Chapter 10 pt. 2 Flashcards

(29 cards)

1
Q

What are 3 Sources of Gas

A
  • Out-gassing from volcanoes
  • evaporation of surface liquid; sublimation of surface ice
  • Impacts of particles and photons
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2
Q

What are 5 Losses of Gas

A
  • Thermal escape of atoms
  • Sweeping by solar wind
  • Condensation onto surface
  • Chemical reactions with surface
  • Large impacts blasting gas into space
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3
Q

Thermal Escape

A

When heating of an atmosphere allows molecules to escape

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4
Q

Does the Moon and Mercury have any atmosphere?

A

Yes, but they are very thin

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5
Q

What is the Moon’s exosphere like?

A

it extends high above it’s surface

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6
Q

What is Mercury’s exosphere like?

A

Much of it is escaping

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7
Q

Does the Moon and Mercury have polar ice craters?

A

Yes

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8
Q

What is Mars like?

A
  • Cold
  • Dry
  • Frozen
  • Strong seasonal changes cause CO2 to move from pole to pole creating dust storms
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9
Q

How does Mars’ orbit effect it’s seasons

A

The ellipticity of Mars’s orbit makes seasons more extreme in the southern hemisphere

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10
Q

What are the polar ice caps of Mars like?

A
  • Residual ice of the south polar cap remain during the summer is mostly water ice
  • Carbon dioxide ice of polar cap sublimates as summer approaches and condenses at the opposite pole
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11
Q

What are the dust storms on Mars like?

A
  • Seasonal winds drive the dust storms
  • Dust in the atmosphere absorbs blue light, makes the sky brownish-pink
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12
Q

What is the range of Mars’ tilt?

A

0 to 60 degrees

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13
Q

How does Mars’ tilt affect the planet?

A
  • Causes climate changes
  • Alternating layers of ice and dust show this
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14
Q

What is the history of climate change on Mars?

A
  • Has not had widespread surface water for 3 billion years
  • Greenhouse Effect probably kept the surface warmer before that
  • Somehow lost most of its’ atmosphere
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15
Q

What about Mars’ atmosphere?

A
  • Magnetic field may have preserved its’ early atmosphere
  • Solar wind may have stripped atmosphere after field decreased because of interior cooling
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16
Q

What is the atmosphere of Venus like?

A
  • Thick carbon dioxide atmosphere
  • surface pressure 90x that of Earth
  • Slow rotation produces very weak Coriolis Effect
  • Little weather
17
Q

The Greenhouse Effect on Venus

A

Thick carbon dioxide atmosphere produces very strong greenhouse effect

18
Q

How did Venus get so hot?

A
  • Reflective clouds w sulfuric acid
  • The upper atmosphere has fast winds that remain unexplained
19
Q

Runaway Greenhouse Effect

A

a planet’s atmosphere traps so much heat that its surface temperature rises uncontrollably, leading to a planet becoming uninhabitable
(Venus)

20
Q

What is the main reason Venus is hotter than Earth?

A

Greenhouse effect is much stronger on Venus that on Earth

21
Q

How did Earth’s atmosphere end up so different?

A
  • We have oceans that can dissolved atmospheric carbon dioxide, trapping it in rocks
  • Ultraviolet light can break up o2 molecules allowing the ozone to form
22
Q

Why does Earth’s climate stay relatively stable?

A

The carbon dioxide cycle

23
Q

What are the consequences of Earth changing its tilt?

A
  • May lead to ice ages
  • Widespread ice tends to lower global temperatures by increasing Earth’s reflectivity
24
Q

What is current CO2 concentration looking like?

A

The highest it’s been in at least 500,000 years

25
What are the consequences of Climate Change?
- Storms are more numerous + intense - Rising ocean levels - Melting Glaciers - Availability of fresh water
26
How did Earth become so different?
Temperatures are just right for oceans of water. Oceans keep most C O2 out of atmosphere. Nitrogen remains in the atmosphere. Life releases some oxygen into atmosphere
27
Why does Earth's climate stay relatively stable?
Carbon dioxide cycle acts as a thermostat
28
How is human activity changing our planet?
Destruction of ozone High rate of extinction Global warming from the production of greenhouse gases
29