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Astronomy190 - Topics in Astronomy
Astronomy and Astrobiology
Lecture 6 : Atmospheric Science
Ty Robinson
Questions of the Day• How do atmospheres help make a world
habitable?
• Why/how do the compositions of the atmospheres of Mars, Venus and Earth differ?
• How does the greenhouse effect work to warm a world’s surface?
• What factors affect the ability of a world to maintain its atmosphere?
Questions?What would happen to Earth’s oceans if we did not have an atmosphere?
our oceans would sublimate
the oceans will remain liquid, but expand
our oceans would freeze through
nothing
Earth’s Atmospheric Composition
Gas Amount [%]Nitrogen 78
Oxygen 21
Water 1 - 4
Carbon Dioxide 0.04
Methane 2 x 10-4
Ozone 7 x 10-6
Venus, Earth and Mars
Surface Pressure [bars] 0.01 1 100
Composition [%]
Nitrogen 3 72 3
Oxygen 0.1 21 0
Water 0.03 1 - 4 0.01
Carbon Dioxide 95 0.04 97
Methane ? 2 x 10-4 0
Ozone 0 7 x 10-6 0
Earth’s Atmospheric Structure : Troposphere
Lapse Rate8º C per km
Questions
What happens to water vapor
as you lift it higherinto the
atmosphere?
Why is the surface the
warmest part of the troposphere?
Absorption of solar radiation at
the surface
The gas cools andcondenses toform clouds.
Earth’s Atmospheric Structure : Stratosphere
QuestionWhy does the temperature
increase with height in the
stratosphere?
UV light
O3
O2O
(absorption)
Earth’s Atmospheric Structure : Mesosphere
How do thestructure and composition of
the atmosphere determine surface
conditions?
Transmission/Absorption of UV and Vis Light
(Sun)
Ozone Layer
Cloud
Cloud
Surface
In the UV and visible…
(heating)
(heating)
(scattering)
(scattering)
Albedo
(Bolometric) Albedo = Reflected Light / Incident Light
Albedo 0.15 0.37 0.65
Now for the infrared (IR)…
Effective
Temperature [ºC]
-55 -17 -43
4πR2σTe4 = S(1-A) πR2
Greenhouse Gasses
Transmittance : how wella gas transmits radiation
Low transmittanceimplies the gas is a
good absorber
Important greenhousegasses (on Earth):
H2OCO2
O3
CH4
Greenhouse Effect I
In the infrared…
Ozone Layer
Cloud
Cloud
Surface
(absorption)
(absorption)
(absorption)
(absorption)
(emission)
Greenhouse Effect II
In the infrared…
Ozone Layer
Cloud
Cloud
Surface
(emission)
(emission)
(emission)
(absorption)
(emission)
Surface Temperatures
Effective
Temperature [ºC]
-55 -17 -43
Surface
Temperature [ºC]
-50 15 470
Greenhouse
Warming
[ºC]
5 32 513
Questions?What factor(s) determine a world’s ability to retain an atmosphere?
temperature, gravity, magnetic field and atmospheric composition
planetary composition
gravity and atmospheric composition
magnetic field
Gas Escape I
gravity
velocityEach molecule in Earth’s upper atmosphere has a velocity (whichdepends on its mass and surroundingtemperature). If this velocity is large enough, a molecule can escape Earth’s gravity.
Earth’s magnetic field prevents theSolar wind from stripping away our atmosphere.
Gas Escape II
Mercury: weak magnetic field, low gravity, high temperature : no atmosphere
Venus: no magnetic field, high gravity, relatively high temperature : thick atmosphere even after a great deal of gas has escaped
Moon: no magnetic field, low gravity, same distance from the Sun as Earth : no atmosphere
Gas Escape IV
Question
Why does Mars have such a thin atmosphere?
Massive impacts can also drive off atmospheric gasses, especially on worlds with low gravity.
Questions of the Day• How do atmospheres help make a world
habitable?
• Why/how do the compositions of the atmospheres of Mars, Venus and Earth differ?
• How does the greenhouse effect work to warm a world’s surface?
• What factors affect the ability of a world to maintain its atmosphere?
Quiz
1 - Consider two stacked sedimentary layers. The lower layer has been determined to be 1.5 Gyrs old. Most likely, how was this age determined? What can we deduce about the upper layer?
2 - Describe the different processes that can affect visible radiation as it passes through Earth’s atmosphere.
3 - What is one thing you did not understand from today’s lecture?