'Tierra' images and/or videos results

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

Your ongoing selection

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4612278","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_centaurus_galaxy_centaurus_a_ngc_5128_the_galaxy_ngc_5128_","item_variant":"undefined"},{"item_id":"MMM7341748","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"wyllie_william_lionel_1851_1931","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_german_high_seas_fleet_caged_in_scapa_c_1918_wash_grey_heightened_with_white","item_variant":"undefined"},{"item_id":"SRB1202745","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_temples_of_angkor_angkor_cambodia_photo","item_variant":"undefined"},{"item_id":"SRB3584743","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"inside_the_archaeological_complex_of_machu_picchu_peru_photo","item_variant":"undefined"},{"item_id":"NAM5922558","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"cable_railway_table_mountain_3rd_county_of_london_yeomanry_sharpshooters_shore_leave_en_route_to_egy","item_variant":"undefined"},{"item_id":"BOF2650251","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cuban_crisis_missiles_removed_1962","item_variant":"undefined"},{"item_id":"BL3296263","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"after_archbishop_hubert_walter_s_death_in_1205_and_the_rejection_of_other_nominees_to_the_see_of_can","item_variant":"undefined"},{"item_id":"DPA2493613","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"new_york","item_variant":"undefined"},{"item_id":"NAM5920291","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"unknown_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"group_of_kalash_kafirs_1919_b_w_photo","item_variant":"undefined"},{"item_id":"PFH1774481","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"burma_myanmar_the_building_housing_the_mingun_bell_in_sagaing_division_burma","item_variant":"undefined"},{"item_id":"SRB3584744","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"inside_the_archaeological_complex_of_machu_picchu_peru_photo","item_variant":"undefined"},{"item_id":"SRB1202746","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_temples_of_angkor_angkor_cambodia_photo","item_variant":"undefined"},{"item_id":"SRB1202747","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_temples_of_angkor_angkor_cambodia_photo","item_variant":"undefined"},{"item_id":"SRB1202895","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"beach_in_one_foot_island_aitutaki_cook_island_polynesia_south_pacific_ocean_photo","item_variant":"undefined"},{"item_id":"SRB1202896","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"beach_in_one_foot_island_aitutaki_cook_island_polynesia_south_pacific_ocean_photo","item_variant":"undefined"},{"item_id":"PIX4616696","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_phoenix_probe_on_its_landing_site_phoenix_landing_site_mosaic_of_polar_projection_images_showing","item_variant":"undefined"},{"item_id":"PIX4613022","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"irregular_galaxy_ngc_6822_in_sagittarius_irregular_galaxy_ngc_6822_in_sagittarius_the_galaxy_ngc_682","item_variant":"undefined"},{"item_id":"PIX4613167","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_7331_in_pegase_spiral_galaxy_ngc_7331_in_pegasus_the_galaxy_ngc_7331_is_located_ab","item_variant":"undefined"},{"item_id":"PIX4564335","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_ngc_1806_in_dorado_globular_cluster_ngc_1806_in_dorado_image_of_the_globular_cluste","item_variant":"undefined"},{"item_id":"PIX4572253","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_field_in_the_constellation_sagittarius_scattered_stars_in_sagittarius_stars_in_sagittarius_seen","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":"PIX4609816","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1345_in_eridan_barred_spiral_galaxy_ngc_1345_in_eridanus_located_about_85_m","item_variant":"undefined"},{"item_id":"PIX4611051","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_4038_4039_in_the_raven_the_antennae_galaxy_in_corvus_on_the_left_seen_from_","item_variant":"undefined"},{"item_id":"PIX4649416","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"decolishing_the_space_shuttle_atlantis_05_2010_space_shuttle_atlantis_lift_off_05_2010_decolving_the","item_variant":"undefined"},{"item_id":"NAM5923192","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"regimental_parade_on_quayside_3rd_county_of_london_yeomanry_sharpshooters_cape_town_south_africa_en_","item_variant":"undefined"},{"item_id":"NAM5922560","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"orion_leaving_cape_town_3rd_county_of_london_yeomanry_sharpshooters_on_board_hmt_orion_en_route_to_e","item_variant":"undefined"},{"item_id":"NAM5929361","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"velde_willem_van_de_the_elder_1611_93","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_grand_review_on_hounslow_heath_1687_pen_and_ink_with_wash","item_variant":"undefined"},{"item_id":"PRX3116722","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"poussin_nicolas_1594_1665_after","item_category5":"not_balown","item_list_name":"search_results","item_name":"moses_defending_the_daughters_colour_litho","item_variant":"undefined"},{"item_id":"PIX4583175","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"supernova_remnants_snr_b0509_67_5_supernova_remnant_snr_b0509_67_5_snr_b0509_67_5_or_snr_0509_is_the","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":"PIX4610335","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4569076","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_cluster_of_stars_pismis_