'Satellite' 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":"PIX4630291","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planets_of_the_solar_system_2006_our_solar_system_2006_planets_are_represented_in_order_of_proximity","item_variant":"undefined"},{"item_id":"PIX4637908","item_category2":"no_copyright","item_category3":"standard","item_category4":"serge_brunier","item_category5":"not_balown","item_list_name":"search_results","item_name":"panorama_of_the_milky_way_panorama_of_the_milky_way_photographic_mosaic_reconstructing_the_entire_la","item_variant":"undefined"},{"item_id":"PIX4609643","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1097_ngc_1097_a_barred_spiral_galaxy_and_elliptical_companion_located_at_a_","item_variant":"undefined"},{"item_id":"PIX4608970","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"andromede_galaxy_m31_view_in_ultraviolet_the_andromeda_galaxy_seen_in_uv_this_ultraviolet_image_is_a","item_variant":"undefined"},{"item_id":"PIX4567832","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"ngc_1850_star_cluster_in_dorado_double_cluster_ngc_1850_in_dorado_the_double_cluster_ngc_1850_is_loc","item_variant":"undefined"},{"item_id":"PIX4620798","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_n159_in_the_great_magellan_cloud_n159_star_forming_region_in_large_magellanic_cloud_lmc_n159_","item_variant":"undefined"},{"item_id":"PIX4609266","item_category2":"no_copyright","item_category3":"standard","item_category4":"d_de_martin","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m33_in_the_triangle_spiral_galaxy_m33_in_triangulum_m33_ngc_598_the_galaxy_of_the_tria","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":"PIX4608891","item_category2":"no_copyright","item_category3":"standard","item_category4":"sebastian_voltmer","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m31_in_andromede_spiral_galaxy_m31_in_andromeda_the_galaxy_of_andromede_is_located_abo","item_variant":"undefined"},{"item_id":"PIX4621402","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_iras_05437_2502_nebula_iras_05437_2502_nebula_iras_05437_2502_is_located_in_the_constellation","item_variant":"undefined"},{"item_id":"PIX4613420","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"irregular_galaxy_of_the_little_magellan_cloud_ngc_292_the_small_magellanic_cloud_the_galaxy_of_the_l","item_variant":"undefined"},{"item_id":"PIX4609650","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1097_in_the_furnace_barred_spiral_galaxy_ngc_1097_in_fornax_located_at_a_di","item_variant":"undefined"},{"item_id":"PIX4609641","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1097_in_the_furnace_barred_spiral_galaxy_ngc_1097_in_fornax_located_at_a_di","item_variant":"undefined"},{"item_id":"IMO8757626","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX5619685","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"distorted_moonrise","item_variant":"undefined"},{"item_id":"PIX4649091","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"two_space_shuttles_on_fire_pads_09_2008_two_space_shuttles_on_launch_pads_09_2008_view_of_shooting_s","item_variant":"undefined"},{"item_id":"PIX4649108","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"two_space_shuttles_on_fire_pads_09_2008_two_space_shuttles_on_launch_pads_09_2008_view_of_shooting_s","item_variant":"undefined"},{"item_id":"PIX4583187","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":"IMO8757602","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4565011","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_m54_in_sagittarius_globular_cluster_m54_in_sagittarius_the_globular_cluster_m54_pho","item_variant":"undefined"},{"item_id":"PIX4620802","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"nebula_n44_in_the_large_magellan_cloud_superbubble_lha_120_n_44_in_the_large_magellanic_cloud_this_i","item_variant":"undefined"},{"item_id":"PIX4609662","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"active_galaxy_ngc_1068_in_the_whale_active_galaxy_ngc_1068_this_composite_image_shows_that_a_strong_","item_variant":"undefined"},{"item_id":"IMO8757604","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757612","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757640","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4565684","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_cluster_1e_0657_556_dark_matter_in_the_galaxy_cluster_1e_0657_556_composite_view_of_the_gal","item_variant":"undefined"},{"item_id":"IMO8757605","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757620","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4649085","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"two_space_shuttles_on_fire_pads_09_2008_two_space_shuttles_on_launch_pads_09_2008_view_of_shooting_s","item_variant":"undefined"},{"item_id":"PIX4649103","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"two_space_shuttles_on_fire_pads_09_2008_two_space_shuttles_on_launch_pads_09_2008_view_of_shooting_s","item_variant":"undefined"},{"item_id":"PIX4604573","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_european_launch_vehicle_vega_illustration_european_vega_launcher_illustration_vega_is_a_european","item_variant":"undefined"},{"item_id":"PIX4577012","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"moon_cratere_copernic_moon_copernicus_crater_cratere_copernic_image_obtained_in_december_1972_from_t","item_variant":"undefined"},{"item_id":"PIX4608699","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m31_in_andromede_first_color_photo_the_first_color_image_of_spiral_galaxy_m31_in_andro","item_variant":"undefined"},{"item_id":"PIX4637936","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_galactic_center_seen_by_spitzer_space_telescope_the_galactic_center_region_seen_by_spitzer_satel","item_variant":"undefined"},{"item_id":"IMO8757695","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757701","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757589","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757593","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757653","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757659","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757677","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757680","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757681","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757690","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757596","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4608878","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m31_in_andromede_detail_the_southern_arm_of_the_andromeda_galaxy_m31_view_of_the_south","item_variant":"undefined"},{"item_id":"PIX4608960","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"infrared_view_of_the_andromeda_galaxy_infrared_view_of_the_andromeda_galaxy_this_image_shows_the_dif","item_variant":"undefined"},{"item_id":"IMO8757684","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757697","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757619","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757629","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757636","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757660","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757666","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4565787","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_clusters_abell_2744_black_material_x_rays_dark_matter_and_galaxies_in_cluster_abell_2744","item_variant":"undefined"},{"item_id":"PIX4583131","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"pulsar_of_crab_in_taurus_seen_in_x_the_crab_nebula_pulsar_pulsar_of_crab_in_taurus_seen_in_x_by_sate","item_variant":"undefined"},{"item_id":"IMO8757685","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757644","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"IMO8757645","item_category2":"no_copyright","item_category3":"standard","item_category4":"sachsische_zeitung","item_category5":"not_balown","item_list_name":"search_results","item_name":"saxony_gdr_historical_turn_upheaval_autumn_89_fall_of_the_wall_case_the_wall_opening_of_borders_repo","item_variant":"undefined"},{"item_id":"PIX4623257","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planetary_nebula_ngc_6543_in_the_dragon_planetary_nebula_ngc_6543_in_draco_composite_view_of_the_pla","item_variant":"undefined"}]}}

