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1016466 Search Results for Photography

Nebuleuse NGC 7129 in Cephe
Nebuleuse NGC 7129 in Cephe

PIX4620570: Nebuleuse NGC 7129 in Cephe / Bridgeman Images

ID: PIX4620570

Nebuleuse NGC 7129 in Cephe

Nebuleuse NGC 7635 in Cassiopee - 2005 Image acquired at the Nighthawk Observator
Nebuleuse NGC 7635 in Cassiopee - 2005 Image acquired at the Nighthawk Observator

PIX4620644: Nebuleuse NGC 7635 in Cassiopee - 2005 Image acquired at the Nighthawk Observator / Bridgeman Images

ID: PIX4620644

Nebuleuse NGC 7635 in Cassiopee - 2005 Image acquired at the Nighthawk Observator

Nebula Sh2 - 142 in Cephee - Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Nebula Sh2 - 142 in Cephee - Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

PIX4621031: Nebula Sh2 - 142 in Cephee - Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed / Bridgeman Images

ID: PIX4621031

Nebula Sh2 - 142 in Cephee - Nebula Sh2 - 142 in Cephee - Star formation region in Cephee and star clusters NGC 7380. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

Nebulae VDB 14 and VDB 15 - Nebulae VDB 14 and VDB 15 - Nebulae reflexion in the constellation Giraf
Nebulae VDB 14 and VDB 15 - Nebulae VDB 14 and VDB 15 - Nebulae reflexion in the constellation Giraf

PIX4621173: Nebulae VDB 14 and VDB 15 - Nebulae VDB 14 and VDB 15 - Nebulae reflexion in the constellation Giraf / Bridgeman Images

ID: PIX4621173

Nebulae VDB 14 and VDB 15 - Nebulae VDB 14 and VDB 15 - Nebulae reflexion in the constellation Giraf

Molecular cloud B 68 in Ophiuchus seen in infrared - False - colour composite based on a visible (here rendered as blue), a near - infrared (green) and an infrared (red) image. Since the light from stars behind the cloud is only visible at the longest (infrared) wavelengths, they appear red. At a distance of only 410 light - years, Barnard 68 is one of the nearest dark clouds. Its size is about 12,500 AU (= 2 million km; 1 Astronomical Unit [AU] = 150 million km), or just about the same as the so - called “” Oort Cloud””” of long - period comets that surrounds the solar system. The temperature of Barnard 68 is 16 Kelvin (- 257* C) The total mass of the cloud is about twice that of the Sun
Molecular cloud B 68 in Ophiuchus seen in infrared - False - colour composite based on a visible (here rendered as blue), a near - infrared (green) and an infrared (red) image. Since the light from stars behind the cloud is only visible at the longest (infrared) wavelengths, they appear red. At a distance of only 410 light - years, Barnard 68 is one of the nearest dark clouds. Its size is about 12,500 AU (= 2 million km; 1 Astronomical Unit [AU] = 150 million km), or just about the same as the so - called “” Oort Cloud””” of long - period comets that surrounds the solar system. The temperature of Barnard 68 is 16 Kelvin (- 257* C) The total mass of the cloud is about twice that of the Sun

PIX4621267: Molecular cloud B 68 in Ophiuchus seen in infrared - False - colour composite based on a visible (here rendered as blue), a near - infrared (green) and an infrared (red) image. Since the light from stars behind the cloud is only visible at the longest (infrared) wavelengths, they appear red. At a distance of only 410 light - years, Barnard 68 is one of the nearest dark clouds. Its size is about 12,500 AU (= 2 million km; 1 Astronomical Unit [AU] = 150 million km), or just about the same as the so - called “” Oort Cloud””” of long - period comets that surrounds the solar system. The temperature of Barnard 68 is 16 Kelvin (- 257* C) The total mass of the cloud is about twice that of the Sun / Bridgeman Images