24_in_the_scorpio_pismis_24_star_cluster_in_scorpius_this_image_obtained","item_variant":"undefined"},{"item_id":"PIX4649419","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"decolishing_the_space_shuttle_atlantis_05_2010_space_shuttle_atlantis_lift_off_05_2010_decolving_the","item_variant":"undefined"},{"item_id":"PIX4645744","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"james_webb_space_telescope_mirrors_jwst_testing_of_the_jwst_s_mirrors_six_of_the_18_jwst_james_webb_","item_variant":"undefined"},{"item_id":"PFH1774480","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"burma_myanmar_the_mingun_bell_in_sagaing_division_burma","item_variant":"undefined"},{"item_id":"NAM5922555","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"jenner_jones_freddie_crowley_john_grimwade_table_mountain_3rd_county_of_london_yeomanry_sharpshooter","item_variant":"undefined"},{"item_id":"NAM5922556","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"top_of_the_mountain_freddie_crowley_jimmy_sale_table_mountain_3rd_county_of_london_yeomanry_sharpsho","item_variant":"undefined"},{"item_id":"NAM5923188","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"orion_docked_troops_on_quayside_3rd_county_of_london_yeomanry_sharpshooters_cape_town_south_africa_e","item_variant":"undefined"},{"item_id":"SRB3584745","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"inside_the_archaeological_complex_of_machu_picchu_peru_photo","item_variant":"undefined"},{"item_id":"NAM5928231","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"unknown_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"wounded_being_brought_on_board_a_destroyer_off_dieppe_august_1942_b_w_photo","item_variant":"undefined"},{"item_id":"PIX4623359","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_m57_ngc_6720_in_lyra_m57_ngc_6720_planetary_nebula_in_lyra_the_planetary_nebula_of_","item_variant":"undefined"},{"item_id":"PIX4617504","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_cluster_ic_1590_in_ngc_281_cassiopee_open_cluster_and_bok_globules_in_ngc_281_view_of_a_detail_","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":"PIX4610399","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_in_the_great_bear_spiral_galaxy_m81_in_ursa_major_the_spiral_galaxy_m81_is_located","item_variant":"undefined"},{"item_id":"PIX4613035","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_6872_in_interaction_with_ic_4970_in_the_peacock_barred_spiral_interacting_g","item_variant":"undefined"},{"item_id":"PIX4574313","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_7098_barred_spiral_galaxy_ngc_7098_the_barree_spiral_galaxy_ngc_7098_is_loc","item_variant":"undefined"},{"item_id":"PIX4618453","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_of_the_rosette_in_the_unicorn_seen_in_false_colors_rosette_nebula_in_monoceros_the_nebula_of_","item_variant":"undefined"},{"item_id":"PIX4649404","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"decolishing_the_space_shuttle_atlantis_05_2010_space_shuttle_atlantis_lift_off_05_2010_decolving_the","item_variant":"undefined"},{"item_id":"PIX4648054","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"depart_of_astronauts_sts_107_01_2003_sts_107_crew_is_going_to_launch_pad_16_01_2003_the_crew_of_the_","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":"PIX4565685","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cl0024_17_galaxy_cluster_cl0024_17_galaxy_cluster_cl0024_17_cl0024_17_galaxy_cluster_located_about_5","item_variant":"undefined"},{"item_id":"BEG752383","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"drawings_made_in_secret_by_women_from_a_women_s_camp_in_indonesia_about_their_living_conditions","item_variant":"undefined"},{"item_id":"SRB1202744","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_temples_of_angkor_angkor_cambodia_photo","item_variant":"undefined"},{"item_id":"PFH1774479","item_category2":"no_copyright","item_category3":"standard","item_category4":"david_henley","item_category5":"not_balown","item_list_name":"search_results","item_name":"burma_myanmar_the_mingun_bell_in_sagaing_division_burma","item_variant":"undefined"},{"item_id":"SRB3584747","item_category2":"no_copyright","item_category3":"standard","item_category4":"sergi_reboredo","item_category5":"not_balown","item_list_name":"search_results","item_name":"terraces_inside_the_archaeological_complex_of_machu_picchu_peru_photo","item_variant":"undefined"},{"item_id":"NAM5922554","item_category2":"no_copyright","item_category3":"standard","item_category4":"sale_wilfred_herbert_james","item_category5":"not_balown","item_list_name":"search_results","item_name":"3rd_county_of_london_yeomanry_sharpshooters_shore_leave_table_mountain_cape_town_en_route_to_egypt_1","item_variant":"undefined"},{"item_id":"MOD6437290","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"sardinia_the_future_is_called_rebirth_1968","item_variant":"undefined"},{"item_id":"MMM7295642","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"fanshawe_admiral_sir_edward_gennys_1814_1906","item_category5":"not_balown","item_list_name":"search_results","item_name":"hms_daphne_off_cape_horn_28_may_1852_watercolour","item_variant":"undefined"},{"item_id":"MMM7340624","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"hornbrook_thomas_l_1780_1850","item_category5":"not_balown","item_list_name":"search_results","item_name":"hms_britannia_sailing_from_the_hamoaze_to_plymouth_sound_with_the_duke_of_clarence_on_board_as_lord_","item_variant":"undefined"},{"item_id":"NAM5920290","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"unknown_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"kafir_archers_1919_b_w_photo","item_variant":"undefined"}]}}

