The monochrome plates from which this 3 - colour picture were made were taken in 1988 (blue), 1991 (red) and 1993 (green) showing its movement over 15 years

Barnard's Star Movement - The proper motion of Barnard's star - Barnard's Star is a red dwarf less than six years from Earth in the constellation Ophiuchus. Its proximity makes it move quickly ahead of the other stars. Barnard's star is known for having the most important clean movement. This composite image made from three images taken in 1988 (blue), 1991 (red) and 1993 (green) shows the shift of the star in 15 years. Barnard's Star is red dwarf star approximately 6 light - years away from Earth in the constellation of Ophiuchus Its proper motion is 10.3 arcseconds per year, which remains the largest known proper motion of any star relative to the Sun. The monochrome plates from which this 3 - colour picture were made were taken in 1988 (blue), 1991 (red) and 1993 (green) showing its movement over 15 years

PIX4571864

Echinoderms, c.1860 (colour litho)

Echinoderms, c.1860 (colour litho)

German School, (19th century)

PRX1109874

Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

Red Dwarf Star Proxima of Centauri - Proxima Centauri in X - Ray - Proxima of Centaur (in the center of the image) is the closest star to the Sun, at a distance of 4.2 years - light. It belongs to the triple Alpha star system of the Centaurus being the least bright star of this system; it is a red dwarf star. X-ray image obtained by the Chandra space telescope. Chandra and XMM - Newton observations of the red dwarf star Proxima Centauri have shown that its surface is in a state of turmoil. Flares, or explosive outbursts, occur almost continually. This behavior can be traced to Proxima Centauri's low mass, about a tenth that of the Sun. In the cores of low mass stars, nuclear fusion reactions that convert hydrogen to helium proceed very slowly, and create a turbulent, convective motion throughout their interiors. This motion stores up magnetic energy which is often released explosively in the star's upper atmosphere where it produces flares in X - rays and other forms of light. The same

PIX4571790

Chimborazo - Chimborazo and Milky Way - The lactee road over the Chimborazo volcano (6268 metres) in Ecuador. Mosaic of 28 images. With an altitude of 6268 meters (20564 ft) above sea level, Chimborazo volcano is the highest summit in Ecuador but of course not the highest summit on the planet. This record belongs to Mount Everest (8848 metres/29029 ft above sea level). However, because the Earth is not a perfect sphere but rather an oblate spheroid (a sphere flattened along the axis from pole to pole such that there is a bulge around the equator) and that Chimborazo is very close to the equator line (only -1 degree in latitude), Chimborazo is known as the “” the farthest location from the center of the Earth”. 6384.687 Km against 6382.467 Km for Everest that is, a difference of 2.220 Km/1.38 miles. The image is a mosaic of 28 images in order to cover all the sky with a 35 mm focal length lens. The exposure time for each image is only 15 seconds with a modified Canon 5Dii camera. The au

Chimborazo - Chimborazo and Milky Way - The lactee road over the Chimborazo volcano (6268 metres) in Ecuador. Mosaic of 28 images. With an altitude of 6268 meters (20564 ft) above sea level, Chimborazo volcano is the highest summit in Ecuador but of course not the highest summit on the planet. This record belongs to Mount Everest (8848 metres/29029 ft above sea level). However, because the Earth is not a perfect sphere but rather an oblate spheroid (a sphere flattened along the axis from pole to pole such that there is a bulge around the equator) and that Chimborazo is very close to the equator line (only -1 degree in latitude), Chimborazo is known as the “” the farthest location from the center of the Earth”. 6384.687 Km against 6382.467 Km for Everest that is, a difference of 2.220 Km/1.38 miles. The image is a mosaic of 28 images in order to cover all the sky with a 35 mm focal length lens. The exposure time for each image is only 15 seconds with a modified Canon 5Dii camera. The au

Stephane Guisard

PIX4636564

Sunflower Sea star (Pycnopodia Helianthoides)

Sunflower Sea star (Pycnopodia Helianthoides)

UIG3524469

Shooting Star-Illustration - Meteor with milky way. Artwork - Artist's view of a shooting star and lactee way

Shooting Star-Illustration - Meteor with milky way. Artwork - Artist's view of a shooting star and lactee way

