Massive planet found orbiting 2 of the hottest, most massive stars
This image shows double-star system b Centauri and its giant planet b Centauri b. The star pair is the bright object at top left. The planet is visible as a bright dot in the lower right. The other bright dot (top right) is a background star.
This artist’s rendering shows a Jupiter-like planet orbiting a dead white dwarf star 6,500 light-years away from Earth. The planet survived the violent phases of stellar evolution leading to the star’s death.
This artist’s illustration shows the night-side view of the exoplanet WASP-76b, where iron rains down from the sky.
Astronomers have identified a new class of habitable planets, which they call Hycean planets. These are hot, ocean-covered planets with hydrogen-rich atmospheres.
This artist’s illustration shows L 98-59b, one of the planets in a planetary system 35 light-years away from Earth. This planet has half the mass of Venus.
In this artist’s illustration, two gaseous exoplanets can be seen orbiting the bright sun-like star HD 152843.
An artist’s rendering of TOI-1231 b, a Neptune-like planet about 90 light years away from Earth.
This artist’s conception depicts a violent flare erupting on the star Proxima Centauri as seen from the viewpoint of a planet orbiting the star called Proxima Centauri b.
After losing its gaseous envelope, the Earth-size core of an exoplanet formed a second atmosphere. It’s a toxic blend of hydrogen, methane, and hydrogen cyanide that is likely fueled by volcanic activity occurring beneath a thin crust, leading to its cracked appearance.
This illustration shows the metaphorical measuring of the density of each of the seven planets in the nearby TRAPPIST-1 system. New measurements have revealed the most precise densities yet for these planets and they’re very similar — which means they also likely have similar compositions.
This artist’s illustration shows the view from the furthest planet in the TOI-178 system.
This artist’s illustration shows TOI-561b, one of the oldest and most metal-poor planetary systems discovered yet in the Milky Way galaxy. Astronomers found a super-Earth and two other planets orbiting the star.
This massive and distant exoplanet, called HD106906 b, has an elongated and angled orbit that causes it to take 15,000 Earth years to complete one lap around its twin stars.
This is an artist’s impression of a free-floating rogue planet being detected in our Milky Way galaxy using a technique called microlensing. Microlensing occurs when an object in space can warp space-time.
This is an artist’s impression of exoplanet WASP-189 b orbiting its host star. The star appears to glow blue because it’s more than 2,000 degrees hotter than our sun. The planet, which is slightly larger than Jupiter, has a tilted orbit around the star’s poles rather than its equator.
For the first time, an exoplanet has been found orbiting a dead star known as a white dwarf. In this artist’s illustration, the Jupiter-sized planet WD 1856 b orbits the white dwarf every day and a half.
This illustration shows a carbon-rich planet with diamond and silica as ts main minerals. Water can convert a carbon-rich planet into one that’s made of diamonds. In the interior, the main minerals would be diamond and silica (a layer with crystals in the illustration). The core (dark blue) might be made of an iron-carbon alloy.
This image shows a young sun-like star being orbited by two gas giant exoplanets. It was taken by the SPHERE instrument on European Southern Observatory’s Very Large Telescope. The star can be seen in the top left corner, and the planets are the two bright dots.
This artist’s impression shows a Neptune-sized planet in the Neptunian Desert. It is extremely rare to find an object of this size and density so close to its star.
This is an artist’s impression of the multiplanetary system of newly discovered super-Earths orbiting a nearby red dwarf star called Gliese 887.
The newly discovered exoplanet AU Mic b is about the size of Neptune.
This artist’s impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. Proxima b is a little more massive than the Earth.
This is an artist’s illustration of an exoplanet’s atmosphere with a white dwarf star visible on the horizon. The starlight of a white dwarf filtered through the atmosphere of an exoplanet that’s orbiting it could reveal if the planet has biosignatures.
This is an artist’s illustration of the Kepler-88 planetary system, where one giant exoplanet and two smaller planets orbit the Kepler-88 star. The system is more than 1,200 light-years away.
This is an illustration of newly discovered exoplanet Kepler-1649c orbiting around its host red dwarf star.
This is an artist’s concept of a ringed planet passing in front of its host star. It shows how “puffy” a ringed planet may look to us from afar.
The sizes of the 17 new planet candidates, seen here in orange, are compared to colorized representations of Mars, Earth and Neptune. The green planet is KIC-7340288 b, a rocky planet in the habitable zone of its star.
Artist’s impression of K2-18b. CREDIT Amanda Smith
This is an artist’s illustration a massive planet orbiting a cool, young star. In the case of the newly discovered system, the planet is 10 times more massive than Jupiter, and the orbit of the planet is nearly 600 times that of Earth around the sun.
Welcome to the KELT-9 system. The host star is a hot, rapidly rotating A-type star that is about 2.5 times more massive and almost twice as hot as our sun. The hot star blasts its nearby planet KELT-9b with massive amounts of radiation, leading to a daylight temperature of 7800 degrees Fahrenheit, hotter that most stars and only 2000 degrees cooler than the sun.
This is an artist’s rendering of the Proxima Centauri planetary system. The newly discovered super-Earth exoplanet Proxima c, on the right, has an orbit of about 5.2 Earth years around its host star. The system also comprises the smaller Proxima b, on the left, discovered in 2016. Illustration by Lorenzo Santinelli.
This is an artist’s concept of GJ180d, the nearest temperate super-Earth to us with the potential to support life.
An illustration of WASP-12b as it spirals in a death dance towards its star. The planet will meet its end in three million years.
TOI 700 d is the first potentially habitable Earth-size planet spotted by NASA’s planet-hunting TESS mission.
TOI 1338 b is silhouetted by its two host stars, making it the first such discovery for the TESS mission. TESS only detects transits from the larger star
This artist’s illustration shows a wet exoplanet with an oxygen atmosphere. The red sphere is the M-dwarf star the exoplanet orbits.
This artist’s illustration shows a dry exoplanet with an oxygen atmosphere. The red sphere is the M-dwarf star the exoplanet orbits.
This artist’s illustration of the Kepler 51 system shows newly discovered super-puff exoplanets, which are also called “cotton candy” exoplanets because they’re so lightweight.