Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 11 April 2003:
Vol. 300. no. 5617, pp. 260 - 261
DOI: 10.1126/science.1083626

Perspectives

Also see the archival list of Science's Compass: Enhanced Perspectives

PLANETARY SCIENCE:
Enhanced: A Liquid Core for Mars?

Veronique Dehant

Early in their evolution, both Earth and Mars must have been sufficiently hot to be molten. Earth still has a liquid core, whereas the smaller Mars, having cooled faster, could be completely solid today. But is it? In her Perspective, Dehant highlights the report by Yoder et al., who have analyzed long-term changes in the orbit of Mars Global Surveyor around Mars. The data suggest that at least part of the martian core is liquid, with important consequences for the interior and evolution of our neighboring planet.


The author is at the Observatoire Royal de Belgique, Bruxelles, B-1180 Belgium. E-mail: veronique.dehant{at}oma.be

Read the Full Text





To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)