Star · K9 V/M0 V
TOI-1075
TOI-1075 is a main-sequence star of spectral type K9 V/M0 V in the constellation Pavo, 200.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pavo |
|---|---|
| Distance | 200.3 light-years (61.4 pc) |
| Apparent magnitude | magnitude 12.68 |
| Absolute magnitude | magnitude 8.74 |
| Spectral type | K9 V/M0 V |
| Surface temperature | 3,880 K |
| Luminosity | 0.0717 L☉ |
| Radius | 0.581 R☉ |
| Mass | 0.604 M☉ |
| Age | 6.0 billion years |
| Metallicity [Fe/H] | -0.08 |
| Right ascension (J2000) | 20h 39m 53.1s |
| Declination (J2000) | −65° 26′ 59″ |
| Space velocity (relative to the Sun) | 46.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.68. Visible from the whole Southern Hemisphere and north to latitude 25° N. South of latitude 25° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1826. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.6 million years.
The Sun seen from there
From a planet around TOI-1075, the Sun would look like a star of magnitude 8.77, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.
Planets
- TOI-1075 b 0.605-day orbit · 1.79 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 101102 8.54 light-years
- HIP 101684 10.6 light-years
- HIP 101031 11.3 light-years
- ρ Pav 14.1 light-years
- HIP 103031 18.4 light-years
- HIP 97674 18.5 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.