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pmb_phy said:The principle of conservation of momentum applies to total momentum of a closed system.
Pete
I disagree. The principle of conservation of momentum, Newton's First Law, applies to a body, not to a closed system of bodies:
or in English,Newton said:Lex I: Corpus omne perseverare in statu suo quiescendi vel movendi uniformiter in directum, nisi quatenus a viribus impressis cogitur statum illum mutare.
Classical Dynamics said:A body remains at rest or in uniform motion unless acted upon by a force.
A closed system has no external forces acting upon it. The all-important qualifier unless acted upon by a force is tautologically zero for a closed system.
The First Law doesn't say much -- to paraphrase it, "A body remains in uniform motion except when it doesn't". The First Law is a generalization of Galileo's Principle to all directions of travel. It introduces the concept of a force but does not define what that is. The Second Law defines forces, and the First Law can be derived from the Second. So why did Newton even write his First Law? The reason is that First Law threw out Aristotle's physics, thereby creating the need for a new physics.
I have not yet said that conservation of momentum does not apply on the Earth, period. I said that it does not apply in the case of a book falling because it has an external force acting upon it.
Zapper previously asked
ZapperZ said:If what you're saying is correct, then we, on earth, cannot apply the conservation of momentum, just because our "reference frame" is inappropriate for it! Would you like to stand by this claim?
To infinite precision, conservation of momentum does not apply to an Earth-fixed (or even Earth-centered) reference frame. Newton's Laws (including the first) are valid only to an observer in an inertial reference frame. The Earth rotates about its axis, creating the need for fictitious forces such as the Coriolus force. The Earth accelerates toward the Sun and Moon (and the center of the galaxy and ...), creating the need for fictitious forces such as third-body accelerations.