J
Jeremie Vaubaillon
Researcher at Institut de mécanique céleste et de calcul des éphémérides
Publications - 129
Citations - 2388
Jeremie Vaubaillon is an academic researcher from Institut de mécanique céleste et de calcul des éphémérides. The author has contributed to research in topics: Meteoroid & Comet. The author has an hindex of 24, co-authored 122 publications receiving 2097 citations. Previous affiliations of Jeremie Vaubaillon include Paris Observatory & California Institute of Technology.
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Journal ArticleDOI
The impact and recovery of asteroid 2008 TC 3
Peter Jenniskens,Muawia H. Shaddad,D. Numan,S. Elsir,Ayman M. Kudoda,Michael E. Zolensky,L. Le,G. A. Robinson,Jon M. Friedrich,Jon M. Friedrich,D. Rumble,Andrew Steele,Steve Chesley,Alan Fitzsimmons,Samuel R. Duddy,Henry H. Hsieh,G. Ramsay,Peter Brown,Wayne N. Edwards,E. Tagliaferri,Mark Boslough,R. E. Spalding,Ron Dantowitz,M. Kozubal,Petr Pravec,Jiri Borovicka,Z. Charvat,Jeremie Vaubaillon,J. Kuiper,Jim Albers,Janice L. Bishop,Rocco L. Mancinelli,Scott A. Sandford,Stefanie N. Milam,Michel Nuevo,Simon P. Worden +35 more
TL;DR: A dedicated search along the approach trajectory recovered 47 meteorites, fragments of a single body named Almahata Sitta, with a total mass of 3.95 kg, identifying the asteroid as F class, now firmly linked to dark carbon-rich anomalous ureilites, a material so fragile it was not previously represented in meteorite collections.
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The population of natural Earth satellites
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A dynamical model of the sporadic meteoroid complex
TL;DR: In this paper, a physics-based model of the Earth's meteoroid complex is presented, which uses the observed meteor patrol radar strengths of the sporadic meteors to solve for the dust production rates of the populations of comets modeled.
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Explosion of Comet 17P/Holmes as revealed by the Spitzer Space Telescope
TL;DR: In this paper, the authors modeled the explosion as being due to crystallization and release of volatiles from interior amorphous ice within a subsurface cavity; once the pressure in the cavity exceeded the surface strength, the material above the cavity was propelled from the comet.
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A new method to predict meteor showers. I. Description of the model
TL;DR: In this paper, the authors proposed a new model to compute the time and level of a meteor shower whose parent body is a known periodic comet, using all available knowledge on cometary dust to avoid most of the "a priori" hypotheses of previous meteoroid stream models.