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- W2564442962 abstract "Most asteroids of the near-Earth population have experienced significant collisional processing since they formed, being disrupted and excavated and consequently producing smaller bodies that are delivered from the Main asteroid Belt to the near-Earth asteroid region, thanks to planetary resonances and non-gravitational forces. By studying meteorites arrived to Earth we can obtain clues on this processing through the study of shock metamorphism and brecciation of their rock constituents, among other features. The massive Chelyabinsk meteorite fall produced about one metric ton of meteorites that can be analyzed to decipher the physical processes affecting the surface of this Potentially Hazardous Asteroid. Here we describe physical properties of Chelyabinsk samples, and how impact processing has affected asteroid albedos, a first step in order to relate this data with the reflectance properties of near-Earth asteroids population. This information will be of major interest for future asteroid deflecting missions." @default.
- W2564442962 created "2017-01-06" @default.
- W2564442962 creator A5021308810 @default.
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- W2564442962 creator A5083215581 @default.
- W2564442962 creator A5084734769 @default.
- W2564442962 date "2016-12-20" @default.
- W2564442962 modified "2023-09-26" @default.
- W2564442962 title "Chelyabinsk Meteorite as a Proxy for Studying the Properties of Potentially Hazardous Asteroids and Impact Deflection Strategies" @default.
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- W2564442962 doi "https://doi.org/10.1007/978-3-319-46179-3_11" @default.
- W2564442962 hasPublicationYear "2016" @default.
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