© 2010 pearson education, inc. slide 19-2 19 optical instruments

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© 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

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Page 1: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc. Slide 19-2

19 Optical Instruments

Page 2: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc. Slide 19-3

Page 3: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc. Slide 19-4

Page 4: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc. Slide 19-5

Page 5: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

The Camera

Slide 19-14

Page 6: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Focusing a Camera

Slide 19-15

Page 7: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

A digital image is made up of millions of pixels.

Digital Cameras

A CCD chip records the digital image.

Slide 19-16

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© 2010 Pearson Education, Inc.

The Human Eye

Slide 19-17

Page 9: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Focusing and Accommodation

Slide 19-18

Page 10: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Refractive Power

Slide 19-19

The refractive power of a lens of focal length f is the inverse of that focal length.

The unit of refractive power is meters-1, or diopters

Eyeglasses are measure in units of diopters, positive or negative

Page 11: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Hyperopia

Slide 19-20

Example for a person who can only focus at 1.5 meters away

Need to create a virtual image at 1.5 meters

3.3m-1 = 3.3 diopters

Page 12: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Myopia

Slide 19-21

To correct nearsightedness, need to create a virtual image of an object that is at infinity that appears to be at 2.0 meters distance, the far point of the person’s vision.

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© 2010 Pearson Education, Inc.

Apparent Size

Slide 19-22

Page 14: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

The Magnifier

Largest angular size without a magnifier is

With a magnifier, the angular size is

The magnification is thus

Slide 19-23

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© 2010 Pearson Education, Inc.

The Microscope

Slide 19-24

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© 2010 Pearson Education, Inc.

Maya performs light microscopy

Slide 19-34

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© 2010 Pearson Education, Inc.

The Microscope

Slide 19-25

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© 2010 Pearson Education, Inc.

The Telescope

Slide 19-26

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© 2010 Pearson Education, Inc.

Color and Dispersion

Slide 19-27

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© 2010 Pearson Education, Inc.

Chromatic Aberration

Slide 19-30

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© 2010 Pearson Education, Inc.

Resolution and the Wave Nature of Light

Slide 19-31

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© 2010 Pearson Education, Inc.

Two objects are resolvable if their angular separation is greater than

Rayleigh’s Criterion

Slide 19-32

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© 2010 Pearson Education, Inc.

The Resolution of a Microscope

Slide 19-33

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© 2010 Pearson Education, Inc.

Rainbows

Slide 19-28

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© 2010 Pearson Education, Inc.

Lens Aberrations: Spherical Aberration

The Hubble space telescope originally suffered from spherical aberration.

Slide 19-29

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© 2010 Pearson Education, Inc.

The Very Large Telescope – a four telescope array

“The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.”

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© 2010 Pearson Education, Inc.

Center of the Milky Way

Region near supermassive black hole

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© 2010 Pearson Education, Inc.

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© 2010 Pearson Education, Inc.

Optical and Electron Micrographs of e. coli

Slide 19-34

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© 2010 Pearson Education, Inc.

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© 2010 Pearson Education, Inc.

Scanning electron microscope (SEM)

Beam of electrons, collimated, scanned over specimen in a vacuum

Backscattered electrons are collected, used to determine image

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© 2010 Pearson Education, Inc.

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© 2010 Pearson Education, Inc.

Creepy nasty bugs shown under SEM

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© 2010 Pearson Education, Inc.

Transmission electron microscope (TEM)

Passes electrons through the specimen

Page 35: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Electron Diffraction Images

Page 36: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Chandra X-Ray ObservatoryFocuses X-Rays by glancing them off hyperbolic surfaces

Page 37: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Chandra X-Ray Observatory ImageColliding galaxies with supermassive black holes

Page 38: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Porro prism and roof prism binocular designs

Page 39: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Stage lightingCompact near-point light source

Computer controlled filters, masks, altazimuth mount

Light 230 watt

Light angle down to 2.25º

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© 2010 Pearson Education, Inc.

Solar Architecture and Engineering

Page 41: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Passive solar homes accept or reject sunlight to control climate

Page 42: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Dimetrodons probably used their “sails” for solar heating

Page 43: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Cliff dwellings are early solar homes – Made desert life cool

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© 2010 Pearson Education, Inc.

Atomic force microscopy These are individual atoms

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© 2010 Pearson Education, Inc.

Near Field Microscopy – Bypassing the Rayleigh Limit

Page 46: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Reading Quiz1. The units of refractive power are

A. watts.

B. m2.

C. m–1.

D. joules.

Slide 19-6

Page 47: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Answer 1. The units of refractive power are

A. watts.

B. m2.

C. m–1.

D. joules.

Slide 19-7

Page 48: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Reading Quiz2. Accommodation of the eye refers to its ability to

A. focus on both nearby and distant objects.

B. move in the eye socket to look in different directions.

C. see on both the brightest days and in the dimmest light.

D. see both in air and while under water.

Slide 19-8

Page 49: © 2010 Pearson Education, Inc. Slide 19-2 19 Optical Instruments

© 2010 Pearson Education, Inc.

Answer 2. Accommodation of the eye refers to its ability to

A. focus on both nearby and distant objects.

B. move in the eye socket to look in different directions.

C. see on both the brightest days and in the dimmest light.

D. see both in air and while under water.

Slide 19-9

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© 2010 Pearson Education, Inc.

Reading Quiz3. The magnification of a microscope is increased when

A. the focal length of the objective lens is increased.

B. the focal length of the objective lens is decreased.

C. the focal length of the eyepiece is increased.

D. the distance between the objective lens and eyepiece is decreased.

Slide 19-10

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© 2010 Pearson Education, Inc.

Answer 3. The magnification of a microscope is increased when

A. the focal length of the objective lens is increased.

B. the focal length of the objective lens is decreased.

C. the focal length of the eyepiece is increased.

D. the distance between the objective lens and eyepiece is decreased.

Slide 19-11

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© 2010 Pearson Education, Inc.

4. The fundamental resolution of an optical instrument is set by

A. the accuracy to which lenses can be polished.

B. the fact that white light is composed of all visible colors.

C. the fact that all types of glass have nearly the same index of refraction.

D. the wave nature of light.

Reading Quiz

Slide 19-12

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© 2010 Pearson Education, Inc.

Answer 4. The fundamental resolution of an optical instrument is set by

A. the accuracy to which lenses can be polished.

B. the fact that white light is composed of all visible colors.

C. the fact that all types of glass have nearly the same index of refraction.

D. the wave nature of light.

Slide 19-13