Astrophysics: Lenses and Telescopes Flashcards

1
Q

Do mirrors have a principle axis

A

Yes

Perpendicular to its surface and passes through its centre

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2
Q

What do lenses do

A

Change the direction of light rays

By refraction since light travels slower in glass than in air

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3
Q

Converging lenses

A

Convex
Thicker across the middle than the edges
So refract light rays towards each other

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4
Q

Principle axis

A

Horizontal axis through the centre of a lens

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5
Q

Lens axis

A

Vertical axis though the middle of a lens

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6
Q

What are axial rays

A

Rays parallel to the principle axis of a lens

Converge at the principle focus

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7
Q

What are non-axial rays

A

Rays that aren’t parallel to the principle axis

Converge somewhere along the focal plane but not the principle focus

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8
Q

Focal plane

A

The plane perpendicular to the principle axis that contains the principle focus

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9
Q

Focal length

A

Perpendicular distance between the lens axis and the focal plane
f

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10
Q

What do ray diagrams show

A

How light rays passing through a lens travels and where and what type of image is formed when they converge

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11
Q

How do you draw a ray diagram

A

One ray parallel to the principle axis straight through the top of the lens
That gets refracted through the principle focus

Another ray passing straight though the centre of the lens
That doesn’t get refracted at all

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12
Q

What 7 things can a ray diagram tell you

A

Real or virtual
Magnified or diminished or same size
Inverted or not

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13
Q

If an object hasn’t been magnified or diminished where will it be

A

The same distance from the lens axis as the object is from the lens axis

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14
Q

If an object has been magnified then where will it be

A

Image is further from the lens axis than the object is from the lens axis

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15
Q

If an object has been diminished then where will it be

A

Image is closer to the lens axis than the object is to the lens axis

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16
Q

What is a real image

A

Formed when light rays from one object are made to pass through another point in space
The light rays are actually there
Can be captured on a screen

17
Q

What is a virtual image

A

Formed when light rays from a point on an object seem to have come from another point in space
Light rays aren’t where the image appears to be
So can’t be captured on a screen
Image is located at infinity

18
Q

What does how big an object appears depend on

A

The angle which it subtends at the eye

19
Q

Equation for how powerful a telescope is

A

Angle subtended by image at eye / angle subtended by object at unaided eye

20
Q

Equation for angular magnification

A

Angle subtended by image at eye / angle subtended by object at unaided eye

21
Q

How do reflecting telescopes work

A

Use a mirror to collect light and form an image

22
Q

How do refracting telescopes work

A

Use two converging lenses

23
Q

Function of objective lens in astronomy/normal adjustment

A

The object/planet is effectively at infinity

A large lens known as the objective lens forms a real, inverted and diminished image at its focal point

24
Q

Two lenses in astronomy

A

Objective lens

Eye piece lens

25
Q

Function of eye piece lens in astronomy/normal adjustment

A

Produce a final image of the first image at infinity
Has principle focus coinciding with the focal point of the objective lens
Final image is inverted

26
Q

Assumption for ray diagrams

A

The bottom of the object lies on the principle axis

27
Q

Angular magnification equation in normal adjustment

A

angle at objective/angle at eye piece

28
Q

Expression for the length of a telescope in normal adjustment diagrams

A

fo+fe

Essentially the length from the centre of objective to centre of eye piece

29
Q

Equation linking angular magnification to fo and fe

A

a/b=fo/fe

Obtained using trigonometry and the small angle approximation

30
Q

Disadvantages of refracting telescopes

DDDMM

A

Using glass of sufficient clarity and purity free from defects to make a large diameter telescope is extremely difficult

Large diameter lenses are heavy and tend to distort under their own weight

Suffer from distorting factors (chromatic and spherical aberration)

Heavy and difficult to manoeuvre quickly

Large magnifications require large objective lenses and long focal lengths

31
Q

Advantages of reflecting telescopes

A

Large single mirrors can be made which are light and easily supportable from behind

Mirror surfaces can be made a few nanometres thick so give excellent image properties

No chromatic or spherical aberration when using parabolic mirrors

Relatively light mirrors allow rapid responses to astronomical events

32
Q

Two types of aberration

A

Chromatic

Spherical

33
Q

Explain chromatic aberration

A

Different wavelengths of light are refracted by different amounts
Issue with lens telescopes since they use refraction
Effect is more pronounced at the edges

34
Q

Which wavelengths of light are refracted most in chromatic aberration

A

Blue since shorter wavelength

35
Q

Explain spherical aberration

A

Blurry images

Refraction increases at lens edges