Question 1
Question
What type of lens is used for observing the night sky?
Answer
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Converging
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Diverging
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Concatonating
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Diffracting
Question 2
Question
What happens to light when it passes from air into a lens?
Question 3
Question
A convex lens is a type of converging lens
Question 4
Question
What are components of a ray diagram?
Answer
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Principal Axis
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The Singularity
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The Focal Length
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The Principal Focus
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The Headline
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The Lens Cap
Question 5
Question
True or False - This ray diagram shows an object between F and 2F
Question 6
Question
True or False - This image shows a ray diagram of an object at 2F
Question 7
Question
What are the 3 properties of an image on a ray diagram?
Answer
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Magnification
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Direction
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Orientation
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Nature
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Shape
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Curvature
Question 8
Question
True or False - The image shows The Lens Formula
Question 9
Question
True or False - Converging lenses must have positive focal lengths, and diverging lenses must have negative focal lengths for the formula to work.
Question 10
Question
True or False - For the formula to work, distances to real images should be negative and those to virtual images should be positive
Question 11
Question
True or False - this diagram shows an Astronomical Telescope in normal adjustment
Question 12
Question
The formula for Angular Magnificatio = fe/f0
Question 13
Question
Select features which define a reflecting telescope
Answer
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They use a spherical mirror
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They can suffer from spherical aberration
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They feature a principal axis
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They use the idea of angle of incidence = angle of refraction
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A parabolic mirror is used
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They suffer from chromatic aberration
Question 14
Question
What are the differences and similarities between reflecting telescopes and Cassegrain Telescopes?
Answer
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They both use elliptical mirrors
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They both suffer from spherical aberration
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A reflecting telescope has only one mirror, while a cassegrain telescope has two - a primary mirror and a secondary mirror
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Both mirrors have holes in them
Question 15
Question
A Cassegrain reflector uses a secondary mirror to direct light rays reflected by the primary mirror through a hole in the primary mirror towards the observer
Question 16
Question
The Hipparcos satellite used the parallax method to measure the distance to more than 100,000 stars with a precision of 0.002 arc seconds. Calculate, in metres, the maximum distance measurable by Hipparcos.
Answer
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2x10^21m
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2 × 10^19 m
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3.6x10^12m
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4.5x10^19m
Question 17
Question
Wien’s displacement law for black body radiation is given by λmaxT = constant.
Is λmax wavelength at which maximum emission occurs
Question 18
Question
Given the suns output power is 4.0x10^26. Find the average temperature of the sun
Question 19
Question
A: absolute magnitude: 1.40 apparent magnitude: –1.4 diameter / 10^3 km: 2400 temperature/K: 10 000
B: absolute magnitude: 11.2 apparent magnitude: 8.4 diameter / 10^3 km: 12 temperature/K 25 000
Calculate the distance to Star B in Pc
Question 20
Question
Which star will be the hottest and why?
Answer
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R - has largest wavelength
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P - has highest intensity
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Q - ratio of intensity to wavelength closest to 1
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P - has lowest wavelength
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R - Has lowest intensity
Question 21
Question
In which two spectral classes are the presence of Hydrogen Balmer absorption lines prominent features?
Question 22
Question
Describe how Hydrogen absorption lines are produced in the spectrum of a star:
Light from the star passes through the [blank_start]atmosphere[blank_end] of the star which contains [blank_start]hydrogen[blank_end] with electrons in [blank_start]n = 2[blank_end] state electrons in this state absorb certain energies and hence [blank_start]frequencies[blank_end] of light the light is re-emitted in all [blank_start]directions[blank_end], so that the [blank_start]intensity[blank_end] of these frequencies is [blank_start]reduced[blank_end] in any given direction, resulting in [blank_start]absorption lines[blank_end].
Answer
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atmosphere
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hydrogen
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n = 2
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frequencies
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directions
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intensity
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reduced
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absorption lines
Question 23
Question
Explain what is meant by light year and parsec.
Answer
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light year : distance travelled by light in one year
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light year : distance travelled by light in one AU
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Parsec : 10 AU
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parsec : distance to an object subtending 1 sec of arc to Earth’s orbit