Datura family: the 2009 update

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F09%3A00206982" target="_blank" >RIV/00216208:11320/09:00206982 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Datura family: the 2009 update

Original language description

We determined the rotation state of (1270) Datura, the largest member of its own family. Its major properties are short rotation period of 3.36 h and small obliquity. The second largest member of the Datura family (90265) 2003 CL5 - appears to be very slow rotator with the rotation period 24 h. The large amplitude of its rotation curve suggests its shape is extremely elongate.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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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)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2009

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy and Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

507

Issue of the periodical within the volume

1

Country of publishing house

FR - FRANCE

Number of pages

10

Pages from-to

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UT code for WoS article

000271782900047

EID of the result in the Scopus database

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