Star · G0
TOI-1135
TOI-1135 is a main-sequence star of spectral type G0 in the constellation Camelopardalis, 372.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Other names | HIP 62908 |
|---|---|
| Constellation | Camelopardalis |
| Distance | 372.4 light-years (114.2 pc) |
| Apparent magnitude | magnitude 9.54 |
| Absolute magnitude | magnitude 4.25 |
| Spectral type | G0 |
| Surface temperature | 6,320 K |
| Luminosity | 2.08 L☉ |
| Radius | 1.2 R☉ |
| Mass | 1.12 M☉ |
| Age | 3.3 billion years |
| Metallicity [Fe/H] | -0.04 |
| Right ascension (J2000) | 12h 53m 35.0s |
| Declination (J2000) | +85° 07′ 46″ |
| Space velocity (relative to the Sun) | 23.0 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.54. Visible from the whole Northern Hemisphere and south to latitude 5° S. North of latitude 5° N it never sets.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1654. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 6.6 million years.
The Sun seen from there
From a planet around TOI-1135, the Sun would look like a star of magnitude 10.12, in the direction where our sky has the constellation Octans. It would be invisible to the naked eye.
Planets
- TOI-1135 b 8.03-day orbit · 9.92 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.