Star · G2V
K2-350
K2-350 is a main-sequence star of spectral type G2V in the constellation Virgo, 1,596 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Virgo |
|---|---|
| Distance | 1,596 light-years (489.4 pc) |
| Apparent magnitude | magnitude 13.45 |
| Absolute magnitude | magnitude 5.00 |
| Spectral type | G2V |
| Surface temperature | 5,790 K |
| Luminosity | 0.973 L☉ |
| Radius | 1.04 R☉ |
| Mass | 0.98 M☉ |
| Metallicity [Fe/H] | -0.02 |
| Right ascension (J2000) | 13h 36m 08.5s |
| Declination (J2000) | −14° 00′ 33″ |
| Space velocity (relative to the Sun) | 45.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.45. Visible from the whole Southern Hemisphere and north to latitude 76° N. South of latitude 76° S it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 430. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 28 million years.
The Sun seen from there
From a planet around K2-350, the Sun would look like a star of magnitude 13.28, in the direction where our sky has the constellation Pisces. It would be invisible to the naked eye.
Planets
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.