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Angular Momentum in Planetary Atmospheres Buffalo Astronomical Association May 8, 2009 Jude S. Sabato Assistant Professor of Earth Science Buffalo State College

Angular Momentum in Planetary Atmospheres

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Angular Momentum in Planetary Atmospheres. Buffalo Astronomical Association May 8, 2009 Jude S. Sabato Assistant Professor of Earth Science Buffalo State College. Outline. Overview of p lanetary atmospheres Angular momentum in rotating atmospheres - PowerPoint PPT Presentation

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Page 1: Angular Momentum in Planetary Atmospheres

Angular Momentum in Planetary Atmospheres

Buffalo Astronomical AssociationMay 8, 2009

Jude S. SabatoAssistant Professor of Earth Science

Buffalo State College

Page 2: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 3: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 4: Angular Momentum in Planetary Atmospheres

Planetary Atmospheres

Atmospheres we’ll talk about today…

• Earth• Mars• Venus• Titan (Saturn’s largest moon)• Jupiter

Page 5: Angular Momentum in Planetary Atmospheres

Planetary AtmospheresObject Composition

(“dry”)Condensibles Surface

PressureSurface Temperature

Atmospheric Dynamics

Venus 97% CO23% N2

SO2H2SO4

90,000 mbar 750 K Super-rotating

Earth 78% N221% O21% Ar

H2O 1000 mbar 288 K Hadley CellsJet StreamsMonsoons

Mars 96% CO22.5% N21.5% Ar

CO2H2O (trace)

10 mbar 220 K Hadley CellsJet StreamsDry Monsoons?

Jupiter 90% H210% He

NH3H5NSH2O?

No solid surface

165 K (at 1000 mbar)

Multiple jetsMacroturbulence

Titan 100% N2 CH4 1500 mbar 95 K Global Hadley CellSuper-rotationMethane cycle

Page 6: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 7: Angular Momentum in Planetary Atmospheres

Momentum

Momentum measures motion and mass:

momentum = mass x velocity

Page 8: Angular Momentum in Planetary Atmospheres

Momentum

Newton’s First Law: “An object at rest will remain at rest and an object in motion will move in a straight line at constant speed,

unless acted on by a force.”

force = change in momentum

Page 9: Angular Momentum in Planetary Atmospheres

Momentum

Page 10: Angular Momentum in Planetary Atmospheres

Angular Momentum

Angular Momentum measures spinning motion:

Angular Momentum = radius x mass x velocity

Page 11: Angular Momentum in Planetary Atmospheres

Angular Momentum

Newton’s First Law (revisited): “An object that is not spinning will remain so and a spinning object will

continue spinning at constant speed and in the same orientation, unless acted on by a twisting force

(torque).”

torque = change in angular momentum

Page 12: Angular Momentum in Planetary Atmospheres

Angular Momentum

Page 13: Angular Momentum in Planetary Atmospheres

Let’s break down the atmosphere into symmetric and wavy components…

Atmospheric Angular MomentumJet Streams and Storms

Flow variable (Wind, Temperature, Pressure, etc.)

Symmetric part Wavy part

= +Symmetric part

conserves its angular

momentum…

…if there are no waves

Page 14: Angular Momentum in Planetary Atmospheres

Take home points:• Atmospheric angular momentum is conserved

if 1. There are no torques on the atmosphere2. There are no atmospheric waves

• Atmospheric waves open the door to super-rotation

• angular momentum transfer associated with atmospheric waves can generate E-W jets

Atmospheric Angular Momentum

Page 15: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 16: Angular Momentum in Planetary Atmospheres

EarthThere are so many interesting dynamical

phenomena in Earth’s atmosphere!We’ll focus on the Hadley Circulation and Jet

Streams…• Hadley Cells Driven by low latitude convection• Hadley Cells approximately conserve angular

momentum• Angular momentum conservation means fluid

moves in rings around the planet – not at all true!

Page 17: Angular Momentum in Planetary Atmospheres

Earth

Page 18: Angular Momentum in Planetary Atmospheres

Earth

Page 19: Angular Momentum in Planetary Atmospheres

Earth

Page 20: Angular Momentum in Planetary Atmospheres

Earth

• Angular momentum conservation in the Hadley Cell generates a subtropical Jet Stream– Subtropical jet is unstable and becomes wavy– These atmospheric waves (midlatitude storms)

can sometimes generate a second jet stream

Page 21: Angular Momentum in Planetary Atmospheres

Earth

Page 22: Angular Momentum in Planetary Atmospheres

Monsoons by angular momentum too!

