Star · G2V
TOI-2416
TOI-2416 is a main-sequence star of spectral type G2V in the constellation Reticulum, 1,819 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Reticulum |
|---|---|
| Distance | 1,819 light-years (557.7 pc) |
| Apparent magnitude | magnitude 13.02 |
| Absolute magnitude | magnitude 4.29 |
| Spectral type | G2V |
| Surface temperature | 5,810 K |
| Luminosity | 1.57 L☉ |
| Radius | 1.24 R☉ |
| Mass | 1.12 M☉ |
| Age | 4.9 billion years |
| Metallicity [Fe/H] | 0.32 |
| Right ascension (J2000) | 3h 49m 21.3s |
| Declination (J2000) | −60° 47′ 14″ |
| Space velocity (relative to the Sun) | 35.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.02. Visible from the whole Southern Hemisphere and north to latitude 29° N. South of latitude 29° S 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 207. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 32 million years.
The Sun seen from there
From a planet around TOI-2416, the Sun would look like a star of magnitude 13.56, in the direction where our sky has the constellation Draco. It would be invisible to the naked eye.
Planets
- TOI-2416 b 8.28-day orbit · 9.86 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.