Star · G2V
MOA-2010-BLG-117L
MOA-2010-BLG-117L is a main-sequence star of spectral type G2V in the constellation Sagittarius, 11,400 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Sagittarius |
|---|---|
| Distance | 11,400 light-years (3,500 pc) |
| Apparent magnitude | magnitude 24.30 |
| Absolute magnitude | magnitude 11.58 |
| Spectral type | G2V |
| Surface temperature | 5,780 K |
| Luminosity | 0.00217 L☉ |
| Radius | 0.0464 R☉ |
| Mass | 0.58 M☉ (estimated) |
| Right ascension (J2000) | 18h 07m 49.7s |
| Declination (J2000) | −25° 20′ 41″ |
In the sky
A telescope is needed to see it: its apparent magnitude is 24.30. Visible from the whole Southern Hemisphere and north to latitude 65° N. South of latitude 65° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 11 thousand years ago. At that time the first farming villages were being founded; there was no writing yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 203 million years.
The Sun seen from there
From a planet around MOA-2010-BLG-117L, the Sun would look like a star of magnitude 17.55, in the direction where our sky has the constellation Gemini. It would be invisible to the naked eye.
Planets
- MOA-2010-BLG-117L b 14.2 R⊕
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.