32 alien planets that really exist

by Pelican Press
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32 alien planets that really exist

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 An artist's rendering comparing the

Credit: BENOIT GOUGEON, UNIVERSITÉ DE MONTRÉAL

Far beyond the eight familiar planets in our solar system, countless bizarre and extreme worlds await discovery — and some have already been found.

Thanks to rapidly advancing telescope technology, astronomers have detected more than 5,600 planets outside our solar system. These exoplanets, as scientists call them, are worlds of lava, and worlds of water. They’re worlds being ravaged by the heat of their stars, and worlds locked in eternal night. There are worlds that look like they were stolen straight from “Star Wars,” and worlds that may hold exotic forms of life never dreamed up in science fiction.

Join us as we tour some of the strangest and most fascinating exoplanets in our ever-surprising universe.

The “hell planet” where it rains lavaAn illustration of a hot, rocky exoplanet. The planet's surface is gray with orange marbling the surfaceAn illustration of a hot, rocky exoplanet. The planet's surface is gray with orange marbling the surface

An illustration of a hot, rocky exoplanet. The planet’s surface is gray with orange marbling the surface

55 Cancri e is a rocky world about eight times the size of Earth, making it a type of exoplanet known as a “super Earth.” Despite its ample size, nothing is “super” about the living conditions here. Often nicknamed the “hell planet,” 55 Cancri e is completely covered in flowing seas of lava, and it may even rain lava there as well. The exoplanet is located 41 light-years from Earth, making it a popular target for studies (but not for summer getaways).

Related: 38 jaw-dropping James Webb Space Telescope images

The water world with (potentially) living oceansA rendering of a large, blue circular exoplanet on the left of a starry, black background. A small, orange star lies on the right of the image. In between, lies a crescent, white exoplanet, K2-18 cA rendering of a large, blue circular exoplanet on the left of a starry, black background. A small, orange star lies on the right of the image. In between, lies a crescent, white exoplanet, K2-18 c

A rendering of a large, blue circular exoplanet on the left of a starry, black background. A small, orange star lies on the right of the image. In between, lies a crescent, white exoplanet, K2-18 c

K2-18 b is a large world located about 120 light-years from the sun. It inhabits the “Goldilocks zone” around its star, meaning that liquid water (and potentially life) could exist there. A recent analysis with the James Webb Space Telescope (JWST) supports the idea that the exoplanet may have its own liquid water ocean — and that the ocean may be home to living creatures. In the study, JWST detected possible traces of dimethyl sulfide, a chemical known to be emitted only by phytoplankton on Earth, in the exoplanet’s atmosphere.

The real-world “Tatooine”An artist image shows a marbled, white and beige planet in the foreground. In the background is a glowing, yellow star and a glowing, orange star on a starry, black backgroundAn artist image shows a marbled, white and beige planet in the foreground. In the background is a glowing, yellow star and a glowing, orange star on a starry, black background

An artist image shows a marbled, white and beige planet in the foreground. In the background is a glowing, yellow star and a glowing, orange star on a starry, black background

Luke Skywalker would feel right at home on Kepler-16b. This exoplanet is the first known circumbinary planet — a planet that orbits two stars at the same time, just like Tatooine from the Star Wars franchise. However, because this huge planet has a gassy surface similar to Saturn’s, even a Jedi would have a hard time finding their footing on this exoplanet, which is located about 200 light-years from the sun.

The rule-breaking behemothArtistic rendering of the possible view from LHS 3154b towards its low mass host star. Given its large mass, LHS 3154b probably has a Neptune-like composition.Artistic rendering of the possible view from LHS 3154b towards its low mass host star. Given its large mass, LHS 3154b probably has a Neptune-like composition.

Artistic rendering of the possible view from LHS 3154b towards its low mass host star. Given its large mass, LHS 3154b probably has a Neptune-like composition.

The giant exoplanet LHS 3154b has scientists scratching their heads, because it seems far too large for its tiny star. This planet, which is about 13 times more massive than Earth but orbits a star nine times less massive than the sun, doesn’t seem like it could exist, researchers said upon its discovery in 2023. Future studies of this “impossible” world could upend the known rules of planet formation.

