Exploring the Cosmos - Degree Exam 2009 - Particles, Forces & the Big Bang
1. In the Geocentric view of the Universe, what are the stars?
Perfect celestial objects.
Objects reflecting the light of the Sun.
Symbols of the gods.
Far away bright objects.
2. We now reject the Geocentric view of the Universe. What is the main objection?
It does not provide any physical understanding.
The model is too contrived.
It does not fit the observed data.
It cannot explain the Retrograde motion.
3. Kepler’s laws state that the
Sun is at the centre of the Universe.
planets rotate about their own axis of rotation.
planets follow circular orbits.
speed of the planets changes over time.
4. The Observable Universe refers to the portion of the Universe
that is made up of ordinary matter.
from which light has had time to reach the Earth.
visible to an observer on the surface of the Earth.
able to be resolved by the most powerful telescope.
5. In a uniformly expanding Universe
the speed of travel of all the objects are uniform.
the further the object the faster they move away.
objects at the edge of the Universe will, in fact, expand less.
all the objects will move away from each other at uniform speed.
6. If the cosmological (density) parameter of the Universe is greater than 1, then we
still don’t know the shape because density and shape are independent parameters.
live in a closed universe.
live in a flat universe.
live in an open universe.
7. The String Theory postulates that the Universe
is made up of lots of tiny strings.
progresses from one event to the next as if moving along a stretched string.
is just one manifestation of many, like the notes on a vibrating string.
started with the Big Bang.
8. In the Big Bang theory as we approach the beginning of time the temperature
becomes a meaningless concept.
decreases.
remains the same.
increases.
9. How can measurements of the rotation of galaxies detect the presence of dark matter?
The presence of dark matter will distort the rotation path of a galaxy.
As galaxies rotate, dark matter can periodically obscure parts of a galaxy.
Dark matter does not move. So, it slows down the rotation of galaxies.
The rate of rotation of a galaxy tells us what is its mass.
10. The smoothness problem in Big Bang cosmology refers to the problem of the
celestial bodies appearing to be less smooth as the theory predicts.
geometry of the Universe being almost flat.
older parts of the Universe appearing to be smooth.
Cosmic Microwave Background Radiation being not as smooth as expected.
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