'Distant Galaxies' Bilder und Clips Suchergebnisse

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

Ihre AuswahlIhre aktuelle Auswahl

{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"PIX4612895","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_6090_interacting_galaxies_ngc_6090_the_galaxy_ngc_6090_is_located_about_400","item_variant":"undefined"},{"item_id":"PIX4610936","item_category2":"no_copyright","item_category3":"standard","item_category4":"adam_block","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_3718_and_ngc_3729_in_ursa_major","item_variant":"undefined"},{"item_id":"UIG867353","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"this_image_shows_one_of_the_most_distant_galaxies_known_called_gn_108036_dating_back_to_750_million_","item_variant":"undefined"},{"item_id":"UIS5104636","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_ultra_deep_field_view_of_galaxies_2003_2004","item_variant":"undefined"},{"item_id":"PIX4611005","item_category2":"no_copyright","item_category3":"standard","item_category4":"adam_block","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_3718_and_ngc_3729_in_the_great_bear","item_variant":"undefined"},{"item_id":"PIX4610687","item_category2":"no_copyright","item_category3":"standard","item_category4":"vincent_toporenko","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_m105_ngc_3384_and_ngc_3389_in_the_lion_m105_ngc_3384_and_ngc_3389_galaxies_in_leo_these_gal","item_variant":"undefined"},{"item_id":"PIX4610710","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_m105_ngc_3384_and_ngc_3389_in_the_lion_galaxies_m105_ngc_3384_and_ngc_3389_in_leo_these_gal","item_variant":"undefined"},{"item_id":"PIX4610701","item_category2":"no_copyright","item_category3":"standard","item_category4":"jim_misti","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_m105_ngc_3384_and_ngc_3389_in_the_lion_galaxies_m105_ngc_3384_and_ngc_3389_in_leo_these_gal","item_variant":"undefined"},{"item_id":"PIX4610568","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxies_ngc_3314_a_and_b_in_hydra_galaxy_pair_ngc_3314_in_hydra_ngc_3314_is_a_pair_of_spiral","item_variant":"undefined"},{"item_id":"FPA7355397","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355405","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355406","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355408","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355400","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355395","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355398","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"PIX4610320","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"ultraviolet_view_of_the_galaxies_m81_and_m82_ultraviolet_image_of_m81_and_m82_m81_left_is_a_spiral_g","item_variant":"undefined"},{"item_id":"FPA7355396","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355401","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355403","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355394","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355399","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355402","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355404","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"FPA7355407","item_category2":"no_copyright","item_category3":"standard","item_category4":"francois_palluau","item_category5":"not_balown","item_list_name":"search_results","item_name":"francois_hammer_2021_photo","item_variant":"undefined"},{"item_id":"PIX4609879","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1483_in_dorado_barred_spiral_galaxy_ngc_1483_in_dorado_ngc_1483_is_a_barree","item_variant":"undefined"},{"item_id":"PIX4612130","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_jay_gabany","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_5078_and_ic_879_in_hydra_galaxies_ngc_5078_and_ic_879_in_hydra_ngc_5078_is_a_spiral_gal","item_variant":"undefined"},{"item_id":"PIX4613003","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_6786_and_leda_62867_interacting_galaxies_ngc_6786_and_leda_62867_the_galaxy","item_variant":"undefined"},{"item_id":"PIX4612142","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_5078_and_ic_879_in_hydra_galaxies_ngc_5078_and_ic_879_in_hydra_ngc_5078_is_a_spiral_gal","item_variant":"undefined"},{"item_id":"PIX4610539","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"interacting_galaxies_ngc_3256_interacting_galaxies_ngc_3256_the_special_galaxy_ngc_3256_is_located_a","item_variant":"undefined"},{"item_id":"PIX4610948","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_3718_and_ngc_3729_in_the_great_bear_galaxies_ngc_3718_and_ngc_3729_in_ursa_major_ngc_37","item_variant":"undefined"},{"item_id":"PIX4608837","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"center_of_the_andromede_galaxy_m31_center_of_the_andromeda_galaxy_the_andromede_galaxy_is_located_ab","item_variant":"undefined"},{"item_id":"PIX4612223","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_5078_and_ic_879_in_hydra_galaxies_ngc_5078_and_ic_879_in_hydra_ngc_5078_is_a_spiral_gal","item_variant":"undefined"},{"item_id":"PIX4609816","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1345_in_eridan_barred_spiral_galaxy_ngc_1345_in_eridanus_located_about_85_m","item_variant":"undefined"},{"item