Venus Express
The mission
Venus Express is a re-use of the Mars Express orbiter design and will be the first European mission to
Venus. Launched
successfully 9 November 2005 on Soyuz-Fregat, arrival 11 April 2006.
Science objectives
 Venus Express will answer
many questions about the atmosphere, plasma environment and surface of our sister planet. Our
interest at MSSL-UCL is in how the solar wind, after it is deflected and slowed by the Venus bow
shock, interacts with the Venus upper atmosphere and
ionosphere. We will study how atmospheric escape occurs and how the energy input into the upper
atmosphere works.
Venus has no magnetic field
- but it does have a thick, carbon dioxide-rich atmosphere. The surface pressure is 90 times the
Earth's. As there is no planetary magnetic field, the solar wind can reach the outer regions of the
Venus atmosphere. An ionosphere forms where the internal plasma pressure balances the solar wind
pressure. Neutral atoms and molecules can be picked up, in a similar process to that at comets,
by the solar wind and escape along the tail of the planet.
MSSL are co-investigator in the Aspera team, providing electron calibration (electron sensor built
by SwRI), blackening, a radiation shield and
scientific collaboration.
Further Information
The Venus Express homepage at ESA
The IRF Aspera homepage at IRF
|
+44 (0)1483 204100
- Copyright © 1999-2005 UCL