HD 222872: An Uneven Double in Sculptor

Illustration of double star system.

For those of us in the Northern Hemisphere, autumn is a great time to wander through the southern reaches of the sky and appreciate the stars of Sculptor. One of its most familiar treasures is the Silver Coin Galaxy, HD 3605, and HD 3074. Joining these notable doubles is HD 222872, first recorded by John Herschel in 1836.

The primary shines at magnitude 6.28. Classified as an F7V star, it’s just a bit cooler than our Sun. Its companion is dimmer, with a magnitude of 9.41. Even though the two stars lie 8.1 arcseconds apart, Stelle Doppie reports that it’s uncertain if these two stars are physically related.

This pair lies about 224 light-years away.

My Observations

DateNovember 13, 2025
Time8:00 p.m.
LocationTampa, FL
Magnification169x
ScopeMeade 8″ SCT
Eyepiece12mm
SeeingAverage
TransparencyAverage
Sketch of HD 222872 double star, showing the brighter primary star with a dim secondary nearby.
Sketch of HD 222872 on a November night

While I expected the brighter primary to show a yellow hue, it appeared distinctly white through the scope tonight. The dimmer secondary lies far enough away that the split is reasonably easy to resolve. A few additional stars share the field of view, but based on my research, they do not appear to be physically related to the pair.

For observers interested in comparing separations between double stars, it may be good to study this system and then switch to HD 3074, which features two stars separated by roughly half the distance, about 4 arcseconds apart.

Key Stats

ConstellationSculptor
Best ViewingAutumn
Visual Magnitude+6.28 | +9.41
Separation8.1″
Position Angle318.4°
Distance224.36 light-years
Milky Way LocationOrion Spur
My Viewing GradeB-
DesignationsSAO 192116, HJ 5417, HIP 117107, HR 8999, GC 32962, HD 222872

Sources and Notes

Stelle Doppie. (n.d.). Double star database: HD 222872. https://www.stelledoppie.it/index2.php?iddoppia=105122

Sketch by Wayne McGraw

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