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Images of 'Star Fish' found, 319

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Erythrin of Malabar (colour litho)

Erythrin of Malabar (colour litho)

German School, (19th century)

PRX998731

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

PIX4593501

Starfish

Starfish

English School, (20th century)

LAL319223

Constellation of Fish - Constellation of Pisce

Constellation of Fish - Constellation of Pisce

B&S.Fletcher

PIX4593476

Galaxy NGC 660 in Pisces - Galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image of the central part of the galaxy obtained by the Hubble Space Telescope (HST). NGC 660 is described as being a “” polar ring””” galaxy. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million light years away. Image taken with the Hubble space telescope (HST)

Galaxy NGC 660 in Pisces - Galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image of the central part of the galaxy obtained by the Hubble Space Telescope (HST). NGC 660 is described as being a “” polar ring””” galaxy. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million light years away. Image taken with the Hubble space telescope (HST)

R. Gendler

PIX4609420

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

PIX4593469

Constellation of Pisces - The constellation of Pisces with its main stars. Constellation of Pisces with its main stars

Constellation of Pisces - The constellation of Pisces with its main stars. Constellation of Pisces with its main stars

PIX4593531

Galaxy NGC 660 in Pisces - Polar ring galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image made with a telescope 61 cm in diameter. NGC 660 is described as being a “” polar ring””” galaxy. Another remarkable picture of this rare type of galaxy was taken by the Hubble Space Telescope - the example in this case is NGC4650A. These galaxies are believed to have formed from the collision of two galaxies in the past. In the case of NGC 660 it would appear that our perspective is inclined from the axis of the disk so that the foreground portion of the ring does not cross the plane in the middle - but instead towards one side. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million

Galaxy NGC 660 in Pisces - Polar ring galaxy NGC 660 in Pisces - The galaxy NGC 660 is located about 20 million light years ago in the constellation Pisces. It is a polar ring galaxy, a fairly rare type of galaxy that features a ring of gas and dust almost perpendicular to the main galactic plane. Image made with a telescope 61 cm in diameter. NGC 660 is described as being a “” polar ring””” galaxy. Another remarkable picture of this rare type of galaxy was taken by the Hubble Space Telescope - the example in this case is NGC4650A. These galaxies are believed to have formed from the collision of two galaxies in the past. In the case of NGC 660 it would appear that our perspective is inclined from the axis of the disk so that the foreground portion of the ring does not cross the plane in the middle - but instead towards one side. The central region of this galaxy is considered a “” starburst”” due to the extreme amount of luminous star formation.This galaxy is estimated to be 24 million

Adam Block

PIX4609435

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

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

Aquarius

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Aquarius

SAB114449

Equestrian Star fish, a Star fish producing its rays, the Violet Asteria, upper and under surface of a Star fish (litho)

Equestrian Star fish, a Star fish producing its rays, the Violet Asteria, upper and under surface of a Star fish (litho)

English School, (19th century)

LLM970867

Galaxy AM 0644 - 741 in Flying Fish - Ring galaxy AM 0644 - 741 in Volans - The annular galaxy AM 0644 - 741 is about 300 million years away - light from Earth. A collision with another galaxy causes its ring shape. This ring extends over 150,000 years - light and is composed of recently formed and extremely bright blue stars. Image obtained by the Hubble Space Telescope in January 2004. This galaxy, cataloged as AM 0644 - 741, is a member of the class of so - called “” ring galaxies.”” It lies 300 million light - years away in the direction of the southern constellation Volans. Ring galaxies are an especially striking example of how collisions between galaxies can dramatically change their structure, while also triggering the formation of new stars. In the case of AM 0644 - 741, the galaxy that pierced through the ring galaxy is out of the image but visible in larger - field images. The soft spiral galaxy that is visible to the left of the ring galaxy in the image is a coincidental ba

