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Extreme exospheric dynamics at Charon: Implications for the red spot

Abstract:
Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi-annually drives frozen methane off the polar night zones. Charon's pole-centric red spot has been proposed to be the product of Ly-α photolysis of frozen methane into refractory hydrocarbon “tholins”, but the role of exospheric dynamics in the red material's formation has not been investigated. We show with exospheric modeling that methane “polar-swap”, in which exospheric CH4 sublimated from the spring polar zone is rapidly re-frozen onto the autumn hemisphere, deposits ∼30 μm polar frosts too thick for Ly-α light to penetrate. Ethane, the primary methane photoproduct under these conditions, may unlike methane remain frozen decades after polar sunrise under solar wind exposure. Solar wind radiolysis of polar ethane frost synthesizes higher-order refractories that may contribute to the coloration of Charon's polar zones.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1029/2021GL097580

Authors


More by this author
Role:
Author
ORCID:
0000-0001-8386-6413
More by this author
Role:
Author
ORCID:
0000-0002-6036-1575
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
St Edmund Hall
Role:
Author
ORCID:
0000-0003-1869-4947


Publisher:
Wiley
Journal:
Geophysical Research Letters More from this journal
Volume:
49
Issue:
8
Article number:
e2021GL097580
Publication date:
2022-04-21
Acceptance date:
2022-04-02
DOI:
EISSN:
1944-8007
ISSN:
0094-8276


Language:
English
Keywords:
Pubs id:
1261815
Local pid:
pubs:1261815
Deposit date:
2022-07-01

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