ID: PIX4621267

Molecular cloud B 68 in Ophiuchus seen in infrared - False - colour composite based on a visible (here rendered as blue), a near - infrared (green) and an infrared (red) image. Since the light from stars behind the cloud is only visible at the longest (infrared) wavelengths, they appear red. At a distance of only 410 light - years, Barnard 68 is one of the nearest dark clouds. Its size is about 12,500 AU (= 2 million km; 1 Astronomical Unit [AU] = 150 million km), or just about the same as the so - called “” Oort Cloud””” of long - period comets that surrounds the solar system. The temperature of Barnard 68 is 16 Kelvin (- 257* C) The total mass of the cloud is about twice that of the Sun

Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse and core formation within the dense compact clouds. Lower and intermediate mass stars ultimately form from the compact gas and dust within the blood cells
Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse and core formation within the dense compact clouds. Lower and intermediate mass stars ultimately form from the compact gas and dust within the blood cells

PIX4621601: Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse and core formation within the dense compact clouds. Lower and intermediate mass stars ultimately form from the compact gas and dust within the blood cells / Bridgeman Images

ID: PIX4621601

Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse

Nebulae VdB 93 and IC 2177 in Unicorn - VDB 93 (NGC 2327) is a star-forming region belonging to nebula IC 2177. The star SAO 152320, in the center of the image, illuminates this nebula located in the constellation Unicorn, about 4000 years old - light from Earth. Mosaic of images obtained in 1983 and 1989 with the 1.2m Schmidt UK Telescope from Siding Spring
Nebulae VdB 93 and IC 2177 in Unicorn - VDB 93 (NGC 2327) is a star-forming region belonging to nebula IC 2177. The star SAO 152320, in the center of the image, illuminates this nebula located in the constellation Unicorn, about 4000 years old - light from Earth. Mosaic of images obtained in 1983 and 1989 with the 1.2m Schmidt UK Telescope from Siding Spring

PIX4622555: Nebulae VdB 93 and IC 2177 in Unicorn - VDB 93 (NGC 2327) is a star-forming region belonging to nebula IC 2177. The star SAO 152320, in the center of the image, illuminates this nebula located in the constellation Unicorn, about 4000 years old - light from Earth. Mosaic of images obtained in 1983 and 1989 with the 1.2m Schmidt UK Telescope from Siding Spring / Bridgeman Images

ID: PIX4622555

Nebulae VdB 93 and IC 2177 in Unicorn - VDB 93 (NGC 2327) is a star-forming region belonging to nebula IC 2177. The star SAO 152320, in the center of the image, illuminates this nebula located in the constellation Unicorn, about 4000 years old - light from Earth. Mosaic of images obtained in 1983 and 1989 with the 1.2m Schmidt UK Telescope from Siding Spring

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which are compact dark structures first described by the astronomer Bart Bok (1906 - 1983) in the 1940's. Bok Globules are small dark clouds of gas and dust that are found in HII regions and typically have a mass of about 10 to 50 solar masses. They often span a region of about one light year across. Their contents are predominantly molecular hydrogen, carbon oxides and helium but also contain about small amounts (1%) of silicate dust. Infrared observations in the 1990's detected the existence of protostars within the dense confines of Bok globules confirming the hypothesis of Bok, who strongly believed that these globules represented cocoons of starbirth. The larger Bok Globules seen in the image are about 1.4 light years across and contain enough mass to make 15 suns. Four Frame Mosaic, Total Exposure 28 Hours 14.5”” RCOS telescope
Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which are compact dark structures first described by the astronomer Bart Bok (1906 - 1983) in the 1940's. Bok Globules are small dark clouds of gas and dust that are found in HII regions and typically have a mass of about 10 to 50 solar masses. They often span a region of about one light year across. Their contents are predominantly molecular hydrogen, carbon oxides and helium but also contain about small amounts (1%) of silicate dust. Infrared observations in the 1990's detected the existence of protostars within the dense confines of Bok globules confirming the hypothesis of Bok, who strongly believed that these globules represented cocoons of starbirth. The larger Bok Globules seen in the image are about 1.4 light years across and contain enough mass to make 15 suns. Four Frame Mosaic, Total Exposure 28 Hours 14.5”” RCOS telescope

