Star · K9V
K2-72
K2-72 is a main-sequence star of spectral type K9V in the constellation Aquarius, 216.9 light-years from the Sun. It is orbited by 4 confirmed exoplanet(s).
| Constellation | Aquarius |
|---|---|
| Distance | 216.9 light-years (66.5 pc) |
| Apparent magnitude | magnitude 15.28 |
| Absolute magnitude | magnitude 11.17 |
| Spectral type | K9V |
| Surface temperature | 3,360 K |
| Luminosity | 0.0146 L☉ |
| Radius | 0.331 R☉ |
| Mass | 0.271 M☉ |
| Right ascension (J2000) | 22h 18m 29.5s |
| Declination (J2000) | −9° 36′ 43″ |
| Space velocity (relative to the Sun) | 66.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.28. Visible from the whole Southern Hemisphere and north to latitude 80° N. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1809. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.8 million years.
The Sun seen from there
From a planet around K2-72, the Sun would look like a star of magnitude 8.94, in the direction where our sky has the constellation Leo. It would be invisible to the naked eye.
Planets
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.