S. Numazawa

PIX4599279

Shooting Star - Meteor - A shooting star passes through the star sky. September 28, 2011. A meteor seen on September 28, 2011

Shooting Star - Meteor - A shooting star passes through the star sky. September 28, 2011. A meteor seen on September 28, 2011

Sebastian Voltmer

PIX4599231

Shooting star, Orionide - Orionid meteor - An Orionid swarm car seen on October 27, 2011. Orionid meteor seen on October 27, 2011

Shooting star, Orionide - Orionid meteor - An Orionid swarm car seen on October 27, 2011. Orionid meteor seen on October 27, 2011

Sebastian Voltmer

PIX4599222

Nebula N81 in the Small Magellan Cloud - Celestial Maternity Ward N81 in the Small Magellanic Cloud A NASA Hubble Space Telescope “” family portrait””” of young, ultra - bright stars nested in their embryonic cloud of glowing gases. The celestial maternity ward, called N81, is located 200,000 light - years away in the Small Magellanic Cloud (SMC), a small irregular satellite galaxy of our Milky Way. Hubble's exquisite resolution allows astronomers to pinpoint 50 separate stars tightly packed in the nebula's core within a 10 light - year diameter - slightly more than twice the distance between earth and the nearest star to our sun. The closest pair of stars is only 1/3 of a light - year apart (0.3 arcseconds in the sky). This furious rate of mass loss from these super - hot stars is evident in the Hubble picture that reveals dramatic shapes sculpted in the nebula's wall of glowing gases by violent stellar winds and shock waves. A pair of bright stars in the center of the nebula is pouri

Nebula N81 in the Small Magellan Cloud - Celestial Maternity Ward N81 in the Small Magellanic Cloud A NASA Hubble Space Telescope “” family portrait””” of young, ultra - bright stars nested in their embryonic cloud of glowing gases. The celestial maternity ward, called N81, is located 200,000 light - years away in the Small Magellanic Cloud (SMC), a small irregular satellite galaxy of our Milky Way. Hubble's exquisite resolution allows astronomers to pinpoint 50 separate stars tightly packed in the nebula's core within a 10 light - year diameter - slightly more than twice the distance between earth and the nearest star to our sun. The closest pair of stars is only 1/3 of a light - year apart (0.3 arcseconds in the sky). This furious rate of mass loss from these super - hot stars is evident in the Hubble picture that reveals dramatic shapes sculpted in the nebula's wall of glowing gases by violent stellar winds and shock waves. A pair of bright stars in the center of the nebula is pouri

PIX4620890

Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. Spitzer looks towards the Rho Ophiuchi star - formation region looming just above the disk of the Milky Way. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. Spitzer looks towards the Rho Ophiuchi star - formation region looming just above the disk of the Milky Way. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

PIX4645603

Asterias aurantiaca and Comatula carinata, from The Mollusca and Radiata, pub. 1833 (Hand coloured engraving)

Asterias aurantiaca and Comatula carinata, from The Mollusca and Radiata, pub. 1833 (Hand coloured engraving)

English School, (17th century)

STC4071282

Around the Baade window - The Baade's window region - The Baade Window (at the bottom right of the Gamma star of Sagittarius, the brightest of this image) is a region of the Lactee Way in the constellation of Sagittarius containing little interstellar dust. This region, named in reference to the astronomer Walter Baade, allows astronomers to have a more degagee view of the center of our galaxy. The Baade window, (at the bottom right of the bright star close to the center of this image), is a region of the Milky Way, in the Sagittarius constellation, with relatively little interstellar dust along our line of sight. It is therefore really a unique 'window' through which the astronomers can observe the Milky Way galactic Bulge, only a few degrees from the galactic center. The 'line of sight' through this 'window' passes 1800 light year nearby the Milky Way heart. This region of the sky was named after German astronomer Walter Baade

Around the Baade window - The Baade's window region - The Baade Window (at the bottom right of the Gamma star of Sagittarius, the brightest of this image) is a region of the Lactee Way in the constellation of Sagittarius containing little interstellar dust. This region, named in reference to the astronomer Walter Baade, allows astronomers to have a more degagee view of the center of our galaxy. The Baade window, (at the bottom right of the bright star close to the center of this image), is a region of the Milky Way, in the Sagittarius constellation, with relatively little interstellar dust along our line of sight. It is therefore really a unique 'window' through which the astronomers can observe the Milky Way galactic Bulge, only a few degrees from the galactic center. The 'line of sight' through this 'window' passes 1800 light year nearby the Milky Way heart. This region of the sky was named after German astronomer Walter Baade

