'Solar' immagini e video risultati

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

La tua selezione corrente

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4565015","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_ngc_6752_stars_in_globular_cluster_ngc_6752_image_of_the_center_of_the_globular_clu","item_variant":"undefined"},{"item_id":"PIX4592258","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"constellation_of_lyra_constellation_of_lyra_constellation_of_lyra_with_bright_star_vega_lyra_the_lyr","item_variant":"undefined"},{"item_id":"UIS5090356","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_phases_of_the_moon_c_1860","item_variant":"undefined"},{"item_id":"UIG2903526","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"skyline_photo","item_variant":"undefined"},{"item_id":"UIG2903533","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dusky_skyline_photo","item_variant":"undefined"},{"item_id":"UIS5082813","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"instruments_polariscopes_wheatstone_polar_clock_1848_1860","item_variant":"undefined"},{"item_id":"PIX4625850","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"geyser_sur_enceladus_artist_view_water_geyser_on_enceladus_artist_view_artist_view_of_an_ice_geyser_","item_variant":"undefined"},{"item_id":"UIS5086422","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"sundials_compass_octagonal_louis_xvi_sundial_and_compass_french_early_18th_century","item_variant":"undefined"},{"item_id":"GRL6253614","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_italy_photo","item_variant":"undefined"},{"item_id":"PIX4613427","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_large_magellanic_cloud_the_large_magellanic_cloud_the_great_magellan_cloud_galaxy_is_located_abo","item_variant":"undefined"},{"item_id":"PIX4640224","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"space_lift_on_the_moon_artist_s_view_lunar_elevator_lunar_base_lunar_base_equipped_with_a_space_lift","item_variant":"undefined"},{"item_id":"PHL450964","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"indian_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"simurgh_attacking_a_gaja_simha_carrying_elephants_early_19th_century_opaque_w_c_gold_on_paper","item_variant":"undefined"},{"item_id":"PIX4625211","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"southern_aurora_on_the_planet_saturn_aurora_on_saturn_the_planet_saturn_accompanied_by_a_southern_au","item_variant":"undefined"},{"item_id":"PIX4625896","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"geyser_sur_enceladus_artist_s_view_water_geyser_on_enceladus_artist_s_view_of_an_ice_geyser_on_the_s","item_variant":"undefined"},{"item_id":"GRL6253623","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253631","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"PIX4624042","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"neptune_illustration_neptune_s_great_dark_spot_illustration_artist_s_view_of_neptune_with_its_ring_s","item_variant":"undefined"},{"item_id":"GRL6253619","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253628","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253610","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_facade_with_the_entrance_door_and_the_roses_cathedral_of_st_feliciano_foligno_umbria_italy_photo","item_variant":"undefined"},{"item_id":"GRL6253616","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253621","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253627","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"GRL6253633","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_frieze_of_the_portal_entrance_door_facade_cathedral_of_st_feliciano_foligno_umbria_ita","item_variant":"undefined"},{"item_id":"UIS5096283","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_phases_of_the_moon_c_1860","item_variant":"undefined"},{"item_id":"UIS5070769","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"artistso_aids_camera_obscuras_backplate_from_storer_s_oroyal_delineatoro_c_1778","item_variant":"undefined"},{"item_id":"UIS5062913","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"desaguliers_cometarium_1755","item_variant":"undefined"},{"item_id":"PIX4664981","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"condensation_trains_over_brittany_airplane_contrails_over_brittany_france_a_multitude_of_condensatio","item_variant":"undefined"},{"item_id":"GRL6253607","item_category2":"no_copyright","item_category3":"standard","item_category4":"ghigo_roli","item_category5":"not_balown","item_list_name":"search_results","item_name":"detail_of_the_entrance_door_and_the_romanesque_rose_entrance_door_facade_cathedral_of_st_feliciano_f","item_variant":"undefined"},{"item_id":"NTB8727760","item_category2":"no_copyright","item_category3":"standard","item_category4":"sverre_a_borretzen","item_category5":"not_balown","item_list_name":"search_results","item_name":"dale_in_hordaland_19530425_dale_fabrikker_is_norway_s_largest_textile_factory_with_1000_employees_19","item_variant":"undefined"},{"item_id":"NAM5923993","item_category2":"undetermined_copyright","item_category3":"standard","item_category4":"unknown_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"main_guard_of_camp_at_jatta_post_1919_circa_b_w_photo","item_variant":"undefined"},{"item_id":"PIX4622088","item_category2":"no_copyright","item_category3":"standard","item_category4":"stephane_guisard","item_category5":"not_balown","item_list_name":"search_results","item_name":"horsehead_nebula_ic_434_in_orion_horsehead_nebula_b33_in_orion_the_horse_s_head_nebula_barnard_33_is","item_variant":"undefined"},{"item_id":"PIX4623396","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_ngc_6781_a_planetary_nebula_ngc_6781_this_fairly_inconspicuous_planetary_nebula_is_","