| Literature DB >> 18276883 |
B S Gaudi1, D P Bennett, A Udalski, A Gould, G W Christie, D Maoz, S Dong, J McCormick, M K Szymanski, P J Tristram, S Nikolaev, B Paczynski, M Kubiak, G Pietrzynski, I Soszynski, O Szewczyk, K Ulaczyk, L Wyrzykowski, D L Depoy, C Han, S Kaspi, C-U Lee, F Mallia, T Natusch, R W Pogge, B-G Park, F Abe, I A Bond, C S Botzler, A Fukui, J B Hearnshaw, Y Itow, K Kamiya, A V Korpela, P M Kilmartin, W Lin, K Masuda, Y Matsubara, M Motomura, Y Muraki, S Nakamura, T Okumura, K Ohnishi, N J Rattenbury, T Sako, To Saito, S Sato, L Skuljan, D J Sullivan, T Sumi, W L Sweatman, P C M Yock, M D Albrow, A Allan, J-P Beaulieu, M J Burgdorf, K H Cook, C Coutures, M Dominik, S Dieters, P Fouqué, J Greenhill, K Horne, I Steele, Y Tsapras, B Chaboyer, A Crocker, S Frank, B Macintosh.
Abstract
Searches for extrasolar planets have uncovered an astonishing diversity of planetary systems, yet the frequency of solar system analogs remains unknown. The gravitational microlensing planet search method is potentially sensitive to multiple-planet systems containing analogs of all the solar system planets except Mercury. We report the detection of a multiple-planet system with microlensing. We identify two planets with masses of approximately 0.71 and approximately 0.27 times the mass of Jupiter and orbital separations of approximately 2.3 and approximately 4.6 astronomical units orbiting a primary star of mass approximately 0.50 solar mass at a distance of approximately 1.5 kiloparsecs. This system resembles a scaled version of our solar system in that the mass ratio, separation ratio, and equilibrium temperatures of the planets are similar to those of Jupiter and Saturn. These planets could not have been detected with other techniques; their discovery from only six confirmed microlensing planet detections suggests that solar system analogs may be common.Entities:
Year: 2008 PMID： 18276883 DOI： 10.1126/science.1151947
Source DB: PubMed Journal: Science ISSN： 0036-8075 Impact factor: 47.728