PIX4622567: Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which are compact dark structures first described by the astronomer Bart Bok (1906 - 1983) in the 1940's. Bok Globules are small dark clouds of gas and dust that are found in HII regions and typically have a mass of about 10 to 50 solar masses. They often span a region of about one light year across. Their contents are predominantly molecular hydrogen, carbon oxides and helium but also contain about small amounts (1%) of silicate dust. Infrared observations in the 1990's detected the existence of protostars within the dense confines of Bok globules confirming the hypothesis of Bok, who strongly believed that these globules represented cocoons of starbirth. The larger Bok Globules seen in the image are about 1.4 light years across and contain enough mass to make 15 suns. Four Frame Mosaic, Total Exposure 28 Hours 14.5”” RCOS telescope / Bridgeman Images

ID: PIX4622567

Nebulae IC 2948 and 2944 in Centaur - A large southern emission nebula, IC 2948 - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaur. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. IC2944 is a large HII region (star forming cloud) in the southern constellation of Centaurus. The bright blue star in the upper right is Lambda Centauri, one of the brightest stars in the southern sky.The cluster of hot blue stars to the right of center are illuminating the gases of IC2944 and causing it to glow in the red and magenta light of excited hydrogen. The compact black objects adjacent to the bright blue stars are called Thackeray's Globules named for the astronomer A.D. Thackeray who described these in 1950. Thackeray Globules are similar to Bok Globules which

Nebulae IC 4592 and IC 4601 in Scorpio - Nebulae IC 4592 and IC 4601 in Scorpio - IC 4592 is a reflexion nebula, the fine normally dark dust is illuminated by the light of Nu Scorpii, a five star system, very bright. Top right, another reflexion nebula, IC 4601
Nebulae IC 4592 and IC 4601 in Scorpio - Nebulae IC 4592 and IC 4601 in Scorpio - IC 4592 is a reflexion nebula, the fine normally dark dust is illuminated by the light of Nu Scorpii, a five star system, very bright. Top right, another reflexion nebula, IC 4601

PIX4622581: Nebulae IC 4592 and IC 4601 in Scorpio - Nebulae IC 4592 and IC 4601 in Scorpio - IC 4592 is a reflexion nebula, the fine normally dark dust is illuminated by the light of Nu Scorpii, a five star system, very bright. Top right, another reflexion nebula, IC 4601 / Bridgeman Images

ID: PIX4622581

Nebulae IC 4592 and IC 4601 in Scorpio - Nebulae IC 4592 and IC 4601 in Scorpio - IC 4592 is a reflexion nebula, the fine normally dark dust is illuminated by the light of Nu Scorpii, a five star system, very bright. Top right, another reflexion nebula, IC 4601

Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 in the middle left of the image is surrounded at the bottom by the star cluster NGC 6231, and by the NGC 6242 cluster at the top of the image. A beautiful collection of open clusters and nebulosity is seen here in Scorpius, just north of the double star Zeta Scorpii. Zeta is visible at the far bottom right and is also know as the “Little Cat's Eyes””. NGC 6231 is a lovely open cluster above Zeta. IC 4628 is the emission nebula just northeast of two loose open clusters, Cr 316 and Tr 24 in the center of the photo. NGC 6242 is the other small open cluster at top left. (c) 2006 Jerry Lodriguss/www.astropix.co
Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 in the middle left of the image is surrounded at the bottom by the star cluster NGC 6231, and by the NGC 6242 cluster at the top of the image. A beautiful collection of open clusters and nebulosity is seen here in Scorpius, just north of the double star Zeta Scorpii. Zeta is visible at the far bottom right and is also know as the “Little Cat's Eyes””. NGC 6231 is a lovely open cluster above Zeta. IC 4628 is the emission nebula just northeast of two loose open clusters, Cr 316 and Tr 24 in the center of the photo. NGC 6242 is the other small open cluster at top left. (c) 2006 Jerry Lodriguss/www.astropix.co

