Chronology | Current Month | Current Thread | Current Date |
[Year List] [Month List (current year)] | [Date Index] [Thread Index] | [Thread Prev] [Thread Next] | [Date Prev] [Date Next] |
----- Original Message -----undaunted
From: John Mallinckrodt <ajmallinckro@CSUPOMONA.EDU>
I've proposed exercises that I thought might reveal some conceptual
difficulties previously in this thread. Nobody took me up on them, so
maybe I shouldn't bother trying to do it again. Nevertheless,
of...
Consider two identical, spherically symmetric, nonrotating planets of
radius R and mass M orbiting their common center of mass in a circle
nearradius 2R (and don't worry about Roche limits and all that!)
a) What is the Newtonian "force of gravity" on an object of mass m
missing?the surface of one planet when the other is directly overhead.
8/9(GMm/R^2) from GMm/R^2 - GMn/(3R)^2
b) What would a properly functioning scale read if it were used to
weigh the object?
8/9(GMm/R^2)
c) If the object were allowed to fall, what would be its acceleration
relative to the nearby planet?
8/9(GM/R^2) (approximately over a short range near the surface)
John Mallinckrodt mailto:ajm@csupomona.edu
Cal Poly Pomona http://www.csupomona.edu/~ajm
I would say all in agreement with W = m x (Grav Field). What am I
The second planet certainly affects the net gravitational force, thefield,
and hence the weight and acceleration.
Rick