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Images of 'NASA' found, 8,704

 
Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

PIX4629885

Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

PIX4629885

 
Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

PIX4629935

Terre Lune et Soleil - artist view - Earth Moon and Sun - Artwork

PIX4629935

 
Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

PIX4630564

Traces of the impact crater Chicxulub - Chicxulub impact crater - Excessive relief view of the Yucatan peninsula obtained from radar altimetric data acquired by the SRTM instrument aboard the space shuttle Endeavour in 2000. An arc of circle is visible to the north-west of the peninsula, marking the outer edge of the Chicxulub impact crater whose centre is located off the Mexican coast. This meteorite impact would have caused the disappearance of dinosaurs 65 million years ago. This shaded relief image of Mexico's Yucatan Peninsula show a subtle, but unmistakable, indication of the Chicxulub impact crater. Most scientists now agree that this impact was the cause of the Cretatious - Tertiary Extinction, the event 65 million years ago that marked the sudden extinction of the dinosaurs as well as the majority of life then on Earth. Most of the peninsula is visible here, along with the island of Cozumel off the east coast. The Yucatan is a plateau composed mostly of limestone and is an are

PIX4630564

 
Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

PIX4622792

Neptune seen by Voyager 2 1989 - Image of Neptune obtained by the Voyager 2 probe at 16 million km from the planet. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. On this photo, on the left, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, a small shiny cloud of irregular shape moving very quickly, nicknames the scooter

PIX4622792

 
Neptune seen by Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 20, 1989. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. In this photo, in the centre, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, on the left, a small cloud of irregular shape moving very quickly, nicknamed the scooter

PIX4622802

Neptune seen by Voyager 2 - Image of Neptune obtained by the Voyager 2 probe on August 20, 1989. Neptune has an equatorial diameter of about 49,000 kilometres. Its blue color is due to the abundance of methane in its atmosphere. In this photo, in the centre, the Great Dark Spot, which is the size of the Earth where winds are blowing at 300 m/s. This spot has now disappeared but other dark spots have been detected since then. Under the Great Dark Spot, on the left, a small cloud of irregular shape moving very quickly, nicknamed the scooter

PIX4622802

 
Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

PIX4621980

Detail nebuleuse de la Tete de Cheval by HST - The Horsehead, also known as Barnard 33, is a cold, dark cloud of gas and dust, silhouetted against the bright nebula, IC 434. The bright area at the top left edge is a young star still embedded in its nursery of gas and dust. Radiation from this hot star is eroding its gaseous birthplace. A massive star located outside Hubble's view is, in a similar fashion, sculpting the top of the Horsehead itself. The Horsehead, located in the constellation Orion, is a cousin of the famous pillars of dust and gas known as the Eagle nebula. Both tower - like nebulae are cocoons of young stars. The Horsehead nebula lies just south of the bright star Zeta Orionis, which is easily visible to the unaided eye as the left - hand star in the line of three that form Orion's Belt. Amateur astronomers often use the Horsehead as a test of their observing skills - it is known as one of the more difficult objects to observe visually with an amateur - sized telescope

PIX4621980

 
Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

PIX4623115

Planetary nebula NGC 5189 in the fly - This nebula is located about 3000 light years from Earth in the southern constellation of the fly. Image obtained by the Gemini and Hubble telescopes (HST). NGC 5189 is a planetary nebula. At the end of its life, a star with a mass less than eight times that of the Sun will blow its outer layers away, giving rise to a planetary nebula. Some of these stellar puffballs are almost round, resembling huge soap bubbles or giant planets (hence the name), but others, such as NGC 5189 are more intricate. In particular, this planetary nebula exhibits a curious S” - shaped profile, with a central bar that is most likely the projection of an inner ring of gas discharged by the star, seen edge on. The details of the physical processes producing such a complex symmetry from a simple, spherical star are still the object of astronomical controversy. One possibility is that the star has a very close (but unseen) companion. Over time the orbits drift due to precess

