Exoplanet LTT9779 b orbiting its host star. Image credit: Ricardo Ramírez Reyes (Universidad de Chile)
Aside from the Moon, the brightest object in our night sky is planet Venus, whose thick cloud layer reflects around 75% of the Sun’s light. By comparison, Earth only reflects around 30% of incoming sunlight.
Now for the first time, astronomers have found an exoplanet that can match Venus’ shininess: planet LTT9779 b. New detailed measurements by ESA’s Cheops mission reveal that this planet reflects a whopping 80% of the light shone on it by its host star.
Cheops’ high-precision measurements were a targeted follow-up from the planet’s initial discovery and characterisation in 2020 by NASA’s TESS mission and ground-based instruments such as the ESO HARPS instrument in Chile.
The exoplanet is around the size of Neptune, making it the largest “mirror” in the Universe that we know of today. The reason for its high reflectivity is that metallic clouds cover it. These are mostly silicate – the same stuff that sand and glass are made of – mixed with metals like titanium.
“Imagine a burning world, close to its star, with heavy clouds of metals floating aloft, raining down titanium droplets,” says James Jenkins, astronomer at Diego Portales University and CATA (Santiago, Chile). James co-authored a scientific paper describing the new research, published in the journal Astronomy & Astrophysics today.
Cheops shows scorching exoplanet acts like a mirror. Image credit: ESA (Acknowledgement: work performed by ATG under contract for ESA)
A sky filled with clouds of metal
The fraction of light that an object reflects is called its ‘albedo’. Most planets have a low albedo, either because they have an atmosphere that absorbs a lot of light, or because their surface is dark or rough. Exceptions tend to be frozen ice-worlds, or planets like Venus which have a reflective cloud layer.
LTT9779 b’s high albedo came as a surprise because the planet’s side facing its star is estimated to be around 2000 °C. Any temperature above 100 °C is too hot for clouds of water to form, but the temperature of this planet’s atmosphere should even be too hot for clouds made of metal or glass.
“It was really a puzzle, until we realised we should think about this cloud formation in the same way as condensation forming in a bathroom after a hot shower,” notes Vivien Parmentier, researcher at the Observatory of Côte d’Azur (France) and co-author of this research.
Vivien explains: “To steam up a bathroom you can either cool the air until water vapour condenses, or you can keep the hot water running until clouds form because the air is so saturated with vapour 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 vapours.”
The planet that shouldn’t exist
Being shiny isn’t the only surprising thing about LTT9779 b. Its size and temperature make it a so-called ‘ultra-hot Neptune’, but no other planets of this size and mass have been found to orbit so close to their star. This means it lives in what’s known as the ‘hot Neptune desert’.
The planet has a radius 4.7 times as big as Earth’s, and a year on LTT9779 b takes just 19 hours. All previously discovered planets that orbit their star in less than a day are either ‘hot Jupiters’ – gas giants with a radius at least ten times larger than Earth’s – or rocky planets smaller than two Earth radii.
“It’s a planet that shouldn’t exist,” says Vivien. “We expect planets like this to have their atmosphere blown away by their star, leaving behind bare rock.”
First author Sergio Hoyer of the Marseille Astrophysics Laboratory comments: “’We believe these metal clouds help the planet to survive in the hot Neptune desert. The clouds reflect light and stop the planet from getting too hot and evaporating. Meanwhile, being highly metallic makes the planet and its atmosphere heavy and harder to blow away.”
Studying an exoplanet by looking when it’s hidden
To determine LTT9779 b’s properties, ESA’s exoplanet-characterising Cheops mission looked when the planet moved behind its host star. Because the planet reflects light, the star and planet combined send more light towards the space telescope right before the planet is out of view than right after. The difference in visible light received right before and after the planet is hidden tells you how much light the planet reflects.
This project relied on Cheops’ precision and 24/7 coverage. “Precisely measuring the tiny change in signal from the star eclipsing the planet was only possible with Cheops,” says Sergio.
ESA’s Cheops project scientist Maximilian Günther adds: “Cheops is the first ever space mission dedicated to the follow-up and characterisation of already known exoplanets. Unlike large survey missions focused on discovering new exoplanet systems, Cheops has enough flexibility to focus on interesting targets swiftly and can reach a coverage and precision that we often simply cannot get any other way.”
We get the full picture by looking at the same exoplanet with different instruments. “LTT9779 b is an ideal target for follow-up with the exceptional capabilities of both the Hubble and James Webb space telescopes,” notes ESA science operations scientist Emily Rickman.
“They will allow us to explore this exoplanet with a wider wavelength range including infrared and UV light to understand the composition of its atmosphere better.”
The future of exoplanet research is bright, as Cheops is the first of a trio of dedicated exoplanet missions. It will be joined by Plato in 2026, which will focus on Earth-like planets orbiting at a possibly life-supporting distance from their star. Ariel will join the fleet in 2029 and specialise in studying exoplanet atmospheres.
The extremely high albedo of LTT 9779 b revealed by Cheops by S. Hoyer et al. (2023) is published in Astronomy & Astrophysics. DOI: https://www.aanda.org/10.1051/0004-6361/202346117
Source: European Space Agency
