Star · G3V
HATS-51
HATS-51 is a main-sequence star of spectral type G3V in the constellation Canis Major, 1,271 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Canis Major |
|---|---|
| Distance | 1,271 light-years (389.6 pc) |
| Apparent magnitude | magnitude 12.53 |
| Absolute magnitude | magnitude 4.58 |
| Spectral type | G3V |
| Surface temperature | 5,760 K |
| Luminosity | 2.04 L☉ |
| Radius | 1.44 R☉ |
| Mass | 1.19 M☉ |
| Age | 4.7 billion years |
| Right ascension (J2000) | 6h 51m 23.4s |
| Declination (J2000) | −29° 03′ 31″ |
| Space velocity (relative to the Sun) | 33.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.53. Visible from the whole Southern Hemisphere and north to latitude 61° N. South of latitude 61° S 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 755. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 23 million years.
The Sun seen from there
From a planet around HATS-51, the Sun would look like a star of magnitude 12.78, in the direction where our sky has the constellation Lyra. It would be invisible to the naked eye.
Planets
- HATS-51 b 3.35-day orbit · 15.8 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.