Star · G3V
HATS-32
HATS-32 is a main-sequence star of spectral type G3V in the constellation Aquarius, 2,430 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Aquarius |
|---|---|
| Distance | 2,430 light-years (745.1 pc) |
| Apparent magnitude | magnitude 14.39 |
| Absolute magnitude | magnitude 5.03 |
| Spectral type | G3V |
| Surface temperature | 5,700 K |
| Luminosity | 1.14 L☉ |
| Radius | 1.1 R☉ |
| Mass | 1.1 M☉ |
| Age | 3.5 billion years |
| Metallicity [Fe/H] | 0.39 |
| Right ascension (J2000) | 23h 04m 18.0s |
| Declination (J2000) | −21° 16′ 19″ |
| Space velocity (relative to the Sun) | 71.2 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.39. Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° S it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around 405 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 43 million years.
The Sun seen from there
From a planet around HATS-32, the Sun would look like a star of magnitude 14.19, in the direction where our sky has the constellation Leo. It would be invisible to the naked eye.
Planets
- HATS-32 b 2.81-day orbit · 14 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.