Star · M0V
TOI-782
TOI-782 is a main-sequence star of spectral type M0V in the constellation Corvus, 170.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Corvus |
|---|---|
| Distance | 170.3 light-years (52.2 pc) |
| Apparent magnitude | magnitude 14.83 |
| Absolute magnitude | magnitude 11.24 |
| Spectral type | M0V |
| Surface temperature | 3,370 K |
| Luminosity | 0.0198 L☉ |
| Radius | 0.413 R☉ |
| Mass | 0.397 M☉ |
| Metallicity [Fe/H] | 0.34 |
| Right ascension (J2000) | 12h 15m 40.9s |
| Declination (J2000) | −18° 54′ 37″ |
| Space velocity (relative to the Sun) | 41.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.83. Visible from the whole Southern Hemisphere and north to latitude 71° N. South of latitude 71° S it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1856. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.0 million years.
The Sun seen from there
From a planet around TOI-782, the Sun would look like a star of magnitude 8.42, in the direction where our sky has the constellation Pisces. It would be invisible to the naked eye.
Planets
- TOI-782 b 8.02-day orbit · 2.73 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.