Star · G0
TOI-5082
TOI-5082 is a main-sequence star of spectral type G0 in the constellation Gemini, 140.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | HIP 34271 |
|---|---|
| Constellation | Gemini |
| Distance | 140.4 light-years (43.0 pc) |
| Apparent magnitude | magnitude 8.25 |
| Absolute magnitude | magnitude 5.08 |
| Spectral type | G0 |
| Surface temperature | 5,670 K |
| Luminosity | 0.814 L☉ |
| Radius | 0.93 R☉ |
| Mass | 0.997 M☉ |
| Metallicity [Fe/H] | 0.09 |
| Right ascension (J2000) | 7h 06m 16.8s |
| Declination (J2000) | +22° 41′ 01″ |
| Space velocity (relative to the Sun) | 49.4 km/s |
In the sky
Too faint for the naked eye (magnitude 8.25); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 67° S. North of latitude 67° N it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1886. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.5 million years.
The Sun seen from there
From a planet around TOI-5082, the Sun would look like a star of magnitude 8.00, in the direction where our sky has the constellation Sagittarius. It would be invisible to the naked eye.
Planets
- TOI-5082.01 4.24-day orbit · 2.55 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.