item_variant":"undefined"},{"item_id":"UIS5061218","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"desaguliers_cometarium_1755","item_variant":"undefined"},{"item_id":"SVA660202","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"egyptian_school","item_category5":"not_balown","item_list_name":"search_results","item_name":"pectoral_and_necklace_of_psusennes_i","item_variant":"undefined"},{"item_id":"PIX4641302","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"iss_and_inflatable_module_large_habitat_and_iss_artist_s_view_of_a_large_inflatable_module_much_larg","item_variant":"undefined"},{"item_id":"PIX4581325","item_category2":"no_copyright","item_category3":"standard","item_category4":"stephane_guisard","item_category5":"not_balown","item_list_name":"search_results","item_name":"circumpolar_in_ecuador_star_trail_from_the_equator_ecuador_star_line_taken_from_ecuador_ecuador_10_h","item_variant":"undefined"},{"item_id":"PIX4623698","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_hen_1357_dans_l_altar_hst_this_wide_field_and_planetary_camera_2_image_captures_the","item_variant":"undefined"},{"item_id":"PIX4607298","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_dawn_probe_near_ceres_artist_s_view_dawn_approaches_ceres_artist_view_of_the_dawn_probe_near_the","item_variant":"undefined"},{"item_id":"XCL499508","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"egyptian_18th_dynasty_c_1567_1320_bc","item_category5":"balown","item_list_name":"search_results","item_name":"talatat_men_hoeing_the_earth_c_1353_1347_bc_painted_sandstone","item_variant":"undefined"},{"item_id":"MMM7340358","item_category2":"in_copyright","item_category3":"standard","item_category4":"rhemann_gerald_21st_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"comet_c_2016_r2_panstarrs_the_blue_carbon_monoxide_comet_rotating_comet_tails_on_january_19th_2018_d","item_variant":"undefined"},{"item_id":"PIX4641303","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"iss_and_inflatable_module_large_habitat_and_iss_artist_s_view_of_a_large_inflatable_module_much_larg","item_variant":"undefined"},{"item_id":"PIX4641310","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"iss_and_inflatable_module_large_habitat_and_iss_artist_s_view_of_a_large_inflatable_module_much_larg","item_variant":"undefined"},{"item_id":"PIX4615389","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"mars_view_of_the_north_pole_mars_north_pole_image_based_on_altimetric_data_obtained_by_the_mars_glob","item_variant":"undefined"},{"item_id":"PIX4572090","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"super_massive_star_eta_carinae_super_massive_star_eta_carinae_eta_carinae_is_one_of_the_most_massive","item_variant":"undefined"},{"item_id":"PIX4620193","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"center_of_the_omega_nebula_m17_in_the_sagittarius_seen_by_hst_center_of_the_omega_nebula_a_hotbed_of","item_variant":"undefined"},{"item_id":"PIX4621983","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"horse_s_head_nebula_ic_434_in_orion_horsehead_nebula_in_orion_the_horse_s_head_nebula_barnard_33_is_","item_variant":"undefined"},{"item_id":"PIX4582251","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"pluto_seen_by_the_new_horizons_probe_pluto_seen_by_new_horizons_pluto_s_atmosphere_seen_by_the_new_h","item_variant":"undefined"},{"item_id":"PIX4622085","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"horsehead_nebula_ic_434_in_orion_horsehead_nebula_b33_in_orion_the_horse_s_head_nebula_barnard_33_is","item_variant":"undefined"},{"item_id":"PIX4612179","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"centaurus_a_elliptical_galaxy_ngc_5128_in_the_centaurus_galaxy_centaurus_a_ngc_5128_the_galaxy_ngc_5","item_variant":"undefined"},{"item_id":"PIX4620555","item_category2":"no_copyright","item_category3":"standard","item_category4":"adam_block","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_7023_in_cephee_ngc_7023_the_iris_nebula_in_cepheus_the_iris_nebula_ngc_7023_is_a_reflexio","item_variant":"undefined"},{"item_id":"PIX4622070","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"horsehead_nebula_ic_434_in_orion_horsehead_nebula_b33_in_orion_the_horse_s_head_nebula_barnard_33_is","item_variant":"undefined"},{"item_id":"PIX4573224","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"exoplanets_around_70_virginis_a_jovian_planet_orbiting_70_virginis_artist_s_view_of_the_extrasolar_p","item_variant":"undefined"},{"item_id":"PIX4619228","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_6164_5_in_the_rule_the_emission_nebula_ngc_6164_65_this_nebula_is_located_about_4000_year","item_variant":"undefined"},{"item_id":"BL3283144","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"rama_and_ravana_renew_their_assaults_on_each_other_the_gods_have_decided_that_the_contest_is_unequal","item_variant":"undefined"},{"item_id":"PIX4610340","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":"PIX4620159","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"centre_de_la_nebula_omega_m17_by_hst_center_of_the_omega_nebula_a_hotbed_of_newly_born_stars_wrapped","item_variant":"undefined"},{"item_id":"PIX4572109","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"super_massive_star_eta_carinae_super_massive_star_eta_carinae_eta_carinae_is_one_of_the_most_massive","item_variant":"undefined"},{"item_id":"PIX4619260","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_ngc_6164_5_in_the_rule_the_emission_nebula_ngc_6164_65_this_nebula_is_located_about_4000_ligh","item_variant":"undefined"},{"item_id":"SVA660198","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"egyptian_school","item_category5":"not_balown","item_list_name":"search_results","item_name":"outer_sarcophagus_of_khonsu","item_variant":"undefined"}]}}