_id":"PIX4608904","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"core_of_the_andromede_galaxy_m31_the_andromede_galaxy_is_located_about_2_million_years_away_light_fr","item_variant":"undefined"},{"item_id":"PIX4609570","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m77_in_the_whale_active_galaxy_m77_ngc_1068_in_cetus_m77_ngc_1068_this_active_galaxy_i","item_variant":"undefined"},{"item_id":"PIX4610955","item_category2":"no_copyright","item_category3":"standard","item_category4":"jim_misti","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxies_ngc_3718_in_the_great_bear_galaxy_ngc_3718_in_ursa_major_ngc_3718_arp_214_is_a_special_gala","item_variant":"undefined"},{"item_id":"PIX4613338","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"large_and_small_magellan_clouds_large_and_small_magellanic_clouds_these_two_irregular_galaxies_are_c","item_variant":"undefined"},{"item_id":"PIX4564299","item_category2":"no_copyright","item_category3":"standard","item_category4":"d_de_martin","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_47_toucan_the_globular_cluster_47_tucanae_ngc_104_the_globular_cluster_47_toucan_or","item_variant":"undefined"},{"item_id":"UIS5104199","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"mystery_blobs_in_space_c_2006","item_variant":"undefined"},{"item_id":"PIX4609750","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_1309_in_eridan_spiral_galaxy_ngc_1309_in_eridanus_located_about_100_million_years_","item_variant":"undefined"},{"item_id":"PIX4620946","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_formation_region_lh_95_in_the_great_magellan_cloud_nasa_esa_hubble_heritage_team_novapix_lh_95_","item_variant":"undefined"},{"item_id":"PIX4610557","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxies_ngc_3314_a_and_b_in_hydra_galaxy_pair_ngc_3314_in_hydra_ngc_3314_is_a_pair_of_spiral","item_variant":"undefined"},{"item_id":"PIX4612306","item_category2":"no_copyright","item_category3":"standard","item_category4":"e_mouquet","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m51_in_hunting_dogs_spiral_galaxy_m51_in_canes_venatici_the_spiral_galaxy_m51_ngc_5194","item_variant":"undefined"},{"item_id":"PIX7331184","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"first_image_of_the_jwst_smacs_galaxy_cluster_0723_2022_photography","item_variant":"undefined"},{"item_id":"PIX4613035","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_6872_in_interaction_with_ic_4970_in_the_peacock_barred_spiral_interacting_g","item_variant":"undefined"},{"item_id":"PIX4609731","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1300_in_eridan_ngc_1300_barred_spiral_galaxy_in_eridanus_the_galaxy_ngc_130","item_variant":"undefined"},{"item_id":"PIX4564305","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_47_toucan_the_globular_cluster_47_tucanae_ngc_104_the_globular_cluster_47_toucan_or","item_variant":"undefined"},{"item_id":"PIX4611058","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_ngc_4027_in_the_raven_galaxy_ngc_4027_in_corvus_ngc_4027_is_a_spiral_galaxy_located_about_80_","item_variant":"undefined"},{"item_id":"PIX4609752","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_1300_in_eridan_barred_spiral_galaxy_ngc_1300_in_eridanus_the_galaxy_ngc1300","item_variant":"undefined"},{"item_id":"UIS5090990","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_constellation_leo_1603","item_variant":"undefined"},{"item_id":"MMM7341114","item_category2":"in_copyright","item_category3":"standard","item_category4":"bryzgalov_oleg_21st_century","item_category5":"not_balown","item_list_name":"search_results","item_name":"m63_star_streams_and_the_sunflower_galaxy_2016_digital_photo","item_variant":"undefined"},{"item_id":"PIX4620019","item_category2":"no_copyright","item_category3":"standard","item_category4":"r_gendler","item_category5":"not_balown","item_list_name":"search_results","item_name":"eagle_nebula_ic_4703_and_m16_star_cluster_in_the_snake_the_eagle_nebula_in_serpens_the_m16_star_clus","item_variant":"undefined"},{"item_id":"PIX4609334","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m33_infrared_view_spiral_galaxy_m33_seen_in_infrared_m33_ngc_598_the_galaxy_of_the_tri","item_variant":"undefined"},{"item_id":"PIX4613329","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":"PIX4609997","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_ngc_1964_in_the_constellation_lievre_spiral_galaxy_ngc_1964_in_lepus_the_galaxy_ngc_19","item_variant":"undefined"},{"item_id":"PIX4612348","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_of_hunting_dogs_m51_seen_in_x_the_whirlpool_galaxy_seen_in_x_ray_the_spiral_galaxy_m51_ngc_51","item_variant":"undefined"},{"item_id":"PIX4609481","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_ngc_891_in_andromede_edge_on_spiral_galaxy_ngc_891_in_andromeda_spiral_galaxy_seen_by_the_sli","item_variant":"undefined"},{"item_id":"PIX4609474","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_ngc_891_in_andromede_edge_on_spiral_galaxy_ngc_891_in_andromeda_spiral_galaxy_seen_by_the_sli","item_variant":"undefined"},{"item_id":"PIX4565139","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"globular_cluster_ngc_6934_globular_cluster_ngc_6934_ngc_6934_is_located_about_50_000_light_years_awa","item_variant":"undefined"}]}}

