|
|
|
|||||||||||||||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |
1 Department of Earth and Planetary Sciences
University of
Tennessee
Knoxville, TN 37996-1410, USA
E-mail:
mcsween{at}utk.edu
Water on Mars exists at the poles and in the subsurface. It has interacted with crustal rocks, providing geomorphological, geochemical, and mineralogical insights into Mars' geological history and inferences about its biological potential. The roles of water are revealed through studies of altered materials using orbiting-spacecraft imagery and spectroscopy, instruments mounted on rovers, and laboratory measurements on Martian meteorites.
KEYWORDS: water, aqueous alteration, spacecraft, rovers, meteorites
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |