Skip to main content

Astronomers spot the shiniest exoplanet ever discovered

When you look up at the night sky you see mostly stars, not planets — and that’s simply because planets are so much smaller and dimmer than stars. But you can see planets in our solar system, like Venus, which is one of the brightest objects in the night sky. Due to its thick, dense atmosphere, Venus reflects 75% of the sun’s light, making it shine brightly. Recently, though, astronomers discovered a planet that reflects even more of its star’s light, making it the shiniest exoplanet ever found.

Exoplanet LTT9779 b reflects 80% of the light from its star, which it orbits very close to. That makes it extremely hot, and researchers believe that the planet is covered in clouds of silicate and liquid metal, which is what makes it so reflective.

“Imagine a burning world, close to its star, with heavy clouds of metals floating aloft, raining down titanium droplets,” said one of the researchers, James Jenkins of Diego Portales University, in a statement.

An artist impression of exoplanet LTT9779b orbiting its host star.
An artist impression of exoplanet LTT9779b orbiting its host star. The planet is around the size of Neptune and reflects 80% of the light shone on it, making it the largest known “mirror” in the Universe. This shininess was discovered by detailed measurements made by ESA’s Cheops of the amount of light coming from the planet-star system. Because the planet reflects starlight back to us, the amount of light reaching Cheops’ instruments slightly decreased when the planet moved out of view behind its star. This small decrease could be measured thanks to the high precision of the detectors. Ricardo Ramírez Reyes (Universidad de Chile)

In fact, the planet is so hot that the presence of clouds at all was somewhat befuddling. The surface temperatures there reach up to 2,000 degrees Celsius, which should be too hot for clouds of water or even metals to form.

“It was really a puzzle, until we realized we should think about this cloud formation in the same way as condensation forming in a bathroom after a hot shower,” explained researcher Vivien Parmentier of the Observatory of Côte d’Azur. “To steam up a bathroom you can either cool the air until water vapor condenses, or you can keep the hot water running until clouds form because the air is so saturated with vapor that it simply can’t hold any more. Similarly, LTT9779 b can form metallic clouds despite being so hot because the atmosphere is oversaturated with silicate and metal vapors.”

The planet is also unusual because of its size and location. At 4.7 times the size of the Earth, it is a type of planet called a hot Neptune which is rarely found orbiting so close to its star. “It’s a planet that shouldn’t exist,” said Vivien. “We expect planets like this to have their atmosphere blown away by their star, leaving behind bare rock.”

The researchers theorize that it could be the metallic clouds that have protected the planet’s atmosphere by reflecting light and stopping it from getting too hot, which prevents the atmosphere from being boiled away.

The research is published in the journal Astronomy & Astrophysics.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
First indications of a rare, rainbow ‘glory effect’ on hellish exoplanet
For the first time, potential signs of the rainbow-like ‘glory effect’ have been detected on a planet outside our Solar System. Glory are colourful concentric rings of light that occur only under peculiar conditions. Data from ESA’s sensitive Characterising ExOplanet Satellite, Cheops, along with several other ESA and NASA missions, suggest this delicate phenomenon is beaming straight at Earth from the hellish atmosphere of ultra-hot gas giant WASP-76b, 637 light-years away.

Just from looking at our own solar system, we can see that planets come in a wide variety of colors -- from the dusty red of Mars to the bright blues of Uranus and Neptune. Planets like Jupiter have beautiful bands of color caused by variations in the atmosphere, while it's hard to even see the surface of Venus because its atmosphere is so thick. But there are other variations in color which planets can display, like a stunning rainbow-hued set of circular rings called a glory.

Glories are observed on Earth, and have been seen just once on another planet, Venus. But now, researchers believe they may have identified a glory on a planet outside our solar system for the first time. The extreme exoplanet WASP-76b could be host to the first known extrasolar glory, observed by the European Space Agency (ESA)'s Characterising ExOplanet Satellite (Cheops).

Read more
See planets being born in new images from the Very Large Telescope
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) instrument on ESO’s Very Large Telescope (VLT). The blue regions on the other hand correspond to observations performed with the Atacama Large Millimeter/submillimeter Array (ALMA).

Astronomers have used the Very Large Telescope to peer into the disks of matter from which exoplanets form, looking at more than 80 young stars to see which may have planets forming around them. This is the largest study to date on these planet-forming disks, which are often found within the same huge clouds of dust and gas that stars form within.

A total of 86 young stars were studied in three regions known to host star formation: Taurus and Chamaeleon I, each located around 600 light-years away, and Orion, a famous stellar nursery located around 1,600 light-years away. The researchers took images of the disks around the stars, looking at their structures for clues about how different types of planets can form.

Read more
Three tiny new moons spotted orbiting Uranus and Neptune
Neptune

Our solar system has a few new entries with the recent discovery of three moons of Uranus and Neptune. These ice giant planets are so far away that it is difficult to detect small moons orbiting them, especially when one of the recently discovered moons is the faintest moon ever discovered by a ground-based telescope.

Unlike Jupiter and Saturn, which both have a plethora of moons, Uranus is known to host 28 moons and Neptune just 16. That includes Uranus's new diminutive moon, which is just 5 miles across. Like Uranus' other moons, it will be named after a character from a Shakespeare plays, but a new name has not yet been chosen, so for now it is S/2023 U1.

Read more