Galaxy AM 0644 - 741 in Flying Fish - Ring galaxy AM 0644 - 741 in Volans - The annular galaxy AM 0644 - 741 is about 300 million years away - light from Earth. A collision with another galaxy causes its ring shape. This ring extends over 150,000 years - light and is composed of recently formed and extremely bright blue stars. Image obtained by the Hubble Space Telescope in January 2004. This galaxy, cataloged as AM 0644 - 741, is a member of the class of so - called “” ring galaxies.”” It lies 300 million light - years away in the direction of the southern constellation Volans. Ring galaxies are an especially striking example of how collisions between galaxies can dramatically change their structure, while also triggering the formation of new stars. In the case of AM 0644 - 741, the galaxy that pierced through the ring galaxy is out of the image but visible in larger - field images. The soft spiral galaxy that is visible to the left of the ring galaxy in the image is a coincidental ba

PIX4613542

Constellations of Flying Fish and Painter - Constellations of Volans and Pictor - The Flying Fish is a small constellation of the southern hemisphere. The bright star on its right is Canopus. Under Canopus, the constellation of the Painter

Constellations of Flying Fish and Painter - Constellations of Volans and Pictor - The Flying Fish is a small constellation of the southern hemisphere. The bright star on its right is Canopus. Under Canopus, the constellation of the Painter

Christopher Picking

PIX4593444

Spiral galaxy NGC 488 in Pisces - Spiral galaxy NGC 488 in Pisces - NGC 488 is a spiral galaxy located about 90 million years ago - light from Earth in the constellation Pisces. Spiral galaxy located at about 90 million light - years away in Pisces

Spiral galaxy NGC 488 in Pisces - Spiral galaxy NGC 488 in Pisces - NGC 488 is a spiral galaxy located about 90 million years ago - light from Earth in the constellation Pisces. Spiral galaxy located at about 90 million light - years away in Pisces

Adam Block

PIX4609206

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

PIX4610013

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

PIX4591661

Astrology: representation of the sign of the fish. Page of the manuscript Physiognomia (Liber physiognomiae) (ms. 697) by Michael Scotus (or Scot) (1170-1236). Biblioteca estense, Modene, Italy.

Astrology: representation of the sign of the fish. Page of the manuscript Physiognomia (Liber physiognomiae) (ms. 697) by Michael Scotus (or Scot) (1170-1236). Biblioteca estense, Modene, Italy.

Marco Ravenna

VEN5027469

Collision galaxy NGC 520 - Galaxy NGC 520 in Pisces - The galaxy NGC 520, is about 100 million light years away from Earth in the constellation Pisces. This system consists of two colliding galaxies. The merger started 300 million years ago. The two galaxies are only in the middle of this process, their disk having merged but not yet their kernel. NGC 520 is among the brightest pairs of galaxies, and is visible with a small telescope. NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It examplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd - looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescope towards the constellation of Pisces, the Fish, having the appear

Collision galaxy NGC 520 - Galaxy NGC 520 in Pisces - The galaxy NGC 520, is about 100 million light years away from Earth in the constellation Pisces. This system consists of two colliding galaxies. The merger started 300 million years ago. The two galaxies are only in the middle of this process, their disk having merged but not yet their kernel. NGC 520 is among the brightest pairs of galaxies, and is visible with a small telescope. NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It examplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd - looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescope towards the constellation of Pisces, the Fish, having the appear

Adam Block

PIX4609250

Constellation of Pisces - Constellation of Pisces - Composite of two images. The sky is enlarged in relation to reality. Constellation of Pisces. Composite image. Stars are bigger than in reality

Constellation of Pisces - Constellation of Pisces - Composite of two images. The sky is enlarged in relation to reality. Constellation of Pisces. Composite image. Stars are bigger than in reality

B&S.Fletcher

PIX4593482

Horoscope (Pisces), 2017 (lino print)

premium — Horoscope (Pisces), 2017 (lino print)

Horoscope (Pisces), 2017 (lino print)

Morrocco, Annalisa (b.1950)

NAL6290156

Collision galaxy NGC 520 - Galaxy NGC 520 in Pisces - The galaxy NGC 520, is about 100 million light years away from Earth in the constellation Pisces. This system consists of two colliding galaxies. The merger started 300 million years ago. The two galaxies are only in the middle of this process, their disk having merged but not yet their kernel. NGC 520 is among the brightest pairs of galaxies, and is visible with a small telescope. Image obtained by the Hubble Space Telescope on October 22, 2004. NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It examplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd - looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescop

