Scroll to load additional results for large searches. Thumbnails may rearrange to maintain sort order until page is fully populated.
14 Herculis c (NIRCam)
This image of 14 Herculis c, a planet orbiting a star 60 light-years away from Earth, was taken with the coronagraph on NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera). A star symbol marks the location of the host star 14 Herculis, whose light has been blocked by the...
51 Eri (NIRCam Image)
NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) captured this image of Eridani 51 b, a cool, young exoplanet that orbits 890 million miles from its star, similar to Saturn’s orbit in our solar system. The observations detected the planet is rich in carbon dioxide, providing...
Close-up of K2-25
Close-up of exoplanet K2-25b’s host star K2-25.
2M1510 AB, a pair of brown dwarfs with an exoplanet in a perpendicular orbit
This image, taken in visible light, shows 2M1510 AB, a pair of brown dwarfs orbiting each other. The two brown dwarfs, A and B, are seen as a single source in this image, but we know there are two of them because they periodically eclipse each other. When monitoring their orbits, astronomers...
A joint VLT and ALMA view of the disc around the star HD 135344B
This image shows the dusty disc around the young star HD 135344B. It’s a combination of data taken with two different facilities: the Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) instrument at ESO’s VLT in red, and the Atacama Large Millimeter/submillimeter Array (ALMA) in...
The disc around the star HD 135344B as seen with SPHERE
This image, captured with ESO’s Very Large Telescope (VLT), shows a spiral disc around the young star HD 135344B. The image, which was released in 2016, was obtained with the Spectro-Polarimetric High-contrast Exoplanet Research (SPHERE) instrument. Spiral features like these can be sculpted...
DESI Imaging Legacy Surveys Publish Seventh Data Release
he slideshow above highlights images from the Legacy Surveys’ Data Release 7 (DR7), which covers more than a quarter of the sky. More DR7 images of galaxies in Halton Arp’s Atlas of Peculiar Galaxies are available online. Read more about DR7 in the latest issue of NOAO Currents, which also...
Location of K2-25 (No Annotations)
A view showing the location of exoplanet K2-25b’s host star in the Hyades star cluster.
You can’t judge a star by its protoplanetary disc
Today’s Picture of the Week tells a story of redemption for one lonely star. The young star MP Mus (PDS 66) was thought to be all alone in the Universe, surrounded by nothing but a featureless band of gas and dust called a protoplanetary disc. In most cases, the material inside a protoplanetary...
Boulevard of broken rings
This Picture of the Week illustrates the remarkable capabilities of SPHERE (the Spectro-Polarimetric High-contrast Exoplanet REsearch instrument), a planet-hunting instrument mounted on ESO’s Very Large Telescope (VLT) in Chile: It shows a series of broken rings of dust around a nearby star....
A sparkling galactic neighbour
The galaxy ESO 300-16 looms over this image from the NASA/ESA Hubble Space Telescope. This galaxy, which lies 28.7 million light-years from Earth in the constellation Eridanus, is a ghostly assemblage of stars which resembles a sparkling cloud. A rogue’s gallery of distant galaxies and...
The MWC 758 planet-forming disc as seen by SPHERE and ALMA
This composite image shows the MWC 758 planet-forming disc, located about 500 light-years away in the Taurus region, as seen with two different facilities. The yellow colour represents infrared observations obtained with the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE)...
Giant star HD 47536
Sky area of 10 x 10 square arcmin around the 6th-magnitude giant star HD 47536 at which an exoplanet has been found in 2003 (reproduced from the Digital Sky Survey). The pattern is caused by internal reflections in the telescope from this relatively bright object.
2M1207b - first image of an exoplanet
This composite image shows an exoplanet (the red spot on the lower left), orbiting the brown dwarf 2M1207 (centre). 2M1207b is the first exoplanet directly imaged and the first discovered orbiting a brown dwarf (see the press release). It was imaged the first time by the VLT in 2004. Its...
The brown dwarf 2M1207 and its planetary companion
This composite image shows the first planet outside of our solar system (right) found orbiting a brown dwarf, dubbed 2M1207 (centre). The fainter planetary companion is at an angular distance of 778 milliarcsec from 2M1207. The exoplanet orbits at a distance from the brown dwarf that is nearly...