PIX4622614: Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 in the middle left of the image is surrounded at the bottom by the star cluster NGC 6231, and by the NGC 6242 cluster at the top of the image. A beautiful collection of open clusters and nebulosity is seen here in Scorpius, just north of the double star Zeta Scorpii. Zeta is visible at the far bottom right and is also know as the “Little Cat's Eyes””. NGC 6231 is a lovely open cluster above Zeta. IC 4628 is the emission nebula just northeast of two loose open clusters, Cr 316 and Tr 24 in the center of the photo. NGC 6242 is the other small open cluster at top left. (c) 2006 Jerry Lodriguss/www.astropix.co / Bridgeman Images

ID: PIX4622614

Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 and star clusters in Scorpio - Nebula IC 4628 in the middle left of the image is surrounded at the bottom by the star cluster NGC 6231, and by the NGC 6242 cluster at the top of the image. A beautiful collection of open clusters and nebulosity is seen here in Scorpius, just north of the double star Zeta Scorpii. Zeta is visible at the far bottom right and is also know as the “Little Cat's Eyes””. NGC 6231 is a lovely open cluster above Zeta. IC 4628 is the emission nebula just northeast of two loose open clusters, Cr 316 and Tr 24 in the center of the photo. NGC 6242 is the other small open cluster at top left. (c) 2006 Jerry Lodriguss/www.astropix.co

Pelican Nebula (IC 5070) in the Cygn
Pelican Nebula (IC 5070) in the Cygn

PIX4622665: Pelican Nebula (IC 5070) in the Cygn / Bridgeman Images

ID: PIX4622665

Pelican Nebula (IC 5070) in the Cygn

Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula - IC 5146 130 EDT f/8 working at f/6 6 minute exposure hypered Fujicolor Super HG 400 3:20 am May 14, 1994 Sentinel, A
Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula - IC 5146 130 EDT f/8 working at f/6 6 minute exposure hypered Fujicolor Super HG 400 3:20 am May 14, 1994 Sentinel, A

PIX4622694: Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula - IC 5146 130 EDT f/8 working at f/6 6 minute exposure hypered Fujicolor Super HG 400 3:20 am May 14, 1994 Sentinel, A / Bridgeman Images

ID: PIX4622694

Cocoon Nebula (IC 5146) in the Swan - Cocoon Nebula - IC 5146 130 EDT f/8 working at f/6 6 minute exposure hypered Fujicolor Super HG 400 3:20 am May 14, 1994 Sentinel, A

Cocon Nebula (IC 5146) in Swan - Cocon Nebula (IC 5146) in Swan - Cocon Nebula is located about 4000 light years from Earth in the constellation Swan. It's a star-forming region. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Cocon Nebula (IC 5146) in Swan - Cocon Nebula (IC 5146) in Swan - Cocon Nebula is located about 4000 light years from Earth in the constellation Swan. It's a star-forming region. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

PIX4622715: Cocon Nebula (IC 5146) in Swan - Cocon Nebula (IC 5146) in Swan - Cocon Nebula is located about 4000 light years from Earth in the constellation Swan. It's a star-forming region. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed / Bridgeman Images

ID: PIX4622715

Cocon Nebula (IC 5146) in Swan - Cocon Nebula (IC 5146) in Swan - Cocon Nebula is located about 4000 light years from Earth in the constellation Swan. It's a star-forming region. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

Planetary nebula NGC 1360 in the Fournea
Planetary nebula NGC 1360 in the Fournea

PIX4622906: Planetary nebula NGC 1360 in the Fournea / Bridgeman Images

ID: PIX4622906

Planetary nebula NGC 1360 in the Fournea

Nebula of the Lagoon (M8) in the Sagittarius - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL. Composite Image
Nebula of the Lagoon (M8) in the Sagittarius - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL. Composite Image

PIX4619713: Nebula of the Lagoon (M8) in the Sagittarius - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL. Composite Image / Bridgeman Images

ID: PIX4619713

Nebula of the Lagoon (M8) in the Sagittarius - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL. Composite Image

Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth
Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth

