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An Excess Due to Small Grains Around The Nearby K 0 V Star HD 69830 : Asteroid or Cometary Debris ?
| Content Provider | Semantic Scholar |
|---|---|
| Copyright Year | 2005 |
| Abstract | Spitzer photometry and spectroscopy of the star HD 69830 reveal an excess of emission relative to the stellar photosphere between 8 and 35 m dominated by strong features attributable to crystalline silicates with an emitting surface area more than 1000 times that of our zodiacal cloud. The spectrum closely resembles that of the comet C/1995 O1 (Hale-Bopp). Since no excess is detected at 70 m, the emitting material must be quite warm, be confined within a few AU of the star, and originate in grains with low, long-wavelength emissivity, i.e., grains much smaller than 70 m/2 10 m.The strongmineralogical features are evidence for even smaller, possibly submicronsized grains. This small grain size is in direct contrast to the 10–100 m grains that dominate the relatively featureless spectra of our zodiacal dust cloud and most other main-sequence stars with excesses. The upper limit at 70 m also implies that any Kuiper Belt analog must be either very cold or less massive than 5 times our own Kuiper Belt. With collisional and Poynting-Robertson drag times of less than 1000 yr for small grains, the emitting material must either (1) be created through continual grinding down of material in a dense asteroid belt, or (2) originate in cometary debris arising from either a single ‘‘supercomet’’ or a very large number of individual comets arriving from a distant reservoir. In the case of a cometary origin for the emission, the mass requirements for continuous generation by many individual comets are unreasonable, and we favor the capture of a single super comet into a 0.5–1 AU orbit, where it can evolve a large number of small grains over a 2 Myr period. Subject headinggs: circumstellar matter — comets: general — infrared: stars — Kuiper Belt — planetary systems Online material: color figures |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://arxiv.org/pdf/astro-ph/0504491v2.pdf |
| Alternate Webpage(s) | http://w.astro.berkeley.edu/~kalas/disksite/library/beichman05b.pdf |
| Alternate Webpage(s) | http://arxiv.org/pdf/astro-ph/0504491v1.pdf |
| Language | English |
| Access Restriction | Open |
| Subject Keyword | Analog Belt machine Cloud computing Comet Scoring Engine Command & Conquer:Yuri's Revenge GUCY2C protein, human Gold Greater Than Less Than Listeria monocytogenes O1 Ab:Titr:Pt:Ser:Qn Offset binary One Thousand Photometry Planetary scanner Poynting's theorem Requirement Reservoir Device Component Significant figures Silicates Small Stars, Celestial Stellar (payment network) Structure of lens capsule wavelength |
| Content Type | Text |
| Resource Type | Article |