Star · K0
BD+49 828
BD+49 828 is a supergiant star of spectral type K0 in the constellation Perseus, 1,411 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Perseus |
|---|---|
| Distance | 1,411 light-years (432.6 pc) |
| Apparent magnitude | magnitude 9.51 |
| Absolute magnitude | magnitude 1.33 |
| Spectral type | K0 |
| Surface temperature | 4,940 K |
| Luminosity | 29.5 L☉ |
| Radius | 7.6 R☉ |
| Mass | 1.52 M☉ |
| Age | 2.3 billion years |
| Metallicity [Fe/H] | -0.19 |
| Right ascension (J2000) | 3h 02m 33.7s |
| Declination (J2000) | +49° 43′ 48″ |
| Space velocity (relative to the Sun) | 25.5 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.51. 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 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 615. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 25 million years.
The Sun seen from there
From a planet around BD+49 828, the Sun would look like a star of magnitude 13.01, in the direction where our sky has the constellation Lupus. It would be invisible to the naked eye.
Planets
- BD+49 828 b 2,590-day orbit · 13.5 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.