MOA-2007-BLG-192L is a star with 0.06 times the mass of the Sun, and NaN times its radius. It is located 3261.56 light years away from the solar system.
MOA-2007-BLG-192L is known to have 1 exoplanets in orbit around it.
MOA-2007-BLG-192L b was discovered by the MOA observatory, in 2008-09, using the microlensing method. Its semi-major axis is 0.62 astronomical units, as compared to Earth's which is 1 astronomical unit. The mass of MOA-2007-BLG-192L b is 3.180 times the mass of Earth. The radius of MOA-2007-BLG-192L b is 1.630 that of Earth. At 3.180 Earth masses, MOA-2007-BLG-192L b is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses. With a mass below 5 Earth masses, and a semi-major axis of 0.62 astronomical units, which is outside the habitable zone of MOA-2007-BLG-192L, MOA-2007-BLG-192L b is likely an icy world.