Week 3 Flashcards

(35 cards)

1
Q

What lenses can give you inverted images?

A

-only plus lenses!!!!(convex)

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2
Q

What lenses can give you magnified images?

A

-only plus lenses!!!!(convex)

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3
Q

What lenses can give you an image that is 1/2 the size of the object?

A

-both convex and concave lenses

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4
Q

What lenses can give you an image that is 2 times the size of the object?

A

-only plus lenses!!!(convex)

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5
Q

Where are the front and back focal lengths measured from?

A

-measured from vertex of the lens

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6
Q

Where are the effective focal lengths measured from?

A

-measured from principal planes

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7
Q

What is the power of the human eye?

A
  • cornea=+40D

- Crystalline lens=+20D

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8
Q

What kind of image is projected on the retina?

A
  • small
  • inverted
  • real
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9
Q

Why is the human eye a plus lens?

A

-the index of refraction of the aqueous solution it sits in gives it a plus power

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10
Q

Microscope lens set up

A
  • two lens structure
  • both plus lenses
  • image from the first lens is the object of the second lens
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11
Q

Microscope imaging

A
  • object for second lens is image from the first
  • object for second lens is on focal point, so image is projected at optical infinity
  • magnified, virtual image
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12
Q

Magnification of a microscope and telescope

A

M=Mobjective*Meyepiece

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13
Q

Resolution Limit

A
  • the SEPARATION between closest distinguishable points imaged through an optical instrument
  • smaller the better(smaller separation=higher resolution)
  • expressed in angle or length
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14
Q

Resolving Power

A
  • the RECIPROCAL OF THE SEPARATION between the closest distinguishable points imaged through an optical instrument
  • the larger the better
  • expressed in inverse angle or inverse length
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15
Q

Resolution and resolving power

A

-dependent on wavelength

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16
Q

Resolution of the human eye

A
  • 2mm for day light

- with wavelength, about 0.86 arcmin

17
Q

Telescope structure

A
  • two lens system
  • light from distant object(optical infinity, collimated light)
  • collimated beams exit second lens, with a smaller diameter than the ones that entered
18
Q

Power of a telescope

A
  • vergence is zero before AND after, so power is ZERO

- principal planes are at optical infinity

19
Q

Compare microscope and telescope

A

Microscope: observe near object

  • distance between lenses is larger than sum of focal lengths
  • image is magnified, inverted, dim
  • strong vergence for entering beam

Telescrope: observe distant object

  • distance between lenses is equal to the sum on the focal lengths
  • Image is minified, inverted, bright
20
Q

Telescope magnification

A
  • minifies object
  • -changes the angle in which we see the object, not the size of the object!!
  • looks 20-50 times larger than it would with the naked eye
21
Q

Telescope resolution

A
  • minimum angle of resolution=( 1.22* wavelength)/objective lens diameter
  • a telescope with D=2, separation is 0.06 arcsec
22
Q

Eye resolving power

A

Museful*angle of resolution

-0.3mrad

23
Q

Field of view

A

-can have same magnification and different field of view

24
Q

telescope resolution dependent factors

A
  • higher resolution for smaller wavelength
  • use blue filter for better resolution
  • increase Diameter of lens for smaller/finer resolution
25
Kepler-type telescrope
- 2 plus lenses - used in astronomy - lenses separated by sum of focal lengths - objective lens has larger diameter - eye piece has higher power
26
Kepler-type telescope imaging
- image is virtual and at optical infinity | - image is inverted
27
Galilei-type telescope
- one plus(objective lens) and one minus(eye piece) - used for terrestrial things - lenses are separated by focal objective-focal eyepiece - low vision aids
28
Galilei-type telescope imaging
-image is virtual and ERECT
29
Newtonian refractor
-adds a deviation mirroe
30
Catadioptric telescopes
-combination of refraction and diffraction
31
Radiotelescope
- uses radio waves instead of light | - hydrogen atom emission
32
Why do stars twinkle?
- atmosphere is non uniform lens | - pollution, scattering, hot/ cold, can alter images
33
Benefits to reflection
- no chromatic aberration - only one surface precision - no need for large volume of glass - better support(less weight)
34
What is the primary shape large mirrors use for their little pieces?
Hexagonal
35
What electromagnetic waves are used for space observation?
IR