The escape velocity of the Earth and that planet:
"v=\\sqrt{\\frac{2GM}{R}},\\\\\\space\\\\\nu=\\sqrt{\\frac{8GM}{R}}=2v." The escape velocity should be two times greater.
(C) Obtain the stress-strain relation.
"\\sigma=\\frac FA=\\frac{FL}{V}.\\\\\\space\\\\\n\\epsilon=\\frac{\\Delta L}{L}=\\frac{\\Delta LA}{V}.\\\\\\space\\\\\n\\sigma(\\epsilon)=\\frac{FL}{\\Delta LA}\\epsilon."
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