Type # for projects,to access projects, > for users, and ? for help.
Reverse Image
Lightboxes
[]
Your ongoing selection
Asset(s) Assets
Your quote 0

Your selection

Clear selection
Request a quote now

Leave the work to our dedicated Account Managers.

{"event":"pageview","page_type1":"undetected","page_type2":"_assets_search_override","language":"en","user_logged":"false","user_type":"ecommerce","nl_subscriber":"false"}
{"event":"ecommerce_event","event_name":"view_item","event_category":"browse_catalog","ecommerce":{"items":[{"item_id":"UIG2912228","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"planet_xena","item_variant":"undefined"},{"item_id":"PIX4572188","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cepheide_rs_puppis_cepheides_are_very_bright_variable_stars_that_serve_as_cosmic_beacons_to_measure_","item_variant":"undefined"},{"item_id":"UIG534561","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope_nasa_photograph","item_variant":"undefined"},{"item_id":"UIG1580022","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"butterfly_shape_emerges_from_stellar_demise_in_planetary_nebula_ngc_6302_2009","item_variant":"undefined"},{"item_id":"UIG532201","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope_above_the_earth_nasa_photograph","item_variant":"undefined"},{"item_id":"UIG867040","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_ant_nebula_whose_technical_name_is_mz3_located_between_3_000_and_6_000_light_years_from_earth_in","item_variant":"undefined"},{"item_id":"UIG867032","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"six_hundred_and_fifty_light_years_away_in_the_constellation_aquarius_a_dead_star_about_the_size_of_e","item_variant":"undefined"},{"item_id":"UIG867033","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"six_hundred_and_fifty_light_years_away_in_the_constellation_aquarius_a_dead_star_about_the_size_of_e","item_variant":"undefined"},{"item_id":"PIX4571310","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_ison_comete_05_2013_the_ison_comet_seen_on_may_8_2013_by_the_hubble_space_telescope_hst_hubble_s","item_variant":"undefined"},{"item_id":"UIG867137","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_central_region_of_our_milky_way_galaxy_hubble_spitzer_and_chandra","item_variant":"undefined"},{"item_id":"UIG867138","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_central_region_of_our_milky_way_galaxy_hubble_spitzer_and_chandra","item_variant":"undefined"},{"item_id":"UIG532091","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope_launch","item_variant":"undefined"},{"item_id":"UIG867139","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_central_region_of_our_milky_way_galaxy_hubble_spitzer_and_chandra","item_variant":"undefined"},{"item_id":"UIG867136","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_central_region_of_our_milky_way_galaxy_hubble_spitzer_and_chandra","item_variant":"undefined"},{"item_id":"UIG532087","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope","item_variant":"undefined"},{"item_id":"UIG867135","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_central_region_of_our_milky_way_galaxy_hubble_spitzer_and_chandra","item_variant":"undefined"},{"item_id":"PIX4571322","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_ison_comete_10_2013_the_ison_comet_seen_on_october_9_2013_by_the_hubble_space_telescope_hst_hubb","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":"UIG867037","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"galaxy_ngc_3079_located_50_million_light_years_from_earth_in_the_constellation_ursa_major_has_a_huge","item_variant":"undefined"},{"item_id":"PIX4569558","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_comet_shoemaker_levy_9_01_1994_shoemaker_levy_9_comet_01_1994_the_comet_shoemaker_levy_9_seen_in","item_variant":"undefined"},{"item_id":"UIG529096","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"a_recent_hubble_space_telescope_hst_view_reveals_uranus_surrounded_by_its_4_major_rings_and_10_of_it","item_variant":"undefined"},{"item_id":"UIG529159","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope_the_tenth_planet_currently_nicknamed_xena_and_found_that_it_s_only_slightly_l","item_variant":"undefined"},{"item_id":"PIX4612901","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_6217_barred_galaxy_ngc_6217_the_barree_spiral_galaxy_ngc_6217_is_located_60","item_variant":"undefined"},{"item_id":"UIG528807","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"spiral_galaxy_m81_viewed_from_the_hubble_space_telescope_credit_nasa_science_astronomy_stellar","item_variant":"undefined"},{"item_id":"UIG867098","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_spiral_galaxy_known_as_messier_81_or_m81_galex_orbiter_hubble_space_telescope_spitzer_space_tele","item_variant":"undefined"},{"item_id":"UIG867124","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_spiral_galaxy_messier_101_from_composite_of_views_from_spitzer_hubble_and_chandra","item_variant":"undefined"},{"item_id":"UIG867029","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_many_sides_of_the_supernova_remnant_cassiopeia_a_located_10_000_light_years_away_in_the_northern","item_variant":"undefined"},{"item_id":"UIG867097","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_spiral_galaxy_known_as_messier_81_or_m81_galex_orbiter_hubble_space_telescope_spitzer_space_tele","item_variant":"undefined"},{"item_id":"PIX4610088","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_2442_in_flying_fish_barred_spiral_galaxy_ngc_2442_in_volans_ngc_2442_is_a_b","item_variant":"undefined"},{"item_id":"PIX5940218","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"saturn_planet_hubble_space_telescope_on_june_20_2019","item_variant":"undefined"},{"item_id":"UIG867028","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_many_sides