PIX4619806: Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth / Bridgeman Images

ID: PIX4619806

Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth

Nebulae M20 - M8 in Sagittair
Nebulae M20 - M8 in Sagittair

PIX4619821: Nebulae M20 - M8 in Sagittair / Bridgeman Images

ID: PIX4619821

Nebulae M20 - M8 in Sagittair

Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Star field in Sagittarius with dark nebulae Barnard 92 and Barnard 93 to the bottom of nebulae IC 1283 - 84 and NGC 6589 - 90 and Sagittarius cluster M24
Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Star field in Sagittarius with dark nebulae Barnard 92 and Barnard 93 to the bottom of nebulae IC 1283 - 84 and NGC 6589 - 90 and Sagittarius cluster M24

PIX4619889: Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Star field in Sagittarius with dark nebulae Barnard 92 and Barnard 93 to the bottom of nebulae IC 1283 - 84 and NGC 6589 - 90 and Sagittarius cluster M24 / Bridgeman Images

ID: PIX4619889

Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Nebulae IC 1283 - 84 and M24 clusters in Sagittarius - Star field in Sagittarius with dark nebulae Barnard 92 and Barnard 93 to the bottom of nebulae IC 1283 - 84 and NGC 6589 - 90 and Sagittarius cluster M24

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Messier 16 is a cluster of stars formed about 2 million years ago from the gas and dust that still surrounds it today. The nebula always forms new stars. It is located about 7000 light years from Earth in the constellation Serpent
Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Messier 16 is a cluster of stars formed about 2 million years ago from the gas and dust that still surrounds it today. The nebula always forms new stars. It is located about 7000 light years from Earth in the constellation Serpent

PIX4619938: Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Messier 16 is a cluster of stars formed about 2 million years ago from the gas and dust that still surrounds it today. The nebula always forms new stars. It is located about 7000 light years from Earth in the constellation Serpent / Bridgeman Images

ID: PIX4619938

Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Eagle Nebula (IC 4703) and M16 star cluster in the Snake - Messier 16 is a cluster of stars formed about 2 million years ago from the gas and dust that still surrounds it today. The nebula always forms new stars. It is located about 7000 light years from Earth in the constellation Serpent

Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - The M16 Star Cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle Nebula, IC 4703 3. These stars are much warmer than the Sun and can be 30 times more massive.
Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - The M16 Star Cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle Nebula, IC 4703 3. These stars are much warmer than the Sun and can be 30 times more massive.

PIX4619985: Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - The M16 Star Cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle Nebula, IC 4703 3. These stars are much warmer than the Sun and can be 30 times more massive. / Bridgeman Images

ID: PIX4619985

Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - Eagle Nebula (IC 4703) and M16 Star Cluster in the Snake - The M16 Star Cluster is a cluster of young stars from 7000 years - light, formed about 2 million years ago in the Eagle Nebula, IC 4703 3. These stars are much warmer than the Sun and can be 30 times more massive.

Omega nebula (M17) in Sagittair
Omega nebula (M17) in Sagittair

PIX4620127: Omega nebula (M17) in Sagittair / Bridgeman Images

ID: PIX4620127

Omega nebula (M17) in Sagittair

Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - The Cone nebula, in the right center, is a H II region located about 2600 years - light from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Upstairs, an open cluster of stars, Trumpler 5. Below, to the right, the Hubble nebula. Image obtained with a Takahashi FSQ 106 bezel, through various filters
Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - The Cone nebula, in the right center, is a H II region located about 2600 years - light from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Upstairs, an open cluster of stars, Trumpler 5. Below, to the right, the Hubble nebula. Image obtained with a Takahashi FSQ 106 bezel, through various filters

PIX4618750: Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - The Cone nebula, in the right center, is a H II region located about 2600 years - light from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Upstairs, an open cluster of stars, Trumpler 5. Below, to the right, the Hubble nebula. Image obtained with a Takahashi FSQ 106 bezel, through various filters / Bridgeman Images

