Titan's Rotation

Surface Feature Observed

Mark T. Lemmon, Erich Karkoschka, Martin G Tomasko

Research output: Contribution to journalArticle

83 Citations (Scopus)

Abstract

We have detected time variation in Titan's geometric albedo in methane windows at 0.94, 1.08, and 1.28 μm, relative to its albedo in adjacent methane bands, of 8 ± 5%, 14 ± 3%, and 22 ± 3%, respectively. We attribute these changes to a surface feature or a feature near the surface. Our observations are consistent with synchronous rotation and can be explained by a higher surface albedo by 0.1 on Titan's leading hemisphere.

Original languageEnglish (US)
Pages (from-to)329-332
Number of pages4
JournalIcarus
Volume103
Issue number2
DOIs
StatePublished - Jun 1993

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Titan
albedo
methane
hemispheres

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Titan's Rotation : Surface Feature Observed. / Lemmon, Mark T.; Karkoschka, Erich; Tomasko, Martin G.

In: Icarus, Vol. 103, No. 2, 06.1993, p. 329-332.

Research output: Contribution to journalArticle

Lemmon, MT, Karkoschka, E & Tomasko, MG 1993, 'Titan's Rotation: Surface Feature Observed', Icarus, vol. 103, no. 2, pp. 329-332. https://doi.org/10.1006/icar.1993.1074
Lemmon, Mark T. ; Karkoschka, Erich ; Tomasko, Martin G. / Titan's Rotation : Surface Feature Observed. In: Icarus. 1993 ; Vol. 103, No. 2. pp. 329-332.
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