_of_the_supernova_remnant_cassiopeia_a_located_10_000_light_years_away_in_the_northern","item_variant":"undefined"},{"item_id":"UIG2911252","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"pluto","item_variant":"undefined"},{"item_id":"UIG867075","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_supernova_remnant_1e0102_2_7219_sits_next_to_the_nebula_n76_in_a_bright_star_forming_region_of_t","item_variant":"undefined"},{"item_id":"UIG867026","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_many_sides_of_the_supernova_remnant_cassiopeia_a_located_10_000_light_years_away_in_the_northern","item_variant":"undefined"},{"item_id":"UIG528801","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"bright_spiral_galaxy_m81_viewed_from_the_hubble_telescope_credit_nasa_science_astronomy_stellar_spac","item_variant":"undefined"},{"item_id":"UIG2911253","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"pluto","item_variant":"undefined"},{"item_id":"UIG867074","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_supernova_remnant_1e0102_2_7219_sits_next_to_the_nebula_n76_in_a_bright_star_forming_region_of_t","item_variant":"undefined"},{"item_id":"UIG532089","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_space_telescope_repair","item_variant":"undefined"},{"item_id":"PIX4583130","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"visible_crab_nebula_infrared_and_x_the_crab_nebula_m1_the_crab_nebula_is_the_rest_of_a_supernova_tha","item_variant":"undefined"},{"item_id":"UIG867072","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"ngc_2207_and_ic_2163_met_and_began_a_sort_of_gravitational_tango_about_40_million_years_ago_the_two_","item_variant":"undefined"},{"item_id":"UIG531595","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"image_of_mars_from_hubble_space_telescope","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":"PIX4569561","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_comet_shoemaker_levy_9_01_1994_shoemaker_levy_9_comet_01_1994_the_comet_shoemaker_levy_9_seen_in","item_variant":"undefined"},{"item_id":"PIX4626476","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"kepler_is_the_rest_of_a_supernova_that_exploded_about_400_years_ago_located_about_13_000_light_years","item_variant":"undefined"},{"item_id":"PIX4611731","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_4639_in_virgo_barred_galaxy_ngc_4639_in_virgo_the_barree_spiral_galaxy_ngc_","item_variant":"undefined"},{"item_id":"UIG867073","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"ngc_2207_and_ic_2163_met_and_began_a_sort_of_gravitational_tango_about_40_million_years_ago_the_two_","item_variant":"undefined"},{"item_id":"UIG867038","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_horsehead_also_known_as_barnard_33_is_a_cold_dark_cloud_of_gas_and_dust_silhouetted_against_the_","item_variant":"undefined"},{"item_id":"PIX4611257","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_4319_and_markarian_quasar_205_galaxy_ngc_4319_and_quasar_markarian_205_the_","item_variant":"undefined"},{"item_id":"PIX4568849","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cloud_ic_349_illuminates_by_the_star_merope_barnard_s_merope_nebula_ic_349_ic_349_is_an_interstellar","item_variant":"undefined"},{"item_id":"PIX4572025","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"polaris_system_polaris_is_a_triple_system_consisting_of_a_supergiant_star_and_two_dwarf_stars_it_is_","item_variant":"undefined"},{"item_id":"PIX4611351","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"barree_spiral_galaxy_ngc_4394_in_berenice_s_hair_barred_spiral_galaxy_ngc_4394_in_coma_berenices_ngc","item_variant":"undefined"},{"item_id":"UIG867039","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_horsehead_also_known_as_barnard_33_is_a_cold_dark_cloud_of_gas_and_dust_silhouetted_against_the_","item_variant":"undefined"},{"item_id":"PIX4613806","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"hubble_deep_field_sud_hubble_deep_field_south_in_the_southern_constellation_of_toucan_the_hubble_spa","item_variant":"undefined"},{"item_id":"PIX4572282","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_v838_monocerotis_28_10_2004_v838_monocerotis_10_2004_this_variable_star_is_located_approximatel","item_variant":"undefined"},{"item_id":"PIX4572319","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_v838_monocerotis_09_2006_v838_monocerotis_seen_by_the_hubble_space_telescope_09_2006_this_varia","item_variant":"undefined"},{"item_id":"UIG867082","item_category2":"undetermined_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_eagle_nebula_an_industrious_star_making_factory_located_7_000_light_years_away_in_the_serpens_co","item_variant":"undefined"},{"item_id":"UDK844647","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"the_hubble_space_telescope","item_variant":"undefined"},{"item_id":"PIX4572295","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_v838_monocerotis_11_2005_star_v838_monocerotis_seen_by_the_hubble_space_telescope_11_2005_this_","item_variant":"undefined"},{"item_id":"PIX4572157","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"cepheides_in_the_galaxy_m81_cepheids_in_the_galaxy_m81_cepheides_are_very_bright_variable_stars_that","item_variant":"undefined"},{"item_id":"PIX4572231","item_category2":"no_copyright","item_category3":"standard","item_category5":"not_balown","item_list_name":"search_results","item_name":"star_field_in_the_constellation_sagittarius_starfield_in_sagittarius_stars_in_sagittarius_towards_th","item_variant":"undefined"}]}}
{"event":"custom_event","event_name":"view_search_result","event_category":"browse_catalog","keyword":"hubble telescope","search_type":"standard","search_bridgeman_artists":"false","search_mode":"automatic","search_zero_result":"false","search_results":984,"search_results_page_number":1}

