3.9 Article

Titan: Earth-like on the Outside, Ocean World on the Inside

期刊

PLANETARY SCIENCE JOURNAL
卷 2, 期 3, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/PSJ/abf7c9

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资金

  1. JHU APL and Cassini Data Analysis Program (CDAP) [NH16ZDA001N]
  2. CDAP grant
  3. NASA Astrobiology Institute project entitled Habitability of Hydrocarbon Worlds: Titan and Beyond
  4. Center for Space Sciences and Technology of the University of Maryland Baltimore County
  5. [80NSSC19K0888]

向作者/读者索取更多资源

Titan, revealed to be a dynamic, hydrologically shaped, organic-rich ocean world by the Cassini-Huygens mission, offers unparalleled opportunities to explore prebiotic chemistry. Future exploration of Titan will address some of the most compelling planetary science questions of the next decade.
Thanks to the Cassini-Huygens mission, Titan, the pale orange dot of Pioneer and Voyager encounters, has been revealed to be a dynamic, hydrologically shaped, organic-rich ocean world offering unparalleled opportunities to explore prebiotic chemistry. And while Cassini-Huygens revolutionized our understanding of each of the three layers of Titan-the atmosphere, the surface, and the interior-we are only beginning to hypothesize how these realms interact. In this paper, we summarize the current state of Titan knowledge and discuss how future exploration of Titan would address some of the next decade's most compelling planetary science questions. We also demonstrate why exploring Titan, both with and beyond the Dragonfly New Frontiers mission, is a necessary and complementary component of an Ocean Worlds Program that seeks to understand whether habitable environments exist elsewhere in our solar system.

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