Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling

Abstract During its first seven years of operation, the Sample Analysis at Mars Tunable Laser Spectrometer (TLS) on board the Curiosity rover has detected seven methane spikes above a low background abundance in Gale crater. The methane spikes are likely sourced by surface emission within or around...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Y. Luo, M. A. Mischna, J. C. Lin, B. Fasoli, X. Cai, Y. L. Yung
Formato: article
Lenguaje:EN
Publicado: American Geophysical Union (AGU) 2021
Materias:
MSL
TLS
TGO
Acceso en línea:https://doaj.org/article/420e0bb444864c81b53e8d26dc64c8d2
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:420e0bb444864c81b53e8d26dc64c8d2
record_format dspace
spelling oai:doaj.org-article:420e0bb444864c81b53e8d26dc64c8d22021-11-23T21:03:07ZMars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling2333-508410.1029/2021EA001915https://doaj.org/article/420e0bb444864c81b53e8d26dc64c8d22021-11-01T00:00:00Zhttps://doi.org/10.1029/2021EA001915https://doaj.org/toc/2333-5084Abstract During its first seven years of operation, the Sample Analysis at Mars Tunable Laser Spectrometer (TLS) on board the Curiosity rover has detected seven methane spikes above a low background abundance in Gale crater. The methane spikes are likely sourced by surface emission within or around Gale crater. Here, we use inverse Lagrangian modeling techniques to identify upstream emission regions on the Martian surface for these methane spikes at an unprecedented spatial resolution. Inside Gale crater, the northwestern crater floor casts the strongest influence on the detections. Outside Gale crater, the upstream regions common to all the methane spikes extend toward the north. The contrasting results from two consecutive TLS methane measurements performed on the same sol point to an active emission site to the west or the southwest of the Curiosity rover on the northwestern crater floor. The observed spike magnitude and frequency also favor emission sites on the northwestern crater floor, unless there are fast methane removal mechanisms at work, or either the methane spikes of TLS or the non‐detections of ExoMars Trace Gas Orbiter cannot be trusted.Y. LuoM. A. MischnaJ. C. LinB. FasoliX. CaiY. L. YungAmerican Geophysical Union (AGU)articleMarsmethaneback trajectoryMSLTLSTGOAstronomyQB1-991GeologyQE1-996.5ENEarth and Space Science, Vol 8, Iss 11, Pp n/a-n/a (2021)
institution DOAJ
collection DOAJ
language EN
topic Mars
methane
back trajectory
MSL
TLS
TGO
Astronomy
QB1-991
Geology
QE1-996.5
spellingShingle Mars
methane
back trajectory
MSL
TLS
TGO
Astronomy
QB1-991
Geology
QE1-996.5
Y. Luo
M. A. Mischna
J. C. Lin
B. Fasoli
X. Cai
Y. L. Yung
Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
description Abstract During its first seven years of operation, the Sample Analysis at Mars Tunable Laser Spectrometer (TLS) on board the Curiosity rover has detected seven methane spikes above a low background abundance in Gale crater. The methane spikes are likely sourced by surface emission within or around Gale crater. Here, we use inverse Lagrangian modeling techniques to identify upstream emission regions on the Martian surface for these methane spikes at an unprecedented spatial resolution. Inside Gale crater, the northwestern crater floor casts the strongest influence on the detections. Outside Gale crater, the upstream regions common to all the methane spikes extend toward the north. The contrasting results from two consecutive TLS methane measurements performed on the same sol point to an active emission site to the west or the southwest of the Curiosity rover on the northwestern crater floor. The observed spike magnitude and frequency also favor emission sites on the northwestern crater floor, unless there are fast methane removal mechanisms at work, or either the methane spikes of TLS or the non‐detections of ExoMars Trace Gas Orbiter cannot be trusted.
format article
author Y. Luo
M. A. Mischna
J. C. Lin
B. Fasoli
X. Cai
Y. L. Yung
author_facet Y. Luo
M. A. Mischna
J. C. Lin
B. Fasoli
X. Cai
Y. L. Yung
author_sort Y. Luo
title Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
title_short Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
title_full Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
title_fullStr Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
title_full_unstemmed Mars Methane Sources in Northwestern Gale Crater Inferred From Back Trajectory Modeling
title_sort mars methane sources in northwestern gale crater inferred from back trajectory modeling
publisher American Geophysical Union (AGU)
publishDate 2021
url https://doaj.org/article/420e0bb444864c81b53e8d26dc64c8d2
work_keys_str_mv AT yluo marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
AT mamischna marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
AT jclin marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
AT bfasoli marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
AT xcai marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
AT ylyung marsmethanesourcesinnorthwesterngalecraterinferredfrombacktrajectorymodeling
_version_ 1718416089193381888