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Spectroscopically resolved binary stars (RSBs) are stellar pairs we can separate and study in fine detail. They are precious because they allow us to measure their distance dynamically, without assumptions, just like a cosmic ruler. But a recent study in *Galaxies* uncovered a trick: for distant binaries (beyond 500 parsecs, about 1,600 light-years), trigonometric parallax measurements from the Gaia and Hipparcos satellites **overestimate** the true distance by 10 to 50%.

Why does this happen? These systems appear as single stars in official catalogs. Their double nature escapes standard analysis but leaves a trace: comparing data from different Gaia "releases" (data publications), the parallaxes shift suspiciously. It is as if the star "wobbles" slightly, betraying the presence of an invisible companion altering its apparent position.

This discrepancy is crucial: if reference distances are wrong, our 3D map of the Milky Way risks being distorted. Understanding these "systematic errors" helps astronomers correct their aim, making Gaia even more precise for future discoveries. The lesson? Even the most advanced telescopes can be fooled by a game of stellar perspective.

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The study, published in *Galaxies* (Vol. 13, p. 96), analyzes the most comprehensive sample to date of spectroscopically resolved binaries (RSBs). RSBs are unique: by combining the visual orbit (resolved via interferometry or high-resolution imaging) with the spectroscopic orbit (radial velocities), one obtains the "orbital parallax", a purely geometric and dynamical distance, free from the photometric or kinematic assumptions plaguing other methods.

Results show a systematic discrepancy for systems with distance > 0.5 kpc: trigonometric parallaxes (Gaia DR2/DR3, Hipparcos) are systematically *smaller* (larger distance) than orbital ones. The overestimation ranges from 10% to 50%. The author hypothesizes that the orbital motion of the photocenter (the center of light of the unresolved system) introduces unmodeled astrometric "noise" into Gaia's standard 5-parameter solution (position, parallax, proper motion). Since the orbital period is often comparable to the mission duration (or not an integer multiple), the photocenter motion is partially absorbed into the parallax estimate, biasing it.

Comparing different Data Releases (e.g., DR2 vs DR3 vs Hipparcos) reveals that trigonometric parallaxes of these "single" objects vary beyond formal uncertainties, acting as a diagnostic for hidden binarity. This has profound implications for calibrating the galactic distance scale and mapping spiral structure, as many standard candles (Cepheids, red giants) might be unresolved binaries with systematically erroneous parallaxes.

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Authors:
Oleg Y. MalkovArseniy M. Sachkov
Date Published:
Original Article www.mdpi.com
Fact-check verified on 05/08/2026
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Creative Commons License CC BY-NC-SA 4.0

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