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Saturn and satellites seen by Voyager - Saturn system montage - Mounting made from the photos obtained by the Voyager 1 and 2 probes showing Saturn accompanied by its satellites. Enceladus is the largest satellite on the image, then clockwise we find Dione, Rhea, Titan (top right), Japet, Tethys, and Mimas. This montage of images of the Saturnian system was prepared from an assemblage of images taken by the Voyager 1 and 2 spacecrafts during their Saturn encounter. The large satellite at left is Enceladus, followed in clockwise order by Dione, Rhea, Titan (in top right corner), Iapetus, Tethys, & Mimas

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Saturn and satellites seen by Voyager - Saturn system montage - Mounting made from the photos obtained by the Voyager 1 and 2 probes showing Saturn accompanied by its satellites. Enceladus is the largest satellite on the image, then clockwise we find Dione, Rhea, Titan (top right), Japet, Tethys, and Mimas. This montage of images of the Saturnian system was prepared from an assemblage of images taken by the Voyager 1 and 2 spacecrafts during their Saturn encounter. The large satellite at left is Enceladus, followed in clockwise order by Dione, Rhea, Titan (in top right corner), Iapetus, Tethys, & Mimas

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Hurricanes Katia, Irma, and Jose seen by satellite 09/2017 - Hurricanes Katia, Irma, and Jose 09/2017: Hurricanes Katia, Irma, and Jose seen by the Suomi NPP satellite on September 8, 2017. The Visible Infrared Imaging Radiometer Suite (VIIS) on the Suomi NPP satellite captured the data for a mosaic of Katia, Irma, and Jose as they appeared in the early hours of September 8, 2017. The images were acquired by the VIIRS “” day-night band,””” which detects light signals in a range of wavelengths from green to near-infrared, and uses filtering techniques to observe signals such as city lights, auroras, wildfires, and reflected moonlight. In this case, the clouds were lit by the nearly full Moon. The image is a composite, showing cloud imagery combined with data on city lights

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Hurricanes Katia, Irma, and Jose seen by satellite 09/2017 - Hurricanes Katia, Irma, and Jose 09/2017: Hurricanes Katia, Irma, and Jose seen by the Suomi NPP satellite on September 8, 2017. The Visible Infrared Imaging Radiometer Suite (VIIS) on the Suomi NPP satellite captured the data for a mosaic of Katia, Irma, and Jose as they appeared in the early hours of September 8, 2017. The images were acquired by the VIIRS “” day-night band,””” which detects light signals in a range of wavelengths from green to near-infrared, and uses filtering techniques to observe signals such as city lights, auroras, wildfires, and reflected moonlight. In this case, the clouds were lit by the nearly full Moon. The image is a composite, showing cloud imagery combined with data on city lights

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Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

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Seyfert's Sextet Group of Galaxies in the Snake - Seyfert's Sextet group of galaxies - This group of interacting galaxies resides approximately 190 million years ago - light in the constellation of the Snake and extends over 100,000 years - light. The small spiral galaxy seen from the front does not belong to this group. The small face - on spiral with the prominent arms [center] of gas and stars is a background galaxy almost five times farther away than the other four. Only a chance alignment makes it appear as if it is part of the group. The sixth member of the sextet isn't a galaxy at all but a long “” tidal tail””” of stars [below, right] torn from one of the galaxies. The group resides 190 million light - years away in the constellation Serpens. This densely packed grouping spans just 100,000 light - years, occupying less volume than the Milky Way galaxy. Each galaxy is about 35,000 light - years wide. Three of the galaxies [the elliptical galaxy, second from top, and the two spir

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Palm islands, Dubai 10/2002 - Palm islands, artificial islands built on the coast of the Emirates of Dubai. False colour image obtained by the Terra satellite in October 2002. The vegetation appears in red, the water in dark blue, the constructions in light blue or grey, the desert in beige. This image, acquired in October 2002 by Terra satellite, shows the early stages of Palm Jumeirah, also known as The Palm”” in Dubai. The circular outline of the archipelago is largely completed, and the palm fronds are beginning to take shape. Inland, cityscape begins to push eastward into the desert, with a combination of roads and buildings. The conspicuously vegetated area southeast of Palm Jumeirah is a golf course. East of this course, however, the land is mostly undeveloped desert. In this false - color image, bare ground appears light brown, vegetation appears red, water appears dark blue, and buildings and paved surfaces appear light blue or gray. The United Arab Emirates falls within the E

