'Exposed' images et/ou videos résultats

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

Votre Sélection en cours

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4600102","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_international_space_station_iss_12_2000_the_international_space_station_iss_12_2000_the_internat","item_variant":"undefined"},{"item_id":"PIX4602998","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"astronaut_exit_into_space_astronauts_extravehicular_activity_astronaut_exit_steve_bowen_and_alvin_dr","item_variant":"undefined"},{"item_id":"PIX4597546","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"apollo_16_j_young_drives_the_lrv_apollo_16_john_young_driving_the_lrv_john_young_driving_the_lunar_j","item_variant":"undefined"},{"item_id":"PIX4597685","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"apollo_16_exit_of_t_mattingly_and_c_duke_apollo_16_eva_astronauts_thomas_mattingly_on_the_right_assi","item_variant":"undefined"},{"item_id":"PIX4597551","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"apollo_16_j_young_drives_the_lrv_apollo_16_john_young_driving_the_lrv_john_young_driving_the_lunar_j","item_variant":"undefined"},{"item_id":"ZUM4864906","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"jul_20_1953_coloured_photos_on_stone_professor_kleinschmidt_teacher_at_the_highschool_for_art_in_ber","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":"PIX4623489","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_dumbbell_m27_in_little_fox_dumbell_planetary_nebula_m27_in_vulpecula_the_planetary_","item_variant":"undefined"},{"item_id":"PIX4621590","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dark_nebula_in_scorpio_a_dark_cloud_in_scorpius_this_dark_nebula_is_located_about_5000_years_from_ea","item_variant":"undefined"},{"item_id":"PIX4580071","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"laminate_structures_near_the_north_pole_on_mars_layers_exposed_at_north_polar_cap_on_mars_laminated_","item_variant":"undefined"},{"item_id":"PIX4621577","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dark_nebula_in_scorpio_a_dark_cloud_in_scorpius_wide_field_this_dark_nebula_is_located_about_5000_ye","item_variant":"undefined"},{"item_id":"PIX4623523","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_dumbbell_m27_in_little_fox_dumbell_planetary_nebula_m27_in_vulpecula_the_planetary_","item_variant":"undefined"},{"item_id":"PIX4623530","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_dumbbell_m27_in_little_fox_dumbell_planetary_nebula_m27_in_vulpecula_the_planetary_","item_variant":"undefined"},{"item_id":"PIX4577258","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"sunrise_on_the_crater_tycho_tycho_crater_sunrise_sunrise_on_the_central_peak_of_the_crater_tycho_on_","item_variant":"undefined"},{"item_id":"PIX4626113","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"astronauts_on_titan_illustration_releasing_a_weather_balloon_on_titan_astronauts_make_meteorological","item_variant":"undefined"},{"item_id":"PIX4647074","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"release_of_mr_lee_09_1994_astronaut_m_lee_during_eva_sep_16_1994_extra_vehicle_release_by_mark_lee_t","item_variant":"undefined"},{"item_id":"PIX4672818","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"sandy_cay_bahamas_seabed_currents_and_sandbanks_on_sandy_cay_and_long_island_bahamas_image_obtained_","item_variant":"undefined"},{"item_id":"PIX4633276","item_category2":"no_copyright","item_category3":"standard","item_category4":"walter_b_myers","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_earth_650_million_years_ago_artist_s_view_snowball_earth_the_earth_seen_in_a_period_of_glaciatio","item_variant":"undefined"},{"item_id":"PIX4582378","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"supernova_1987a_before_and_after_explosion_supernova_1987a_with_precursor_image_overlaid_image_of_th","item_variant":"undefined"},{"item_id":"PIX4665861","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"straits_of_gibraltar_seen_by_the_envisat_satellite_with_the_asar_instrument_on_20_may_2002","item_variant":"undefined"},{"item_id":"PIX4623419","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_m_27_ngc_6853_in_the_little_fox_this_excellent_image_of_the_dumbbell_nebula_m27_ngc","item_variant":"undefined"},{"item_id":"PIX4616152","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"march_hebes_chasma_mars_hebes_chasma_hebes_chasma_is_a_basin_of_almost_8000_m_deep_located_in_the_no","item_variant":"undefined"},{"item_id":"PIX4660817","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"dead_sea_from_space_2013_dead_sea_from_space_in_2013_dead_sea_from_space_in_july_2013_by_landsat_8_s","item_variant":"undefined"},{"item_id":"PIX4582330","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"supernova_1987a_in_the_great_magellan_cloud_before_and_after_explosion_sometime_during_23_february_1","item_variant":"undefined"},{"item_id":"PIX4660989","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"aral_sea_seen_by_the_shuttle_endeavour_09_1992_aral_sea_seen_from_the_space_shuttle_endeavour_09_199","item_variant":"undefined"},{"item_id":"PIX4623431","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_planetary_nebula_dumbbell_m27_is_located_about_1200_light_years_from_earth_in_the_constellation_","item_variant":"undefined"},{"item_id":"PIX4675640","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"atafu_atoll_tokelau_islands_south_pacific_atafu_atoll_tokelau_southern_pacific_ocean_atafu_is_a_smal","item_variant":"undefined"},{"item_id":"PIX4565332","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"persee_galaxy_cluster_perseus_galaxy_cluster_the_persee_galaxy_cluster_abell_426_contains_at_least_5","item_variant":"undefined"},{"item_id":"NHM1458224","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"aerially_exposed_corals","item_variant":"undefined"},{"item_id":"LLM959547","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"american_school_19th_century_after","item_category5":"not_balown","item_list_name":"search_results","item_name":"portion_of_charleston_exposed_to_the_fire_of_the_federal_fleet_august_1863_engraving","item_variant":"undefined"},{"item_id":"LLM6004420","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"she_was_exposed_to_the_wild_beasts_engraving","item_variant":"undefined"},{"item_id":"LLM3106235","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