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

Advanced Search Search Tips

Images of 'Tierra' found, 46,701

«
1
…
773
774
775
…
779
»

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. 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. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

Centaurus A elliptical galaxy (NGC 5128) in Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million light years away from Earth in the southern constellation of Centaurus. A broad dark band crosses it in the middle, a probable vestige of a collision with a spiral galaxy. 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. The green dot visible in the dust strip is a supernova, the supernova 1986g. It appears green because the red filter image that made this trichromy image was only taken a year after the event and the supernova had weakened. Image obtained from the 3.9m telescope of Siding Spring, Australia. Centaurus A is a most unusual galaxy. The circular, uniformly bright portion is composed of several thousand million stars, most of them old and yellowish. The galaxy is girded by a dense dust lane which obscures and reddens the light of stars behind it. Some

PIX4612278

The German High Seas Fleet caged in Scapa, c.1918 (wash, grey, heightened with white)

The German High Seas Fleet caged in Scapa, c.1918 (wash, grey, heightened with white)

Wyllie, William Lionel (1851-1931)

MMM7341748

The Temples of Angkor, Angkor, Cambodia (photo)

The Temples of Angkor, Angkor, Cambodia (photo)

Sergi Reboredo

SRB1202745

Inside the archaeological complex of Machu Picchu, Peru (photo)

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584743

Cable railway. Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, en route to Egypt, 1941 (b/w photo)

Cable railway. Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5922558

Cuban Crisis Missiles Removed 1962

Cuban Crisis Missiles Removed 1962

BOF2650251

After Archbishop Hubert Walter's death in 1205 and the rejection of other nominees to the see of Canterbury, the monks of Christ Church elected Stephen Langton (d. 1228) as Walter's successor. King John's refusal to accept Langton's election led to the kingdom of England being placed under a papal Interdict in 1208, prohibiting the people from receiving the sacraments or being buried in consecrated ground. Few contemporary accounts have survived from that time, an exception being the Chronicon Anglicanum, written by Ralph (fl. 1207-26), Abbot of Coggeshall Abbey in Essex. There is an abrupt change in Ralph's chronicle for the years 1206 to 1212, roughly coinciding with the Interdict; previously, Ralph had made extensive notes about the events of each year, but for this period he provided a summary instead. The autograph manuscript of the Chronicon Anglicanum reveals that the original account had been removed and a replacement inserted. It is possible that Ralph of Coggeshall purged the

After Archbishop Hubert Walter's death in 1205 and the rejection of other nominees to the see of Canterbury, the monks of Christ Church elected Stephen Langton (d. 1228) as Walter's successor. King John's refusal to accept Langton's election led to the kingdom of England being placed under a papal Interdict in 1208, prohibiting the people from receiving the sacraments or being buried in consecrated ground. Few contemporary accounts have survived from that time, an exception being the Chronicon Anglicanum, written by Ralph (fl. 1207-26), Abbot of Coggeshall Abbey in Essex. There is an abrupt change in Ralph's chronicle for the years 1206 to 1212, roughly coinciding with the Interdict; previously, Ralph had made extensive notes about the events of each year, but for this period he provided a summary instead. The autograph manuscript of the Chronicon Anglicanum reveals that the original account had been removed and a replacement inserted. It is possible that Ralph of Coggeshall purged the

BL3296263

New York

New York

DPA2493613

Group of Kalash Kafirs, 1919 (b/w photo)

Group of Kalash Kafirs, 1919 (b/w photo)

Unknown photographer, (20th century)

NAM5920291

Burma / Myanmar: The building housing the Mingun Bell in Sagaing Division, Burma

Burma / Myanmar: The building housing the Mingun Bell in Sagaing Division, Burma

David Henley

PFH1774481

Inside the archaeological complex of Machu Picchu, Peru (photo)

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584744

The Temples of Angkor, Angkor, Cambodia (photo)

The Temples of Angkor, Angkor, Cambodia (photo)

Sergi Reboredo

SRB1202746

The Temples of Angkor, Angkor, Cambodia (photo)

The Temples of Angkor, Angkor, Cambodia (photo)

Sergi Reboredo

SRB1202747

Beach in One Foot Island, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Beach in One Foot Island, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Sergi Reboredo

SRB1202895

Beach in One Foot Island, Aitutaki, Cook Island, Polynesia , South Pacific Ocean (photo)

