Star · G4V
Kepler-1877
Kepler-1877 is a main-sequence star of spectral type G4V in the constellation Cygnus, 930.6 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 930.6 light-years (285.3 pc) |
| Apparent magnitude | magnitude 12.29 |
| Absolute magnitude | magnitude 5.01 |
| Spectral type | G4V |
| Surface temperature | 5,620 K |
| Luminosity | 0.837 L☉ |
| Radius | 0.936 R☉ |
| Mass | 1.02 M☉ |
| Age | 4.9 billion years |
| Metallicity [Fe/H] | 0.24 |
| Right ascension (J2000) | 19h 39m 28.1s |
| Declination (J2000) | +46° 47′ 26″ |
| Space velocity (relative to the Sun) | 21.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.29. Visible from the whole Northern Hemisphere and south to latitude 43° S. North of latitude 43° 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 the year 1095. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 17 million years.
The Sun seen from there
From a planet around Kepler-1877, the Sun would look like a star of magnitude 12.11, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-1877 b 2.38-day orbit · 0.624 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.