The high-resolution map of Oxia Planum, Mars; the landing site of the ExoMars Rosalind Franklin rover mission

Autor: Peter Fawdon, Csilla Orgel, Solmaz Adeli, Matt Balme, Fred J. Calef, Joel M. Davis, Alessandro Frigeri, Peter Grindrod, Ernst Hauber, Laetitia Le Deit, Damien Loizeau, Andrea Nass, Cathy Quantin-Nataf, Elliot Sefton-Nash, Nick Thomas, Ines Torres, Jorge L. Vago, Matthieu Volat, Sander De Witte, Francesca Altieri, Andrea Apuzzo, Julene Aramendia, Gorka Arana, Rickbir Singh Bahia, Steven G. Banham, Robert Barnes, Alexander M. Barrett, Wolf-Stefan Benedix, Anshuman Bhardwaj, Sarah Jane Boazman, Tomaso R. R. Bontognali, John Bridges, Benjamin Bultel, Valérie Ciarletti, Maria Cristina De Sanctis, Zach Dickeson, Elena A. Favaro, Marco Ferrari, Frédéric Foucher, Walter Goetz, Albert F. C. Haldemann, Elise Harrington, Angeliki Kapatza, Detlef Koschny, Agata M. Krzesinska, Alice Le Gall, Stephen R. Lewis, Tanya Lim, Juan Manuel Madariaga, Benjamin James Man, Lucia Mandon, Nicolas Mangold, Javier Martin-Torres, Joseph D. McNeil, Antonio Molina, Andoni G. Moral, Sara Motaghian, Sergei Nikiforov, Nicolas Oudart, Andrea Pacifici, Adam Parkes Bowen, Dirk Plettemeier, Pantelis Poulakis, Alfiah Rizky Diana Putri, Ottaviano Ruesch, Lydia Sam, Christian Schröder, Christoph Statz, Rebecca Thomas, Daniela Tirsch, Zsuzsanna Toth, Stuart Turner, Martin Voelker, Stephanie C. Werner, Frances Westall, Barry J. Whiteside, Adam Williams, Rebecca M. E. Williams, Jack Wright, Maria-Paz Zorzano

Publikováno v: Journal of Maps, Vol 20, Iss 1 (2024)

ABSTRACTThis 1:30,000 scale geological map describes Oxia Planum, Mars, the landing site for the ExoMars Rosalind Franklin rover mission. The map represents our current understanding of bedrock units and their relationships prior to Rosalind Franklin

Externí odkaz: https://doaj.org/article/d318e2b1c9b2411b8ae23abceaad3914

Atmospheric Retrievals Suggest the Presence of a Secondary Atmosphere and Possible Sulfur Species on L98-59 d from JWST Nirspec G395H Transmission Spectroscopy

Autor: Agnibha Banerjee, Joanna K. Barstow, Amélie Gressier, Néstor Espinoza, David K. Sing, Natalie H. Allen, Stephan M. Birkmann, Ryan C. Challener, Nicolas Crouzet, Carole A. Haswell, Nikole K. Lewis, Stephen R. Lewis, Jingxuan Yang

Publikováno v: The Astrophysical Journal Letters, Vol 975, Iss 1, p L11 (2024)

L 98-59 d is a Super-Earth planet orbiting an M-type star. We performed retrievals on the transmission spectrum of L 98-59 d obtained using NIRSpec G395H during a single transit, from JWST Cycle 1 GTO 1224. The wavelength range of this spectrum allow

Externí odkaz: https://doaj.org/article/d1fc4c64ee6b42a7ab9ccdd1cff70132

Enhanced Super‐Rotation Before and During the 2018 Martian Global Dust Storm

Autor: Kylash Rajendran, Stephen R. Lewis, James A. Holmes, Paul M. Streeter, Anna A. Fedorova, Manish R. Patel

Publikováno v: Geophysical Research Letters, Vol 48, Iss 16, Pp n/a-n/a (2021)

Abstract Super‐rotation affects—and is affected by—the distribution of dust in the martian atmosphere. We modeled this interaction during the 2018 global dust storm (GDS) of Mars Year 34 using data assimilation. Super‐rotation increased by a

Externí odkaz: https://doaj.org/article/6686df7a7feb4b85a78d2e7b15f3fd68

Effect of Centrifugal Force on Transmission Spectroscopy of Exoplanet Atmospheres

Autor: Agnibha Banerjee, Joanna K Barstow, Carole A Haswell, Stephen R Lewis

Transmission spectroscopy is one of the most successful methods of learning about exoplanet atmospheres. The process of retrievals using transmission spectroscopy consists of creating numerous forward models and comparing them to observations to solv

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f0c1296e710cebb017907d5fb55c32f
http://arxiv.org/abs/2305.08610

Eskers associated with buried glaciers in Mars' mid latitudes: recent advances and future directions

Autor: Frances E. G. Butcher, Neil S. Arnold, Matthew R. Balme, Susan J. Conway, Christopher D. Clark, Colman Gallagher, Axel Hagermann, Stephen R. Lewis, Alicia M. Rutledge, Robert D. Storrar, Savana Z. Woodley

Until recently, the influence of basal liquid water on the evolution of buried glaciers in Mars' mid latitudes was assumed to be negligible because the latter stages of Mars' Amazonian period (3 Ga to present) have long been thought to have been simi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be1fdbd4b023f5124247917f46065457