HD 33564 [SEP] constellation
HD 33564
HD 33564 is a 5th magnitude star located approximately 68 light-years away in the constellation of Camelopardalis. It is an F-type main sequence, indicating that the star is hotter and more massive than our Sun. The age of the star is only 3 Ga; despite of this, the star is only 76% the solar abundance of iron. HD 33564 is a naked eye planetary host star.
Planetary system.
In September 2005, a massive planet was found orbiting the star surrounded by
as their F9 V standard. Eta Cassiopeiae A should probably be avoided as a standard star because it was often considered F9 V in Keenan's publications, but G0 V in Morgan's publications.
Planets.
Some of the nearest F-type stars known to have planets include Upsilon Andromedae, Tau Boötis, HD 10647, HD 33564, HD 142, HD 60532 and KOI-3010.
Habitability.
Some studies show that there is a possibility that life could also develop on planets that orbit a F-type star