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Palm islands, Dubai 10/2002 - Palm islands, artificial islands built on the coast of the Emirates of Dubai. False colour image obtained by the Terra satellite in October 2002. The vegetation appears in red, the water in dark blue, the constructions in light blue or grey, the desert in beige. This image, acquired in October 2002 by Terra satellite, shows the early stages of Palm Jumeirah, also known as The Palm”” in Dubai. The circular outline of the archipelago is largely completed, and the palm fronds are beginning to take shape. Inland, cityscape begins to push eastward into the desert, with a combination of roads and buildings. The conspicuously vegetated area southeast of Palm Jumeirah is a golf course. East of this course, however, the land is mostly undeveloped desert. In this false - color image, bare ground appears light brown, vegetation appears red, water appears dark blue, and buildings and paved surfaces appear light blue or gray. The United Arab Emirates falls within the E

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Volcano Paluweh, Indonesia - Paluweh Volcano - Indonesia - Smoke escapes from the stratovolcano Rokatenda, also called Paluweh, on this image obtained by the satellite Landsat-8 on April 29, 2013. This volcano of Indonesia is located in the small islands of the Prode, on the island of Palu'e, north of Flores. An ash plume drifts from Paluweh volcano in Indonesia in this image, taken April 29, 2013 from the Landsat-8 satellite. Rokatenda (Paluweh) volcano is a stratovolcano located in the northern region of Palu'e, north of Flores Island. The volcano erupted on August 10, 2013

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Volcano Paluweh, Indonesia - Paluweh Volcano - Indonesia - Smoke escapes from the stratovolcano Rokatenda, also called Paluweh, on this image obtained by the satellite Landsat-8 on April 29, 2013. This volcano of Indonesia is located in the small islands of the Prode, on the island of Palu'e, north of Flores. An ash plume drifts from Paluweh volcano in Indonesia in this image, taken April 29, 2013 from the Landsat-8 satellite. Rokatenda (Paluweh) volcano is a stratovolcano located in the northern region of Palu'e, north of Flores Island. The volcano erupted on August 10, 2013

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North pole by satellite - September 9, 2008 - Arctic sea ice - September 9, 2008 - Arctic ice coverage September 9, 2008. Image based on data obtained by the Aqua satellite. This image shows the sea ice that occurred on September 9, 2008. Sea ice is frozen seawater floating on the surface of the ocean. Some sea ice is semi-permanent, persisting from year to year, and some is seasonal, melting and refreezing from season to season. The sea ice cover reaches its minimum extent at the end of each summer and the remaining ice is called the perennial ice cover. Image made from Aqua satellite instrument

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North pole by satellite - September 9, 2008 - Arctic sea ice - September 9, 2008 - Arctic ice coverage September 9, 2008. Image based on data obtained by the Aqua satellite. This image shows the sea ice that occurred on September 9, 2008. Sea ice is frozen seawater floating on the surface of the ocean. Some sea ice is semi-permanent, persisting from year to year, and some is seasonal, melting and refreezing from season to season. The sea ice cover reaches its minimum extent at the end of each summer and the remaining ice is called the perennial ice cover. Image made from Aqua satellite instrument

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New York view from space - New York City seen from space - New York, with Manhattan Island in the center of the image, seen by Terra satellite on 8 September 2002. This image taken by satellite Terra shows New York City and the Island of Manhattan, bordered by the Hudson and East Rivers. Parts of Long Island and Staten Island are also visible. Two of New York's major airports (Newark and La Guardia) are within the image. In the middle of Manhattan, Central Park appears as a long green rectangle with a large lake in the middle. The image covers an area of 27 x 37 km, and was acquired September 8, 2002, and is located at 40.7 degrees north latitude and 74 degrees west longitude

