P138
Did the Hilda collisional family form during the late heavy bombardment?Constraining the cometary flux through the asteroid belt during the late heavy bombardmentThe primordial excitation and clearing of the asteroid belt—RevisitedContamination of the asteroid belt by primordial trans-Neptunian objectsAn asteroid breakup 160 Myr ago as the probable source of the K/T impactorYarkovsky/YORP chronology of asteroid familiesThe origin and evolution of stony meteoritesLarge impact crater histories of Mars: The effect of different model crater age techniquesExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid PopulationThe breakup of a main-belt asteroid 450 thousand years ago.The recent breakup of an asteroid in the main-belt region.The vector alignments of asteroid spins by thermal torques.An Archaean heavy bombardment from a destabilized extension of the asteroid belt.A late Miocene dust shower from the break-up of an asteroid in the main belt.An anomalous basaltic meteorite from the innermost main belt.Widespread mixing and burial of Earth's Hadean crust by asteroid impacts.Growing the terrestrial planets from the gradual accumulation of submeter-sized objects.Global resurfacing of Mercury 4.0-4.1 billion years ago by heavy bombardment and volcanism.Stochastic late accretion to Earth, the Moon, and MarsThe mass disruption of Oort cloud cometsIron meteorites as remnants of planetesimals formed in the terrestrial planet regionSuper-catastrophic disruption of asteroids at small perihelion distances.High-velocity collisions from the lunar cataclysm recorded in asteroidal meteoritesTHE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid DynamicsOn a Scattered-Disk Origin for the 2003 EL61 Collisional Family—an Example of the Importance of Collisions on the Dynamics of Small BodiesThe Irregular Satellites: the Most Collisionally Evolved Populations in the Solar SystemCometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites. Implications for Hot Debris DisksExploreNEOs. II. The Accuracy of the Warm Spitzer Near-Earth Object SurveyExploreNEOs. III. Physical Characterization of 65 Potential Spacecraft Target AsteroidsYarkovsky origin of the unstable asteroids in the 2/1 mean motion resonance with JupiterThe onset of the lunar cataclysm as recorded in its ancient crater populationsModeling the Historical Flux of Planetary ImpactorsYarkovsky footprints in the Eos familyObserved Binary Fraction Sets Limits on the Extent Of Collisional Grinding in the Kuiper BeltTowards initial mass functions for asteroids and Kuiper Belt ObjectsErosion and Ejecta Reaccretion on 243 Ida and Its MoonCollisional and Dynamical History of IdaKarin cluster formation by asteroid impactRecent Origin of the Solar System Dust BandsDelivery of dark material to Vesta via carbonaceous chondritic impacts
P50
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P50
description
planetair wetenschapper
@nl
planetary scientist
@en
name
William F. Bottke
@ast
William F. Bottke
@ca
William F. Bottke
@en
William F. Bottke
@es
William F. Bottke
@fr
William F. Bottke
@nl
ウィリアム・ボトキ
@ja
type
label
William F. Bottke
@ast
William F. Bottke
@ca
William F. Bottke
@en
William F. Bottke
@es
William F. Bottke
@fr
William F. Bottke
@nl
ウィリアム・ボトキ
@ja
prefLabel
William F. Bottke
@ast
William F. Bottke
@ca
William F. Bottke
@en
William F. Bottke
@es
William F. Bottke
@fr
William F. Bottke
@nl
ウィリアム・ボトキ
@ja
P214
P244
P269
P21
P213
0000 0000 3758 3511
P214
P244
n2002159933
P269
P31
P569
1966-01-01T00:00:00Z
P7859
lccn-n2002159933