Star · G1V
Kepler-1348
Kepler-1348 is a main-sequence star of spectral type G1V in the constellation Cygnus, 3,959 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 3,959 light-years (1,214 pc) |
| Apparent magnitude | magnitude 14.87 |
| Absolute magnitude | magnitude 4.45 |
| Spectral type | G1V |
| Surface temperature | 5,910 K |
| Luminosity | 1.6 L☉ |
| Radius | 1.04 R☉ |
| Mass | 1.04 M☉ |
| Age | 3.7 billion years |
| Metallicity [Fe/H] | -0.01 |
| Right ascension (J2000) | 19h 28m 21.0s |
| Declination (J2000) | +49° 47′ 19″ |
| Space velocity (relative to the Sun) | 47.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.87. Visible from the whole Northern Hemisphere and south to latitude 40° S. North of latitude 40° 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 1934 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 70 million years.
The Sun seen from there
From a planet around Kepler-1348, the Sun would look like a star of magnitude 15.25, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.
Planets
- Kepler-1348 b 27.6-day orbit · 1.94 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.