Ancient and present surface evolution processes in the Ash region of comet 67P/Churyumov-Gerasimenko

Autor: Laurent Jorda, François Costard, A. Bouquety, Sylvain Bouley, A. Séjourné, Olivier Groussin
Přispěvatelé: Géosciences Paris Saclay (GEOPS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Jazyk: angličtina
Rok vydání: 2021
Předmět:
010504 meteorology & atmospheric sciences
Comet
FOS: Physical sciences
Detailed data
surfaces
01 natural sciences
Physics - Geophysics
0103 physical sciences
Cliff
comets
individual
Digital elevation model
010303 astronomy & astrophysics
Geomorphology
ComputingMilieux_MISCELLANEOUS
0105 earth and related environmental sciences
Earth and Planetary Astrophysics (astro-ph.EP)
geography
geography.geographical_feature_category
67P/Churyumov-Gerasimenko -methods
Astronomy and Astrophysics
Landslide
data analysis -planets and satellites
Geophysics (physics.geo-ph)
Morphometric analysis
13. Climate action
Space and Planetary Science
[SDU]Sciences of the Universe [physics]
Physics - Data Analysis
Statistics and Probability

Geology
Data Analysis
Statistics and Probability (physics.data-an)

Astrophysics - Earth and Planetary Astrophysics
Zdroj: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, In press, ⟨10.1051/0004-6361/202140516⟩
Astronomy and Astrophysics-A&A, 2021, 649, ⟨10.1051/0004-6361/202140516⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, ⟨10.1051/0004-6361/202140516⟩
ISSN: 0004-6361
DOI: 10.1051/0004-6361/202140516⟩
Popis: Aims. The Rosetta mission provided us with detailed data of the surface of the nucleus of comet 67P/Churyumov-Gerasimenko. In order to better understand the physical processes associated with the comet activity and the surface evolution of its nucleus, we performed a detailed comparative morphometrical analysis of two depressions located in the Ash region. Methods. To detect morphological temporal changes, we compared pre- and post-perihelion high-resolution (pixel scale of 0.07–1.75 m) OSIRIS images of the two depressions. We quantified the changes using the dynamic heights and the gravitational slopes calculated from the digital terrain model of the studied area. In particular, we measured seven geometric parameters associated with the two depressions (length, three width values, height, area, and volume) using the ArcGIS software before and after perihelion. Results. Our comparative morphometrical analysis allowed us to detect and quantify the temporal changes that occurred in two depressions of the Ash region during the last perihelion passage. We find that the two depressions grew by several meters. The area of the smallest depression (structure I) increased by 90 ± 20%, with two preferential growths: one close to the cliff associated with the apparition of new boulders at its foot, and a second one on the opposite side of the cliff. The largest depression (structure II) grew in all directions, increasing in area by 20 ± 5%, and no new deposits have been detected. We interpreted these two depression changes as being driven by the sublimation of ices, which explains their global growth and which can also trigger landslides. The deposits associated with depression II reveal a stair-like topography, indicating that they have accumulated during several successive landslides from different perihelion passages. Overall, these observations bring additional evidence of complex active processes and reshaping events occurring on short timescales (months to years), such as depression growth and landslides, and on longer timescales (decades to millenniums), such as cliff retreat.
Databáze: OpenAIRE