Star · ?
Gl 169.1B
Gl 169.1B is a white dwarf of spectral type ? in the constellation Camelopardalis, 18.0 light-years from the Sun.
| Constellation | Camelopardalis |
|---|---|
| Distance | 18.0 light-years (5.52 pc) |
| Apparent magnitude | magnitude 12.44 |
| Absolute magnitude | magnitude 13.73 |
| Spectral type | ? |
| Surface temperature | 8,000 K |
| Luminosity | 2.90 × 10⁻⁴ L☉ |
| Radius | 0.012 R☉ |
| Mass | 0.6 M☉ (estimated) |
| Right ascension (J2000) | 4h 31m 11.4s |
| Declination (J2000) | +58° 58′ 56″ |
| Space velocity (relative to the Sun) | 61.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.44. Visible from the whole Northern Hemisphere and south to latitude 31° S. North of latitude 31° 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 2008. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 319 thousand years.
The Sun seen from there
From a planet around Gl 169.1B, the Sun would look like a star of magnitude 3.54, in the direction where our sky has the constellation Norma. It would be visible to the naked eye.
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.