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

Ricerca Avanzata Search Tips

Immagini di 'Solar' trovate, 26,238

«
1
…
435
436
437
…
438
»

Globular cluster NGC 6752 - Stars in globular cluster NGC 6752 - Image of the center of the globular cluster NGC 6752 located in the constellation Peacock. The Hubble Space Telescope (HST) observed blue straggler. NGC 6752 is a globular cluster, and at over 10 billion years old is one the most ancient collections of stars known. It has been blazing for well over twice as long as our Solar System has existed. NGC 6752 contains a high number of blue straggler”” stars, some of which are visible in this image. These stars display characteristics of stars younger than their neighbours, despite models suggesting that most of the stars within globular clusters should have formed at approximately the same time. Their origin is therefore something of a mystery. Studies of NGC 6752 may shed light on this situation. It appears that a very high number - - up to 38% - - of the stars within its core region are binary systems. Collisions between stars in this turbulent area could produce the blue str

Globular cluster NGC 6752 - Stars in globular cluster NGC 6752 - Image of the center of the globular cluster NGC 6752 located in the constellation Peacock. The Hubble Space Telescope (HST) observed blue straggler. NGC 6752 is a globular cluster, and at over 10 billion years old is one the most ancient collections of stars known. It has been blazing for well over twice as long as our Solar System has existed. NGC 6752 contains a high number of blue straggler”” stars, some of which are visible in this image. These stars display characteristics of stars younger than their neighbours, despite models suggesting that most of the stars within globular clusters should have formed at approximately the same time. Their origin is therefore something of a mystery. Studies of NGC 6752 may shed light on this situation. It appears that a very high number - - up to 38% - - of the stars within its core region are binary systems. Collisions between stars in this turbulent area could produce the blue str

PIX4565015

Constellation of Lyra - Constellation of Lyra - Constellation of Lyra with bright star Vega. Lyra, The Lyre is one of the 48 constellations listed by Ptolemy, and represents a stringed musical instrument widely used in Greek classical times. Apparently, the young god Hermes (Mercury) created the lyre from the body of a large tortoise shell covered with animal hide sporting antelope horns. The instrument is associated with the virtues of moderation and equilibrium, and was given by Hermes to his half - brother Apollo, who in turn gave it to his son Orpheus. Lyra is a small constellation, but rather obvious to the eye. Its principal star, Vega, is the second brightest star in the northern hemisphere and is also interesting because it is seen almost pole - on and is one of the most rapidly rotating stars known, so it could see it from a different direction it would appear distinctly flattened. Because of precession, Vega is destined to be the Pole Star in about 12,000 years. Entirely unco

Constellation of Lyra - Constellation of Lyra - Constellation of Lyra with bright star Vega. Lyra, The Lyre is one of the 48 constellations listed by Ptolemy, and represents a stringed musical instrument widely used in Greek classical times. Apparently, the young god Hermes (Mercury) created the lyre from the body of a large tortoise shell covered with animal hide sporting antelope horns. The instrument is associated with the virtues of moderation and equilibrium, and was given by Hermes to his half - brother Apollo, who in turn gave it to his son Orpheus. Lyra is a small constellation, but rather obvious to the eye. Its principal star, Vega, is the second brightest star in the northern hemisphere and is also interesting because it is seen almost pole - on and is one of the most rapidly rotating stars known, so it could see it from a different direction it would appear distinctly flattened. Because of precession, Vega is destined to be the Pole Star in about 12,000 years. Entirely unco

PIX4592258

The Phases of the Moon', c 1860

The Phases of the Moon', c 1860

UIS5090356

Skyline (photo)

Skyline (photo)

UIG2903526

Dusky Skyline (photo)

Dusky Skyline (photo)

UIG2903533

Instruments, Polariscopes Wheatstone Polar Clock, 1848-1860

Instruments, Polariscopes Wheatstone Polar Clock, 1848-1860

UIS5082813

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid wate

Geyser sur Enceladus - Artist view - Water geyser on Enceladus - Artist view - Artist view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid wate

Walter B Myers

PIX4625850

Sundials, Compass Octagonal Louis XVI sundial and compass, French, early 18th Century

Sundials, Compass Octagonal Louis XVI sundial and compass, French, early 18th Century

UIS5086422

Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253614

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

The Large Magellanic Cloud - The Large Magellanic Cloud - The Great Magellan Cloud galaxy is located about 160,000 light years away from Earth in the southern constellation of Dorado. Visible with the naked eye in the southern hemishere it is one of the closest galaxies to us. It contains large star-forming zones such as the Tarantula Nebula (30 Sea bream, visible to the left), the most active star-forming regions of the local group. Image obtained by the 1.2m UK Schmidt telescope from Siding Spring, Australia. The Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 160,000 light years and is visible to the unaided eye from southern latitudes, rather like a detached piece of the Milky Way. The nearness of the LMC ensures that it is well resolved into stars in quite a modest telescope, and deep

PIX4613427

Space lift on the Moon - Artist's view - Lunar elevator lunar base - Lunar base equipped with a space lift. A manned lunar space elevator prepares to depart from its manned lunar base. Surrounding it are support facilities and cargo. The yellow machine on the right is an articulated manned manipulator for handling cargo and managing the elevator. The space elevator concept involves running a cable from the surface of a planet or moon up to a gravitationally - stable point in space, whereupon a specially - designed vehicle can climb and descend the cable. Also known as tether propulsion and non-rocket space launch, this method permits an alternative way to access space. In the case of the lunar space elevator, the cable is anchored to the surface of the Moon and ascends to a stable Lagrange point. In this illustration the cable, in the form of a ribbon, is anchored to the southern hemisphere of the near - side of the Moon and ascends approximately 35,000 miles towards the Earth. The man

Space lift on the Moon - Artist's view - Lunar elevator lunar base - Lunar base equipped with a space lift. A manned lunar space elevator prepares to depart from its manned lunar base. Surrounding it are support facilities and cargo. The yellow machine on the right is an articulated manned manipulator for handling cargo and managing the elevator. The space elevator concept involves running a cable from the surface of a planet or moon up to a gravitationally - stable point in space, whereupon a specially - designed vehicle can climb and descend the cable. Also known as tether propulsion and non-rocket space launch, this method permits an alternative way to access space. In the case of the lunar space elevator, the cable is anchored to the surface of the Moon and ascends to a stable Lagrange point. In this illustration the cable, in the form of a ribbon, is anchored to the southern hemisphere of the near - side of the Moon and ascends approximately 35,000 miles towards the Earth. The man

