A new measurement of D/H on Mars using EXES aboard SOFIA

Abstract : The distribution of D/H ratio on Mars is crucial for understanding the planet’s water cycle including the exchange with surface reservoirs, and for estimating the amount of liquid water in the past. We have employed EXES (Echelle Cross Echelle Spectrograph) aboard SOFIA (Stratospheric Observatory For Infrared Astronomy) to map D/H on Mars in the thermal infrared, starting with the first measurement in April 2014 (Ls = 113°). Here we present a new measurement obtained in March 2016 (Ls = 127°). The disk-integrated value of D/H is found be 4.0 (+0.7, -0.6) x VSMOW, in agreement with our earlier result (4.4 (+1.0, -0.6) x VSMOW) [3]
Document type :
Conference papers
Complete list of metadatas

https://hal-insu.archives-ouvertes.fr/insu-01670006
Contributor : Catherine Cardon <>
Submitted on : Thursday, December 21, 2017 - 9:24:32 AM
Last modification on : Friday, September 20, 2019 - 8:20:04 AM

File

EPSC2017-168.pdf
Files produced by the author(s)

Identifiers

  • HAL Id : insu-01670006, version 1

Citation

Therese Encrenaz, C. Dewitt, M. Richter, T. Greathouse, T. Fouchet, et al.. A new measurement of D/H on Mars using EXES aboard SOFIA. European Planetary Science Congress 2017, Sep 2017, Riga, Latvia. pp.EPSC2017-168. ⟨insu-01670006⟩

Share

Metrics

Record views

259

Files downloads

19