Detecting and characterizing the atmospheres of rocky exoplanets has proven to be challenging for JWST. Transit spectroscopy of the TRAPPIST-1 planets has been impacted by the effects of spots and faculae on the host star. Secondary eclipses have detected hot rocks, but evidence for atmospheres has been difficult to obtain. However, there is a third [...]The post The Third Option: Color Phase Curves to Characterize the Atmospheres of Temperate Rocky Exoplanets appeared first on Astrobiology.
The Third Option: Color Phase Curves to Characterize the Atmospheres of Temperate Rocky Exoplanets
