Star · F8V
Kepler-355
Kepler-355 is a main-sequence star of spectral type F8V in the constellation Lyra, 4,671 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Lyra |
|---|---|
| Distance | 4,671 light-years (1,432 pc) |
| Apparent magnitude | magnitude 15.24 |
| Absolute magnitude | magnitude 4.46 |
| Spectral type | F8V |
| Surface temperature | 6,180 K |
| Luminosity | 1.57 L☉ |
| Radius | 1.07 R☉ |
| Mass | 0.933 M☉ |
| Age | 10.0 billion years |
| Metallicity [Fe/H] | -0.06 |
| Right ascension (J2000) | 19h 03m 11.9s |
| Declination (J2000) | +42° 48′ 42″ |
| Space velocity (relative to the Sun) | 66.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.24. Visible from the whole Northern Hemisphere and south to latitude 47° S. North of latitude 47° N it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out 4,671 years ago. At that time the first farming villages were being founded; there was no writing yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 83 million years.
The Sun seen from there
From a planet around Kepler-355, the Sun would look like a star of magnitude 15.61, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-355 b 11-day orbit · 1.46 R⊕
- Kepler-355 c 25.8-day orbit · 2.71 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.