Barnard's Star planets have masses 0.19-0.84 M_earth, are tidally locked, unlikely to retain primary atmospheres, and possess mantles rich in ferropericlase with less than half Earth's water capacity and radiogenic heating.
Introducing the ECCOPLANETS code
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
A convex hull algorithm on composition-Gibbs energy points, supplemented by simplex classification, computes phase diagrams including solidus, liquidus, tie lines, and eutectic points for systems up to four components.
citing papers explorer
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The Barnard's Star Planetary System: Stability, Composition, and Evolution of Four Sub-Earth Exoplanets
Barnard's Star planets have masses 0.19-0.84 M_earth, are tidally locked, unlikely to retain primary atmospheres, and possess mantles rich in ferropericlase with less than half Earth's water capacity and radiogenic heating.
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Computing phase diagrams using a convex hull algorithm
A convex hull algorithm on composition-Gibbs energy points, supplemented by simplex classification, computes phase diagrams including solidus, liquidus, tie lines, and eutectic points for systems up to four components.