Stephane Guisard

PIX4621390

Double cluster of Persee - Double cluster in Perseus - NGC 884, on the left and h Persei (NGC 869) on the right are located about 7000 years - light in the constellation Persee. This field corresponds to that of binoculars or a small telescope. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC 884, on the left) and h Persei (NGC 869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness. This skyview is corresponding to binoculars and small telescopes

Double cluster of Persee - Double cluster in Perseus - NGC 884, on the left and h Persei (NGC 869) on the right are located about 7000 years - light in the constellation Persee. This field corresponds to that of binoculars or a small telescope. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC 884, on the left) and h Persei (NGC 869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness. This skyview is corresponding to binoculars and small telescopes

PIX4567770

Affiche du film Dark Star l Etoile Noire de JohnCarpenter 1974

Affiche du film Dark Star l Etoile Noire de JohnCarpenter 1974

XRD1710804

Polaris System - Polaris is a triple system consisting of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This montage shows the polar star and constellations of the Little Bear and the Big Bear (left), Polaris A and his companion Polaris B seen by the Hubble Space Telescope (top right), and Polaris Ab photographed for the first time by the Hubble Space Telescope (bottom right). This sequence of images shows that the North Star, Polaris is really a triple star system. For the first time, the close companion of Polaris has been seen directly. The left frame shows Polaris's location very close to the position of Earth's north celestial pole in Ursa Minor (the Small Bear). The upper right image shows Polaris A and its distant companion Polaris B, as viewed by Hubble. They are separated by approximately 240 billion miles. Polaris B, the wide companion, is visible in small telescopes, and was first noticed by William Herschel in 1780. The c

Polaris System - Polaris is a triple system consisting of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This montage shows the polar star and constellations of the Little Bear and the Big Bear (left), Polaris A and his companion Polaris B seen by the Hubble Space Telescope (top right), and Polaris Ab photographed for the first time by the Hubble Space Telescope (bottom right). This sequence of images shows that the North Star, Polaris is really a triple star system. For the first time, the close companion of Polaris has been seen directly. The left frame shows Polaris's location very close to the position of Earth's north celestial pole in Ursa Minor (the Small Bear). The upper right image shows Polaris A and its distant companion Polaris B, as viewed by Hubble. They are separated by approximately 240 billion miles. Polaris B, the wide companion, is visible in small telescopes, and was first noticed by William Herschel in 1780. The c

PIX4572025

Shooting Star - Meteor - A shooting star passes through the star sky. September 28, 2011. A meteor seen on September 28, 2011

Shooting Star - Meteor - A shooting star passes through the star sky. September 28, 2011. A meteor seen on September 28, 2011

Sebastian Voltmer

PIX4599254

Shooting star, Perseide - Perseid meteor - A car seen during the rain of shooting stars from August 12-13, 2010. Perseid meteor seen on august 12 2010

Shooting star, Perseide - Perseid meteor - A car seen during the rain of shooting stars from August 12-13, 2010. Perseid meteor seen on august 12 2010

Sebastian Voltmer

PIX4598975

Nebula RCW38 in the constellation of sails seen in infrared by the VLT - Three - colour composite image of RCW38, obtained through three near - infrared filters. This is a region in the Milky Way at a distance of about 5,000 light years, where stars which have recently formed in clouds of gas and dust are still heavily obscured and cannot be observed in the visible part of the spectrum. Contrarily, as this image shows, they are very well seen at infrared wavelengths where the obscuration is substantially lower. The diffuse radiation is a mixture of starlight scattered by the dust and gas in the area, and atomic and molecular hydrogen line emission. RCW 38 is at a distance of ~ 1.7 kpc (~ 5500 light years) from us, near the famous Vela supernova remnant and the Gum nebul

