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Selection and Characteristics of the Dragonfly Landing Site near Selk Crater, Titan

Authors :
Alyssa Werynski
Jason W. Barnes
Alice Le Gall
J. E. Hedgepeth
Catherine D. Neish
Erich Karkoschka
Shannon MacKenzie
Elizabeth P. Turtle
Melissa G. Trainer
Ralph D. Lorenz
Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL)
Department of Earth Sciences [London, ON]
University of Western Ontario (UWO)
Planetary Science Institute [Tucson] (PSI)
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Department of Physics [Moscow,USA]
University of Idaho [Moscow, USA]
NASA Goddard Space Flight Center (GSFC)
Lunar and Planetary Laboratory [Tucson] (LPL)
University of Arizona
Source :
The Planetary Science Journal, The Planetary Science Journal, IOP Science, 2021, 2 (1), pp.24. ⟨10.3847/PSJ/abd08f⟩
Publication Year :
2021
Publisher :
American Astronomical Society, 2021.

Abstract

The factors contributing to the initial selection of a dune site near the Selk impact structure on Titan as the first landing site for the Dragonfly mission are described. These include arrival geometry and aerodynamic/aerothermodynamic considerations, illumination, and Earth visibility, as well as the likely presence of exposed deposits of water-rich material, potentially including materials where molten ice has interacted with organics. Cassini observations of Selk are summarized and interpreted: near-infrared reflectance and microwave emission data indicate water-rich materials in and around the crater. Radar topography data shows the rim of Selk to have slopes on multi-km scales reaching only ∼2° degrees, an order of magnitude shallower than early photoclinometric estimates.

Details

ISSN :
26323338
Volume :
2
Database :
OpenAIRE
Journal :
The Planetary Science Journal
Accession number :
edsair.doi.dedup.....cfa40321956ebd531f77955744b16361
Full Text :
https://doi.org/10.3847/psj/abd08f