Star · K7V
HATS-76
HATS-76 is a main-sequence star of spectral type K7V in the constellation Caelum, 1,258 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Caelum |
|---|---|
| Distance | 1,258 light-years (385.7 pc) |
| Apparent magnitude | magnitude 16.68 |
| Absolute magnitude | magnitude 8.75 |
| Spectral type | K7V |
| Surface temperature | 4,020 K |
| Luminosity | 0.0916 L☉ |
| Radius | 0.626 R☉ |
| Mass | 0.662 M☉ |
| Age | 4.6 billion years |
| Metallicity [Fe/H] | 0.32 |
| Right ascension (J2000) | 4h 41m 21.5s |
| Declination (J2000) | −32° 19′ 14″ |
| Space velocity (relative to the Sun) | 71.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 16.68. Visible from the whole Southern Hemisphere and north to latitude 58° N. South of latitude 58° S 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 768. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 22 million years.
The Sun seen from there
From a planet around HATS-76, the Sun would look like a star of magnitude 12.76, in the direction where our sky has the constellation Hercules. It would be invisible to the naked eye.
Planets
- HATS-76 b 1.94-day orbit · 12.1 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.