Nebula RCW38 in the constellation of sails seen in infrared by the VLT - Three - colour composite image of RCW38, obtained through three near - infrared filters. This is a region in the Milky Way at a distance of about 5,000 light years, where stars which have recently formed in clouds of gas and dust are still heavily obscured and cannot be observed in the visible part of the spectrum. Contrarily, as this image shows, they are very well seen at infrared wavelengths where the obscuration is substantially lower. The diffuse radiation is a mixture of starlight scattered by the dust and gas in the area, and atomic and molecular hydrogen line emission. RCW 38 is at a distance of ~ 1.7 kpc (~ 5500 light years) from us, near the famous Vela supernova remnant and the Gum nebul

PIX4621658

Artist's view of a pulsating variable star - A pulsating variable star. Artwor

Artist's view of a pulsating variable star - A pulsating variable star. Artwor

S. Numazawa

PIX4572668

Nebula Sh2 - 101 (Sharpless 101) in the Swan - Looking towards the constellation Cygnus, a stunning and complex region of nebulae strewn along the plane of our Milky Way galaxy is revealed in this sky view. The image emphasizes cosmic gas clouds in a wide field centered on the Sharpless 101 Nebula, a faint emission type nebula known also as Tulip Nebula, in the well known Northern Cross asterism. These Cygnus nebulosities are all located about 2,000 light - years away. Along with the Sun, they lie within the Orion spiral arm of our galaxy

Nebula Sh2 - 101 (Sharpless 101) in the Swan - Looking towards the constellation Cygnus, a stunning and complex region of nebulae strewn along the plane of our Milky Way galaxy is revealed in this sky view. The image emphasizes cosmic gas clouds in a wide field centered on the Sharpless 101 Nebula, a faint emission type nebula known also as Tulip Nebula, in the well known Northern Cross asterism. These Cygnus nebulosities are all located about 2,000 light - years away. Along with the Sun, they lie within the Orion spiral arm of our galaxy

D. De Martin

PIX4620981

Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The cloud complexes around Orion and the disk of the Milky Way are seen behind the observatory. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The cloud complexes around Orion and the disk of the Milky Way are seen behind the observatory. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

PIX4645602

Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. Milky way above Cerro Tololo observatory, Chile

Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. Milky way above Cerro Tololo observatory, Chile

Alex Tudorica

PIX4652865

Shooting Stars - Meteor

Shooting Stars - Meteor

Oshin Zakarian

PIX4598719

Shooting star rain -Leonides - Leonid meteor storm Nov 19 2001 - Nov 19 2001

Shooting star rain -Leonides - Leonid meteor storm Nov 19 2001 - Nov 19 2001

S. Numazawa

PIX4598681

Alpha Centauri - Alpha Centauri - Alpha Centauri is a double star (Alpha Centauri A and B) near the Sun, 4.36 years - light. These two stars are relatively similar to the Sun. Alpha Centauri is a binary star (Alpha Centauri A and B) located at a distance of 4.36 light - years, or 41 million km, in the direction of the southern constellation Centaurus (The Centaur). Alpha Centauri A and Alpha Centauri B, are rather similar to the Sun; their stellar spectral types are “” G2V”” and “” K1V””, respectively. Alpha Centauri A and B orbit each other at a distance of about 3600 million km, or somewhat more than the distance of planet Uranus from the Sun. The orbital period is almost exactly 80 years

Alpha Centauri - Alpha Centauri - Alpha Centauri is a double star (Alpha Centauri A and B) near the Sun, 4.36 years - light. These two stars are relatively similar to the Sun. Alpha Centauri is a binary star (Alpha Centauri A and B) located at a distance of 4.36 light - years, or 41 million km, in the direction of the southern constellation Centaurus (The Centaur). Alpha Centauri A and Alpha Centauri B, are rather similar to the Sun; their stellar spectral types are “” G2V”” and “” K1V””, respectively. Alpha Centauri A and B orbit each other at a distance of about 3600 million km, or somewhat more than the distance of planet Uranus from the Sun. The orbital period is almost exactly 80 years

PIX4571865

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

Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. The 4 meter telescope Blanco and the small telescopes. Milky way above the 4 meter Blanco telescope and small telescopes in Cerro Tololo observatory, Chile

Cerro Tololo Observatory - Cerro Tololo Observatory - Lactee road above Cerro Tololo Observatory, Chile. The 4 meter telescope Blanco and the small telescopes. Milky way above the 4 meter Blanco telescope and small telescopes in Cerro Tololo observatory, Chile

