Published 2009
| public
Book Section - Chapter
Seasonal changes on Titan
Abstract
Titan displays seasonal changes in the distribution of gas and hazes in its atmosphere, in the character of its methane clouds, and in its temperatures and winds. While Cassini has observed some of these changes in detail, some are observable from Earth, and the period of most rapid change may be just about to begin in the years after equinox.
Additional Information
© 2009 Springer Science+Business Media B.V. RL acknowledges the support of a Cassini Data Analysis Program grant. MEB is supported by a grant from the National Science Foundation Planetary Astronomy program.Additional details
- Eprint ID
- 34372
- Resolver ID
- CaltechAUTHORS:20120925-155543351
- NASA
- NSF
- Created
-
2012-09-25Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences