Charon’s refractory factory

Author:

Raut Ujjwal123ORCID,Teolis Benjamin D.123ORCID,Kammer Joshua A.2ORCID,Gimar Caleb J.123ORCID,Brody Joshua S.12ORCID,Gladstone G. Randall23ORCID,Howett Carly J. A.45ORCID,Protopapa Silvia4ORCID,Retherford Kurt D.123ORCID

Affiliation:

1. Center for Laboratory Astrophysics and Space Science Experiments (CLASSE), Space Science and Engineering, Southwest Research Institute, San Antonio, TX 78238, USA.

2. Space Science and Engineering, Southwest Research Institute, San Antonio, TX 78238, USA.

3. Department of Physics and Astronomy, University of Texas at San Antonio, San Antonio, TX 78249, USA.

4. Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA.

5. Department of Physics, University of Oxford, Oxfordshire, UK.

Abstract

We combine novel laboratory experiments and exospheric modeling to reveal that “dynamic” Ly-α photolysis of Plutonian methane generates a photolytic refractory distribution on Charon that increases with latitude, consistent with poleward darkening observed in the New Horizons images. The flux ratio of the condensing methane to the interplanetary medium Ly-α photons, φ, controls the distribution and composition of Charon’s photoproducts. Mid-latitude regions are likely to host complex refractories emerging from low-φ photolysis, while high-φ photolysis at the polar zones primarily generate ethane. However, ethane being colorless does not contribute to the reddish polar hue. Solar wind radiolysis of Ly-α–cooked polar frost past spring sunrise may synthesize increasingly complex, redder refractories responsible for the unique albedo on this enigmatic moon.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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