Star · M4V
2MASS J00062250+1300451
2MASS J00062250+1300451 is a main-sequence star of spectral type M4V in the constellation Pegasus, 231.6 light-years from the Sun.
| Constellation | Pegasus |
|---|---|
| Distance | 231.6 light-years (71.0 pc) |
| Apparent magnitude | magnitude 22.46 |
| Absolute magnitude | magnitude 18.20 |
| Spectral type | M4V |
| Surface temperature | 2,980 K |
| Luminosity | 8.21 × 10⁻⁵ L☉ |
| Radius | 0.0341 R☉ |
| Mass | 0.075 M☉ (estimated) |
| Right ascension (J2000) | 0h 06m 22.5s |
| Declination (J2000) | +13° 00′ 45″ |
| Space velocity (relative to the Sun) | 22.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 22.46. Visible from the whole Northern Hemisphere and south to latitude 77° S. North of latitude 77° N it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1794. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.1 million years.
The Sun seen from there
From a planet around 2MASS J00062250+1300451, the Sun would look like a star of magnitude 9.09, in the direction where our sky has the constellation Corvus. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 867 10.9 light-years
- SDSS J000632.60+140606.3 13.7 light-years
- HIP 795 18.8 light-years
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.