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

Advanced Search Search Tips

Images of 'Satellite' found, 14,404

«
1
…
238
239
240
…
241
»

Planets of the solar system -2006 - Our solar system. 2006 - Planets are represented in order of proximity to the sun. From top to bottom: Mercury, Venus, Earth and Moon, its satellite, Mars, Jupiter, Saturn, Uranus, Neptune. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. This is a montage of planetary images taken by spacecraft managed by the Jet Propulsion Laboratory in Pasadena, CA. Included are (from top to bottom) images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus and Neptune. The spacecraft responsible for these images are as follows: the Mercury image was taken by Mariner 10, the Venus image by Magellan, the Earth and Moon images by Galileo, the Mars image by Mars Global Surveyor, the Jupiter image by Cassini, and the Saturn, Uranus and Neptune images by Voyager. Pluto is not shown as no spacecraft has yet visited it. The inner planets (Mercury, Venus, Earth, Moon, and Mars) are roug

Planets of the solar system -2006 - Our solar system. 2006 - Planets are represented in order of proximity to the sun. From top to bottom: Mercury, Venus, Earth and Moon, its satellite, Mars, Jupiter, Saturn, Uranus, Neptune. Since August 2006, Pluto is now called 134340 Pluto and is no longer considered a planet but designed as a dwarf planet. This is a montage of planetary images taken by spacecraft managed by the Jet Propulsion Laboratory in Pasadena, CA. Included are (from top to bottom) images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus and Neptune. The spacecraft responsible for these images are as follows: the Mercury image was taken by Mariner 10, the Venus image by Magellan, the Earth and Moon images by Galileo, the Mars image by Mars Global Surveyor, the Jupiter image by Cassini, and the Saturn, Uranus and Neptune images by Voyager. Pluto is not shown as no spacecraft has yet visited it. The inner planets (Mercury, Venus, Earth, Moon, and Mars) are roug

PIX4630291

Panorama of the Milky Way - Panorama of the Milky Way - Photographic mosaic reconstructing the entire lactee path. The shots taken between summer 2008 and summer 2009 were taken from two perfect astronomical sites, the Atacama desert for the southern hemisphere, the Caldera de Taburiente in the Canary Islands for the boreal hemisphere. This magnificent 360-degree panoramic image, covering the entire southern and northern celestial sphere, reveals the cosmic landscape that surrounds our tiny blue planet. The plane of our Milky Way Galaxy, which we see edge-on from our perspective on Earth, cuts a luminous swath across the image. From this vantage point, the general components of our spiral galaxy come clearly into view, including its disc, marbled with both dark and glowing nebulae, which harbours bright, young stars, as well as the Galaxy's central bulge and its satellite galaxies. As filming extended over several months, objects from the Solar System came and went through the star fie

