Earth, Moon, Sun interactions Flashcards

1
Q

Why do the sun and the moon appear to be the same size in the sky?

A

Because the angular size of the Sun and the Moon are exactly the same from the Earth (coincidence).

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2
Q

Why do we not have a total solar eclipse every month?

A

The Ecliptic and the plane of Moon’s orbit around Earth are different.

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3
Q

Describe a total solar eclipse.

A
  • Occurs at new moon.
  • The Moon passes directly in front of the Sun.
  • Light from the Sun’s photosphere obscured if observer is in the umbra.
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4
Q

What are Bailey’s Beads?

A
  • Small bright spots of sunlight caused by Sun’s rays shining through valley’s on the Moon
  • At the beginning and end of totality.
  • Diamond ring effect.
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5
Q

Describe a partial solar eclipse.

A

Moon only partly obscures light from the Sun. i.e. Earth’s surface lies in penumbra.

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6
Q

What is a lunar eclipse?

A
  • Occurs at full moon
  • When Earth passes between Sun and Moon.
  • Moon given reddish glow.
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7
Q

What type of eclipse is most common and why?

A

A lunar eclipse because it is visible from most of the Earth’s Night Side.

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8
Q

Why does the Moon appear red during a Lunar eclipse?

A

Because “blues bend best.”

Light from the Sun is refracted by the Earth’s atmosphere.

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9
Q

In which direction does the Earth spin?

A

From west to east

Anticlockwise when observed looking down on the North Pole.

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10
Q

What is a Sidereal Day?

A
  • The actual time it takes for Earth to spin 360 degrees on its axis.
  • The time taken for successive crossings for a given star across the observer’s meridian.
  • It is 23h 56 min and 4.1 seconds.
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11
Q

What is a Solar Day?

A
  • This is exactly 24 h
  • the time taken for successive crossings of the Sun across the Observer’s Meridian
  • An extra 4 minutes is needed because the Earth has move slightly in Its orbit around the Sun.
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12
Q

Name the Aurorae.

A
Aurora Borealis (Northern Lights)
Aurora Australis (Southern Lights)
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13
Q

What causes the Aurorae?

A
  • Electrons in the Solar Wind are accelerated by the Earth’s magnetic field at the poles.
  • Atoms of Nitrogen and Oxygen in the upper atmosphere become excited.
  • As they de-excite they emit particular wavelengths of light.
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