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It operates in the visible, ultraviolet, and near infrared spectral ranges, and maps surface brightness distribution searching for volcanic activity, monitoring airglow, studying the distribution of unknown ultraviolet absorbing phenomenon at the cloud-tops, and making other science observations.
However, some mission characteristics led to design changes: primarily in the areas of thermal control, communications and electrical power.
It is also made global maps of the Venusian surface temperatures.
Its nominal mission was originally planned to last for 500 Earth days (approximately two Venusian sidereal days), but the mission was extended five times: first on 28 February 2007 until early May 2009; then on 4 February 2009 until 31 December 2009; and then on 7 October 2009 until 31 December 2012.
On the other hand, the more intense illumination of the solar panels results in more generated photovoltaic power. It was eventually launched by a Soyuz-FG/Fregat rocket from the Baikonur Cosmodrome in Kazakhstan on 9 November 2005 at UTC into a parking Earth orbit and 1 h 36 min after launch put into its transfer orbit to Venus.
The Venus Express mission also uses some spare instruments developed for the Rosetta spacecraft. A first trajectory correction maneuver was successfully performed on 11 November 2005.
VMC: The Venus Monitoring Camera is a wide-angle, multi-channel CCD.
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