Images of Neptune's ring arcs obtained by a ground-based telescope

被引:32
作者
Sicardy, B [1 ]
Roddier, F
Roddier, C
Perozzi, E
Graves, JE
Guyon, O
Northcott, MJ
机构
[1] Univ Paris 06, Observ Paris, Inst Univ France, DESPA, F-92195 Meudon, France
[2] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[3] Telespazio SpA, I-00156 Rome, Italy
[4] Ecole Normale Super, F-75230 Paris 05, France
关键词
D O I
10.1038/23410
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Neptune has a collection of incomplete narrow rings, known as ring arcs, which should in isolation be destroyed by differential motion in a matter of months. Yet since first discovered(1) by stellar occultations in 1984, they appear to have persisted(2-6), perhaps through a gravitational resonance effect involving the satellite Galatea(6-8). Here we report ground-based observations of the ring arcs, obtained using an adaptive optics system. Our data, and those obtained using the Hubble Space Telescope (reported in a companion paper(9)), indicate that the ring arcs are near, but not within the resonance with Galatea, in contrast to what is predicted by some models.
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页码:731 / 733
页数:3
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