Earth-centred Universe Flashcards

1
Q

How long is a sidereal day and what reference frame is it in?

A

23hr 56min, A complete rotation of the Earth with respect to the stars.

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2
Q

How long is a solar day?

A

24hr, a complete rotation of the Earth with respect to the Sun.

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3
Q

What way is the celestial sphere rotating for you?

A

Anti-clockwise looking north.

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4
Q

What are the fixed points of the celestial sphere?

A

North celestial pole and the South celestial pole.

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5
Q

Where can you find the pole star?

A

At the same angle above your northern horizon as your latitude.

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6
Q

How many regions is the sky divided into today and what can they be called ?

A

88 regions known as costellations

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7
Q

What positions are used to locate celestial bodies in the sky?

A

Declination and right Ascension

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8
Q

What are the steps for scientific method?

A

-Recognize a problem, by doing observations
- Make a hypothesis
- Predict the consequences of the hypothesis
- Perform experiments to test predictions
- Find a rule that leads to a theory

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9
Q

What is the criteria for Scientific model

A

Does the model fit the data?
Model must make predictions that can be tested and that it must be possible to disprove the model.
It should require the fewest assumptions.

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10
Q

What is parallax?

A

The apparent shifting of nearby objects with respect to distant ones as the position of the observer changes.

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11
Q

What is stellar parallax?

A

The apparent annual shifting of nearby stars with respect to background stars, measured as the angle of shift.

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12
Q

What is the parallax angle?

A

Half of the angle shift measured in half a year.

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13
Q

What did the Greeks predict?

A

The Earth being spherical: during lunar eclipses the edge of the Earth’s shadow is always circular.

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14
Q

What did Aristarchus do?

A

First person to propose the new heliocentric idea and estimated sizes of the Moon and Sun.

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15
Q

What was the purpose of Ptolemy’s geocentric model?

A

To account for the positions of all heavenly bodies.

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16
Q

What was Ptolemy’s model?

A

The sun, moon and 5 planets went round uniformly in circular orbits, called epicycles, whose centres moved uniformly around large circles (deferents) centred on the Earth.