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Contact: James Devitt
james.devitt@nyu.edu
212-998-6808
New York University

HD 52265 and its Orbiting Jupiter-Like Planet

Caption: A team of researchers has devised a way to measure the internal properties of stars -- a method that offers more accurate assessments of their orbiting planets. The researchers examined HD 52265 and a single planet in the star's orbit. This is an artistic rendering of HD 52265 and its orbiting Jupiter-like planet.

Credit: Image courtesy of MPI for Solar System Research/Mark A. Garlick.

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Related news release: Pulsating star sheds light on exoplanet


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