9.1 Telescopes Flashcards

1
Q

What is the lens equation?

A
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2
Q

What do the letters represent in this equation?

A
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3
Q

What is the equation for power of a lens?

A
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4
Q

What do the letters represent in this equation?

A
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5
Q

What is the axis of symmetry called?

A

Principal axis.

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6
Q

What is the principal focus?

A
  • A point on the axis which is the same distance from the optical centre as the focal length.
  • Where light rays travelling parallel to the principal axis prior to refraction converge.
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7
Q

What is the focal length?

A

Distance between the centre of the lens and the principal focus.

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8
Q

What is the role of the objective lens?

A

To collext as much light as possible.

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9
Q

What is the purpose of the eyepiece lens?

A

To magnify the image produced by the objective lens.

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10
Q

What is normal adjustment?

A

When the distance between the objective and eyepiece lenses is equal to the sum of their focal lengths.

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11
Q

Draw a lens diagram of normal adjustment.

A
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12
Q

What is the equation for angular magnification in normal adjustment?

A
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13
Q

What is the equation for angular magnification in terms of focal lengths and what is the condition it can be used?

A

When both angle are less than 10o

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14
Q

What do the letters represent in this equation?

A
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15
Q

Draw an annoted ray diagram for a Cassegrain telescope.

A
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16
Q

What is chromatic aberration?

A
  • When a lens refracts white light into different colours due to their wavelengths.
  • Causing the image for each colour to form in different positions, resulting in coloured fringes around the image.
17
Q

What is spherical aberration?

A
  • Light is focused in different places due to the curvature of a lens or mirror, causing image blurring.
  • Can be resolved in reflecting telescopes by using a parabolic mirror.
18
Q

Describe a solution to chromatic and spherical aberration in lenses.

A

Using an achromatic doublet brings all rays of light into focus in the same position by using a convex lens and a concave lens of different types of glass cemented together.

19
Q

Define collecting power.

A

A measure of the ability of a lens or mirror to collect incident EM radiation.

20
Q

What is collecting power proportional to?

A

The square of the objective diameter.

21
Q

Define resolving power.

A

The ability of a telelscope to produce separate images of close-together objects.

22
Q

State the Rayleigh Criterion.

A

Two objects will not be resolved if any part of the central maximum of either of the images falls within the first minimum diffraction ring of the other.

23
Q

What is the equation for the minimum angular separation?

24
Q

What do the letters represent in this equation?

25
Q

What are the advantages of large diameter telescopes?

A

Greater collecting power (brighter) and resolving power (clearer).

26
Q

What is a CCD?

A

An array of light-sensitive pixels which become charged when they are exposed to light (by the photoelectric effect).