Panorama of the Milky Way - Panorama of the Milky Way - Photographic mosaic reconstructing the entire lactee path. The shots taken between summer 2008 and summer 2009 were taken from two perfect astronomical sites, the Atacama desert for the southern hemisphere, the Caldera de Taburiente in the Canary Islands for the boreal hemisphere. This magnificent 360-degree panoramic image, covering the entire southern and northern celestial sphere, reveals the cosmic landscape that surrounds our tiny blue planet. The plane of our Milky Way Galaxy, which we see edge-on from our perspective on Earth, cuts a luminous swath across the image. From this vantage point, the general components of our spiral galaxy come clearly into view, including its disc, marbled with both dark and glowing nebulae, which harbours bright, young stars, as well as the Galaxy's central bulge and its satellite galaxies. As filming extended over several months, objects from the Solar System came and went through the star fie

Serge Brunier

PIX4637908

Barree spiral galaxy NGC 1097 - NGC 1097, a barred spiral galaxy and elliptical companion - Located at a distance of about 45 million years - light in the constellation of the Furnneau, NGC 1097 is subject to intense star formation and is an active nucleus galaxy with a supermassive black hole in its heart. At the top right of the image, a special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by Siding Spring's 3.9m telescope. NGC 1097 is a fine, barred spiral galaxy seen from a distance of about 50 million light years. The galaxy is unusual in several respects. It is a fairly strong radio source and is also bright at far infrared wavelenghts, indicating the presence of warm dust. The galaxy is also interacting woth a small elliptical galaxy, seen in the upper right (NW) corner of the picture. This galaxy shows the subtle interleaved 'shells' or stepped changes in brightness resulting from the interaction. Finally, the galaxy is k

Barree spiral galaxy NGC 1097 - NGC 1097, a barred spiral galaxy and elliptical companion - Located at a distance of about 45 million years - light in the constellation of the Furnneau, NGC 1097 is subject to intense star formation and is an active nucleus galaxy with a supermassive black hole in its heart. At the top right of the image, a special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by Siding Spring's 3.9m telescope. NGC 1097 is a fine, barred spiral galaxy seen from a distance of about 50 million light years. The galaxy is unusual in several respects. It is a fairly strong radio source and is also bright at far infrared wavelenghts, indicating the presence of warm dust. The galaxy is also interacting woth a small elliptical galaxy, seen in the upper right (NW) corner of the picture. This galaxy shows the subtle interleaved 'shells' or stepped changes in brightness resulting from the interaction. Finally, the galaxy is k

PIX4609643

Andromede Galaxy (M31) view in ultraviolet - The Andromeda galaxy seen in UV - This ultraviolet image is a mosaic of 10 images obtained by the GALEX satellite in September and October 2003. Regions of blue stars, young, warm and massive stars are clearly visible in the arms, where the stars are formed; in the center near the core, colder, orange-white, much older stars. The stars visible in the foreground belong to our Lactee Way. The GALEX observation of the large galaxy in Andromeda, Messier 31, was performed during September and October 2003. The image is a mosaic of 10 separate GALEX images combining the Far UV (colored blue) and Near UV detector (colored red) images together to make a color image of the sky almost six full moons across. The Andromeda galaxy is the most massive in the local group of galaxies, which includes our Milky Way, and is the nearest large galaxy to our own. The GALEX image shows blue regions of young, hot, high mass stars tracing out the spiral arms where s

Andromede Galaxy (M31) view in ultraviolet - The Andromeda galaxy seen in UV - This ultraviolet image is a mosaic of 10 images obtained by the GALEX satellite in September and October 2003. Regions of blue stars, young, warm and massive stars are clearly visible in the arms, where the stars are formed; in the center near the core, colder, orange-white, much older stars. The stars visible in the foreground belong to our Lactee Way. The GALEX observation of the large galaxy in Andromeda, Messier 31, was performed during September and October 2003. The image is a mosaic of 10 separate GALEX images combining the Far UV (colored blue) and Near UV detector (colored red) images together to make a color image of the sky almost six full moons across. The Andromeda galaxy is the most massive in the local group of galaxies, which includes our Milky Way, and is the nearest large galaxy to our own. The GALEX image shows blue regions of young, hot, high mass stars tracing out the spiral arms where s

PIX4608970

NGC 1850 Star Cluster in Dorado - Double Cluster NGC 1850 in Dorado - The double cluster NGC 1850 is located in the galaxy of the Great Magellan Cloud. It contains a cluster of globular form, but young, 50 million years, in the center of the image and another cluster, at the bottom right, even younger (4 million years), consists of warm and blue stars and a few T - Tauri stars. NGC 1850, imaged here with the NASA/ESA Hubble Space Telescope, is an unusual double cluster that lies in the bar of the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. After the 30 Doradus complex, NGC 1850 is the brightest star cluster in the Large Magellanic Cloud. It is representative of a special class of objects - young, globular - like star clusters - that have no counterpart in our own Galaxy. The two components of the cluster are both relatively young and consist of a main globular - like cluster in the centre and an even younger, smaller cluster, seen below and to the right, composed o

