Magnitude 8.05 Apparent magnitude (V) 8.05 | ||
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HD 109271 is an old yellow main-sequence dwarf star.
Planetary system
From 2003 to 2012, the star was under observance from HARPS.
In 2012, two eccentric hot Neptune-mass planets were deduced by radial velocity. They were published in January 2013. These are close to a 1:4 resonance. The system is like HD 69830.
A third Neptune in the Venus zone was hypothesised from the data.
References
HD 109271 Wikipedia(Text) CC BY-SA