Final Exam Flashcards

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1
Q

What is our solar system and its components?

A

our solar system is composed of several objects in space: moons, asteroids, our soon and Pluto

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2
Q

How have Radar and Infrared technology helped us understand other planets in our solar system?

A
  • Radar observations: Venus is a solid covered with thick clouds, Jupiter does not have a solid central portion
  • Infrared methods: temperatures of planet surfaces, chemical composition, presence of water
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3
Q

What were the goals of the following space probes:
Apollo, Voyager, Magellan, Pathfinder

A

A: mission to land man on the moon, bring back rocks for analysis and mapping of surface
V: to look at Jupiter in detail
M: mission to Venus, had to use radar map surface
P: landed on Mars for first surface investigation studied atmosphere and soils

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4
Q

What do the inner terrestrial planets have in common?

A

solid surface, core of iron, nickel, sulfur

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5
Q

Why does Mercury have such a great temperature change in one day?

A

it is close to the sun and has no atmosphere, meaning heat dissipates into space at night quickly

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6
Q

Why is Venus so hot?

A

thick atmosphere of clouds trap heat and it is mostly carbon dioxide and sulfuric acid

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7
Q

What kind of evidence do we have that Mars once had abundant water?

A
  • large erosional cavities
  • volcanoes present but not active
  • plenty of sedimentary rocks
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8
Q

Which of the outer planets is largest?

A

Jupiter

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9
Q

Describe the atmospheres of Jupiter, Uranus, and Neptune.

A

J - atmosphere of hydrogen and helium, giant red spot
S - thick atmosphere of hydrogen and helium, surface with very strong winds and large storms like on Jupiter
U - atmosphere oh hydrogen and helium, no developed storm systems, rings present but faint, in several bands

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10
Q

Describe the rings of Saturn.

A
  • three major rings, numerous smaller ones
  • some very small, other quite large
  • composition mostly of ice
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11
Q

Why are Uranus and Neptune so blue?

A

U - rocky core with liquid component of water, methane and ammonia
N - Atmosphere with much methane

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12
Q

How long does it take for Saturn, Uranus, and Neptune to orbit the sun (in Earth years)?

A

S - 29.5 earth years
U - 84 earth years
N - 165 earth years

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13
Q

What two outer planets are known for large storm systems?

A

Neptune and Jupiter

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14
Q

What is unusual of Pluto’s orbit around the sun?

A

it is very elliptical and sometimes closer to the sun than Neptune

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15
Q

Describe our moon’s orbit and revolution.

A
  • revolution around Earth every 28 days
  • rotation once each rotation; thus, same side faces us at all times
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16
Q

How does the geology of the Moon compare to Earth?

A
  • rocks very similar to Earths igneous
  • also discovered that water is present, but below the surfce
17
Q

Why are there changes in the phases of the moon (new, quarter, full)?

A

when sun and moon on same side we have a new moon, when sun and moon are on opposite sides we have a full moon

18
Q

What are the two types of eclipses?

A

Lunar and solar

19
Q

Describe a solar and lunar eclipse.

A

L - when Earth between sun and moon, moon is in shadow of Earth
S - when moon is between sun and Earth, Moon shadow is on Earth

20
Q

What is the cause of the ocean tides?

A

tides are the result of moon’s gravitational influence on Earth along with that of the sun, highest tides when earth moon and the sun are in a row

21
Q

What is the link between the moon phases and intensity of tides?

A
  • water pulled toward moon when it is over head, high tide
  • pulled toward when opposite
22
Q

Contrast Spring and Neap tides.

A

S - when the sun and moon are on the same side of Earth, the tides will be a little higher
N - when the sun and moon are not aligned high tides will be a little lower

23
Q

Describe the celestial terms Light Year, Parsec, and Astronomical Unit.

A

LY - distance light movies in one year
P - 3.26 light years
A - earth to sun distance

24
Q

What is the value of studying parallax?

A

apparent positional change of an object due to change of perspective, so we can estimate distance

25
Q

What is the value of measuring the Doppler Effect?

A

extent of change used to determine velocity of star and we can determine if it is moving toward or away from us

26
Q

Describe the celestial terms Solar System, Galaxy, and Universe.

A

U - all of space
G - cluster of stars, planets and stellar dust, galaxy which includes us is the milky way
SS - one star and its revolving objects, we have eight planets and other objects

27
Q

Describe the terms Nebula and Protostar relative to the beginnings of a star.

A

N - condensation of gases to form clouds, gravity pulls them together
P - movement of particles inward to produce an optically dense object, spinning of material, increased temperatures

28
Q

How do a Red Giant, White Dwarf, and Black Hole relate to the “life” of a star?

A
  • expansion of outside layers to many sizes to a red giant
  • release of a portion of the material remaining core shrinks to high density to become a white dwarf
  • complete collapse, extreme density and small size to become a black hole
29
Q

What is the photosphere of our Sun?

A

the source of most light we see, mostly of gasses

30
Q

Where does the Aurora Borealis have its origin?

A

seen near poles at night as the northern lights due to outburst of energy from our sun

31
Q

What is the Milky Way.

A

the galaxy that contains our solar system, including earth

32
Q
A