OGLE-2005-BLG-390
True-colour image of the OGLE-2005-BLG-390 field (as observed by the PLANET team with the Danish 1.54m telescope).
Modeling of the light curve indicates that the deviation in the light curve of OGLE-2005-BLG-390 is caused by a record small mass planet. The new planetary system is also the most distant among all known extrasolar planetary system. Parameters of the OGLE-2005-BLG-390 event
| Mplanet / Mstar | (Mass ratio of the lens components) | 7.6+/-0.7 * 10^-5 | ||||
| aproj / RE | (Orbital
distance assuming circular orbit in Einstein ring units) | 1.610 +/-0.008 | ||||
| φ | (Position angle) | 2.756 +/-0.003 [rad] | ||||
| u0 | (Impact parameter in
Einstein ring units) | 0.359 +/-0.005 | ||||
| t0 | (Time of the closest approach
to the center of mass) | 31.231+/-0.005 July 2005 | ||||
| tE | (Einstein ring crossing time) | 11.03 +/-0.11 [days] | ||||
| I0 | (Unmagnified brightness of the
source star in the I-band) | 15.561 +/-0.002 [mag] | ||||
| Ibaseline | (I-band
magnitude of the blend at baseline) | 15.561 +/-0.002 [mag] |
Estimation of parameters of the lensing system:
| Mstar | (Mass of the star) | 0.22 +0.21-0.11 [MSun] | ||||
| Mplanet | (Mass of the planet) | 5.5 +5.5-2.7 [MEarth] | ||||
| a | (Projected distance) | 2.6 +1.5-0.6 [AU] | ||||
| Dlens | (Distance to the lensing system) | 6.6 +/-1.0 [kpc] |
Equatorial coordinates of OGLE-2005-BLG-390:
RA = 17:54:19.19 DEC = -30:22:38.3 (J2000.0)
OGLE photometric data of OGLE-2005-BLG-390 (regularly updated when additional observations of the lens field are collected) are available from the OGLE-2005-BLG-390 EVENT PAGE.
PLANET photometric data of OGLE-2005-BLG-390 are
available HERE:
MOA-2 photometric data of OGLE-2005-BLG-390 are available HERE.
Additional information can be found on the PLANET team WWW pages.