"an_accra_belle_in_all_her_youthful_pride_colour_photo","item_variant":"undefined"},{"item_id":"UIG3735835","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_syrian_criminal_being_punished","item_variant":"undefined"},{"item_id":"LLM5992219","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"she_was_exposed_to_the_wild_beasts_engraving","item_variant":"undefined"},{"item_id":"PC1278453","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"window_depicting_saint_stephen_s_body_exposed_to_the_animals_stained_glass","item_variant":"undefined"},{"item_id":"LCL364339","item_category2":"no_copyright","item_category3":"standard","item_category4":"lola_claeys_bouuaert","item_category5":"not_balown","item_list_name":"search_results","item_name":"squatted_building_2002_photo","item_variant":"undefined"},{"item_id":"LLW993120","item_category2":"no_copyright","item_category3":"standard","item_category4":"lucinda_lambton","item_category5":"not_balown","item_list_name":"search_results","item_name":"jamaican_interior_photo","item_variant":"undefined"},{"item_id":"LIP1621908","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_great_disaster_on_the_thames_engraving","item_variant":"undefined"},{"item_id":"LLJ608128","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_18th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"john_hayes_s_head_exposed_in_st_margaret_s_church_yard_engraving","item_variant":"undefined"},{"item_id":"LCL364340","item_category2":"no_copyright","item_category3":"standard","item_category4":"lola_claeys_bouuaert","item_category5":"not_balown","item_list_name":"search_results","item_name":"squatted_building_2002_photo","item_variant":"undefined"},{"item_id":"UIG5307615","item_category2":"out_of_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_syrian_criminal_being_punished","item_variant":"undefined"},{"item_id":"BST424886","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"greek_school_2nd_century_bc","item_category5":"not_balown","item_list_name":"search_results","item_name":"flying_nike_victory_hellenistic_period_terracotta","item_variant":"undefined"},{"item_id":"BAL37956","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"orley_richard_van_1663_1732","item_category5":"not_balown","item_list_name":"search_results","item_name":"diana_and_callisto","item_variant":"undefined"},{"item_id":"LLW993141","item_category2":"no_copyright","item_category3":"standard","item_category4":"lucinda_lambton","item_category5":"not_balown","item_list_name":"search_results","item_name":"jamaican_interior_photo","item_variant":"undefined"},{"item_id":"XJL197005","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"colombe_jean_c_1430_c_93","item_category5":"balown","item_list_name":"search_results","item_name":"ms_lat_q_v_i_126_fol_17_the_drunkenness_of_noah_from_book_of_hours_of_louis_d_orleans_1490_vellum","item_variant":"undefined"},{"item_id":"XIR420042","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"weenix_jan_1642_1719","item_category5":"balown","item_list_name":"search_results","item_name":"woman_sitting_in_a_park_1688_oil_on_canvas","item_variant":"undefined"},{"item_id":"TRV227729","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"i_swear_you_are_an_englishman_the_author_s_disguise_is_exposed_in_herat_from_travels_in_central_asia","item_variant":"undefined"},{"item_id":"STC437628","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"deveria_achille_1800_57","item_category5":"not_balown","item_list_name":"search_results","item_name":"couple_indulging_in_sexual_play_c_1820_35_colour_litho","item_variant":"undefined"},{"item_id":"BAL192502","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"buonarroti_michelangelo_1475_1564","item_category5":"not_balown","item_list_name":"search_results","item_name":"study_for_noah_in_the_drunkenness_of_noah_1508_12_charcoal_on_paper_recto","item_variant":"undefined"},{"item_id":"LLM5212217","item_category2":"no_copyright","item_category3":"standard","item_category4":"european_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_baggara_married_lady_omdurman_b_w_photo","item_variant":"undefined"},{"item_id":"LMG100073","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"stott_william_edward_1859_1918","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_snow_storm_c_1891_oil_on_canvas","item_variant":"undefined"},{"item_id":"DND357827","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"paint_on_wall_photo","item_variant":"undefined"},{"item_id":"LLM5220378","item_category2":"in_copyright","item_category3":"standard","item_category4":"roughley_theodore_cleveland_1881_1961","item_category5":"not_balown","item_list_name":"search_results","item_name":"coral_exposed_during_a_low_spring_tide_colour_photo","item_variant":"undefined"},{"item_id":"NUM712154","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"gervex_henri_1852_1929","item_category5":"not_balown","item_list_name":"search_results","item_name":"girl_with_red_hair_pastel_on_canvas","item_variant":"undefined"},{"item_id":"LLM3093011","item_category2":"no_copyright","item_category3":"standard","item_category4":"european_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"three_female_artistes_wearing_body_stockings_b_w_photo","item_variant":"undefined"},{"item_id":"LLM3623156","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"harding_s_18th_century_after","item_category5":"not_balown","item_list_name":"search_results","item_name":"miss_lucy_waters_engraving","item_variant":"undefined"},{"item_id":"LLM5212230","item_category2":"no_copyright","item_category3":"standard","item_category4":"european_photographer_20th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"jeune_egyptienne_b_w_photo","item_variant":"undefined"},{"item_id":"STC437630","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"deveria_achille_1800_57","item_category5":"not_balown","item_list_name":"search_results","item_name":"lovers_in_the_open_air_c_1830_40_colour_litho","item_variant":"undefined"},{"item_id":"PIX4672551","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"copper_mines_in_arizona_usa_open_pit_copper_mines_arizona_three_open_air_copper_mines_near_the_city_","item_variant":"undefined"},{"item_id":"LIP1054549","item_category2":"out_of_copyright","item_category3":"standard","item_category4":"english_school_19th_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"york_illustrated_engraving","item_variant":"undefined"}]}}

