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