Beach in One Foot Island, Aitutaki, Cook Island, Polynesia , South Pacific Ocean (photo)

Sergi Reboredo

SRB1202896

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

The Phoenix probe on its landing site - Phoenix landing site - Mosaic of polar projection images showing the Phoenix probe placed on Martian soil. The black circle corresponds to the position of the probe camera. The hundreds of clicks needed to make this image were taken between June 5 and July 12, 2008. Phoenix landed on a vast plain north of Mars, in the Vastitas Borealis region. This view is a polar projection that combines more than 500 exposures taken by the Surface Stereo Imager camera on Nasa's Mars Phoenix Lander and projects them as if looking down from above. The black circle on the spacecraft is where the camera itself is mounted on the lander, out of view in images taken by the camera. North is toward the top of the image. The lander's meteorology mast extends above the southwest horzon and is topped by the telltale wind gauge. The ground surface around the lander has polygonal patterning similar to patterns in permafrost areas on Earth. The landing site is at 68.22 degree

PIX4616696

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is about 1.6 million years away - light from Earth. She belongs to our local group. Image obtained with a telescope of 35 cm, 12 hours of poses. The irregular dwarf galaxy NGC 6822 is located at only 1,6 million light year. It is a member of our local group and the third nearest galaxy to the Milky Way after the Sagittarius Dwarf Elliptical and the Magellanic Clouds. The galaxy was discovered by Barnard in 1881 using a 6 inch refractor. It is very similar to the LMC with its weak bar and its irregular distribution of bright OB associations and HII regions. In 1925 in a classic paper, Edwin Hubble reported on several bright objects in NGC 6822, later found to represent a grouping of bright star clusters and HII regions. The galaxy is rich in neutral hydrogen gas, the essential fuel of star formation. NGC 6822 started forming stars some 10 billion years ago. Similar to the LMC it has

R. Gendler

PIX4613022

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus: The galaxy NGC 7331 is located about 45 million light years away from Earth. Image obtained with the Hubble Space Telescope. NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it's beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble's Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star - a supernova - which can still be faintly seen as a tiny red dot near the galaxy's central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich - in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the

Spiral galaxy NGC 7331 in Pegase - Spiral galaxy NGC 7331 in Pegasus: The galaxy NGC 7331 is located about 45 million light years away from Earth. Image obtained with the Hubble Space Telescope. NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it's beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble's Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star - a supernova - which can still be faintly seen as a tiny red dot near the galaxy's central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich - in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the

PIX4613167

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

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

PIX4564335

Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are sma

Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are sma

PIX4572253

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

Barree spiral galaxy NGC 1345 in Eridan - Barred Spiral galaxy NGC 1345 in Eridanus - Located about 85 million years ago - light from Earth, NGC 1345 is a barree spiral galaxy located in the constellation Eridan. This galaxy belongs to the Eridan galaxy cluster, a group of 70 galaxies. Many galaxies are visible in the background. The spiral galaxy NGC 1345 and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster - - a group of about 70 galaxies that lies 85 million light - years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light - years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster. Apart from the main galaxy that dominates the picture, lots more di

Barree spiral galaxy NGC 1345 in Eridan - Barred Spiral galaxy NGC 1345 in Eridanus - Located about 85 million years ago - light from Earth, NGC 1345 is a barree spiral galaxy located in the constellation Eridan. This galaxy belongs to the Eridan galaxy cluster, a group of 70 galaxies. Many galaxies are visible in the background. The spiral galaxy NGC 1345 and its loose and ragged arms dominate this rich image from the NASA/ESA Hubble Space Telescope. It is a member of the Eridanus Galaxy Cluster - - a group of about 70 galaxies that lies 85 million light - years away in the constellation of Eridanus (the River). This region of the night sky is well populated with bright galaxies, with the Fornax Cluster of galaxies also nearby on the celestial sphere, although the two clusters are actually separated by about 20 million light - years. Collectively, they are known as the Fornax Supercluster or the Southern Supercluster. Apart from the main galaxy that dominates the picture, lots more di

PIX4609816

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

Interacting galaxies NGC 4038 - 4039 in the Raven - The Antennae galaxy in Corvus - On the left, seen from the ground of the galaxy NGC 4038 - 39 (antenna galaxy), located about 45 million years ago - light. These two galaxies are interacting. The collision started at least 100 million years ago causes intense star formation. On the right, the image made by the space telescope Hubble on 20 January 1996 shows in detail the nuclei of these two twin galaxies surrounded by young clusters of blue stars, more than 1000, made up of young and massive stars. At left, a ground - based telescopic view of the Antennae galaxies (known formally as NGC 4038/4039) - so named because a pair of long tails of luminous matter, formed by the gravitational tidal forces of their encounter, resemble an insect's antennae. The galaxies are located 45 million light - years away in the southern constellation Corvus. At right, the respective cores of the twin galaxies are the orange blobs, left and right of image