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

Erweiterte Suche Suchtipps

Bilder zu 'Distant Galaxies' gefunden, 148

«
1
2
3
»

Interacting galaxies NGC 6090 - Interacting galaxies NGC 6090 - The galaxy NGC 6090 is located about 400 million light years away from Earth in the constellation of the Dragon. This interacting galaxy consists of two spiral galaxies whose nuclei are distant from 10,000 light years. This system is halfway through its merger process. Image obtained by the Hubble Space Telescope on November 12, 2005. NGC 6090 is a beautiful pair of spiral galaxies with an overlapping central region and two long tidal tails formed from material ripped out of the galaxies by gravitational interaction. The two visible cores are approximately 10,000 light - years apart, suggesting that the two galaxies are at an intermediate stage in the merging process. The Hubble image reveals bright knots of newborn stars in the region where the two galaxies overlap. The right hand component has a clear spiral structure if viewed face - on, while the other is seen edge - on with no spiral arms visible. NGC 6090 is located

Interacting galaxies NGC 6090 - Interacting galaxies NGC 6090 - The galaxy NGC 6090 is located about 400 million light years away from Earth in the constellation of the Dragon. This interacting galaxy consists of two spiral galaxies whose nuclei are distant from 10,000 light years. This system is halfway through its merger process. Image obtained by the Hubble Space Telescope on November 12, 2005. NGC 6090 is a beautiful pair of spiral galaxies with an overlapping central region and two long tidal tails formed from material ripped out of the galaxies by gravitational interaction. The two visible cores are approximately 10,000 light - years apart, suggesting that the two galaxies are at an intermediate stage in the merging process. The Hubble image reveals bright knots of newborn stars in the region where the two galaxies overlap. The right hand component has a clear spiral structure if viewed face - on, while the other is seen edge - on with no spiral arms visible. NGC 6090 is located

PIX4612895

Galaxies NGC 3718 and NGC 3729 in Ursa Major

Galaxies NGC 3718 and NGC 3729 in Ursa Major

Adam Block

PIX4610936

This image shows one of the most distant galaxies known, called GN-108036, dating back to 750 million years after the Big Bang.

This image shows one of the most distant galaxies known, called GN-108036, dating back to 750 million years after the Big Bang.

UIG867353

Hubble ultra deep field view of galaxies, 2003-2004

Hubble ultra deep field view of galaxies, 2003-2004

UIS5104636

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Galaxies NGC 3718 and NGC 3729 in the Great Bear

Adam Block

PIX4611005

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - M105, NGC 3384 and NGC 3389 galaxies in Leo - These galaxies belong to the group of Leo 1 galaxies. Below is the elliptical galaxy M105, type E1, located about 40 million years ago - light from Earth; above, NGC 3384, at the top NGC 3389, a galaxy in the background. M105 (bottom) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 40 million light - years away. Also visble are galaxies NGC 3384 (above and right of center), which is part of the Leo I group, and NGC 3389 (top left), which is a more distant background galaxy

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - M105, NGC 3384 and NGC 3389 galaxies in Leo - These galaxies belong to the group of Leo 1 galaxies. Below is the elliptical galaxy M105, type E1, located about 40 million years ago - light from Earth; above, NGC 3384, at the top NGC 3389, a galaxy in the background. M105 (bottom) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 40 million light - years away. Also visble are galaxies NGC 3384 (above and right of center), which is part of the Leo I group, and NGC 3389 (top left), which is a more distant background galaxy

Vincent Toporenko

PIX4610687

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - Galaxies M105, NGC 3384 and NGC 3389 in Leo - These galaxies belong to the group of Leo 1 galaxies. On the right is the elliptical galaxy M105, type E1, located about 37 million years ago - light from the Earth; on its left, the galaxy NGC 3384, down, NGC 3389, a galaxy in the background. M105 (right) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 37 million light - years away. Also visble are galaxies NGC 3384 (left), which is part of the Leo I group, and NGC 3389 (bottom), which is a more distant background galaxy

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - Galaxies M105, NGC 3384 and NGC 3389 in Leo - These galaxies belong to the group of Leo 1 galaxies. On the right is the elliptical galaxy M105, type E1, located about 37 million years ago - light from the Earth; on its left, the galaxy NGC 3384, down, NGC 3389, a galaxy in the background. M105 (right) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 37 million light - years away. Also visble are galaxies NGC 3384 (left), which is part of the Leo I group, and NGC 3389 (bottom), which is a more distant background galaxy

R. Gendler

PIX4610710

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - Galaxies M105, NGC 3384 and NGC 3389 in Leo - These galaxies belong to the group of Leo 1 galaxies. Below is the elliptical galaxy M105, type E1, located about 40 million years ago - light from Earth; above, NGC 3384, at the top NGC 3389, a galaxy in the background. M105 (bottom) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 40 million light - years away. Also visble are galaxies NGC 3384 (above and right of center), which is part of the Leo I group, and NGC 3389 (top left), which is a more distant background galaxy

Galaxies M105, NGC 3384 and NGC 3389 in the Lion - Galaxies M105, NGC 3384 and NGC 3389 in Leo - These galaxies belong to the group of Leo 1 galaxies. Below is the elliptical galaxy M105, type E1, located about 40 million years ago - light from Earth; above, NGC 3384, at the top NGC 3389, a galaxy in the background. M105 (bottom) is a type E1 elliptical galaxy and the brightest member of the Leo I galaxy grouping. The entire group is about 40 million light - years away. Also visble are galaxies NGC 3384 (above and right of center), which is part of the Leo I group, and NGC 3389 (top left), which is a more distant background galaxy

Jim Misti

PIX4610701

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Nasa's Hubble Space Telescope shows a rare view of a pair of overlapping galaxies, called NGC 3314. The two galaxies look as if they are colliding, but they are actually separated by tens of millions of light - years, or about ten times the distance between our Milky Way and the neighboring Andromeda galaxy. The chance alignment of the two galaxies, as seen from Earth, gives a unique look at the silhouetted spiral arms in the closer face - on spiral, NGC 3314A. The motion of the two galaxies indicates that they are both relatively undisturbed and that they are moving in markedly different directions. The color composite was produced from exposures taken in blue and red light with Hubble's Advanced Camera for Surveys. The pair of gal

