Secondary Atmosphere Of Distant Planets
According to a new analysis of Hubble Space Telescope observations gathered in 2017, scientists think that the exoplanet GJ-1132b lost its atmosphere – and then conjured itself a new one. After GJ-1132b lost its hydrogen and helium-rich preliminary atmosphere due to the intense radiation of the star it orbits, it became a bare world. However, GJ-1132b is tidally locked – its parent star, a red dwarf, pulls it strongly enough to keep the same side of the planet facing it, thereby dramatically heating the planet, leading to volcanic activity.
The new secondary atmosphere, then, is suspected to be borne of gases leaching out of molten rock on the planet. The Hubble’s observations suggest that today, GJ-1132b is swathed in a mix of hydrogen, hydrogen cyanide, methane, and aerosol-rich haze resembling earth’s smog.