Struve 572: A Tight White Binary Star in Taurus

Struve 572 is a nice binary star in the constellation Taurus, the Bull. Taurus is most prominent during winter evenings in the Northern Hemisphere. The next time you’re out under winter skies, be sure to visit this tight pair first observed by astronomer Friedrich Georg Wilhelm Struve in 1822.

This binary star features two white-yellow stars close in magnitude. The primary star with a magnitude of +7.2 is slightly brighter than its companion star with a magnitude of +7.4. Both stars have the same white-yellow stellar classification of F2V. Modest backyard scopes should be able to split the two stars, which are only separated by 4.5 arcseconds. The two stars are physically related so they orbit a common center of mass as illustrated on the stelledoppie site and lie 203 light years away from Earth.

My Observations

DateNovember 23, 2023
Time10:20 p.m.
LocationSeattle, WA
Magnification169x
ScopeMeade 8″ SCT
Eyepiece12mm
SeeingAbove Average
TransparencyAbove Average
Sketch of Struve 572 shows a binary star in the winter constellation Taurus. The tight double star features two star close in brightness and color. The drawing illustrates how the pair appear through an 8-inch SCT telescope with a 12mm eyepiece under light-polluted skies Also know as STF 572, SAO 76682, HR 1470, HD 29364.
Sketch of the tight binary pair called Struve 572 on a November evening in 2023.

I love this type of binary star featuring two close stars of similar brightness. The stars are like a pair of eyes staring back at me. While some observers see a yellow tint in these stars, they both appear white to me. My 12mm eyepiece, through the 8-inch SCT scope, is enough power to separate the pair nicely.

Key Stats

ConstellationTaurus
Best ViewingWinter
Visual Magnitude+7.2 | +7.4
Separation4.5″
Position Angle188°
Spectral ClassF2V & F2V
Milky Way LocationOrion Spur
My Viewing GradeB
DesignationsSTF 572, SAO 76682, HR 1470, HD 29364

Sources and Notes

Banner adapted from an illustration created by Pablo Budassi. The illustration is licensed under the Creative Commons Attribution-Share Alike 4.0 International license. Full details here.

04385+2656 STF 572 AB (NSV1676). WDS 04385+2656 STF 572 AB (NSV1676). (n.d.). https://www.stelledoppie.it/index2.php?iddoppia=16156

Sketch by Wayne McGraw

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