ID: PIX4618750

Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - Nebula NGC 2264, S Monocerotis, Hubble nebula and Trumpler 5 clusters in Unicorn - The Cone nebula, in the right center, is a H II region located about 2600 years - light from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Upstairs, an open cluster of stars, Trumpler 5. Below, to the right, the Hubble nebula. Image obtained with a Takahashi FSQ 106 bezel, through various filters

Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae. All around it, many star clusters are visible, including the South Pleiades, IC 2602, top left
Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae. All around it, many star clusters are visible, including the South Pleiades, IC 2602, top left

PIX4618911: Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae. All around it, many star clusters are visible, including the South Pleiades, IC 2602, top left / Bridgeman Images

ID: PIX4618911

Nebula NGC 3372 and cluster of stars in the Carene - The nebula of the Carene is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae. All around it, many star clusters are visible, including the South Pleiades, IC 2602, top left

Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It is home to many hot stars, including the star Eta Carinae
Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It is home to many hot stars, including the star Eta Carinae

PIX4618921: Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It is home to many hot stars, including the star Eta Carinae / Bridgeman Images

ID: PIX4618921

Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It is home to many hot stars, including the star Eta Carinae

Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It's a star-forming region. It also houses a dozen massive stars, including the star Eta Carinae (left). On the right, a cluster of young stars, Trumpler 14. Image made with ACS camera of the Hubble space telescope, 48-frame mosaic
Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It's a star-forming region. It also houses a dozen massive stars, including the star Eta Carinae (left). On the right, a cluster of young stars, Trumpler 14. Image made with ACS camera of the Hubble space telescope, 48-frame mosaic

PIX4618962: Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It's a star-forming region. It also houses a dozen massive stars, including the star Eta Carinae (left). On the right, a cluster of young stars, Trumpler 14. Image made with ACS camera of the Hubble space telescope, 48-frame mosaic / Bridgeman Images

ID: PIX4618962

Nebula NGC 3372 in the Carene - The nebula of the Carene is located about 7000 light years from the Earth. It's a star-forming region. It also houses a dozen massive stars, including the star Eta Carinae (left). On the right, a cluster of young stars, Trumpler 14. Image made with ACS camera of the Hubble space telescope, 48-frame mosaic

Nebulae in the Carene - H - Alpha - The Carene nebula (NGC 3372), on the right, is located about 7000 light years from Earth. It is home to many hot stars, including the star Eta Carinae. Lower left, nebulae NGC 3603 and NGC 3576. Image made with an H - alpha filter in Chile
Nebulae in the Carene - H - Alpha - The Carene nebula (NGC 3372), on the right, is located about 7000 light years from Earth. It is home to many hot stars, including the star Eta Carinae. Lower left, nebulae NGC 3603 and NGC 3576. Image made with an H - alpha filter in Chile

PIX4618998: Nebulae in the Carene - H - Alpha - The Carene nebula (NGC 3372), on the right, is located about 7000 light years from Earth. It is home to many hot stars, including the star Eta Carinae. Lower left, nebulae NGC 3603 and NGC 3576. Image made with an H - alpha filter in Chile / Bridgeman Images

ID: PIX4618998

Nebulae in the Carene - H - Alpha - The Carene nebula (NGC 3372), on the right, is located about 7000 light years from Earth. It is home to many hot stars, including the star Eta Carinae. Lower left, nebulae NGC 3603 and NGC 3576. Image made with an H - alpha filter in Chile

Nebulae NGC 3603 and NGC 3576 in the Carene - Nebulae NGC 3603 and NGC 3576 in the Carene - NGC 3576 (right) is located about 10,000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene
Nebulae NGC 3603 and NGC 3576 in the Carene - Nebulae NGC 3603 and NGC 3576 in the Carene - NGC 3576 (right) is located about 10,000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene

PIX4619203: Nebulae NGC 3603 and NGC 3576 in the Carene - Nebulae NGC 3603 and NGC 3576 in the Carene - NGC 3576 (right) is located about 10,000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene / Bridgeman Images