Walter B Myers

PIX4640224

Simurgh Attacking a Gaja-Simha Carrying Elephants, early 19th century (opaque w/c & gold on paper)

Simurgh Attacking a Gaja-Simha Carrying Elephants, early 19th century (opaque w/c & gold on paper)

Indian School, (19th century)

PHL450964

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

Southern Aurora on the Planet Saturn - Aurora on Saturn - The Planet Saturn accompanied by a Southern Aurora, seen in visible and infrared by the Cassini probe on November 1, 2008. This false - color composite image, constructed from data obtained by Nasa's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 kilometers (600 miles) from the cloud tops of Saturn's south polar region. In this image constructed from data collected in the near - infrared wavelengths of light, the auroral emission is shown in green. Scientists designated blue to indicate sunlight reflected at wavelengths from 2 to 3 microns, green to indicate light from hydrogen ions at wavelengths between 3 and 4 microns and red to indicate thermal emission at 5 microns. Saturn's rings and high altitude haze only reflect sunlight at 3 microns or less, so they appear deep blue. The glow from the aurora can only be seen at the wavelengths in the green channel. The heat emission from the interior of Saturn

PIX4625211

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Geyser sur Enceladus - Artist's view - Water geyser on Enceladus - Artist's view of an ice geyser on the surface of the Enceladus satellite. In the sky, the planet Saturn and its satellite Mimas. Liquid water reaches the surface of Enceladus' south pole and drives a massive plume of ice crystals into the sky. The combination of Enceladus' low surface gravity and the geyser's force accelerate the crystals to escape velocity, where sunlight breaks the water molecules down into their constituent atoms of hydrogen and oxygen. Saturn itself appears low on the horizon due to the proximity to Enceladus' pole. The small object immediately to Saturn's left is another icy moon named Mimas. Somewhat smaller than Enceladus and closer to Saturn, Mimas sprints around Saturn in slightly less than one Earth day. In March 2006 Nasa's Cassini probe revealed evidence of water - driven geysers on the surface of Enceladus. At first glance Enceladus doesn't seem to be a likely host for liquid water as the s

Walter B Myers

PIX4625896

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253623

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253631

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Neptune - Illustration - Neptune's Great Dark Spot - Illustration - Artist's view of Neptune with its ring system and large dark spot observed by the Voyager 2 probe in 1989. This is how Neptune's Great Dark Spot and rings may have looked in 1989 from a position just beneath Neptune's ring plane. The outermost Adams ring is near the top of the frame, and beneath that is the much broader and diffuse Lassell ring. Further in toward Neptune and abutting the Lassell ring is the thin Le Verrier ring, and beyond that is the diffuse Galle ring. The Great Dark Spot is believed to be a storm similar to, but only half the size of, Jupiter's Great Red Spot. While Jupiter's Great Red Spot has been raging for at least 400 years, subsequent observations of Neptune's Great Dark Spot in 1994 by the Hubble Space Telescope revealed that this storm has since disappeared. The Great Dark Spot was a very dynamic weather system, generating massive, white clouds similar to high - altitude cirrus clouds on Ear

Walter B Myers

PIX4624042

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253619

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253628

The façade with the entrance door and the roses, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

The façade with the entrance door and the roses, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253610

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253616

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253621

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253627

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the frieze of the portal, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253633

The Phases of the Moon', c 1860

The Phases of the Moon', c 1860

UIS5096283

ArtistsÕ Aids, Camera Obscuras Backplate from Storer's ÔRoyal DelineatorÕ, c 1778

ArtistsÕ Aids, Camera Obscuras Backplate from Storer's ÔRoyal DelineatorÕ, c 1778

UIS5070769

Desaguliers' Cometarium, 1755

Desaguliers' Cometarium, 1755

UIS5062913

Condensation trains over Brittany - Airplane contrails over Brittany, France - A multitude of condensation trains caused by air traffic appear on this image obtained by the Terra satellite on 25 April 2004. This true - color Moderate Resolution Imaging Spectroradiometer (MODIS) image, acquired on April 25, 2004 by the Terra satellite, shows a web of contrails over northwestern Europe. These contrails are straight lines of ice crystals that form in the wake of jet liners where air temperatures at altitude are lower than about 40* C. Newer contrails are thin whereas older trails have widened with time as a result of light winds. The problem with contrails is that they can spread into extensive high, thin cirrus clouds, which tend to warm the Earth because they reflect less sunlight back to space than the amount of heat they trap

Condensation trains over Brittany - Airplane contrails over Brittany, France - A multitude of condensation trains caused by air traffic appear on this image obtained by the Terra satellite on 25 April 2004. This true - color Moderate Resolution Imaging Spectroradiometer (MODIS) image, acquired on April 25, 2004 by the Terra satellite, shows a web of contrails over northwestern Europe. These contrails are straight lines of ice crystals that form in the wake of jet liners where air temperatures at altitude are lower than about 40* C. Newer contrails are thin whereas older trails have widened with time as a result of light winds. The problem with contrails is that they can spread into extensive high, thin cirrus clouds, which tend to warm the Earth because they reflect less sunlight back to space than the amount of heat they trap

PIX4664981

Detail of the entrance door and the romanesque rose, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Detail of the entrance door and the romanesque rose, Entrance door, façade, Cathedral of St. Feliciano, Foligno, Umbria, Italy (photo)