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

Recherche avancée Astuces de recherche

Images de 'Exposed' médias trouvés, 1,579

«
1
2
3
…
27
»

The International Space Station (ISS) 12/2000 - The International Space Station (ISS) 12/2000 - The International Space Station after stowage with the shuttle Endeavour. ISS STS-97. 09/12/2000. This picture is one of a series of 70 mm frames exposed of the International Space Station (ISS) following undocking at 1:13 p.m. (CST), December 9, 2000. This series of images, as well as video and digital still imagery taken at the same time, represent the first imagery of the entire station with its new solar array panels deployed. Before separation, the shuttle and space station had been docked to one another for 6 days, 23 hours and 13 minutes

The International Space Station (ISS) 12/2000 - The International Space Station (ISS) 12/2000 - The International Space Station after stowage with the shuttle Endeavour. ISS STS-97. 09/12/2000. This picture is one of a series of 70 mm frames exposed of the International Space Station (ISS) following undocking at 1:13 p.m. (CST), December 9, 2000. This series of images, as well as video and digital still imagery taken at the same time, represent the first imagery of the entire station with its new solar array panels deployed. Before separation, the shuttle and space station had been docked to one another for 6 days, 23 hours and 13 minutes

PIX4600102

Astronaut Exit into Space - Astronauts extravehicular activity - Astronaut Exit Steve Bowen and Alvin Drew (at the bottom of the picture) into space. Maintenance of the International Space Station (ISS). 28 February 2011. NASA astronauts Steve Bowen and Alvin Drew, both STS - 133 mission specialists, participate in the mission's first session of extravehicular activity (EVA) as construction and maintenance continue on the International Space Station. During the six - hour, 34 - minute spacewalk, Bowen and Drew installed the J612 power extension cable, move a failed ammonia pump module to the External Stowage Platform 2 on the Quest Airlock for return to Earth at a later date, installed a camera wedge on the right hand truss segment, installed extensions to the mobile transporter rail and exposed Japanese “” Message in a Bottle”” experiment to space. 28 Feb. 2011

Astronaut Exit into Space - Astronauts extravehicular activity - Astronaut Exit Steve Bowen and Alvin Drew (at the bottom of the picture) into space. Maintenance of the International Space Station (ISS). 28 February 2011. NASA astronauts Steve Bowen and Alvin Drew, both STS - 133 mission specialists, participate in the mission's first session of extravehicular activity (EVA) as construction and maintenance continue on the International Space Station. During the six - hour, 34 - minute spacewalk, Bowen and Drew installed the J612 power extension cable, move a failed ammonia pump module to the External Stowage Platform 2 on the Quest Airlock for return to Earth at a later date, installed a camera wedge on the right hand truss segment, installed extensions to the mobile transporter rail and exposed Japanese “” Message in a Bottle”” experiment to space. 28 Feb. 2011

PIX4602998

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

PIX4597546

Apollo 16: exit of T. Mattingly and C. Duke - Apollo 16: EVA astronauts - Thomas Mattingly (on the right, assisted by Charles Duke, from the back) takes the cameras and cameras in the service module Apollo 16. 25/04/1972. Astronaut Thomas K. Mattingly II, command module pilot, performs an Extravehicular Activity (EVA) during the Apollo 16 trans - Earth coast. Mattingly is assisted by astronaut Charles M. Duke, Jr., lunar module pilot. Mattingly inspected the SIM Bay or Service Module (SM), and retrieved film from the Mapping and Panoramic Cameras. Mattingly is wearing the helmet of astronaut John W. Young, commander. The helmet's lunar EVA visor assembly helped protect Mattingly's eyes from the bright Sun. This view is a frame from motion picture film exposed by a 16 mm Maurer camera. 25 April 1972

Apollo 16: exit of T. Mattingly and C. Duke - Apollo 16: EVA astronauts - Thomas Mattingly (on the right, assisted by Charles Duke, from the back) takes the cameras and cameras in the service module Apollo 16. 25/04/1972. Astronaut Thomas K. Mattingly II, command module pilot, performs an Extravehicular Activity (EVA) during the Apollo 16 trans - Earth coast. Mattingly is assisted by astronaut Charles M. Duke, Jr., lunar module pilot. Mattingly inspected the SIM Bay or Service Module (SM), and retrieved film from the Mapping and Panoramic Cameras. Mattingly is wearing the helmet of astronaut John W. Young, commander. The helmet's lunar EVA visor assembly helped protect Mattingly's eyes from the bright Sun. This view is a frame from motion picture film exposed by a 16 mm Maurer camera. 25 April 1972

PIX4597685

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

Apollo 16: J. Young drives the LRV - Apollo 16: John Young driving the LRV - John Young driving the lunar jeep (Lunar Rover Vehicle). 23/04/1972. (23 April 1972) The Lunar Roving Vehicle (LRV) gets a speed workout by astronaut John W. Young in the “” Grand Prix”” run during the third Apollo 16 Extravehicular Activity (EVA 3) at the Descartes landing site. This view is a frame from motion picture film exposed by a 16 mm Maurer camera held by astronaut Charles M. Duke, Jr. While Astronaut's Young, commander, and Duke, lunar module pilot, descended in the Lunar Module (LM) “” Orion””” to explore the Descartes highlands region of the Moon, astronaut Thomas K. Mattingly II, command module pilot, remained with the Command and Service Modules (CSM) “” Casper””” in lunar orbit