Sky field with OGLE-TR-132
Sky field in the southern constellation Carina (The Ship Keel) with the images of the star OGLE-TR-132, around which a transiting extra-solar planet (exoplanet) has been identified. The field measures 10 x 10 square arcmin; North is up and East is left. This image has been reproduced from the...
Sky Field with OGLE-TR-113
Sky field in the southern constellation Carina (The Ship Keel) with the images of the star OGLE-TR-113, around which a transiting exoplanet has been identified. The field measures 10 x 10 square arcmin; North is up and East is left. This image has been reproduced from the Digitized Sky Survey...
Combined SPHERE and ALMA image of material orbiting V960 Mon
At the centre of this image is the young star V960 Mon, located over 5000 light-years away in the constellation Monoceros. Dusty material with potential to form planets surrounds the star. Observations obtained using the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument...
Hot Gas-Giant Exoplanet WASP-43 b (MIRI Phase Curve)
This light curve shows the change in brightness of the WASP-43 system over time as the planet orbits the star. This type of light curve is known as a phase curve because it includes the entire orbit, or all phases of the planet. Because it is tidally locked, different sides of WASP-43 b rotate...
Hot Gas-Giant Exoplanet WASP-43 b (Artist’s Concept)
This artist’s concept shows what the hot gas-giant exoplanet WASP-43 b could look like. WASP-43 b is a Jupiter-sized planet circling a star roughly 280 light-years away, in the constellation Sextans. The planet orbits at a distance of about 1.3 million miles (0.014 astronomical units, or AU),...
Warm Gas-Giant Exoplanet WASP-107 b Transmission Spectrum (NIRSpec)
This transmission spectrum, captured using Webb’s NIRSpec (Near-Infrared Spectrograph), shows the amounts of different wavelengths (colors) of near-infrared starlight blocked by the atmosphere of the gas-giant exoplanet WASP-107 b. The spectrum was made by observing the planet-star system for...
Warm Gas-Giant Exoplanet WASP-107 b (Artist's Concept)
This artist’s concept shows what the exoplanet WASP-107 b could look like based on recent data gathered by NASA’s James Webb Space Telescope, along with previous observations from Hubble and other space- and ground-based telescopes. WASP-107 b is a “warm Neptune” exoplanet orbiting a...
Warm Gas-Giant Exoplanet WASP-107 b Transmission Spectrum (Hubble WFC3, Webb NIRCam, Webb MIRI)
This transmission spectrum, captured using NASA’s Hubble and James Webb space telescopes, shows the amounts of different wavelengths (colors) of starlight blocked by the atmosphere of the gas-giant exoplanet WASP-107 b. The spectrum includes light collected over five separate observations...
Super-Earth Exoplanet 55 Cancri e (Artist’s Concept)
This artist’s concept shows what the exoplanet 55 Cancri e could look like. Also called Janssen, 55 Cancri e is a so-called super-Earth, a rocky planet significantly larger than Earth but smaller than Neptune, which orbits its star at a distance of only 1.4 million miles (0.015 astronomical...
Super-Earth Exoplanet 55 Cancri e (NIRCam + MIRI Emission Spectrum)
A thermal emission spectrum captured by Webb’s NIRCam (Near-Infrared Camera) in November 2022, and MIRI (Mid-Infrared Instrument) in March 2023, shows the brightness (y-axis) of different wavelengths of infrared light (x-axis) emitted by the super-Earth exoplanet 55 Cancri e. The spectrum shows...
Super-Earth Exoplanet 55 Cancri e (MIRI Secondary Eclipse Light Curve)
This light curve shows the change in brightness of the 55 Cancri system as the rocky planet 55 Cancri e, the closest of the five known planets in the system, moves behind the star. This phenomenon is known a secondary eclipse. When the planet is next to the star, the mid-infrared light emitted...
Intricate spiral arms around V960 Mon captured with SPHERE
This image of the young star V960 Mon and its surrounding material was taken with the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument on ESO’s VLT. The material orbiting the young star is assembling together in a series of intricate spiral arms that extend to distances...
This image of the sky around the star Tau Boötis was created from the Digitized Sky Survey 2 images. The star itself, which is bright enough to be seen with the unaided eye, is at the centre. The spikes and coloured circles around it are artifacts of the telescope and photographic plate used...
