The Galactic Exoplanet Survey Telescope (GEST)

被引:13
作者
Bennett, DP [1 ]
Bally, J [1 ]
Bond, I [1 ]
Cheng, E [1 ]
Cook, K [1 ]
Deming, D [1 ]
Gamavich, P [1 ]
Griest, K [1 ]
Jewitt, D [1 ]
Kaiser, N [1 ]
Lauer, T [1 ]
Lunine, J [1 ]
Luppino, G [1 ]
Mather, J [1 ]
Minniti, D [1 ]
Peale, S [1 ]
Rhie, S [1 ]
Rhodes, J [1 ]
Schneider, J [1 ]
Sonneborn, G [1 ]
Stevenson, R [1 ]
Stubbs, C [1 ]
Tenerelli, D [1 ]
Woolf, N [1 ]
Yock, P [1 ]
机构
[1] Univ Notre Dame, Notre Dame, IN 46556 USA
来源
FUTURE EUV/UV AND VISIBLE SPACE ASTROPHYSICS MISSIONS AND INSTRUMENTATION | 2003年 / 4854卷
关键词
extra-solar planets; gravitational lensing; SPIE proceedings;
D O I
10.1117/12.459816
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The Galactic Exoplanet Survey Telescope (GEST) will observe a 2 square degree field in the Galactic bulge to search for extra-solar planets using a gravitational lensing technique. This gravitational lensing technique is the only method employing currently available technology that can detect Earth-mass planets at high signal-to-noise, and can measure the abundance of terrestrial planets as a function of Galactic position. GEST's sensitivity extends down to the mass of Mars, and it can detect hundreds of terrestrial planets with semi-major axes ranging from 0.7 AU to infinity. GEST will be the first truly comprehensive survey of the Galaxy for planets like those, in our own Solar System.
引用
收藏
页码:141 / 157
页数:17
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