Star · K7V
TOI-1105
TOI-1105 is a main-sequence star of spectral type K7V in the constellation Octans, 259.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Octans |
|---|---|
| Distance | 259.0 light-years (79.4 pc) |
| Apparent magnitude | magnitude 11.45 |
| Absolute magnitude | magnitude 6.95 |
| Spectral type | K7V |
| Surface temperature | 4,680 K |
| Luminosity | 0.244 L☉ |
| Radius | 0.756 R☉ |
| Mass | 0.74 M☉ |
| Right ascension (J2000) | 9h 44m 15.0s |
| Declination (J2000) | −89° 28′ 18″ |
| Space velocity (relative to the Sun) | 29.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.45. Visible from the whole Southern Hemisphere and north to latitude 1° N. South of latitude 1° S it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1767. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.6 million years.
The Sun seen from there
From a planet around TOI-1105, the Sun would look like a star of magnitude 9.33, in the direction where our sky has the constellation Ursa Minor. It would be invisible to the naked eye.
Planets
- TOI-1105 b 10.9-day orbit · 3.06 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 78866 5.53 light-years
- χ Oct 12.8 light-years
- HIP 50605 14.4 light-years
- HIP 13844 16.1 light-years
- HIP 73883 18.7 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.