Using the James Webb Space Telescope (JWST), astronomers have detected carbon dioxide and hydrogen peroxide on the frozen surface of Pluto’s largest moon, Charon. Detecting these molecules could tell scientists how Charon and other icy bodies at the solar system’s edge were born.
Since its discovery in 1978, Charon has been extensively studied — but previous research has been limited in terms of what wavelengths of light could be explored during these analyses. That left gaps in our understanding of the surface composition of this moon of Pluto. As a result, though scientists have detected water ice, ammonia-bearing species and organic compounds on Charon, carbon dioxide and hydrogen peroxide have evaded detection. Until now, that is.
The team, led by Silvia Protopapa of the Southwest Research Institute (SwRI), filled in these gaps by studying Charon with the JWST‘s Near-Infrared Spectrograph (NIRSpec) instrument.
“Our research reveals that Charon’s surface preserves evidence of its
formation through the presence of carbon dioxide, as well as signs of irradiation processes, indicated by the presence of hydrogen peroxide,” Protopapa told Space.com. “These discoveries expand Charon’s known compositional inventory, which includes water ice, ammonia-bearing species and organic materials responsible for its gray and red coloration.”
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Source www.space.com
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