PIX4611051

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649416

Regimental parade on quayside, 3rd County of London Yeomanry (Sharpshooters), Cape Town, South Africa, en route to Egypt, 1941 (b/w photo)

Regimental parade on quayside, 3rd County of London Yeomanry (Sharpshooters), Cape Town, South Africa, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5923192

Orion leaving Cape Town, 3rd County of London Yeomanry (Sharpshooters) on board HMT Orion, en route to Egypt, 1941 (b/w photo)

Orion leaving Cape Town, 3rd County of London Yeomanry (Sharpshooters) on board HMT Orion, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5922560

A Grand Review on Hounslow Heath, 1687 (pen and ink with wash)

A Grand Review on Hounslow Heath, 1687 (pen and ink with wash)

Velde, Willem van de, the Elder (1611-93)

NAM5929361

Moses defending the Daughters (colour litho)

Moses defending the Daughters (colour litho)

Poussin, Nicolas (1594-1665) (after)

PRX3116722

Supernova Remnants SNR B0509 - 67.5 - Supernova Remnant SNR B0509 - 67.5 - SNR B0509 - 67.5 (or SNR 0509) is the rest of a star explosion in the galaxy of the Great Magellan Cloud. This 23-year bubble - light of diameter extends at a speed of 18 million km/h. Composite of images obtained by the Hubble Space Telescope (HST) in 2006 and 2010. This delicate shell, photographed by the NASA/ESA Hubble Space Telescope, appears to float serenely in the depths of space, but this apparent calm hides an inner turmoil. The gaseous envelope formed as the expanding blast wave and ejected material from a supernova tore through the nearby interstellar medium. Called SNR B0509 - 67.5 (or SNR 0509 for short), the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light - years from Earth. Ripples in the shell's surface may be caused either by subtle variations in the density of the ambient interstellar gas, or possibly be driv

Supernova Remnants SNR B0509 - 67.5 - Supernova Remnant SNR B0509 - 67.5 - SNR B0509 - 67.5 (or SNR 0509) is the rest of a star explosion in the galaxy of the Great Magellan Cloud. This 23-year bubble - light of diameter extends at a speed of 18 million km/h. Composite of images obtained by the Hubble Space Telescope (HST) in 2006 and 2010. This delicate shell, photographed by the NASA/ESA Hubble Space Telescope, appears to float serenely in the depths of space, but this apparent calm hides an inner turmoil. The gaseous envelope formed as the expanding blast wave and ejected material from a supernova tore through the nearby interstellar medium. Called SNR B0509 - 67.5 (or SNR 0509 for short), the bubble is the visible remnant of a powerful stellar explosion in the Large Magellanic Cloud (LMC), a small galaxy about 160,000 light - years from Earth. Ripples in the shell's surface may be caused either by subtle variations in the density of the ambient interstellar gas, or possibly be driv

PIX4583175

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

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

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

R. Gendler

PIX4610335

The cluster of stars Pismis 24 in the Scorpio - Pismis 24 star cluster in Scorpius - This image obtained by the Hubble space telescope shows the cluster of young stars Pismis 24, located about 8000 years - light in the nebula NGC 6357 of the Scorpio. This cluster houses a star that was thought to be the most massive star in our galaxy, between 200 and 300 solar masses (the brightest star in the top center of the image). The measurements obtained by the Hubble telescope showed that this star, Pismis 24 - 1, was actually a double star and that its mass was actually only about 100 solar masses. The small open star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 in Scorpius, about 8,000 light - years away from Earth. Some of the stars in this cluster are extremely massive and emit intense ultraviolet radiation. The brightest object in the picture is designated Pismis 24 - 1. It was once thought to weigh as much as 200 to 300 solar masses. This would not only have m

The cluster of stars Pismis 24 in the Scorpio - Pismis 24 star cluster in Scorpius - This image obtained by the Hubble space telescope shows the cluster of young stars Pismis 24, located about 8000 years - light in the nebula NGC 6357 of the Scorpio. This cluster houses a star that was thought to be the most massive star in our galaxy, between 200 and 300 solar masses (the brightest star in the top center of the image). The measurements obtained by the Hubble telescope showed that this star, Pismis 24 - 1, was actually a double star and that its mass was actually only about 100 solar masses. The small open star cluster Pismis 24 lies in the core of the large emission nebula NGC 6357 in Scorpius, about 8,000 light - years away from Earth. Some of the stars in this cluster are extremely massive and emit intense ultraviolet radiation. The brightest object in the picture is designated Pismis 24 - 1. It was once thought to weigh as much as 200 to 300 solar masses. This would not only have m

