Star · G4V
K2-220
K2-220 is a main-sequence star of spectral type G4V in the constellation Pisces, 761.6 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pisces |
|---|---|
| Distance | 761.6 light-years (233.5 pc) |
| Apparent magnitude | magnitude 11.87 |
| Absolute magnitude | magnitude 5.03 |
| Spectral type | G4V |
| Surface temperature | 5,610 K |
| Luminosity | 0.869 L☉ |
| Radius | 1.03 R☉ |
| Mass | 0.91 M☉ |
| Metallicity [Fe/H] | -0.05 |
| Right ascension (J2000) | 0h 51m 04.8s |
| Declination (J2000) | +9° 31′ 00″ |
| Space velocity (relative to the Sun) | 34.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.87. Visible from the whole Northern Hemisphere and south to latitude 80° S. It stands highest at midnight in October, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1264. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 14 million years.
The Sun seen from there
From a planet around K2-220, the Sun would look like a star of magnitude 11.67, in the direction where our sky has the constellation Virgo. It would be invisible to the naked eye.
Planets
- K2-220 b 13.7-day orbit · 2.37 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.