Earth and its Motions (Pres III) Flashcards

1
Q

What are the two hierarchies of motion?

A

1) Diurnal Rotation - days & nights ( ~23h 56m 4s)

2) Annual Revolution - seasons ( ~365.25 days)

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2
Q

What is Kepler’s 1st law?

A

Orbits of all planets are ellipses w/ sun located at foci of the ellipses

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3
Q

Why are the orbits ellipses?

A

Because the planets are made of many different materials, the gravity is not uniform, resulting in elliptical orbits.
If the earth was made on a single material, the orbit would be spherical

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4
Q

What is Kepler’s 2nd law?

A

The area swept out by the radius vector “r” is constant for a given time period. Remember elliptical drawing with shaded areas*
The areal vector is constant
Areal velocity: area of ellipse/period
Consequence: planets go faster when closer to the sun

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5
Q

What is Kepler’s 3rd law?

A

The squares of the sidereal orbital periods of the planets are in direct proportion to the cubes of the semimajor axes of their orbits

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6
Q

What is Newton’s First Law?

A

An object at rest tends to stay at rest and an object in motion tends to stay in motion with the same speed and in the same direction unless acted upon by an unbalanced force (Law of inertia)

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7
Q

What is Newton’s Second Law?

A

The acceleration of an object as produced by a net force is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the object

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8
Q

What is Newton’s Third Law?

A

For every action, there is an equal and opposite reaction

action and reaction forces

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9
Q

What is Newton’s Law of Universal Gravitation?

A

Every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them

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10
Q

Why are Kepler’s Laws assumptions

A

Because they assume gravity is uniform, which is not true. Forces such as solar winds, air resistance, and gravity of other bodies affect the gravity field

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11
Q

How much is Earth’s axis tilted

A

23.5 degrees

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12
Q

What is the solar day?

A

Period of rotation about spin axis w/respect to the sun = 24 hours

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13
Q

What is the sidereal day?

A

Period of rotation about spin axis w/respect to the fixed stars = 23h 56m 4.09s

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14
Q

What is the solar period?

A

Time of orbital revolution of a planet with respect to the sun

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15
Q

What is the sidereal period?

A

Time of orbital revolution of a planet with respect to the “fixed” stars

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16
Q

What is the synodic period?

A

From the time celestial bodies align to the next time they align

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17
Q

What is the solar year?

A

Period of orbital motion w/respect to the sun ~ 365 days, 5h, 48m, 45.51s

18
Q

What is the sidereal year?

A

Period of orbital motion w/respect to the fixed stars
~ 365.2564 … solar days
~ 366.2564 … sidereal days

19
Q

Ecliptic

A

The path of the Earth’s orbit

20
Q

Equinox

A

Direction in space coinciding with the intersection of the Earth’s equatorial plane with the ecliptic

21
Q

Solstice

A

Occasion when sun reaches the tropics
Summer solstice - tropic of cancer
Winter solstice - tropic of capricorn

22
Q

What is precession?

A

The Earth’s wobble

latin - forward shifting

23
Q

Who was instrumental in understanding precession?

A

Hipparchus - discovered in 2nd century BC
Copernicus - first ascribed as motion of axis
Newton - first explained properly

24
Q

Why does precession happen?

A

Because of the torque of unequal pull on the equatorial bulges of surrounding gravity bodies (sun, moon, planets)
If the earth was a sphere, the would be no precession

25
Q

What is the period of precession?

A

Platonic year ~25,765 years

26
Q

What are the requirements for precession?

A

1) Planet spinning on rotation axis in space
2) Source of gravitational attraction
3) Non-spherical shape
4) Inclination of equator to plane of orbit (obliquity of the ecliptic)

27
Q

What is Lunisolar Precession?

A

The moon is responsible for 2/3 of precessional motion

The sun is responsible for 1/3 of precessional motion

28
Q

Planetary precession

A

Other planet’s effect on precession

29
Q

General Precession

A

Lunisolar and planetary precession combined

30
Q

What are the season determined by?

A

Obliquity of orbit

Orbital period

31
Q

What has to be corrected for precession?

A

Calendar year

32
Q

What is nutation?

A

Periodic variations in precessional motion

33
Q

When was nutation discovered?

A

In 1747 by Bradley

34
Q

What 3 things cause it to happen?

A

1) Ellipticity of earth’s orbit
2) Ellipticity of moon’s orbit
3) Non-coincident of moon’s orbit w/ ecliptic inclination: 5 degrees 11 seconds

35
Q

What is the main period of nutation?

A

18.6 years

36
Q

What is the wobble of Polar Motion?

A

The push of the earth’s wobble against it’s crust, which causes changes in latitude

37
Q

What probably causes polar motion?

A

That the earth is not completely solid

38
Q

How long does polar motion take to complete a cycle?

A

~ 428 days

39
Q

Who calculated the mean position of the rotational pole?

A

The Conventional International Origin (CIO) in 1903-1905

40
Q

What is happening to the Length of the Day?

A

It’s changing slowly over time

Increased velocity = shorter day

41
Q

What is causes changes in day length

A

Interactions of atmosphere, oceans, winds, inner parts of earth being non-rigid