Planetary surfaces

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Ground-breaking Exoplanet Science with the ANDES spectrograph at the ELT

(2023)

Authors:

Enric Palle, Katia Biazzo, Emeline Bolmont, Paul Molliere, Katja Poppenhaeger, Jayne Birkby, Matteo Brogi, Gael Chauvin, Andrea Chiavassa, Jens Hoeijmakers, Emmanuel Lellouch, Christophe Lovis, Roberto Maiolino, Lisa Nortmann, Hannu Parviainen, Lorenzo Pino, Martin Turbet, Jesse Wender, Simon Albrecht, Simone Antoniucci, Susana C Barros, Andre Beaudoin, Bjorn Benneke, Isabelle Boisse, Aldo S Bonomo, Francesco Borsa, Alexis Brandeker, Wolfgang Brandner, Lars A Buchhave, Anne-Laure Cheffot, Robin Deborde, Florian Debras, Rene Doyon, Paolo Di Marcantonio, Paolo Giacobbe, Jonay I Gonzalez Hernandez, Ravit Helled, Laura Kreidberg, Pedro Machado, Jesus Maldonado, Alessandro Marconi, BL Canto Martins, Adriano Miceli, Christoph Mordasini, Mamadou N'Diaye, Andrezj Niedzielski, Brunella Nisini, Livia Origlia, Celine Peroux, Alex GM Pietrow, Enrico Pinna, Emily Rauscher, Sabine Reffert, Philippe Rousselot, Nicoletta Sanna, Adrien Simonnin, Alejandro Suarez Mascareno, Alessio Zanutta, Mathias Zechmeister
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The radiometric environment for Mars limb observations by the Mars Sample Return Earth Return Orbiter

Advances in Space Research Elsevier 72:9 (2023) 4048-4063

Authors:

Marek Slipski, Armin Kleinböhl, Daniela Tirsch, Gerhard Kminek, Gregory Jonniaux, Klaus-Dieter Matz, Anni Määttänen, Austin Nicholas, Franck Montmessin, Soren N Madsen, Matthew Abrahamson, Manuel Sanchez-Gestido, Michael A Mischna, Neil Paul Murray, Michael J Wolff, Pierre Blanc-Paques, Fabrice Cipriani, Colin F Wilson, Dmitri Titov, Richard Zurek
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Correction to: Venus Evolution Through Time: Key Science Questions, Selected Mission Concepts and Future Investigations

Space Science Reviews Springer 219:8 (2023) 72

Authors:

Thomas Widemann, Suzanne E Smrekar, James B Garvin, Anne Grete Straume-Lindner, Adriana C Ocampo, Mitchell D Schulte, Thomas Voirin, Scott Hensley, M Darby Dyar, Jennifer L Whitten, Daniel C Nunes, Stephanie A Getty, Giada N Arney, Natasha M Johnson, Erika Kohler, Tilman Spohn, Joseph G O’Rourke, Colin F Wilson, Michael J Way, Colby Ostberg, Frances Westall, Dennis Höning, Seth Jacobson, Arnaud Salvador, Guillaume Avice

Abstract:

In the original publication, there has been a discrepancy between values mentioned in the text of Sect. 4.3.3 and in Table 1. The corrected version is provided here: Wrong: The gravity field harmonic coefficients up to an average degree strength of 130 (∼145 km) are generated together with corrections to the spin rate and to the pole right ascension and declination. Correct: The gravity field harmonic coefficients up to an average degree strength of 200 (∼105 km, see Table 1) are generated together with corrections to the spin rate and to the pole right ascension and declination.
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A Tectonic Origin for the Largest Marsquake Observed by InSight

Geophysical Research Letters American Geophysical Union (AGU) 50:20 (2023)

Authors:

Benjamin Fernando, Ingrid J Daubar, Constantinos Charalambous, Peter M Grindrod, Alexander Stott, Abdullah Al Ateqi, Dimitra Atri, Savas Ceylan, John Clinton, Matthew Fillingim, Ernest Hauber, Jonathon R Hill, Taichi Kawamura, Jianjun Liu, Antoine Lucas, Ralph Lorenz, Lujendra Ojha, Clement Perrin, Sylvain Piqueux, Simon Stähler, Daniela Tirsch, Colin Wilson, Natalia Wójcicka, Domenico Giardini, Philippe Lognonné, W Bruce Banerdt
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L’Ralph: A Visible/Infrared Spectral Imager for the Lucy Mission to the Trojans

Space Science Reviews Springer 219:8 (2023) 69

Authors:

DC Reuter, AA Simon, A Lunsford, H Kaplan, M Garrison, J Simpson, G Casto, Z Dolch, P Finneran, W Grundy, C Howett, P Kim, M Loose, T Null, F Parong, J Rodriguez-ruiz, P Roming, K Smith, P Thompson, B Tokarcik, T Veach, S Wall, J Ward, E Weigle, H Levison

Abstract:

Abstract The Lucy Mission to the Trojan asteroids in Jupiter’s orbit carries an instrument named L’Ralph, a visible/near infrared multi-spectral imager and a short wavelength infrared hyperspectral imager. It is one of the core instruments on Lucy, NASA’s first mission to the Trojans. L’Ralph’s primary purpose is to map the surface geology and composition of these objects, but it will also be used to search for possible tenuous exospheres. It is compact, low mass (32.3 kg), power efficient (24.5 W), and robust with high sensitivity and excellent imaging. These characteristics, and its high degree of redundancy, make L’Ralph ideally suited to this long-duration multi-flyby reconnaissance mission.
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