University of Cincinnati Studies, Τόμος 10,Μέρος 1University of Cincinnati., 1915 |
Συχνά εμφανιζόμενοι όροι και φράσεις
A₁ angular velocity areal velocity axes axis of rotation C₂ center of mass centrifugal force changing the oblateness coefficients of restitution common axis component of force condition configuration of particles considered corresponding decrease develop direct central impact discussion earth's ellipsoid energy of rotation equation 37 equipotential surfaces eruption occurs eruptive force fluid forces acting outward forces of constraint given gravitational energy gravitational force Hence increase indicated inner shell k-body kinetic energy kinetic potential LIGHT CURVE light variation loss of kinetic m₁ mass rotation matter observed opposite directions outer shell particles ejected particles of shell phenomena plane positive problem quantity radial velocities radiant energy represented resistance to eruptive respectively S₁ shell A5 solar spherical spheroid spiral nebula star's summation surface through particle tangential components ticles tion UNIVERSITY OF CINCINNATI V₁ variable stars variation of light vector representation wave motion
Δημοφιλή αποσπάσματα
Σελίδα 5 - Poincaré, and Darwin on the figures of equilibrium of rotating homogeneous fluids, and on their stabilities. In particular, considering a series of homogeneous fluid masses of the same density but of different rates of rotation it is shown that there is a continuous series of figures of stable equilibrium beginning with the sphere for zero rate of rotation; then, with increasing rotation, passing along a line of oblate spheroids until a certain rate of rotation is reached; then, with decreasing...