Super-catastrophic disruption of asteroids at small perihelion distances
Status PubMed-not-MEDLINE Jazyk angličtina Země Anglie, Velká Británie Médium print
Typ dokumentu časopisecké články, práce podpořená grantem, Research Support, U.S. Gov't, Non-P.H.S.
PubMed
26887492
DOI
10.1038/nature16934
PII: nature16934
Knihovny.cz E-zdroje
- Publikační typ
- časopisecké články MeSH
- práce podpořená grantem MeSH
- Research Support, U.S. Gov't, Non-P.H.S. MeSH
Most near-Earth objects came from the asteroid belt and drifted via non-gravitational thermal forces into resonant escape routes that, in turn, pushed them onto planet-crossing orbits. Models predict that numerous asteroids should be found on orbits that closely approach the Sun, but few have been seen. In addition, even though the near-Earth-object population in general is an even mix of low-albedo (less than ten per cent of incident radiation is reflected) and high-albedo (more than ten per cent of incident radiation is reflected) asteroids, the characterized asteroids near the Sun typically have high albedos. Here we report a quantitative comparison of actual asteroid detections and a near-Earth-object model (which accounts for observational selection effects). We conclude that the deficit of low-albedo objects near the Sun arises from the super-catastrophic breakup (that is, almost complete disintegration) of a substantial fraction of asteroids when they achieve perihelion distances of a few tens of solar radii. The distance at which destruction occurs is greater for smaller asteroids, and their temperatures during perihelion passages are too low for evaporation to explain their disappearance. Although both bright and dark (high- and low-albedo) asteroids eventually break up, we find that low-albedo asteroids are more likely to be destroyed farther from the Sun, which explains the apparent excess of high-albedo near-Earth objects and suggests that low-albedo asteroids break up more easily as a result of thermal effects.
Department of Physics PO Box 64 00014 University of Helsinki Finland
Finnish Geospatial Research Institute PO Box 15 02430 Masala Finland
Institute for Astronomy University of Hawaii 2680 Woodlawn Drive Honolulu Hawaii 96822 USA
Institute of Astronomy Charles University 5 Holešovikách 2 CZ 18000 Prague 8 Czech Republic
Observatoire de la Cote d'Azur Boulevard de l'Observatoire F 06304 Nice Cedex 4 France
Southwest Research Institute 1050 Walnut Street Suite 300 Boulder Colorado 80302 USA
University of Arizona 933 North Cherry Avenue Tucson Arizona 85721 0065 USA
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