Star · F7V
TOI-6884
TOI-6884 is a main-sequence star of spectral type F7V in the constellation Coma Berenices, 1,834 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Coma Berenices |
|---|---|
| Distance | 1,834 light-years (562.4 pc) |
| Apparent magnitude | magnitude 11.99 |
| Absolute magnitude | magnitude 3.24 |
| Spectral type | F7V |
| Surface temperature | 6,330 K |
| Luminosity | 4.91 L☉ |
| Radius | 1.84 R☉ |
| Mass | 1.41 M☉ |
| Age | 2.6 billion years |
| Metallicity [Fe/H] | 0.09 |
| Right ascension (J2000) | 12h 52m 02.1s |
| Declination (J2000) | +26° 40′ 26″ |
| Space velocity (relative to the Sun) | 31.4 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.99. Visible from the whole Northern Hemisphere and south to latitude 63° S. North of latitude 63° N it never sets. It stands highest at midnight in April, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 192. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 33 million years.
The Sun seen from there
From a planet around TOI-6884, the Sun would look like a star of magnitude 13.58, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.
Planets
- TOI-6884 b 4.81-day orbit · 10.4 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.