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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.ASPERA-4: An acronym for "Analyzer of Space Plasmas and Energetic Atoms," ASPERA-4 investigated the interaction between the solar wind and the Venusian atmosphere, determine the impact of plasma processes on the atmosphere, determine global distribution of plasma and neutral gas, study energetic neutral atoms, ions and electrons, and analyze other aspects of the near Venus environment.ASPERA-4 is a re-use of the ASPERA-3 design used on Mars Express, but adapted for the harsher near-Venus environment.VMC: The Venus Monitoring Camera is a wide-angle, multi-channel CCD.
Mission manager Patrick Martin expected the spacecraft would fall below 150 kilometres (93 mi) in early January 2015, with destruction occurring in late January or early February.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.At this point the spacecraft was running on an ellipse substantially closer to the planet than during the initial orbit.The polar orbit ranged between 250 and 66,000 kilometres (160 and 41,010 mi) over Venus.
It arrived at Venus on 11 April 2006, after 153 days of journey, and fired its main engine between and UTC SCET to reduce its velocity so that it could be captured by Venusian gravity into a nine-day orbit of 400 by 330,000 kilometres (250 by 205,050 mi).