Exploring the Cosmos - Degree Exam 2013 - Mapping the universe
1. A Schmidt-Cassegrain telescope is one that has?
A corrector plate, a primary mirror and a secondary mirror.
A corrector plate and a primary mirror only.
Only lenses.
Only mirrors.
2. Why are astronomers interested in measuring light at different parts of the electromagnetic spectrum?
Stars emit mainly ultraviolet radiation.
Because visible light is hard to detect on Earth.
Because in vacuum light travels at different speeds at different wavelengths.
Different parts of the spectrum provide different information.
3. What does the frequency of light mean?
The distance it will travel in 1 second.
The distance from one maximum to another.
How bright the light will be.
The number of times the wave cycle repeats every second.
4. The energy of a photon can be expressed by
E=hf.
E=cλ.
E=hc.
E=f/λ.
5. What is the purpose of the objective lens in a refracting telescope?
To diffract the incoming light.
To focus the incoming light.
To interfere the incoming light.
To change the speed of the incoming light.
6. If a refracting telescope has an objective lens with a focal length of 300cm and has an eyepiece with a focal length of 3cm, the magnification is?
M = 100.
M = 3/300.
M = 1/100.
M = 300.
7. Active optics is used in modern telescopes to
change the focal length of the primary mirror for different astronomical objects.
change the shape of the primary mirror to correct for atmospheric disturbances.
maximise the light gathering power of the telescope.
change the detector sensitivity for measuring different wavelengths.
8. The Earth’s atmosphere is responsible for which three phenomena in observational astronomy?
Wave particle duality, Atmospheric scattering, and Atmospheric absorption.
Atmospheric scattering, Spherical aberration, and Atmospheric refraction.
Atmospheric refraction, Atmospheric scattering, and Atmospheric absorption.
Atmospheric diffraction, Chromatic aberration, and Atmospheric scattering.
9. For what reason is interferometry used when using multiple telescopes to observe astronomical objects?
To increase the resolving power of the detector.
To measure different frequencies of light simultaneously.
To remove the effect of light pollution.
To reduce the magnification.
10. Gravitational wave detectors aim to measure the radiation emitted by accelerating masses by
detecting Cherenkov radiation with photomultiplier tubes.
using the James Webb Space Telescope.
using multiple radio telescopes around the world.
using long-baseline laser interferometers.
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