Alex Tudorica

PIX4652859

Double cluster of Persee - Double cluster in Perseus - NGC884, on the left and h Persei NGC869 on the right are located about 7000 years - light in the constellation Persee. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC884, on the left) and h Persei (NGC869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

Double cluster of Persee - Double cluster in Perseus - NGC884, on the left and h Persei NGC869 on the right are located about 7000 years - light in the constellation Persee. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC884, on the left) and h Persei (NGC869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

Jerry Lodriguss

PIX4567707

Double cluster of Persee - Double cluster in Perseus - NGC884, on the left and h Persei NGC869 on the right are located about 7000 years - light in the constellation Persee. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC884, on the left) and h Persei (NGC869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

Double cluster of Persee - Double cluster in Perseus - NGC884, on the left and h Persei NGC869 on the right are located about 7000 years - light in the constellation Persee. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC884, on the left) and h Persei (NGC869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

R. Gendler

PIX4567708

Double cluster of Persee - Double cluster in Perseus - Chi Persei (NGC 884), on the left and h Persei (NGC 869) on the right are located about 7000 years - light in the constellation Persee. Mosaic of two images obtained with a 30 cm telescope. Time: 14 hours. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC 884, on the left) and h Persei (NGC 869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

Double cluster of Persee - Double cluster in Perseus - Chi Persei (NGC 884), on the left and h Persei (NGC 869) on the right are located about 7000 years - light in the constellation Persee. Mosaic of two images obtained with a 30 cm telescope. Time: 14 hours. The double cluster in the constellation Perseus, normally known by its Greek designation transliterated. chi Persei (NGC 884, on the left) and h Persei (NGC 869) are about 7000 light - years away and less than 100 light - years apart. Although open clusters are quite common, this pair is exceptional due to the large number of young bright O and B stars in each, and their closeness

R. Gendler

PIX4567773

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

Nebuleuse N44 in the Great Magellan Cloud - This photo shows the southern part of the spectacular N44 region in the Large Magellanic Cloud. The green colour indicates areas that are particularly hot. The field measures 27.5 x 26.5 arcmin2., North is up and East is left. The two best known satellite galaxies of the Milky Way, the Magellanic Clouds, are located in the southern sky at a distance of about 170,000 light - years. They host many giant nebular complexes with very hot and luminous stars whose intense ultraviolet radiation causes the surrounding interstellar gas to glow. The intricate and colourful nebulae are produced by ionised gas that shines as electrons and positively charged atomic nuclei recombine, emitting a cascade of photons at well defined wavelengths. Such nebulae are called “” H II regions””, signifying ionised hydrogen, i.e. hydrogen atoms that have lost one electron (protons). Their spectra are characterized by emission lines whose relative intensities carry usefu

PIX4620812

Summer Milky Way - The lactee route, from Sagittarius to the constellation of Swan, obtained August 13, 2007 in Brittany. Summer milky way from Sagittarius to Cygnus constellation. August 13 2007 (Trevignon-France

Summer Milky Way - The lactee route, from Sagittarius to the constellation of Swan, obtained August 13, 2007 in Brittany. Summer milky way from Sagittarius to Cygnus constellation. August 13 2007 (Trevignon-France

Laurent Laveder

PIX4636832

Summer Lactee Route - Summer sky with the milky way above south horizon. August 13 2006, Treguennec (Finistere-France)

Summer Lactee Route - Summer sky with the milky way above south horizon. August 13 2006, Treguennec (Finistere-France)

Laurent Laveder

PIX4636848

«
1
2
3
…
234
»

Pourquoi choisir Bridgeman Images

Art. Culture. Histoire.

Nous travaillons en partenariat avec les plus grands musées, galeries et artistes du monde entier, ce qui vous permet d'avoir accès à des images de la plus haute qualité.

Découvrez notre collection Consultez nos FAQs

Simple. Rapide. Fiable.

Nos équipes peuvent vous aider à trouver le contenu idéal et s'occuper de toutes les exigences en matière de droits d'auteur et de licences.

Contactez-nous

Découvrez des millions d'images et de vidéos pour vos projets.

Commencez votre recherche

© Droits d'auteur 2024 Bridgeman Art Library Limited. Enregistrée en Angleterre et au Pays de Galles sous le numéro d'entreprise 01056394.