Search of Large Super-Fast Rotator between NEAs

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470342" target="_blank" >RIV/67985815:_____/16:00470342 - 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

Search of Large Super-Fast Rotator between NEAs

Original language description

Asteroids of size larger than 0.15 km generally do not have periods smallernthan 2.2 hours, a limit known as cohesionless spin-barrier. This barrier can be explainednby the rubble-pile structure in which the asteroids are made up of collisional breakup frag-nments bound together by mutual gravitational force. The exceptions to this rule, called LargenSuper-Fast Rotators (LSFRs), are very few as 2001 OE84 and 2005 UW163. Preliminarynresults of some NEAs (Near Earth Asteroids) photometric observations are presented, wenreport the value of new rotation periods for these elusive asteroids.

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

<a href="/en/project/GAP209%2F12%2F0229" target="_blank" >GAP209/12/0229: Study of non-gravitational asteroid evolution processes via photometric observations</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2016

Confidentiality

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

Name of the periodical

Memorie della Societa Astronomica Italiana

ISSN

0037-8720

e-ISSN

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Volume of the periodical

87

Issue of the periodical within the volume

1

Country of publishing house

IT - ITALY

Number of pages

6

Pages from-to

66-71

UT code for WoS article

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EID of the result in the Scopus database

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