Star · K0V
TOI-2211
TOI-2211 is a main-sequence star of spectral type K0V in the constellation Microscopium, 229.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | HIP 101503 |
|---|---|
| Constellation | Microscopium |
| Distance | 229.8 light-years (70.5 pc) |
| Apparent magnitude | magnitude 10.00 |
| Absolute magnitude | magnitude 5.76 |
| Spectral type | K0V |
| Surface temperature | 5,250 K |
| Luminosity | 0.478 L☉ |
| Radius | 0.834 R☉ |
| Mass | 0.9 M☉ |
| Right ascension (J2000) | 20h 34m 09.3s |
| Declination (J2000) | −29° 40′ 20″ |
| Space velocity (relative to the Sun) | 66.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 10.00. Visible from the whole Southern Hemisphere and north to latitude 60° N. South of latitude 60° 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 1796. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.1 million years.
The Sun seen from there
From a planet around TOI-2211, the Sun would look like a star of magnitude 9.07, in the direction where our sky has the constellation Cancer. It would be invisible to the naked eye.
Planets
- TOI-2211.01 3.09-day orbit · 1.56 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 101469 11.9 light-years
- HIP 100224 15.7 light-years
- HIP 102200 16.5 light-years
- HIP 100474 17.8 light-years
- HIP 100893 18.5 light-years
- HIP 99739 19.3 light-years
- HIP 102014 19.6 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.