Star · G2V
TIC 183374187
TIC 183374187 is a main-sequence star of spectral type G2V in the constellation Phoenix, 3,942 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Phoenix |
|---|---|
| Distance | 3,942 light-years (1,209 pc) |
| Apparent magnitude | magnitude 14.64 |
| Absolute magnitude | magnitude 4.23 |
| Spectral type | G2V |
| Surface temperature | 5,770 K |
| Luminosity | 1.74 L☉ |
| Radius | 1.34 R☉ |
| Mass | 0.853 M☉ |
| Age | 12.3 billion years |
| Metallicity [Fe/H] | -0.39 |
| Right ascension (J2000) | 23h 50m 27.8s |
| Declination (J2000) | −41° 24′ 45″ |
| Space velocity (relative to the Sun) | 125.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 14.64. Visible from the whole Southern Hemisphere and north to latitude 49° N. South of latitude 49° 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 1917 BC. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 70 million years.
The Sun seen from there
From a planet around TIC 183374187, the Sun would look like a star of magnitude 15.24, in the direction where our sky has the constellation Ursa Major. It would be invisible to the naked eye.
Planets
- TIC 183374187 b 5.06-day orbit · 14 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.