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XZ Andromedae: The Eclipsing Binary Star System That Appears to Wink

XZ Andromedae is an Algol-type eclipsing binary whose brightness drops when its cooler star passes in front of its hotter companion. Light-curve studies also hint that more stars may orbit the system.
September 27, 2026   Neela Asman   Beginner-friendly astronomy update
XZ Andromedae: The Eclipsing Binary Star System That Appears to Wink

Some stars seem to blink, but the effect can come from orbital geometry rather than a star switching on and off. XZ Andromedae is a pair of stars orbiting in a plane that is almost edge-on from Earth.

As the cooler member crosses in front of the hotter and brighter star, the combined light from the system falls. Astronomers record that change as a light curve and use it to study the stars and their orbit.

Why this matters: Eclipsing binaries let astronomers measure stellar properties with unusual precision. The same light-curve techniques are also used to study transiting exoplanets and other objects whose brightness changes with time.
Object typeAlgol-type eclipsing binary
MethodDifferential photometry
Extra companionsPossibly two
ConstellationAndromeda

Why XZ Andromedae appears to wink

The system contains two stars whose orbit is aligned so that one periodically passes in front of the other from our viewpoint. During the eclipse, the total amount of light reaching Earth decreases.

What an Algol-type eclipsing binary is

Algol-type systems contain stars that remain roughly spherical while producing distinct eclipses. Their light curves usually show a deeper primary eclipse and a shallower secondary eclipse.

What an Algol-type eclipsing binary is
Real astronomy image relevant to this section.

How astronomers build a light curve

Differential photometry compares the brightness of the target star with nearby comparison stars. This reduces many changes caused by Earth’s atmosphere or the observing instrument.

Why extra companion stars are suspected

Analyses of multiple XZ Andromedae light curves suggest that the timing of the eclipses may be influenced by additional bodies, with NASA’s APOD noting that two more stars may orbit the system.

Why extra companion stars are suspected
Real astronomy image relevant to this section.

Why variable-star observations still matter

Repeated brightness measurements can reveal orbital changes, hidden companions and stellar evolution. Even modest telescopes can contribute useful data when observations are carefully calibrated.

Simple takeaway: XZ Andromedae does not truly blink. Its changing brightness is created by stars eclipsing one another, turning a simple-looking point of light into a measurable stellar laboratory.

FAQ

Is XZ Andromedae one star?

No. The central system is an eclipsing binary containing two stars.

Why does it get dimmer?

The cooler star periodically passes in front of the hotter, brighter star from Earth’s perspective.

Could there be more than two stars?

NASA’s APOD notes that analyses of several light curves indicate two additional stars may orbit the system.

Can amateur astronomers study eclipsing binaries?

Yes. Differential photometry can be performed with suitable imaging equipment and careful calibration.

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