Planet around Beta Pictoris
For the first time, astronomers have been able to directly follow the motion of an exoplanet as it moves to the other side of its host star. The planet has the smallest orbit so far of all directly imaged exoplanets, lying as close to its host star as Saturn is to the Sun. The team of...
Exoplanet caught on the move
For the first time, astronomers have been able to directly follow the motion of an exoplanet as it moves to the other side of its host star. The planet has the smallest orbit so far of all directly imaged exoplanets, lying as close to its host star as Saturn is to the Sun. The team of...
Planet around Beta Pictoris (annotated)
For the first time, astronomers have been able to directly follow the motion of an exoplanet as it moves to the other side of its host star. The planet has the smallest orbit so far of all directly imaged exoplanets, lying as close to its host star as Saturn is to the Sun. The team of...
Wide-field image centred on the exoplanet HIP 13044 b
This visible light wide-field image of the region around the exoplanet HIP 13044 b was created from photographs forming part of the Digitized Sky Survey 2. The field of view is approximately three degrees across. HIP 13044 is visible as an unremarkable, moderate brightness star at the exact...
The system around HR 8799 (annotated)
The bright and very young star HR 8799, about 130 light-years away from Earth, hosts a planetary system that looks like a scaled-up model of our own Solar System. Three giant planetary companions have been detected so far, with masses between 7 and 10 times that of Jupiter and being between 20...
The system around HR 8799
The bright and very young star HR 8799, about 130 light-years away from Earth, hosts a planetary system that looks like a scaled-up model of our own Solar System. Three giant planetary companions have been detected so far, with masses between 7 and 10 times that of Jupiter and being between 20...
Wide-field view of the sky around the star 51 Pegasi
This image shows the sky around the star 51 Pegasi in the northern constellation of Pegasus (The Winged Horse). In 1995 the first exoplanet to be discovered was detected orbiting this star. Twenty years later this object was also the first exoplanet to be be directly detected spectroscopically...
VLT image of exoplanet HD 95086 b
This image from ESO's Very Large Telescope (VLT) shows the newly discovered planet HD95086 b, next to its parent star. The observations were made using NACO, the adaptative optics instrument for the VLT in infrared light, and using a technique called differential imaging, which improves the...
NGC 6902 Caught by SPECULOOS
This Picture of the Week is a special treat: a first-light image from the newest resident of ESO’s Paranal Observatory, the SPECULOOS Southern Observatory. This planet-hunting machine aims to observe nearby but dim stars to locate exoplanets for other telescopes — such as ESO’s forthcoming...
ALMA Explores Fomalhaut’s Debris Disc
Fomalhaut is one of the brightest stars in the sky. At roughly 25 light-years away the star lies especially close to us, and can be seen shining brightly in the constellation of Piscis Austrinus (The Southern Fish). This image from the Atacama Large Millimeter/submillimeter Array (ALMA) shows...
Planet-hunting SPHERE images first circumbinary planet system with disc
Observations by ESO’s planet-finding instrument, SPHERE, a high-contrast adaptive optics system installed on the third Unit Telescope of ESO’s Very Large Telescope, have revealed the edge-on disc of gas and dust present around the binary star system HD 106906AB. HD 106906AB is a double star...
Moon-forming disc around the PDS 70c exoplanet as seen with ALMA
This image, taken with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, shows a close-up view on the moon-forming disc surrounding PDS 70c, a young Jupiter-like gas giant nearly 400 light-years away. It shows this planet and its disc centre-front, with the...
The sky around the red dwarf star Ross 128
This image shows the sky around the red dwarf star Ross 128 in the constellation of Virgo (The Virgin). It was created from images forming part of the Digitized Sky Survey 2. Ross 128 appears at the centre of the picture. Close inspection reveals that Ross 128 has a strange multiple appearance...
SPHERE observations of the planet HD 131399Ab
This composite image shows the newly discovered exoplanet HD 131399Ab in the triple-star system HD 131399. The image of the planet was obtained with the SPHERE imager on the ESO Very Large Telescope in Chile. This is the first exoplanet to be discovered by SPHERE and one of very few...
VLT snaps an exotic exoplanet “first”
Astronomers hunt for planets orbiting other stars (exoplanets) using a variety of methods. One successful method is direct imaging; this is particularly effective for planets on wide orbits around young stars, because the light from the planet is not overwhelmed by light from the host star and...