NGC 1850 Star Cluster in Dorado - Double Cluster NGC 1850 in Dorado - The double cluster NGC 1850 is located in the galaxy of the Great Magellan Cloud. It contains a cluster of globular form, but young, 50 million years, in the center of the image and another cluster, at the bottom right, even younger (4 million years), consists of warm and blue stars and a few T - Tauri stars. NGC 1850, imaged here with the NASA/ESA Hubble Space Telescope, is an unusual double cluster that lies in the bar of the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. After the 30 Doradus complex, NGC 1850 is the brightest star cluster in the Large Magellanic Cloud. It is representative of a special class of objects - young, globular - like star clusters - that have no counterpart in our own Galaxy. The two components of the cluster are both relatively young and consist of a main globular - like cluster in the centre and an even younger, smaller cluster, seen below and to the right, composed o

PIX4567832

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

Nebula N159 in the Great Magellan Cloud - N159 star forming region in Large Magellanic Cloud (LMC): N159 is a star-forming region located in the galaxy of the Great Magellan Cloud. Image obtained by the Hubble Space Telescope (HST) - This shot from the NASA/ESA Hubble Space Telescope shows a maelstrom of glowing gas and dark dust within one of the Milky Way's satellite galaxies, the Large Magellanic Cloud (LMC). This stormy scene shows a stellar nursery known as N159, an HII region over 150 light-years across. N159 contains many hot young stars. These stars are emitting intense ultraviolet light, which causes nearby hydrogen gas to glow, and torrential stellar winds, which are carving out ridges, arcs, and filaments from the surrounding material. At the heart of this cosmic cloud lies the Papillon Nebula, a butterfly-shaped region of nebulosity. This small, dense object is classified as a High-Excitation Blob, and is thought to be tightly linked to the early stages of massive star form

PIX4620798

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This image is a composite of two black and white images obtained from the 1.2m telescope of Mount Palomar, California. Spiral galaxy M33 is a mid - sized member of our Local Group of Galaxies. M33 is also called the Triangulum Galaxy for the constellation in which it resides. About four times smaller (in radius) than our Milky Way Galaxy and the Andromeda Galaxy (M31), it is much larger than the many of the local dwarf spheroidal galaxies. M33's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon, and be visible with a good pair of binoculars. <BR>This image is a composite from black and

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This image is a composite of two black and white images obtained from the 1.2m telescope of Mount Palomar, California. Spiral galaxy M33 is a mid - sized member of our Local Group of Galaxies. M33 is also called the Triangulum Galaxy for the constellation in which it resides. About four times smaller (in radius) than our Milky Way Galaxy and the Andromeda Galaxy (M31), it is much larger than the many of the local dwarf spheroidal galaxies. M33's proximity to M31 causes it to be thought by some to be a satellite galaxy of this more massive galaxy. M33's proximity to our Milky Way Galaxy causes it to appear more than twice the angular size of the Full Moon, and be visible with a good pair of binoculars. <BR>This image is a composite from black and

D. De Martin

PIX4609266

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

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) at the top, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great Galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years. Die Andromeda - Galaxie liegt in einer Entfernung von rund 2,5 Millionen Lichtjahren. Der Durchmesser der sichtbaren Scheibe betraegt 150.

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) at the top, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. M31, the Great Galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years. Die Andromeda - Galaxie liegt in einer Entfernung von rund 2,5 Millionen Lichtjahren. Der Durchmesser der sichtbaren Scheibe betraegt 150.

Sebastian Voltmer

PIX4608891

Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 is located in the constellation Taurus. Image obtained by the Hubble Space Telescope (HST). The little - known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. It appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye - catching shapes of the gas. However, the bright boomerang - shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp - edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 20

Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 - Nebula IRAS 05437+2502 is located in the constellation Taurus. Image obtained by the Hubble Space Telescope (HST). The little - known nebula IRAS 05437+2502 billows out among the bright stars and dark dust clouds that surround it in this striking image from the Hubble Space Telescope. It is located in the constellation of Taurus (the Bull), close to the central plane of our Milky Way galaxy. It appears to be a small, rather isolated, region of star formation and one might assume that the effects of fierce ultraviolet radiation from bright young stars probably were the cause of the eye - catching shapes of the gas. However, the bright boomerang - shaped feature may tell a more dramatic tale. The interaction of a high velocity young star and the cloud of gas and dust may have created this unusually sharp - edged bright arc. Such a reckless star would have been ejected from the distant young cluster where it was born and would travel at 20

