タイトル | The 1983 June 15 occultation by Neptune. I - Limits on a possible ring system |
著者(英) | Dunham, E. W.; Erickson, E. F.; Meech, K. J.; Baron, R. L.; Mink, D. J.; French, R. G.; Elliot, J. L. |
著者所属(英) | Massachusetts Inst. of Tech.|NASA Ames Research Center |
発行日 | 1985-12-01 |
言語 | eng |
内容記述 | Observations on 15 June 1983 of an occultation of a star by Neptune from Mauna Kea, Mount Stromlo, Siding Spring, and the Kuiper Airborne Observatory show no evidence for equatorial rings between 25,300 and 200,000 km (R/N/ = 25,269 km). Within most of this region, the upper limit on the optical depth along the line of sight, for rings broader than 6 km , is 0.04, which corresponds to a normal optical depth of 0.016. These results rule out a Neptunian ring system similar to that of Saturn or Uranus, but not a system of low optical depth similar to the Jovian rings. The data show no features that appear likely to have been caused by material in the equatorial plane of Neptune near the Roche limit. |
NASA分類 | ASTRONOMY |
レポートNO | 86A18270 |
権利 | Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/387233 |
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