Thin Lenses A lens is an optical device consisting of two refracting surfaces The simplest lens has two spherical surfaces close enough together that we.

Slides:



Advertisements
Similar presentations
Chapter 23.
Advertisements

Consider Refraction at Spherical Surfaces:
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Physics 2102 Jonathan Dowling Lecture 25 Optics: Images.
Flat Mirrors Consider an object placed in front of a flat mirror
Chapter 27 Optical Instruments.
Chapter 31 Images.
Chapter 23 Mirrors and Lenses.
Chapter 23 Mirrors and Lenses Conceptual questions: 4,5,10,14,15,17
Physics Light: Geometric Optics 23.1 The Ray Model of Light 23.2 Reflection - Plane Mirror 23.3 Spherical Mirrors 23.5 Refraction - Snell’s law.
Chapter 23 Mirrors and Lenses. Notation for Mirrors and Lenses The object distance is the distance from the object to the mirror or lens Denoted by p.
Chapter 23 Mirrors and Lenses.
and Optical Instruments
Lecture 25-1 Locating Images Real images form on the side of a mirror where the objects are, and virtual images form on the opposite side. only using the.
Reference Book is Geometric Optics.
Light: Geometric Optics
Physics 1502: Lecture 30 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Friday Optics –Mirrors –Lenses –Eye.
Physics 1402: Lecture 31 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Wednesday (after midterm 2) Optics –Lenses –Eye.
Geometric Optics Ray Model assume light travels in straight line
Copyright © 2012 Pearson Education Inc. PowerPoint ® Lectures for University Physics, Thirteenth Edition – Hugh D. Young and Roger A. Freedman Lectures.
7. Optical instruments 1) Cameras
Chapter 23 Mirrors and Lenses.
7. Optical instruments 1) Cameras
Optics 1----by Dr.H.Huang, Department of Applied Physics
Cameras Major components Lens (or combo) Film (or CCD) Aperture Shutter speed.
Lecture 26 Ch. 34 Physics 2102 Jonathan Dowling Optics: Images — Lenses.
Physics. PHS 5041 Optics Lenses Lenses are transparent objects with at least one curved surface. Lenses can be: _Convex or converging (***thickest at.
Copyright © 2009 Pearson Education, Inc. Chapter 33 Lenses and Optical Instruments.
Optical Instruments. Power of a lens Optometrists, instead of using focal length, use the reciprocal of the focal length to specify the strength of eyeglasses.
Physics 213 General Physics Lecture Last Meeting: Diffraction Today: Optical Instruments.
Camera No lens Inverted, real image Film or screen.
 Mirrors that are formed from a section of a sphere.  Convex: The reflection takes place on the outer surface of the spherical shape  Concave: The.
Chapter 23 Mirrors and Lenses.
Fundamental of Optical Engineering Lecture 3.  Aberration happens when the rays do not converge to a point where it should be. We may distinguish the.
A diffraction grating with 10,000 lines/cm will exhibit the first order maximum for light of wavelength 510 nm at what angle? (1 nm = 10-9 m) 0.51° 0.62°
Magnifiers, Projectors, CamerasPaul Avery (PHY 3400)1 Magnifiers, Projectors, Cameras Applied Optics Paul Avery University of Florida
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 27 Physics, 4 th Edition James S. Walker.
Chapter 34 Lecture Eight: Images: II. Image Formed by a Thin Lens A thin lens is one whose thickness is small compared to the radii of curvature For a.
Chapter 36 Image Formation (Lens and Mirrors) Using the ray approximation of geometric optics, we can now study how images are formed with mirrors and.
Unit 11: Part 2 Mirrors and Lenses. Outline Plane Mirrors Spherical Mirrors Lenses The Lens Maker’s Equation Lens Aberrations.
Geometric Optics This chapter covers how images form when light bounces off mirrors and refracts through lenses. There are two different kinds of images:
Chapter 35 MirrorsLenses Images. We will use geometrical optics: light propagates in straight lines until its direction is changed by reflection or refraction.
 When light strikes the surface of an object  Some light is reflected  The rest is absorbed (and transferred into thermal energy)  Shiny objects,
Test Corrections Due Tuesday, April 26 th Corrections must be done in a different ink color Lots of 4’s for effort – doesn’t mean answer is right! Check.
Optical Density - a property of a transparent medium that is an inverse measure of the speed of light through the medium. (how much a medium slows the.
Lesson 25 Lenses Eleanor Roosevelt High School Chin-Sung Lin.
1 32 Optical Images image formation reflection & refraction mirror & lens equations Human eye Spherical aberration Chromatic aberration.
The Refraction of Light: Lenses and Optical Instruments
Lecture 18 Optical Instruments
1 Thin Lens Light refracts on the interface of two media, following Snell’s law of refraction: Light bends through a triangular prism: θ 1 and θ 2 are.
Thin-lens equation: 1/f = 1/d 0 + 1/d i. Magnification equation: h i /h o = d i /d o.
3.30. Image location by ray tracing Consider a real object that is placed in front of a convex lens. The location of the image can be found by considering.
Physics 203/204 4: Geometric Optics Images formed by refraction Lens Makers Equation Thin lenses Combination of thin lenses Aberration Optical Instruments.
Dispersion The spreading of light into its color components is called dispersion. When light enters a prism, the refracted ray is bent towards the normal,
Lab 9: Geometrical optics Only 3 more labs to go!! Today we are going to do three experiments: 1. Measure the intensity of light as a function of distance.
Physics 1202: Lecture 23 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Lecture Outlines Chapter 27 Physics, 3rd Edition James S. Walker
 Mirrors that are formed from a section of a sphere.  Convex: The reflection takes place on the outer surface of the spherical shape  Concave: The.
Physics 1202: Lecture 22 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
1 The law of reflection: The law of refraction: Snell’s Law Image formation.
Geometric Optics: Mirrors and Lenses. Mirrors with convex and concave spherical surfaces. Note that θ r = θ i for each ray.
Part 10 Optics --Mirrors and Lenses Chapter 24 Geometric Optics.
Refraction & lenses. Types Of Lenses Image Formation via Refraction by thin lenses Thin lenses are those whose thickness is small compared to their radius.
Mirrors and Lenses How do eyeglasses correct your vision? When you look in a mirror, where is the face you see? In which ways is a cell phone camera similar.
Refraction & Lenses. Refraction of Light When a ray of light traveling through a transparent medium encounters a boundary leading into another transparent.
Lenses Converging Lens Diverging Lens F F f f.
Lecture 2: Reflection of Light: Mirrors (Ch 25) & Refraction of Light: Lenses (Ch 26)
Ch. 30 Lenses.
lens that causes light rays parallel to central axis to converge
Presentation transcript:

