Star · G4V
TOI-2714
TOI-2714 is a main-sequence star of spectral type G4V in the constellation Eridanus, 1,950 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Eridanus |
|---|---|
| Distance | 1,950 light-years (597.9 pc) |
| Apparent magnitude | magnitude 13.47 |
| Absolute magnitude | magnitude 4.59 |
| Spectral type | G4V |
| Surface temperature | 5,670 K |
| Luminosity | 1.45 L☉ |
| Radius | 1.25 R☉ |
| Mass | 1.07 M☉ |
| Age | 5.5 billion years |
| Metallicity [Fe/H] | 0.30 |
| Right ascension (J2000) | 4h 05m 36.3s |
| Declination (J2000) | −14° 55′ 36″ |
| Space velocity (relative to the Sun) | 35.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 13.47. Visible from the whole Southern Hemisphere and north to latitude 75° N. South of latitude 75° S it never sets. It stands highest at midnight in November, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 76. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 35 million years.
The Sun seen from there
From a planet around TOI-2714, the Sun would look like a star of magnitude 13.71, in the direction where our sky has the constellation Serpens. It would be invisible to the naked eye.
Planets
- TOI-2714 b 2.5-day orbit · 13.7 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.