Star · G7IV
TOI-5624
TOI-5624 is a subgiant star of spectral type G7IV in the constellation Ursa Major, 330.7 light-years from the Sun. It is orbited by 5 confirmed exoplanet(s).
| Constellation | Ursa Major |
|---|---|
| Distance | 330.7 light-years (101.4 pc) |
| Apparent magnitude | magnitude 10.89 |
| Absolute magnitude | magnitude 5.86 |
| Spectral type | G7IV |
| Surface temperature | 5,330 K |
| Luminosity | 0.486 L☉ |
| Radius | 0.82 R☉ |
| Mass | 0.858 M☉ |
| Age | 5.7 billion years |
| Metallicity [Fe/H] | -0.02 |
| Right ascension (J2000) | 12h 03m 22.8s |
| Declination (J2000) | +49° 15′ 04″ |
| Space velocity (relative to the Sun) | 48.1 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 10.89. Visible from the whole Northern Hemisphere and south to latitude 41° S. North of latitude 41° N it never sets. It stands highest at midnight in March, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1695. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.9 million years.
The Sun seen from there
From a planet around TOI-5624, the Sun would look like a star of magnitude 9.86, in the direction where our sky has the constellation Phoenix. It would be invisible to the naked eye.
Planets
- TOI-5624 b 3.39-day orbit · 2.31 R⊕
- TOI-5624 c 7.89-day orbit · 2.47 R⊕
- TOI-5624 d 13.7-day orbit · 3.58 R⊕
- TOI-5624 e 21.5-day orbit · 3.25 R⊕
- TOI-5624 f 45.4-day orbit · 3.66 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.