Star · K7V
TOI-1410
TOI-1410 is a main-sequence star of spectral type K7V in the constellation Lacerta, 236.7 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Lacerta |
|---|---|
| Distance | 236.7 light-years (72.6 pc) |
| Apparent magnitude | magnitude 11.24 |
| Absolute magnitude | magnitude 6.94 |
| Spectral type | K7V |
| Surface temperature | 4,640 K |
| Luminosity | 0.239 L☉ |
| Radius | 0.756 R☉ |
| Mass | 0.794 M☉ |
| Age | 6.6 billion years |
| Metallicity [Fe/H] | 0.33 |
| Right ascension (J2000) | 22h 19m 32.0s |
| Declination (J2000) | +42° 33′ 37″ |
| Space velocity (relative to the Sun) | 23.7 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.24. Visible from the whole Northern Hemisphere and south to latitude 47° S. North of latitude 47° 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 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-1410, the Sun would look like a star of magnitude 9.13, in the direction where our sky has the constellation Vela. It would be invisible to the naked eye.
Planets
- TOI-1410.01 1.22-day orbit · 3.1 R⊕
- TOI-1410 c 47.6-day orbit · 5.63 R⊕
Neighbours
Its nearest neighbours in the catalogue (within 20 light-years):
- HIP 110071 2.38 light-years
- HIP 109881 19.0 light-years
- HIP 110170 19.9 light-years
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.