'Hubble Telescope' images and/or videos results

Main filters
Buy Print option
Royalty-Free Option
Reuters Results
Media Type
Orientation
Colour
Rights Type
Rights
More filters
Bridgeman Artists
Bridgeman Photographers
Century
Footage filters
Video Original Format
Video Resolution
Video Category
Filter group
Order By:
per page
Filter group
Rights Type
Media Type
No copyright

Display options

View
Image Size

Images of 'Hubble Telescope' found, 984

 
Planet Xena

UIG2912228

Planet Xena

UIG2912228

 
Cepheide RS Puppis - Cepheides are very bright variable stars that serve as cosmic beacons to measure the distance of nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope photographed one of the brightest cepheids, RS Puppis (in the center of the image), located 6500 years - light in the southern constellation of the Puppi. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our Sun and 200 times larger. RS Puppis rhythmically brightens and dims over a six - week cycle. It is one of the most luminous in the class of so - called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our Sun's luminosity. The nebula flickers in brightness a

PIX4572188

Cepheide RS Puppis - Cepheides are very bright variable stars that serve as cosmic beacons to measure the distance of nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope photographed one of the brightest cepheids, RS Puppis (in the center of the image), located 6500 years - light in the southern constellation of the Puppi. The bright southern hemisphere star RS Puppis, at the center of the image, is swaddled in a gossamer cocoon of reflective dust illuminated by the glittering star. The super star is ten times more massive than our Sun and 200 times larger. RS Puppis rhythmically brightens and dims over a six - week cycle. It is one of the most luminous in the class of so - called Cepheid variable stars. Its average intrinsic brightness is 15,000 times greater than our Sun's luminosity. The nebula flickers in brightness a

PIX4572188

 
Hubble Space Telescope. NASA photograph.

UIG534561

Hubble Space Telescope. NASA photograph.