Ghigo Roli

GRL6253607

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with 1000 employees. …, 1953 (photo)

Dale in Hordaland 19530425. Dale Fabrikker is Norway's largest textile factory with 1000 employees. …, 1953 (photo)

Sverre A. Børretzen

NTB8727760

Main Guard of camp at Jatta Post, 1919 circa (b/w photo)

Main Guard of camp at Jatta Post, 1919 circa (b/w photo)

Unknown photographer, (20th century)

NAM5923993

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20

Stephane Guisard

PIX4622088

Planetary nebula NGC 6781 - A planetary nebula, NGC 6781 - This fairly inconspicuous planetary nebula is in Aquila and it marks the end of the long life of a sun - like star. Despite the longevity of their parent stars and the very brief lifetime of the nebula (typically less than 100,000 years) such sights are common because sun - like stars are common. The nebula has nothing to do with planet formation, indeed the formation of the nebula would effectively destroy any planets the parent star had, rather the name refers to the telescopic appearance of the nebula. Some planetaries are very bright and their discs look like solar system planets. A close look at this picture shows some structure in the expanding shell of gas around the star, reminiscent of the much more complex Helix nebula. The nebula we see is the ejected surface of the star expanding into material left from an earlier stage in its decline, when it briefly expanded as a 'red giant'. Irregularities in the earlier ejecta,

Planetary nebula NGC 6781 - A planetary nebula, NGC 6781 - This fairly inconspicuous planetary nebula is in Aquila and it marks the end of the long life of a sun - like star. Despite the longevity of their parent stars and the very brief lifetime of the nebula (typically less than 100,000 years) such sights are common because sun - like stars are common. The nebula has nothing to do with planet formation, indeed the formation of the nebula would effectively destroy any planets the parent star had, rather the name refers to the telescopic appearance of the nebula. Some planetaries are very bright and their discs look like solar system planets. A close look at this picture shows some structure in the expanding shell of gas around the star, reminiscent of the much more complex Helix nebula. The nebula we see is the ejected surface of the star expanding into material left from an earlier stage in its decline, when it briefly expanded as a 'red giant'. Irregularities in the earlier ejecta,

PIX4623396

Desaguliers' Cometarium, 1755

Desaguliers' Cometarium, 1755

UIS5061218

pectoral and necklace of Psusennes I

pectoral and necklace of Psusennes I

Egyptian School

Sandro Vannini

SVA660202

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew exploration vehicle) type Orion is moored to the inflatable module. A spacious inflatable habitat is attached to the International Space Station (ISS) with a manned Crew Exploration Vehicle (CEV) docked on one end. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the other end of the habitat features an Interna

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew exploration vehicle) type Orion is moored to the inflatable module. A spacious inflatable habitat is attached to the International Space Station (ISS) with a manned Crew Exploration Vehicle (CEV) docked on one end. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the other end of the habitat features an Interna

Walter B Myers

PIX4641302

Circumpolar in Ecuador - Star Trail from the Equator (Ecuador) - Star line taken from Ecuador, Ecuador. 10 hours of cumulative poses show us more than 90% of all the visible sky (the remaining 10% are drowned in solar light). A shooting star indicates the South Pole to the horizon to the left of the image. The north pole is on the right horizon. This image is an unprecedented star trail image taken from the Equator (this imaginary line that splits the Earth into the two hemispheres) in Ecuador (the country). If you stand on the Equator line you can see the Southern Pole at the horizon to the South (left of the image) and the Northern pole at the horizon on the opposite direction. The Earth rotation will make all the sky and stars look like they rotate around these two points, making them appear as concentric circles (which look like ellipses on this distorsioning fish eye image). Note that on this image, that cumulates 10 hours of exposure starting 1 hour after sunset and finishing 1 h

Circumpolar in Ecuador - Star Trail from the Equator (Ecuador) - Star line taken from Ecuador, Ecuador. 10 hours of cumulative poses show us more than 90% of all the visible sky (the remaining 10% are drowned in solar light). A shooting star indicates the South Pole to the horizon to the left of the image. The north pole is on the right horizon. This image is an unprecedented star trail image taken from the Equator (this imaginary line that splits the Earth into the two hemispheres) in Ecuador (the country). If you stand on the Equator line you can see the Southern Pole at the horizon to the South (left of the image) and the Northern pole at the horizon on the opposite direction. The Earth rotation will make all the sky and stars look like they rotate around these two points, making them appear as concentric circles (which look like ellipses on this distorsioning fish eye image). Note that on this image, that cumulates 10 hours of exposure starting 1 hour after sunset and finishing 1 h

Stephane Guisard

PIX4581325

Planetary Nebula Hen - 1357 dans l'Altar/HST - This Wide Field and Planetary Camera 2 image captures the infancy of the Stingray nebula (Hen - 1357), the youngest known planetary nebula. In this image, the bright central star is in the middle of the green ring of gas. Its companion star is diagonally above it at 10 o'clock. A spur of gas (green) is forming a faint bridge to the companion star due to gravitational attraction. The image also shows a ring of gas (green) surrounding the central star, with bubbles of gas to the lower left and upper right of the ring. The wind of material propelled by radiation from the hot central star has created enough pressure to blow open holes in the ends of the bubbles, allowing gas to escape. The red curved lines represent bright gas that is heated by a “” shock””” caused when the central star's wind hits the walls of the bubbles. The nebula is as large as 130 solar systems, but, at its distance of 18,000 light - years, it appears only as big as a di

