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Images of 'NASA' found, 2,032

 
The Helix Nebula (NGC 7293) (photo)

UIG529309

The Helix Nebula (NGC 7293) (photo)

UIG529309

 
Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

PIX4573412

Artist's view of the Exoplanet HD 189733b - Artist's impression of exoplanet HD 189733b - Artist's view of the Exoplanet HD 189733b, a hot Jupiter (gas-like planet very close to its star), in front of its star. HD 189733b was discovered in 2005 in the constellation Little Fox. We discovered water vapor and methane in his atmosphere. Artist's impression of the extrasolar planet HD 189733b, now known to have methane and water. Astronomers used the Hubble Space Telescope to detect methane - - the first organic molecule found on an extrasolar planet. Hubble also confirmed the presence of water vapour in the Jupiter - size planet's atmosphere, a discovery made in 2007 with the help of the Spitzer Space Telescope. They made the finding by studying how light from the host star filters through the planet's atmosphere

PIX4573412

 
Sagittarius dwarf irregular galaxy - SagDig - Sagittarius dwarf irregular galaxy - Image of the irregular dwarf galaxy ESO 594 - 4 located 3.5 million years ago - light seen by the Hubble space telescope on August 18, 2003. The Sagittarius dwarf irregular galaxy (SagDig, ESO 594 - 4) lies some 3.5 million light - years (1.1 Megaparsecs) from us. Background galaxies (reddish/brown extended objects with spiral arms and halos) are located even further beyond SagDig at several tens of millions parsecs away. This dwarf irregular galaxy was observed by the Advanced Camera for Surveys on - board the Hubble Space Telescope on 18 August 2003. Fifty-minute exposures were taken in blue, green and red filters

PIX4613853

Sagittarius dwarf irregular galaxy - SagDig - Sagittarius dwarf irregular galaxy - Image of the irregular dwarf galaxy ESO 594 - 4 located 3.5 million years ago - light seen by the Hubble space telescope on August 18, 2003. The Sagittarius dwarf irregular galaxy (SagDig, ESO 594 - 4) lies some 3.5 million light - years (1.1 Megaparsecs) from us. Background galaxies (reddish/brown extended objects with spiral arms and halos) are located even further beyond SagDig at several tens of millions parsecs away. This dwarf irregular galaxy was observed by the Advanced Camera for Surveys on - board the Hubble Space Telescope on 18 August 2003. Fifty-minute exposures were taken in blue, green and red filters

PIX4613853

 
Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. 3D recomposed view, vertical exaggeration: 2.5 times. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its

PIX4616341

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained in light visible by the probe 2001 Mars Odyssey, shows Tenuis Cavus, the end of this valley or the canyon is only 35 km wide. The cliffs s'elevent 1400 meters above ground. The walls are covered with ice, while at the bottom of the bowl many sand dunes are present. 3D recomposed view, vertical exaggeration: 2.5 times. Chasma Boreale is a huge canyon in the northern polar cap. It runs into the ice cap for 570 kilometers (350 miles), making a broad valley that ends at a point called Tenuis Cavus, shown in this THEMIS image taken at visible wavelengths.tapering from a width of 120 km (75 miles) at its mouth, Chasma Boreale is only about 35 km (22 miles) wide here. The cliffs rise about 1,400 meters (4,600 feet) above the base. On the inside walls of this gigantic amphitheater are stacked layers of ice, while on its

PIX4616341

 
Core of Comet Wild 2 - Comet Wild 2 nucleus - The nucleus of Comet Wild 2 (5 km in diameter) seen by the Stardust probe on January 2, 2004. This image was taken during the close approach phase of Stardust's Jan 2, 2004 flyby of comet Wild 2. It is a distant side view of the roughly spherical comet nucleus. One hemisphere is in sunlight and the other is in shadow analogous to a view of the quarter moon. Several large depressed regions can be seen. Comet Wild 2 is about five kilometers (3.1 miles) in diameter

PIX4570213

Core of Comet Wild 2 - Comet Wild 2 nucleus - The nucleus of Comet Wild 2 (5 km in diameter) seen by the Stardust probe on January 2, 2004. This image was taken during the close approach phase of Stardust's Jan 2, 2004 flyby of comet Wild 2. It is a distant side view of the roughly spherical comet nucleus. One hemisphere is in sunlight and the other is in shadow analogous to a view of the quarter moon. Several large depressed regions can be seen. Comet Wild 2 is about five kilometers (3.1 miles) in diameter

