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Physics 110: Homework #9 Solutions
- 9.1
- Orbital velocities: 250 km/s, 275 km/s, 300 km/s, 300 km/s.
Masses:
,
,
,
. or
,
,
,
.
- 9.2
- The rapid revolution of the stars near the center of the
Andromeda Galaxy shows that 10 to 100 million solar masses of material
lie within the central 1 or 2 parsecs of the galaxy.
- 9.3
- We do not know the intrinsic brightness or luminosity of
astronomical objects, so we cannot use their apparent brightness to
determine distances. Likewise we do not know the intrinsic sizes of
astronomical objects, so we cannot use their angular sizes to
determine distances. Much astronomical research is directed toward
finding classes of objects (e.g., supernovae, planetary nebulae,
bright galaxies, and so on) that can be considered to have the
same intrinsic brightness or intrinsic size so that they can be used
as distance indicators. Evolution of intrinsic properties could have
a significant impact on a tertiary distance indicator. For example,
if a class of long-lived astronomical objects tended to grow dimmer as the
objects aged, then such objects observed nearby would be intrinsically
fainter than such objects viewed at great distances from us. This is
because far away objects are being viewed when they're much younger
than nearby objects.
- 9.4
- Hubble's Law says that the apparent recessional speed of a
galaxy (based on its measured redshift) is proportional to its
distance from us. So by measuring a galaxy's redshift, we can
determine its distance if we know the constant of proportionality,
which is Hubble's constant. Hubble's Law is explained in the
following way: The expansion of the Universe carries all galaxies away
from one another. The apparent speed of recession increases with the
distance between two galaxies. All observers in the Universe see the
Universe expanding.
- 9.5
- We know quasars are distant by determining their redshifts
from emission lines and using Hubble's Law. Quasars are compact in
size because the changes in their brightness as a function of time are
fairly rapid, of order a day or so. This suggests that they can't be
much larger than a size that corresponds to the distance that light
travels in a day, which is about 170 AU. The orbit of Pluto (the
outermost planet) is about 40 AU, so the size of a quasar is roughly
the size of the solar system.
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John Hughes
Tue Apr 13 16:51:56 EDT 1999