The largest exoplanet in the known universe?An artist rendering of 10 round exoplanets, 5 on top and 5 on bottom in front of a starry backgroundAn artist rendering of 10 round exoplanets, 5 on top and 5 on bottom in front of a starry background

An artist rendering of 10 round exoplanets, 5 on top and 5 on bottom in front of a starry background

With twice the radius of Jupiter, the exoplanet HAT-P-67 b may be the largest known planet in the universe, in terms of width. But despite its monumental girth, there are more massive worlds out there. This honkin’ world, located about 1,200 light-years from Earth, has a very low density, giving it only about one-third the mass of Jupiter.

The “fluffy” planet where it rains sandArtist's impression of WASP-107b and its parent star, orange, red and yellow gaseous masses in the universe.Artist's impression of WASP-107b and its parent star, orange, red and yellow gaseous masses in the universe.

Artist’s impression of WASP-107b and its parent star, orange, red and yellow gaseous masses in the universe.

Located 200 light-years from Earth, the exoplanet WASP-107b also has a very low density, making it appear “fluffy” in telescope observations. A recent JWST study of the planet revealed clouds potentially made of fine-grained silicate particles, meaning it may literally rain sand on this puffed-up world.

The “eyeball planet” with potentially living seasAn artist's rendering comparing the An artist's rendering comparing the

An artist’s rendering comparing the

Sitting just 50 light-years from Earth, the beady-eyed exoplanet LHS 1140 b may be a candidate for alien life thanks to its one-of-a-kind surface. Scientists studying the world with JWST found that the planet may be covered in ice — except for the one part of its surface that permanently points toward its host star. Here, the star’s heat may melt just enough ice for a circular, liquid water ocean to form, according to the researchers. Besides giving the planet a distinct bull’s-eye appearance, this rare ocean may be a prime place for extraterrestrial life to flourish, the team wrote.

The rotten-egg worldArtist's interpretation of a blue gas giant exoplanet very close to a sun-like starArtist's interpretation of a blue gas giant exoplanet very close to a sun-like star

Artist’s interpretation of a blue gas giant exoplanet very close to a sun-like star

The exoplanet HD 189733 b, located about 64 light-years from Earth, has a chemical composition so distinct that astronomers can practically smell it from across the galaxy. A recent JWST study of the planet found that its atmosphere contains significant amounts of hydrogen sulfide — a toxic and flammable gas given off by decaying organic matter and volcanoes on Earth — which smells like rotten eggs. The smelly egg planet is far too hot for life to exist (thank goodness), but the mere fact that scientists can detect such distinct molecules in its atmosphere is a good sign that JWST may soon be able to detect signatures of life elsewhere in the universe.

The “Vulcan planet” that may not existhd 106906 bhd 106906 b

hd 106906 b

In a remarkable case of science fiction reflected in reality, scientists have reported the discovery of a planet similar to Vulcan, the home world of Dr. Spock in the Star Trek franchise. The planet was discovered in 2018 around the real star 40 Eridani A — the very same star that hosts Spock’s home planet in the famous sci-fi series. However, recent follow-up observations of the star have called the planet’s existence into question; subtle wobbles in the star’s light signature may result not from a nearby planet’s tugging on it but rather from regular eruptions on the star’s surface. The existence of the Vulcan planet, named HD 26965 b, now seems in doubt.

The Earth-like planet around a small, red starAn illustration of the newly discovered Earth-sized exoplanet Gliese 12An illustration of the newly discovered Earth-sized exoplanet Gliese 12

An illustration of the newly discovered Earth-sized exoplanet Gliese 12

Earth may have a long-lost twin in a nearby star system. Named Gliese 12 b, the planet orbits a hot, red star in a system roughly 40 light-years from Earth. Remarkably, the exoplanet appears to have a width 1.1 times that of Earth, giving it similar properties to our own planet. And while Gliese 12 b orbits its home star much more closely than our planet does the sun (one year there lasts about 13 Earth days), that star is also much smaller, keeping the planet in the habitable zone where liquid water can form on the planet’s surface. That means our distant twin may even have its own version of life.

