Star · F9V
K2-177
K2-177 is a main-sequence star of spectral type F9V in the constellation Taurus, 1,605 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Taurus |
|---|---|
| Distance | 1,605 light-years (492.2 pc) |
| Apparent magnitude | magnitude 12.68 |
| Absolute magnitude | magnitude 4.22 |
| Spectral type | F9V |
| Surface temperature | 6,060 K |
| Luminosity | 2.2 L☉ |
| Radius | 1.21 R☉ |
| Mass | 1.21 M☉ |
| Metallicity [Fe/H] | 0.41 |
| Right ascension (J2000) | 3h 40m 55.1s |
| Declination (J2000) | +20° 44′ 10″ |
| Space velocity (relative to the Sun) | 26.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.68. Visible from the whole Northern Hemisphere and south to latitude 69° S. North of latitude 69° N it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 421. 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 K2-177, the Sun would look like a star of magnitude 13.29, in the direction where our sky has the constellation Libra. It would be invisible to the naked eye.
Planets
- K2-177 b 14.2-day orbit · 2.12 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.