This preview shows page 1. Sign up to view the full content.
(d) This part refers specifically to the very large black hole treated in the previous part.
With that mass for
M
in Eq. 13–16, and
r
= 2.002
GM
/
c
2
, we obtain
()
(
)
6
33
2
2
2
=2
=
2.002
2.002
/
g
GM
c
da
dr
dr
GM
GM c
−−
where
dr
→
1.70 m as in Sample Problem 133. This yields (in absolute value) an
acceleration difference of 7.30
×
10
−
15
m/s
2
.
(e) The miniscule result of the previous part implies that, in this case, any effects due to
the differences of gravitational forces on the body are negligible.
This is the end of the preview. Sign up
to
access the rest of the document.
This note was uploaded on 05/17/2011 for the course PHY 2049 taught by Professor Any during the Spring '08 term at University of Florida.
 Spring '08
 Any
 Physics

Click to edit the document details