Star · G8V
TOI-2193 A
TOI-2193 A is a main-sequence star of spectral type G8V in the constellation Pavo, 1,113 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Pavo |
|---|---|
| Distance | 1,113 light-years (341.4 pc) |
| Apparent magnitude | magnitude 12.06 |
| Absolute magnitude | magnitude 4.39 |
| Spectral type | G8V |
| Surface temperature | 5,970 K |
| Luminosity | 1.78 L☉ |
| Radius | 1.25 R☉ |
| Mass | 1.08 M☉ |
| Age | 5.5 billion years |
| Metallicity [Fe/H] | 0.03 |
| Right ascension (J2000) | 20h 54m 45.9s |
| Declination (J2000) | −72° 48′ 17″ |
| Space velocity (relative to the Sun) | 19.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.06. Visible from the whole Southern Hemisphere and north to latitude 17° N. South of latitude 17° 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 913. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 20 million years.
The Sun seen from there
From a planet around TOI-2193 A, the Sun would look like a star of magnitude 12.50, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.
Planets
- TOI-2193 A b 2.12-day orbit · 19.8 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.