Planetary Nebula Hen - 1357 dans l'Altar/HST - This Wide Field and Planetary Camera 2 image captures the infancy of the Stingray nebula (Hen - 1357), the youngest known planetary nebula. In this image, the bright central star is in the middle of the green ring of gas. Its companion star is diagonally above it at 10 o'clock. A spur of gas (green) is forming a faint bridge to the companion star due to gravitational attraction. The image also shows a ring of gas (green) surrounding the central star, with bubbles of gas to the lower left and upper right of the ring. The wind of material propelled by radiation from the hot central star has created enough pressure to blow open holes in the ends of the bubbles, allowing gas to escape. The red curved lines represent bright gas that is heated by a “” shock””” caused when the central star's wind hits the walls of the bubbles. The nebula is as large as 130 solar systems, but, at its distance of 18,000 light - years, it appears only as big as a di

PIX4623698

The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays pr

The Dawn probe near Ceres - Artist's view - Dawn approaches Ceres - Artist view of the Dawn probe near the dwarf planet Ceres. In February 2015 the unmanned Dawn spacecraft is scheduled to arrive at the dwarf planet Ceres. The 65 foot long, 2.5 ton probe was launched from the Earth in 2007, passed March in 2009, and went into orbit around the protoplanet Vesta in July 2011 where it stayed until September 2012. Once in orbit around Ceres, Dawn is expected to operate for about a year making observations of this largest object in the asteroid belt. In this image Dawn's three xenon electrostatic ion thrusters can be seen emitting ionized xenon's characteristic blue/magenta glow, gently propelling the probe toward Ceres. While the ion engines have relatively low specific thrust (about equal to the weight of a few sheets of paper), they can operate continuously for long periods making efficient use of the approximately 1,000 pounds of xenon propellant onboard. The wing - like solar arrays pr

Walter B Myers

PIX4607298

Talatat: Men Hoeing the Earth, c.1353-1347 BC (painted sandstone)

Talatat: Men Hoeing the Earth, c.1353-1347 BC (painted sandstone)

Egyptian 18th Dynasty (c.1567-1320 BC)

XCL499508

Comet C/2016 R2 Panstarrs the blue carbon monoxide comet - rotating comet tails on January 19th 2018 (digital photo)

Comet C/2016 R2 Panstarrs the blue carbon monoxide comet - rotating comet tails on January 19th 2018 (digital photo)

Rhemann, Gerald (21st century)

MMM7340358

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew Exploration Vehicle) type Orion prepares to moor to the inflatable module. A manned Crew Exploration Vehicle (CEV) prepares to dock with a spacious inflatable habitat attached to the International Space Station (ISS) at an altitude of 250 nautical miles. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the othe

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew Exploration Vehicle) type Orion prepares to moor to the inflatable module. A manned Crew Exploration Vehicle (CEV) prepares to dock with a spacious inflatable habitat attached to the International Space Station (ISS) at an altitude of 250 nautical miles. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the othe

Walter B Myers

PIX4641303

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew Exploration Vehicle) type Orion prepares to moor to the inflatable module. A manned Crew Exploration Vehicle (CEV) prepares to dock with a spacious inflatable habitat attached to the International Space Station (ISS) at an altitude of 250 nautical miles. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the othe

ISS and inflatable module - Large habitat and ISS: Artist's view of a large inflatable module (much larger than all existing modules) installed on the International Space Station (ISS). A live module or CEV (Crew Exploration Vehicle) type Orion prepares to moor to the inflatable module. A manned Crew Exploration Vehicle (CEV) prepares to dock with a spacious inflatable habitat attached to the International Space Station (ISS) at an altitude of 250 nautical miles. This inflatable habitat, much larger than any existing ISS module, is a combination of layers of flexible material capped by sturdy docking hardware at either end. The inflatable portion is collapsed and sandwiched between the docking hardware portions for launch from earth and then inflated and pressurized with a breathable atmosphere once in orbit. The habitat features a pair of 42 x 24 inch windows to the outside. The habitat is attached to a pressurized module of the ISS via a Common Berthing Mechanism (CBM) while the othe

Walter B Myers

PIX4641310

Mars - View of the north pole - Mars north pole - Image based on altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It's about 1100 km long. The ice - rich north polar cap (the quasi - circular white area at center) is approximately 1,000 kilometers (621 miles) across. The white cap is riven with dark, spiral - shaped bands. These are deep troughs that are in shadow. They do not reflect sunlight as well or have more internal layers exposed. To the right of center, a large canyon, Chasma Boreale, almost bisects the ice cap. Chasma Boreale is about the length of the United States' famous Grand Canyon and up to 2 kilometers (1.2 miles) deep. The image synthesizes topographic data from Mars Orbiter Laser Altimeter (MOLA) and images from the Mars Orbiter Camera (MOC)

Mars - View of the north pole - Mars north pole - Image based on altimetric data obtained by the Mars Global Surveyor probe. The northern polar cap is mostly made up of water ice. It's about 1100 km long. The ice - rich north polar cap (the quasi - circular white area at center) is approximately 1,000 kilometers (621 miles) across. The white cap is riven with dark, spiral - shaped bands. These are deep troughs that are in shadow. They do not reflect sunlight as well or have more internal layers exposed. To the right of center, a large canyon, Chasma Boreale, almost bisects the ice cap. Chasma Boreale is about the length of the United States' famous Grand Canyon and up to 2 kilometers (1.2 miles) deep. The image synthesizes topographic data from Mars Orbiter Laser Altimeter (MOLA) and images from the Mars Orbiter Camera (MOC)

PIX4615389

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

PIX4572090

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

Center of the Omega Nebula (M17) in the sagittarius seen by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls

PIX4620193

Horse's Head Nebula (IC 434) in Orion - Horsehead nebula in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star

