MOA-2008-BLG-310Lb [SEP] constellation
MOA-2008-BLG-310Lb
MOA-2008-BLG-310Lb is an extrasolar planet which orbits probably the late K-type star MOA-2008-BLG-310L, located at least 20000 light years away in the constellation Scorpius. This planet has mass 23% of Jupiter or 77% of Saturn and orbits at 1.25 AU from the star. This planet was discovered by using the gravitational microlensing method on August 4, 2009. As it is typical for exoplanets detected by microlensing method, the orbital period and eccentricity are not determined.
See also.
- MOA-2007-BLG-192Lb
- OGLE-2005-BLG-390Lb
References
extrasolar planets.
Planets discovered.
μFUN played an important role in discovery and analysis of the following extrasolar planets:
- OGLE-2005-BLG-071Lb
- OGLE-2005-BLG-071Lb
- OGLE-2005-BLG-169Lb
- OGLE-2006-BLG-109Lb, OGLE-2006-BLG-109Lc
- MOA-2007-BLG-400Lb
- MOA-2008-BLG-310Lb
- MOA-2009-BLG-387Lb
- MOA-2009-BLG-319Lb
- MOA-2011-BLG-293Lb,
- MOA-2010-BLG-477,
Public involvement.
There are various ways to get involved with μFUN. Since μFUN is a follow-up network, initial data and observations come from outside sources, primarily OGLE-III and MOA. However, many