Star · G4V
TOI-6174
TOI-6174 is a main-sequence star of spectral type G4V in the constellation Pegasus, 2,343 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pegasus |
|---|---|
| Distance | 2,343 light-years (718.3 pc) |
| Apparent magnitude | magnitude 13.86 |
| Absolute magnitude | magnitude 4.58 |
| Spectral type | G4V |
| Surface temperature | 5,640 K |
| Luminosity | 1.38 L☉ |
| Radius | 1.23 R☉ |
| Mass | 1 M☉ |
| Metallicity [Fe/H] | 0.35 |
| Right ascension (J2000) | 22h 25m 36.0s |
| Declination (J2000) | +32° 31′ 28″ |
| Space velocity (relative to the Sun) | 28.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.86. Visible from the whole Northern Hemisphere and south to latitude 57° S. North of latitude 57° N it never sets. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around 318 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 42 million years.
The Sun seen from there
From a planet around TOI-6174, the Sun would look like a star of magnitude 14.11, in the direction where our sky has the constellation Antlia. It would be invisible to the naked eye.
Planets
- TOI-6174 b 3.52-day orbit · 7.83 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.