In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10314983" target="_blank" >RIV/00216208:11320/15:10314983 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1016/j.icarus.2014.09.046" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2014.09.046</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.icarus.2014.09.046" target="_blank" >10.1016/j.icarus.2014.09.046</a>
Alternative languages
Result language
angličtina
Original language name
In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model
Original language description
Asteroid (101955) Bennu, the target of NASA's OSIRIS-REx sample return mission, is a D approximate to 0.5 km diameter low albedo near-Earth object. It has a spectral signature consistent with primitive carbonaceous chondrites, and an orbit similar to that of the Earth. A plausible evolution scenario for Bennu is that it migrated inward across the inner main belt from a low albedo family by Yarkovsky thermal forces over many hundreds of Myr. Eventually, it entered a resonance that took it into the terrestrial planet region, where a combination of planetary encounters and resonances took it to its current orbit over a few Myr to tens of Myr. When it departed the main belt, Bennu probably had an eccentricity 0.1 < e < 0.2 and an inclination 1 degrees < i< 6 degrees. Several low albedo families have the appropriate dynamical, color, albedo, and broad spectral characteristics to produce Bennu: Clarissa, Erigone, Eulalia, New Polana, and Sulamitis. Here we used a suite of numerical simulati
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA13-01308S" target="_blank" >GA13-01308S: Dynamics of small bodies in the solar system</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Icarus
ISSN
0019-1035
e-ISSN
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Volume of the periodical
247
Issue of the periodical within the volume
Neuveden
Country of publishing house
US - UNITED STATES
Number of pages
27
Pages from-to
191-217
UT code for WoS article
000346691400015
EID of the result in the Scopus database
2-s2.0-84910025944