UIG534561

 
Butterfly shape emerges from Stellar Demise in Planetary Nebula NGC 6302, 2009

UIG1580022

Butterfly shape emerges from Stellar Demise in Planetary Nebula NGC 6302, 2009

UIG1580022

 
Hubble Space Telescope above the Earth. NASA photograph.

UIG532201

Hubble Space Telescope above the Earth. NASA photograph.

UIG532201

 
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867137

The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867137

 
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867138

The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867138

 
Hubble Space Telescope Launch

UIG532091

Hubble Space Telescope Launch

UIG532091

 
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867139

The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867139

 
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867136

The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867136

 
Hubble Space Telescope

UIG532087

Hubble Space Telescope

UIG532087

 
The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867135

The central region of our Milky Way galaxy. Hubble, Spitzer and Chandra.

UIG867135

 
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

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

 
Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble space telescope. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This is a mosaic image of the spiral galaxy NGC 2442 in Volans processed and assembled from unpublished Hubble Telescope data

PIX4610088

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble space telescope. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This is a mosaic image of the spiral galaxy NGC 2442 in Volans processed and assembled from unpublished Hubble Telescope data

PIX4610088

 
Saturn Planet - Hubble Space Telescope on June 20, 2019.

PIX5940218

Saturn Planet - Hubble Space Telescope on June 20, 2019.

PIX5940218

 
Pluto

UIG2911252

Pluto

UIG2911252

 
Pluto

UIG2911253

Pluto

UIG2911253

 
Hubble Space Telescope Repair

UIG532089

Hubble Space Telescope Repair

UIG532089

 
Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

Visible Crab Nebula - Infrared and X - The Crab Nebula - M1, the Crab Nebula, is the rest of a supernova that exploded on July 4, 1054. It is located about 7000 light years from Earth in the constellation Taurus. At the heart of this nebula is a pulsar. To obtain this photo, three spatial observatories combined their observations: the Hubble telescope for the visible part (here in red and yellow), the Chandra telescope for the X-ray data (blue) and the Spitzer telescope for the infrared image (purple). The pulsar is the bright spot in the center of the image. The Crab Nebula (M1) is a supernova remnant at about 7,000 light - year from Earth in the constellation Taurus. The star explosion occured on July 04 1054. At the center of this nebula lies a pulsar. This composite image uses data from three of Nasa's Great Observatories. The Chandra X - ray image is shown in blue, the Hubble Space Telescope optical images are in red and yellow, and the Spitzer Space Telescope's infrared image is

PIX4583130

 
Image of Mars from Hubble Space Telescope

UIG531595

Image of Mars from Hubble Space Telescope

UIG531595

 
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

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

 
Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

PIX4626476

Kepler is the rest of a supernova that exploded about 400 years ago located about 13,000 light years from Earth in the constellation Ophiuchus. This image obtained from the Hubble space telescope shows the filamentous structures of gases heated in contact with the shock wave. Composite of images obtained in August 2003 and May 2004; cumulative poses of 6 hours 30 minutes - Visible-light images from the Hubble telescope's Advanced Camera for Surveys reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge-on. These filaments reveal where the shock wave is encountering low-density, more uniform interstellar material. Hubble's image was taken with the Advanced Camera for Surveys (ACS) on August 28/29, 2003 & May 26, 2004 for a total of 6.5 hours: Remains of the supernova K

PIX4626476

 
Barree spiral galaxy NGC 4639 in Virgo - Barred galaxy NGC 4639 in Virgo - The barree spiral galaxy NGC 4639 is located 78 million years - light in the Virgin's galaxy cluster. The blue dots visible on this image obtained by the Hubble Space Telescope are young stars. Other stars, cepheides have also been observed in this galaxy, allowing us to measure their distance with precision. This Hubble Space Telescope image shows NGC 4639, a spiral galaxy located 78 million light - years away in the Virgo cluster of galaxies. The blue dots in the galaxy's outlying regions indicate the presence of young stars. Among them are older, bright stars called Cepheids, which are used as reliable milepost markers to obtain accurate distances to nearby galaxies. Astronomers measure the brightness of Cepheids to calculate the distance to a galaxy. After using Cepheids to calculate the distance to NGC 4639, the team compared the results to the peak brightness measurements of SN 1990N, a type Ia supernova l

