Star · F9V
TOI-4379
TOI-4379 is a main-sequence star of spectral type F9V in the constellation Scorpius, 2,104 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Scorpius |
|---|---|
| Distance | 2,104 light-years (645.2 pc) |
| Apparent magnitude | magnitude 12.66 |
| Absolute magnitude | magnitude 3.61 |
| Spectral type | F9V |
| Surface temperature | 6,020 K |
| Luminosity | 4.34 L☉ |
| Radius | 1.98 R☉ |
| Mass | 1.37 M☉ |
| Age | 4.5 billion years |
| Metallicity [Fe/H] | 0.16 |
| Right ascension (J2000) | 16h 48m 11.5s |
| Declination (J2000) | −32° 26′ 02″ |
| Space velocity (relative to the Sun) | 62.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.66. Visible from the whole Southern Hemisphere and north to latitude 58° N. South of latitude 58° S it never sets. It stands highest at midnight in June, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around 79 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 37 million years.
The Sun seen from there
From a planet around TOI-4379, the Sun would look like a star of magnitude 13.88, in the direction where our sky has the constellation Auriga. It would be invisible to the naked eye.
Planets
- TOI-4379 b 3.25-day orbit · 16.7 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.