The Pioneer Venus Orbiter: 11 years of data. A laboratory for atmospheres seminar talk

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Pioneer Project, Pioneer Venus 1 Spacecraft, Planetary Geology, Planetary Ionospheres, Solar Activity Effects, Venus (Planet), Venus Atmosphere, Venus Surface, Planetary Magnetic Fields, Plates (Tectonics), Solar Wind, Venus Clouds

Scientific paper

The Pioneer Venus Orbiter has been in operation since orbit insertion on December 4, 1978. For the past 11 years, it has been acquiring data in the salient features of the planet, its atmosphere, ionosphere, and interaction with the solar wind. A few of the results of this mission are summarized and their contribution to our general understanding of the planet Venus is discussed. Although Earth and Venus are often called twin planets, they are only superficially similar. Possessing no obvious evidence of plate tectonics, lacking water and an intrinsic magnetic field, and having a hot, dense carbon dioxide atmosphere with sulfuric acid clouds makes Venus a unique object of study by the Orbiter's instruments.

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