Iota Horologii

Dust disk around Iota Horologii.
Iota Horologii, also known as HR 810, is a Sun-like star with an exoplanet that moves in the most Earth-like orbit yet found. Iota Horologii has a surface temperature of 6150 K and a mass 1.25 times that of the Sun. It is believed to be about 625 million years old and is more metal-rich than the Sun by about 50%. It has drifted to its present position from the Hyades cluster where it formed.
| Host star | |
|---|---|
| distance | 50.5 light-years (15.5 pc) |
| spectral type | G0 V |
| apparent magnitude | 5.4 |
| Planet | |
|---|---|
| mass (Jupiter=1) | 2.26 |
| semi-major axis | 0.93 AU (140 million km, 86 million mi) |
| orbital period | 320 days |
| eccentricity | 0.16 |
| discovery | 1999, ESO Coudé Échelle Spectrometer, La Silla |
| method of discovery | radial velocity |