PIX4597551

Jul. 20, 1953 - Coloured Photos on Stone.: Professor Kleinschmidt, teacher at the highschool for art in Berlin, brought out an invention which took him and his co-operators 5 years and which is quite a senstaion on the field of photo- and publicity tecnhnics. Huge photos on stone! The photos do not react to heat, cold, snow or rain. They are made the following way: eternit-plate sensitive to light a size 120 to 150 centimeters are exposed to the light in the dark room as with normal enlarging. The stone photos may be produced in black and white or in colours. It is quite obvious that this process bears quite new possibilities for publicity

Jul. 20, 1953 - Coloured Photos on Stone.: Professor Kleinschmidt, teacher at the highschool for art in Berlin, brought out an invention which took him and his co-operators 5 years and which is quite a senstaion on the field of photo- and publicity tecnhnics. Huge photos on stone! The photos do not react to heat, cold, snow or rain. They are made the following way: eternit-plate sensitive to light a size 120 to 150 centimeters are exposed to the light in the dark room as with normal enlarging. The stone photos may be produced in black and white or in colours. It is quite obvious that this process bears quite new possibilities for publicity

ZUM4864906

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

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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. Image obtained with a 90 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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. Image obtained with a 90 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

PIX4623489

Dark Nebula in Scorpio - A dark cloud in Scorpius - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

Dark Nebula in Scorpio - A dark cloud in Scorpius - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

PIX4621590

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

PIX4580071

Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

Dark Nebula in Scorpio - A dark cloud in Scorpius, wide field - This dark nebula is located about 5000 years from Earth. Image obtained by Siding Spring's 3.9m telescope. This curious un - named nebula is governed by radiation from very luminous stars some distance from the nebula. The direction of the radiation source can be seen from the flow pattern in the dark cloud and the extensive bright red rims at the end of the nebula that is exposed to radiation from the hot stars. This part of the nebula is reminiscent of the famous Horsehead nebula in Orion, which is also the consequence of starlight destroying a dark cloud. The source of the energy here is the Scorpius OB association, a group of brilliant, very hot stars, about 5000 light years away from us

PIX4621577

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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. Image obtained with a 50 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC 6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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. Image obtained with a 50 cm telescope, through various filters including an H-alpha filter. The Dumbbell Nebula (M27, NGC 6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud

R. Jay GaBany

PIX4623523

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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 with a 90 cm telescope, and the Hubble and Subaru telescopes. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. Image Composite

Planetary nebula Dumbbell (M27) in Little Fox - Dumbell planetary nebula (M27) in Vulpecula - The planetary nebula Dumbbell (M27) is located about 1400 years - light from Earth in the constellation Little Fox. 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 with a 90 cm telescope, and the Hubble and Subaru telescopes. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. Image Composite

PIX4623530

Sunrise on the crater Tycho - Tycho Crater Sunrise - Sunrise on the central peak of the crater Tycho on the Moon. This crater is about 82 km in diameter and its central peak rises at 2 km above sea level. Image obtained on June 10, 2011 by the LRO (Lunar Reconnaissance Orbiter) probe. On 10 June 2011 the LRO spacecraft slewed 65* to the west, allowing the LROC NACs to capture this dramatic sunrise view of Tycho crater. A very popular target with amateur astronomers, Tycho is located at 43.37* S, 348.68* E, and is ~ 82 km (51 miles) in diameter. The summit of the central peak is 2 km (6562 ft) above the crater floor, and the crater floor is about 4700 m (15,420 ft) below the rim. Many “” clasts”” ranging in size from 10 meters to 100s of meters are exposed in the central peak slopes

Sunrise on the crater Tycho - Tycho Crater Sunrise - Sunrise on the central peak of the crater Tycho on the Moon. This crater is about 82 km in diameter and its central peak rises at 2 km above sea level. Image obtained on June 10, 2011 by the LRO (Lunar Reconnaissance Orbiter) probe. On 10 June 2011 the LRO spacecraft slewed 65* to the west, allowing the LROC NACs to capture this dramatic sunrise view of Tycho crater. A very popular target with amateur astronomers, Tycho is located at 43.37* S, 348.68* E, and is ~ 82 km (51 miles) in diameter. The summit of the central peak is 2 km (6562 ft) above the crater floor, and the crater floor is about 4700 m (15,420 ft) below the rim. Many “” clasts”” ranging in size from 10 meters to 100s of meters are exposed in the central peak slopes

PIX4577258

Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well

Astronauts on Titan - Illustration - Releasing a weather balloon on Titan - Astronauts make meteorological measurements on the surface of Titan. A titanian explorer prepares to release a weather balloon while another direct a flood lamp to illuminate the activity. On the left is a supply cart with a portable weather station, featuring an interactive control panel designed to accommodate hands enclosed in thick gloves. All exposed hardware would have to function at temperatures of minus 300* F and below. With an atmosphere 10 times denser than the Earth's, weather would be of keen interest to Titan's visitors. High in Titan's atmosphere wind velocities in excess of 400 mph have been detected. While not much is known about winds and weather at Triton's surface, terrain features resembling dune fields have been observed, suggesting surface winds have occurred at some locations. Fogs of methane gas would likely be present at the surface as well

Walter B Myers

PIX4626113

Release of Mr Lee 09/1994 - Astronaut M.Lee during EVA. Sep 16 1994 - Extra vehicle release by Mark Lee testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Mark C. Lee, STS - 64 mission specialist, tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The forward cargo bay is reflected in Lee's helmet visor in the 35 mm frame, exposed through the space shuttle Discovery's aft flight deck windows. Part of the hardware for the LIDAR - in - Space Technology Experiment (LITE) is in center foreground. Astronauts Lee and Carl J. Meade, mission specialist, took turns using the SAFER hardware during their shared Extrahicular Activity (EVA) on Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a p

