Iota Piscium
Iota Piscium (ι Psc) is a star 45 light years away from Earth,[2] in the constellation Pisces. The star is a yellowish dwarf (main sequence) star of spectral type F7V, which is somewhat larger and brighter than our sun, but still within the range considered to have the potential for Earth-like planets. It has a surface temperature of about 6,000 to 7,500 kelvin. Iota Piscium is a suspected variable star, and was once thought to have one or two stellar companions, but both are line-of-sight coincidences.[3]has oppisote poles
References
- ^ "Simbad Query Result". Simbad. http://simbad.u-strasbg.fr/simbad/sim-id?protocol=html&Ident=HD+222368&NbIdent=1&Radius=10&Radius.unit=arcmin&submit=submit+id. Retrieved April 4, 2007.
- ^ a b c d e f van Leeuwen, F. (2007). "HIP 116771". Hipparcos, the New Reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=116381. Retrieved 2010-10-11.
- ^ ""Iota Piscium"". http://www.astro.uiuc.edu/~kaler/sow/iotapsc.html. Retrieved September 27, 2007.
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In left column are stellar classes of primary members of star systems. ‡Distance error margin extends out of declared distance interval. Italic are systems possibly located within declared distance interval, but probably not.
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