MOA-2011-BLG-262L is a red dwarf[citation needed] or possibly a rogue planet[1] which may have an exomoon named MOA-2011-BLG-262L b. The exomoon is still most likely a Neptune-like planet.[2]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 18 M🜨 | ~1 | — | — | — | — |
| Discovery | |
|---|---|
| Discovery date | 2013 |
Detection method | Microlensing |
| Designations | |
Alternative names | MOA-2011-BLG-262 |
| Orbital characteristics | |
| Periastron | N/A |
| Apastron | N/A |
Semi-major axis | N/A AU |
| Eccentricity | N/A |
Orbital period (sidereal) | N/A d (N/A y) |
Average orbital speed | N/A km/s |
| Inclination | N/A |
Angular distance | ? mas |
Longitude of periastron | N/A° |
Time of periastron | N/A JD |
| Semi-amplitude | N/A m/s |
| Star | N/A |
| Physical characteristics | |
| Mass | ~4 MJ |
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