Computer Science
Scientific paper
Nov 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..pres...33.&link_type=abstract
XMM Press Release PR 33-2007
Computer Science
Scientific paper
The launch of Venus Express back in November 2005 represented a major milestone in the exploration of Venus — a planet unvisited by any dedicated spacecraft since the early 1990s.
One of the fundamental questions being addressed by the Venus Express mission is why a world so similar to Earth in mass and size has evolved so differently, to become the noxious and inhospitable planet it is today.
Since it started its scientific observations in July 2006, Venus Express has been making the most detailed study of the planet’s thick and complex atmosphere to date.
The latest findings not only highlight the features that make Venus unique in the solar system but also provide fresh clues as to how the planet is — despite everything — a more Earth-like planetary neighbour than one could have imagined.
The results will appear in a special section of the 29 November issue of the journal Nature containing nine individual papers devoted to Venus Express science activities.
Media organisations interested in attending the press conference are invited to register via the form attached below. Media that cannot attend will have the opportunity to follow the press conference via the following phone line: +33 1 58 99 57 42 (listening-mode only).The results presented at the press conference are embargoed until 28 November 19:00 CET.
For more information
ESA Media Relations Office
Tel: +33 1 5369 7299
Fax: +33 1 5369 7690
Media event programme
‘Venus: a more Earth-like planetary neighbour’
Latest results from Venus Express
28 November 2007, 15:00, room 137
ESA Headquarters, 8-10 rue Mario-Nikis, Paris
15:00 Introduction, by Håkan Svedhem, ESA Venus Express Project Scientist
15:07 Venus: What we knew before, by Fred Taylor, Venus Express Interdisciplinary Scientist
15:15 Temperatures in the atmosphere of Venus, by Jean-Loup Bertaux, SPICAV Principal Investigator
15:25 The dynamic atmosphere of Venus, by Giuseppe Piccioni, VIRTIS Principal Investigator
15:40 Venus’s atmosphere and the solar wind, by Stas Barabash, ASPERA Principal Investigator
15:50 Climate and evolution, by David Grinspoon, Venus Express Interdisciplinary Scientist
16:00 Conclusion, by Dmitri Titov, Venus Express Science Coordinator and VMC scientist
16:05 Questions and Answers
16:25 Individual interviews
17:30 End of event
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