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Home > Art, Film & Photography > Types of Planet: Gas Giant, Double Planet, Extrasolar Planet, Terrestrial Planet, Brown Dwarf, Protoplanet, Habitable Zone, Super-Earth
Types of Planet: Gas Giant, Double Planet, Extrasolar Planet, Terrestrial Planet, Brown Dwarf, Protoplanet, Habitable Zone, Super-Earth

Types of Planet: Gas Giant, Double Planet, Extrasolar Planet, Terrestrial Planet, Brown Dwarf, Protoplanet, Habitable Zone, Super-Earth


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About the Book

Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Pages: 31. Chapters: Gas giant, Double planet, Extrasolar planet, Terrestrial planet, Brown dwarf, Protoplanet, Habitable zone, Super-Earth, Hot Jupiter, Circumbinary planet, Pulsar planet, Planetar, Extragalactic planet, Sub-brown dwarf, Eccentric Jupiter, Mesoplanet, Iron planet, Hot Neptune, Carbon giant. Excerpt: An extrasolar planet, or exoplanet, is a planet outside the Solar System. As of August 10, 2011, 573 extra-solar planets have been identified. A substantial fraction of stars have planetary systems, including 10% of Sun-like stars, though the actual proportion may be higher. Data from the Kepler mission has been used to estimate that there are at least 50 billion planets in our own galaxy. There also exist planetary-mass objects that orbit brown dwarfs and that orbit the galaxy directly just as stars do, although it is unclear if either type should be labeled as a "planet." Extrasolar planets became an object of investigation in the nineteenth century. Many supposed that they existed, but there was no way of knowing how common they are or how similar they are to the planets of our solar system. The first confirmed detection was in 1992, with the discovery of several terrestrial-mass planets orbiting the pulsar PSR B1257+12. The first confirmed detection of an exoplanet orbiting a main-sequence star was made in 1995, when a giant planet, 51 Pegasi b, was found in a four-day orbit around the nearby G-type star 51 Pegasi. The frequency of detections has increased since then. Many exoplanets are detected through radial velocity observations and other indirect methods rather than sensor imaging. Most are giant planets resembling Jupiter; this partly reflects a sampling bias, as more massive planets are easier to observe. Several relatively lightweight exoplanets, only a few times more massive than Earth, were detected and projec...


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Product Details
  • ISBN-13: 9781157617242
  • Publisher: Books LLC, Wiki Series
  • Publisher Imprint: Books LLC, Wiki Series
  • Height: 246 mm
  • No of Pages: 32
  • Spine Width: 2 mm
  • Weight: 77 gr
  • ISBN-10: 1157617247
  • Publisher Date: 04 Sep 2011
  • Binding: Paperback
  • Language: English
  • Returnable: N
  • Sub Title: Gas Giant, Double Planet, Extrasolar Planet, Terrestrial Planet, Brown Dwarf, Protoplanet, Habitable Zone, Super-Earth
  • Width: 189 mm


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