ID: PIX4619203

Nebulae NGC 3603 and NGC 3576 in the Carene - Nebulae NGC 3603 and NGC 3576 in the Carene - NGC 3576 (right) is located about 10,000 years - light from Earth; NGC 3603 (left) is twice as far away. These two nebulae are located in the constellation Carene

Nebula NGC 6188 in the Altar - Nebula NGC 6188 is located about 4000 light years from Earth. It is home to a cluster of young stars NGC 6193, formed three million years ago. Image obtained by Siding Spring's 3.9m telescope
Nebula NGC 6188 in the Altar - Nebula NGC 6188 is located about 4000 light years from Earth. It is home to a cluster of young stars NGC 6193, formed three million years ago. Image obtained by Siding Spring's 3.9m telescope

PIX4619247: Nebula NGC 6188 in the Altar - Nebula NGC 6188 is located about 4000 light years from Earth. It is home to a cluster of young stars NGC 6193, formed three million years ago. Image obtained by Siding Spring's 3.9m telescope / Bridgeman Images

ID: PIX4619247

Nebula NGC 6188 in the Altar - Nebula NGC 6188 is located about 4000 light years from Earth. It is home to a cluster of young stars NGC 6193, formed three million years ago. Image obtained by Siding Spring's 3.9m telescope

Nebula NGC 6357 in the Scorpio - This nebulae is located about 5500 light years from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Nebula NGC 6357 in the Scorpio - This nebulae is located about 5500 light years from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

PIX4619414: Nebula NGC 6357 in the Scorpio - This nebulae is located about 5500 light years from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed / Bridgeman Images

ID: PIX4619414

Nebula NGC 6357 in the Scorpio - This nebulae is located about 5500 light years from Earth. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

The nebula of the Lagoon (M - 8/ngc 6523) - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL
The nebula of the Lagoon (M - 8/ngc 6523) - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL

PIX4619605: The nebula of the Lagoon (M - 8/ngc 6523) - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL / Bridgeman Images

ID: PIX4619605

The nebula of the Lagoon (M - 8/ngc 6523) - View of the nebula of the Lagoon (M - 8/ngc 6523). Located in Sagittarius, at a distance of 6500 light years, it extends over a diameter of 60 AL

Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe
Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe

PIX4617146: Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe / Bridgeman Images

ID: PIX4617146

Mercury by Mariner 10 - Mercury by Mariner 10 - Basin Caloris - The Basin Caloris is the rest of a large impact crater; visible half on the left of the image, it measures 1300 km in diameter. Mosaic of images obtained by the Mariner 10 probe

Mercury by Mariner 10 - Mercury by Mariner 10 - Shakespeare crater region - Mosaic of images made by the Mariner 10 probe. Shakespeare crater area (poorly visible on the left; In the right center of the image, the 45 km Degas crater with its bright star ejectas. On the left, part of the Caloris basin
Mercury by Mariner 10 - Mercury by Mariner 10 - Shakespeare crater region - Mosaic of images made by the Mariner 10 probe. Shakespeare crater area (poorly visible on the left; In the right center of the image, the 45 km Degas crater with its bright star ejectas. On the left, part of the Caloris basin

PIX4617207: Mercury by Mariner 10 - Mercury by Mariner 10 - Shakespeare crater region - Mosaic of images made by the Mariner 10 probe. Shakespeare crater area (poorly visible on the left; In the right center of the image, the 45 km Degas crater with its bright star ejectas. On the left, part of the Caloris basin / Bridgeman Images

ID: PIX4617207

Mercury by Mariner 10 - Mercury by Mariner 10 - Shakespeare crater region - Mosaic of images made by the Mariner 10 probe. Shakespeare crater area (poorly visible on the left; In the right center of the image, the 45 km Degas crater with its bright star ejectas. On the left, part of the Caloris basin