Exoplanet WASP-17 b (MIRI Transmission Spectrum)
A transmission spectrum of the hot gas giant exoplanet WASP-17 b captured by MIRI (Webb’s Mid-Infrared Instrument) on March 12-13, 2023, reveals the first evidence for quartz (crystalline silica, SiO2) in the clouds of an exoplanet. The spectrum was made by measuring the change in brightness...
Exoplanet WASP-17 b (Artist's Concept)
This artist's concept shows what the exoplanet WASP-17 b could look like. WASP-17 b, also called Ditsö̀, is a hot gas giant that orbits its star at a distance of just 0.051 AU (about 4.75 million miles, or one-eighth the distance between Mercury and the Sun), completing one full circuit in...
Atmosphere Composition of Exoplanet K2-18 b (NIRISS & NIRSpec)
Spectra of K2-18 b, obtained with Webb’s NIRISS (Near-Infrared Imager and Slitless Spectrograph) and NIRSpec (Near-Infrared Spectrograph) displays an abundance of methane and carbon dioxide in the exoplanet’s atmosphere, as well as a possible detection of a molecule called dimethyl sulfide...
Exoplanet K2-18 b (Illustration)
This illustration shows what exoplanet K2-18 b could look like based on science data. K2-18 b, an exoplanet 8.6 times as massive as Earth, orbits the cool dwarf star K2-18 in the habitable zone and lies 120 light years from Earth. A new investigation with NASA’s James Webb Space Telescope...
TRAPPIST-1 c Light Curve
This light curve shows the change in brightness of the TRAPPIST-1 system as the second planet, TRAPPIST-1 c, moves behind the star. This phenomenon is known as a secondary eclipse. Astronomers used Webb’s Mid-Infrared Instrument (MIRI) to measure the brightness of mid-infrared light. When the...
Rocky Exoplanet TRAPPIST-1 c (Artist Concept)
This artist' concept shows what the hot rocky exoplanet TRAPPIST-1 c could look like based on this work. TRAPPIST-1 c, the second of seven known planets in the TRAPPIST-1 system, orbits its star at a distance of 0.016 AU (about 1.5 million miles), completing one circuit in just 2.42 Earth-days....
Exoplanet GJ 486 b (Transmission Spectrum)
This graphic shows the transmission spectrum obtained by Webb observations of rocky exoplanet GJ 486 b. The science team’s analysis shows hints of water vapor; however, computer models show that the signal could be from a water-rich planetary atmosphere (indicated by the blue line) or from...
Exoplanet GJ 486 b (Artist Concept)
This artist concept represents the rocky exoplanet GJ 486 b, which orbits a red dwarf star that is only 26 light-years away in the constellation Virgo. By observing GJ 486 b transit in front of its star, astronomers sought signs of an atmosphere. They detected hints of water vapor. However,...
Image of Exoplanet HIP 65426b in Near and Mid Infrared
This image shows the exoplanet HIP 65426 b in different bands of infrared light, as seen from the James Webb Space Telescope: purple shows the NIRCam instrument’s view at 3.00 microns, blue shows the NIRCam instrument’s view at 4.44 microns, yellow shows the MIRI instrument’s view at 11.4...
Exoplanet WASP-96 b (NIRISS Transit Light Curve)
A light curve from Webb’s Near-Infrared Imager and Slitless Spectrograph (NIRISS) shows the change in brightness of light from the WASP-96 star system over time as the planet transits the star. A transit occurs when an orbiting planet moves between the star and the telescope, blocking some of...
NASA’s Webb Reveals Steamy Atmosphere of Distant Planet in Exquisite Detail
Webb’s enormous mirror and precise instruments join forces to capture the most detailed spectrum of an exoplanet atmosphere to date.
AB Aurigae b Illustration
This is an artist’s impression of a massive, newly forming exoplanet called AB Aurigae b. Researchers used new and archival data from the Hubble Space Telescope and the Subaru Telescope to confirm this protoplanet is forming through an intense and violent process, called disk instability. Disk...
AB Aurigae b Hubble Images Compass
Researchers were able to directly image newly forming exoplanet AB Aurigae b over a 13-year span using Hubble’s Space Telescope Imaging Spectrograph (STIS) and its Near Infrared Camera and Multi-Object Spectrograph (NICMOS). In the top right, Hubble’s NICMOS image captured in 2007 shows AB...