PIX4569076

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649419

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

James Webb Space Telescope Mirrors (JWST) - Testing of the JWST's mirrors - Six of the 18 JWST (James Webb Space Telescope) mirrors seen at Nasa's Marshall Space Center. These mirrors will be tested there to ensure they will withstand the extreme temperatures of space vacuum. The JWST will replace the Hubble Space Telescope in 2014. Equipped with a 6.5 m mirror, he will observe the universe mainly in infrared. Six of the 18 James Webb Space Telescope mirror segments are being moved into the X - ray and Cryogenic Facility, or XRCF, at Nasa's Marshall Space Flight Center in Huntsville, Ala., to eventually experience temperatures dipping to a chilling - 414 degrees Fahrenheit to ensure they can withstand the extreme space environments. The test chamber takes approximately five days to cool a mirror segment to cryogenic temperatures. Marshall's X - ray & Cryogenic Facility is the world's largest X - ray telescope test facility and a unique, cryogenic, clean room optical test location. The

PIX4645744

Burma / Myanmar: The Mingun Bell in Sagaing Division, Burma

Burma / Myanmar: The Mingun Bell in Sagaing Division, Burma

David Henley

PFH1774480

Jenner Jones. Freddie Crowley. John Grimwade, Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, Cape Town, en route to Egypt, 1941. (b/w photo)

Jenner Jones. Freddie Crowley. John Grimwade, Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, Cape Town, en route to Egypt, 1941. (b/w photo)

Sale, Wilfred Herbert James

NAM5922555

Top of the mountain. Freddie Crowley. Jimmy Sale, Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, Cape Town, en route to Egypt, 1941 (b/w photo)

Top of the mountain. Freddie Crowley. Jimmy Sale, Table mountain, 3rd County of London Yeomanry (Sharpshooters) shore leave, Cape Town, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5922556

Orion docked. Troops on quayside, 3rd County of London Yeomanry (Sharpshooters), Cape Town, South Africa, en route to Egypt, 1941 (b/w photo)

Orion docked. Troops on quayside, 3rd County of London Yeomanry (Sharpshooters), Cape Town, South Africa, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5923188

Inside the archaeological complex of Machu Picchu, Peru (photo)

Inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584745

Wounded being brought on board a destroyer off Dieppe, August 1942 (b/w photo)

Wounded being brought on board a destroyer off Dieppe, August 1942 (b/w photo)

Unknown photographer, (20th century)

NAM5928231

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

Planetary nebula M57 (NGC 6720) in Lyra - M57 (NGC 6720) planetary nebula in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. With a magnitude of 9.0, this nebula is easily observed with a small telescope. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Composite image obtained by different telescopes. The Ring Nebula, M57, is the most famous example of a planetary nebula. Located about 2,000 light years away, it has an apparent diameter of 1 arc minute and a real diameter of about one light year. At magnitude 9.0 its high surface brightness makes it an easy object, even from the city and even with small telescopes. Planetary nebula are shells of gas shed by stars late in their life cycles after using up all of their nuclear fuel. The star then ejects a significant portion of its mass in a gaseous shell, which is illuminated by its extremely

PIX4623359

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

Star cluster IC 1590 in NGC 281 (Cassiopee) - Open cluster and Bok globules in NGC 281 - View of a detail in the center of the nebula NGC 281 in Cassiopee. The brightest stars of the open cluster IC 1590 are visible, accompanied by Bok's blood cells, dark interstellar clouds consisting of gas and dust that absorb light. Image obtained by the Hubble Space Telescope (HST). Astronomers have used the NASA/ESA Hubble Space Telescope to study the young open star cluster IC 1590, which is found within the star formation region NGC 281 - - nicknamed the Pacman Nebula due to its resemblance to the famous arcade game character. This image only shows the central part of the nebula, where the brightest stars at the core of the cluster are found, with part of the Pacman's hungry mouth visible as the dark region below. But Pacman isn't gobbling up these stars. Instead, the nebula's gas and dust are being used as raw ingredients to make new stars. However, the stars in IC 1590 are still plotting thei

PIX4617504

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

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

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

PIX4610399

Barree spiral galaxy NGC 6872 in interaction with IC 4970 in the Peacock - Barred spiral interacting galaxy NGC 6872 in Pavo - The barree spiral galaxy NGC 6872 and lenticular IC 4970 are located about 300 million years away - light from Earth. NGC 6872 extends over nearly 750,000 years - light. Image obtained by the ANTU telescope of the VLT on March 29, 1999. View of the spectacular barred spiral galaxy NGC 6872 obtained with FORS1 at ANTU telescope (VLT) in the morning of March 29, 1999. It is of type SBB and is accompanied by a smaller, interacting galaxy, IC 4970 of type S0 (just above the centre). The bright object to the lower right of the galaxies is a star in the Milky Way whose image has been strongly overexposed and exhibits multiple optical reflections in the telescope and instrument. There are also many other, fainter and more distant galaxies of many different forms in the field. The upper left spiral arm of NGC 6872 is significantly disturbed and is populated by a pletho