Release of Mr Lee 09/1994 - Astronaut M.Lee during EVA. Sep 16 1994 - Extra vehicle release by Mark Lee testing the SAFER (Simplified Aid for EVA Rescue) system. 16/09/1994. Astronaut Mark C. Lee, STS - 64 mission specialist, tests the new Simplified Aid for EVA Rescue (SAFER) system 130 nautical miles above Earth. The forward cargo bay is reflected in Lee's helmet visor in the 35 mm frame, exposed through the space shuttle Discovery's aft flight deck windows. Part of the hardware for the LIDAR - in - Space Technology Experiment (LITE) is in center foreground. Astronauts Lee and Carl J. Meade, mission specialist, took turns using the SAFER hardware during their shared Extrahicular Activity (EVA) on Sept. 16, 1994. The test of SAFER is the first phase of a larger SAFER program whose objectives are to establish a common set of requirements for both space shuttle and space station program needs, develop a flight demonstration of SAFER, validate system performance and, finally, develop a p

PIX4647074

Sandy Cay - Bahamas - Seabed currents and sandbanks on Sandy Cay and Long Island, Bahamas. Image obtained on 27 November 2010 from the International Space Station (ISS). This astronaut photograph, taken from the International space station on November 27, 2010, provides a view of tidal flats and channels near Sandy Cay, on the western side of Long Island and along the eastern margin of the Great Bahama Bank (North is top). The continuously exposed parts of the island are brown, a result of soil formation and vegetation growth. To the north of Sandy Cay, an off - white tidal flat composed of carbonate sediments is visible; light blue - green regions indicate shallow water on the tidal flat. The tidal flow of seawater is concentrated through gaps in the land surface, leading to the formation of relatively deep channels that cut into the sediments. The channels and areas to the south of the island have a vivid blue color that indicates deeper water

Sandy Cay - Bahamas - Seabed currents and sandbanks on Sandy Cay and Long Island, Bahamas. Image obtained on 27 November 2010 from the International Space Station (ISS). This astronaut photograph, taken from the International space station on November 27, 2010, provides a view of tidal flats and channels near Sandy Cay, on the western side of Long Island and along the eastern margin of the Great Bahama Bank (North is top). The continuously exposed parts of the island are brown, a result of soil formation and vegetation growth. To the north of Sandy Cay, an off - white tidal flat composed of carbonate sediments is visible; light blue - green regions indicate shallow water on the tidal flat. The tidal flow of seawater is concentrated through gaps in the land surface, leading to the formation of relatively deep channels that cut into the sediments. The channels and areas to the south of the island have a vivid blue color that indicates deeper water

PIX4672818

The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (bot

The Earth 650 million years ago - Artist's view - Snowball Earth - The Earth seen in a period of glaciation (Varanger glaciation), about 650 to 630 million years ago. This is how the Earth may have appeared about 650 million years ago during a period when snow and ice may have covered most, if not all, of the Earth's surface and oceans. This image suggests the Earth's appearance during the Marinoan glaciation from 650 to 630 million years ago. The southern and eastern hemispheres are dominated by glacier - covered land masses while the opposing hemisphere is frozen ocean save for a few areas of exposed liquid water, AKA refugia for the Earth's surviving soft - bodied multicellular organisms. In addition to the Marinoan glaciation there may have been at least two, and possibly three previous Proterozoic glacial periods going back to two billion years ago. The causes of these snowball periods are unknown but may have been due to massive volcanic eruptions, massive meteoritic impacts (bot

Walter B Myers

PIX4633276

Supernova 1987A before and after explosion - Supernova 1987A with precursor image overlaid - Image of the Supernova 1987A, obtained on March 8, 1987. The photo of the star Sanduleak - 69* 202, photographed two years ago. Images obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. The brightest star in the colour photograph is supernova 1987A, photographed with the AAT two months before it reached its maximum brightness. Superimposed in register on this image is a negative photograph of the region around the supernova copied from an AAT plate that was exposed in 1985, two years before the supernova was seen to explode. The precursor star appears to be a peculiar shape only because its image is blended with those of two other stars that happen to lie in the same line of sight. Many similar blended images can be seen in the colour photograph. However, it was soon found that the brighter of the three had exploded, and tha

Supernova 1987A before and after explosion - Supernova 1987A with precursor image overlaid - Image of the Supernova 1987A, obtained on March 8, 1987. The photo of the star Sanduleak - 69* 202, photographed two years ago. Images obtained with Siding Spring's 3.9m telescope. Supernova 1987A appeared in the constellation Doradus on February 23, 1987. The brightest star in the colour photograph is supernova 1987A, photographed with the AAT two months before it reached its maximum brightness. Superimposed in register on this image is a negative photograph of the region around the supernova copied from an AAT plate that was exposed in 1985, two years before the supernova was seen to explode. The precursor star appears to be a peculiar shape only because its image is blended with those of two other stars that happen to lie in the same line of sight. Many similar blended images can be seen in the colour photograph. However, it was soon found that the brighter of the three had exploded, and tha

PIX4582378

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

Straits of Gibraltar seen by the Envisat satellite with the ASAR instrument on 20 May 2002

