Star · F8 V
HD 110082
HD 110082 is a main-sequence star of spectral type F8 V in the constellation Octans, 342.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | HIP 62662 |
|---|---|
| Constellation | Octans |
| Distance | 342.9 light-years (105.1 pc) |
| Apparent magnitude | magnitude 9.23 |
| Absolute magnitude | magnitude 4.12 |
| Spectral type | F8 V |
| Surface temperature | 6,200 K |
| Luminosity | 1.91 L☉ |
| Radius | 1.19 R☉ |
| Mass | 1.21 M☉ |
| Age | 0.3 billion years |
| Metallicity [Fe/H] | 0.08 |
| Right ascension (J2000) | 12h 50m 21.9s |
| Declination (J2000) | −88° 07′ 16″ |
| Space velocity (relative to the Sun) | 13.2 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.23. Visible from the whole Southern Hemisphere and north to latitude 2° N. South of latitude 2° S it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1683. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 6.1 million years.
The Sun seen from there
From a planet around HD 110082, the Sun would look like a star of magnitude 9.94, in the direction where our sky has the constellation Cepheus. It would be invisible to the naked eye.
Planets
- HD 110082 b 10.2-day orbit · 3.2 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.