Venus is 12,100 kilometers in diameter and has a mass of 4.869e+24 kilograms. This makes Venus similar to the Earth and has often been called Earths sister planet. But the similarities end there. One major difference between the Earth and Venus is that Venus rotates on its axis from east to west, which means if you lived on Venus you would see the Sun rise in the west and set in the east. The atmosphere on Venus is mostly carbon dioxide choked with sulfuric acid and has a pressure at the surface more than 92 times the pressure at sea level on Earth. Unlike the Earth, Venus does not have a magnetic field generated by its iron core. This may be the result of how slowly Venus rotates on its axis. The only magnetic field Venus has is very weak and is produced by the interaction of the solar wind and the ionosphere of Venus.
The surface of Venus is difficult to see through the thick, dense clouds and the first crude images of the surface were obtained using ground based radar. More detailed images were obtained by the Magellan spacecraft which was launched to Venus on May 4, 1989 and spent four and a half years radar mapping 98 percent of the surface of Venus. Later, the European Space Agency launched the Venus Express on November 9, 2005 and on April 11, 2006 it slipped into a polar orbit around Venus. These probes have now provided us with an accurate map of Venus.
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