Collision galaxy NGC 520 - Galaxy NGC 520 in Pisces - The galaxy NGC 520, is about 100 million light years away from Earth in the constellation Pisces. This system consists of two colliding galaxies. The merger started 300 million years ago. The two galaxies are only in the middle of this process, their disk having merged but not yet their kernel. NGC 520 is among the brightest pairs of galaxies, and is visible with a small telescope. Image obtained by the Hubble Space Telescope on October 22, 2004. NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It examplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd - looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescop

PIX4609218

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. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This picture of the Meathook Galaxy (NGC 2442) was taken by the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla, Chile. This view includes the whole galaxy and the surrounding sky, and clearly shows the asymmetric spiral arms. The longer of the two arms has intense star formation, which is visible here as a pink glow: this is due to the radiation of young stars ionising the gas they form from. The asymmetric shape and star formation are both thought to be caused by tidal disruptions from a near - miss with another galaxy at some point in its history

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. Image obtained by the 2.2 meter MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This picture of the Meathook Galaxy (NGC 2442) was taken by the Wide Field Imager on the MPG/ESO 2.2 - metre telescope at La Silla, Chile. This view includes the whole galaxy and the surrounding sky, and clearly shows the asymmetric spiral arms. The longer of the two arms has intense star formation, which is visible here as a pink glow: this is due to the radiation of young stars ionising the gas they form from. The asymmetric shape and star formation are both thought to be caused by tidal disruptions from a near - miss with another galaxy at some point in its history

PIX4610133

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

Flying Fish Constellation - Constellation of Volans - Flying Fish is a small constellation in the southern hemisphere. The bright star on its left is Miaplacidus, in Carene. Volans was introduced by Johann Bayer in 1603 as Piscis Volans, the Flying Fish and in old star atlases is seen flying alongside the ancient sailing ship Argo Navis. However, the fish has flown and only the adjective Volans (flying) remains. The stars form a distinctive pattern but at magnitudes between 3.7 and 4.0 they are not bright. On the other hand the constellation is easily found between the bright stars Avior (epsilon Carinae) and Miaplacidus (beta Carinae) with the fish apparently flying towards the LM

PIX4593478

Pisces (w/c on paper)

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Pisces (w/c on paper)

Bradbury, Catherine

CBB118691

Add. 17367, f.3r Aquarius & Pisces, from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)

Add. 17367, f.3r Aquarius & Pisces, from Almanac, containing table of dominical letters and golden numbers; directions to find the movable feasts; calendar of Saints, epochs, list of English Sovereigns, prognostications of weather, influence of the signs of the zodiac (vellum)

English School, (16th century)

BL5053987

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 and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

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 and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

PIX4610093

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

Pisces Constellation - Constellation of Pisces - Pisces (the Fishes) is a large constellation of mostly quite faint stars at the edge of an ancient and huge part of the sky known as 'the Sea'. Pisces is said to resemble two fish, which are tied to a (alpha) Piscium by long lines. Alpha Piscium is known as Al Rischa in English, where it means 'the cord'. Some Greek mythologies have two men tethered to this star, though some of the other stars have fishy names. The Sun is in Pisces from March 13 to April 19, and it crosses the ecliptic on March 21, which marks the vernal Equinox, the first day of autumn in the southern hemisphere. This used to be called the first point in Aries, but precession has now moved it into Pisces. However, this point in the sky is the origin of right ascension (RA) in the astronomical equatorial coordinate sytem, and because it moves with precession, RA and Dec are defined at a certain date

PIX4593517

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - This galaxy measures about 80,000 years - light and is 30 million years away - light. Image obtained with a 50 cm telescope, composite of several poses. M74 is located roughly 30 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky Way. Its perfectly symmetrical spiral arms emanate from the central nucleus and are dotted with clusters of young blue stars and glowing pink regions of ionized hydrogen (hydrogen atoms that have lost their electrons). These regions of star formation show an excess of light at ultraviolet wavelengths. Tracing along the spiral arms are winding dust lanes that also begin very near the galaxy's nucleus and follow along the length of the spiral arms

