The impression of this artist shows a view of the surface of the planet Proxima in orbit around the red dwarf star Proxima Centauri, the star closest to the Solar System. Proxima b is a little more massive on Earth.
This is an illustration by the artist of the atmosphere of an exoplanet with a white dwarf star visible on the horizon. The starlight of a white dwarf filtered through the atmosphere of an exoplanet in orbit could reveal whether the planet has biosignatures.
This is an illustration by the artist of the planetary system Kepler-88, in which a giant exoplanet and two smaller planets orbit the star Kepler-88. The system is over 1,200 light years away.
This is an illustration of the newly discovered exoplanet Kepler-1649c in orbit around its host red dwarf star.
The illustration by this artist shows the night view of the exoplanet WASP-76b, where iron is raining from the sky.
This is the artist’s concept of a ringed planet passing in front of its host star. It shows how “swollen” a ringed planet can look at us from afar.
The dimensions of the 17 new candidates on the planet, seen here in orange, are compared with colored representations of Mars, Earth and Neptune. The green planet is KIC-7340288 b, a rocky planet in the habitable zone of its star.
Impression of the artist of K2-18b. CREDIT Amanda Smith
This is the impression of an artist of a hot Jupiter in orbit near a star.
This is an illustration by an artist of a huge planet in orbit around a cool young star. In the case of the newly discovered system, the planet is 10 times more massive than Jupiter and the planet’s orbit is almost 600 times that of the Earth around the sun.
Welcome to the KELT-9 system. The host star is a hot, rapidly rotating type A star that is about 2.5 times more massive and almost twice as hot as our sun. The hot star detonates its nearby planet KELT-9b with huge amounts of radiation, leading to a daytime temperature of 7800 degrees Fahrenheit, warmer than most stars and only 2000 degrees colder than the sun.
This is an artist’s rendering of the planetary system Proxima Centauri. The newly discovered exoplanet Proxima c, on the right, has an orbit of about 5.2 Earth years around its host star. The system also includes the smaller Proxima b, on the left, discovered in 2016. Illustration by Lorenzo Santinelli.
This is the concept of the artist from GJ180d, the temperate super-Earth closest to us with the potential to sustain life.
An illustration of WASP-12b as it spirals in a dance of death towards its star. The planet will reach its end in three million years.
TOI 700 d is the first potentially habitable terrestrial-sized planet identified by NASA’s TESS planet hunting mission.
TOI 1338 b stands out from its two guest stars, making it the first such discovery for the TESS mission. TESS only detects transits from the largest star
The illustration by this artist shows a wet exoplanet with an oxygen atmosphere. The red sphere is the M-nana star of the exoplanet’s orbits.
The illustration by this artist shows a dry exoplanet with an oxygen atmosphere. The red sphere is the M-nana star of the exoplanet’s orbits.
This artist’s illustration of the Kepler 51 system shows newly discovered puff exoplanets, which are also called “cotton candy” exoplanets because they are so light.
The conceptual illustration by this artist shows an exoplanet with two moons in orbit inside the habitable zone of a red dwarf star.
This is an illustration by the artist of two exoplanets colliding in a binary star system.
This is an illustration by the artist of a Neptune-type exoplanet in the icy external features of his star system. It could resemble a newly discovered large gas giant that takes about 20 years to orbit a star 11 light years from Earth.
This image shows a comparison of the red dwarf star GJ 3512 with our solar system, as well as other nearby red dwarf planetary systems.
This artist’s illustration shows the exoplanet K2-18b in orbit around its host star. It is currently the only super-terrestrial exoplanet that has water vapor in its atmosphere and may be at the right temperature to sustain life.
This is an example of an esomoon that loses mass as it is dragged around the gas giant that orbits.
An illustration shows what the orbit of exoplanet HR 5183 b would look like if it had fallen into our solar system. It would probably swing from the asteroid belt to pass Neptune, the eighth planet in our solar system.
At least two giant planets, at most 20 million years old, orbit the star Beta Pictoris. A disc of dust and gas surrounding the star can be seen in the background.
This is an artist’s interpretation of what the super-Earth GJ 357 d might look like. It is located within the habitable zone of its star which is 31 light years from Earth.
The impression of an artist of a circumplanetary disk around PDS 70 c, a giant gas exoplanet in a star system 370 light years away.
The illustration by this artist shows two gas giant exoplanets in orbit around the young star PDS 70. These planets are still growing by collecting material from a surrounding disk. In the process, they gravitated to a large disc gap.
An illustration by the artist of HD 21749c, the first Earth-sized planet found by TESS, as well as his brother, HD 21749b, a hot mini-Neptune.
A “hot Saturn” passes in front of its host star in this illustration. Astronomers studying the stars used “earthquakes” to characterize the star, which provided critical information about the planet.
The concept of the artist of TESS against the background of stars and planets orbiting the Milky Way. Credit: ESA, M. Kornmesser (ESO), Aaron E. Lepsch (ADNET Systems Inc.), Britt Griswold (Maslow Media Group), NASA’s Goddard Space Flight Center and Cornell University
A super telescope made the first direct observation of an exoplanet using optical interferometry. This method revealed a complex exoplanetary atmosphere with iron and silicate clouds swirling in a planetary storm. The technique presents unique possibilities to characterize many of the exoplanets known today.
This image shows an artist’s impression of the surface of Barnard’s star b, a cold Super-Earth discovered in orbit around Barnard’s star 6 light years away.
This artist’s illustration shows the newly discovered exoplanet K2-288Bb, 226 light years away and half the size of Neptune. Orbit around the weakest member of a pair of fantastic M-type stars every 31.3 days.
