Scientists Find Out Why Some Distant Planets Have Clouds of Sands in Their Atmosphere

The study used observations of brown dwarfs made by NASA’s retired Spitzer Space Telescope.

Scientists Find Out Why Some Distant Planets Have Clouds of Sands in Their Atmosphere

Photo Credit: NASA/JPL-Caltech

Spitzer telescope spotted traces of silica clouds in the atmosphere of some brown dwarfs

Highlights
  • The formation of any type of cloud is the same
  • Once the ingredient is trapped and cooled down, clouds are created
  • The same principle is involved in the formation of silica clouds

While clouds are made of water on Earth, their composition is quite different on other distant planets. Scientists have noted that some of these planets have sand clouds of silicates but could not unravel the conditions under which they are formed. Now, a new study has revealed the common trait that is conducive to sand cloud development. Led by researchers at the Western University, the study used observations of brown dwarfs made by NASA's retired Spitzer Space Telescope. Brown dwarfs are celestial bodies having size larger than a planet but smaller than a star.

“Understanding the atmospheres of brown dwarfs and planets where silicate clouds can form can also help us understand what we would see in the atmosphere of a planet that's closer in size and temperature to Earth,” said Stanimir Metchev, a professor of exoplanet studies at Western University in London, Ontario, and co-author of the study.

The formation of any type of cloud is the same where the key ingredient gets heated up to form vapours. Once the ingredient — which can be anything from water, salt, sulphur, or ammonia — is trapped and cooled down, clouds are created.

The same principle is involved in the formation of silica clouds but as rock requires a high temperature to vaporise, such clouds are only found on hot celestial bodies like brown dwarfs. Researchers have used incorporated the brown dwarfs in their study as many of them have atmospheres similar to that of gas-dominated planets like Jupiter.

The Spitzer telescope had already spotted traces of silica clouds in the atmosphere of some brown dwarfs. However, the evidence wasn't concrete enough. In the new study, researchers made use of over 100 of the detections and grouped them in accordance with the temperature of the brown dwarf. This helped them unearth a definitive trait and the temperature range in which silica clouds are formed.

“We had to dig through the Spitzer data to find these brown dwarfs where there was some indication of silicate clouds, and we really didn't know what we would find,” said lead author Genaro Suarez.


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