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - This galaxy measures about 80,000 years - light and is 30 million years away - light. Image obtained with a 50 cm telescope, composite of several poses. M74 is located roughly 30 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky Way. Its perfectly symmetrical spiral arms emanate from the central nucleus and are dotted with clusters of young blue stars and glowing pink regions of ionized hydrogen (hydrogen atoms that have lost their electrons). These regions of star formation show an excess of light at ultraviolet wavelengths. Tracing along the spiral arms are winding dust lanes that also begin very near the galaxy's nucleus and follow along the length of the spiral arms

R. Jay GaBany

PIX4609387

Shooting star rain - Perseides - Milky Way and Perseid meteors - Shooting star rain of the Perseid swarm seen at the wide angle on August 13, 2015. The Perseides are a rain of shooting stars associated with the comet Swift-Tuttle. Meteors as appeared in the sky during the peak hours of 2015 Perseid Meteor Shower

Shooting star rain - Perseides - Milky Way and Perseid meteors - Shooting star rain of the Perseid swarm seen at the wide angle on August 13, 2015. The Perseides are a rain of shooting stars associated with the comet Swift-Tuttle. Meteors as appeared in the sky during the peak hours of 2015 Perseid Meteor Shower

Sebastian Voltmer

PIX4599048

Star sky and Gegenschein - Gegenschein - View of Gegenschein in the constellation Pisces. Gegenschein is a very low glow created by the reflection of the sun's light on dust particles. The planet Uranus is also present in this image obtained on September 20, 2009. The Gegenschein, or counterglow, is visible here, just below the center of the image and to the lower left of the circlet of Pisces. It can be seen as a large diffuse oval area of very faint light just above the brightness of the sky background. The planet Uranus also happened to be located in the Gegenschein when the image was taken. Very faint extensions, called the Zodiacal Bridge, or Zodiacal Bands, connect the Gegenschein to the Zodiacal Light along the ecliptic. The Zodiacal light and Gegenschein are made of very small particles of dust that orbit the Sun in the plane of the Ecliptic. These particles are created by asteroid collisions and comets. The Gegenschein is at the anti-solar point, directly opposite the Sun in t

Star sky and Gegenschein - Gegenschein - View of Gegenschein in the constellation Pisces. Gegenschein is a very low glow created by the reflection of the sun's light on dust particles. The planet Uranus is also present in this image obtained on September 20, 2009. The Gegenschein, or counterglow, is visible here, just below the center of the image and to the lower left of the circlet of Pisces. It can be seen as a large diffuse oval area of very faint light just above the brightness of the sky background. The planet Uranus also happened to be located in the Gegenschein when the image was taken. Very faint extensions, called the Zodiacal Bridge, or Zodiacal Bands, connect the Gegenschein to the Zodiacal Light along the ecliptic. The Zodiacal light and Gegenschein are made of very small particles of dust that orbit the Sun in the plane of the Ecliptic. These particles are created by asteroid collisions and comets. The Gegenschein is at the anti-solar point, directly opposite the Sun in t

Jerry Lodriguss

PIX4581436

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its eclat was decreasing (box). Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its br

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its eclat was decreasing (box). Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its br

PIX4610028

Virgo-Pisces, 2009 (mixed media)

premium — Virgo-Pisces, 2009 (mixed media)

Virgo-Pisces, 2009 (mixed media)

SAB361659

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. M74 (NGC 628) is located roughly 30 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky Way

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. M74 (NGC 628) is located roughly 30 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky Way

R. Gendler

PIX4609396

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns. Thirty six, fifteen minute photographs were combined to create this picture, with a total exposure time of almost nine hours. The images were taken with a

R. Jay GaBany

PIX4609403

The Oyster's Chief Enemy (engraving)

The Oyster's Chief Enemy (engraving)

English School, (20th century)

LLM5209674

Woman and Starfish, 1989 (oil on canvas)

premium — Woman and Starfish, 1989 (oil on canvas)

Woman and Starfish, 1989 (oil on canvas)

PEW347755

Asterias Papposa or Twelve rayed Star Fish, from 'Zoological lectures delivered at the Royal institution in the years 1806 and 1807' by George Shaw, 1809 (engraving)