This is the impression of an artist from the exoplanet HAT-P-11b. The planet has an extended helium atmosphere that is blown away by the star, a smaller but more active orange dwarf star than our sun.
An artist’s illustration of what the super-Earth might look like around the orange star 26665 (also known as 40 Eridani A). The newly discovered exoplanet is compared to Vulcan’s fictional planet because Star Trek creator Gene Roddenberry claimed that the star was the ideal candidate to host Vulcan, Spock’s home world.
The TRAPPIST-1 star, an ultra-cool dwarf, has seven Earth-sized planets orbiting it.
For the first time, eight planets have been found in orbit around another star, binding to our solar system for the most well-known planets around a single star. The Kepler-90 system is located in the constellation of Draco, over 2,500 light years from Earth.
The illustration by this artist shows exoplanet Ross 128 b, with its red dwarf host star in the background. The planet is only 11 light years from our solar system. It is now the second closest temperate planet to be detected, after Proxima b.
WASP-121b, 880 light years away, is considered a hot planet similar to Jupiter. It has a greater mass and radius than Jupiter, making it “swollen”. If WASP-121b were closer to its host star, it would be torn apart by the gravity of the star.
NASA’s Kepler space telescope team identified 219 other planetary candidates, 10 of whom are close to Earth and in the habitable zone of their stars.
The concept of this artist shows OGLE-2016-BLG-1195Lb, a planet in orbit around an incredibly weak star 13,000 light years away from us. It is an “ice ball” planet with temperatures reaching minus 400 degrees Fahrenheit.
LHS 1140b is located in the habitable zone of liquid water surrounding its host star, a small weak red star called LHS 1140. The planet weighs approximately 6.6 times the mass of the Earth and is shown in front of LHS 1140. Depicted in blue is the atmosphere that the planet may have maintained.
Conceptual image of an artist of the surface of the exoplanet TRAPPIST-1f. Of the seven exoplanets discovered in orbit around the ultracool dwarf star TRAPPIST-1, this may be the most suitable for life. It is similar in size to Earth, is a little colder than Earth’s temperature and is in the habitable zone of the star, which means that liquid water (and even oceans) may be on the surface. The proximity of the star gives the sky a salmon-colored tinge and the other planets are so close as to appear in the sky, just like our moon.
Artist’s conception of the binary system with three uncovered giant planets, where one star houses two planets and the other houses the third. The system represents the minimum separation track where both stars are home to unobserved planets.
The impression of this artist shows the planet Proxima in orbit around the red dwarf star Proxima Centauri, the star closest to our solar system.
An artist’s rendering shows the Earth-sized exoplanets TRAPPIST-1b and 1c in a rare double-transit event as they pass their ultracool red dwarf star, which allowed Hubble to take a look at their atmospheres.
From a new discovery of 104 exoplanets, astronomers have discovered four Earth-like dimensions that orbit around a dwarf star. Two of them have the potential to sustain life. The vessel depicted in this illustration is NASA’s Kepler space telescope, which has helped confirm the existence of thousands of exoplanets.
The impression of this artist shows a view of the triple star system HD 131399 from near the giant planet in orbit in the system. Located approximately 320 light years from Earth, the planet is approximately 16 million years old, making it also one of the youngest exoplanets discovered to date.
An artistic impression of the planet Kepler-1647b, which is almost identical in size and mass to Jupiter. The planet is expected to look approximately similar. But it is much warmer: Kepler-1647b is in the habitable zone.
HD-106906b is a gas planet 11 times more massive than Jupiter. The planet is believed to have formed at the center of its solar system, before being sent flying to the edges of the region by a violent gravitational event.
Orbits of Kepler-10b at a distance more than 20 times closer to its star than Mercury is in our own sun. Daytime temperatures exceed 1,300 degrees Celsius (2,500 degrees Fahrenheit), which is warmer than lava flows on Earth.
This Jupiter-like planet in the HD-188753 system, 149 light years from Earth, has three suns. The main star is similar in mass to our Sun. The system has been compared to Luke Skywalker’s home planet, Tatooine, in “Star Wars”.
Kepler-421b is a transiting exoplanet the size of Uranus with the longest known year, since it rotates around its star once every 704 days. The planet orbits an orange K-type star that is colder and dimmer than our Sun and is located approximately 1,000 light years from Earth in the constellation of Lira.
Astronomers discovered two planets less than three times larger than Earth in orbit around sun-like stars in a crowded star cluster about 3000 light years from Earth in the Swan constellation.
The conception of this artist shows a hypothetical planet with two moons in orbit in the habitable zone of a red dwarf star. Most of the stellar neighbors closest to the sun are red dwarfs.
Kepler-186f was the first validated Earth-sized planet to be found in orbit around a distant star in the habitable zone. This area is at a distance from a star where liquid water could accumulate on the surface of the planet.
Kepler-69c is a planet the size of a super Earth similar to Venus. The planet is located in the habitable zone of a star like our sun, about 2,700 light years from Earth in the constellation of the Swan.
The Kepler-444 system was formed when the Milky Way was only 2 billion years old. The compact system encompasses five planets of varying sizes, the smallest being comparable to the size of Mercury and the largest to Venus, orbiting their sun in less than 10 days.
This image of the artistic concept compares the Earth, on the left, with Kepler-452b, which is approximately 60% larger. Both planets orbit a G2 type star of approximately the same temperature; however, the star that houses Kepler-452b is 6 billion years old, 1.5 billion years older than our sun.
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