Star · M3
TOI-6383 A
TOI-6383 A is a main-sequence star of spectral type M3 in the constellation Camelopardalis, 558.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Camelopardalis |
|---|---|
| Distance | 558.8 light-years (171.3 pc) |
| Apparent magnitude | magnitude 16.63 |
| Absolute magnitude | magnitude 10.46 |
| Spectral type | M3 |
| Surface temperature | 3,440 K |
| Luminosity | 0.0326 L☉ |
| Radius | 0.457 R☉ |
| Mass | 0.458 M☉ |
| Right ascension (J2000) | 4h 01m 41.9s |
| Declination (J2000) | +60° 53′ 29″ |
| Space velocity (relative to the Sun) | 53.4 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 16.63. Visible from the whole Northern Hemisphere and south to latitude 29° S. North of latitude 29° N it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1467. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 9.9 million years.
The Sun seen from there
From a planet around TOI-6383 A, the Sun would look like a star of magnitude 11.00, in the direction where our sky has the constellation Triangulum Australe. It would be invisible to the naked eye.
Planets
- TOI-6383 A b 1.79-day orbit · 11.3 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.