Study Findings: Four Sub-Earth Planets Orbiting Barnard’s Star from MAROON-X and ESPRESSO

Posted on by onespaceman2000
Image (Credit): Conceptual art showing Barnard’s Star from the surface of one of its four orbiting planets. (Illustration by International Gemini Observatory/NOIRLab/NSF/AURA/R. Proctor/J. Pollard)

The Astrophysical Journal Letters abstract of the study findings:

Barnard’s Star is an old, single M dwarf star that comprises the second-closest extrasolar system. It has a long history of claimed planet detections from both radial velocities and astrometry. However, none of these claimed detections have so far withstood further scrutiny. Continuing this story, extreme precision radial velocity measurements from the ESPRESSO instrument have recently been used to identify four new sub-Earth-mass planet candidates around Barnard’s Star. We present here 112 radial velocities of Barnard’s Star from the MAROON-X instrument that were obtained independently to search for planets around this compelling object.

Citation: Ritvik Basant et al. Four sub-Earth planets orbiting Barnard’s Star from MAROON-X and ESPRESSO. ApJL 982 L1 (2025).
https://doi.org/10.3847/2041-8213/adb8d5

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