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Nasa's Hubble Space Telescope shows a rare view of a pair of overlapping galaxies, called NGC 3314. The two galaxies look as if they are colliding, but they are actually separated by tens of millions of light - years, or about ten times the distance between our Milky Way and the neighboring Andromeda galaxy. The chance alignment of the two galaxies, as seen from Earth, gives a unique look at the silhouetted spiral arms in the closer face - on spiral, NGC 3314A. The motion of the two galaxies indicates that they are both relatively undisturbed and that they are moving in markedly different directions. The color composite was produced from exposures taken in blue and red light with Hubble's Advanced Camera for Surveys. The pair of gal

PIX4610568

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355397

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355405

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355406

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355408

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355400

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355395

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355398

Ultraviolet view of the galaxies M81 and M82 - Ultraviolet image of M81 and M82 - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 10 - 12 million light years away from Earth. In ultraviolet, the Galex satellite highlights star-forming regions. Ultraviolet image of Messier 81 and Messier 82 (NGC 3031 and 3034), a pair of galaxies lying 10 million light - years distant. The stars in M81 spiral arms have formed within the last 100 million years, as have most of the stars in a nearby dwarf galaxy just to the left of M81. GALEX reveals that star formation is occurring quite distant from the nucleus of M81 in the faint blue extensions to the brighter spiral arms. The upper half of the full GALEX field of view shows the remarkable star forming galaxy M82

Ultraviolet view of the galaxies M81 and M82 - Ultraviolet image of M81 and M82 - M81 (left) is a spiral galaxy. M82 (right) an irregular galaxy. Separated for about 150,000 light years, these two galaxies belong to the galaxy cluster closest to our local group. These galaxies are approximately 10 - 12 million light years away from Earth. In ultraviolet, the Galex satellite highlights star-forming regions. Ultraviolet image of Messier 81 and Messier 82 (NGC 3031 and 3034), a pair of galaxies lying 10 million light - years distant. The stars in M81 spiral arms have formed within the last 100 million years, as have most of the stars in a nearby dwarf galaxy just to the left of M81. GALEX reveals that star formation is occurring quite distant from the nucleus of M81 in the faint blue extensions to the brighter spiral arms. The upper half of the full GALEX field of view shows the remarkable star forming galaxy M82

PIX4610320

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355396

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355401

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355403

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355394

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355399

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355402

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355404

François Hammer, 2021 (photo)

François Hammer, 2021 (photo)

Francois Palluau

FPA7355407

Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred s

Barree spiral galaxy NGC 1483 in Dorado - Barred spiral galaxy NGC 1483 in Dorado - NGC 1483 is a barree spiral galaxy located about 60 million years ago - light in the southern constellation of Dorado. Image obtained by the Hubble Space Telescope (HST). NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star - forming regions. In the background, many other distant galaxies can be seen. The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprising an estimated 70 galaxies and located some 62 million light - years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the Universe to be held together by their gravity. Barred s

PIX4609879

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image obtained with a 50 cm telescope, composite of several poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 95 million ligh

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image obtained with a 50 cm telescope, composite of several poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 95 million ligh

R. Jay GaBany

PIX4612130

Interacting galaxies NGC 6786 and LEDA 62867 - Interacting galaxies NGC 6786 and LEDA 62867 - The galaxy NGC 6786, on the right, is about 350 million years away - light from Earth in the constellation of the Dragon. It interacts with another spiral galaxy, LEDA 62867, on the left; it will probably swallow it in the distant future. Image obtained by the Hubble Space Telescope on March 10, 2002. This Hubble image displays a beautiful pair of interacting spiral galaxies with swirling arms. The smaller of the two, dubbed LEDA 62867 and positioned to the left of the frame, seems to be safe for now, but will probably be swallowed by the larger spiral galaxy, NGC 6786 (to the right) eventually. There is already some disturbance visible in both components. The pair is number 538 in Karachentsev's Catalog of Pairs of Galaxies. A supernova was seen to explode in the large spiral in 2004. NGC 6786 is located in the constellation of Draco, the Dragon, about 350 million light - years away. Image ta

Interacting galaxies NGC 6786 and LEDA 62867 - Interacting galaxies NGC 6786 and LEDA 62867 - The galaxy NGC 6786, on the right, is about 350 million years away - light from Earth in the constellation of the Dragon. It interacts with another spiral galaxy, LEDA 62867, on the left; it will probably swallow it in the distant future. Image obtained by the Hubble Space Telescope on March 10, 2002. This Hubble image displays a beautiful pair of interacting spiral galaxies with swirling arms. The smaller of the two, dubbed LEDA 62867 and positioned to the left of the frame, seems to be safe for now, but will probably be swallowed by the larger spiral galaxy, NGC 6786 (to the right) eventually. There is already some disturbance visible in both components. The pair is number 538 in Karachentsev's Catalog of Pairs of Galaxies. A supernova was seen to explode in the large spiral in 2004. NGC 6786 is located in the constellation of Draco, the Dragon, about 350 million light - years away. Image ta

PIX4613003

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, on its left, is probably interacting with it. Image obtained with a 35 cm telescope, 6 hours of poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The galaxies are about 95 million light years distant. Image taken with 14.5”” RCOS telescope, 6 Hours of exposure

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, on its left, is probably interacting with it. Image obtained with a 35 cm telescope, 6 hours of poses. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The galaxies are about 95 million light years distant. Image taken with 14.5”” RCOS telescope, 6 Hours of exposure

R. Gendler

PIX4612142

Interacting galaxies NGC 3256 - Interacting galaxies NGC 3256 - The special galaxy NGC 3256 is located about 100 million light years away from Earth in the southern constellation of Sails. A vestige of the collision of two galaxies, this system presents a double nucleus and many young clusters of stars. Image obtained by the Hubble Space Telescope on November 5, 2001. NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra - Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters. Image taken by the Hubble space telescope on November 5

