Star · G3V
TIC 320419023
TIC 320419023 is a main-sequence star of spectral type G3V in the constellation Canis Minor, 942.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Canis Minor |
|---|---|
| Distance | 942.3 light-years (288.9 pc) |
| Apparent magnitude | magnitude 12.16 |
| Absolute magnitude | magnitude 4.86 |
| Spectral type | G3V |
| Surface temperature | 5,700 K |
| Luminosity | 0.956 L☉ |
| Radius | 0.952 R☉ |
| Mass | 1.06 M☉ |
| Right ascension (J2000) | 7h 52m 17.4s |
| Declination (J2000) | +11° 49′ 27″ |
| Space velocity (relative to the Sun) | 40.6 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.16. Visible from the whole Northern Hemisphere and south to latitude 78° S. North of latitude 78° N it never sets. It stands highest at midnight in January, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1084. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 17 million years.
The Sun seen from there
From a planet around TIC 320419023, the Sun would look like a star of magnitude 12.13, in the direction where our sky has the constellation Sagittarius. It would be invisible to the naked eye.
Planets
- TIC 320419023 b 5.26-day orbit · 2.77 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.