Evidence for disequilibrium chemistry from vertical mixing in hot Jupiter atmospheres: A comprehensive survey of transiting close-in gas giant exoplanets with warm-Spitzer/IRAC
ASTRONOMY & ASTROPHYSICS 648 (2021) ARTN A127
Upper limits for phosphine (PH3) in the atmosphere of Mars
Astronomy and Astrophysics EDP Sciences 649:May 2021 (2021) L1
Abstract:
Phosphine (PH3) is proposed to be a possible biomarker in planetary atmospheres and has been claimed to have been observed in the atmosphere of Venus, sparking interest in the habitability of Venus’s atmosphere. Observations of another biomarker, methane (CH4), have been reported several times in the atmosphere of Mars, hinting at the possibility of a past or present biosphere. The Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter has a spectral range that includes several absorption lines of PH3 with line strengths comparable to previously observed CH4 lines. The signature of PH3 was not observed in the 192 observations made over a full Martian year of observations, and here we report upper limits of 0.1–0.6 ppbv.Lucy Mission to the Trojan Asteroids: Instrumentation and Encounter Concept of Operations
(2021)
Persephone: A Pluto-system Orbiter and Kuiper Belt Explorer
The Planetary Science Journal American Astronomical Society 2:2 (2021) 75
A Comodulation Analysis of Atmospheric Energy Injection Into the Ground Motion at InSight, Mars
Journal of Geophysical Research Planets American Geophysical Union (AGU) 126:4 (2021)