Interacting galaxies NGC 3256 - Interacting galaxies NGC 3256 - The special galaxy NGC 3256 is located about 100 million light years away from Earth in the southern constellation of Sails. A vestige of the collision of two galaxies, this system presents a double nucleus and many young clusters of stars. Image obtained by the Hubble Space Telescope on November 5, 2001. NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra - Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters. Image taken by the Hubble space telescope on November 5

PIX4610539

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

Galaxies NGC 3718 and NGC 3729 in the Great Bear - Galaxies NGC 3718 and NGC 3729 in Ursa Major - NGC 3718 is a special galaxy located about 42 million years ago - light from Earth in the constellation of the Great Bear. It's an active nucleus galaxy. Its tormented shape is probably due to the attraction exerted by another galaxy, NGC 3729, visible to its left. To the south, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million light years away from Earth. NGC 3718 and its companion NGC 3729 (left) are physically related members of the Ursa Major galaxy cluster. The two galaxies appear to orbit each other at a projected separation of 147,000 light years. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is

R. Gendler

PIX4610948

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) on the left and M110 (NGC 205) (off-field). Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. The several distinct stars that surround Andromeda's image are actually stars in our Galaxy that are well in front of the background object. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei

Center of the Andromede Galaxy (M31) - Center of the Andromeda galaxy - The Andromede galaxy is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) on the left and M110 (NGC 205) (off-field). Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. The diffuse light from Andromeda is caused by the hundreds of billions of stars that compose it. The several distinct stars that surround Andromeda's image are actually stars in our Galaxy that are well in front of the background object. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei

R. Gendler

PIX4608837

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image made with Siding Spring's 3.9m telescope. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 80 million light years distant

Galaxies NGC 5078 and IC 879 in Hydra - Galaxies NGC 5078 and IC 879 in Hydra - NGC 5078 is a spiral galaxy located about 95 million years ago - light. A small galaxy, IC 879, at the bottom of the picture, is probably interacting with it. Image made with Siding Spring's 3.9m telescope. NGC 5078 is a lenticular (lens - shaped) galaxy crossed by a distinct dusty band which is seen against the bright background of the galaxy itself. The dust lane is warped and broadened, probably by interaction with the faint companion galaxy IC 879, which is itself distorted into an 'S' shape by the interaction. The slightly bluish colour of parts of the fainter galaxy is suggestive of star formation, probably triggered by the interaction. Encounters between galaxies such as this are common, and often lead to them merging into a single entity. It is likely that the dust lane of NGC 5078 is the remnant of a dusty spiral which fell into it long ago. The galaxies are about 80 million light years distant

PIX4612223

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

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

PIX4609816

Core of the Andromede Galaxy (M31) - The Andromede Galaxy is located about 2 million years away - light from Earth. View of its dual nucleus obtained by the Hubble Space Telescope (HST). Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei. Image taken with the Hubble space telescope (HST)

Core of the Andromede Galaxy (M31) - The Andromede Galaxy is located about 2 million years away - light from Earth. View of its dual nucleus obtained by the Hubble Space Telescope (HST). Andromeda is the nearest major galaxy to our own Milky Way Galaxy. Our Galaxy is thought to look much like Andromeda. Together these two galaxies dominate the Local Group of galaxies. M31 is so distant it takes about two million years for light to reach us from there. Much about M31 remains unknown, including how the center acquired two nuclei. Image taken with the Hubble space telescope (HST)

R. Gendler

PIX4608904

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum. <BR>The common feature of these galaxy types is a small, very bright nucleus thought to host

Spiral galaxy M77 in the Whale - Active galaxy M77 (NGC 1068) in Cetus - M77 (NGC 1068). This active galaxy is the typical example of a Seyfert II galaxy. It has an active core and houses a massive black hole. She is the object of intense star formation in her spiral arms. NGC 1068 is around 50 million years of light from Earth. Image obtained by Siding Spring's 3.9m telescope. M77 is a Seyfert galaxy, a class of galaxy named for Karl Seyfert who first identified galaxies with emission lines superimposed on the normal radiation from their nuclei in 1943. Such galaxies are a subset of an ill - defined species generally known as 'active galaxies' whose nuclei emit radio - and X - radiation as well as visible light. The least active of the active galaxies are the Seyferts, the most active are the quasars which are mostly so distant that they can only be distinguished from stars by their spectrum. <BR>The common feature of these galaxy types is a small, very bright nucleus thought to host

PIX4609570

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Galaxies NGC 3718 in the Great Bear - Galaxy NGC 3718 in Ursa Major - NGC 3718 (Arp 214) is a special galaxy located about 42 million years ago - light from the Earth in the constellation Big Bear. It's an active nucleus galaxy. Its tormented form is probably due to the attraction exerted by another galaxy, NGC 3729 (off-field). On the right, Arp 322 (or Hickson 56), is a group of 5 galaxies far farther away, located about 300 million years from Earth. NGC 3718 (Arp 214) seems to have a rudimentary bar and spiral structure although it is recognized as a peculiar galaxy and as such is listed within ARP's Atlas of Peculiar Galaxies. NGC 3718 contains an active galactic nucleus (AGN) and is known as a Seyfert type 1.9 galaxy. Its strange shape is probably due to a gravitational interaction with its companion NGC 3729 (out of field). A grouping of 5 background galaxies 300 million light years distant are projected at right of NGC 3718 and are designated Arp 322 (also Hickson 56). Several m