The Earth-size planet with eternal nighta rocky planet orbiting a hot red star in spacea rocky planet orbiting a hot red star in space

a rocky planet orbiting a hot red star in space

Not all Earth-size planets are lucky enough to be habitable. Take SPECULOOS-3 b, a rocky, Earth-like world whose orbit around its red dwarf star is a little too close for comfort. Completing an orbit every 17 hours, the rocky world is exposed to so much radiation that its atmosphere was likely blasted away long ago, leaving the unlucky planet totally barren. The roasting temperatures aren’t a global phenomenon, however; this planet is tidally locked, meaning one side always faces its star in eternal day, while the other side sits in perpetual night.

The red volcano world that’s “melting from within”An illustration of a glowing planetAn illustration of a glowing planet

An illustration of a glowing planet

Astronomers have discovered a planet in a distant star system that appears to be erupting with so many volcanoes, the world literally glows red when seen through telescopes. The smoldering exoplanet, named TOI-6713.01, is located roughly 66 light-years from Earth and orbits its star closely, completing a loop every 2.2 Earth days. Observations suggest the planet is covered in molten lava, released by hundreds of active volcanoes. The planet is also subject to incredible internal friction from the gravity of its star and its neighboring planets, which may be causing the world to literally melt from within.

The gas giant with bullet-like windAn artist's concept of WASP-43b.An artist's concept of WASP-43b.

An artist’s concept of WASP-43b.

Scientists have mapped the weather on an enormous exoplanet 280 light-years from Earth, and the forecast looks grim. The planet, named WASP-43b, is tidally locked, with one massive face always pointing toward its star and the other cloaked in eternal darkness. Significant temperature differences between the two sides drive fierce winds, which scientists estimated to blow at up to 5,600 mph (9,000 km/h) — several times faster than a speeding bullet.

The hellish world with glorious rainbowsExoplanet WASP-76b.Exoplanet WASP-76b.

Exoplanet WASP-76b.

The exoplanet WASP-76 b — located about 637 light-years from Earth — is not the type of place you’d want to vacation. Orbiting 20 times closer to its home star than Mercury orbits the sun, the planet’s dayside is estimated to reach 4,350 degrees Fahrenheit (2,400 degrees Celsius), making it a true hell world. There is one draw, however: A strange bright spot observed on the planet’s surface, right where the day and night sides meet, could be a “glory” — a rare visual phenomenon, sometimes seen on Earth, made up of concentric rainbow rings forming a giant circle.

The giant planets orbiting dead starsAn illustration shows a Jupiter like world orbiting a dead white dwarf star.An illustration shows a Jupiter like world orbiting a dead white dwarf star.

An illustration shows a Jupiter like world orbiting a dead white dwarf star.

One day, the sun will die — but some planets in our solar system may live on. Scientists made this inference after discovering two enormous planets orbiting “dead” white dwarf stars in distant star systems. Named WD 1202-232 and WD 2105-82, the planets are estimated to be between one and seven times as massive as Jupiter, and both orbit small, dead stars at distances of at least 11.5 times that between Earth and the sun. Their discovery, if confirmed, hints that our solar system’s comparable planets, Jupiter and Saturn, may be able to survive the inevitable death of the sun one day. (Earth, sadly, is likely to be swallowed up during our star’s final expansion.)

The “rogue” planets of OrionAn image of a young star-forming region filled with wispy blue, grey, green, and red nebulosity that is brightest towards the centre and fainter towards the edges, especially in the top left corner and on the right side. Thousands of stars are seen sprinkled across the field, concentrated towards the centre, and the brightest stars show the eight spikes due to diffraction that are characteristic of Webb images.An image of a young star-forming region filled with wispy blue, grey, green, and red nebulosity that is brightest towards the centre and fainter towards the edges, especially in the top left corner and on the right side. Thousands of stars are seen sprinkled across the field, concentrated towards the centre, and the brightest stars show the eight spikes due to diffraction that are characteristic of Webb images.

An image of a young star-forming region filled with wispy blue, grey, green, and red nebulosity that is brightest towards the centre and fainter towards the edges, especially in the top left corner and on the right side. Thousands of stars are seen sprinkled across the field, concentrated towards the centre, and the brightest stars show the eight spikes due to diffraction that are characteristic of Webb images.

Most known planets orbit stars, but there may be countless others that don’t. Scientists using the JWST have discovered hundreds of free-floating “rogue planets” zooming through the Orion Nebula, untethered to any star. Strangely, about 80 of these rogue worlds are trapped in binary orbits with each other, tumbling through space in pairs. Scientists are not certain how these worlds got ejected from their home star systems or why they are trapped in binary orbits. Given that these planets are roughly as massive as Jupiter, scientists have dubbed them Jupiter-mass binary objects — or JuMBOs, for short.

