Exploring the Cosmos - Degree Exam 2008 - Particles, Forces & the Big Bang
1. Hubble expansion refers to the discovery in the 1920s and 1930s by Edwin Hubble that
the universe is expanding.
far away galaxies are older.
the speed at which galaxies are moving is a function of their distance from us.
stars are moving away from us wherever he looked.
2. The age of the universe
can be determined from observation of the stars in the heavens.
is the same as that of the Sun.
can be estimated from the age of the Milky Way.
is unknown and unknowable.
3. The horizon of the observable universe refers to the
edge of the universe which one can observe at any one time.
horizon of the sky.
newest bits of the universe only just become possible to be observed.
furthest part of the universe our telescope is able to resolve.
4. Which of the following Galileo did not observe through his telescope?
Venus has phases.
The moon is not made of perfect celestial material.
Other planets can have moons.
Sun spots.
5. In Ptolemy's model of the universe, the stars
are features on the surface of a perfect sphere.
are just like the sun.
have epicycles
orbit around the sun.
6. Kepler's laws show that
forces acting on the planets must balance with the forces acting on the star.
planets are held by the gravitational force of the star around which they orbit.
the Earth is not the centre of the universe.
planetary orbits are elliptical.
7. The fundamental particles are
neutrinos and gluons.
waves not particles.
fermions and bosons.
quarks and electrons.
8. Which of the following is ranked in descending order of temperature?
Planck era, Era of atoms, Particle era.
Particle era, Planck era, Era of atoms.
Planck era, Particle era, Era of atoms.
Particle era, Era of atoms, Planck era.
9. Dark matter
is dark and absorbs all light incident upon it.
is made up of black holes.
can not be seen.
can potentially be detected on earth.
10. The "flatness problem" in cosmology refers to the fact that
because the universe is flat, we will never see parts of the universe.
the universe is very close to the critical density.
if we squash the universe flat, it will be no denser than the density of paper.
three space dimensions are "flattened" to two in the space-time diagram.
Submit Quiz