Zodi

From Wikipedia, the free encyclopedia

The zodi is a unit of zodiacal dust.[1] One zodi is the amount of interplanetary dust in the inner Solar System.[2] This dust absorbs light from the Sun and re-radiates it as thermal radiation. The luminosity of the zodiacal dust in the Solar System is about relative to the luminosity of the Sun,[3] and in practice, this is the observable characteristic defining one zodi.

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References[]

  1. ^ O. Guyon & F. Roddier (2002-02-19). "A nulling wide field imager for exoplanets detection and general astrophysics" (PDF). p. 37. Retrieved 2008-10-20.
  2. ^ Alycia J. Weinberger, "Building Planets in Disks of Chaos" in Sky & Telescope, November 2008, p. 37.
  3. ^ D. Nesvorny; et al. (2010). "Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites. Implications for Hot Debris Disks". in The Astrophysical Journal, 713, p. 816


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