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Reading:

Rolnick section 4.1 (review)
Carroll and Ostlie, Modern Astrophysics section 16.1, attached.
Problems:

  1. If the inertial mass $m_i$ were not the same as the gravitational mass $m_g$, what would be the period $T$ of a simple pendulum of length $l$ at a distance $r$ from the center of a spherical mass $M_g$?

  2. Consider a horizontally travelling photon on the surface of a 1.4 solar mass neutron star, with radius 10 km.
    1. What is the gravitational acceleration $g$ on the surface of the neutron star?
    2. Neglecting time dilation effects between the freefalling observer $O$ and observer $O'$ on the neutron star surface, through what angle does $O'$ see a light ray bend over a path of horizontal length $l$? What angle does this give for $l= 1$ m? $l= 100 $ m?
    3. At what speed does $O'$ travel relative to $O$ when the photon reaches horizontal length $l$, if initially at rest with respect to $O$?
    4. From (b) and (c), what can you say about the relevance of general and special relativistic effects for a neutron star?

  3. A satellite moves in a circular orbit about the earth. Inside the satellite, two objects are simultaneously released from rest relative to the satellite, one object being $\Delta r$ above the other. After one revolution, the objects will no longer lie on the same vertical. What is their relative horizontal displacement; that is, by what horizontal distance does the higher object lag, when the lower one completes its first orbit? (This indicates a ``tidal'' effect even for particles in circular orbit, and indicates that even in this special case a finite laboratory frame cannot be a local inertial frame.)

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2004-02-19