Thin Lenses A lens is an optical device consisting of two refracting surfaces The simplest lens has two spherical surfaces close enough together that we can neglect the distance between the surfaces (i.e., thin) Consider two spherical surfaces (with radii of curvature R1 and R2), separating three materials of index of refraction n1, n2, and n3 For the first surface, we can use the refracting surface equation to relate the object distance p1, image distance q1, and radius of curvature R1, ignoring the second surface.

From diagram (on board), we get Now let the image formed by surface 1, I1, be the object for surface 2, O2 I1 is a virtual image. Therefore Here, we neglect the thickness of the lens Again apply the refracting surface equation, but for surface 2, neglecting surface 1 The image, I2, is real

Let n1=n3=1 (air or vacuum) and n2=n Adding with p1=p and q2=q, gives Letting p and q f gives This is the lens maker’s equation q p

Example Problem 36.36 The projection lens in a certain slide projector is a single thin lens. A slide 24.0 mm high is to be projected so that its image fills a screen 1.80 m high. The slide-to-screen distance is 3.00 m (a) Determine the focal length of the projection lens. (b) How far from the slide should the lens of the projector be placed in order to form the image on the screen?

Aberrations In our development of the mirror and lens equations, we assumed paraxial rays, i.e. rays with small angles with respect to the principal axis We also assumed for lenses that they are thin These are approximations (but reasonable) For more precise determinations of images, we must use the laws of refraction and reflection to trace the paths of rays We find that two types of aberrations result from the use of spherical surfaces

Spherical Aberrations A geometrical for rays of the same  Rays further from the principal axis are focused closer to the lens for a converging lens Spherical aberration can be eliminated by the use of, for example, parabolic mirrors – all rays focus to a common point – but expensive Or apertures can be used to remove the non-paraxial rays

Chromatic Aberration Since the index of refraction is a function of , rays with different  will refract at different angles when passing through a lens (for the same paraxial ray) The rays focus at different locations for each  Not a problem for monochromatic light beams For ordinary (polychromatic) light, chromatic aberration can be reduced by - choose materials with minimal  dependence of n - use combinations of diverging and converging lenses

Optical Devices: The Camera The camera system consists of a converging lens, aperture, shutter, and film q is adjusted to focus a real, inverted images on the film for large object distance (p>>q) The shutter is opened for a time duration t. Usually, between 1/30 to 1/250 s exposure time. This allows light to strike the film creating the image.

The intensity of the light reaching the film is proportional to the area “viewed” by the camera and the effective area of the lens – controlled by the diameter D of the aperture) Light intensity I is the rate of light energy received by the film per unit area (energy/area/time) – see chap. 34 When p>>f and q  f, the area of the image is f2. Therefore, I is proportional to D2/f2. In photography, the light-gathering capability of a lens is expressed in terms of f/D called the f-number. Therefore Increasing D by 2 reduces f-number by 1/2 and increases I by 2 at the film

Typical f-numbers. f/2, f/2. 8, f/4, f/5. 6, f/8, f/11, f/16 Typical f-numbers f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16 large  small aperture (exposure) The following combinations give same exposure f/4 & 1/500s = f/5.6 & 1/250s = f/8 & 1/125 s Example Problem 36.46 A camera is being used with a correct exposure at f/4 and a shutter speed of 1/16 s. In order to photograph a rapidly moving subject, the shutter speed is changed to 1/128 s. Find the new f-number needed to maintain satisfactory exposure.

Example Problem 36.49 A person sees clearly when he wears eyeglasses that have a power of -4.00 diopters and sit 2.00 cm in front of his eyes. If the person wants to switch to contact lenses, what lens power should be prescribed?