Astronomers have developed a new approach to studying planet formation by focusing on "twin" binary star systems, where two stars born at the same time and place orbit each other. This fresh perspective, detailed in a Yale study, suggests that certain binary systems could offer unique insights into how planetary systems form, much like comparing human twins in biological research.
Malena R by Clarence Oxford
Los Angeles CA (SPX) May 15, 2025
Astronomers have developed a new approach to studying planet formation by focusing on "twin" binary star systems, where two stars born at the same time and place orbit each other. This fresh perspective, detailed in a Yale study, suggests that certain binary systems could offer unique insights into how planetary systems form, much like comparing human twins in biological research.
Malena Rice, an assistant professor of astronomy at Yale, and her colleagues have shown that specific "edge-on" configurations of binary star systems may be particularly valuable for planet detection. In these systems, the stars' orbits are perfectly aligned, allowing their gravitational interactions to stabilize the orbits of their planets, potentially reducing the risk of extreme climate variations that could hinder life. This alignment also produces a detectable wobble as the stars move directly toward and away from Earth, boosting observational signals for astronomers.
The research team, including Joseph Hand, a University of Kansas undergraduate and Dorrit Hoffleit Undergraduate Research Scholar, and Yale Ph.D. candidate Konstantin Gerbig, identified nearly 600 edge-on binary systems using data from the European Space Agency's Gaia DR3 stellar catalog. They then simulated the planets likely to orbit these stars, effectively creating a guide for where future astronomers might find new exoplanets.
"This could be an unprecedented avenue for examining how deterministic, or orderly, the process of planet formation is," said Rice. The study's findings provide a roadmap for comparing planets across twin star systems, offering the first true "control sample" for such studies.
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