Published February 10, 2009 | Version v1
Journal article

COUPLING CONVECTIVELY DRIVEN ATMOSPHERIC CIRCULATION TO SURFACE ROTATION: EVIDENCE FOR ACTIVE METHANE WEATHER IN THE OBSERVED SPIN RATE DRIFT OF TITAN

  • 1. Institute for Advanced Study, Princeton, NJ 08540 (United States)

Description

A large drift in the rotation rate of Titan observed by Cassini provided the first evidence of a subsurface ocean isolating the massive core from the icy crust. Seasonal exchange of angular momentum between the surface and atmosphere accounts for the magnitude of the effect, but observations lag the expected signal by a few years. We argue that this time lag is due to the presence of an active methane weather cycle in the atmosphere. An analytic model of the seasonal cycle of atmospheric angular momentum is developed and compared with time-dependent simulations of Titan's atmosphere with and without methane thermodynamics. The disappearance of clouds at the summer pole suggests the drift rate has already switched direction, signaling the change in season from solstice to equinox.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/692/1/168

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
692
Journal Issue
1
Journal Page Range
p. 168-173
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41024166
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ATMOSPHERIC CIRCULATION; METHANE; ROTATION; SATELLITES; SATURN PLANET; SEASONS; SIGNALS; SIMULATION; SPIN; THERMODYNAMICS; TIME DEPENDENCE
Descriptors DEC
ALKANES; ANGULAR MOMENTUM; HYDROCARBONS; MOTION; ORGANIC COMPOUNDS; PARTICLE PROPERTIES; PLANETS