Trojan Asteroids
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Home > Art, Film & Photography > Trojan Asteroids: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eure
Trojan Asteroids: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eure

Trojan Asteroids: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eure


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About the Book

Purchase includes free access to book updates online and a free trial membership in the publisher's book club where you can select from more than a million books without charge. Chapters: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eureka, (101429) 1998 Vf31, 2007 Ns2, 2005 Tn53, 2007 Vl305, 2003 Fe42, (90569) 2004 Gy14, (183309) 2002 Vq, 129137 Hippolochos, 2006 Rj103, 2007 Rw10, List of Mars Trojan Asteroids, 2004 Up10, 2005 To74, (4489) 1988 Ak. Excerpt: The Jupiter Trojans, commonly called Trojans or Trojan asteroids, are a large group of objects that share the orbit of the planet Jupiter around the Sun. Relative to Jupiter, each Trojan librates around one of the planet's two Lagrangian points of stability, L4 and L5, that respectively lie 60 ahead of and behind the planet in its orbit. Trojan asteroids are distributed in two elongated, curved regions around these Lagrangian points with an average semi-major axis of about 5.2 AU. The first Trojan discovered, 588 Achilles, was spotted in 1906 by the German astronomer Max Wolf. A total of 4,076 Jupiter Trojans have been found as of February 2010. The term "Trojan" derives from the fact that, by convention, they are each named after a mythological figure from the Trojan War. The total number of Jupiter Trojans larger than 1 km in diameter is believed to be about, approximately equal to the number of asteroids larger than 1 km in the main asteroid belt. Like main belt asteroids, Trojans form families. Jupiter Trojans are dark bodies with reddish, featureless spectra. No firm evidence of the presence of water, organic matter or other chemical compounds on their surfaces has been obtained. The Trojans' densities (as measured by studying binaries or rotational lightcurves) vary from 0.8 to 2.5 gcm. Trojans are thought to have been captured into their orbits during the early stages of the Solar System's formation or slightly later, during... More: http: //booksllc.net/?id=30972


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Product Details
  • ISBN-13: 9781157969082
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • No of Pages: 54
  • Spine Width: 3 mm
  • Weight: 91 gr
  • ISBN-10: 1157969089
  • Publisher Date: 11 Jun 2010
  • Binding: Paperback
  • Language: English
  • Returnable: N
  • Sub Title: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eure
  • Width: 229 mm


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Trojan Asteroids: Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, Jupiter Trojans, Mars Trojans, Neptune Trojans, 2001 Qr322, (121514) 1999 Uj7, 5261 Eure

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