Barree spiral galaxy NGC 6872 in interaction with IC 4970 in the Peacock - Barred spiral interacting galaxy NGC 6872 in Pavo - The barree spiral galaxy NGC 6872 and lenticular IC 4970 are located about 300 million years away - light from Earth. NGC 6872 extends over nearly 750,000 years - light. Image obtained by the ANTU telescope of the VLT on March 29, 1999. View of the spectacular barred spiral galaxy NGC 6872 obtained with FORS1 at ANTU telescope (VLT) in the morning of March 29, 1999. It is of type SBB and is accompanied by a smaller, interacting galaxy, IC 4970 of type S0 (just above the centre). The bright object to the lower right of the galaxies is a star in the Milky Way whose image has been strongly overexposed and exhibits multiple optical reflections in the telescope and instrument. There are also many other, fainter and more distant galaxies of many different forms in the field. The upper left spiral arm of NGC 6872 is significantly disturbed and is populated by a pletho

PIX4613035

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

Barree spiral galaxy NGC 7098 - Barred spiral galaxy NGC 7098: The barree spiral galaxy NGC 7098 is located about 95 million light years away from Earth in the southern constellation of the octant. Image obtained by the Very Large Telescope (VLT). Approximately 95 million light-years away, in the southern constellation of Octans (The Octant), lies NGC 7098 - an intriguing spiral galaxy with numerous sets of double features. The first of NGC 7098's double features is a duo of distinct ring-like structures that loop around the galaxy's hazy heart. This central region hosts a second double feature: a double bar. NGC 7098 has also developed features known as ansae, visible as small, bright streaks at each end of the central region. Ansae are visible areas of overdensity - they commonly take looping, linear, or circular shapes, and can be found at the extremities of planetary ring systems, in nebulous clouds, and, as is the case with NGC 7098, in parts of galaxies that are packed to the bri

PIX4574313

Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

Nebula of the Rosette in the Unicorn seen in false colors - Rosette nebula in Monoceros - The nebula of the Rosette is a vast cloud of dust and gas situated about 5500 years - light from the Earth. In the center of the nebula, a cluster of blue stars, NGC 2244, formed less than a million years ago. Image in false colors obtained by Kitt Peak's 90 cm telescope. The Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Its parts have been assigned different NGC numbers: 2237, 2238, 2239, and 2246. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. This stunning emission - line image of the Rosette nebula (NGC2237) in the constellation Monoceros (the Unicorn) was taken at the National Science Foundation's 0.9 - m tele

PIX4618453

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

Decolishing the space shuttle Atlantis - 05/2010 - Space Shuttle Atlantis lift - off - 05/2010 - Decolving the space shuttle Atlantis with the crew of the STS - 132 mission on board, 14 May 2010. Last flight of shuttle Atlantis. Space shuttle Atlantis and its six - member STS - 132 crew head towards Earth orbit and rendezvous with the International Space Station. Liftoff was at 2:20 p.m. (EDT) on May 14, 2010, from launch pad 39A at Nasa's Kennedy Space Center. Onboard are NASA astronauts Ken Ham, commander; Tony Antonelli, pilot; Garrett Reisman, Michael Good, Steve Bowen and Piers Sellers, all mission specialists. The crew will deliver the Russian - built Mini - Research Module 1 (MRM - 1) to the International Space Station. Named Rassvet, Russian for “” dawn,”” the module is the second in a series of new pressurized components for Russia and will be permanently attached to the Earth - facing port of the Zarya Functional Cargo Block (FGB). Rassvet will be used for cargo storage and w

PIX4649404

Depart of astronauts STS - 107 01/2003 - STS - 107 crew is going to launch pad - 16/01/2003. The crew of the STS-107 mission joins firing pad 39A for decolving. Front, from left to right, William “” Willie”” McCool and Rick Husband, behind, Kalpana Chawla and Laurel Clark; in the back, from left to right, Ilan Ramon, Michael Anderson, David Brown. The STS - 107 crew, waving to onlookers, exits the Operations and Checkout Building on their way to Launch Pad 39A for liftoff. Leading the way are Pilot William “” Willie””” McCool (left) and Commander Rick Husband (right). Following in the second row are Mission Specialists Kalpana Chawla (left) and Laurel Clark; in the rear are Payload Specialist Ilan Ramon, Payload Commander Michael Anderson and Mission Specialist David Brown. Ramon is the first astronaut from Israel to fly on a Shuttle. The 16 - day mission is devoted to research and will include more than 80 experiments that will study Earth and space science, advanced technology develo

