Star · F9V
Kepler-757
Kepler-757 is a main-sequence star of spectral type F9V in the constellation Cygnus, 3,486 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 3,486 light-years (1,069 pc) |
| Apparent magnitude | magnitude 15.07 |
| Absolute magnitude | magnitude 4.93 |
| Spectral type | F9V |
| Surface temperature | 6,010 K |
| Luminosity | 1.45 L☉ |
| Radius | 1.13 R☉ |
| Mass | 1.08 M☉ |
| Age | 3.3 billion years |
| Metallicity [Fe/H] | 0.02 |
| Right ascension (J2000) | 19h 46m 43.3s |
| Declination (J2000) | +41° 23′ 11″ |
| Space velocity (relative to the Sun) | 22.2 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 15.07. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° 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 around 1461 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 62 million years.
The Sun seen from there
From a planet around Kepler-757, the Sun would look like a star of magnitude 14.97, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-757 b 1.02-day orbit · 1.36 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.