On the shapes and spins of ?rubble pile asteroids

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F09%3A00335568" target="_blank" >RIV/67985815:_____/09:00335568 - isvavai.cz</a>

Result on the web

—

DOI - Digital Object Identifier

—

Result language

angličtina

Original language name

On the shapes and spins of ?rubble pile asteroids

Original language description

We examined the shape of a ?rubble pile asteroid as it slowly gains angular momentum by YORP torque, to the point where ?landsliding occurs. We find that it evolves to a ?top shape with constant angle of repose from the equator up to mid-latitude, closely resembling the shapes of several nearly critically spinning asteroids imaged by radar.

Czech name

—

Czech description

—

Type

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

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

—

Project

<a href="/en/project/GA205%2F05%2F0604" target="_blank" >GA205/05/0604: Photometric study of asynchronous binary systems among near-Earth asteroids</a><br>

Continuities

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

Icarus

ISSN

0019-1035

e-ISSN

—

Volume of the periodical

199

Issue of the periodical within the volume

2

Country of publishing house

US - UNITED STATES

Number of pages

9

Pages from-to

—

UT code for WoS article

000263250600009

EID of the result in the Scopus database

—