Star · G8V
HATS-14
HATS-14 is a main-sequence star of spectral type G8V in the constellation Capricornus, 1,673 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Capricornus |
|---|---|
| Distance | 1,673 light-years (513.0 pc) |
| Apparent magnitude | magnitude 14.05 |
| Absolute magnitude | magnitude 5.50 |
| Spectral type | G8V |
| Surface temperature | 5,350 K |
| Luminosity | 0.672 L☉ |
| Radius | 0.933 R☉ |
| Mass | 0.967 M☉ |
| Age | 4.9 billion years |
| Metallicity [Fe/H] | 0.33 |
| Right ascension (J2000) | 20h 52m 51.7s |
| Declination (J2000) | −25° 41′ 15″ |
| Space velocity (relative to the Sun) | 24.2 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.05. Visible from the whole Southern Hemisphere and north to latitude 64° N. South of latitude 64° S it never sets. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 353. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 30 million years.
The Sun seen from there
From a planet around HATS-14, the Sun would look like a star of magnitude 13.38, in the direction where our sky has the constellation Cancer. It would be invisible to the naked eye.
Planets
- HATS-14 b 2.77-day orbit · 11.6 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.