AB Aurigae b Hubble Images
Researchers were able to directly image newly forming exoplanet AB Aurigae b over a 13-year span using Hubble’s Space Telescope Imaging Spectrograph (STIS) and its Near Infrared Camera and Multi-Object Spectrograph (NICMOS). In the top right, Hubble’s NICMOS image captured in 2007 shows AB...
HR 8799 EXOPLANET SYSTEM
LEFT: This is an image of the star HR 8799 taken by Hubble's Near Infrared Camera and Multi-Object Spectrometer (NICMOS) in 1998. A mask within the camera (coronagraph) blocks most of the light from the star. In addition, software has been used to digitally subtract more starlight....
ARTWORK OF EXOPLANET GJ 1132 B
This is an artist's impression of the Earth-sized, rocky exoplanet GJ 1132 b, located 41 light-years away around a red dwarf star. Scientists using NASA's Hubble Space Telescope have found evidence this planet may have lost its original atmosphere but gained a second one that contains a toxic...
Hubble Pins Down Weird Exoplanet That Behaves Like the Long-Sought “Planet Nine”
HOT JUPITER ILLUSTRATION OF WASP-79B
BLOATED, SEETHING WORLD HAS A WEIRD ATMOSPHERE This is an artist's illustration of the super-hot exoplanet WASP-79b, located 780 light-years away. The planet orbits precariously close to a star that is much hotter than our Sun. The planet is larger than Jupiter, and its very deep, hazy...
NASA's Great Observatories Probe New Class of Exoplanet
Mysterious World Is Unlike Anything Found in Our Solar System
Too Hot and too Close for Comfort
Hubble Uncovers a 'Heavy Metal' Exoplanet Shaped Like a Football
EXOPLANET RADIUS VS. DISTANCE FROM STAR
ILLUSTRATION SHOWS LOCATION OF STAR-HUGGING EXOPLANETS
ARTIST'S ILLUSTRATION OF GAS STREAMING FROM GJ 3470B
This artist's illustration shows a giant cloud of hydrogen streaming off a warm, Neptune-sized planet just 97 light-years from Earth. The exoplanet is tiny compared to its star, a red dwarf named GJ 3470. The star's intense radiation is heating the hydrogen in the planet's upper atmosphere to a...
Artist’s impression of WASP-107b
The exoplanet WASP-107b is a gas giant, orbiting a highly active K-type main sequence star. The star is about 200 light-years from Earth. Using spectroscopy, scientists were able to find helium in the escaping atmosphere of the planet — the first detection of this element in the atmosphere of...
NASA Finds a Large Amount of Water in an Exoplanet’s Atmosphere
Researchers Surprised by How Much Water Found in Atmosphere of WASP-39b
NASA Finds a Large Amount of Water in an Exoplanet’s Atmosphere
Researchers Surprised by How Much Water Found in Atmosphere of WASP-39b
Hubble Directly Measures Rotation of Cloudy 'Super-Jupiter'
Though nearly 2,000 planets have been found around other stars, the light from only a handful of them has ever been collected by the world's most powerful telescopes. Ironically, a lot of them are detected by the shadows they cast, as they pass in front of their parent stars. Follow-up...
Hubble Directly Measures Rotation of Cloudy 'Super-Jupiter'
Though nearly 2,000 planets have been found around other stars, the light from only a handful of them has ever been collected by the world's most powerful telescopes. Ironically, a lot of them are detected by the shadows they cast, as they pass in front of their parent stars. Follow-up...
Artist's rendering of a "hot Jupiter," with samples of "light curve" data from hot Jupiters obtained by the Spitzer Space Telescope. Image credit: NASA/JPL-Caltech HIP 67522 b was identified as a planet candidate by NASA's Transiting Exoplanet Survey Satllite (TESS), which detects planets via the...
Artist's Impression of "Hot Jupiter" Exoplanets
This image shows an artist's impression of the 10 hot Jupiter exoplanets studied using the Hubble and Spitzer space telescopes. From top left to lower left, these planets are WASP-12b, WASP-6b, WASP-31b, WASP-39b, HD 189733b, HAT-P-12b, WASP-17b, WASP-19b, HAT-P-1b and HD 209458b.
