Star · ?
GJ 1082
GJ 1082 is a white dwarf of spectral type ? in the constellation Auriga, 104.9 light-years from the Sun.
| Constellation | Auriga |
|---|---|
| Distance | 104.9 light-years (32.1 pc) |
| Apparent magnitude | magnitude 14.75 |
| Absolute magnitude | magnitude 12.21 |
| Spectral type | ? |
| Surface temperature | 8,000 K |
| Luminosity | 0.00118 L☉ |
| Radius | 0.012 R☉ |
| Mass | 0.6 M☉ (estimated) |
| Right ascension (J2000) | 5h 36m 20.0s |
| Declination (J2000) | +41° 30′ 12″ |
| Space velocity (relative to the Sun) | 21.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.75. Visible from the whole Northern Hemisphere and south to latitude 48° S. North of latitude 48° N it never sets. It stands highest at midnight in December, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1921. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.
The Sun seen from there
From a planet around GJ 1082, the Sun would look like a star of magnitude 7.37, in the direction where our sky has the constellation Scorpius. It would be invisible 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.