The Birth of Modern Astronomy Flashcards

1
Q

What was so mysterious about planetary moton in our sky to early astronomers?

A

Like the Sun and Moon, planets usually drif
eastward relatve to the stars from night to night; but sometmes, for a few weeks or few months, a planet turns
westward in its apparent retrograde moton

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2
Q

Why did the ancient Greeks reject the real explanaton for planetary moton?

A

Most Greeks concluded that Earth
must be statonary, because they thought the stars could not be so far away as to make parallax undetectable

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3
Q

How did Copernicus, Tycho and Kepler challenge the Earth-centered idea?

A

Copernicus created a sun-centered
model; Tycho provided the data needed to improve this model; Kepler found a model that ft Tycho’s data

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4
Q

Which astronomers challenged the Earth-centered idea?

A

Copernicus, Tycho and Kepler

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5
Q

How did Copernicus, Tycho and Kepler challenge the Earth-centered idea?

A

Copernicus created a sun-centered
model; Tycho provided the data needed to improve this model Kepler found a model that ft Tycho’s data

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6
Q

What was Galileo’s role in solidifying the Copernican revoluton?

A

His experiments and observatons overcame the remaining objectons to the Sun-centered solar system. (Tycho’s observatons of comet and supernova already challenged this idea.)

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7
Q

Using his telescope, Galileo saw:

A
  • Sunspots on Sun (“imperfectons”)
  • Mountains and valleys on the Moon (proving it is not a perfect sphere)
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8
Q

Who invented telescopes and thermometers?

A

Galileo

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9
Q

Who discovered Moon’s craters, Jupiter’s moons, phases of Venus, and stars in Milky Way?

A

Galileo

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10
Q

Kepler’s 1st law of planetary motion

A
  1. The orbit of each planet is an ellipse with the Sun at one focus
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11
Q

Kepler’s 2nd law of planetary motion

A
  1. As a planet moves around its orbit it sweeps our equal areas in equal tmes
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12
Q

Kepler’s 3rd law of planetary motion

A
  1. More distant planets orbit the Sun at slower average speeds: p^2 = a^3
    p = orbital period in years
    a = avg. distance from Sun in AU
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13
Q

Does 3-rd Kepler’s law depends on masses of planets?

A

No

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14
Q

Will a small rock and a big planet have the same period of rotaton if they happen to be at the same distance to the Sun?

A

Yes

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15
Q

Which planet is the fastest in a solar system - Mercury, Venus Mars, Jupiter? Which Kepler’s law explains it?

A

Mercury (Kepler’s 3rd law)

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16
Q

What did Copernicus conclude?

A

Copernicus concluded that Earth is a planet and that all the planets circle the Sun. Only the Moon orbits Earth

17
Q

What did Copernicus conclude?

A

Copernicus argued that the apparent motion of the Sun about Earth during the course of a year could be represented equally well by a motion of Earth about the Sun.

18
Q

Could Copernicus prove that Earth revolves about the Sun?

A

no

19
Q

Why, in Copernicus’s time there was little motivation to carry out observations or experiments to distinguish between competing cosmological theories

A

In Copernicus’ time, in fact, few people thought there were ways to prove whether the heliocentric or the older geocentric system was correct. A long philosophical tradition, going back to the Greeks and defended by the Catholic Church, held that pure human thought combined with divine revelation represented the path to truth.

20
Q

Who showed that rest is no more natural than motion.

A

Galileo

21
Q

accelerate

A

—change their speed or direction of motion.

22
Q

Galileo’s Astronomical Observations about jupiter

A
  • Galileo found four moons revolving about Jupiter in times ranging from just under 2 days to about 17 days. This discovery was particularly important because it showed that not everything has to revolve around Earth.
  • Within a few months, he had found that Venus goes through phases like the Moon, showing that it must revolve about the Sun,
23
Q

Meridian

A

a half-circle extending from your horizon due north, through your zenith, to your horizon due south

24
Q

What is a circumpolar star?

A

a star that always remains above your horizon

25
Q

You are standing on Earth’s equator. Which way is Polaris, the North star?

A

on the northern horizon

26
Q

Orion is visible on winter evenings but not summer evenings because of

A

the location of Earth in its orbit.

27
Q

He discovered that Jupiter has moons.

A

Galileo

28
Q

Kepler’s third law, p2 = a3, means that

A

all orbits with the same semi-major axis have the same period.
the period of a planet does not depend on its mass.
a planet’s period does not depend on the eccentricity of its orbit.
planets that are farther from the Sun move at slower average speeds than nearer planets.

29
Q

From Kepler’s third law, a hypothetical planet that is twice as far from the Sun as Earth should have a period of

A

more than 2 Earth years.

30
Q

Kepler’s second law, which states that as a planet moves around its orbit it sweeps out equal areas in equal times, means that

A

a planet travels faster when it is nearer to the Sun and slower when it is farther from the Sun.