PIX4621402

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Infrared image obtained by Spitzer space telescope. This infrared portrait of the Small Magellanic Cloud, taken by Nasa's Spitzer Space Telescope, reveals the stars and dust in this galaxy as never seen before. The Small Magellanic Cloud is a nearby satellite galaxy to our Milky Way galaxy, approximately 200,000 light - years away. The image shows the main body of the Small Magellanic Cloud, which is comprised of the “” bar”” on the left and a “” wing”” extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. In addition, the image contains a galactic globular cluster in the lower left (blue cluster of stars) and emission from

Irregular Galaxy of the Little Magellan Cloud (NGC 292) - The Small Magellanic Cloud - The galaxy of the Little Magellan Cloud is about 240,000 light years from Earth in the southern constellation of Toucan. It's one of the closest galaxies of the Lactee Way. Infrared image obtained by Spitzer space telescope. This infrared portrait of the Small Magellanic Cloud, taken by Nasa's Spitzer Space Telescope, reveals the stars and dust in this galaxy as never seen before. The Small Magellanic Cloud is a nearby satellite galaxy to our Milky Way galaxy, approximately 200,000 light - years away. The image shows the main body of the Small Magellanic Cloud, which is comprised of the “” bar”” on the left and a “” wing”” extending to the right. The bar contains both old stars (in blue) and young stars lighting up their natal dust (green/red). The wing mainly contains young stars. In addition, the image contains a galactic globular cluster in the lower left (blue cluster of stars) and emission from

PIX4613420

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. A special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by combining several poses of several hours. Located at a distance of about 45 million light - years in the southern constellation Fornax, NGC 1097 is a relatively bright, barred spiral galaxy of type SBB, seen face - on. At magnitude 9.5, and thus just 25 times fainter than the faintest object that can be seen with the unaided eye, it appears in small telescopes as a bright, circular disc. NGC 1097 is an active galaxy with an Active Galactic Nuclei (AGN), whose emission is thought to arise from matter (gas and stars) falling into oblivion in a central black hole. There is indeed much evidence that a supermassiv

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. A special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by combining several poses of several hours. Located at a distance of about 45 million light - years in the southern constellation Fornax, NGC 1097 is a relatively bright, barred spiral galaxy of type SBB, seen face - on. At magnitude 9.5, and thus just 25 times fainter than the faintest object that can be seen with the unaided eye, it appears in small telescopes as a bright, circular disc. NGC 1097 is an active galaxy with an Active Galactic Nuclei (AGN), whose emission is thought to arise from matter (gas and stars) falling into oblivion in a central black hole. There is indeed much evidence that a supermassiv

R. Gendler

PIX4609650

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. At the top right of the image, a special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by combining several poses of several hours. Located at a distance of about 45 million light - years in the southern constellation Fornax, NGC 1097 is a relatively bright, barred spiral galaxy of type SBB, seen face - on. At magnitude 9.5, and thus just 25 times fainter than the faintest object that can be seen with the unaided eye, it appears in small telescopes as a bright, circular disc. NGC 1097 is an acive galaxy with an Active Galactic Nuclei (AGN), whose emission is thought to arise from matter (gas and stars) falling into oblivion in a central black hole. There is indeed mu

Barree spiral galaxy NGC 1097 in the Furnace - Barred spiral galaxy NGC 1097 in Fornax - Located at a distance of about 45 million years - light, NGC 1097 is the object of intense star formation and is an active core galaxy with a supermassive black hole in its heart. At the top right of the image, a special elliptical satellite galaxy, NGC 1097A, probably interacted with NGC 1097 in the past. Image obtained by combining several poses of several hours. Located at a distance of about 45 million light - years in the southern constellation Fornax, NGC 1097 is a relatively bright, barred spiral galaxy of type SBB, seen face - on. At magnitude 9.5, and thus just 25 times fainter than the faintest object that can be seen with the unaided eye, it appears in small telescopes as a bright, circular disc. NGC 1097 is an acive galaxy with an Active Galactic Nuclei (AGN), whose emission is thought to arise from matter (gas and stars) falling into oblivion in a central black hole. There is indeed mu

PIX4609641

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757626

Distorted Moonrise

Distorted Moonrise

PIX5619685

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). With a rainbow serving as a backdrop in the sky, space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). With a rainbow serving as a backdrop in the sky, space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with

PIX4649091

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). Space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with the payload changeout rooms revealed. The rotatin

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). Space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with the payload changeout rooms revealed. The rotatin

