Rocky exoplanet of Moon or Mercury
- The observation marks the first time that Spitzer telescope’s data has been able to provide details about the atmosphere of a terrestrial world around an M dwarf star, NASA’s Jet Propulsion Laboratory (JPL) announced in a release.
- Published in the Nature journal, the study is titled Absence of a Thick Atmosphere on the Terrestrial Exoplanet LHS 3844b.
- This study has found out that LHS 3844b planet is likely to lack atmosphere, and says that its surface may resemble that of the Earth’s Moon or the Mercury. It is also said that LHS 3844b could be covered in the same cooled volcanic material found in the dark areas of the surface of the Moon, called mare.
- The LHS 3844b planet was discovered in 2018 by NASA’s Transiting Exoplanet Satellite Survey (TESS) mission through the transit method, which involves detecting when the observed light of a parent star dims due to a planet which is orbiting is between the star and Earth.
- Detecting light coming directly from a planet’s surface – another method – is difficult because the star is so much brighter and drowns out the planet’s light.
- During its follow-up observations, the Spitzer telescope was able to detect light from the surface of LHS 3844b. The planet makes one full revolution around its parent star in only 11 hours.
- With such tight orbit, the LHS 3844b planet is most likely to be “tidally locked,” which means that when one side of a planet is permanently facing the star.
- The side which is facing towards the star, or dayside, has a temperature of about 1,410 degrees Fahrenheit (770 degrees Celsius). Because it is extremely hot, the LHS 3844b planet radiates a lot of infrared light, which could be observed by the Spitzer telescope because it is an infrared telescope.
- Though the parent star is cool, it is still comparatively much hotter than the planet, so making direct observation of LHS 3844b’s dayside possible.
- By measuring the temperature difference between the hot and cold sides of the LHS 3844b, the team was able to find that there is a negligible amount of heat being transferred between the two.
- If the planet had an atmosphere, the hot air on the dayside would naturally expand, generating winds that would transfer heat around the planet. With a rocky surface and little to no atmosphere, there is no air present to transfer the heat.
- The presence of an atmosphere on the Earth is the reason liquid water can exist on the surface, enabling life on the planet. On the other hand, the atmospheric pressure of Mars is now less than 1 per cent of that of the Earth, and the oceans and rivers that once dotted the Red Planet’s surface have disappeared.
- In comparison to Sun-like stars, M dwarfs stars emit high levels of ultraviolet (UV) light, which is harmful to life and can erode a planet’s atmosphere. They’re particularly violent in their youth, belching up a large number of flares, or bursts of radiation and particles that could strip away budding planetary atmospheres.