Geometrical Optics 01/31/2008 UW ASTR 597 surface normal incident ray same angle exit ray Spring 2011 2 UW ASTR 597 UW ASTR 597 “real” you A too long shortest path; equal angles B mirror only needs to be half as high as you are tall. Your image will be twice as far from you as the mirror. Spring 2011 Lecture 5 3 Spring 2011 “image” you 4 1 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 5 UW ASTR 597 Spring 2011 6 UW ASTR 597 UW ASTR 597 A n1 = 1.0 n2 = 1.5 Snell’s Law: n1sinθ1 = n2sinθ2 θ1 A B C road dirt θ2 D (house) Lecture 5 dist. 5 16 20 15 12 Δt@5 1 3.2 — — — AD: 6.67 minutes ABD: 6.0 minutes: the optimal path is a “refracted” one ACD: 7.2 minutes B Spring 2011 leg AB AC AD BD CD 7 Spring 2011 Δt@3 — — 6.67 5 4 Note: both right triangles in figure are 3-4-5 8 2 Geometrical Optics 01/31/2008 UW ASTR 597 incoming ray hugs surface n1 = 1.0 n2 = 1.5 Note that the wheels move faster (bigger space) on the sidewalk, slower (closer) in the grass 42° Spring 2011 UW ASTR 597 9 Spring 2011 10 UW ASTR 597 UW ASTR 597 n1 = 1.5 n2 = 1.0 incoming ray (100%) 96% 8% reflected in two reflections (front & back) Wheel that hits sidewalk starts to go faster, which turns the axle, until the upper wheel re-enters the grass and goes straight again 4% 92% transmitted 4% Spring 2011 Lecture 5 image looks displaced due to jog 11 Spring 2011 0.16% 12 3 Geometrical Optics 01/31/2008 UW ASTR 597 UW ASTR 597 pinhole object A lens, with front and back curved surfaces, bends light twice, each diverting incoming ray towards centerline. Follows laws of refraction at each surface. Parallel rays, coming, for instance from a specific direction (like a distant bird) are focused by a convex (positive) lens to a focal point. image at film plane In a pinhole camera, the hole is so small that light hitting any particular point on the film plane must have come from a particular direction outside the camera object image at film plane lens Placing film at this point would record an image of the distant bird at a very specific spot on the film. Lenses map incoming angles into positions in the focal plane. Spring 2011 13 In a camera with a lens, the same applies: that a point on the film plane more-or-less corresponds to a direction outside the camera. Lenses have the important advantage of collecting more light than the pinhole admits Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 15 14 UW ASTR 597 Spring 2011 16 4 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 17 UW ASTR 597 Spring 2011 UW ASTR 597 real foci Lecture 5 UW ASTR 597 virtual foci s=∞ s’ = f s=∞ s’ = -f s=f s’ = ∞ s = -f s’ = ∞ s=∞ s’ = f s=∞ s’ = -f Spring 2011 18 19 Spring 2011 20 5 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 21 UW ASTR 597 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 23 22 UW ASTR 597 Spring 2011 24 6 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 25 UW ASTR 597 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 27 26 UW ASTR 597 Spring 2011 28 7 Geometrical Optics 01/31/2008 UW ASTR 597 UW ASTR 597 Take the parabola: y = x2 Slope is y’ = 2x Curvature is y’’ = 2 So R = 1/y’’ = 0.5 Slope is 1 (45°) at: x = 0.5; y = 0.25 So focus is at 0.25: f = R/2 Note that pathlength to focus is the same for depicted ray and one along x = 0 Spring 2011 29 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 31 30 UW ASTR 597 Spring 2011 32 8 Geometrical Optics 01/31/2008 UW ASTR 597 f=D D UW ASTR 597 f = 4D D f/1 beam: “fast” Spring 2011 f/4 beam: “slow” 33 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 35 34 UW ASTR 597 Spring 2011 36 9 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 37 UW ASTR 597 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 39 38 UW ASTR 597 Spring 2011 40 10 Geometrical Optics 01/31/2008 UW ASTR 597 UW ASTR 597 neg. S.A. lens side zero S.A. pos. S.A. Spring 2011 41 Spring 2011 UW ASTR 597 Spring 2011 Lecture 5 43 42 UW ASTR 597 Spring 2011 44 11 Geometrical Optics 01/31/2008 UW ASTR 597 Spring 2011 45 UW ASTR 597 Spring 2011 46 UW ASTR 597 Spring 2011 Lecture 5 47 12