This artist's concept shows a cloudy Jupiter-like planet that orbits very close to its fiery hot star. NASA's Spitzer Space Telescope was recently used to capture spectra, or molecular fingerprints, of two "hot Jupiter" worlds like the one depicted here.
Wide-Field View of GJ 1132 bs Host Star
Pictured here is the region around the host star of the exoplanet GJ 1132 b.
Region of the Sky Around HD 106906b
Pictured here is the region surrounding the exoplanet HD106906b. Located nearly 336 light-years from Earth, this 11-Jupiter-mass planet occupies an unlikely orbit around a double star 336 light-years away and may be offering clues to something that might be much closer to home: a hypothesized...
Possible Interiors of the TRAPPIST-1 Exoplanets
Three possible interiors of the TRAPPIST-1 exoplanets. The more precisely scientists know the density of a planet, the more they can narrow down the range of possible interiors for that planet. All seven planets have very similar densities, so they likely have a similar compositions.
HIP 67522 b: The Youngest Known Hot Jupiter
This artwork illustrates the newly-discovered the exoplanet HIP 67522 b, which appears to be the youngest hot Jupiter ever found. It orbits a well-studied star that is about 17 million years old, meaning the hot Jupiter is likely only a few million years younger, whereas most known hot Jupiters...
This artist's rendering shows a large exoplanet causing small bodies to collide in a disk of dust.
Kepler-10 Stellar Family Portrait
This artist's conception depicts the Kepler-10 star system, located about 560 light-years away near the Cygnus and Lyra constellations.
The varying brightness of an exoplanet called 55 Cancri e is shown in this plot of infrared data captured by NASA's Spitzer Space Telescope.
Exoplanet is Extremely Hot and Incredibly Close (Artist's Concept)
Astronomers using NASA's Spitzer Space Telescope have detected what they believe is an alien world just two-thirds the size of Earth one of the smallest on record. The exoplanet candidate, known as UCF-1.01, orbits a star called GJ 436, which is located a mere 33 light-years away. UCF-1.01 might...
First Map of an Exoplanet Atmosphere
This is the first-ever map of the surface of an exoplanet, or a planet beyond our solar system. The map, which shows temperature variations across the cloudy tops of a gas giant called HD 189733b, is made up of infrared data taken by NASA's Spitzer Space Telescope.
Surface of TRAPPIST-1f
Imagine standing on the surface of the exoplanet TRAPPIST-1f. This artist's concept is one interpretation of what it could look like.
Exotic Exoplanet
An unusual, methane-free world is partially eclipsed by its star in this artist's concept.
Hot-Lava World Illustration
This illustration shows one possible scenario for the hot, rocky exoplanet called 55 Cancri e, which is nearly two times as wide as Earth. New data from NASA's Spitzer Space Telescope show that the planet has extreme temperature swings from one side to the other and a possible reason for this...
Hot, Rocky World
This artist's rendition shows one possible appearance for the planet HD 219134b, the nearest rocky exoplanet found to date outside our solar system. The planet is 1.6 times the size of Earth, and whips around its star in just three days.
Using data from NASA's Kepler and Spitzer Space Telescopes, scientists have made the most precise measurement ever of the size of a world outside our solar system, as illustrated in this artist's conception The diameter of the exoplanet, dubbed Kepler-93b, is now known with an uncertainty of just...
Dark World (Full)
This artist's illustration depicts the exoplanet LHS 3844b, which is 1.3 times the mass of Earth and orbits an M dwarf star. The planet's surface may be covered mostly in dark lava rock, with no apparent atmosphere, according to observations by NASA's Spitzer Space Telescope.
The super-Earth exoplanet 55 Cancri e, depicted with its star in this artist's concept, likely has an atmosphere thicker than Earth's, with ingredients that could be similar to those of Earth's atmosphere.
The atmosphere of the distant "warm Neptune" HAT-P-26b, illustrated here, is unexpectedly primitive, composed primarily of hydrogen and helium.
Location of Nearest Rocky Exoplanet Known
This sky map shows the location of the star HD 219134, host to the nearest confirmed rocky planet found to date outside of our solar system.
