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)

Authors:

Paul G Lucey, Benjamin Greenhagen, Kerri Donaldson Hanna, Neil Bowles, Abigail Flom, David A Paige

Origins space telescope: from first light to life

Experimental Astronomy Springer Nature 51:3 (2021) 595-624

Authors:

MC Wiedner, S Aalto, L Armus, E Bergin, J Birkby, CM Bradford, D Burgarella, P Caselli, V Charmandaris, A Cooray, E De Beck, JM Desert, M Gerin, J Goicoechea, M Griffin, P Hartogh, F Helmich, M Hogerheijde, L Hunt, A Karska, Q Kral, D Leisawitz, G Melnick, M Meixner, M Matsuura, S Milam, C Pearson, DW Pesce, KM Pontoppidan, A Pope, D Rigopoulou, T Roellig, I Sakon, J Staguhn, K Stevenson

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)

Authors:

C Charalambous, JB McClean, M Baker, WT Pike, M Golombek, M Lemmon, V Ansan, C Perrin, A Spiga, RD Lorenz, ME Banks, N Murdoch, S Rodriguez, CM Weitz, JA Grant, NH Warner, J Garvin, IJ Daubar, E Hauber, AE Stott, CL Johnson, A Mittelholz, T Warren, S Navarro, LM Sotomayor, J Maki, A Lucas, D Banfield, C Newman, D Viúdez‐Moreiras, J Pla‐García, P Lognonné, WB Banerdt

System-level fractionation of carbon from disk and planetesimal processing

Astrophysical Journal Letters American Astronomical Society 913:2 (2021) L20

Authors:

Tim Lichtenberg, Sebastiaan Krijt

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

Authors:

Denis A Belyaev, Anna A Fedorova, Alexander Trokhimovskiy, Juan Alday, Franck Montmessin, Oleg I Korablev, Franck Lefevre, Andrey S Patrakeev, Kevin S Olsen, Alexey V Shakun

Abstract:

We present the first water vapor profiles encompassing the upper mesosphere of Mars, 100–120 km, far exceeding the maximum altitudes where remote sensing has been able to observe water to date. Our results are based on solar occultation measurements by Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter (TGO). The observed wavelength range around 2.7 μm possesses strong CO2 and H2O absorption lines allowing sensitive temperature and density retrievals. We report a maximum H2O mixing ratio varying from 10 to 50 ppmv at 100–120 km during the global dust storm (GDS) of Martian Year (MY) 34 and around southern summer solstice of MY 34 and 35. During other seasons water remains persistently below ∼2 ppmv. We claim that contributions of the MY34 GDS and perihelion periods into the projected hydrogen escape from Mars are nearly equivalent.