Jim Misti

PIX4610955

Large and Small Magellan Clouds - Large and Small Magellanic clouds - These two irregular galaxies are close to our galaxy. Visible in the southern hemisphere, they are located approximately 160,000 (Grand Cloud, right) and 240,000 light years (Small Cloud, left). The Magellanic Clouds are the nearest galaxies to the Milky Way, about 170,000 and 240,000 light years distant respectively. They are in the far southern sky, practically invisible from northern latitudes, and their low surface brightness makes them difficult to see unless they are high in the sky. Both Magellanic Clouds are less than 25 degrees from the South Celestial Pole and are visible at some time on any clear, dark night from Siding Spring, where this picture was taken. To the dark adapted eye the Magellanic Clouds look like detached pieces of the Milky Way, but this apparent detachment is misleading because both are in orbit around it. Although the Magellanic Clouds are separate galaxies they are interacting with each

Large and Small Magellan Clouds - Large and Small Magellanic clouds - These two irregular galaxies are close to our galaxy. Visible in the southern hemisphere, they are located approximately 160,000 (Grand Cloud, right) and 240,000 light years (Small Cloud, left). The Magellanic Clouds are the nearest galaxies to the Milky Way, about 170,000 and 240,000 light years distant respectively. They are in the far southern sky, practically invisible from northern latitudes, and their low surface brightness makes them difficult to see unless they are high in the sky. Both Magellanic Clouds are less than 25 degrees from the South Celestial Pole and are visible at some time on any clear, dark night from Siding Spring, where this picture was taken. To the dark adapted eye the Magellanic Clouds look like detached pieces of the Milky Way, but this apparent detachment is misleading because both are in orbit around it. Although the Magellanic Clouds are separate galaxies they are interacting with each

PIX4613338

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. 47 Tuc is about 15,000 light years distant and contains several million stars, as many as some minor galaxies

D. De Martin

PIX4564299

Mystery blobs in space, c 2006

Mystery blobs in space, c 2006

UIS5104199

Spiral galaxy NGC 1309 in Eridan - Spiral galaxy NGC 1309 in Eridanus - Located about 100 million years ago - light from Earth, NGC 1309 extends over 30,000 years - light in the constellation Eridan. A supernova and a few cepheides have been observed in this galaxy. Many galaxies are visible in the background. The image was taken in 2005 by the Hubble space Telescope. NGC 1309 is 100 million light - years (30 Megaparsecs) distant

Spiral galaxy NGC 1309 in Eridan - Spiral galaxy NGC 1309 in Eridanus - Located about 100 million years ago - light from Earth, NGC 1309 extends over 30,000 years - light in the constellation Eridan. A supernova and a few cepheides have been observed in this galaxy. Many galaxies are visible in the background. The image was taken in 2005 by the Hubble space Telescope. NGC 1309 is 100 million light - years (30 Megaparsecs) distant

PIX4609750

Star Formation Region LH 95 in the Great Magellan Cloud - NASA/ESA/Hubble Heritage team/Novapix - LH 95 is a star-forming region located in the galaxy of the Great Magellan Cloud at 160,000 years - light from Earth. Blue giant stars, two to three solar masses cohabit with barely formed stars. In the background, some more distant galaxies are visible. Image obtained from the ACS camera of the Hubble Space Telescope in 2006

Star Formation Region LH 95 in the Great Magellan Cloud - NASA/ESA/Hubble Heritage team/Novapix - LH 95 is a star-forming region located in the galaxy of the Great Magellan Cloud at 160,000 years - light from Earth. Blue giant stars, two to three solar masses cohabit with barely formed stars. In the background, some more distant galaxies are visible. Image obtained from the ACS camera of the Hubble Space Telescope in 2006

PIX4620946

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

PIX4610557

Spiral Galaxy M51 in Hunting Dogs - Spiral galaxy M51 in Canes Venatici - The spiral galaxy M51 (NGC 5194) is located about 37 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. Another galaxy far more distant appears at the bottom left of the image. M51 (NGC 5194) is about 37 Mly from Earth and is interacting with its dwarf galaxy companion (NGC 5195)

Spiral Galaxy M51 in Hunting Dogs - Spiral galaxy M51 in Canes Venatici - The spiral galaxy M51 (NGC 5194) is located about 37 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. Another galaxy far more distant appears at the bottom left of the image. M51 (NGC 5194) is about 37 Mly from Earth and is interacting with its dwarf galaxy companion (NGC 5195)

E Mouquet

PIX4612306

First image of the JWST - SMACS galaxy cluster 0723, 2022 (photography)

First image of the JWST - SMACS galaxy cluster 0723, 2022 (photography)

PIX7331184

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

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

PIX4613035

Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

Barree spiral galaxy NGC 1300 in Eridan - NGC 1300, barred spiral galaxy in Eridanus - The galaxy NGC 1300 is located about 60 million years ago - light and extends over about 85 000 years - light. Spiral galaxies appear in a variety of guises, but none are more intriguing than the barred variety. As their name suggests, these galaxies are distinguished by a bar, extending (in this case) like two more of less straight assemblies of stars either side of the bright nucleus. Caught up in the bar are two dust lanes, emerging on either side of the nuclear mass. At some distance from the nucleus, the straight, almost structurreless bar and dust lanes abruptly turn at a sharp angle. It is here that the delicately curved arms of the spiral begin, and it is here that star formation is at its most concentrated. Many spirals have such bars, including the Milky Way, where it is a subtle feature, very difficult to detect. NGC 1300, in the southern constellation of Eridanus is among the finest examp