PIX4665861

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

Planetary nebula M 27 (NGC 6853) in the little fox - This excellent image of the Dumbbell Nebula (M27, NGC6853), a planetary nebula in the constellation of Vulpecula, was taken at the 3.5 - meter WIYN telescope using the mini - mosaic imager. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high - energy, ultraviolet light from the core ionizes the cloud. This makes the nebula emit mostly a strong emission - line spectrum. This color image was obtained by combining three separate pictures, each one taken through a narrow filter centered at the emission wavelengths of Hydrogen (H alpha, red, 656 nm), doubly ionized Oxygen (OII, green, 501 nm), and neutral Oxygen (OI, blue, 630 nm). It is physically very interesting that neutral gas can survive in a region right next to highly ionized gas, and this image shows

PIX4623419

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

March: Hebes Chasma - Mars: Hebes Chasma - Hebes Chasma is a basin of almost 8000 m deep located in the northern part of Valles Marineris, the great Martian canyon. At the centre of this depression is a stratified plateau that constitutes sedimentary deposits. Image obtained by the Mars Express probe in 2005. View of Hebes Chasma obtained by the High Resolution Stereo Camera (HRSC) on ESA's Mars Express spacecraft. Hebes Chasma is an enclosed trough, almost 8000 m deep, in Valles Marineris, the Grand Canyon of Mars. A mesa - like mountain is located in the center of Hebes Chasma. It reaches 8000 meters above the graben floor and extends almost to the top of the surrounding plain. The mountain is made up by numerous stacked rock layers. The layering may consists of remnants of the older plateau, lake sediments, wind blown sediments or volcanic rock. The rock layers were exposed by erosional processes. Newest data acquired by the OMEGA spectrometer on - board Mars Express revealed hydrat

PIX4616152

Dead Sea from Space 2013 - Dead Sea from Space in 2013 - Dead Sea from Space in July 2013 by Landsat-8 satellite. The most prominent feature in this image is the Dead Sea: the lowest point on Earth's surface, more than 420 m below sea level. The extremely high salinity means fish cannot live in this water body, although there are bacteria and fungi. Note the greenish rectangles just south of the Sea. This is a large complex of mineral evaporation ponds used to produce sodium chloride and other salts for the chemical industry and human and animal consumption. These ponds are separated from the northern part of the Dead Sea by what once was the Lisan Peninsula but lowering water levels have exposed the sea bed, dividing the two sections completely. Throughout the rest of the image we can see built-up areas such as Amman, the capital of Jordan, in the upper right and Jerusalem near the green hills west of the Dead Sea. Further west we can see green patches of agriculture on the coastal pl

Dead Sea from Space 2013 - Dead Sea from Space in 2013 - Dead Sea from Space in July 2013 by Landsat-8 satellite. The most prominent feature in this image is the Dead Sea: the lowest point on Earth's surface, more than 420 m below sea level. The extremely high salinity means fish cannot live in this water body, although there are bacteria and fungi. Note the greenish rectangles just south of the Sea. This is a large complex of mineral evaporation ponds used to produce sodium chloride and other salts for the chemical industry and human and animal consumption. These ponds are separated from the northern part of the Dead Sea by what once was the Lisan Peninsula but lowering water levels have exposed the sea bed, dividing the two sections completely. Throughout the rest of the image we can see built-up areas such as Amman, the capital of Jordan, in the upper right and Jerusalem near the green hills west of the Dead Sea. Further west we can see green patches of agriculture on the coastal pl

PIX4660817

Supernova 1987A in the Great Magellan Cloud before and after explosion - Sometime during 23 February 1987 a supernova exploded in the Large Magellanic Cloud (LMC), a nearby galaxy. However, the LMC is about 170,000 light years distant, so the supernova exploded 170,000 years ago. It was discovered the following day and brightened rapidly to become the first supernova to be easily visible to the unaided eye for almost 400 years. This photograph shows the field around the site of the supernova in great detail, both before the supernova exploded (right) and about 10 days afterwards, when it was still brightening. The image of the star that exploded to create the supernova (mouseover the image) is elongated (better seen on this bigger image). This does not necessarily indicate any peculiarity or a close companion, rather it is the effect of stars being by chance aligned along the line of sight. Several other examples can be seen in this picture and other, different, blended images are seen

Supernova 1987A in the Great Magellan Cloud before and after explosion - Sometime during 23 February 1987 a supernova exploded in the Large Magellanic Cloud (LMC), a nearby galaxy. However, the LMC is about 170,000 light years distant, so the supernova exploded 170,000 years ago. It was discovered the following day and brightened rapidly to become the first supernova to be easily visible to the unaided eye for almost 400 years. This photograph shows the field around the site of the supernova in great detail, both before the supernova exploded (right) and about 10 days afterwards, when it was still brightening. The image of the star that exploded to create the supernova (mouseover the image) is elongated (better seen on this bigger image). This does not necessarily indicate any peculiarity or a close companion, rather it is the effect of stars being by chance aligned along the line of sight. Several other examples can be seen in this picture and other, different, blended images are seen

PIX4582330

Aral Sea seen by the shuttle Endeavour 09/1992 - Aral sea seen from the space shuttle Endeavour. 09/1992 - The Aral Sea observed by the shuttle Endeavour in September 1992. A much depleted Aral Sea can be seen in this south - looking, low - oblique view. The emerging, pointed island of Barsa - Kel'mes and the expanding, broad Vozrozhdeniya Island are visible in the center of the sea. Vozrozhdeniya Island is expanding southward towards the Amu Darya River Delta and northward towards the growing Kulandy Peninsula. Continued shrinkage of the Aral Sea water levels will eventually cut off the western portion from the rest of the sea. This phenomenon has already occurred in the extreme northern portion of the sea. Because of dropping water levels, the Karatyup Peninsula (the stretch of land visible north of the main portion of the Aral Sea) has expanded eastward and connected with the delta of the Syr Darya River, cutting off the extreme northern portion from the larger main area of the Aral

