Zodi

Zodi je jedinica zodijačke svjetlosti.^[1] Jedan zodi je količina međuplanetarne tvari u unutrašnjem Sunčevom sustavu.^[2] Ova prašina upija svjetlost sa Sunca i ponovno je zrači kao toplinsko zračenje. Svjetlost zodijačke svjetlosti u Sunčevom sustavu je približno $10^{-7}$ u odnosu na sjaj Sunca^[3] a u praksi je ovo uočljiva karakteristika koja definira jedan zodi.

Izvori

↑ O. Guyon (2002-02-19). A nulling wide field imager for exoplanets detection and general astrophysics ID: o_guyon-a_nulling_wide_field_imager_for_exoplanets_detection_and_general_astrophysics.
↑ Alycia J. Weinberger, "Building Planets in Disks of Chaos" in Sky & Telescope, November 2008, p. 37.
↑ D. Nesvorny (2010). Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites. Implications for Hot Debris Disks ID: d_nesvorny-cometary_origin_of_the_zodiacal_cloud_and_carbonaceous_micrometeorites_implications_for_hot_debris_disks. in The Astrophysical Journal, 713, p. 816

[aa020219-1] O. Guyon (2002-02-19). A nulling wide field imager for exoplanets detection and general astrophysics ID: o_guyon-a_nulling_wide_field_imager_for_exoplanets_detection_and_general_astrophysics.

[st0811-2] Alycia J. Weinberger, "Building Planets in Disks of Chaos" in Sky & Telescope, November 2008, p. 37.

[doi:10.1088/0004-637X/713/2/816-3] D. Nesvorny (2010). Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites. Implications for Hot Debris Disks ID: d_nesvorny-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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Zodi

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