Tarantula Nebula (NGC 2070) in the Sea bream - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Mosaic of 14 images, 70 hours of cumulative poses. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a huge stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula is thought to contain more than half a million times the mass of the Sun in gas and this vast, blazing labyrinth hosts some of the most massive stars known. Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions. 14 Panel Mosaic, Total Exposure 70 Hours with a 14.5” telescope
Tarantula Nebula (NGC 2070) in the Sea bream - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Mosaic of 14 images, 70 hours of cumulative poses. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a huge stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula is thought to contain more than half a million times the mass of the Sun in gas and this vast, blazing labyrinth hosts some of the most massive stars known. Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions. 14 Panel Mosaic, Total Exposure 70 Hours with a 14.5” telescope

PIX4618298: Tarantula Nebula (NGC 2070) in the Sea bream - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Mosaic of 14 images, 70 hours of cumulative poses. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a huge stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula is thought to contain more than half a million times the mass of the Sun in gas and this vast, blazing labyrinth hosts some of the most massive stars known. Surrounding this nebula is a huge and much fainter series of interlocking bubbles and shells of gas and dust blow away from the center of activity by intense stellar winds and supernova explosions. 14 Panel Mosaic, Total Exposure 70 Hours with a 14.5” telescope / Bridgeman Images

ID: PIX4618298

Tarantula Nebula (NGC 2070) in the Sea bream - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula (or 30 Bream bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Mosaic of 14 images, 70 hours of cumulative poses. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a huge stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula is thought to contain more than half a million times the mass of the Sun in gas and this vast, blazing labyrinth hosts some of the most massive stars known. Su

Nebula NGC 2174 in Orion - Nebula NGC 2174 in Orion - NGC2174 is a large nebula that surrounds the cluster of stars NGC 2175 in the constellation Orion
Nebula NGC 2174 in Orion - Nebula NGC 2174 in Orion - NGC2174 is a large nebula that surrounds the cluster of stars NGC 2175 in the constellation Orion

PIX4618389: Nebula NGC 2174 in Orion - Nebula NGC 2174 in Orion - NGC2174 is a large nebula that surrounds the cluster of stars NGC 2175 in the constellation Orion / Bridgeman Images

ID: PIX4618389

Nebula NGC 2174 in Orion - Nebula NGC 2174 in Orion - NGC2174 is a large nebula that surrounds the cluster of stars NGC 2175 in the constellation Orion

Nebula of the cone Ngc 2264 in the Unicorn - The Cone Nebula (also known as NGC 2264) is an H II region in the constellation of Monoceros. It was discovered by William Herschel in 1785. The nebula is located about 800 parsecs or 2,600 light - years away from Earth. The Cone Nebula is part of the nebulosity surrounding the Christmas Tree Cluster. The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone
Nebula of the cone Ngc 2264 in the Unicorn - The Cone Nebula (also known as NGC 2264) is an H II region in the constellation of Monoceros. It was discovered by William Herschel in 1785. The nebula is located about 800 parsecs or 2,600 light - years away from Earth. The Cone Nebula is part of the nebulosity surrounding the Christmas Tree Cluster. The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone

PIX4618597: Nebula of the cone Ngc 2264 in the Unicorn - The Cone Nebula (also known as NGC 2264) is an H II region in the constellation of Monoceros. It was discovered by William Herschel in 1785. The nebula is located about 800 parsecs or 2,600 light - years away from Earth. The Cone Nebula is part of the nebulosity surrounding the Christmas Tree Cluster. The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone / Bridgeman Images

ID: PIX4618597

Nebula of the cone Ngc 2264 in the Unicorn - The Cone Nebula (also known as NGC 2264) is an H II region in the constellation of Monoceros. It was discovered by William Herschel in 1785. The nebula is located about 800 parsecs or 2,600 light - years away from Earth. The Cone Nebula is part of the nebulosity surrounding the Christmas Tree Cluster. The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone

Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from the Earth. The bright star is S Monocerotis, a star of magnitude 4.7
Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from the Earth. The bright star is S Monocerotis, a star of magnitude 4.7

PIX4618635: Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from the Earth. The bright star is S Monocerotis, a star of magnitude 4.7 / Bridgeman Images

ID: PIX4618635

Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from the Earth. The bright star is S Monocerotis, a star of magnitude 4.7


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