Skip to main content

All the weird and wonderful exoplanets CHEOPS investigated in its first year

Illustration of CHEOPS, ESA’s first exoplanet mission
Illustration of CHEOPS, ESA’s first exoplanet mission ESA / ATG medialab

This week marks the one-year anniversary of the launch of CHEOPS, the European Space Agency’s exoplanet investigation satellite. CHEOPS looks at known exoplanets discovered by other missions and probes them in more detail, uncovering new information about these distant worlds. Here’s what it discovered in its first year:

Blurry stars

The first image taken by CHEOPS in February this year was not in fact of a planet, but a star — HD 70843, located 150 light-years away. The telescope took a deliberately blurry picture of this particularly bright star to check its brightness was properly detected, and all boded well.

Recommended Videos

CHEOPS also imaged another star, HD 88111, which doesn’t host any known exoplanets, but was useful as a test. That’s because CHEOPS detect exoplanets by looking at stars and waiting for planets to pass in front of them, in an event called a transit. By observing the star dimming by a tiny amount, scientists can infer the presence of an exoplanet and calculate properties like its size and orbital period.

A wispy puff

Artist's impression of the star HD 93396 and its hot Jupiter planet, KELT-11b.
Artist’s impression of the star HD 93396 and its hot Jupiter planet, KELT-11b. ESA

With the instruments confirmed to be working well, CHEOPS detected its first exoplanet in April this year. It looked to the star HD 93396, located 320 light-years away, around which orbits a planet called KELT-11b. KELT-11b is a large gas giant, being about a third larger than Jupiter but only one-fifth of its mass. That makes it one of the “puffiest planets” discovered so far.

CHEOPS was able to observe an eight-hour-long transit of the planet and to detect its size more accurately than any instrument before, pinning its diameter down to 181,600 km with an uncertainty of just 4,300 km.

Scorchingly hot

Artist impression of WASP-189
Artist impression of WASP-189 b ESA

In September this year, CHEOPS investigated a “hot Jupiter” called WASP-189 b, which turned out to be one of the most extreme planets ever found. It sits so close to its star that a year there lasts just 2.7 days, with its orbit being twenty times closer to the star than Earth is to the sun. Not only that, but its host star, WASP-189, is 2,000 degrees hotter than the sun, which so incredibly hot that it appears to glow blue.

That makes WASP-189 b one of the few known planets to orbit a star this hot and this bright. The researchers estimate that the temperatures on the planet would be a scorching 3,200 degrees Celsius, which is hot enough to not only melt metals but also to turn them into gas. It also orbits at an unusual inclination, passing over the star’s poles rather than its equator.

A dramatic dodge

CHEOPS also had a close call in October this year, when it had to evade a piece of space debris. If the debris had collided with the satellite it could have destroyed it entirely, according to Willy Benz, head of the CHEOPS consortium. Fortunately, CHEOPS was able to maneuver out of the way and avoid the incoming debris.

With this exciting first year under its belt, CHEOPS will move on to studying hundreds of known exoplanets in the next few years, gathering more accurate information about them and learning new things about these strange, distant worlds.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
This exoplanet is over 2,000-degrees Celsius, has vaporized metal in its atmosphere
This artist impression illustrates how astronomers using the Gemini North telescope, one half of the International Gemini Observatory operated by NSF’s NOIRLab, have made multiple detections of rock-forming elements in the atmosphere of a Jupiter-sized exoplanet, WASP-76b. The so-called “hot Jupiter” is perilously close to its host star, which is heating the planet’s atmosphere to astounding temperatures and vaporized rock-forming elements such as magnesium, calcium and iron, providing insight into how our own Solar System formed.

Astronomers have studied a strange, puffy, scorching-hot planet located 600 light-years away, and have seen elements that would normally form rocks, but are so hot that they have vaporized into the atmosphere.

The planet, named WASP-76b, is around the mass of Jupiter, but orbits its star 12 times closer than Mercury is to the sun. Being so close, its atmosphere its heated to a scorching 2,000- degrees Celsius, which makes it puff up to a large size that's six times the volume of Jupiter. These high temperatures also give astronomers the opportunity to observe elements that would normally be hard to identify in the atmosphere of a gas giant.

Read more
CHEOPS planet-hunter detects four rarely seen mini-Neptunes
Artist's impression of Cheops, ESA's Characterising Exoplanet Satellite, in orbit above Earth.

The European Space Agency (ESA)'s CHEOPS satellite has discovered four new exoplanets -- and they are a hard-to-detect type called a mini-Neptune. These planets are notable because they are the "missing link" between rocky Earth-sized planets and ice giants like Neptune. They are thought to be very common in our galaxy, but they are hard to spot because they are small and cool compared to the big, bright hot Jupiters which are most commonly detected by exoplanet-hunting telescopes.

Mini-Neptunes do orbit close to their stars, typically being found closer to their stars than Mercury is to the sun. However, hot Jupiters orbit even closer -- which gives them very high surface temperatures of over 1,000 degrees Celsius. Mini-Neptunes have relatively cooler surface temperatures of around 300 degrees Celsius.

Read more
James Webb spots exoplanet with gritty clouds of sand floating in its atmosphere
This illustration conceptualises the swirling clouds identified by the James Webb Space Telescope in the atmosphere of the exoplanet VHS 1256 b. The planet is about 40 light-years away and orbits two stars that are locked in their own tight rotation. Its clouds, which are filled with silicate dust, are constantly rising, mixing, and moving during its 22-hour day.

One of the most exciting things about the James Webb Space Telescope is that not only can it detect exoplanets, but it can even peer into their atmospheres to see what they are composed of. Understanding exoplanet atmospheres will help us to find potentially habitable worlds, but it will also turn up some fascinating oddities -- like a recent finding of an exoplanet with an atmosphere full of gritty, sand clouds.

Exoplanet VHS 1256 b, around 40 light-years away, has a complex and dynamic atmosphere that shows considerable changes over a 22-hour day. Not only does the atmosphere show evidence of commonly observed chemicals like water, methane, and carbon monoxide, but it also appears to be dotted with clouds made up of silicate grains.

Read more