nats 1311 - from the cosmos to earth our second exam will be next thursday, october 30 at the...
TRANSCRIPT
NATS 1311 - From the Cosmos to Earth
Our second exam will be next Thursday, October 30 at the regular class time. We will have a review Tuesday (Oct. 28) - at a time to be determined in class today - in the room next to where the regular lab is held. The exams will cover everything that we have covered in class up to the end of class Tuesday.
NATS 1311 - From the Cosmos to Earth
Properties of Light
Law of Reflection - Angle of Incidence = Angle of reflection
Law of Refraction - Light beam is bent towards the normal when passing into a medium of higher Index of Refraction.
Light beam is bent away from the normal when passing into a medium of lower Index of Refraction.
Index of Refraction -
Inverse square law - Light intensity diminishes with square of distance from source.
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n=Speedof lightin vacuumSpeedof lightin amedium
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NATS 1311 - From the Cosmos to Earth
Normal
Law of Reflection
Angle of incidence () = angle of reflection ()
The normal is the ray path perpendicular to the mirror’s surface.
NATS 1311 - From the Cosmos to Earth
Center of curvature - the center of the circle of which the mirror represents a small arcPrincipal axis - a radius drawn to the mirror surface from the center of curvature of the mirror - normal to mirror surfaceFocus - the point where light rays parallel to principal axis converge; the focus is always found on the inner part of the "circle" of which the mirror is a small arc; the focus of a mirror is one-half the radiusVertex - the point where the mirror crosses the principal axisFocal length - the distance from the focus to the vertex of the mirror
Geometry of a Concave Mirror
Focus
Principal axisVertex
Focal length
NATS 1311 - From the Cosmos to Earth
Index of Refraction
As light passes from one medium (e.g., air) to another (e.g., glass, water, plexiglass, etc…), the speed of light changes. This causes to light to be “bent” or refracted. The amount of refraction is called the index of refraction.
NATS 1311 - From the Cosmos to Earth
Imagine that the axles of a car represent wave fronts. If the car crosses from a smooth to a rough surface at an angle, one tire of the axle will slow down first while the other continues at normal speed. With one tire traveling faster the other, the car will turn in the direction of the slow tire. This is how refraction works.
Refraction
NATS 1311 - From the Cosmos to Earth
AIR
GLASS / WATER
Slower Propagating Speed
Car
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
AIR
GLASS / WATER
Slower Propagating Speed
Car
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
AIR
GLASS / WATER
Slower Propagating Speed
NORMAL LIGHT BENDING TOWARDS THE
NORMAL
LIGHT RAY
NATS 1311 - From the Cosmos to Earth
n2
AIR
GLASS / WATER
Slower Propagating Speed
NORMAL LIGHT BENDING TOWARDS THE
NORMAL
n1
Snell's Law
( Next Slide )
NATS 1311 - From the Cosmos to Earth
GLASS / WATER
Car
AIR
Slower Propagating Speed
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
GLASS / WATER
Car
AIR
Slower Propagating Speed
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
GLASS / WATER
Car
AIR
Slower Propagating Speed
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
AIR
Slower Propagating Speed
GLASS / WATER
NORMAL
AGAIN, LIGHT BENDS TOWARDS THE NORMAL
upon entering a region with slower speed.
LIGHT RAY
NATS 1311 - From the Cosmos to Earth
Slower Propagating Speed
GLASS /WATER
Car
AIR
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
Slower Propagating Speed
GLASS /WATER
Car
AIR
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
Slower Propagating Speed
GLASS /WATER
Car
AIR
( Sand / Gravel )
NATS 1311 - From the Cosmos to Earth
NOW LIGHT BENDS AWAY FROM THE NORMAL
Slower Propagating Speed
GLASS /WATER
AIR
LIGHT RAY
NORMAL
NATS 1311 - From the Cosmos to Earth
Optical axis - axis normal to both sides of lens - light is not refracted along the optical axisFocus - the point where light rays parallel to optical axis converge; the focus is always found on the opposite side of the lens from the objectFocal length - the distance from the focus to the centerline of the lens
Geometry of a Converging (Convex) Lens
Optical axisFocus
Focal length
NATS 1311 - From the Cosmos to Earth
Fo
cal
Plan
el1 l2
o i
Geometry of a Simple Lens
€
1
o+
1
i=
1
f
M =−i
o=l2l1
f
Lens formula
Linear Magnification
Using the Gaussian form of the lens equation, a negative sign is used on the linear magnification equation as a reminder that all real images are inverted
The focal plane is where incoming light from one direction and distance (object distance o greater than focal length) is focused.
NATS 1311 - From the Cosmos to Earth
Focal length
€
1
o+
1
i=
1
f
For astronomical distances, o ≅ ∞ and
1
i=
1
f or f = i
Fo
cal P
lane
NATS 1311 - From the Cosmos to EarthThe Eye
The eye consists of pupil that allows light into the eye - it controls the amount of light allowed in through the lens - acts like a simple glass lens which focuses the light on the retina - which consists of light sensitive cells that send signals to the brain via the optic nerve. An eye with perfect vision has its focus on the retina when the muscles controlling the shape of the lens are completely relaxed - when viewing an object far away - essentially at infinity.
NATS 1311 - From the Cosmos to Earth
When viewing an object not at infinity, the eye muscles contract and change the shape of the lens so that the focal plane is at the retina (in an eye with perfect vision). The image is inverted as with a single lens - the brain interprets the image and rights it.
NATS 1311 - From the Cosmos to Earth
Geometry of a Concave Mirror
Vertex
Focal length
€
1
o+
1
i=
1
f
For astronomical distances, o ≅ −∞ and
1
i=
1
f or f = i
Focal plane
NATS 1311 - From the Cosmos to Earth
Refracting Telescope
Uses lens to focus light from distant object - the eyepiece contains a small lens that brings the collected light to a focus and magnifies it for an observer looking through it.
NATS 1311 - From the Cosmos to Earth
The largest refracting telescope in the world is the at the University of Chicago’s Yerkes Observatory - it is 40 inches in diameter and 63 feet long.
NATS 1311 - From the Cosmos to Earth
Reflecting Telescope
The primary mirror focuses light at the prime focus. A camera or another mirror that reflects the light into an eyepiece is placed at the prime focus.
NATS 1311 - From the Cosmos to Earth
Types of Reflecting Telescopes
Each design incorporates a small mirror just in front of the prime focus to reflect the light to a convenient location for viewing.
NATS 1311 - From the Cosmos to Earth
Mirror Position and Focus Animation
Focus Inversion Animation
The image from reflecting and refracting telescopes is inverted.
The focus is adjusted by changing the secondary mirror position.
NATS 1311 - From the Cosmos to Earth
The Keck Telescopes
Largest in the world - on Mauna Kea in Hawaii. 36 hexagonal mirrors function as single 10-meter mirror.