Aral Sea seen by the shuttle Endeavour 09/1992 - Aral sea seen from the space shuttle Endeavour. 09/1992 - The Aral Sea observed by the shuttle Endeavour in September 1992. A much depleted Aral Sea can be seen in this south - looking, low - oblique view. The emerging, pointed island of Barsa - Kel'mes and the expanding, broad Vozrozhdeniya Island are visible in the center of the sea. Vozrozhdeniya Island is expanding southward towards the Amu Darya River Delta and northward towards the growing Kulandy Peninsula. Continued shrinkage of the Aral Sea water levels will eventually cut off the western portion from the rest of the sea. This phenomenon has already occurred in the extreme northern portion of the sea. Because of dropping water levels, the Karatyup Peninsula (the stretch of land visible north of the main portion of the Aral Sea) has expanded eastward and connected with the delta of the Syr Darya River, cutting off the extreme northern portion from the larger main area of the Aral

PIX4660989

The planetary nebula Dumbbell (M27) is located about 1200 light years from Earth in the constellation Little Fox. 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. In this image the nova appeared on August 18, 2005 is visible. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high-energy, ultraviolet light from the core ionizes the cloud. On the evening of August 17- 18, 2005, two European astronomers simultaneously discovered a new star in the Dumbbell Nebula. This image is a portrait of the Dumbbell Nebula featuring the 2005 nova. It is comprised of thirty separate fifte

The planetary nebula Dumbbell (M27) is located about 1200 light years from Earth in the constellation Little Fox. 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. In this image the nova appeared on August 18, 2005 is visible. The Dumbbell Nebula (M27, NGC6853), is a planetary nebula located about 1200 light years from the earth in the constellation of Vulpecula. The nebula was formed when an evolved, red giant star ejected its outer envelope near the end of its lifetime. The expanding cloud of gas becomes visible once the hot core of the star, visible near the center, is exposed and the high-energy, ultraviolet light from the core ionizes the cloud. On the evening of August 17- 18, 2005, two European astronomers simultaneously discovered a new star in the Dumbbell Nebula. This image is a portrait of the Dumbbell Nebula featuring the 2005 nova. It is comprised of thirty separate fifte

R. Jay GaBany

PIX4623431

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

Atafu Atoll - Tokelau Islands, South Pacific - Atafu Atoll, Tokelau, Southern Pacific Ocean - Atafu is a small atoll belonging to the Tokelau Archipelago, in the South Pacific Ocean. With an elevation of two metres above the water, this coral reef is still vulnerable to cyclones and to the rise of water due to global warming. At roughly eight kilometers wide, Atafu Atoll is the smallest of three atolls and one island (Nukunonu and Fakaofo Atoll to the southeast and Swains Island to the south are not shown) comprising the Tokelau Islands group located in the southern Pacific Ocean. The primary settlement on Atafu is a village located at the northwestern corner of the atoll - - indicated by an area of light gray dots in this astronaut photograph. The typical ring shape of the atoll is the result of coral reefs building up around a former volcanic island. Over geologic time, the central volcano has subsided beneath the water surface, leaving the fringing reefs and a central lagoon that co

PIX4675640

Persee Galaxy Cluster - Perseus galaxy cluster - The Persee galaxy cluster (Abell 426) contains at least 500 galaxies including the large elliptical galaxy NGC 1275. This galaxy (the galaxy with pink filaments to the left of the image) is located about 235 million years ago - light; it is a very strong source of radio wave transmission known as Perseus A. In the right center of the image, note the presence of a supernova, SN 2008fg, in a small blue spiral galaxy, NGC 1268. Perseus galaxy cluster (Abell 426) is a cluster of about 500 galaxies. The biggest (left) is NGC 1275, located 235 million light years away; it is a strong radio source known as Perseus A. The gravity exerted by the luminous parts of a galaxy cluster is insufficient to hold the cluster together. Thus, scientists have concluded the missing adhesive must be dark matter and since it's invisible to modern instruments - it can only be inferred. So, when one views the image of the Perseus Galaxy Cluster, ones sees only a s

Persee Galaxy Cluster - Perseus galaxy cluster - The Persee galaxy cluster (Abell 426) contains at least 500 galaxies including the large elliptical galaxy NGC 1275. This galaxy (the galaxy with pink filaments to the left of the image) is located about 235 million years ago - light; it is a very strong source of radio wave transmission known as Perseus A. In the right center of the image, note the presence of a supernova, SN 2008fg, in a small blue spiral galaxy, NGC 1268. Perseus galaxy cluster (Abell 426) is a cluster of about 500 galaxies. The biggest (left) is NGC 1275, located 235 million light years away; it is a strong radio source known as Perseus A. The gravity exerted by the luminous parts of a galaxy cluster is insufficient to hold the cluster together. Thus, scientists have concluded the missing adhesive must be dark matter and since it's invisible to modern instruments - it can only be inferred. So, when one views the image of the Perseus Galaxy Cluster, ones sees only a s

R. Jay GaBany

PIX4565332

Aerially exposed corals

Aerially exposed corals

NHM1458224

Portion of Charleston exposed to the fire of the Federal fleet, August 1863 (engraving)

Portion of Charleston exposed to the fire of the Federal fleet, August 1863 (engraving)

American School, (19th century) (after)

LLM959547

"She was exposed to the wild beasts" (engraving)

"She was exposed to the wild beasts" (engraving)

English School, (19th century)

