Sensitivity of rocky planet structures to the equation of state
arxiv.org · 4,447 words · saved by 1 readers
N/A
Sensitivity of rocky planet structures to the equation of state Damian C. Swift PLS-CMMD, Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550, USA (Dated: June 10, 2009 – LLNL-TR-414058) arXiv:0908.3294v1 [astro-ph.EP] 23…
related reading
- Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrumarxiv.org
- [2501.14054] Probing the Limits of Habitability: A Catalog of Rocky Exoplanets in the Habitable Zonearxiv.org
- Circular Restricted Three-Body Problem — Orbital Mechanics & Astrodynamicsorbital-mechanics.space
- Bartosz Ciechanowskiciechanow.ski
- Dyson Spheresarxiv.org
- EquationOfState.pdfbayes.wustl.edu
- Increasing Access and Capabilities of CubeSats for Investigation of Earth Trojan Asteroidsdigital.lib.washington.edu
- Type Ia supernova explosion models are inherently multidimensionalarxiv.org
- Good Vibrations.tifcs.toronto.edu
- arXiv:gr-qc/0202090v1 26 Feb 2002arxiv.org
- [2607.28013] The physical origin of the maximum stellar sizearxiv.org
- 0903.4186arxiv.org