PIX4570213

 
Futuristic advertising poster for tourism on Kepler-16 b - Illustration - Futuristic Advert for tourism on Kepler-16 b - Illustration: Advertising promoting tourism on Kepler-16 b. This exoplanet is orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. An astronaut could contemplate a double sunset. Like Luke Skywalker's planet “” Tatooine””” in Star Wars, Kepler-16b orbits a pair of stars. Described here as a terrestrial planet, Kepler-16b might also be a gas giant like Saturn. Prospects for life on this unusual world aren't good, as it has a temperature similar to that of dry ice. But the discovery indicates that the movie's iconic double-sunset is anything but science fiction.

PIX4608238

Futuristic advertising poster for tourism on Kepler-16 b - Illustration - Futuristic Advert for tourism on Kepler-16 b - Illustration: Advertising promoting tourism on Kepler-16 b. This exoplanet is orbiting in the habitable area of the Starsystem Kepler-16 (AB), an Algol-type binary star located at a distance of about 200 light years from the Sun in the constellation of Swan. An astronaut could contemplate a double sunset. Like Luke Skywalker's planet “” Tatooine””” in Star Wars, Kepler-16b orbits a pair of stars. Described here as a terrestrial planet, Kepler-16b might also be a gas giant like Saturn. Prospects for life on this unusual world aren't good, as it has a temperature similar to that of dry ice. But the discovery indicates that the movie's iconic double-sunset is anything but science fiction.

PIX4608238

 
Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

PIX4574942

Infrared Jupiter seen by the New Horizons probe. - Jupiter seen by New Horizons spacecraft - View of Jupiter obtained on February 28, 2007 by the New Horizons probe. This infrared image shows the different altitudes of the Jovian clouds; in blue, the high altitudes clouds, in red, the lower clouds. Jupiter seen by New Horizons spacecraft during the Jupiter flyby in early 2007. This image is an infrared color composite taken by the spacecraft's near - infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 um, green: 1.94 um, blue: 1.85 um) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high - altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish - white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter's rotation du

PIX4574942

 
Jupiter and Io seen by the New Horizons probe

PIX4574952

Jupiter and Io seen by the New Horizons probe

PIX4574952

 
Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The cloud complexes around Orion and the disk of the Milky Way are seen behind the observatory. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

PIX4645602

Space Telescope Spitzer - Artist view - The Spitzer space telescope. Artwork - The Spitzer space telescope observes the universe in infrared; it was launched and put into orbit in August 2003. The cloud complexes around Orion and the disk of the Milky Way are seen behind the observatory. The Spitzer Space Telescope (formerly SIRTF, the Space Infrared Telescope Facility) was launched into space by a Delta rocket from Cape Canaveral, Florida on 25 August 2003. During its mission, Spitzer will obtain images and spectra by detecting the infrared energy, or heat, radiated by objects in space between wavelengths of 3 and 180 microns (1 micron is one - millionth of a meter). Most of this infrared radiation is blocked by the Earth's atmosphere and cannot be observed from the ground

PIX4645602

 
Eagle nebula (IC 4703) in the Snake -JWST, 2022 (photography)

PIX7331195

Eagle nebula (IC 4703) in the Snake -JWST, 2022 (photography)

PIX7331195

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

PIX4568849

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

PIX4568849

 
Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

Saturn and satellites seen by the Hubble space telescope - Saturn rings edge - on with satellites - Saturn observed by the Hubble space telescope on February 24, 2009 when the Earth is in the same plane as the rings, seen by the slice. This phenomene occurs every 15 years. This sequence of images taken for just over three hours shows the movement from left to right of four satellites in front of the planet. From left to right on the top image we see the satellites Enceladus, Dione (the brightest ice satellite), Mimas and the largest satellite, Titan, orange. This sequence of images captures the parade of several of Saturn's moons transiting the face of the gas giant planet from left to right during more than three hours. This is a rare event because the rings are tilted edge on to Earth every 15 years. The top frame captures the giant moon Titan and its shadow near Saturn's northern polar hood. Tiny Mimas and its shadow have just entered the left limb of Saturn, slightly above the ring

PIX4624891

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