Astronomers Discover 27 Potential Planets Orbiting Binary Stars Using Novel Timing Method

May 4, 2026
Astronomers Discover 27 Potential Planets Orbiting Binary Stars Using Novel Timing Method
  • Astronomers have identified 27 candidate circumbinary planets—worlds that orbit two stars—using a novel timing-based method, expanding the known sample of planets in binary-star systems.

  • The candidate planets, ranging from Neptune-like to up to about ten Jupiter masses, are located between roughly 650 and 18,000 light-years away and would occupy a broad span of sizes.

  • The team analyzed data from 1,590 binary systems observed by NASA's TESS, employing eclipse timing variations and apsidal precession to infer planetary-mass objects without direct transits.

  • Future ground-based spectroscopic observations will be needed to measure stellar velocities and confirm the gravitational influence of the planets.

  • The findings were published in the May issue of Monthly Notices of the Royal Astronomical Society, with lead author Margo Thornton and co-author Benjamin Montet highlighting implications for planet formation in binary environments.

  • Coinciding with Star Wars Day, the study echoes popular fiction by suggesting two-star planetary systems, and suggests refinements to timing-based techniques could reveal more such worlds.

  • Circumbinary planets face extreme environments, but there may be a stable region in the dual-star system where such planets could reside, making Tatooine-like worlds plausible.

  • The work builds on context about the rarity of circumbinary planets in prior surveys and links to previous research suggesting binary dynamics can hinder planet formation.

  • NASA researchers emphasize TESS's ongoing value beyond exoplanets, inviting public participation in citizen science projects like Planet Hunters TESS to analyze light curves for new candidates.

  • While these are strong planet candidates, additional spectroscopic analysis is required to determine exact masses and confirm whether they are planets, brown dwarfs, or low-mass stars.

  • Further analysis of light curves and supplementary observations are needed to rule out false positives and verify planetary status.

  • Spectroscopy will be essential to distinguish planets from brown dwarfs or small stars and to nail down the true nature of the candidates.

Summary based on 5 sources


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