Chapter 16 Earth and Moon Flashcards

1
Q

Define time and describe location on the surface

Causes season

A

Earth’s Movement

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2
Q

Yearly revolution about the sun
Daily rotation about its axis
Clockwise wobble of its rotation axis

A

Motion of Earth

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3
Q

Not circular
2.5 million km closer in January
2.5 million km more distant in July
Earth receive about 6% more solar energy in January

A

Elliptical orbit

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4
Q

Earth’s rotation axis inclined at…

A

23.5 degrees

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5
Q

Line on celestial sphere above earth’s equator

A

Celestial Equator

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6
Q

Pendulum oscillates in fixed direction

Orientation changes as earth rotates

A

Foucault pendulum

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7
Q

Deflection of path as earth rotates beneath moving objects

A

Coriolis effect

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8
Q

Changes direction of rotation axis on celestial sphere

Reaction of earth to gravitation pull on its equatorial bulge by the moon and sun

A

Precession

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9
Q

Intersection of two straight lines
Won’t work for earth’s curved surface

Identifying place

A

Position on flat surface

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10
Q

Intersection of parallels and meridians defined with respect to rotation axis
Parallels: Latitude
Meridians: longitude

Identifying place

A

Position on earth

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11
Q

Time standards depend on measuring…

A

Intervals between evenly spaced periodic events

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12
Q

Viewed from above North Pole
Earth revolves counterclockwise about the sun and rotates in the same direction
Sun rises in the east and sets in the West

A

Earth_Sun Motion ( daily time)

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13
Q

Time at which the sun is at the celestial meridian

A

“Noon”

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14
Q

Given by position of sun in the sky

Can be measures with gnomon or sundial

A

Apparent local star

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15
Q

Time averaged from apparent solar time

A

Mean solar time

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16
Q

Interval Between two consecutive crossings of celestial Meridian by a particular store
Little variation because of earth’s constant rotational rate

A

Sidereal Day

17
Q

Interval between two consecutive crossings of the celestial Meridian by the sun
About 4 minutes longer than sidereal day

A

Apparent solar day

18
Q

360 degrees of longitude divided into 24 15 degree zones

A

Standard time zones

19
Q

Clocks sit in the hate in spring and back in the fall for one extra hour of sunlight during summer evenings

A

Daylight saving time

20
Q

The 180° meridian

Designated to correlate days with 24 hour time zones

A

International dateline

21
Q

Intocable between two consecutive spring equinox

A

Tropical year

22
Q

About 20 minutes longer than the tropical year

A

Sidereal year

23
Q

Orbital time measured with respect to the stars

27 1/3 days

A

Sidereal month

24
Q

Time interval between two consecutive phases

29 1/2 days

A

Synodic month

25
Q

Characterized by craters lunar highlands and Maria
Subject of 12 Apollo missions
380,000 km distant

A

The moon

26
Q

Origin stage formed from material eject it from a collision of a large object with her

A

Stage 1

27
Q

Molten surface stage molten surface 100 km deep to hundred million years after formation
Heating from Solar System debris impacts

A

Stage 2

28
Q

Molten interior stage
Accumulated heat from radioactive decay
Began 3.8 million years ago

A

Stage 3

29
Q

Cold and quiet stage

Cypress scared by micrometeorites in meteorites

A

Stage 4