Week 4 Lectures Flashcards

1
Q

WhichstatementaboutancientGreekastronomersis correct?

A

They performed a test to see whether Earth went around the Sun but misinterpreted what they saw.

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2
Q

First to reject previous Ptolemaic model on purely empirical (as opposed to philosophical) grounds – it didn’t match the observations well enough, so there must be a better model!
• Made a model with lots of epicycles (circles on circles on circles). Not pretty, but mathematically rigourous, and better match to observations.

A

Ibn Al-Shatir

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3
Q

First formal testable model with Sun at the center. Predictions about as good as Ptolemy’s.

A

Nicolaus Copernicus

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4
Q

Heliocentric model that matched observations better than Copernicus’s, using elliptical orbits.

A

Johannes Kepler

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5
Q

was ultimately responsible for acceptance of heliocentric model.

A

Success of Kepler’s predictions matching the observations

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6
Q

Kepler’s First Law

A

— Planets orbit in elliptical
orbits with the Sun at one focus.

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7
Q

Kepler’sSecondLaw

A

Planets sweep out equal areas in equal time (i.e. they move faster when closer to the Sun).

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8
Q

Which statement is correct about how fast the Earth moves around the Sun?.

A

A. It moves fastest in January

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9
Q

Kepler’sThirdLaw

A

Innerplanetshaveshorteryears than outer planets, with a precise mathematical relationship between orbital distance and period

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10
Q

Made major improvements to the recently-invented telescope, and turned it
up to the sky!

• A few key observations and experiments convinced remaining
doubters.

A

Galileo Galilei

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11
Q

Galileo’s Discoveries

A

Demonstrated that we feel acceleration, not motion. Answered “why don’t we feel like we’re moving?” objection.
2. Observed all phases of Venus, so Venus must sometimes be behind the Sun.
3. Discovered moons of Jupiter. (proved that Earth is not the center of everything)

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12
Q

Galileo’s Legacy

A

• According to the Catholic Church’s interpretation at the time, the Earth must be at the center of the Universe. They forced him to recant his views (1633) and put him under house arrest.
• By 1700, Kepler’s model + Galileo’s observations had convinced everyone (incl. Catholic Church by 1750s, though they didn’t officially pardon him until 1992!).

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13
Q

Goal of Scientific Method

A

Prove theories false

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14
Q

describe how planets orbit the Sun (and how the Moon orbits Earth, exoplanets orbit their stars)

A

Kepler’s Laws

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15
Q

push or pull on an object that modifies its motion.

A

force

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16
Q

Matter attracts other matter. The force of attraction depends on the
mass.

17
Q

+/- electrical charges. Opposite charges attract, like charges repel, moving charges get pulled sideways.

A

Electromagnetism

18
Q

Very short-range force that keeps the nucleus of an atom stable.

A

Strong Nuclear Force

19
Q

Very short-range force responsible for radioactive decay of nuclei.

A

Weak Nuclear Force

20
Q

Fundamental Forces

A

Gravity
Electromagnetism
Strong Nuclear Force
Weak Nuclear Force

21
Q

Keeps things from floating away from the Earth

22
Q

–Everything else!!!

A

Electromagnetism

23
Q

Gravity is