PIX4649108

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. A composite of visible images and X-rays obtained by the Hubble Space Telescope (HST) in 2006 and 2010 and by the Chandra satellite. 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

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. A composite of visible images and X-rays obtained by the Hubble Space Telescope (HST) in 2006 and 2010 and by the Chandra satellite. 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

PIX4583187

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757602

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

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

PIX4565011

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

Nebula N44 in the Large Magellan Cloud - Superbubble LHA 120 - N 44 in the Large Magellanic Cloud - This image obtained by the Very Large Telescope (VLT) shows the nebula N44 surrounding the cluster of stars NGC 1929. It is a star-forming region located in the galaxy of the Great Magellan Cloud, about 170,000 light years from Earth. Eso's Very Large Telescope captured this striking view of the nebula around the star cluster NGC 1929 within the Large Magellanic Cloud, a satellite galaxy of our own Milky Way. A colossal example of what astronomers call a superbubble dominates this stellar nursery. It is being carved by the winds from bright young stars and the shockwaves from supernova explosions. This nebula is officially known as LHA 120 - N 44, or just N 44 for short. Hot young stars in NGC 1929 are emitting intense ultraviolet light and causing the gas to glow. This effect highlights the aptly - named superbubble, a vast shell of material around 325 by 250 light - years across. For c

PIX4620802

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

Active Galaxy NGC 1068 in the Whale - Active galaxy NGC 1068 - This composite image shows that a strong stellar wind escapes from the heart of the galaxy NGC 1068 or resides a massive black hole. NGC 1068 is located about 50 million light years away from Earth. Images obtained in X-ray by the Chandra satellite (red), visible by the Hubble space telescope (green) and radio waves (blue). This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. X - ray data from the Chandra X - ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X - ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. The X - ray images and spectra obtained using Chandra's High Energy Transmission Grating Spectrometer show that a strong wind is being driven aw

PIX4609662

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757604

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757612

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757640

Galaxies cluster 1E 0657 - 556 - Dark matter in the galaxy cluster 1E 0657 - 556 - Composite view of the galaxy cluster 1E 0657 - 556 visible and X-rays. The hot gas that surrounds this galaxy cluster, detects in X-rays by the Chandra satellite, is visible in pink on this image. The galaxy cluster, photographed by the Magellan telescope and the Hubble space telescope, appears in the background. By studying the mass of this cluster, astronomers were able to determine that most of this mass was concentrated not in the hot gas detected by Chandra but in the blue coloured areas here, suggesting the existence of dark matter. This composite image shows the galaxy cluster 1E 0657 - 556, also known as the “” bullet cluster.”” This cluster was formed after the collision of two large clusters of galaxies, the most energetic event known in the universe since the Big Bang. Hot gas detected by Chandra telescope in X - rays is seen as two pink clumps in the image and contains most of the “” normal,”

Galaxies cluster 1E 0657 - 556 - Dark matter in the galaxy cluster 1E 0657 - 556 - Composite view of the galaxy cluster 1E 0657 - 556 visible and X-rays. The hot gas that surrounds this galaxy cluster, detects in X-rays by the Chandra satellite, is visible in pink on this image. The galaxy cluster, photographed by the Magellan telescope and the Hubble space telescope, appears in the background. By studying the mass of this cluster, astronomers were able to determine that most of this mass was concentrated not in the hot gas detected by Chandra but in the blue coloured areas here, suggesting the existence of dark matter. This composite image shows the galaxy cluster 1E 0657 - 556, also known as the “” bullet cluster.”” This cluster was formed after the collision of two large clusters of galaxies, the most energetic event known in the universe since the Big Bang. Hot gas detected by Chandra telescope in X - rays is seen as two pink clumps in the image and contains most of the “” normal,”

PIX4565684

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757605

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757620

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). With a rainbow serving as a backdrop in the sky, space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). With a rainbow serving as a backdrop in the sky, space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with

PIX4649085

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). Space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with the payload changeout rooms revealed. The rotatin

Two space shuttles on fire pads. 09/2008 - Two Space Shuttles on launch pads. 09/2008 - View of shooting steps A and B from the Kennedy Space center in Florida on September 20, 2008. In the foreground, the shuttle Atlantis, in the background, the shuttle Endeavour on firing pad B. This is the first time since July 2001 that two shuttles have been simultaneously on the firing steps. The shuttle Endeavour was ready to assist the shuttle Atlantis for a rescue mission in case of a problem. Finally, the planned flight of the Atlantis shuttle (STS-125, repair of the Hubble satellite) was postponed until May 2009. The shuttle Endeavour collapsed in November 2008 to continue the construction of the international space station (mission STS-126). Space shuttle Atlantis (foreground) sits on Launch Pad A and Endeavour on Launch Pad B at Nasa's Kennedy Space Center in Florida. At the left of each shuttle are the open rotating service structures with the payload changeout rooms revealed. The rotatin