The distant planet we can actually seeA black background with a large blue glowing orb in the middle and a smaller red orb to the bottom leftA black background with a large blue glowing orb in the middle and a smaller red orb to the bottom left

A black background with a large blue glowing orb in the middle and a smaller red orb to the bottom left

Scientists detect most exoplanets indirectly, by watching changes in the light emitted by distant stars. But in 2004, researchers got direct visual confirmation of an alien world for the first time ever. Called 2M1207b, the exoplanet is located about 170 light-years away, in the constellation Centaurus, and is a gas giant about five times more massive than Jupiter. The team spotted the distant world by looking at it in three different infrared wave bands, which helped reveal the planet’s heat while blocking the light of its home star. Since this groundbreaking discovery, roughly 200 exoplanets have been discovered through direct imaging, while more than 5,000 others have been revealed through other means.

The planet with clouds of quartzAn artist’s impression of the exoplanet WASP-17b, which may contain clouds of quartz in its atmosphere.An artist’s impression of the exoplanet WASP-17b, which may contain clouds of quartz in its atmosphere.

An artist’s impression of the exoplanet WASP-17b, which may contain clouds of quartz in its atmosphere.

Can you imagine a sunset filtered through a crystal sky? That may be a reality on the exoplanet WASP-17b, a Jupiter-like gas giant that’s so hot that its clouds are made of quartz crystals, observations with JWST suggest. The planet orbits extremely close to its home star, giving it an atmosphere with temperatures reaching a blistering 2,700 F (1,500 C). This heat forms tiny, sand-size silica particles in the planet’s atmosphere, which may coalesce into clouds of pure quartz, researchers suggest.

The baby Jupiter about to be bornFour spirals of yellow gas swirl around a distant star. At the center, blue blotches reveal where gas is collapsing into new planetsFour spirals of yellow gas swirl around a distant star. At the center, blue blotches reveal where gas is collapsing into new planets

Four spirals of yellow gas swirl around a distant star. At the center, blue blotches reveal where gas is collapsing into new planets

Exoplanet-hunting scientists zoom in on not just existing worlds but also worlds that are about to be born. While studying the region around the star V960 Mon, located about 5,000 light-years from Earth, scientists spotted a clumpy field of gas where two tendrils of material are apparently being funneled into distinct, planet-like lumps. According to the researchers, who made the discovery using the European Southern Observatory’s Very Large Telescope and the Atacama Large Millimeter/submillimeter Array, this is the first time scientists have imaged a young star system on the verge of birthing its first giant planets.

The sibling planets dancing in lockstepA sub-radio image of the system PDS 70, showing its star in the center; the orbit of a Jupiter-sized planet as a thick-band; and an accompanying debris cloud as a thin band.A sub-radio image of the system PDS 70, showing its star in the center; the orbit of a Jupiter-sized planet as a thick-band; and an accompanying debris cloud as a thin band.

A sub-radio image of the system PDS 70, showing its star in the center; the orbit of a Jupiter-sized planet as a thick-band; and an accompanying debris cloud as a thin band.

Around the distant star PDS 70, located 370 light-years from Earth, resides an incredibly rare pair of sibling planets. One fully formed world roughly the size of Jupiter appears to swirl around its host star; behind it, in the same orbit, is an enormous cloud of gas and dust that researchers suspect may be the planet’s partially formed sibling. Although only one of the objects seems to be a full-fledged planet, the pair is the first evidence of rare “Trojan planets” — two worlds that formed at nearly the same time, in roughly the same place around their home star, moving in the exact same orbit.

The planet turning its star into a “spiral galaxy”Orange spiral arms swirl out of the black center of a distant star systemOrange spiral arms swirl out of the black center of a distant star system

Orange spiral arms swirl out of the black center of a distant star system

About 500 million light-years from Earth is a star system that looks suspiciously familiar. Wrapped in two dusty spiral arms, it resembles our own Milky Way galaxy — although on a much, much smaller scale. The reason for this star’s galactic appearance? Astronomers suspect it’s because of a hidden, Jupiter-size planet dubbed MWC 758 c, which used its massive gravitational pull to sculpt the star’s sheath of dust into spectacular spiral arms. The planet has yet to be fully confirmed, but simulations show it’s a likely cause of its home star’s odd look.

