Ch 9+10 Flashcards

1
Q

Why is it hard to tell depth on the moon?

A

You expect to see shades of shadows on a gray scale, but in reality it’s only black and light.

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2
Q

Moon Composition

A

Highlands (83%), Mare/Maria – flat plains of basaltic lava (17%)

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3
Q

How do craters form?

A

Crater hits, “comes out”, and particles fall back into hole that was made

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4
Q

Cold Traps on Moon

A

Where the sun’s rays never shine (poles of moon) ice in crater is unmelted

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5
Q

Highlands on Moon

A
  • Made of relatively low-density rock that solidified on the cooling Moon
  • Extremely heavily cratered, bearing scars of billions of years of impacts
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6
Q

Maria

A

-dark colored basalt (volcanic lava) laid down in volcanic eruptions years ago

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7
Q

Moon’s Surface

A
  • fine grained soil of tiny, shattered rock fragments

- upper layers are porous with loosely packed dust

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8
Q

Impact Craters

A

Regardless of size or angle of impact, they are roughly round & circular

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9
Q

Formation of Impact Craters

A

(1) Impact occurs
(2) Projectile vaporizes and a shock wave spreads through the lunar rock
(3) Ejecta are thrown out of the crater
(4) Most of the ejected materials fall back to fill the crater, forming an ejecta blanket

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10
Q

Fission Theory

A

Moon was once part of Earth, but somehow separated from it early in history

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11
Q

Sister Theory

A

The Moon formed together but independent of Earth

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12
Q

Capture Theory

A

The Moon formed elsewhere in the solar system and was captured by Earth (least likely theory)

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13
Q

Avg Distance of Mars from the Sun

A

227 million kilometers (1.52 AU)

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14
Q

Avg Distance of Venus from the Sun

A

108 million kilometers (0.72 AU)

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15
Q

Appearance of Venus

A
  • Appears very bright, featureless white ball
  • Goes through phases like Moon
  • Planet’s surface not visible b/c of dense clouds that reflect 70% of sunlight
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16
Q

Appearance of Mars

A
  • Distinctly red due to iron oxides in soil
  • Bright polar ice caps
  • Dusky surface markings that sometimes change in outline and intensity
17
Q

Venu’s Surface

A

Lowland lava plains (75%)

18
Q

Impact Craters on Venus

A
  • Gertrude Stein: Triple impact crater
  • Mrs. Piggy Corona
  • Mead: Largest crater
19
Q

Atmosphere of Venus

A
  • CO2 (96%) then N2 – overall very dry atmosphere, absence of water
  • Huge troposphere
  • Almost 800 K on surface
20
Q

Polar Ice Caps on Mars

A

Mars has 2 year orbit so polar ice caps from 6 month long winter in each hemisphere

21
Q

Percival Lowell

A

A french astronomer that described what he saw on Mars as channels, but were mistranslated to canals (man-made)

22
Q

Mariner 9

A

1971, first spacecraft to orbit another planet, mapping entire surface of mars

23
Q

Twin Viking Spacecrafts

A

1970s, two orbiters surveyed planet and relayed communications for two landers on the surface

24
Q

Mars Global Surveyor (MGS)

A
  • 1997, took high-resolution photos of entire surface for more than one martian year
  • Discovered gullies apparently cut by surface water
25
Q

Odyssey

A

Discovered large amount of subsurface hydrogen

26
Q

Pheonix

A

-2008, measured water ice in the soil

27
Q

Curiosity

A

2011, goals include investigations of climate, geology, assessment of habitability of past and present Mars

28
Q

Atmosphere of Mars

A
  • Avg surface pressure of only 0.007 bar
  • CO2 (95%), N2 (3%), Argon (2%)
  • Winds can reach high speeds but exert much less force than wind on Earth b/c thin atmosphere
29
Q

Runaway Refrigerator Effect

A

Mars is smaller planet, lower gravity, more and more atmosphere escaped into atmosphere – Mars became cold most of water froze out – further reduced ability to retain heat