Star · G
HATS-28
HATS-28 is a main-sequence star of spectral type G in the constellation Telescopium, 1,746 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Telescopium |
|---|---|
| Distance | 1,746 light-years (535.4 pc) |
| Apparent magnitude | magnitude 13.98 |
| Absolute magnitude | magnitude 5.34 |
| Spectral type | G |
| Surface temperature | 5,500 K |
| Luminosity | 0.696 L☉ |
| Radius | 0.922 R☉ |
| Mass | 0.929 M☉ |
| Age | 6.2 billion years |
| Metallicity [Fe/H] | 0.01 |
| Right ascension (J2000) | 18h 57m 35.9s |
| Declination (J2000) | −49° 08′ 19″ |
| Space velocity (relative to the Sun) | 31.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.98. Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 280. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 31 million years.
The Sun seen from there
From a planet around HATS-28, the Sun would look like a star of magnitude 13.47, in the direction where our sky has the constellation Lynx. It would be invisible to the naked eye.
Planets
- HATS-28 b 3.18-day orbit · 13.4 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.