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Venus. By: Ansley Maness, Hannah Hernandez, James Butler. Terrestrial Planet Tilt: 177.3˚ ** 180˚-177.3˚= 2.7˚, so Venus is almost completely upside down. Rotates clockwise, (technically counterclockwise because it’s upside down) 108,200,000 km from Sun. Venus- Basic Properties.
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Venus By: Ansley Maness, Hannah Hernandez, James Butler
Terrestrial Planet • Tilt: 177.3˚ • **180˚-177.3˚= 2.7˚, so Venus is almost completely upside down. • Rotates clockwise, (technically counterclockwise because it’s upside down) • 108,200,000 km from Sun Venus- Basic Properties
Length of day: fully rotates every 116 Earth days • Length of year: completes orbit of Sun every 224.65 Earth days. • Constant temperature: 735˚K (865˚F) Venus- Basic Properties
Mass: 81.5% of Earth’s mass • Density of Venus: 5250 kg/m3 • Density of Earth: 5520 kg/m3 Venus- Basic Properties
Venus- Basic Properties • Believed to have similar internal structure to Earth: core, mantle, crust • Made of rock and metal • Partially liquid core
Venus- Basic Properties • Lower internal pressure • No plate tectonics • Lacks internal magnetic field (due to slow rotation)
Very thick and dense atmosphere, 92x as dense as Earth’s • 96% CO2, 3.5% N2 • Relatively smooth surface • Large number of volcanoes • No ringsor moons Venus- Atmosphere/Surface
Discovered by ancient civilizations, because it’s visible with naked eye • First planet to be reached by a probe • Mariner 2 (1962): flew within 34,400 km of surface • Venera 7: first probe to land on Venus • Magellan (1989): collected radar images of 98% of Venus’s surface Venus- History
http://www.esa.int/Our_Activities/Space_Science/Venus_Express/Venus_compared_to_Earthhttp://www.esa.int/Our_Activities/Space_Science/Venus_Express/Venus_compared_to_Earth • http://www.universetoday.com/36123/axis-of-venus/ • http://en.wikipedia.org/wiki/Venus • http://www.scientificamerican.com/article.cfm?id=why-venus-spins-the-wrong • http://www.windows2universe.org/venus/interior.html • http://space.about.com/od/venus/a/Venus.htm Sources