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Observations of "fresh" and weathered surfaces on asteroid pairs and their implications on the rotational-fission mechanism

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10286611" target="_blank" >RIV/00216208:11320/14:10286611 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.01.014" target="_blank" >http://dx.doi.org/10.1016/j.icarus.2014.01.014</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.icarus.2014.01.014" target="_blank" >10.1016/j.icarus.2014.01.014</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Observations of "fresh" and weathered surfaces on asteroid pairs and their implications on the rotational-fission mechanism

  • Original language description

    The rotational-fission of a "rubble-pile" structured asteroid can result in an "asteroid pair" - two unbound asteroids sharing nearly identical heliocentric orbits. Models suggest that this mechanism exposes material from below the progenitor surface that previously had never have been exposed to the weathering conditions of space. Therefore, the surfaces of asteroid pairs offer the opportunity to observe non-weathered "fresh" spectra. Here we report near-infrared spectroscopic observations of 31 asteroids in pairs. In order to search for spectral indications of fresh surfaces we analyze their spectral slopes, parameters of their 1 ?m absorption band and taxonomic classification. Additionally, through backward dynamical integration we estimate the timeelapsed since the disintegration of the pairs' progenitors. Analyzing the 19 ordinary chondrite-like (S-complex) objects in our sample, we find two Q-type Asteroids (19289 and 54827) that are the first of their kind to be observed in the

  • Czech name

  • Czech description

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

Result continuities

  • 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)

Others

  • Publication year

    2014

  • 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

  • Volume of the periodical

    233

  • Issue of the periodical within the volume

    květen

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    18

  • Pages from-to

    9-26

  • UT code for WoS article

    000333729300002

  • EID of the result in the Scopus database