COUPLING CONVECTIVELY DRIVEN ATMOSPHERIC CIRCULATION TO SURFACE ROTATION: EVIDENCE FOR ACTIVE METHANE WEATHER IN THE OBSERVED SPIN RATE DRIFT OF TITAN
Creators
- 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/692/1/168Additional 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