Star · G5V
TOI-5882
TOI-5882 is a main-sequence star of spectral type G5V in the constellation Cygnus, 1,367 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cygnus |
|---|---|
| Distance | 1,367 light-years (419.1 pc) |
| Apparent magnitude | magnitude 11.39 |
| Absolute magnitude | magnitude 3.28 |
| Spectral type | G5V |
| Surface temperature | 5,920 K |
| Luminosity | 5.67 L☉ |
| Radius | 2.26 R☉ |
| Mass | 1.33 M☉ |
| Age | 4.1 billion years |
| Metallicity [Fe/H] | 0.18 |
| Right ascension (J2000) | 20h 47m 33.3s |
| Declination (J2000) | +34° 44′ 15″ |
| Space velocity (relative to the Sun) | 50.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.39. Visible from the whole Northern Hemisphere and south to latitude 55° S. North of latitude 55° N 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 659. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 24 million years.
The Sun seen from there
From a planet around TOI-5882, the Sun would look like a star of magnitude 12.94, in the direction where our sky has the constellation Pyxis. It would be invisible to the naked eye.
Planets
- TOI-5882 b 7.15-day orbit · 11.5 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.