Star · G9V
TOI-2876
TOI-2876 is a main-sequence star of spectral type G9V in the constellation Canis Major, 736.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Canis Major |
|---|---|
| Distance | 736.3 light-years (225.7 pc) |
| Apparent magnitude | magnitude 12.40 |
| Absolute magnitude | magnitude 5.63 |
| Spectral type | G9V |
| Surface temperature | 5,270 K |
| Luminosity | 0.529 L☉ |
| Radius | 0.873 R☉ |
| Mass | 0.939 M☉ |
| Age | 3.8 billion years |
| Metallicity [Fe/H] | 0.35 |
| Right ascension (J2000) | 7h 20m 59.4s |
| Declination (J2000) | −21° 06′ 53″ |
| Space velocity (relative to the Sun) | 16.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.40. Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° S it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1290. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 13 million years.
The Sun seen from there
From a planet around TOI-2876, the Sun would look like a star of magnitude 11.60, in the direction where our sky has the constellation Vulpecula. It would be invisible to the naked eye.
Planets
- TOI-2876 b 6.3-day orbit · 9.64 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.