PIX4609731

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. Image obtained with a 35 cm telescope, 8h of poses. 47 Tuc is about 15,000 light years distant in southern hemisphere and contains several million stars, as many as some minor galaxies. Image taken with 14.5”” RCOS telescope, 8 hours of exposure

Globular cluster 47 Toucan - The globular cluster 47 Tucanae NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. Image obtained with a 35 cm telescope, 8h of poses. 47 Tuc is about 15,000 light years distant in southern hemisphere and contains several million stars, as many as some minor galaxies. Image taken with 14.5”” RCOS telescope, 8 hours of exposure

R. Gendler

PIX4564305

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies

Galaxy NGC 4027 in the Raven - Galaxy NGC 4027 in Corvus - NGC 4027 is a spiral galaxy located about 80 million years ago - light. The photo shows some nearby dwarf galaxies. Image made with Siding Spring's 3.9m telescope. This galaxy is of interest because of its similarity to the Large Magellanic Cloud, (LMC) our nearest extra - galactic neighbour. Like the LMC, its light comes predominantly from young stars, which are hotter than the Sun and give the galaxy a bluish colour. However, because this galaxy is over 80 million light - years distant we see only the integrated light of millions of unresolved stars, rather than the individuals we see in the LMC. NGC 4027 has a somewhat distorted appearance and an elongated spiral arm, probably due to the gravitational effect of a smaller companion galaxy, not visible in this photograph but rather obvious on a much deeper image. NGC 4027 is less than half a degree south of the Antennae interacting galaxies

PIX4611058

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

Barree spiral galaxy NGC 1300 in Eridan - Barred spiral galaxy NGC 1300 in Eridanus - The galaxy NGC1300 is located about 60 million years ago - light and extends over about 85 000 years - light. This image was obtained by the Hubble Space Telescope in September 2004. NGC 1300 is considered to be prototypical of barred spiral galaxies. Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral all the way into the center, but are connected to the two ends of a straight bar of stars containing the nucleus at its center. At Hubble's resolution, a myriad of fine details, some of which have never before been seen, is seen throughout the galaxy's arms, disk, bulge, and nucleus. Blue and red supergiant stars, star clusters, and star - forming regions are well resolved across the spiral arms, and dust lanes trace out fine structures in the disk and bar. Numerous more distant galaxies are visible in the background, and are seen even through the densest regio

PIX4609752

The constellation Leo, 1603

The constellation Leo, 1603

UIS5090990

M63: Star Streams and the Sunflower Galaxy, 2016 (digital photo)

M63: Star Streams and the Sunflower Galaxy, 2016 (digital photo)

Bryzgalov, Oleg (21st century)

MMM7341114

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - The Eagle nebula in Serpens - The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant

R. Gendler

PIX4620019

Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

Spiral galaxy M33 infrared view - Spiral galaxy M33 seen in infrared - M33, (NGC 598), the galaxy of the Triangle, is located about 2.9 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. This infrared image from the Spitzer space telescope shows stars in blue, gas in green, star formations in red - orange. Red dots are distant galaxies. In infrared, the galaxy appears larger than visible light, revealing cold gas and dust that spread around the galaxy. Also known as M33 or NGC 598, the Triangulum Galaxy is part of the Local Group of galaxies, which includes the Andromeda Galaxy (M31) and our galaxy, the Milky Way. M33 is over thirty thousand light - years across, and more than two million light - years away. Viewed here with Spitzer's infrared eyes, this elegant spiral galaxy sparkles with color and detail. Stars appear as glistening blue gems (several of which are actually foreground stars in our own galaxy), while dust rich

PIX4609334

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. Two globular clusters are visible on this image, on the right the Toucan cluster, on the left, the NGC 362 cluster. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at left is NGC 362. It is about 30,000 light years distant, twice as far away as 47 Tuc

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. Two globular clusters are visible on this image, on the right the Toucan cluster, on the left, the NGC 362 cluster. The Small Magellanic Cloud (SMC) is the second nearest galaxy to the Milky Way, (the LMC being the nearest) and is at the distance of about 240,000 light years. The shape of the SMC defies description and it is therefore classified as an 'irregular' galaxy. The large globular cluster at right is 47 Tucanae, while a smaller one at left is NGC 362. It is about 30,000 light years distant, twice as far away as 47 Tuc

PIX4613329

Spiral galaxy NGC 1964 in the constellation Lievre - Spiral galaxy NGC 1964 in Lepus: The galaxy NGC 1964 is located about 70 million light years away from Earth. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This spectacular spiral galaxy, known as NGC 1964, resides approximately 70 million light-years away in the constellation of Lepus (The Hare). NGC 1964 has a bright and dense core. In addition to containing stars, NGC 1964 lives in a star-sprinkled section of the sky. In this view from the Wide Field Imager (WFI) - an instrument mounted on the MPG/ESO 2.2-metre telescope at Eso's La Silla Observatory, Chile - the star HD 36785 can be seen to the galaxy's immediate right. Above it reside two other prominent stars named HD 36784 and TYC 5928-368-1 - and the large bright star below NGC 1964 is known as BD-22 1147. This view of NGC 1964 also contains an array of galaxies, visible in the background. The WFI is able to observe the light from these distan