"Wrong-way" Winds on CoRoT-2b
This illustration depicts the strange case of the backwards hotspot researchers have found on the hot exoplanet known as CoRoT-2b.
Exoplanet Forecast: Hot and Wet
This plot of data from NASA's Spitzer Space Telescope tells astronomers that a toasty gas exoplanet, or a planet beyond our solar system, contains water vapor.
How to Measure Exoplanet Light
These plots from NASA's Spitzer Space Telescope show light from a distant planet, GJ 436b, and its star, as measured at six different infrared wavelengths.
Detecting the Infrared Glow of a Dark World
This infographic illustrates how astronomers using NASAs Spitzer Space Telescope observations of the LHS 3844b system could deduce how much of the combined infrared light came from the Earth-sized exoplanet.
How to Find a Planetary Hot Spot
This graph of data from NASA's Spitzer Space Telescope shows how astronomers located a hot spot on a distant gas planet named upsilon Andromedae b -- and learned that it was in the wrong place.
A plot of the transmission spectrum for exoplanet HAT-P-11b, with data from NASA's Kepler, Hubble and Spitzer observatories combined. The results show a robust detection of water absorption in the Hubble data. Transmission spectra of selected atmospheric models are plotted for comparison.
Severe Exoplanetary Storm
These computer-generated images chart the development of severe weather patterns on the highly eccentric exoplanet HD 80606b during the days after its closest approach to its parent star.
Cracking the Code of Faraway Worlds: an Exoplanet Atmosphere
This infrared data from NASA's Spitzer Space Telescope called a spectrum tells astronomers that a distant gas planet, a so-called "hot Jupiter" called HD 209458b, might be smothered with high clouds. It is one of the first spectra of an alien world.
Cracking the Code of Faraway Worlds: An Exoplanet Atmosphere
This infrared data from NASA's Spitzer Space Telescope called a spectrum tells astronomers that a distant gas planet, a so-called "hot Jupiter" called HD 189733b, might be smothered with high clouds. It is one of the first spectra of an alien world.
Exoplanet HD 80606b Infrared Light Curve
This figure charts 30 hours of observations taken by NASA's Spitzer Space Telescope of a strongly irradiated exoplanet (an planet orbiting a star beyond our own). It shows the very rapid heating the planet experienced as it swung through its closest approach to the star.
Astronomers watched an exoplanet called HD 80606b heat up and cool off during its sizzling-hot orbit around its star. The results are shown in this data plot from NASA's Spitzer Space Telescope.
This artist's concept shows an exoplanet and debris disk orbiting a polluted white dwarf.
This artist's illustration depicts the exoplanet LHS 3844b, which is 1.3 times the mass of Earth and orbits an M dwarf star. The planet's surface may be covered mostly in dark lava rock, with no apparent atmosphere, according to observations by NASA's Spitzer Space Telescope.
Earth and Super-Earth
This artists concept contrasts our familiar Earth with the exceptionally strange planet known as 55 Cancri e. While it is only about twice the size of the Earth, NASA's Spitzer Space Telescope has gathered surprising new details about this supersized and superheated world.
Partially Cloudy Skies on Kepler-7b
Kepler-7b which is 1.5 times the radius of Jupiter is the first exoplanet to have its clouds mapped.
Infrared Light Curve for Transiting Exoplanet HD 219134b
This plot captures the nearest known rocky exoplanet, dubbed HD 219134b, in the act of passing in front of its star. The data were obtained in infrared light using NASAs Spitzer Space Telescope.
Illustration of TRAPPIST-1 Planets as of Feb. 2018
This illustration shows the seven Earth-size planets of TRAPPIST-1. The image does not show the planets' orbits to scale, but highlights possibilities for how the surfaces of these intriguing worlds might look.
NASA's Chandra Sees Eclipsing Planet in X-rays for First Time
An exoplanet in orbit around a star about 63 light years from Earth
NASA's Chandra X-ray Observatory Finds Planet That Makes Star Act Deceptively Old
An exoplanet about ten times Jupiter's mass located some 330 light years from Earth.
Providers | Sign In
NASA’s Universe of Learning materials are based upon work supported by NASA under cooperative agreement award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and NASA Jet Propulsion Laboratory. The award is part of NASA’s Science Activation program, which strives to further enable NASA science experts and content into the learning environment more effectively and efficiently with learners of all ages.