Depart of astronauts STS - 107 01/2003 - STS - 107 crew is going to launch pad - 16/01/2003. The crew of the STS-107 mission joins firing pad 39A for decolving. Front, from left to right, William “” Willie”” McCool and Rick Husband, behind, Kalpana Chawla and Laurel Clark; in the back, from left to right, Ilan Ramon, Michael Anderson, David Brown. The STS - 107 crew, waving to onlookers, exits the Operations and Checkout Building on their way to Launch Pad 39A for liftoff. Leading the way are Pilot William “” Willie””” McCool (left) and Commander Rick Husband (right). Following in the second row are Mission Specialists Kalpana Chawla (left) and Laurel Clark; in the rear are Payload Specialist Ilan Ramon, Payload Commander Michael Anderson and Mission Specialist David Brown. Ramon is the first astronaut from Israel to fly on a Shuttle. The 16 - day mission is devoted to research and will include more than 80 experiments that will study Earth and space science, advanced technology develo

PIX4648054

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

Cl0024+17 galaxy cluster Cl0024+17 - Galaxy cluster Cl0024+17 - Cl0024+17 galaxy cluster located about 5 billion years ago - light in the constellation Pisces. This image reveals to us, by a gravitational mirage effect, the deformed image of a galaxy, located behind the cluster at a distance of about 10 billion years - light from the Earth. By studying this gravitational mirage, astronomers discovered the presence of black matter around this cluster. Image obtained by the Hubble space telescope in November 2004 with the ACS camera. An international team of astronomers using the NASA/ESA Hubble Space Telescope has discovered a ghostly ring of dark matter that was formed long ago during a titanic collision between two massive galaxy clusters. It is the first time that a dark matter distribution has been found that differs substantially from the distribution of ordinary matter. This image shows the galaxy cluster Cl 0024+17 (ZWCl 0024+1652) located at about 5 billion light - years as seen

Cl0024+17 galaxy cluster Cl0024+17 - Galaxy cluster Cl0024+17 - Cl0024+17 galaxy cluster located about 5 billion years ago - light in the constellation Pisces. This image reveals to us, by a gravitational mirage effect, the deformed image of a galaxy, located behind the cluster at a distance of about 10 billion years - light from the Earth. By studying this gravitational mirage, astronomers discovered the presence of black matter around this cluster. Image obtained by the Hubble space telescope in November 2004 with the ACS camera. An international team of astronomers using the NASA/ESA Hubble Space Telescope has discovered a ghostly ring of dark matter that was formed long ago during a titanic collision between two massive galaxy clusters. It is the first time that a dark matter distribution has been found that differs substantially from the distribution of ordinary matter. This image shows the galaxy cluster Cl 0024+17 (ZWCl 0024+1652) located at about 5 billion light - years as seen

PIX4565685

Drawings made in secret by women from a women's camp in Indonesia about their living conditions.

Drawings made in secret by women from a women's camp in Indonesia about their living conditions.

BEG752383

The Temples of Angkor, Angkor, Cambodia (photo)

The Temples of Angkor, Angkor, Cambodia (photo)

Sergi Reboredo

SRB1202744

Burma / Myanmar: The Mingun Bell in Sagaing Division, Burma

Burma / Myanmar: The Mingun Bell in Sagaing Division, Burma

David Henley

PFH1774479

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Terraces inside the archaeological complex of Machu Picchu, Peru (photo)

Sergi Reboredo

SRB3584747

3rd County of London Yeomanry (Sharpshooters) shore leave, Table mountain, Cape Town, en route to Egypt, 1941 (b/w photo)

3rd County of London Yeomanry (Sharpshooters) shore leave, Table mountain, Cape Town, en route to Egypt, 1941 (b/w photo)

Sale, Wilfred Herbert James

NAM5922554

Sardinia the future is called Rebirth, 1968

Sardinia the future is called Rebirth, 1968

MOD6437290

HMS 'Daphne' off Cape Horn, 28 May 1852 (watercolour)

HMS 'Daphne' off Cape Horn, 28 May 1852 (watercolour)

Fanshawe, Admiral Sir Edward Gennys (1814-1906)

MMM7295642

HMS 'Britannia' sailing from the Hamoaze to Plymouth Sound, with the Duke of Clarence on board as Lord High Admiral, 27 July 1828, c.1828 (oil on canvas)

HMS 'Britannia' sailing from the Hamoaze to Plymouth Sound, with the Duke of Clarence on board as Lord High Admiral, 27 July 1828, c.1828 (oil on canvas)

Hornbrook, Thomas L. (1780-1850)

MMM7340624

Kafir archers, 1919 (b/w photo)

Kafir archers, 1919 (b/w photo)

Unknown photographer, (20th century)

NAM5920290

«
1
…
773
774
775
…
779
»

Why choose Bridgeman Images

Art. Culture. History.

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

Discover our collection Browse FAQs

Simple. Fast. Reliable.

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

Contact us

Discover millions of images and videos for your creative projects.

Start your search

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