The mirror world that shouldn’t existA visual representation of the exoplanet LTT9779 b (right) reflecting light back toward its home star (left).A visual representation of the exoplanet LTT9779 b (right) reflecting light back toward its home star (left).

A visual representation of the exoplanet LTT9779 b (right) reflecting light back toward its home star (left).

Most planets reflect at least a bit of their home star’s light. But the exoplanet LTT9779 b reflects a whopping 80% of its star’s incoming rays — the highest reflectiveness of any planet ever discovered. The key to the planet’s impressive albedo is a layer of metallic clouds that surrounds it. Scientists suspect the Neptune-size world’s sky is mostly full of silicate, or glass, and titanate, a salt containing titanium — turning the planet’s atmosphere into a veritable mirror. The planet’s existence poses a puzzle for scientists: The world orbits so closely to its star that its atmosphere should have been blown away by now. The key to its survival may be the metal in the planet’s skies, which may be too heavy for solar wind to blast it away.

The “zombie” planet that survived its star’s deathAn artist's illustration of Halla surviving a potentially cataclysmic merger between the two stars in its binary system.An artist's illustration of Halla surviving a potentially cataclysmic merger between the two stars in its binary system.

An artist’s illustration of Halla surviving a potentially cataclysmic merger between the two stars in its binary system.

The exoplanet 8 Ursae Minoris b, also known as Halla, is a hot, Jupiter-like world located 520 light-years from Earth. Observations suggest the massive world should have been completely incinerated by its home star, which has already entered its red giant phase and appears to have long since ballooned outward into its system, scorching everything in its path, before shrinking back to its current size. The fact that Halla orbits relatively close to the star suggests it was either born after the star shrank again or the star that’s visible today is one of two binary stars that merged, preventing either one from expanding on its path of destruction.

The water world with a steam atmosphereAn artist's impression of the mini-Neptune planet, cloaked in a hazy atmosphere.An artist's impression of the mini-Neptune planet, cloaked in a hazy atmosphere.

An artist’s impression of the mini-Neptune planet, cloaked in a hazy atmosphere.

The exoplanet GJ 1214b is located just 40 light-years from Earth, but it’s coated in so many thick clouds that scientists had a hard time studying it until recently. Using JWST’s infrared vision to peer through the clouds, scientists analyzed the planet and saw what appeared to be an atmosphere made of steam, suggesting the world below may contain significant amounts of water.

The Earth-like planet with no atmosphereAn illustration of a rocky, Earth-like planet soaking up heat from its small red sunAn illustration of a rocky, Earth-like planet soaking up heat from its small red sun

An illustration of a rocky, Earth-like planet soaking up heat from its small red sun

Around the distant star TRAPPIST-1, seven rocky, Earth-size planets swirl through the star’s habitable zone. Whether any of these planets contain the right conditions for life is a question astronomers are eagerly investigating. But one of them, TRAPPIST-1b, may be officially out of the running. JWST’s observations of the rocky, Earth-like world reveal that the planet is about as hot as an oven — a whopping 450 F (232 C) — and almost certainly doesn’t have an atmosphere. Some of the scorching world’s neighbors may be better positioned for life to emerge, but more research is needed to know for sure.

The extraterrestrial sandstorm planetAn illustration of a fiery red 'super Jupiter' planet with a raging red dust storm on its surfaceAn illustration of a fiery red 'super Jupiter' planet with a raging red dust storm on its surface

An illustration of a fiery red ‘super Jupiter’ planet with a raging red dust storm on its surface

Scientists using JWST have spotted a gargantuan sandstorm raging on the exoplanet VHS 1256 b, located roughly 40 light-years from Earth. An enormous world that’s far from its star, the “super-Jupiter” takes about 10,000 years to complete a single orbit. That large distance means scientists can see the planet’s atmosphere relatively clearly, without too much starlight getting in the way. Recent observations showed incredibly hot clouds made of silicate particles swirling through the planet’s atmosphere. According to the researchers, this may be evidence of a gargantuan dust storm.

The planet hotter than a starThis animated gif shows planet KELT-9b whizzing around its local star, leaving a smear of vapor behind it.This animated gif shows planet KELT-9b whizzing around its local star, leaving a smear of vapor behind it.