Horse's Head Nebula (IC 434) in Orion - Horsehead nebula in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light of the Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star

PIX4621983

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

Pluto seen by the New Horizons probe - Pluto seen by New Horizons - Pluto's atmosphere seen by the New Horizons probe. Image obtained on July 14, 2015 at a distance of 200,000 km from the dwarf planet. Mosaic of six images. This is the high-resolution color departure shot of Pluto's receding crescent from Nasa's New Horizons spacecraft, taken when the spacecraft was 120,000 miles (200,000 kilometers) away from Pluto. Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager (LORRI), with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera (MVIC) color image, all acquired between 15:20 and 15:45 UT - about 3.5 hours after closest approach to Pluto - on July 14, 2015. The resolution of the LORRI images is about 0.6 miles (1 kilometer) per pixel; the sun illuminates the scene from the other side of Pluto and somewhat towards the top of this image. The image is dominated by s

PIX4582251

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant sta

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant sta

PIX4622085

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. This Giant Galaxy is a powerful radio source known as Centaurus A. It is an active galaxy whose energy comes from a supermassive black hole. This image obtained by the Kueyen telescope of the VLT in Chile on 1 February 2000 shows the star flames that occur in the dark band of the galaxy. Centaurus A is one of the foremost examples of a radio - loud active galactic nucleus (AGN). On images obtained at optical wavelengths, thick dust layers almost completely obscure the galaxy's centre. Until 1949, NGC 5128 was thought to be a strange object in the Milky Way, but it was then identified as a powerful radio galaxy and designated Centaurus A. The distance is about 10 - 13 million light - years (3 - 4 Mpc) and the apparent visual magnitude is about 8, or 5 times too faint to be seen with the unaided eye. There is strong evidence th

PIX4612179

Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possi

Nebula NGC 7023 in Cephee - NGC 7023 (The Iris Nebula) in Cepheus - The Iris Nebula (NGC 7023) is a reflexion nebula illuminated by the massive star HD 200775. The bright star HD 200775 shining through the nebula NGC 7023 is a 10 solar mass star centrally imbedded in a region surrounded by ambient molecular cloud material. Suns are born from vast clouds of dust and gas that gather in the dark places between the stars. Gravity causes these interstellar vapors to collapse inward until the pressure causes high enough temperatures at its center to fuse hydrogen, the university's basic building block, into helium - an event that also releases gamma - ray photons. These photons can take a million years to travel outward through the overlying matter until they reach the surface and escape into space as visible light. The push of the photon's rush to make an exit also stops the cloud's collapse and thus what began as thin gas and dust becomes a brilliant star illuminating the heavens and possi

Adam Block

PIX4620555

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant sta

Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant sta

PIX4622070

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Exoplanets around 70 Virginis - A jovian planet orbiting 70 Virginis - Artist's view of the extrasolar planet 70 Vir B, a giant gas planet orbiting around a solar star, about 78 years old - light from the Sun. This exoplanet has about 6 times the mass of Jupiter and its distance from its star 70 Virginis is almost the same as that of Mercury from the Sun. A ringed 70 Vir B presides over the hot and airless terrain of a hypothetical moon. While it is not known if 70 Vir B has rings, it is certainly possible. 70 Vir B's rings would have no ice in them due to is proximity to its sun. Such rings would likely be less than 100 million years old and could have been formed from the shattered remnants of an asteroid that wondered too close to this giant planet. 70 Vir B's eccentric orbit would increase the likelihood of its encountering other objects in orbit around 70 Virginis. About 78 light years from the Earth astronomers believe that there is a large planet orbiting 70 Virginis, a type G5V

Walter B Myers

PIX4573224

Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. NGC 6164 - 65 is a bipolar nebula surrounding the peculiar O 7f star HD 148937. Although the nebula was believed initially to represent a planetary nebula, it is now understood to represent a shell - like ejected nebula, formed by the winds of its young central star. Wind blown nebulae are usually considered the outcome of Wolf - Rayet type stars (WR), evolved O - type stars that have left the main sequence, molding their surroundings by way of fierce stellar winds. In the case of the S - shaped bipolar nebula NGC 6164 - 65, the central star is not a WR star, but a young O - type supergiant of 40 solar masses. Relatively few examples of such objects are known to exist, making NGC 6164 - 5 particularly unique. The true age of the star is not known although estimates of its a

Nebula NGC 6164 - 5 in the Rule - The emission nebula NGC 6164 - 65 - This nebula is located about 4000 years - light from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937. NGC 6164 - 65 is a bipolar nebula surrounding the peculiar O 7f star HD 148937. Although the nebula was believed initially to represent a planetary nebula, it is now understood to represent a shell - like ejected nebula, formed by the winds of its young central star. Wind blown nebulae are usually considered the outcome of Wolf - Rayet type stars (WR), evolved O - type stars that have left the main sequence, molding their surroundings by way of fierce stellar winds. In the case of the S - shaped bipolar nebula NGC 6164 - 65, the central star is not a WR star, but a young O - type supergiant of 40 solar masses. Relatively few examples of such objects are known to exist, making NGC 6164 - 5 particularly unique. The true age of the star is not known although estimates of its a

PIX4619228

Rāma and Rāvaṇa renew their assaults on each other. The gods have decided that the contest is unequal, since Rāvaṇa is in his chariot while Rāma is on foot, so MÄtali, charioteer of the god Indra, at his master's command brings to Rāma Indra's chariot, with Indra's arms and armour in it (arms only according to the text). As a divine happening, MÄtali's meeting with Rāma is depicted over the horizon. MÄtali drives Rāma (now clad in Indra's golden armour) and Lakṣmaṇa into battle, the chariot's pennant being the solar standard of Mewar. Rāvaṇa in his chariot with its serpent standard advances to meet him. The two exchange furious onslaughts on each other as well as threats, but Rāma's attack, combined with the assaults of the monkeys, prove too much for Rāvaṇa, and his charioteer removes him from the battlefield for a respite, much to his master's fury.

