The atmosphere of Mars as observed by InSight

Nature Geoscience Springer Nature 13:3 (2020) 190-198

Authors:

Don Banfield, Aymeric Spiga, Claire Newman, François Forget, Mark Lemmon, Ralph Lorenz, Naomi Murdoch, Daniel Viudez-Moreiras, Jorge Pla-Garcia, Raphaël F Garcia, Philippe Lognonné, Özgür Karatekin, Clément Perrin, Léo Martire, Nicholas Teanby, Bart Van Hove, Justin N Maki, Balthasar Kenda, Nils T Mueller, Sébastien Rodriguez, Taichi Kawamura, John B McClean, Alexander E Stott, Constantinos Charalambous, Ehouarn Millour, Catherine L Johnson, Anna Mittelholz, Anni Määttänen, Stephen R Lewis, John Clinton, Simon C Stähler, Savas Ceylan, Domenico Giardini, Tristram Warren, William T Pike, Ingrid Daubar, Matthew Golombek, Lucie Rolland, Rudolf Widmer-Schnidrig, David Mimoun, Éric Beucler, Alice Jacob, Antoine Lucas, Mariah Baker, Véronique Ansan, Kenneth Hurst, Luis Mora-Sotomayor, Sara Navarro, Josefina Torres, Alain Lepinette, Antonio Molina, Mercedes Marin-Jimenez, Javier Gomez-Elvira, Veronica Peinado, Jose-Antonio Rodriguez-Manfredi, Brian T Carcich, Stephen Sackett, Christopher T Russell, Tilman Spohn, Suzanne E Smrekar, W Bruce Banerdt

The seismicity of Mars

Nature Geoscience Springer Nature 13:3 (2020) 205-212

Authors:

D Giardini, P Lognonné, WB Banerdt, WT Pike, U Christensen, S Ceylan, JF Clinton, M van Driel, SC Stähler, M Böse, RF Garcia, A Khan, M Panning, C Perrin, D Banfield, E Beucler, C Charalambous, F Euchner, A Horleston, A Jacob, T Kawamura, S Kedar, G Mainsant, J-R Scholz, SE Smrekar, A Spiga, C Agard, D Antonangeli, S Barkaoui, E Barrett, P Combes, V Conejero, I Daubar, M Drilleau, C Ferrier, T Gabsi, T Gudkova, K Hurst, F Karakostas, S King, M Knapmeyer, B Knapmeyer-Endrun, R Llorca-Cejudo, A Lucas, L Luno, L Margerin, JB McClean, D Mimoun, N Murdoch, F Nimmo, M Nonon, C Pardo, A Rivoldini, JA Rodriguez Manfredi, H Samuel, M Schimmel, AE Stott, E Stutzmann, N Teanby, T Warren, RC Weber, M Wieczorek, C Yana

Color, composition, and thermal environment of Kuiper Belt object (486958) Arrokoth

Science American Association for the Advancement of Science (AAAS) 367:6481 (2020)

Authors:

WM Grundy, MK Bird, DT Britt, JC Cook, DP Cruikshank, CJA Howett, S Krijt, IR Linscott, CB Olkin, AH Parker, S Protopapa, M Ruaud, OM Umurhan, LA Young, CM Dalle Ore, JJ Kavelaars, JT Keane, YJ Pendleton, SB Porter, F Scipioni, JR Spencer, SA Stern, AJ Verbiscer, HA Weaver, RP Binzel, MW Buie, BJ Buratti, A Cheng, AM Earle, HA Elliott, L Gabasova, GR Gladstone, ME Hill, M Horanyi, DE Jennings, AW Lunsford, DJ McComas, WB McKinnon, RL McNutt, JM Moore, JW Parker, E Quirico, DC Reuter, PM Schenk, B Schmitt, MR Showalter, KN Singer, GE Weigle, AM Zangari

The geology and geophysics of Kuiper Belt object (486958) Arrokoth

Science American Association for the Advancement of Science (AAAS) 367:6481 (2020)

Authors:

JR Spencer, SA Stern, JM Moore, HA Weaver, KN Singer, CB Olkin, AJ Verbiscer, WB McKinnon, J Wm Parker, RA Beyer, JT Keane, TR Lauer, SB Porter, OL White, BJ Buratti, MR El-Maarry, CM Lisse, AH Parker, HB Throop, SJ Robbins, OM Umurhan, RP Binzel, DT Britt, MW Buie, AF Cheng, DP Cruikshank, HA Elliott, GR Gladstone, WM Grundy, ME Hill, M Horanyi, DE Jennings, JJ Kavelaars, IR Linscott, DJ McComas, RL McNutt, S Protopapa, DC Reuter, PM Schenk, MR Showalter, LA Young, AM Zangari, AY Abedin, CB Beddingfield, SD Benecchi, E Bernardoni, CJ Bierson, D Borncamp, VJ Bray, AL Chaikin, RD Dhingra, C Fuentes, T Fuse, PL Gay, SDJ Gwyn, DP Hamilton, JD Hofgartner, MJ Holman, AD Howard, CJA Howett, H Karoji, DE Kaufmann, M Kinczyk, BH May, M Mountain, M Pätzold, JM Petit, MR Piquette, IN Reid, HJ Reitsema, KD Runyon, SS Sheppard, JA Stansberry, T Stryk, P Tanga, DJ Tholen, DE Trilling, LH Wasserman

Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

Nature Geoscience Springer Nature 13:3 (2020) 213-220

Authors:

P Lognonné, WB Banerdt, WT Pike, Tarje Nissen-Meyer, Simon Calcutt, Tristram Warren

Abstract:

Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.