A2 - Lunar disk Flashcards

1
Q

What shape is the Moon?

A

oblate spheroid (wider at equator)

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2
Q

What are craters/ejecta?

A

-asteroid/comet impact locations

-material thrown outwards, forming ejecta rays around crater

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3
Q

What are maria, and how do they form?

A

-asteroid/comet impacts leave craters
-fills with lava that cools
-forms flat basaltic plain

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4
Q

What are terrae?

A

-the lunar highlands
-brighter (higher albedo), more mountainous parts of the Moon

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5
Q

What are mountains (on the Moon)?

A

rim of an impact crater

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6
Q

What are valleys? What are their alternate name?

A

-lava channel flow
-cools and contracts
-forms a valley structure

-rille

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7
Q

Draw the diagram of the Moon labelled with 3 maria, 3 craters and 1 mountain range:

A
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8
Q

What is special about the Moon’s orbital period, and how long is it?

A

-27.3 days

-its orbital period is equal to its rotational period
-ie tidally locked

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9
Q

What is libration, and why does it happen? What does it allow observers to do?

A

-apparent oscillation of the lunar disk
-happens because the Moon’s rotational axis is tilted relative to its orbital plane

-allows observers to see parts of the Moon that aren’t always visible

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10
Q

When would be the best time to observe the Sea of Tranquility and why?

A

-full Moon

-it is a mare, and a flat feature which doesn’t cast shadows
-it is best observed when fully illuminated

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11
Q

When would be the best time to observe Tycho and why?

A

-half Moon (specify the quarter it is in if asked)

-the crater has height, and casts shadows, so the added contrast when it lies along the terminator line helps observations be more detailed

-or full Moon to see its bright ejecta rays being fully illuminated

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12
Q

How do lunar eclipses show that the Earth has a curved surface?

A

-the shadow of the Earth appears curved when cast onto the Moon’s surface
-the curvature of the shadow is different to the curvature of the Moon

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13
Q

Describe a method that allows you to work out the relative size of the Moon, using a lunar eclipse:

Assume you know the Earth’s diameter and the times of each of the umbral contacts, but not the Moon’s orbital period

A

-calculate difference in time between 3rd contact and 1st contact to find how long the Moon took to cross the umbral shadow of the Earth
-do the same with the 2nd and 1st, to see how “long” the Moon is

-divide one by the other to find out their relative “lengths”, and then multiply/divide by the Earth’s diameter

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14
Q

Describe a method that can allow you to figure out the length of the lunar phase cycle:

A

-need to measure time between 2 Full Moons, use a clock to record start time and end time
-observe from same location every time

-repeat over several cycles to improve reliability

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