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Dust Grains from 9P/Tempel 1 Before and After the Encounter with Deep Impact
Gemini-N observed the properties of dust ejected from the nucleus of comet 9P/Tempel 1 before and after its encounter with Deep Impact. Marked changes were seen in the 7.8- to 13-micrometer spectral energy distribution and derived grain properties of the inner coma. A strong, broad silicate feature...
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Published in: | Science (American Association for the Advancement of Science) 2005-10, Vol.310 (5746), p.278-280 |
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description | Gemini-N observed the properties of dust ejected from the nucleus of comet 9P/Tempel 1 before and after its encounter with Deep Impact. Marked changes were seen in the 7.8- to 13-micrometer spectral energy distribution and derived grain properties of the inner coma. A strong, broad silicate feature dominated by emission from amorphous pyroxene, amorphous olivine, and magnesium-rich crystalline olivine had developed by 1 hour after impact. The ejected dust mass is [congruent]10⁴ to 10⁶ kilograms on the basis of our models. Twenty-six hours later the silicate feature had faded, leaving a smooth featureless spectrum, similar to that observed before the impact, suggesting that the impact did not produce a new active region releasing small particles on the nucleus. |
doi_str_mv | 10.1126/science.1119143 |
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Marked changes were seen in the 7.8- to 13-micrometer spectral energy distribution and derived grain properties of the inner coma. A strong, broad silicate feature dominated by emission from amorphous pyroxene, amorphous olivine, and magnesium-rich crystalline olivine had developed by 1 hour after impact. The ejected dust mass is [congruent]10⁴ to 10⁶ kilograms on the basis of our models. Twenty-six hours later the silicate feature had faded, leaving a smooth featureless spectrum, similar to that observed before the impact, suggesting that the impact did not produce a new active region releasing small particles on the nucleus.</abstract><cop>United States</cop><pub>American Association for the Advancement of Science</pub><pmid>16166478</pmid><doi>10.1126/science.1119143</doi><tpages>3</tpages></addata></record> |
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subjects | Analysis Astronomical research Astrophysics Climate Cometary comas Comets Cosmic Dust Electronic publishing Meteoroids Natural history Observational astronomy Observational research Olivine Organic Chemicals - analysis Particle resonance Pyroxenes Silicates Spectrophotometry, Infrared Spectrum analysis |
title | Dust Grains from 9P/Tempel 1 Before and After the Encounter with Deep Impact |
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