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Mass loss rate of the zodiacal dust cloud
The Moon and the Planets, 1983The mass loss rate of the zodiacal dust cloud near the Sun has been estimated on the basis of the orbital behaviour of circumsolar dust grains suffering sublimation. It is found that the solar dust ring located at 4 solar radii from the Sun, which consists of grains whose inward spiraling due to the Poynting-Robertson effect is stopped by the influence
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Can short period comets maintain the zodiacal cloud?
2008The combined effects of the Poynting-Robertson drag, collisions and sputtering are destroying the interplanetary dust cloud. The mass-losses estimated by different authors reveal great discrepancies. The estimations range from 1 t sec −1 (purely Poynting-Robertson loss) over some 10 t sec −1 given by Whipple (1967) to a value of 100 t sec −1 which ...
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Three-dimensional models of the zodiacal dust cloud
Icarus, 1989R.H. Giese, B. Kneiβel
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Evidence for a significant Kuiper belt dust contribution to the zodiacal cloud
Nature Astronomy, 2022Lindsay P. Keller, George J. Flynn
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ORIGINS OF THE ZODIACAL DUST CLOUD II
Annals of the New York Academy of Sciences, 1964openaire +1 more source
Linking studies of tiny meteoroids, zodiacal dust, cometary dust and circumstellar disks
Planetary and Space Science, 2020Jeremie Lasue
exaly
Zodiacal light observations and its link with cosmic dust: A review
Planetary and Space Science, 2020Jeremie Lasue +2 more
exaly