Asterias Papposa or Twelve rayed Star Fish, from 'Zoological lectures delivered at the Royal institution in the years 1806 and 1807' by George Shaw, 1809 (engraving)

English School, (19th century)

XOS4429273

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628). This galaxy is about 80,000 light years and is 30 million light years apart. Viewed face on, as it appeared about 30 million years ago, M74 is considered to be one of the most photogenic spiral galaxies in the sky. The galaxy is rich in young bright blue stars and glowing red regions of dust and molecular hydrogen where new stars are being created. M74, however, is quite camera shy - it has a low surface brightness that makes it challenging for both visual observers and astrophotographers to see it's entire form. The Chandra X - Ray observatory, discovered M74 to be the home of a super massive black hole, tucked away in one of it's outer arms. This black hole is one of the largest ever discovered and has the mass of over 10,000 suns

Adam Block

PIX4609424

Region around the spiral galaxy M74 in Pisces - Region of sky around the spiral galaxy M74 in Pisces - An image of the region of sky around M74, from the Digitized Sky Survey 2. The field - of - view is approximately 2.8 x 2.8 degrees

Region around the spiral galaxy M74 in Pisces - Region of sky around the spiral galaxy M74 in Pisces - An image of the region of sky around M74, from the Digitized Sky Survey 2. The field - of - view is approximately 2.8 x 2.8 degrees

PIX4609416

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

Constellations of Grus and Piscis Austrinus - The Crane is a constellation in the southern hemisphere, located just below the Southern Fish. Grus (the Crane) is meant to represent a water bird, which may be a crane or perhaps a flamingo. This stellar grouping was introduced by Johann Bayer in his star atlas of 1603. Because of its location in the southern sky it is not visible from north latitudes above 40 degrees. Even if it were visible, it would hardly be remarked upon. Piscis Austrinus (the Southern Fish) once included Grus, and nowadays represents the Southern Fish, drinking from the water poured by Aquarius, adjoining it to the north. Piscis Austrinus was one of Ptolemy's 48 constellations and its brightest star is Fomalhaut, a name drived from the English for fish's mouth

PIX4591663

Constellation of Fish - Constellation of Pisces - Plate extracted from the Mirror of Urania by Jehoshaphat Aspin - 1825 Urania's Mirror, by Jehoshaphat Aspin, 1825

Constellation of Fish - Constellation of Pisces - Plate extracted from the Mirror of Urania by Jehoshaphat Aspin - 1825 Urania's Mirror, by Jehoshaphat Aspin, 1825

PIX4593504

The Last Supper, c.1930-1940 (illustration)

The Last Supper, c.1930-1940 (illustration)

French School, (20th century)

CCI1935937

The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees

The star Fomalhaut - Star Fomalhaut - The star Fomalhaut is located 25 years - light from Earth in the constellation Southern Fish. An extrasolar planet, called Fomalhaut b, with a mass close to Jupiter, is in orbit around it. This image shows Fomalhaut, the star around which the discovered planet Fomalhaut b orbits. Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. It is blazing through hydrogen at such a furious rate that it will burn out in only one billion years, 10% the lifespan of our star. The field of view is 2.7 x 2.9 degrees

PIX4571995

Huelgoat Forest - Finistere - Huelgoat Forest, Brittany - Huelgoat Forest in winter. Circular panorama. 30 January 2010. Huelgoat forest in winter. Composite fisheye view. Brittany, France. January 30, 2010

Huelgoat Forest - Finistere - Huelgoat Forest, Brittany - Huelgoat Forest in winter. Circular panorama. 30 January 2010. Huelgoat forest in winter. Composite fisheye view. Brittany, France. January 30, 2010

Laurent Laveder

PIX4667588

February, The Fish, 1898 (colour litho)

February, The Fish, 1898 (colour litho)

Meunier, Henri Georges Jean Isidore (1873-1922)

BST2822873

Aquarius Constellations, Capricorn, Austral Fish and Microscope - Constellations of Aquarius, Capricorn, Piscis Austrinus, Microscopium - Field around the Aquarius constellation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best s

