Physics 3 Flashcards

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1
Q

Parallax

A

the apparent shift in position of an object when its viewed from various angles

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2
Q

Luminous Body

A

emits light waves ex. sun

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3
Q

Illuminated Body

A

reflect light waves ex moon

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4
Q

Luminous Flux ( italicized P)

A

rate at which light is emitted from a source (unit lumens Lm)

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5
Q

Illuminance ( E)

A

the illuminance of a surface (Lm/m^2)

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6
Q

Candela

A

luminous intensity

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7
Q

Transparency

A

transmits light waves and you CAN see through it. ex glass, water, air

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8
Q

Translucent

A

transmits light but you CANNOT see through it. ex. lamp shade, shower doors, skin shower curtains

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9
Q

Opaque

A

light cannot pass through it (reflects off of or absorbs) ex. wall, books

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10
Q

Galileo (1564- 1642)

A

Made the first serious attompt to measure the speed of light
-took 2 lanterns about 1km apart and “flashed” each other (one lantern was flashed and the lantern flashed back upon seeing the first lantern)
- Galileo hoped to use the time interval btwn the flash of each lantern and the distance btwn lanterns, to calculate the speed of light

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11
Q

What was Galileo’s problem

A
  • Problem: it didn’t work. said that the speed of light was infinite and couldn’t be calculated
  • Not an accurate method: Human reaction time is too slow. Reaction time took longer than the time for light to travel this distance.
    Measurement of time was not accurate enough
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12
Q

Olaus Roemer (1644 - 1710)

A

Danish astronomer
- tried to predict the eclipses of Jupiter’s moon (abt Jupiter)
-surprised to find out that the period of the eclipse, as he measured for one of the moons, was different at different times of tear.
- concluded that light has a finite speed (and that it was constant) and that the reason eclipse periods appeared to ching was bc:

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13
Q

Olaus Roemer concluded the reason eclipse periods appeared to change is bc:

A
  • depending on the Earths distance from Jupiter, light needs more or less time to reach Earth from Jupiter
  • difference between the two measured time periods is equal to the time it takes light to travel a distance appoximately equal to the diameter of the earths orbit
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14
Q

What was Olaus’ problem

A

Roemer didnt know how large the diameter of the Earths orbit was

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15
Q

Christian Huygens (approx same time as Roemer)

A

Dutch mathmatican/scientist
- Managed to figure ont the diameter of Earths orbit
- Used his data and Roemers data to calculate the speed of light
- difference between shortest and longest period Δt = 22 min (1320 s)

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16
Q

diameter of earths orbit

A

3x10^11 m/s

17
Q

d= v/t

A