Christiansen Feature Map From the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment: Improved Corrections and Derived Mineralogy
Journal of Geophysical Research Planets American Geophysical Union (AGU) 126:6 (2021)
Origins space telescope: from first light to life
Experimental Astronomy Springer Nature 51:3 (2021) 595-624
Vortex‐Dominated Aeolian Activity at InSight's Landing Site, Part 1: Multi‐Instrument Observations, Analysis, and Implications
Journal of Geophysical Research Planets American Geophysical Union (AGU) 126:6 (2021)
System-level fractionation of carbon from disk and planetesimal processing
Astrophysical Journal Letters American Astronomical Society 913:2 (2021) L20
Abstract:
Finding and characterizing extrasolar Earth analogs will rely on interpretation of the planetary system's environmental context. The total budget and fractionation between C-H-O species sensitively affect the climatic and geodynamic state of terrestrial worlds, but their main delivery channels are poorly constrained. We connect numerical models of volatile chemistry and pebble coagulation in the circumstellar disk with the internal compositional evolution of planetesimals during the primary accretion phase. Our simulations demonstrate that disk chemistry and degassing from planetesimals operate on comparable timescales and can fractionate the relative abundances of major water and carbon carriers by orders of magnitude. As a result, individual planetary systems with significant planetesimal processing display increased correlation in the volatile budget of planetary building blocks relative to no internal heating. Planetesimal processing in a subset of systems increases the variance of volatile contents across planetary systems. Our simulations thus suggest that exoplanetary atmospheric compositions may provide constraints on when a specific planet formed.Revealing a high water abundance in the upper mesosphere of Mars with ACS onboard TGO
Geophysical Research Letters Wiley 48:10 (2021) e2021GL093411