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A star of 15 solar masses exhausts its hydrogen in about one-thousandth the lifetime of our sun.
For stars of less than 4 solar masses, hydrogen burn-up at the center triggers expansion to the red giant phase.
This site demonstrates two-dimensional collisions. Two balls of different masses can be shot at each other and the resulting collision and direction of the balls is shown
The Atwood machine consists of two masses (M1 and M1) connected via a rope running over a pulley. This site considers the frictionless case.
A simulation of two masses (may be altered) falling under the influence of gravity while attached to different sized parachutes.
Neutron degeneracy is a stellar application of the Pauli Exclusion Principle, as is electron degeneracy. No two neutrons can occupy identical states, even under the pressure of a collapsing star of ...
A short description of this topic,
Information on mechanical units and conversions.
Explanation of conservation of isopin in groups of particles with nearly the same mass.
Feature article explain all the different activities of the sun from the solar wind to coronal mass ejections
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