The characterization of exoplanetary atmospheres through transit spectra is becoming increasingly feasible, and technology for direct detection remains ongoing.
spectrsocopy
Posted inBiogeochemical Cycles & Geobiology, Biosignatures & Paleobiology, Enceladus, Habitable Zones, Icy Worlds, Imaging & Spectroscopy, Status Report
Sub-Micrometer Particles Remote Detection in Enceladus Plume Based on Cassini’s UV Spectrograph Data
Enceladus is the Saturnian satellite known to have water vapor erupting from its south pole region called Tiger Stripes.