history Flashcards

1
Q

What is the significance of Nicolaus Copernicus (1473-1543)?

A
  • study of planetary motions- doubted validity of accepted system.
  • from philosophical view
  • sun centred universe
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2
Q

What was Nicolaus Copernicus’ model?

A
  • perfect circles for orbits

- introduced small epicy-cles to improve accuracy.

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3
Q

what were the impacts of the model?

A

1- Rotation of Earth rather than heavens
2- natural order of planets
3- relative distance of planets- found grew systematically within increasing distance from sun
4-further out planet is- slower moves
5-simple explanation for retrograde motion
6-explanation of seasons
7-explanation of changes in planetary brightness

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4
Q

What was the intent of Tycho Brahe (1546-1601) and what did he do?

A
  • observatory on island of Hveen.
  • variety of instruments; 31 1/2 foot radius quadrant- improved angular scales and sighting design
  • accurate observations of positions of planets (1 minute of arc, 10 x better)
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5
Q

what did Tycho Brahe observe in 1577?

A

observed a bright comet, showed that comet was very distant

accumulated large body of data on planetary motion

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6
Q

Why could Tycho Brahe not accept the heliocentric view?

A

no evidence for Earth moving- protestant

developed model with earth fixed, sun orbiting it, all other planets orbit sun.

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7
Q

What was Johannes Kepler (1571-1630) interested in?

A
  • copernican system- mathematical simplicity
  • celestial harmony (spacing between planets determined by the spacing of geometric solids)
  • inherited all Tychos data
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8
Q

What did Kepler do?

A
  • mapped path Mars followed around sun
  • realised sun played central role in making planets move
  • but sun was not central to planets orbit
  • orbit of mars is oval, found it was simple ellipse with sun at focus.
  • found mars moves fastest when near sun
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9
Q

What are Keplers laws of planetary motion?

A

1st: orbits of planets are ellipses- sun at one focus
2nd: for each planet, area swept out in space by a line connecting that planet to sun equal in equal intervals of time
3rd: square of period of a planet is proportional to cube of the semimajor axis.
P^2 ∝ a^3
.

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10
Q

what did Galileo Galilei (1564-1642) do?

A
  • simple experiment and deduction in advancing the perception of universe
  • invented own telescope and discovered:
    1: moon not smooth sphere-craters and mountains
    2: milky way not cloud- stars
    3: Jupiter attended by four satellited
    4: Varying aspect of Venus, like phases of moon- showed venus shines by reflected sunlight- must orbit sun not Earth.
    5: studied dark spots sometimes appeared on face of sun- some thought planets but actually on surface
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11
Q

What did Galileo’s observations violate?

A

ancient philosophies of idealised universe with Earth Centre of all motion. Criticism from the church

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12
Q

What book did Isaac Newton (1642-1726) in 1687?

A

Philosophi, Naturalis Principia Mathematica

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13
Q

What are Newtons three laws?

A

1st: object at rest or in uniform motion will maintain that state unless compelled to do so otherwise with external force
2nd: rate of change of momentum (mass x velocity) of a object is equal to force applied. F= M X A
3rd: for every action, equal and opposite reaction.

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14
Q

How is Newton’s Universal law of gravity wrote?

A

Fgrav= G x (m1 x m2/r^2)

Fgrav= force of gravity 
G= gravitational constant (6.67 x 10^-11)
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15
Q

what does the combination of universal law and newtons 2nd law?

A

why the gravitational acceleration at the Earth’s surface is 9.8 m/s^2 (different on other bodies)

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16
Q

Newtonian gravity is a basis for explaining what?

A

Keplers empirical formula laws .

-an attractive force acting between sun and bodies in the solar system explains why they orbit in the way that they dp