Iota Horologii
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Dust disk around Iota Horologii
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Also known as HR 810, a Sun-like star with an extrasolar planet 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 miles) |
| Orbital period |
320 days |
| Eccentricity |
0.16 |
| Discovery |
1999, ESO Coudé Échelle Spectrometer, La Silla |
| Method of discovery |
radial velocity |
Related categories
NOTABLE STARS
EXTRASOLAR PLANETS AND SUBSTELLAR OBJECTS
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