PIX4611731

Barree spiral galaxy NGC 4639 in Virgo - Barred galaxy NGC 4639 in Virgo - The barree spiral galaxy NGC 4639 is located 78 million years - light in the Virgin's galaxy cluster. The blue dots visible on this image obtained by the Hubble Space Telescope are young stars. Other stars, cepheides have also been observed in this galaxy, allowing us to measure their distance with precision. This Hubble Space Telescope image shows NGC 4639, a spiral galaxy located 78 million light - years away in the Virgo cluster of galaxies. The blue dots in the galaxy's outlying regions indicate the presence of young stars. Among them are older, bright stars called Cepheids, which are used as reliable milepost markers to obtain accurate distances to nearby galaxies. Astronomers measure the brightness of Cepheids to calculate the distance to a galaxy. After using Cepheids to calculate the distance to NGC 4639, the team compared the results to the peak brightness measurements of SN 1990N, a type Ia supernova l

PIX4611731

 
Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

PIX4611257

Barree spiral galaxy NGC 4319 and Markarian quasar 205 - Galaxy NGC 4319 and quasar Markarian 205 - The barree spiral galaxy NGC 4319, in the center, is 80 million years - light in the constellation of the Dragon. The Markarian 205 quasar, on the top right, is 14 times further at about 1 billion light years. These two objects are therefore not interacting; on the other hand, the galaxy NGC 4319 is probably interacting with the galaxy NGC 4291, out of field, as the weak arm at the bottom left allows. Quasars are galaxies that create an extremely bright core. Image made by the Hubble Space Telescope in 2002. In this NASA Hubble Space Telescope image, an odd celestial duo, the spiral galaxy NGC 4319 (center) and a quasar called Markarian 205 (upper right), appear to be neighbors. In reality, the two objects don't even live in the same city. NGC 4319 is 80 million light - years from Earth. Markarian 205 (Mrk 205) is more than 14 times farther away, residing 1 billion light - years from Ear

PIX4611257

 
Cloud IC 349 illuminates by the star Merope - Barnard's Merope Nebula (IC 349) - IC 349 is an interstellar cloud illuminated by the star Merope (off-field) of the Pleiades cluster. Image obtained by the Hubble Space Telescope. This ghostly apparition is actually an interstellar cloud caught in the process of destruction by strong radiation from a nearby hot star. This picture, snapped by the Hubble telescope, shows a cloud illuminated by light from the bright star Merope. Located in the Pleiades star cluster, the cloud is called IC 349 or Barnard's Merope Nebul

PIX4568849

Cloud IC 349 illuminates by the star Merope - Barnard's Merope Nebula (IC 349) - IC 349 is an interstellar cloud illuminated by the star Merope (off-field) of the Pleiades cluster. Image obtained by the Hubble Space Telescope. This ghostly apparition is actually an interstellar cloud caught in the process of destruction by strong radiation from a nearby hot star. This picture, snapped by the Hubble telescope, shows a cloud illuminated by light from the bright star Merope. Located in the Pleiades star cluster, the cloud is called IC 349 or Barnard's Merope Nebul

PIX4568849

 
Polaris System - Polaris is a triple system consisting of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This montage shows the polar star and constellations of the Little Bear and the Big Bear (left), Polaris A and his companion Polaris B seen by the Hubble Space Telescope (top right), and Polaris Ab photographed for the first time by the Hubble Space Telescope (bottom right). This sequence of images shows that the North Star, Polaris is really a triple star system. For the first time, the close companion of Polaris has been seen directly. The left frame shows Polaris's location very close to the position of Earth's north celestial pole in Ursa Minor (the Small Bear). The upper right image shows Polaris A and its distant companion Polaris B, as viewed by Hubble. They are separated by approximately 240 billion miles. Polaris B, the wide companion, is visible in small telescopes, and was first noticed by William Herschel in 1780. The c

