Star · K0V
HATS-43
HATS-43 is a main-sequence star of spectral type K0V in the constellation Columba, 1,182 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Columba |
|---|---|
| Distance | 1,182 light-years (362.3 pc) |
| Apparent magnitude | magnitude 13.56 |
| Absolute magnitude | magnitude 5.76 |
| Spectral type | K0V |
| Surface temperature | 5,100 K |
| Luminosity | 0.4 L☉ |
| Radius | 0.812 R☉ |
| Mass | 0.837 M☉ |
| Age | 8.6 billion years |
| Metallicity [Fe/H] | 0.05 |
| Right ascension (J2000) | 5h 22m 09.2s |
| Declination (J2000) | −30° 58′ 15″ |
| Space velocity (relative to the Sun) | 16.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.56. 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 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 844. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 21 million years.
The Sun seen from there
From a planet around HATS-43, the Sun would look like a star of magnitude 12.63, in the direction where our sky has the constellation Hercules. It would be invisible to the naked eye.
Planets
- HATS-43 b 4.39-day orbit · 13.2 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.