Star · G7
TOI-6041
TOI-6041 is a main-sequence star of spectral type G7 in the constellation Perseus, 237.0 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Perseus |
|---|---|
| Distance | 237.0 light-years (72.7 pc) |
| Apparent magnitude | magnitude 9.93 |
| Absolute magnitude | magnitude 5.62 |
| Spectral type | G7 |
| Surface temperature | 5,450 K |
| Luminosity | 0.613 L☉ |
| Radius | 0.879 R☉ |
| Mass | 0.885 M☉ |
| Age | 7.9 billion years |
| Metallicity [Fe/H] | 0.10 |
| Right ascension (J2000) | 3h 04m 14.5s |
| Declination (J2000) | +43° 33′ 29″ |
| Space velocity (relative to the Sun) | 34.3 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 9.93. Visible from the whole Northern Hemisphere and south to latitude 46° S. North of latitude 46° N 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 1789. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.2 million years.
The Sun seen from there
From a planet around TOI-6041, the Sun would look like a star of magnitude 9.14, in the direction where our sky has the constellation Lupus. It would be invisible to the naked eye.
Planets
- TOI-6041 b 26-day orbit · 4.55 R⊕
- TOI-6041 c 88-day orbit · 10.5 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 14776 9.50 light-years
- HIP 13230 13.5 light-years
- HIP 15688 14.2 light-years
- HIP 15118 14.4 light-years
- HIP 15934 18.2 light-years
- HIP 15998 18.7 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.