Seasonal Changes In Hydrogen Escape From Mars through Analysis of HST Observations of the Martian Exosphere Near Perihelion

D. Bhattacharyya; J. T. Clarke; Jean-Yves Chaufray; M. Mayyasi; Jean-Loup Bertaux; M. S. Chaffin; N. M. Schneider; G. L. Villanueva

Seasonal Changes In Hydrogen Escape From Mars through Analysis of HST Observations of the Martian Exosphere Near Perihelion

D. Bhattacharyya ¹ J. T. Clarke ¹ Jean-Yves Chaufray ² M. Mayyasi ³ Jean-Loup Bertaux ² M. S. Chaffin ⁴ N. M. Schneider ⁴ G. L. Villanueva ⁵

1 CSP - Center for Space Physics [Boston]

2 HEPPI - LATMOS

LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales

3 Department of Astronomy [Boston]

4 LASP - Laboratory for Atmospheric and Space Physics [Boulder]

5 GSFC - NASA Goddard Space Flight Center

Abstract : Hubble Space Telescope (HST) observations of the Martian hydrogen exosphere in Lyman α are presented in this paper for a period when Mars passed perihelion and southern summer solstice in its orbit. The peak intensity in the exospheric Lyman α brightness was recorded after Mars went past its perihelion, slightly after southern summer solstice. The increase in brightness as Mars approached perihelion was found to not be symmetric around the peak, making it impossible to fit the H escape flux trend with a single sinusoidal curve with the peak at perihelion. While the short-term (~30 Earth-days) changes were not directly correlated with changes in the solar Lyman α flux, the long-term (~ 10 Earth-years) trend in the data does show some correlation with solar activity. This suggests that the short-term changes brought about in the exosphere could be due to intrinsic changes occurring within the lower atmosphere. For example, thermospheric heating by dust can alter the cold-trapping mechanism for water vapor resulting in it being present in large quantities at higher altitudes (60-80 km), possibly enhancing the escape flux of H. Therefore, it is important to understand the drivers of atmospheric dynamics in the Martian atmosphere, which produce the yearly-enhanced seasonal changes observed at Mars around periapsis and southern summer solstice in order to accurately determine the total amount of water lost over its history.

Keywords : Hydrogen HST Mars Atmosphere

Document type :

Journal articles

Domain :

Sciences of the Universe [physics]

Complete list of metadatas

https://hal-insu.archives-ouvertes.fr/insu-01636632
Contributor : Catherine Cardon <>
Submitted on : Thursday, November 16, 2017 - 5:46:20 PM
Last modification on : Wednesday, May 15, 2019 - 3:54:22 AM

Seasonal Changes In Hydrogen Escape From Mars through Analysis of HST Observations of the Martian Exosphere Near Perihelion

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Seasonal Changes In Hydrogen Escape From Mars through Analysis of HST Observations of the Martian Exosphere Near Perihelion

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