Cited by 104Astro and Planetary SciencePlanetary Science and ExplorationStellar, planetary, and galactic studies

Thermal evolution of Kuiper belt objects, with implications for cryovolcanism

Desch, Steven J., Cook, Jason C., Doggett, T.C., Porter, Simon B.·2009·Icarus

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Crossref · 10.1016/j.icarus.2009.03.009

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1 of 1 references verified0 citation errors · 0 not checkable

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  • Modeling indicates that heating from long-lived radiogenic nuclides may provide enough warmth to sustain liquid water in large trans-Neptunian objects if antifreezing species such as ammonia are present.

    “Modeling of large trans-neptunian objects, bodies that lie beyond the orbit of Neptune, shows that heating from the long-lived radiogenic nuclides may provide enough warmth to sustain liquid water if there are antifreezing species such as ammonia present (Hussmann et al., 2006; Desch et al., 2009).”

    From The Astrobiology Primer v2.0 (2016) · cites this paper as Desch et al., 2009

  • Trans-Neptunian objects may provide a significant fraction of the Solar System's liquid water reservoir, perhaps collectively as much as on Earth.

    “Given the overwhelming population of the Kuiper Belt (106 objects greater than a few tens of kilometers; Morbidelli and Levison, 2007) and Oort Cloud (∼4 × 1011 objects with a radius larger than 1 km; Levison et al., 2010), trans-neptunian objects may provide a significant fraction of the Solar System's liquid water reservoir, perhaps collectively even as much as on Earth (Desch et al., 2009).”

    From The Astrobiology Primer v2.0 (2016) · cites this paper as Desch et al., 2009

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  • The Astrobiology Primer v2.0

    Domagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136 · see citing works

    “Modeling of large transneptunian objects, bodies that lie beyond the orbit of Neptune, shows that heating from the long-lived radiogenic nuclides may provide enough warmth to sustain liquid water if there are antifreezing species such as ammonia present (Hussmann et al., 2006; Desch et al., 2009).”

Authors
Desch, S. J., Cook, J. C., Doggett, T. C., & Porter, S. B.
Affiliations
  • Arizona State University (US)
  • Southwest Research Institute (US)
Corresponding author
Desch, Steven J.
Venue
Icarus
Publisher
Elsevier BV
Published
2009-08
Volume
202
Issue
2
Pages
694-714
ISSN
0019-1035 (ISSN-L)
OpenAlex
W2066925209
Cited by
104
References
1
Citations by year
2026: 5 · 2025: 4 · 2024: 4 · 2023: 5 · 2022: 11 · 2021: 4 · 2020: 6 · 2019: 9 · 2018: 2 · 2017: 7 · 2016: 10 · 2015: 6 · 2014: 9 · 2013: 1 · 2012: 5
FWCI
3.53
Type
journal article
Language
en
Open access
closed
Locations
Icarus (publishedVersion)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
Kuiper belt objects, thermal evolution, cryovolcanism, Charon, ammonia hydrates, differentiation, icy bodies, internal structure, Pluto system

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