This animated gif shows planet KELT-9b whizzing around its local star, leaving a smear of vapor behind it.

KELT-9b is an extremely hot, Jupiter-like planet located 670 light-years from Earth. With an estimated surface temperature of 7,800 F (4,300 C), it was deemed the hottest exoplanet ever discovered upon its detection and is even hotter than some stars. This intense heat has a nasty impact on the planet’s atmosphere: On KELT-9b’s dayside, the heat of the nearby star beats down so intensely that hydrogen molecules in KELT-9b’s atmosphere are literally ripped to shreds and blown across the planet. With one-half of the planet’s atmosphere constantly melting, this world is one extraterrestrial destination you’d definitely want to avoid.

The toxic football planetfootball-shaped planet WASP121-bfootball-shaped planet WASP121-b

football-shaped planet WASP121-b

Located about 900 light-years from Earth, the exoplanet WASP-121b is so hot that heavy metals are constantly boiling through its atmosphere and venting into space. Scientists spotted iron and magnesium molecules so high above the planet’s surface that they could escape the pull of gravity and drift away. The extreme heat comes from the planet’s ultraclose proximity to its host star. The planet is so close, in fact, that tidal forces generated by the star’s gravity have stretched the planet into a football shape that distinguishes it from the spherical worlds most often discovered.

The ultrasmall world moving at breakneck speedA NASA illustration compares the newly-discovered planet to Earth and Mars.A NASA illustration compares the newly-discovered planet to Earth and Mars.

A NASA illustration compares the newly-discovered planet to Earth and Mars.

Located 35 light-years from Earth, L 98-59b is one of the smallest exoplanets ever discovered, with a mass just 0.4 times that of Earth. The tiny world also rockets around its home star at breakneck speed, completing an orbit in just two days, six hours. Because of this, the planet receives roughly 22 times as much energy from its home star as Earth does from the sun, almost certainly rendering the tiny, fast-moving planet uninhabitable.

Earth’s “older cousin”Artist's concept of a large planet in spaceArtist's concept of a large planet in space

Artist’s concept of a large planet in space

The exoplanet Kepler-452 b appears so similar to our home planet that NASA has dubbed the world “Earth’s older cousin.” The rocky exoplanet orbits a sunlike star at virtually the same distance that our planet orbits the sun, with a year there lasting about 384 days. That puts the planet firmly in the habitable zone, where liquid water could form on its surface. Sadly, our cousin will remain estranged for a good while longer: At nearly 1,800 light-years from Earth, the planet would take at least 30 million years to reach by spacecraft.

The bizarrely close sibling planetsA large planet with a smaller planet near it in front of a starry backgroundA large planet with a smaller planet near it in front of a starry background

A large planet with a smaller planet near it in front of a starry background

The exoplanet Kepler-36b is a rocky world that’s about 1.5 times the size of Earth and orbits bizarrely close to its neighboring world, the Neptune-like exoplanet Kepler-36c. The two alien worlds make extremely close approaches to each other every 97 days, on average; during those cosmic family reunions, the two planets are separated by less than five Earth-moon distances. These ultraclose encounters exert tremendous tidal forces on the sibling planets, possibly promoting active volcanism on the rocky Kepler-36b.

The unlucky planet around a toddler starSmall, black planet in front of a large, orange star. The planet's atmosphere appears to be blowing off in indigo.Small, black planet in front of a large, orange star. The planet's atmosphere appears to be blowing off in indigo.

Small, black planet in front of a large, orange star. The planet’s atmosphere appears to be blowing off in indigo.

The exoplanet AU Microscopii b, located about 32 light-years from Earth, is unlucky enough to have formed a scant 6 million miles (9.6 million km) from its host star — an extremely young, hot, temperamental red dwarf. Estimated to be just 23 million years old, the star is a mere toddler in cosmic terms. (The sun, by comparison, is 4.6 billion years old.) The young star routinely erupts with blasts of radiation thousands of times stronger than the worst solar flares the sun can spit out — and poor AU Microscopii b is often in the firing line. Astronomers have noticed huge globs of planetary material orbiting near the distant world, suggesting that the temperamental star is blasting away pieces of the planet’s atmosphere bit by bit.



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