1.2 - the refracting telescope

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37 Terms

1
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what is the equation for magnification?

magnification = image height / object height

2
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what is the unit for magnification?

there is no unit as it’s a ratio

3
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what is magnification?

the image appears larger than the object

4
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magnification = image height / object height. what units should image and object height be in?

any, providing they are in the same units as each other

5
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what are the 2 types of telescope?

  1. reflective

  2. refractive

6
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what are some features of a refractive telescope?

  • there are 2 converging lenses of different sizes; the large one is the objective lens and the smaller one is the eyepiece

  • i.e., 2 lenses in a tube in which the distance can be adjusted to focus the image

  • image is inverted, real, diminished

<ul><li><p>there are 2 converging lenses of different sizes; the large one is the objective lens and the smaller one is the eyepiece</p></li><li><p>i.e., 2 lenses in a tube in which the distance can be adjusted to focus the image</p></li><li><p>image is inverted, real, diminished</p></li></ul>
7
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is the distance between the lenses in a refractive telescope fixed or can it be moved?

the distance between the lenses can be adjusted

8
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how do we focus the image in a refractive telescope?

by adjusting the distance between the 2 lenses in the tube

9
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are the lenses inside a refractive telescope converging or diverging?

converging

10
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what is the objective lens?

ANSWER LATER

11
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what is the eyepiece lens?

ANSWER LATER

12
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how many lenses are in a refractive telescope?

2 converging ones - an objective lens and an eyepiece

13
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what image does a refractive telescope produce?

an inverted one

14
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how does a refractive telescope work?

  1. parallel light rays passing through an object are refracted when passing through the objective lens

  2. the light rays converge in the within the tube (between the 2 lenses), inverted the image

  3. the light rays refract at the eyepiece into parallel rays

  4. a real, diminished, inverted image is produced

<p></p><ol><li><p>parallel light rays passing through an object are refracted when passing through the objective lens</p></li><li><p>the light rays converge in the within the tube (between the 2 lenses), inverted the image</p></li><li><p>the light rays refract at the eyepiece into parallel rays</p></li><li><p>a real, diminished, inverted image is produced</p></li></ol><p></p>
15
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why does the image in a refractive telescope come out inverted?

because the light rays of the object converges within the tube, inverting the image, before coming out at the eye piece as an inverted image

16
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why is the image in a refractive telescope real?

because it is on the opposite side of the lens

17
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why does the image in a refractive telescope come out diminished?

because the objective lens (which the rays enter from) is larger than the eyepiece lens (which the rays exist from)

18
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ray diagram for a refractive telescope

DIAGRAM HERE

19
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do some questions on the ray diagram for the refractive telescope !

20
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what is normal adjustment?

when the refractive telescope is adjusted so the virtual image is at infinity

21
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what is it called when the refractive telescope is adjusted so the virtual image is at infinity?

normal adjustment

22
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where is the normal adjustment?

  1. where the principal focus of both lenses overlap

  2. where distance between 2 lenses = sum of focal lengths

23
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what happens when the principal focus of both lenses overlap and the distance between the 2 lenses equals the sum of the focal lengths?

normal adjustment

24
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for normal adjustment, what is needed from the distance between the 2 lenses?

to equal the sum of the focal lengths

25
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for normal adjustment, what is needed from the principal focus of both lenses?

they overlap

26
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real image is inverted and diminished ? of the normal adjustment or of the refracting diagram? are they the same thing?

27
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what are all angles in astrophysics measured in?

radians

28
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what is angular size?

  • θ = h/d

θ - angle (in radians) subtended by an object

h - height of object

d - distance (distance subtended?)

29
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what does subtended mean?

area swept out

30
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what is angular size used for?

used to understand sizes of huge objects

31
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what is angular magnification?

  • M = β / α

M - angular magnification (magnifying power)

β - angle (in radians) subtended by final image at infinity to viewer

α - angle (in radians) subtended by distant object to unaided eye

  • M = f0 / fe

M - angular magnification of telescope in normal adjustment

f0 - focal length of object lens (m)

fe - focal length of eyepiece lens (m)

kinda confused about this..

DIAGRAM

32
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what does angular magnification mean?

the magnifying power of a telescope

33
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radians → degrees

x 180 / π

34
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degrees → radians

x π / 180

35
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when can angular size be used?

it can only be used when β or α are < 10°

DIAGRAM

36
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how does length change the angular magnification?

the bigger the length, the higher the angular magnification

37
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why do industrial places have huge telescopes?

because the bigger the length, the higher the angular magnification