Star · K6-K7
TOI-1130
TOI-1130 is a main-sequence star of spectral type K6-K7 in the constellation Corona Australis, 190.5 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).
| Constellation | Corona Australis |
|---|---|
| Distance | 190.5 light-years (58.4 pc) |
| Apparent magnitude | magnitude 11.69 |
| Absolute magnitude | magnitude 7.86 |
| Spectral type | K6-K7 |
| Surface temperature | 4,360 K |
| Luminosity | 0.14 L☉ |
| Radius | 0.697 R☉ |
| Mass | 0.745 M☉ |
| Age | 5.4 billion years |
| Metallicity [Fe/H] | 0.11 |
| Right ascension (J2000) | 19h 05m 30.2s |
| Declination (J2000) | −41° 26′ 15″ |
| Space velocity (relative to the Sun) | 11.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 11.69. Visible from the whole Southern Hemisphere and north to latitude 49° N. South of latitude 49° S it never sets. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1835. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.4 million years.
The Sun seen from there
From a planet around TOI-1130, the Sun would look like a star of magnitude 8.66, in the direction where our sky has the constellation Auriga. It would be invisible to the naked eye.
Planets
- TOI-1130 b 4.07-day orbit · 3.66 R⊕
- TOI-1130 c 8.35-day orbit · 13 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.