The young Datura asteroid family Spins, shapes, and population estimate

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00485038" target="_blank" >RIV/67985815:_____/17:00485038 - isvavai.cz</a>
Alternative codes found
RIV/00216208:11320/17:10367520
Result on the web
<a href="http://dx.doi.org/10.1051/0004-6361/201629670" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201629670</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201629670" target="_blank" >10.1051/0004-6361/201629670</a>

Result language
angličtina
Original language name
The young Datura asteroid family Spins, shapes, and population estimate
Original language description
We study the most suitable known asteroid family with an age of less than 1 Myr, the Datura family. We aim (i) to obtain information about rotation state and shape of the largest members in the family and (ii) to constrain its debiased population down to couple of hundreds of meters in size. We have analyzed the up-to-date catalog of orbital elements of main belt asteroids. We evaluated the detection efficiency of Catalina Sky Survey (CSS) in regard to detections of members in the Datura family, and we have used our photometric observations and lightcurve inversion methods to determine the rotation states and shapes of the largest members of the family.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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