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New York view from space - New York City seen from space - New York, with Manhattan Island in the center of the image, seen by Terra satellite on 8 September 2002. This image taken by satellite Terra shows New York City and the Island of Manhattan, bordered by the Hudson and East Rivers. Parts of Long Island and Staten Island are also visible. Two of New York's major airports (Newark and La Guardia) are within the image. In the middle of Manhattan, Central Park appears as a long green rectangle with a large lake in the middle. The image covers an area of 27 x 37 km, and was acquired September 8, 2002, and is located at 40.7 degrees north latitude and 74 degrees west longitude

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Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

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Satellite Orbiting Carbon Observatory - Artist's concept of the Orbiting Carbon Observatory - Artist's view of the Orbiting Carbon Observatory (OCO) satellite orbiting Earth. This satellite, scheduled to launch in early 2009, will be dedicated exclusively to the study of carbon dioxide on Earth. The mission, scheduled to launch in early 2009, will be the first spacecraft dedicated to studying atmospheric carbon dioxide, the main human - produced driver of climate change. It will provide the first global picture of the human and natural sources of carbon dioxide and the places where this important greenhouse gas is stored. Such information will improve global carbon cycle models as well as forecasts of atmospheric carbon dioxide levels and of how our climate may change in the future

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Urangan Irene - August 26, 2011 - Hurricane Irene - August 26, 2011 - Hurricane Irene on the eastern coast of the United States seen by the GOES-13 meteorological satellite on August 26, 2011. Irene, the first hurricane of the 2011 Atlantic season, was poised on August 26 to be the first to make landfall in the United States since 2008. More than 50 million people were estimated to lie within the path of the storm as it headed towards the major U.S. population centers of Norfolk, Washington, Baltimore, Philadelphia, New York, and Boston

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Urangan Irene - August 26, 2011 - Hurricane Irene - August 26, 2011 - Hurricane Irene on the eastern coast of the United States seen by the GOES-13 meteorological satellite on August 26, 2011. Irene, the first hurricane of the 2011 Atlantic season, was poised on August 26 to be the first to make landfall in the United States since 2008. More than 50 million people were estimated to lie within the path of the storm as it headed towards the major U.S. population centers of Norfolk, Washington, Baltimore, Philadelphia, New York, and Boston

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Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

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Umnak Island - Aleutian Islands - Alaska - Umnak Island - Aleutian Islands - Alaska: Umnak Island is one of the Fox Islands, belonging to the Aleutian Islands in Alaska, USA. With an area of more than 1,776 km, it is the third largest of the Aleutian Islands. At the top right is the Okmok caldera (erupted in 2008), below the Vsevidof volcano; below the left, the Ile des Quatre Montagnes. Image obtained on 3 May 2014 by the Landsat-8 satellite. On May 3, 2014, the Landsat 8 satellite acquired this natural-color image of Umnak Island and its volcanic neighbors in the Aleutian Island chain. Part of the Fox Islands, Umnak is the third largest in the Aleutian chain and lies just southwest of Unalaska. Umnak is mostly unpopulated, with roughly 40 people living in the village of Nikolski near the southwest tip of the island. Being a volcanic island, Umnak has numerous mud pots, hot springs, and the only geysers in Alaska. The landscape is dominated by volcanoes. On the northern half of the is

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Ireland seen by satellite Terra - Ireland satellite view - Image obtained on 4 January 2003. True - color Moderate Resolution Imaging Spectroradiometer (MODIS) image of Ireland taken from Terra satellite on January 4, 2003. The rugged cliffs that mark the island's west coast are showing their red - brown rocky surface, but the low - lying interior region is still wearing the island's signature green. The highest elevation in Ireland is Carrantuohill, located in the rugged terrain of the southwest tip. The bowl - like shape creates the network of lakes scattered across the island, and over time has produced peat bogs, which provide a source of fuel on the island, which is covered mostly by pasture and meadows. Ireland's largest city, Dublin, makes a purplish - gray patch peeking out from the clouds about halfway down the east coast. Belfast is more clearly visible on the coast in the northeast, due east of large Lake Neagh. One Ireland's few other large cities, Cork, is located at the m

