Venus Express

Venus Express
Venus Express in orbit
Mission typeVenus orbiter
OperatorEuropean Space Agency
COSPAR ID2005-045A
SATCAT no.28901
Websitewww.esa.int/venus
Mission durationPlanned: 2 years
Final: 9 years, 2 months, 9 days
Spacecraft properties
ManufacturerEADS Astrium
Launch mass1,270 kg (2,800 lb)
Dry mass700 kg (1,500 lb)
Payload mass93 kg (205 lb)
Dimensions1.5 × 1.8 × 1.4 m (4.9 × 5.9 × 4.6 ft)
Power1,100 watts
Start of mission
Launch date9 November 2005, 03:33:34 (2005-11-09UTC03:33:34) UTC
RocketSoyuz-FG/Fregat
Launch siteBaikonur 31/6
ContractorStarsem
End of mission
DisposalDeorbited
Last contact18 January 2015, 15:01:55 (2015-01-18UTC15:01:56) UTC
Decay dateJanuary / February 2015
Orbital parameters
Reference systemCytherocentric
Pericytherion altitude460 km (290 mi)
Apocytherion altitude63,000 km (39,000 mi)
Inclination90 degrees
Period24 hours
Venus orbiter
Orbital insertion11 April 2006

Contemporary ESA insignia (2000s)

Venus Express (VEX) was the first Venus exploration mission of the European Space Agency (ESA). Launched in November 2005, it arrived at Venus in April 2006 and began continuously sending back science data from its polar orbit around Venus. Equipped with seven scientific instruments, the main objective of the mission was the long term observation of the Venusian atmosphere. The observation over such long periods of time had never been done in previous missions to Venus, and was key to a better understanding of the atmospheric dynamics. ESA concluded the mission in December 2014.

Orbits and trajectories of Mariner 2, Venera 4, Pioneer Venus Orbiter, and Venus Express
Animation of Venus Express's trajectory from 9 November 2005 to 31 December 2006
  Venus Express ·   Venus ·   Earth ·   Sun
Animation of Venus Express's trajectory around Venus from 1 April 2006 to 1 April 2008
  Venus Express ·   Venus
Venus, May 2006
Ultraviolet picture (with arbitrary color) of Venus. The clouds betray the extremely fast winds at mid levels of the atmosphere, which circumnavigate the globe in just four days, August 2008
Ultraviolet picture colored to draw out highlights in the clouds, August 2008
The daylight side shown in visible light and the night side in infrared, September 2008
On the left is what the planet looked like in visible light: a nearly featureless orb of highly-reflective clouds. On the right is a shot taken at about the same time through a filter sensitive to ultraviolet light, which the human eye can't see, September 2008
Venus in infrared (here as red) and ultraviolet light by Venus Express, December 2008