Melted Crumbs from Asteroid Vesta

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Micrometeorite, Cosmic Spherule, South Pole, Iron, Magnesium, Manganese, Hed, Meteorite, Achondrite, Parent Body, Vesta

Scientific paper

Micrometeorite bombardment accounts for almost 30,000 tons of material entering Earth's atmosphere each year. Though most of the material evaporates during entry or is lost to sea or falls on the land unnoticed, thousands of micrometeorites have been collected successfully from deep-sea sediments and from the snow and ice of the polar caps. Susan Taylor (Cold Regions Research and Engineering Laboratory) and colleagues collected micrometeorites with an ingeniously designed robot from a decidedly out-of-the-way place: Amundsen-Scott South Pole Station water well. She and Greg Herzog and Jeremy Delaney (Rutgers University) selected 10 out of thousands of these extraterrestrial particles, 75 to 700 micrometers in size, because of their unusual shapes and mineralogy, and measured the Fe/Mn and Fe/Mg elemental ratios, which are known to help constrain the type and source of meteorites. The results show that nine of the cosmic spherules are broadly chondritic in composition as expected. However, one, along with six others reexamined from a previous study, are atypical with nonchondritic compositions. Taylor and coauthors propose an origin from an achondrite, Howardite-Eucrite-Diogenite (HED)-like parent body such as asteroid Vesta. HED-like objects account for about 6% of all meteorites, and only about 0.5% of all micrometeorites perhaps because of a natural mechanical toughness that would resist breakup and fragmentation.

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