Objectives Flashcards

(40 cards)

1
Q

What is the origin of the names of the days of the week?

A

7 Heavenly bodies which wander relative to fixed background stars. (Sun, Moon, Mars, Mercury, Jupiter, Venus, Saturn)

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2
Q

Parallax

A

An apparent change in position of an object due to an actual change in position of the observer.

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3
Q

Geocentric

A

An earth centered system

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4
Q

Heliocentric

A

A sun-centered system

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5
Q

Retrograde Motion

A

Planets seem to periodically reverse the direction of their wandering in the sky as the Earth passes by them in orbit with a greater velocity.

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6
Q

What is the diameter of the Earth?

A

Approximately 8,000 miles

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7
Q

Eratosthenes

A

Best early determination of Earth’s size

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8
Q

Ptolemy

A

Used epicycles to explain retrograde motion in geocentric system

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9
Q

Copernicus

A

Made 3 proposals which started Modern Astronomy

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10
Q

Tycho Brahe

A

Great Observer

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11
Q

Kepler

A

Formulated 3 famous laws. Worked w/Tycho

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12
Q

Galileo

A
1st to—
•point telescope towards heavens
•see mtns & craters on moon
•detect 4 largest moons of Jupiter
•phases of Venus
•sunspots
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13
Q

3 Proposals made by Copernicus (and their implications)

A
  1. Stars are stationary. —>Earth rotates once daily.
  2. Sun is center of universe —>Earth revolves once yearly.
  3. Heavenly bodies move in perfect circles at constant speeds. —>epicycles only needed to account for variable speeds.
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14
Q

Distinguish between rotation and revolution

A

Rotation—spin around axis

Revolution—orbit around a body/focus

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15
Q

6 Proofs that Earth rotates

A
  1. Satellites in low Earth orbits change positions relative to Earth’s surface on each pass b/c satellite maintains original path while Earth rotates beneath it.
  2. Foucault pendulum
  3. Oblate spheroid shape of Earth.
  4. Falling objects fall to the East.
  5. Moon approaches at 600mph at moonrise; recedes at same rate at moonset.
  6. All weather formations are rotating. Effect of Coriolis forces.
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16
Q

Proofs of revolution

A
  1. Stellar Parallax. (The stars make little aloops.)
  2. Aberration of Starlight. Astronomers must tilt telescope to compensate for Earth’s rotational orbit.
  3. Certain stars approach us at one time, 6mo later receding.
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17
Q

Distinguish: Solar day & Sidereal day

A

Solar day: Measured w/respect to sun. 24hrs long.

Sidereal day: Measured w/respect to stars. (4min less)

18
Q

Earth’s precessional angle

A

23.5° from vertical plane of orbit

Polaris is current N star

Seasons are result

19
Q

Significance of Tropics of Cancer and Capricorn

A

Tropic of Cancer: Most N line on Earth’s surface where Sun rays hit vertically.

Tropic of Capricorn: Most S line where Sun directly overhead.

20
Q

Arctic and Antarctic Circles

A

Arctic Circle: most S line in N hemisphere which can have sunlight for full 24hrs.

Antarctic Circle: most N line in S hemisphere that gets sunlight for full 24hrs.

21
Q

Day, week, month, and year in astronomical terms.

A

Day: One rotation of Earth

Week: Possibly b/c 7 heavenly wanderers

Month: Moon’s revolution once around Earth

Year: One revolution of Earth around sun

22
Q

Newton’s law of gravitation

A

F= (GMeMs)/(r^2)

23
Q

4 Proofs that Earth is approx. spherical

A
  1. If flat—> objects moving away would only get smaller. B/c Earth has curvature—>objects slowly disappear over horizon.
  2. Shadow of Earth on moon is circular during an eclipse.
  3. Magellan’s voyage around world
  4. Pictures from space
24
Q

Diameter of moon; distance to moon

A

2140; 240,000mi

25
One lunar day from sun rise to sunset in terms of earth time.
One earth month
26
Why does size of moon vary over 2 weeks?
Elliptical orbit
27
Density of moon
3.3 g/cc
28
Does the moon have a magnetic field?
No, the moon has no magnetic field.
29
Moon has same rate of rotation and revolution because it is
Tidally locked to the earth.
30
Spring Tides
* When high tide occurs at the time of New Moon, sun and moon pull together to form high tide (higher than average). * Also occur at Full Moon
31
Neap Tides
* Lower than average high tide * during 1st & 3rd quarters * Moon forms high tide, while sun forms high rude where moon causes low. Work against each other.
32
Why don't eclipses occur monthly?
Because there is a 5° angle between the orbital plane of Earth and orbital plane of the moon.
33
Annular eclipse
Moon is lined up w/Sun but ring of light peeks out from behind. Happens when moon is farther from earth in orbit.
34
Total eclipse
When moon entirely blacks out sun. | Happens when moon is closer in orbit.
35
Relation between moon's lack of limb darkening and surface.
Moon has no limb darkening b/c rough surface edges of moon cause it to not be noticeably dimmer. (Rough surface also indicates low reflectivity.) Rough on large scale: mtns. & craters Small scale: dust
36
How was it possible to predict the Moon has no atmosphere?
•low gravitational pull. •Low temps @night; high temps @day -atmosphere would act as blanket and reduce extremes -Kinetic theory of gases, gas molecules in high daytime travel faster then moon's escape V 1.7mi/s
37
2 major theories for origin of lunar craters
1. Most Impact craters: when large objects fall onto moon. | 2. Some Volcanic activity
38
Probable origin of lunar maria
* Large impact craters causes by objects hitting the moon when subsurface material was molten. * Molten labs flowed out through hole and covered most existing craters.
39
4 Ways Moon May Have Originated
1. Adopted—formed elsewhere captured in Earth's orbit. 2. Twins—formed & evolved alongside of Earth. 3. Birth—Once a part of Earth. Moon density = Earth's crust density. 4. Catastrophic collision between early Earth and 2nf object size of Mars. (Current Accepted Theory) - Moon composition same as Earth in certain isotopes, but NOT match any bodies in solar system.
40
How were the relative age of craters determined?
Most recent—Copernican age. Freshly pulverized rocks are white. Ray material must be most recently deposited since it covers everything undisturbed.