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Jan 18, 2008 · The en:main belt is shown in red and blue, and contains 98.5% of all the objects. Within this, the "core" region between the 4:1 and 2:1 en:Kirkwood gaps, and at moderate inclinations and eccentricities is shown in red. It contains 93.4% of all the objects.
Jan 18, 2008 · The main belt region is shown in red, and contains 93.4% of all the objects. For reference, Mars orbits out to 1.666 AU, and Jupiter between 4.95 and 5.46 AU. The diagram was created by Piotr Deuar [1] using orbit data for 120437 numbered minor planets from the Minor Planet Center orbit database, dated 8 Feb 2006.
Location of the main belt This plot shows the location of the main belt with respect to the planets and the Sun as well as the orbital structure of asteroid inclinations and number density of objects (yellow represents the highest number density, blue the lowest). Figure from DeMeo and Carry (2014).
Jun 23, 2013 · It is recommended to name the SVG file “Masses of asteroids vs main belt.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. Licensing [ edit ] Kwamikagami at English Wikipedia , the copyright holder of this work, hereby publishes it under the following licenses:
Active asteroids are small Solar System bodies that have asteroid -like orbits but show comet -like visual characteristics. [1] That is, they show a coma, tail, or other visual evidence of mass-loss (like a comet), but their orbits remain within Jupiter 's orbit (like an asteroid). [2] [3] These bodies were originally designated main-belt ...
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