Aquarius Constellations, Capricorn, Austral Fish and Microscope - Constellations of Aquarius, Capricorn, Piscis Austrinus, Microscopium - Field around the Aquarius constellation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best s

PIX4594319

Constellation of Pisces - Constellation of Pisces - The constellation of Pisces extracted from the Uranographia of Hevelius. Recolorised image. Map showing the constellation of Pisces with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Constellation of Pisces - Constellation of Pisces - The constellation of Pisces extracted from the Uranographia of Hevelius. Recolorised image. Map showing the constellation of Pisces with its mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Sebastien Beaucourt

PIX4593526

The Basket-Fish, a Star-Fish which climbs up coral-branches (chromolitho)

The Basket-Fish, a Star-Fish which climbs up coral-branches (chromolitho)

English School, (20th century)

LLM5206753

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

Aquarius Constellation - Constellation of Aquarius - Field around the Aquarius constelllation. The Helix planetary nebula appears as a red dot towards the center of the image. Aquarius (The Water Carrier) is a large but relatively insconspicuous southern zodiacal constellation and has an area of about 980 square degrees, which makes it the 10th largest. Its origins as a constellation can be traced back to Babylonian times and has usually been delineated as a figure pouring water from a jar in the general direction of Capricornus and Piscis Austrinus, themselves quite watery constellations. The Sun is in this part of the sky in February and March, following the Ecliptic. The constellation embraces many objects of telescopic interest, including the Helix nebula and the Mira - like variable star R Aquarii. Also notable are the globular clusters M2 (NGC 7089) and the Saturn planetary nebula NGC 7009. Best seen in the early evening in August

PIX4594337

Cerro Tololo Observatory: The Lactee Way above the Cerro Tololo Observatory, Chile. Milky Way above the 4 meter Blanco telescope and small telescopes in Cerro Tololo observatory, Chile

Cerro Tololo Observatory: The Lactee Way above the Cerro Tololo Observatory, Chile. Milky Way above the 4 meter Blanco telescope and small telescopes in Cerro Tololo observatory, Chile

Alex Tudorica

PIX4652916

Constellation of Pisces - Constellation of Pisces - Map of the constellation of Pisces with its main celestial objects. The Great Bear is indicated for the scale. Map showing the constellation of Pisces with its main celestial objects. Constellation of Big Dipper is shown at scale

Constellation of Pisces - Constellation of Pisces - Map of the constellation of Pisces with its main celestial objects. The Great Bear is indicated for the scale. Map showing the constellation of Pisces with its main celestial objects. Constellation of Big Dipper is shown at scale

Sebastien Beaucourt

PIX4593522

The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist

The star Fomalhaut and its dust disc - Star Fomalhaut dust ring - The star Fomalhaut is located 25 years - light from Earth in the constellation of the Southern Fish. A dust disc surrounds it, seen here by the Hubble telescopes (left), Herschel (far infrared, centre) and Alma (right). This disc of interplanetary dust revolves around the young star at a distance of about 20 billion kilometers from it. The image taken at 850 microns wavelength by Alma seems to confirm that the planet discovered in 2008 in the Fomalhaut disc by Hubble does not exist. This image shows Fomalhaut and its dust ring. Images taken by the Hubble space telescope (HST, at left), Herschel telescope (middle) and Alma telescope (at right). Fomalhaut is much hotter than our Sun, 15 times as bright, and lies 25 light - years from Earth. An exoplanet was discovered in its dust ring but Alma observations seem to prove this planet doesn't exist

PIX4571988

Spiral galaxy M74 - UV composite - visible - Spiral galaxy M74 in visible and UV - Image of the spiral galaxy M74 (NGC 628) made by Astro satellite - 1. This galaxy is about 80,000 light years and is 30 million light years apart. In this composite image the visible light is in red, in blue the ultraviolet light. Located in the constellation of Pisces the Fish, the telescopic object Messier 74 is one of the finest examples of a giant spiral galaxy seen nearly face - on. In this composite image of M74, the visible - light emission is represented in red, while the UV emission is shown in blue - white tints. Newborn hot stars and associated nebulosity dominate the near - UV emission. The concentration of this starbirth activity along the spiral arms is indicative of global dynamic processes at work. M74 estimated distance is 24 million light years

