Star · G8 V
Copernicus
Copernicus is a main-sequence star of spectral type G8 V in the constellation Cancer, 41.1 light-years from the Sun. It is orbited by 5 confirmed exoplanet(s).
| Other names | ρ¹ Cnc · 55 Cnc · Gl 324A · HIP 43587 |
|---|---|
| Constellation | Cancer |
| Distance | 41.1 light-years (12.6 pc) |
| Apparent magnitude | magnitude 5.96 |
| Absolute magnitude | magnitude 5.46 |
| Spectral type | G8 V |
| Surface temperature | 5,200 K |
| Luminosity | 0.635 L☉ |
| Radius | 0.98 R☉ |
| Mass | 1.02 M☉ |
| Age | 10.0 billion years |
| Metallicity [Fe/H] | 0.39 |
| Right ascension (J2000) | 8h 52m 35.8s |
| Declination (J2000) | +28° 19′ 51″ |
| Space velocity (relative to the Sun) | 42.1 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 5.96). Visible from the whole Northern Hemisphere and south to latitude 62° S. North of latitude 62° N it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1985. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 728 thousand years.
The Sun seen from there
From a planet around Copernicus, the Sun would look like a star of magnitude 5.33, in the direction where our sky has the constellation Microscopium. It would be visible to the naked eye.
Planets
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- 55 Cnc B 0.11 light-years
- Gl 316.1 8.26 light-years
- 2MASSI J0825196+211552 8.52 light-years
- WISEA J083011.95+283716.0 8.71 light-years
- Gl 359 8.98 light-years
- Gl 356B 9.10 light-years
- 11 LMi 9.10 light-years
- Gl 353 9.13 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.