Spiral galaxy NGC 1964 in the constellation Lievre - Spiral galaxy NGC 1964 in Lepus: The galaxy NGC 1964 is located about 70 million light years away from Earth. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. This spectacular spiral galaxy, known as NGC 1964, resides approximately 70 million light-years away in the constellation of Lepus (The Hare). NGC 1964 has a bright and dense core. In addition to containing stars, NGC 1964 lives in a star-sprinkled section of the sky. In this view from the Wide Field Imager (WFI) - an instrument mounted on the MPG/ESO 2.2-metre telescope at Eso's La Silla Observatory, Chile - the star HD 36785 can be seen to the galaxy's immediate right. Above it reside two other prominent stars named HD 36784 and TYC 5928-368-1 - and the large bright star below NGC 1964 is known as BD-22 1147. This view of NGC 1964 also contains an array of galaxies, visible in the background. The WFI is able to observe the light from these distan

PIX4609997

Galaxy of Hunting Dogs (M51) seen in X - The Whirlpool Galaxy seen in X - ray - The spiral galaxy M51 (NGC 5194) is located about 31 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. X-ray image obtained by the Chandra space telescope on June 20, 2000. The Whirlpool Galaxy lies approximately 31 million light years from earth. This spectacular galaxy is paired with a smaller, more distant companion whose matter is being disrupted by the larger spiral in a gravitational tug of war. Eventually, the shape of both will be altered over many more millions of years. Image taken in X - ray by the Chandra space telescope on June 20, 2000

Galaxy of Hunting Dogs (M51) seen in X - The Whirlpool Galaxy seen in X - ray - The spiral galaxy M51 (NGC 5194) is located about 31 million years ago - light from Earth. This galaxy is double; two galaxies interact: the largest, NGC 5194, the smallest NGC 5195. X-ray image obtained by the Chandra space telescope on June 20, 2000. The Whirlpool Galaxy lies approximately 31 million light years from earth. This spectacular galaxy is paired with a smaller, more distant companion whose matter is being disrupted by the larger spiral in a gravitational tug of war. Eventually, the shape of both will be altered over many more millions of years. Image taken in X - ray by the Chandra space telescope on June 20, 2000

PIX4612348

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light.. This image obtained with the 2.5m Isaac Newton telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. However,

PIX4609481

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

Galaxy NGC 891 in Andromede - Edge - on spiral galaxy NGC 891 in Andromeda - Spiral galaxy seen by the slice located at a distance of 10 million years - light. This image was obtained with the Isaac Newton 2.5m telescope of La Palma. If we could view the Milky Way from a distance of about 30 million light years it would look something like NGC 891. But galaxies that look like this are quite rare because the chance alignment of the thin disk of a spiral galaxy with our line of sight is unusual. A few degrees either side of its orientation and NGC 891 would be just another highly inclined spiral galaxy. From this unusual vantage point we can see in NGC 891 the surprising narrowness of the obscuring dust lane, a dark, slightly irregular band across the galaxy. We also see that it is yellowish, confirming that it is dust, which absorbs blue light, as in the Milky Way. Also similar to the Milky Way is the prominent central 'bulge' corresponding to the rich star clouds in Sagittarius. Howeve

PIX4609474

Globular cluster NGC 6934 - Globular Cluster NGC 6934 - NGC 6934 is located about 50,000 light years away from Earth in the constellation Dolphin. Image obtained by the Hubble Space Telescope (HST). This bright spray of stars in the small constellation of Delphinus (the Dolphin) is the globular cluster NGC 6934. Globular clusters are large balls of (typically) a few hundred thousand ancient stars that exist on the edges of galaxies. Lying 50 000 light - years from Earth, in the outer reaches of our Milky Way galaxy, NGC 6934 is home to some of the most distant stars still to be part of our galactic system - - in a sense, it is a far - flung suburb to the Milky Way's city centre. This picture was taken with the Wide Field Channel of the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys

Globular cluster NGC 6934 - Globular Cluster NGC 6934 - NGC 6934 is located about 50,000 light years away from Earth in the constellation Dolphin. Image obtained by the Hubble Space Telescope (HST). This bright spray of stars in the small constellation of Delphinus (the Dolphin) is the globular cluster NGC 6934. Globular clusters are large balls of (typically) a few hundred thousand ancient stars that exist on the edges of galaxies. Lying 50 000 light - years from Earth, in the outer reaches of our Milky Way galaxy, NGC 6934 is home to some of the most distant stars still to be part of our galactic system - - in a sense, it is a far - flung suburb to the Milky Way's city centre. This picture was taken with the Wide Field Channel of the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys

PIX4565139

«
1
2
3
»

Warum Bridgeman Images?

Kunst. Kultur. Geschichte.

Wir arbeiten mit den weltweit führenden Museen, Galerien und Künstlern zusammen, so dass Sie Zugang zu qualitativ hochwertigem Bildmaterial haben.

Entdecken Sie unsere Kollektion FAQs durchsuchen

Einfach. Schnell. Zuverlässig.

Unsere Teams helfen Ihnen bei der Suche nach den perfekten Inhalten und kümmern sich um alle urheberrechtlichen und lizenzrechtlichen Anforderungen.

Kontaktieren Sie uns

Entdecken Sie Millionen von Bildern und Clips für Ihre kreativen Projekte.

Starten Sie Ihre Suche

© Copyright 2024 Bridgeman Art Library Limited. Registriert in England und Wales unter der Firmennummer 01056394.