Author
Listed:
- W. M. Grundy
(Lowell Observatory)
- D. P. Cruikshank
(NASA Ames Research Center)
- G. R. Gladstone
(Southwest Research Institute)
- C. J. A. Howett
(Southwest Research Institute)
- T. R. Lauer
(National Optical Astronomy Observatory)
- J. R. Spencer
(Southwest Research Institute)
- M. E. Summers
(George Mason University)
- M. W. Buie
(Southwest Research Institute)
- A. M. Earle
(Massachussetts Institute of Technology)
- K. Ennico
(NASA Ames Research Center)
- J. Wm. Parker
(Southwest Research Institute)
- S. B. Porter
(Southwest Research Institute)
- K. N. Singer
(Southwest Research Institute)
- S. A. Stern
(Southwest Research Institute)
- A. J. Verbiscer
(University of Virginia)
- R. A. Beyer
(NASA Ames Research Center
Carl Sagan Center, SETI Institute)
- R. P. Binzel
(Massachussetts Institute of Technology)
- B. J. Buratti
(NASA Jet Propulsion Laboratory)
- J. C. Cook
(Southwest Research Institute)
- C. M. Dalle Ore
(NASA Ames Research Center
Carl Sagan Center, SETI Institute)
- C. B. Olkin
(Southwest Research Institute)
- A. H. Parker
(Southwest Research Institute)
- S. Protopapa
(University of Maryland)
- E. Quirico
(Université Grenoble Alpes, CNRS, IPAG)
- K. D. Retherford
(Southwest Research Institute)
- S. J. Robbins
(Southwest Research Institute)
- B. Schmitt
(Université Grenoble Alpes, CNRS, IPAG)
- J. A. Stansberry
(Space Telescope Science Institute)
- O. M. Umurhan
(NASA Ames Research Center)
- H. A. Weaver
(Johns Hopkins University Applied Physics Laboratory)
- L. A. Young
(Southwest Research Institute)
- A. M. Zangari
(Southwest Research Institute)
- V. J. Bray
(Lunar and Planetary Laboratory, University of Arizona)
- A. F. Cheng
(Johns Hopkins University Applied Physics Laboratory)
- W. B. McKinnon
(Washington University in St Louis)
- R. L. McNutt
(Johns Hopkins University Applied Physics Laboratory)
- J. M. Moore
(NASA Ames Research Center)
- F. Nimmo
(University of California, Santa Cruz)
- D. C. Reuter
(NASA Goddard Space Flight Center)
- P. M. Schenk
(Lunar and Planetary Institute)
Abstract
The unusual dark red coloration of Charon’s northern polar cap is shown to be produced from hydrocarbons that are cold-trapped from Pluto’s escaping atmosphere during winter.
Suggested Citation
W. M. Grundy & D. P. Cruikshank & G. R. Gladstone & C. J. A. Howett & T. R. Lauer & J. R. Spencer & M. E. Summers & M. W. Buie & A. M. Earle & K. Ennico & J. Wm. Parker & S. B. Porter & K. N. Singer &, 2016.
"The formation of Charon’s red poles from seasonally cold-trapped volatiles,"
Nature, Nature, vol. 539(7627), pages 65-68, November.
Handle:
RePEc:nat:nature:v:539:y:2016:i:7627:d:10.1038_nature19340
DOI: 10.1038/nature19340
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Citations
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Cited by:
- Silvia Protopapa & Ujjwal Raut & Ian Wong & John Stansberry & Geronimo L. Villanueva & Jason Cook & Bryan Holler & William M. Grundy & Rosario Brunetto & Richard J. Cartwright & Bereket Mamo & Joshua , 2024.
"Detection of carbon dioxide and hydrogen peroxide on the stratified surface of Charon with JWST,"
Nature Communications, Nature, vol. 15(1), pages 1-13, December.
- Stephanie M. Menten & Michael M. Sori & Ali M. Bramson, 2022.
"Endogenically sourced volatiles on Charon and other Kuiper belt objects,"
Nature Communications, Nature, vol. 13(1), pages 1-7, December.
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