3.9.1 Telescopes Flashcards

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1
Q

What is a lens?

A

A piece of equipment which forms an image by refracting light

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2
Q

What are the 2 types of lenses?

A

Convex - converging lens
Concave - diverging lens

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3
Q

What is the focal point?

A

The point on a converging lens where lays of light meet

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4
Q

What is the focal length?

A

The distance between the centre of the lens to the focal point

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5
Q

What does the focal length depend on?

A

How curved/thick the lens is - more curved = shorter focal length.
The shorter the focal length the more powerful the lens is.

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6
Q

What is the difference between real and virtual images?

A

Real - light converges, image is inverted, can be projected into a screen, image formed in front of the lens.
Virtual - Light diverges from the focal point, image is upright, can be projected on a screen, image formed behind the lens.

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7
Q

What are the 3 rays needed to construct a ray diagram?

A

Ray passing through the principle axis and the lens (diagonal)
Ray that is parallel to principal axis and passes through principle focus
Ray that passes through the principle focus and emerges parallel to principle axis

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8
Q

What type of image is formed by a converging lens at varying distances?

A

d>2f:
image between f and 2f, real, inverted, diminished
d=2f:
image at 2f, real, inverted, same size
f<d<2f:
image beyond 2f, real, inverted, magnified
d<f:
image at 2f, virtual, upright, magnified

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9
Q

What is the lens equation?

A

1/f = 1/u + 1/v
- if the image is virtual, the value of v is negative

v = distance of image from lens
u = distance of object from lens

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10
Q

What is the formula for magmification?

A

M=h_1/h_0 = v/u = angle subtended by eye β/ angle subtended by image α

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11
Q

What is normal adjustment for a refractor?

A

The adjustment which enables the final image to be at infinity
conditions:
both lenses must be arranged so their focal points meet in the same place
Focal length of the objective lens must be longer than the focal length of the eyepiece lens

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12
Q

What is the formula for angular magnification?

A

θ= h/d

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13
Q

What is the derivation for the formula of magnification in terms of angles?

A

tan α = h/f_o, using small angle,
α = h/f_o
hence tan β = h/f_e => β=h/f_e

M= β/α = h/f_e / h/f_o ……rearrange….
M=f_o/f_e

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14
Q

What is required to achieve greater magnification for refractors?

A

Objective focal length needs to be longer and eyepiece focal length needs to be shorter (for refractors).
They need to be very long
l = f_o+f_e

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15
Q

What are the properties of mirrors used by the Cassegrain telescope?

A

2 mirrors used:
primary mirror: large and concave
secondary mirror: small and convex

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16
Q

What are the features of the ray diagram for a Cassegrain telescope?

A

Rays enter telescope parallel to principal axis
Curvature of mirrors does not need to be the same
Rays do not cross before the secondary mirror

17
Q

What is the Rayleigh Criterion?

A

States that two sources will be resolved if the central maximum of one diffraction pattern overlaps with the first minimum of the other

18
Q

How can resolving power of a telescope be increased?

A

Increase diameter of aperture
Operate at a shorter wavelength of light

19
Q

What is the formula for the Rayleigh Criterion?

A

θ =s/D
s = separation between 2 objects
D = horizontal distance to eye

20
Q

What is the formula for minimum angular resolution?

A

θ ≈ λ/D
θ >λ/D - sources are resolvable
θ = λ/D - sources are just resolvable
θ <λ/D - sources are not resolvable

21
Q

What is the collecting power of a telescope?

A

A measure of the amount of light energy it collects per second.

It is proportional to diameter^2

22
Q

What is the advantage of having a higher collecting power?

A

Images are brighter and clearer

23
Q

What is the definition of quantum efficiency?

A

The percentage of incident photons which cause an electron to be released in CCDs

24
Q

What is the formula for quantum efficiency?

A

QE = no electrons produced per sec/ no photons absorbed per sec
*100

25
Q

Why are CCDs better than the human eye?

A

Higher quantum efficiency, can observe a broader range of wavelengths, images can be stored and analysed digitally, better resolution