Lecture 6 Flashcards

(22 cards)

1
Q

aristotle’s beliefs?

A
  • earth was stationary
  • moon, sun, planets , stars revolve around the earth on crystalline spheres
  • geocentric cosmology
  • unknown force keeps spheres revolving
  • this view could not explain changes of brightnesses, sizes of planets, apparent retrograde motion of mars
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2
Q

what were ptolemy’s beliefs?

A

tried to unite aristole’s views w/ his observations

introduced epicycles to explain anomalies in planetary motion; explained apparent retrograde motion of mars

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3
Q

what were copernicus’s beliefs/discoveries?

A
  • noticed that ptolemy’s predictions for planetary positions were off
  • realized that earth and other planets orbit around the sun
  • was problematic against the church b/c they thought the earth was the centre of the universe
  • this showed why mercury, venus are always near the sun
  • thought that orbits were circular
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4
Q

what did tycho brahe discover?

A
  • made first precision astrometric measurements
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5
Q

what did kepler discover?

A
  • that planetary orbits are not circles, but are ellipses

- measured time for each planet to orbit the sun

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6
Q

what is the orbital period of earth?

A

365.25 d

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7
Q

what are kepler’s laws?

A

1) planets travel in elliptical orbits w/ sun at one focus
2) planets travel faster when closest to the sun (equal areas are swept out in equal times)
3) square of orbital period P is proportional to cube of semi-major axis

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8
Q

what is the eqn that represents kepler’s third law?

A

P^2 is proportional to a^3

a = semi-major axis

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9
Q

what were galileo’s discoveries?

A
  • first to use a telescope
  • saw craters and sunspots
  • 4 moons of jupiter (not everything orbits the earth) and phases of venus
  • inertia and mass
  • acceleration: all objects accelerate in the same way when it falls toward earth (independent of mass)
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10
Q

what were netwon’s discoveries?

A
  • laws of motion

- universal law of gravitation

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11
Q

what are the 3 laws of motion?

A

1) object stays at rest or at constant speed unless a force acts on it
2) a force results in an acceleration that depends on the object’s mass
3) every force has an equal and opposite rxn force

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12
Q

what kind of rays are blocked by the upper atmosphere?

A

gamma
X
UV

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13
Q

how is visible light affected by the earth’s atmosphere?

A

it is still observable on surface

has some atmospheric distortion

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14
Q

how is infrared spectrumaffected by the earth’s atmosphere?

A

most is absorbed by atm gases

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15
Q

how are radio waves affected by the earth’s atmosphere?

A

they are observable

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16
Q

how are long wavelength radio waves affected by the earth’s atmosphere?

A

they are blocked

17
Q

why have a bigger telescope?

A

the amount of light collected is proportional to the area of the telescope

S is proportional to pi(D/2)^2

s = sensitivity (total number of photons collected)

D = diameter of telescope

18
Q

how much more sensitive is a 10’’ telescope than a 5’’ one?

19
Q

disadvantages of refractors?

A
  • lens gets very big
  • telescope structure bends
  • chromatic aberration
20
Q

what is chromatic aberration?

A

failure of a lens to focus all colors to the same point

It is caused by dispersion; different amounts of light is refracted depending on the wavelength of it

Eg. blue light is refracted a bit more than yellow and red light

21
Q

old telescopes are ____

modern telescopes are _____

A

refractors

reflectors

22
Q

describe modern reflector telescopes.

what are pros of this?

A

uses curved mirror to collect and focus light

pros:

  • has no chromatic aberration
  • lighter
  • can make bigger mirrors