PIX4649103

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. View of Vega artist on his shooting pitch at the Guyanese Space Center (CSG) in Kourou. Artist view of the new launch pad of ESA's Vega small satellite launcher at the Guyana Space Centre (CSG), Europe's Space Port, in Kourou, French Guiana. The Vega launcher will be operated from the former Ariane Launch Complex n* 1 (ELA-1), which was deactivated in 1989. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega i

The European launch vehicle Vega - Illustration - European Vega Launcher - Illustration - Vega is a European Space Agency (ESA) launcher capable of placing a payload of up to 2 tonnes in low orbit. It is expected that it will join from 2010 the range of launchers of the space agency, which includes launchers Soyuz and Ariane. View of Vega artist on his shooting pitch at the Guyanese Space Center (CSG) in Kourou. Artist view of the new launch pad of ESA's Vega small satellite launcher at the Guyana Space Centre (CSG), Europe's Space Port, in Kourou, French Guiana. The Vega launcher will be operated from the former Ariane Launch Complex n* 1 (ELA-1), which was deactivated in 1989. Under development since 1998, the Vega launcher is an all - solid three - stage vehicle with a liquid - fuelled injection module, based on proven technologies from Ariane 5 booster stages and Fiatavio's Zefiro solid rocket motor. Vega will be marketed and operated by Arianespace, in parallel to Ariane 5. Vega i

PIX4604573

Moon: cratere Copernic - Moon: Copernicus crater - Cratere Copernic. Image obtained in December 1972 from the control module of Apollo 17. An oblique view of the large crater Copernicus on the lunar nearside, as photographed from the Apollo 17 spacecraft in lunar orbit. This view is looking generally southwest towards the crater on the horizon. The coordinates of the center of Copernicus are approximately 20 degrees west longitude and 9.5 degrees north latitude

Moon: cratere Copernic - Moon: Copernicus crater - Cratere Copernic. Image obtained in December 1972 from the control module of Apollo 17. An oblique view of the large crater Copernicus on the lunar nearside, as photographed from the Apollo 17 spacecraft in lunar orbit. This view is looking generally southwest towards the crater on the horizon. The coordinates of the center of Copernicus are approximately 20 degrees west longitude and 9.5 degrees north latitude

PIX4577012

Spiral galaxy M31 in Andromede - First color photo - The first color image of spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) on the left, and M110 (NGC 205) on the bottom right. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. This photo is the first color photo of M31. It was obtained on 11 August 1958 at the Schmidt telescope of Mount Palomar. M31 (NGC 224) is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. It has several close companions, the most obvious of which are the compact elliptical galaxy M32 (NGC 221) at lower left centre here, and M110 (NGC 205) at lower right. M 31 is a member of the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the two Magellanic Clouds. This particular picture is of interest becau

Spiral galaxy M31 in Andromede - First color photo - The first color image of spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany him: M32 (NGC 221) on the left, and M110 (NGC 205) on the bottom right. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. This photo is the first color photo of M31. It was obtained on 11 August 1958 at the Schmidt telescope of Mount Palomar. M31 (NGC 224) is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. It has several close companions, the most obvious of which are the compact elliptical galaxy M32 (NGC 221) at lower left centre here, and M110 (NGC 205) at lower right. M 31 is a member of the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the two Magellanic Clouds. This particular picture is of interest becau

PIX4608699

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

The galactic center seen by Spitzer Space Telescope - The galactic center region seen by Spitzer satellite. The area photographed extends over 890 light-years and over 640 light-years high. In visible light, this area is hidden by a large amount of interstellar dust. This picture in false colors shows the old and cold stars in blue, and the red regions the hot and massive stars. Dark and bright filamentous clouds are star-forming regions. The brightest area in the center of the image is the center of our galaxy which houses a supermassive black hole. This infrared image from Nasa's Spitzer Space Telescope shows hundreds of thousands of stars crowded into the swirling core of our spiral Milky Way galaxy. In visible-light pictures, this region cannot be seen at all because dust lying between Earth and the galactic center blocks our view. In this false-color picture, old and cool stars are blue, while dust features lit up by blazing hot, massive stars are shown in a reddish hue. Both brig

PIX4637936

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757695

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757701

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757589

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757593

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757653

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757659

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757677

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757680

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757681

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757690

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757596

Spiral Galaxy M31 in Andromede - Detail - The southern arm of the Andromeda galaxy, M31 - View of the southern arm of the Andromede galaxy. Visible to the naked eye, the Andromede galaxy is located about 2 million years away from Earth. In this image obtained in La Palma, one of its two satellite galaxies is visible to the north-east: M32 (NGC 221). Also visible is the star cloud NGC 206, low centre, one of the largest star formations regions of our local group. Like the lactee path, the Andromede galaxy belongs to the local group, which consists of about thirty galaxies. M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star - forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also he

