Star · K9I
TYC 4282-00605-1
TYC 4282-00605-1 is a supergiant star of spectral type K9I in the constellation Cepheus, 1,547 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).
| Constellation | Cepheus |
|---|---|
| Distance | 1,547 light-years (474.3 pc) |
| Apparent magnitude | magnitude 10.61 |
| Absolute magnitude | magnitude 2.23 |
| Spectral type | K9I |
| Surface temperature | 4,300 K |
| Luminosity | 81.3 L☉ |
| Radius | 16.2 R☉ |
| Mass | 0.97 M☉ |
| Age | 10.1 billion years |
| Metallicity [Fe/H] | -0.07 |
| Right ascension (J2000) | 22h 55m 29.3s |
| Declination (J2000) | +62° 14′ 21″ |
| Space velocity (relative to the Sun) | 80.8 km/s |
In the sky
A telescope is needed to see it: its apparent magnitude is 10.61. Visible from the whole Northern Hemisphere and south to latitude 28° S. North of latitude 28° N it never sets. It stands highest at midnight in September, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 479. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 27 million years.
The Sun seen from there
From a planet around TYC 4282-00605-1, the Sun would look like a star of magnitude 13.21, in the direction where our sky has the constellation Carina. It would be invisible to the naked eye.
Planets
- TYC 4282-00605-1 b 102-day orbit · 12.4 R⊕
Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.