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Ireland seen by satellite Terra - Ireland satellite view - Image obtained on 4 January 2003. True - color Moderate Resolution Imaging Spectroradiometer (MODIS) image of Ireland taken from Terra satellite on January 4, 2003. The rugged cliffs that mark the island's west coast are showing their red - brown rocky surface, but the low - lying interior region is still wearing the island's signature green. The highest elevation in Ireland is Carrantuohill, located in the rugged terrain of the southwest tip. The bowl - like shape creates the network of lakes scattered across the island, and over time has produced peat bogs, which provide a source of fuel on the island, which is covered mostly by pasture and meadows. Ireland's largest city, Dublin, makes a purplish - gray patch peeking out from the clouds about halfway down the east coast. Belfast is more clearly visible on the coast in the northeast, due east of large Lake Neagh. One Ireland's few other large cities, Cork, is located at the m

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France seen by the Terra satellite - France as seen by the Terra satellit

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France seen by the Terra satellite - France as seen by the Terra satellit

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

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

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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International Space Station (ISS) 10/2018 (photo)

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Syvach Lagoons (Sivash Lagoons), Crimea (photo)

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Syvach Lagoons (Sivash Lagoons), Crimea (photo)

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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The International Space Station (ISS) 09/2021 (photo)

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Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

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Star formation in the Sails - Star formation in Vela - Infrared view of the nebulae Gum 22 (top right), Gum 23, IRAS 09002 - 4732 (orange cloud near center), Bran 226 (bottom left), and Gum 25 (bottom left). These star-forming regions are located between 4000 and 10,000 light years of the Earth. The bright green star, down to the right of the image, is a carbon star, IRAS 08535 - 4724. Image obtained by the WISE telescope (Wide - field Infrared Explorer). This image from Nasa's Wide - field Infrared Survey Explorer, or WISE, highlights several star - forming regions. There are five distinct centers of star birth in this one image alone. Star - forming nebulae (called HII regions by astronomers) are clouds of gas and dust that have been heated up by nearby stars recently formed from the same cloud. The largest, brightest cloud, in the upper right is known as Gum 22. It's named after Colin Gum, an Australian astronomer who surveyed the southern hemisphere sky in the early 1950's looking

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

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

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Galaxy Cluster Abell 1656 - Coma Cluster - Wide - field image around the Coma galaxy cluster - Large field around the Coma galaxy cluster. This cluster consists of about a thousand galaxies and is located 330 million light years away in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies (NGC 4874 on the right and NGC 4889 on the left). Below the middle of the image, to the right, is the galaxy NGC 4921. Mosaic of images obtained by the Oschin telescope of 1.2m from Mount Palomar through several filters and composed. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). NGC 4921 is the small circular galaxy below and a little to the right of the centre of the image. The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at

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Galaxy Cluster Abell 1656 - Coma Cluster - Wide - field image around the Coma galaxy cluster - Large field around the Coma galaxy cluster. This cluster consists of about a thousand galaxies and is located 330 million light years away in the constellation Coma Berenices (Berenice hair). This cluster is dominated by two large elliptical galaxies (NGC 4874 on the right and NGC 4889 on the left). Below the middle of the image, to the right, is the galaxy NGC 4921. Mosaic of images obtained by the Oschin telescope of 1.2m from Mount Palomar through several filters and composed. The Coma cluster (Abell 1656) is a particularly rich cluster of individual galaxies (over 1000 members), most prominently the two giant ellipticals, NGC 4874 (right) and NGC 4889 (left). NGC 4921 is the small circular galaxy below and a little to the right of the centre of the image. The remaining members are mostly smaller ellipticals. The cluster is seen towards the constellation Coma Berenices, and is actually at

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