1 / 22

Introduction to Mirrors

Physics 102: Lecture 16. Introduction to Mirrors. HE2 today! Bring your ID, #2 pencil, calculator Cell phones, laptops, ipod, etc must be OFF. Phys 102 recent lectures. Light as a wave. Lecture 14 – EM waves Lecture 15 – Polarization

revat
Télécharger la présentation

Introduction to Mirrors

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Physics 102: Lecture 16 Introduction to Mirrors HE2 today! Bring your ID, #2 pencil, calculator Cell phones, laptops, ipod, etc must be OFF

  2. Phys 102 recent lectures Light as a wave • Lecture 14 – EM waves • Lecture 15 – Polarization • Lecture 20 & 21 – Interference & diffraction (coming soon!) Light as a ray • Lecture 16 – Reflection • Lecture 17 – Spherical mirrors & refraction • Lecture 18 – Refraction & lenses • Lecture 19 – Lenses & your eye

  3. Light incident on an object • Absorption • Reflection (bounces) • See it • Mirrors • Refraction (bends) • Lenses • Often some of each Everything true for wavelengths << object size

  4. y x z Recall: wavefronts Wavefronts represent “crests” of EM wave y y z z Direction of propagation l l Top view: x z

  5. Huygens’ principle Every point on a wavefront acts as a source of tiny “wavelets” that move forward. Direction of propagation “wavelet” wavefront

  6. Law of Reflection Incident wave Reflected wave qr Describe light as “rays” along direction of propagation of EM wave qi Angle of incidence = Angle of reflection qi = qr

  7. Object Location • Light rays from sun bounce off object and go in all directions • Some hit your eyes We know object’s location by where rays come from. • Color results from some light being absorbed by object before bouncing off.

  8. qr qi Flat Mirror • All you see is what reaches your eyes • You thinkobject’s location is where rays appear to come from. Smooth Mirror All rays originating from peak will appear to come from same point behind mirror! Image Object

  9. qr qi d Flat Mirror (1) Draw first ray perpendicular to mirror 0 = qi = qr (2) Draw second ray at angle. qi = qr (3) Lines appear to intersect a distance d behind mirror. This is the image location. Example Light rays don’t really converge there, so it’s a “Virtual Image” Virtual: No light actually gets here d

  10. Flat Mirror Summary • Image appears: • Upright • Same size • Located same distance from, but behind, mirror • Facing opposite direction: Left/Right inverted • Virtual Image:Light rays don’t actually intersect at image location. Preflight 16.1 Why do ambulances have “AMBULANCE” written backwards? So you can read it in your rear-view mirror!

  11. mirror Preflight 16.3 Can you see Fido’s tail in mirror? No! (You) You need light rays from the tail to bounce off mirror and reach your eye! (Fido)

  12. ACT: Flat Mirrors You are standing in front of a short flat mirror which is placed too high, so you can see above your head, but only down to your knees. To see your shoes, you must move (1) closer to the mirror. (2) further from the mirror. (3) to another mirror. Changing distance doesn’t change what you see of yourself

  13. ACT: Flat Mirrors to see feet, bottom of mirror must extend at least as low as midpoint between eyes and feet—independent on how far you are from the mirror.

  14. 2 3 1 ACT/Two Mirrors How many images of money will you see (not including the actual money)? • 1 • 2 • 3 • 4 • 5 Homework lets you quantify positions of the money.

  15. Concave mirror light ray R principal axis • C R light ray Convex mirror R principal axis • C Curved mirrors A Spherical Mirror: section of a sphere. C = Center of curvature In front of concave mirror, behind convex mirror.

  16. Preflight 16.2 An organic chemistry student accidentally drops a glass marble into a silver nitrate mirroring solution, making the outside of the marble reflective. What kind of mirror is this? (1) concave (2) convex (3) flat 15% 63% 22%

  17. Focus f=R/2 Concave Mirror R Principal Axis Angle of incidence = angle of reflection. Thus rays are bent towards the principal axis. Rays parallel to principal axis and near the principal axis (“paraxial rays”) all reflect so they pass through the “Focus” (F). The distance from F to the center of the mirror is called the “Focal Length” (f).

  18. Preflight 16.4, 16.5 What kind of spherical mirror can be used to start a fire? concave convex 65% 35% How far from the match to be ignited should the mirror be held? farther than the focal length closer than the focal length at the focal length 11% 20% 69%

  19. F F Concave Mirror Principal Axis Rays traveling through focus before hitting mirror are reflected parallel to Principal Axis. Rays traveling parallel to Principal Axis before hitting mirror are reflected through focus

  20. Convex Mirror R Principal Axis Focus f=-R/2 Rays are bent away from the principal axis. Rays parallel to principal axis and near the principal axis (“paraxial rays”) all reflect so they appear to originate from the “Focus” (F). The distance from F to the center of the mirror is called the “Focal Length” (f).

  21. ACT: Mirror Focal Lengths A concave mirror has a positive focal length f > 0 A convex mirror has a negative focal length f < 0 What is the focal length of a flat mirror? (1) f =0 (2) f = ∞ The flatter the mirror, the larger the radius of curvature, (e.g. the earth is round, but looks flat)

  22. See You Wednesday.

More Related