Rāma and Rāvaṇa renew their assaults on each other. The gods have decided that the contest is unequal, since Rāvaṇa is in his chariot while Rāma is on foot, so MÄtali, charioteer of the god Indra, at his master's command brings to Rāma Indra's chariot, with Indra's arms and armour in it (arms only according to the text). As a divine happening, MÄtali's meeting with Rāma is depicted over the horizon. MÄtali drives Rāma (now clad in Indra's golden armour) and Lakṣmaṇa into battle, the chariot's pennant being the solar standard of Mewar. Rāvaṇa in his chariot with its serpent standard advances to meet him. The two exchange furious onslaughts on each other as well as threats, but Rāma's attack, combined with the assaults of the monkeys, prove too much for Rāvaṇa, and his charioteer removes him from the battlefield for a respite, much to his master's fury.

BL3283144

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

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

Centre de la nebula Omega (M17) by HST - Center of the Omega Nebula, a hotbed of newly born stars wrapped in colorful blankets of glowing gas and cradled in an enormous cold, dark hydrogen cloud. This picture was taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope. The region of the nebula shown in this photograph is about 3,500 times wider than our solar system. The area represents about 60 percent of the total view captured by ACS. The nebula, also called M17 and the Swan Nebula, resides 5,500 light - years away in the constellation Sagittarius. Like its famous cousin in Orion, the Swan Nebula is illuminated by ultraviolet radiation from young, massive stars, located just beyond the upper right corner of the image. Each star is about six times hotter and 30 times more massive than the Sun. The powerful radiation from these stars evaporates and erodes the dense cloud of cold gas within which the stars formed. The blistered walls of the hollow cloud shin

PIX4620159

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

Super massive star Eta Carinae - Super massive star Eta Carinae - Eta Carinae is one of the most massive stars in our galaxy. Its mass would be about 120 times that of the Sun with a diameter 1000 times larger than our star. The image obtained by the Hubble space telescope reveals two expanding gas lobes; it is the nebula called the Homuncule, vestige of a huge explosion that the star experienced 150 years ago. The star blows its exterior atmosphere and will eventually explode in a supernova. Eta Carinae is located approximately 8000 light years from Earth in the southern constellation of Carene. A huge, billowing pair of gas and dust clouds is captured in this stunning Hubble telescope picture of the super - massive star Eta Carinae. Even though Eta Carinae is more than 8,000 light - years away, features 10 billion miles across (about the diameter of our solar system) can be distinguished. Eta Carinae suffered giant outburst about 150 years ago, when it became one of the brightest sta

PIX4572109

Nebula NGC 6164-5 in the Rule - The emission nebula NGC 6164-65: This nebula is located about 4000 light years from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937 - NGC 6164-65 is a bipolar nebula surrounding the peculiar O 7f star HD 148937. Although the nebula was believed initially to represent a planetary nebula, it is now understood to represent a shell-like ejected nebula, formed by the winds of its young central star. Wind blown nebulae are usually considered the outcome of Wolf-Rayet type stars (WR), evolved O-type stars that have left the main sequence, molding their surroundings by way of fierce stellar winds. In the case of the S-shaped bipolar nebula NGC 6164-65, the central star is not a WR star, but a young O-type supergiant of 40 solar masses. Relatively few examples of such objects are known to exist, making NGC 6164-65 particularly unique. The true age of the star is not known although estimates of its age vary from a pre-ma

Nebula NGC 6164-5 in the Rule - The emission nebula NGC 6164-65: This nebula is located about 4000 light years from Earth. It is a bipolar nebula around a very hot star at the end of life, the star HD 148937 - NGC 6164-65 is a bipolar nebula surrounding the peculiar O 7f star HD 148937. Although the nebula was believed initially to represent a planetary nebula, it is now understood to represent a shell-like ejected nebula, formed by the winds of its young central star. Wind blown nebulae are usually considered the outcome of Wolf-Rayet type stars (WR), evolved O-type stars that have left the main sequence, molding their surroundings by way of fierce stellar winds. In the case of the S-shaped bipolar nebula NGC 6164-65, the central star is not a WR star, but a young O-type supergiant of 40 solar masses. Relatively few examples of such objects are known to exist, making NGC 6164-65 particularly unique. The true age of the star is not known although estimates of its age vary from a pre-ma

PIX4619260

outer sarcophagus of Khonsu

outer sarcophagus of Khonsu

Egyptian School

Sandro Vannini

SVA660198

«
1
…
435
436
437
…
438
»

Perchè scegliere Bridgeman Images

Arte. Cultura. Storia.

Collaboriamo con i principali musei, artisti e gallerie del mondo per darti accesso a immagini di altissima qualità.

Scopri la nostra collezione Sfoglia le domande frequenti

Semplice. Rapido. Affidabile.

Il nostro team ti può aiutare a trovare l'immagine perfetta per il tuo progetto, occupandosi di tutte le necessità di copyright e licenza.

Contattaci

Scoprite milioni di immagini e video per i vostri progetti creativi.

Inizia la tua ricerca

© Copyright 2024 Bridgeman Art Library Limited. Registrata in Inghilterra e Galles con numero di società 01056394