Star · G3V
TOI-5322
TOI-5322 is a main-sequence star of spectral type G3V in the constellation Pisces, 1,555 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pisces |
|---|---|
| Distance | 1,555 light-years (476.9 pc) |
| Apparent magnitude | magnitude 12.73 |
| Absolute magnitude | magnitude 4.34 |
| Spectral type | G3V |
| Surface temperature | 5,690 K |
| Luminosity | 2.03 L☉ |
| Radius | 1.46 R☉ |
| Mass | 0.998 M☉ |
| Age | 9.7 billion years |
| Metallicity [Fe/H] | -0.05 |
| Right ascension (J2000) | 0h 26m 07.0s |
| Declination (J2000) | +14° 20′ 11″ |
| Space velocity (relative to the Sun) | 28.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.73. Visible from the whole Northern Hemisphere and south to latitude 76° S. North of latitude 76° N it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 471. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 28 million years.
The Sun seen from there
From a planet around TOI-5322, the Sun would look like a star of magnitude 13.22, in the direction where our sky has the constellation Corvus. It would be invisible to the naked eye.
Planets
- TOI-5322 b 5.42-day orbit · 16.6 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.