Spiral galaxy M74 - UV composite - visible - Spiral galaxy M74 in visible and UV - Image of the spiral galaxy M74 (NGC 628) made by Astro satellite - 1. This galaxy is about 80,000 light years and is 30 million light years apart. In this composite image the visible light is in red, in blue the ultraviolet light. Located in the constellation of Pisces the Fish, the telescopic object Messier 74 is one of the finest examples of a giant spiral galaxy seen nearly face - on. In this composite image of M74, the visible - light emission is represented in red, while the UV emission is shown in blue - white tints. Newborn hot stars and associated nebulosity dominate the near - UV emission. The concentration of this starbirth activity along the spiral arms is indicative of global dynamic processes at work. M74 estimated distance is 24 million light years

PIX4609373

Star Fish

Star Fish

UIG2902131

Snowflake star or Common sunstar (Crossaster papposus), Solasteridae, Artwork by Rebecca Hardy

Snowflake star or Common sunstar (Crossaster papposus), Solasteridae, Artwork by Rebecca Hardy

DGA1141781

Aurora boreale en Norway - Aurora in Norway - Aurora boreale observed in Norway. 1 December 2011. Aurora Explosion Dec. 1st 2011 Kirkenes, Sollia, Norwa

Aurora boreale en Norway - Aurora in Norway - Aurora boreale observed in Norway. 1 December 2011. Aurora Explosion Dec. 1st 2011 Kirkenes, Sollia, Norwa

Sebastian Voltmer

PIX4670154

Constellations of Crane and Southern Fish - Constellations of Grus and Piscis Austrinus - Constellations of Crane and Southern Fish extracted from Hevelius Uranographia. Recolorised image. Map showing the constellations of Grus and Piscis Austrinus with their mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Constellations of Crane and Southern Fish - Constellations of Grus and Piscis Austrinus - Constellations of Crane and Southern Fish extracted from Hevelius Uranographia. Recolorised image. Map showing the constellations of Grus and Piscis Austrinus with their mythological form from “” Uranographia”” star atlas by Hevelius (1690). Recolored Image

Sebastien Beaucourt

PIX4591671

Turbot (Scophthalmus maximus or Psetta maxima), Scophthalmidae, drawing

Turbot (Scophthalmus maximus or Psetta maxima), Scophthalmidae, drawing

DGA1262128

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628) obtained by the Hubble space telescope in 2003 and 2005. This galaxy is about 80,000 light years and is approximately 30 million light years apart. This image shows in detail the arms of this galaxy or nebulae and clusters of young stars appear in numbers. NASA/ESA Hubble Space Telescope image of the nearby spiral galaxy M74 (NGC 628), is a composite of Advanced Camera for Surveys' data taken in 2003 and 2005. A small segment of this image used data from the Canada - France - Hawaii Telescope and the Gemini Observatory to fill in a region that Hubble did not image. M74 is located roughly 32 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky W

Spiral galaxy M74 in Pisces - Spiral galaxy M74 in Pisces - Image of the spiral galaxy M74 (NGC 628) obtained by the Hubble space telescope in 2003 and 2005. This galaxy is about 80,000 light years and is approximately 30 million light years apart. This image shows in detail the arms of this galaxy or nebulae and clusters of young stars appear in numbers. NASA/ESA Hubble Space Telescope image of the nearby spiral galaxy M74 (NGC 628), is a composite of Advanced Camera for Surveys' data taken in 2003 and 2005. A small segment of this image used data from the Canada - France - Hawaii Telescope and the Gemini Observatory to fill in a region that Hubble did not image. M74 is located roughly 32 million light - years away in the direction of the constellation Pisces, the Fish. It is the dominant member of a small group of about half a dozen galaxies, the M74 galaxy group. In its entirety, it is estimated that M74 is home to about 100 billion stars, making it slightly smaller than our Milky W

PIX4609405

Life on an exoplanet: View of an alien life artist on the surface of an exoplanet. Extraterrestrial life on an exoplanet

Life on an exoplanet: View of an alien life artist on the surface of an exoplanet. Extraterrestrial life on an exoplanet

Miller, Ron (b.1947)

PIX4607759

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