Star · F9V
HATS-52
HATS-52 is a main-sequence star of spectral type F9V in the constellation Pyxis, 1,811 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pyxis |
|---|---|
| Distance | 1,811 light-years (555.1 pc) |
| Apparent magnitude | magnitude 13.84 |
| Absolute magnitude | magnitude 5.12 |
| Spectral type | F9V |
| Surface temperature | 6,010 K |
| Luminosity | 1.17 L☉ |
| Radius | 1.05 R☉ |
| Mass | 1.11 M☉ |
| Age | 1.2 billion years |
| Metallicity [Fe/H] | -0.28 |
| Right ascension (J2000) | 9h 20m 21.0s |
| Declination (J2000) | −31° 16′ 09″ |
| Space velocity (relative to the Sun) | 76.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.84. Visible from the whole Southern Hemisphere and north to latitude 59° N. South of latitude 59° S it never sets. It stands highest at midnight in February, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 215. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 32 million years.
The Sun seen from there
From a planet around HATS-52, the Sun would look like a star of magnitude 13.55, in the direction where our sky has the constellation Cygnus. It would be invisible to the naked eye.
Planets
- HATS-52 b 1.37-day orbit · 15.5 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.