Spiral Galaxy M31 in Andromede - Detail - The southern arm of the Andromeda galaxy, M31 - View of the southern arm of the Andromede galaxy. Visible to the naked eye, the Andromede galaxy is located about 2 million years away from Earth. In this image obtained in La Palma, one of its two satellite galaxies is visible to the north-east: M32 (NGC 221). Also visible is the star cloud NGC 206, low centre, one of the largest star formations regions of our local group. Like the lactee path, the Andromede galaxy belongs to the local group, which consists of about thirty galaxies. M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star - forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also he

PIX4608878

Infrared view of the Andromeda galaxy - Infrared view of the Andromeda galaxy - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, red). By measuring the infrared radiation emitted by a galaxy, more or less important depending on the nature of the stars, the mass of that galaxy can be reduced. According to this method, the mass of stars in the Andromede galaxy would be 110 billion times that of the Sun, which means that this galaxy would have 1 trillion stars (our galaxy had 400 billion). In this image we distinguish the two satellite galaxies of Andromede, M32 at the bottom and NGC 205 (M110) at the top. Infrared composite at the following wavelengths: 3.6 and 4.5 microns: sensitive to star light (blue and green), and 8 micron sensitive to dust in red. 3000 different poses obtained by the Spitzer space telescope in January and August 2005 were required to achieve this complete view o

Infrared view of the Andromeda galaxy - Infrared view of the Andromeda galaxy - This image shows the difference in infrared radiation between the light emitted by the aged stars (blue) and that emitted by the dust (star-forming zone, red). By measuring the infrared radiation emitted by a galaxy, more or less important depending on the nature of the stars, the mass of that galaxy can be reduced. According to this method, the mass of stars in the Andromede galaxy would be 110 billion times that of the Sun, which means that this galaxy would have 1 trillion stars (our galaxy had 400 billion). In this image we distinguish the two satellite galaxies of Andromede, M32 at the bottom and NGC 205 (M110) at the top. Infrared composite at the following wavelengths: 3.6 and 4.5 microns: sensitive to star light (blue and green), and 8 micron sensitive to dust in red. 3000 different poses obtained by the Spitzer space telescope in January and August 2005 were required to achieve this complete view o

PIX4608960

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757684

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757697

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757619

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757629

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757636

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757660

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757666

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

Galaxy clusters Abell 2744 - Black material - X - rays, dark matter and galaxies in cluster Abell 2744

PIX4565787

Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and

Pulsar of Crab in Taurus seen in X - The Crab nebula pulsar - Pulsar of Crab in Taurus seen in X by satellite Chandra. The pulsar is the white dot in the center of the image. This neutron star generates a powerful magnetic field creating material jets at the poles, as well as a strong stellar wind. This image gives the first clear view of the faint boundary of the Crab Nebula's X - ray - emitting pulsar wind nebula. The nebula is powered by a rapidly rotating, highly magnetized neutron star, or pulsar (white dot near the center). The combination of rapid rotating and strong magnetic field generates an intense electromagnetic field that creates jets of matter and anti - matter moving away from the north and south poles of the pulsar, and an intense wind flowing out in the equatorial direction. The inner X - ray ring is thought to be a shock wave that marks the boundary between the surrounding nebula and the flow of matter and antimatter particles from the pulsar. Energetic electrons and

PIX4583131

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757685

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757644

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case the Wall Opening of borders Reportage …, 1985 (photo)

Sächsische Zeitung

IMO8757645

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

Planetary nebula NGC 6543 in the Dragon - Planetary nebula NGC 6543 in Draco - Composite view of the planetary nebula NGC 6543 in the Dragon obtained by the Hubble space telescope and X-ray (blue) by the Chandra satellite. NGC 6543 is located about 3000 years of light from Earth. This composite of data from Nasa's Chandra X - ray Observatory and Hubble Space Telescope is a new look for NGC 6543, better known as the Cat's Eye nebula. This famous object is a so - called planetary nebula that represents a phase of stellar evolution that the Sun should experience several billion years from now. When a star like the Sun begins to run out of fuel, it becomes what is known as a red giant. In this phase, a star sheds some of its outer layers, eventually leaving behind a hot core that collapses to form a dense white dwarf star. A fast wind emanating from the hot core rams into the ejected atmosphere, pushes it outward, and creates the graceful filamentary structures seen with optical telescopes

PIX4623257

«
1
…
238
239
240
…
241
»

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.