PIX4572025

Polaris System - Polaris is a triple system consisting of a supergiant star and two dwarf stars. It is a pulsating variable star, cepheide of low amplitude. This montage shows the polar star and constellations of the Little Bear and the Big Bear (left), Polaris A and his companion Polaris B seen by the Hubble Space Telescope (top right), and Polaris Ab photographed for the first time by the Hubble Space Telescope (bottom right). This sequence of images shows that the North Star, Polaris is really a triple star system. For the first time, the close companion of Polaris has been seen directly. The left frame shows Polaris's location very close to the position of Earth's north celestial pole in Ursa Minor (the Small Bear). The upper right image shows Polaris A and its distant companion Polaris B, as viewed by Hubble. They are separated by approximately 240 billion miles. Polaris B, the wide companion, is visible in small telescopes, and was first noticed by William Herschel in 1780. The c

PIX4572025

 
Barree spiral galaxy NGC 4394 in Berenice's Hair - Barred spiral galaxy NGC 4394 in Coma Berenices: NGC 4394 is a barree spiral galaxy located in the Virgin's cluster about 55 million light years from Earth. Image obtained by the Hubble Space Telescope (HST) - Discovered in 1784 by the German-British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair), and is considered to be a member of the Virgo Cluster. NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy's central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. Liners are active regions that display a characteristic set of emission lines in their spectra- mostl

PIX4611351

Barree spiral galaxy NGC 4394 in Berenice's Hair - Barred spiral galaxy NGC 4394 in Coma Berenices: NGC 4394 is a barree spiral galaxy located in the Virgin's cluster about 55 million light years from Earth. Image obtained by the Hubble Space Telescope (HST) - Discovered in 1784 by the German-British astronomer William Herschel, NGC 4394 is a barred spiral galaxy situated about 55 million light-years from Earth. The galaxy lies in the constellation of Coma Berenices (Berenice's Hair), and is considered to be a member of the Virgo Cluster. NGC 4394 is the archetypal barred spiral galaxy, with bright spiral arms emerging from the ends of a bar that cuts through the galaxy's central bulge. These arms are peppered with young blue stars, dark filaments of cosmic dust, and bright, fuzzy regions of active star formation. At the centre of NGC 4394 lies a region of ionised gas known as a LINER. Liners are active regions that display a characteristic set of emission lines in their spectra- mostl

PIX4611351

 
Hubble deep field sud - Hubble deep field south - In the southern constellation of Toucan, the Hubble space telescope posed 75h to obtain this image of the distant universe. Thousands of galaxies away from 1 to 12 billion light years are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. This picture is the culmination of a 10 - day - long observation called the Hubble Deep Field South which was carried out in October 1998. This new “” far - look”” complements the original Hubble “” deep field””” taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. The new region is in the constellation Tucana, near the south celestial pole. Hubble's sharp vision allows astronomers to sort galaxy shapes. The image is dom

PIX4613806

Hubble deep field sud - Hubble deep field south - In the southern constellation of Toucan, the Hubble space telescope posed 75h to obtain this image of the distant universe. Thousands of galaxies away from 1 to 12 billion light years are visible in this image. From Earth, the target field is the one “” that one would see through the eye of a needle held at arm's length.” If the distribution of galaxies over the entire Celestial vault were similar to this field, the number of galaxies observable up to magnitude 30 would be 50 billion. This picture is the culmination of a 10 - day - long observation called the Hubble Deep Field South which was carried out in October 1998. This new “” far - look”” complements the original Hubble “” deep field””” taken in late 1995, when Hubble was aimed at a small patch of space near the Big Dipper. The new region is in the constellation Tucana, near the south celestial pole. Hubble's sharp vision allows astronomers to sort galaxy shapes. The image is dom

PIX4613806

 
Star V838 Monocerotis 28/10/2004 - V838 Monocerotis 10/2004 - This variable star is located approximately 20,000 years - light from Earth in the constellation Unicorn. In the beginning of 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in October 2004 by the Hubble space telescope, the light echo shows details in the interstellar dust surrounding the star. In January 2002, a variable star in the Monoceros constellation suddenly became 600,000 times more luminous than our Sun, temporarily making it the brightest star in our Milky Way galaxy. The mysterious star, called V838 Monocerotis, has long since faded back to obscurity. Seen here by Nasa's Hubble Space Telescope on October 28, 2004, the light echo around the star has uncovered details in the interstellar dust round the star

