Detection of transits of the nearby hot Neptune GJ 436 b

被引:231
作者
Gillon, M. [1 ]
Pont, F.
Demory, B.-O.
Mallmann, F.
Mayor, M.
Mazeh, T.
Queloz, D.
Shporer, A.
Udry, S.
Vuissoz, C.
机构
[1] Univ Geneva, Observ Geneva, CH-1290 Sauverny, Switzerland
[2] Univ Liege, Inst Astrophys & Geophys, B-4000 Liege, Belgium
[3] Observ Francois Xavier Bagnoud OFXB, CH-3961 St Luc, Switzerland
[4] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[5] EPFL, Astrophys Lab, CH-1290 Sauverny, Switzerland
关键词
stars : planetary systems; stars : individual : GJ 436; techniques : photometric;
D O I
10.1051/0004-6361:20077799
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This Letter reports on the photometric detection of transits of the Neptune-mass planet orbiting the nearby M-dwarf star GJ 436. It is by far the closest, smallest, and least massive transiting planet detected so far. Its mass is slightly larger than Neptune's at M = 22.6 +/- 1.9 M-circle plus. The shape and depth of the transit lightcurves show that it is crossing the host star disc near its limb (impact parameter 0.84 +/- 0.03) and that the planet size is comparable to that of Uranus and Neptune, R = 25 200 +/- 2200 km = 3.95 +/- 0.35 R-circle plus. Its main constituant is therefore very likely to be water ice. If the current planet structure models are correct, an outer layer of H/He constituting up to ten percent in mass is probably needed on top of the ice to account for the observed radius.
引用
收藏
页码:L13 / L16
页数:4
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