LECTURE 2 Flashcards

1
Q

How is our sun moving in the galaxy?

A

The sun moves in a random pattern and at a speed of 70,000km/h
The sun orbits the Milky Way once every 230 million years
The suns’ speed of rotation around the galaxy is 800,000km/h

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2
Q

The angle which Earth is tilted towards

A

23.5 degrees

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3
Q

In which direction does Earth rotate

A

From West to East
Counterclockwise

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4
Q

How do galaxies move within the universe?

A

Of the galaxy as baking bread with raisins in it, the raisins do not increase in size but the distance between the raisins will increase as the size of the bread increases

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5
Q

Who discovered that the universe is expanding?

A

Vesto Slipher 1917
Carl Wirtz 1918
Knut Lundmark 1920
Edwin Hubble 1929

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6
Q

How is Earth moving in our solar system?

A

Rotates on its axis once a day
Orbits the sun at a distance of 1AU

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7
Q

Scientific Thinking

A

everyday ideas of observation and through trial and error experiences

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8
Q

What did ancient civilizations achieve in astronomy?

A

Tracking the seasons
Daily timekeeper
Calendar
Monitoring lunar cycles
Monitoring planets and stars
Predicting eclipses

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9
Q

How did astronomical observations benefit ancient societies?

A

Keeping track of time and seasons
- Agriculture

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10
Q

The Nebra Sky Disk

A

1800-1600BC
Contains symbols for the Sun or full moon
The Crescent Moon
Pleiades (group of stars)

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11
Q

Crab nebula

A

65000 LY away
Observed in 1054 by Chinese Astronomers

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12
Q

Why does modern science trace its roots to the Greeks?

A

Developed models of nature and emphasized that the predictions of models should agree with observations

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13
Q

How did the Greeks explain planetary motion?

A

Earth is at the centre of the universe
Heavens must be perfect Objects moving on perfect spheres

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14
Q

Ptolemaic Model

A

Sufficiently accurate remain in use for 1,500 years

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15
Q

Ptolemaic Model

A

EACH PLANET MOVE ON A SMALL CIRCLE WHOSE CENTER MOVES AROUND EARTH ON A LARGER CIRCLE

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16
Q

Aristarchus Samos

A

310-230 BC
Proposed model of the solar system
Estimated size and distance of the sun and the moon

17
Q

Nicolaus Copernicus

A

Proposed a Sun-centred model (1543)
Used model to determine the layout of the solar system

18
Q

Tycho Brahe

A

The most accurate naked eye ever made of planetary positions
Thought that Earth is at the center of the solar system but recognized that other planets go around the sun

19
Q

Johannes Kepler

A

tried to match Tycho’s observations with circular orbits
8 arcminute discrepancy led him eventually to ellipses

20
Q

What is an ellipse?

A

An elongated circle (oval)

21
Q

Kepler’s First Law

A

1609
The orbit of each planet around the Sun is an ellipse with the sun at one focus

22
Q

Kepler’s second law

A

1609
As a planet moves around its orbit it sweeps out equal areas at equal times

23
Q

Kepler’s third law

A

1619 The farther a planet is from the sun the slower its orbital speed is and vice versa

24
Q
A