PIX4572282

Star V838 Monocerotis 28/10/2004 - V838 Monocerotis 10/2004 - This variable star is located approximately 20,000 years - light from Earth in the constellation Unicorn. In the beginning of 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in October 2004 by the Hubble space telescope, the light echo shows details in the interstellar dust surrounding the star. In January 2002, a variable star in the Monoceros constellation suddenly became 600,000 times more luminous than our Sun, temporarily making it the brightest star in our Milky Way galaxy. The mysterious star, called V838 Monocerotis, has long since faded back to obscurity. Seen here by Nasa's Hubble Space Telescope on October 28, 2004, the light echo around the star has uncovered details in the interstellar dust round the star

PIX4572282

 
Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

PIX4572319

Star V838 Monocerotis. 09/2006 - V838 Monocerotis seen by the Hubble space telescope. 09/2006 - This variable star is located about 20,000 years ago - light from Earth in the constellation of Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in September 2006 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V8

PIX4572319

 
Usage restrictions from our Content Partners
  • Not available to clients invoiced in China
The Hubble space telescope

UDK844647

The Hubble space telescope

UDK844647

 
Star V838 Monocerotis. 11/2005 - Star V838 Monocerotis seen by the Hubble space telescope. 11/2005 - This variable star is located about 20,000 years ago - light from Earth in the constellation Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in November 2005 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V

PIX4572295

Star V838 Monocerotis. 11/2005 - Star V838 Monocerotis seen by the Hubble space telescope. 11/2005 - This variable star is located about 20,000 years ago - light from Earth in the constellation Unicorn. Beginning in 2002, this star illuminated temporarily becoming one of the brightest stars in the sky. Viewed here in November 2005 by the Hubble space telescope, the light echo reveals details in the interstellar dust surrounding the star. Light from a star that erupted almost five years ago continues propagating outward through a cloud of dust surrounding the star. The light reflects or “” echoes”” off the dust and then travels to Earth. Because of the extra distance the scattered light travels, it reaches the Earth long after the light from the stellar outburst itself. Therefore, a light echo is an analog of a sound echo produced, for example, when sound from an Alpine yodeler echoes off of the surrounding mountainsides. The echo comes from the unusual variable star V838 Monocerotis (V

PIX4572295

 
Cepheides in the galaxy M81 - Cepheids in the galaxy M81 - Cepheides are very bright variable stars that serve as cosmic beacons to measure distance from nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope identified cepheides in the M81 galaxy; astronomers were able to deduce a new distance for this galaxy; it would be 11 million years - light from Earth; previous estimates gave a figure of 18 million light years. Image obtained in 1993. Astronomers have discovered variable stars in the spiral galaxy M81, and measured the distance of the galaxy to be 11 million light - years (3.4 megaparsecs). They quote a 10% uncertainty in this result (plus or minus approximately one million light - years). Previous estimates of the galaxy's distance have ranged from 4.5 to 18 million light - years (1.4 to 5.6 megaparsecs). The astrono

PIX4572157

Cepheides in the galaxy M81 - Cepheids in the galaxy M81 - Cepheides are very bright variable stars that serve as cosmic beacons to measure distance from nearby galaxies. Their pulse period is measured and their absolute luminosite is calculated. By comparing the result to their apparent luminosite in the sky, they can be calculated accurately. Here, the space telescope identified cepheides in the M81 galaxy; astronomers were able to deduce a new distance for this galaxy; it would be 11 million years - light from Earth; previous estimates gave a figure of 18 million light years. Image obtained in 1993. Astronomers have discovered variable stars in the spiral galaxy M81, and measured the distance of the galaxy to be 11 million light - years (3.4 megaparsecs). They quote a 10% uncertainty in this result (plus or minus approximately one million light - years). Previous estimates of the galaxy's distance have ranged from 4.5 to 18 million light - years (1.4 to 5.6 megaparsecs). The astrono

PIX4572157

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

Navigation

Contact

Bridgeman Images
77 Sands Street, 6th Floor
Brooklyn, NY 11201
United States

T: +1 212 828 1238

Legal

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