Star · K8V
K2-326
K2-326 is a main-sequence star of spectral type K8V in the constellation Pisces, 920.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pisces |
|---|---|
| Distance | 920.8 light-years (282.3 pc) |
| Apparent magnitude | magnitude 15.98 |
| Absolute magnitude | magnitude 8.73 |
| Spectral type | K8V |
| Surface temperature | 3,920 K |
| Luminosity | 0.105 L☉ |
| Radius | 0.688 R☉ |
| Mass | 0.507 M☉ |
| Right ascension (J2000) | 23h 26m 26.9s |
| Declination (J2000) | +1° 20′ 15″ |
| Space velocity (relative to the Sun) | 30.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.98. Visible from the whole Northern Hemisphere and south to latitude 89° S. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1105. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 16 million years.
The Sun seen from there
From a planet around K2-326, the Sun would look like a star of magnitude 12.08, in the direction where our sky has the constellation Leo. It would be invisible to the naked eye.
Planets
- K2-326 b 1.26-day orbit · 2.28 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.