LLM6004420

An Accra Belle in all her youthful pride (colour photo)

An Accra Belle in all her youthful pride (colour photo)

English Photographer, (20th century)

LLM3106235

A Syrian criminal being punished

A Syrian criminal being punished

UIG3735835

"She was exposed to the wild beasts" (engraving)

"She was exposed to the wild beasts" (engraving)

English School, (19th century)

LLM5992219

Window depicting Saint Stephen's Body exposed to the Animals (stained glass)

Window depicting Saint Stephen's Body exposed to the Animals (stained glass)

PC1278453

Squatted building, 2002 (photo)

Squatted building, 2002 (photo)

Lola Claeys Bouuaert

LCL364339

Jamaican interior (photo)

Jamaican interior (photo)

Lucinda Lambton

LLW993120

The Great Disaster on the Thames (engraving)

The Great Disaster on the Thames (engraving)

English School, (19th century)

LIP1621908

John Hayes's head exposed in St Margaret's church yard (engraving)

John Hayes's head exposed in St Margaret's church yard (engraving)

English School, (18th century)

LLJ608128

Squatted building, 2002 (photo)

Squatted building, 2002 (photo)

Lola Claeys Bouuaert

LCL364340

A Syrian criminal being punished.

A Syrian criminal being punished.

UIG5307615

Flying Nike, Victory, Hellenistic Period (terracotta)

Flying Nike, Victory, Hellenistic Period (terracotta)

Greek school, (2nd century BC)

BST424886

Diana and Callisto

Diana and Callisto

Orley, Richard van (1663-1732)

BAL37956

Jamaican interior (photo)

Jamaican interior (photo)

Lucinda Lambton

LLW993141

Ms Lat. Q.v.I.126 fol.17 The Drunkenness of Noah, from 'Book of Hours of Louis d'Orleans', 1490 (vellum)

Ms Lat. Q.v.I.126 fol.17 The Drunkenness of Noah, from 'Book of Hours of Louis d'Orleans', 1490 (vellum)

Colombe, Jean (c.1430-c.93)

XJL197005

Woman sitting in a park, 1688 (oil on canvas)

Woman sitting in a park, 1688 (oil on canvas)

Weenix, Jan (1642-1719)

XIR420042

'I Swear You Are an Englishman': the author's disguise is exposed in Herat, from 'Travels in Central Asia...in...1863, 1864' by Arminius Vambery (engraving) (b/w photo)

'I Swear You Are an Englishman': the author's disguise is exposed in Herat, from 'Travels in Central Asia...in...1863, 1864' by Arminius Vambery (engraving) (b/w photo)

English School, (19th century)

TRV227729

Couple Indulging in Sexual Play, c.1820-35 (colour litho)

Couple Indulging in Sexual Play, c.1820-35 (colour litho)

Deveria, Achille (1800-57)

STC437628

Study for Noah in 'The Drunkenness of Noah', 1508-12 (charcoal on paper) (recto)

Study for Noah in 'The Drunkenness of Noah', 1508-12 (charcoal on paper) (recto)

Buonarroti, Michelangelo (1475-1564)

BAL192502

A Baggara Married Lady, Omdurman (b/w photo)

A Baggara Married Lady, Omdurman (b/w photo)

European Photographer, (20th century)

LLM5212217

A Snow Storm, c.1891 (oil on canvas)

A Snow Storm, c.1891 (oil on canvas)

Stott, William Edward (1859-1918)

LMG100073

Paint on wall (photo)

Paint on wall (photo)

DND357827

Coral exposed during a low spring tide (colour photo)

Coral exposed during a low spring tide (colour photo)

Roughley, Theodore Cleveland (1881-1961)

LLM5220378

Girl with Red Hair (pastel on canvas)

Girl with Red Hair (pastel on canvas)

Gervex, Henri (1852-1929)

NUM712154

Three female artistes, wearing body stockings (b/w photo)

Three female artistes, wearing body stockings (b/w photo)

European Photographer, (20th century)

LLM3093011

Miss Lucy Waters (engraving)

Miss Lucy Waters (engraving)

Harding, S. (18th century) (after)

LLM3623156

Jeune Egyptienne (b/w photo)

Jeune Egyptienne (b/w photo)

European Photographer, (20th century)

LLM5212230

Lovers in the Open Air, c.1830-40 (colour litho)

Lovers in the Open Air, c.1830-40 (colour litho)

Deveria, Achille (1800-57)

STC437630

Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

Copper Mines in Arizona - USA - Open pit Copper mines - Arizona: Three open-air copper mines near the city of Green Valley in Arizona. Image taken from the International Space Station (ISS) on January 14, 2010. This astronaut photograph illustrates three open-pit mines located west-northwest of the town of Green Valley, Arizona. While the mines appear to be close to each other, each exploits a separate porphyry copper deposit. The mine pits are recognizable by the concentric lines of benches cut into the pit sides. The benches allow equipment and personnel access to the fresh ore (gray) exposed at the bottom of the excavation. Water may also pool at the bottom of inactive pits, such as in the Twin Buttes Mine at image upper right (black areas). The open pit areas are surrounded by an array of sculpted tailings ponds and mine dump areas; these receive mine waste rock for storage and later leaching for further recovery of metals. The green color of the water in the tailings pond at image

PIX4672551

York Illustrated (engraving)

York Illustrated (engraving)

English School, (19th century)

LIP1054549

«
1
2
3
…
27
»

Pourquoi choisir Bridgeman Images

Art. Culture. Histoire.

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

Découvrez notre collection Consultez nos FAQs

Simple. Rapide. Fiable.

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

Contactez-nous

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

Commencez votre recherche

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