Star · ?
TOI-6255
TOI-6255 is a main-sequence star of spectral type ? in the constellation Lacerta, 66.5 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | GJ 4256 |
|---|---|
| Constellation | Lacerta |
| Distance | 66.5 light-years (20.4 pc) |
| Apparent magnitude | magnitude 12.69 |
| Absolute magnitude | magnitude 11.14 |
| Spectral type | ? |
| Surface temperature | 3,420 K |
| Luminosity | 0.0168 L☉ |
| Radius | 0.37 R☉ |
| Mass | 0.353 M☉ |
| Metallicity [Fe/H] | -0.14 |
| Right ascension (J2000) | 22h 06m 00.5s |
| Declination (J2000) | +39° 17′ 55″ |
| Space velocity (relative to the Sun) | 44.9 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 12.69. Visible from the whole Northern Hemisphere and south to latitude 51° S. North of latitude 51° N it never sets. It stands highest at midnight in August, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1960. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.2 million years.
The Sun seen from there
From a planet around TOI-6255, the Sun would look like a star of magnitude 6.38, in the direction where our sky has the constellation Antlia. It would be visible to the naked eye.
Planets
- TOI-6255 b 0.238-day orbit · 1.08 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.