N-body simulations demonstrate long-term dynamical stability of the HD 20794 system across a range of inclinations, with planet d identified as the lowest-mass high-eccentricity HZ-crossing planet.
Lunine, Acta Astronautica131, 123 (2017)
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Laser Ionisation Mass Spectrometry can detect organic molecules, microstructures, and sulphur isotope fractionation as signatures of life for future Solar System missions, with machine learning aiding unbiased analysis.
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Dynamical Stability and Habitability in the HD 20794 System
N-body simulations demonstrate long-term dynamical stability of the HD 20794 system across a range of inclinations, with planet d identified as the lowest-mass high-eccentricity HZ-crossing planet.
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Laser-based mass spectrometry for the detection of signatures of life within our Solar System
Laser Ionisation Mass Spectrometry can detect organic molecules, microstructures, and sulphur isotope fractionation as signatures of life for future Solar System missions, with machine learning aiding unbiased analysis.