D
David Vokrouhlický
Researcher at Charles University in Prague
Publications - 263
Citations - 14248
David Vokrouhlický is an academic researcher from Charles University in Prague. The author has contributed to research in topics: Asteroid & Yarkovsky effect. The author has an hindex of 62, co-authored 254 publications receiving 12735 citations. Previous affiliations of David Vokrouhlický include California Institute of Technology & NASA Lunar Science Institute.
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Journal ArticleDOI
The fossilized size distribution of the main asteroid belt
William F. Bottke,Daniel D. Durda,David Nesvorný,Robert Jedicke,Alessandro Morbidelli,David Vokrouhlický,Hal Levison +6 more
TL;DR: In this paper, a collisional evolution model (CoEM) was proposed to model the evolution of the main belt of the Earth and the Moon over the last 3 Gyr.
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Linking the collisional history of the main asteroid belt to its dynamical excitation and depletion
William F. Bottke,Daniel D. Durda,David Nesvorný,Robert Jedicke,Alessandro Morbidelli,David Vokrouhlický,Harold F. Levison +6 more
TL;DR: This paper used a collisional evolution code to track the evolution of the main belt over 4.6 Gyr and found that only a small fraction of the fragments survived the dynamical depletion event described above.
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Cometary origin of the zodiacal cloud and carbonaceous micrometeorites. implications for hot debris disks
David Nesvorný,David Nesvorný,Peter Jenniskens,Harold F. Levison,Harold F. Levison,William F. Bottke,William F. Bottke,David Vokrouhlický,Matthieu Gounelle +8 more
TL;DR: In this article, the authors present a zodiacal cloud model based on the orbital properties and lifetimes of comets and asteroids, and on the dynamical evolution of dust after ejection.
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An Archaean heavy bombardment from a destabilized extension of the asteroid belt
William F. Bottke,David Vokrouhlický,David Vokrouhlický,David A. Minton,David A. Minton,David Nesvorný,Alessandro Morbidelli,Alessandro Morbidelli,Ramon Brasser,Ramon Brasser,Ramon Brasser,Bruce Simonson,Harold F. Levison +12 more
TL;DR: It is reported that the Late Heavy Bombardment lasted much longer than previously thought, with most late impactors coming from the E belt, an extended and now largely extinct portion of the asteroid belt between 1.7 and 2.1 astronomical units from Earth.
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The iau 2000 resolutions for astrometry celestial mechanics and metrology in the relativistic framework: explanatory supplement
Michael Soffel,Sergei A. Klioner,Gérard Petit,Peter Wolf,Sergei M. Kopeikin,P. Bretagnon,Victor A. Brumberg,N. Capitaine,Thibault Damour,Toshio Fukushima,B. Guinot,Tian-Yi Huang,Tian-Yi Huang,Lennart Lindegren,C. Ma,Kenneth Nordtvedt,John C Ries,P. K. Seidelmann,David Vokrouhlický,Clifford M. Will,Chong-Yu Xu +20 more
TL;DR: The IAU resolutions B1.3, B 1.4, B1 1.5, and B1 2.9 were adopted during the 24th General Assembly in Manchester, 2000, and provides details on and explanations for these resolutions as discussed by the authors.