Star · F9V
TOI-3919
TOI-3919 is a main-sequence star of spectral type F9V in the constellation Canes Venatici, 1,972 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Canes Venatici |
|---|---|
| Distance | 1,972 light-years (604.6 pc) |
| Apparent magnitude | magnitude 12.86 |
| Absolute magnitude | magnitude 3.95 |
| Spectral type | F9V |
| Surface temperature | 6,100 K |
| Luminosity | 2.17 L☉ |
| Radius | 1.32 R☉ |
| Mass | 1.21 M☉ |
| Age | 3.1 billion years |
| Metallicity [Fe/H] | 0.18 |
| Right ascension (J2000) | 13h 55m 46.7s |
| Declination (J2000) | +40° 23′ 31″ |
| Space velocity (relative to the Sun) | 6.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.86. Visible from the whole Northern Hemisphere and south to latitude 50° S. North of latitude 50° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 54. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 35 million years.
The Sun seen from there
From a planet around TOI-3919, the Sun would look like a star of magnitude 13.74, in the direction where our sky has the constellation Phoenix. It would be invisible to the naked eye.
Planets
- TOI-3919 b 7.43-day orbit · 12.3 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.