Star · M3V
2MASS J09352803-2934596
2MASS J09352803-2934596 is a main-sequence star of spectral type M3V in the constellation Antlia, 108.8 light-years from the Sun.
| Constellation | Antlia |
|---|---|
| Distance | 108.8 light-years (33.4 pc) |
| Apparent magnitude | magnitude 21.48 |
| Absolute magnitude | magnitude 18.86 |
| Spectral type | M3V |
| Surface temperature | 3,160 K |
| Luminosity | 2.80 × 10⁻⁵ L☉ |
| Radius | 0.0177 R☉ |
| Mass | 0.075 M☉ (estimated) |
| Right ascension (J2000) | 9h 35m 28.0s |
| Declination (J2000) | −29° 34′ 58″ |
| Space velocity (relative to the Sun) | 11.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 21.48. Visible from the whole Southern Hemisphere and north to latitude 60° N. South of latitude 60° S it never sets. It stands highest at midnight in February, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1917. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.
The Sun seen from there
From a planet around 2MASS J09352803-2934596, the Sun would look like a star of magnitude 7.45, in the direction where our sky has the constellation Cygnus. It would be invisible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.