After Bordoni and Schneider 2008,

Nature Geoscience

Page 23: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 24: Angular Momentum in Planetary Atmospheres

MarsMars has a Hadley Circulation too…• Driven by convection• Much greater degree of angular momentum conservation,

however…• Angular momentum conservation means fluid moves in

rings around the planet – probably not true for Mars either– Jet stream is unstable and becomes wavy (still true for Mars)– Atmospheric waves (midlatitude storms) do not generate a

second jet because the planet is too small– Topography/surface heating can force waves that move the

atmospheric angular momentum from place to place

Page 25: Angular Momentum in Planetary Atmospheres

Mars

Page 26: Angular Momentum in Planetary Atmospheres

Mars

• Mars topography/surface thermal inertia may have an “elevated heat island” effect

• Elevated heat island drives Indian Monsoon (maybe, or better partially)

• Is there a “dry monsoon” on Mars?

• One way or another the atmosphere is not “moving in rings” (transport properties are not axisymmetric)

Page 27: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 28: Angular Momentum in Planetary Atmospheres

Venus

Venus in the ultraviolet

Page 29: Angular Momentum in Planetary Atmospheres

VenusVenus’ atmosphere appears to be super-rotating…

Super-rotation: winds aloft at the equator are faster than the planet’s rotation

This is akin to stirring a cup of coffee and observing that the coffee is circulating faster than your spoon!

Page 30: Angular Momentum in Planetary Atmospheres

Titan

Titan in the infrared

Page 31: Angular Momentum in Planetary Atmospheres

Titan

• Titan has a global Hadley Cell

• Titan’s upper atmosphere is in a state of super-rotation, like Venus

Page 32: Angular Momentum in Planetary Atmospheres

Titan

George Hadley’s original idea to explain the trade winds (1735)

Page 33: Angular Momentum in Planetary Atmospheres

Titan

• CH4 on Titan behaves very much like water on Earth (“methanological” cycle)

• Links between seasonal and methanological cycle could drive angular momentum changes in the atmosphere and the solid surface

Page 34: Angular Momentum in Planetary Atmospheres

Titan

False color RADAR image

Recent observations show a slight change in Titan’s spin rate…

This could be evidence of a liquid water ocean between the solid interior and icy surface.

What’s the culprit? It could be angular momentum transfer between the surface and the atmosphere.

Page 35: Angular Momentum in Planetary Atmospheres

The fly-wheel crust of Titan?

Page 36: Angular Momentum in Planetary Atmospheres

So what about super-rotation…

Any East-West asymmetries could be responsible• On Titan: ???• On Venus:

– “moving candle” = Venus is rotating very slowly; the Sun heats one side for quite a while; radiative cooling on the other side

– Atmospheric waves, from wind over mountains, propagate upward and deposit momentum in the upper atmosphere

• They’re both slow-rotators ---- easy to get super-rotation in a model with slow rotation

• Bottom line: we know what kinds of mechanisms can generate super-rotation but we don’t know which of these, if any, are operating in which atmosphere

Page 37: Angular Momentum in Planetary Atmospheres

Outline

1. Overview of planetary atmospheres2. Angular momentum in rotating atmospheres3. Earth’s Hadley Circulation and Jet Streams4. Mars’ Hadley Circulation5. Super-rotation on Venus and Titan6. Jet formation on Jupiter

Page 38: Angular Momentum in Planetary Atmospheres

Jupiter

Multiple Jets and macroturbulence

Page 39: Angular Momentum in Planetary Atmospheres

Jupiter

Page 40: Angular Momentum in Planetary Atmospheres

Jet Formation

Stirring

wavebreaking

wavebreaking

E-W Wind

Angular momentum divergence

Angular momentum divergence

Angular momentum convergence

Page 41: Angular Momentum in Planetary Atmospheres

Jet Formation

Page 42: Angular Momentum in Planetary Atmospheres

Jupiter

Jets form by stirring at small scales, exciting waves and transporting angular momentum across latitude circles.

• Stirring is thought to be by “thunderstorms”

• Equatorial super-rotation requires atmospheric waves to travel across the equator

• Why so many jets? That is, what determines the jet width? size of the planet speed of the wind rotation rate of the planet

Rhines Length:

Page 43: Angular Momentum in Planetary Atmospheres

SummaryAngular momentum is a unifying concept in

atmospheric dynamics.

Earth• Earth’s Hadley Cell is approximately angular momentum

conserving (sometimes, sort of)• Angular momentum conserving theories accurately predict

width of the cells and the existence of a jet stream• Monsoons may be a result of dynamical regime shifts

between nearly (symmetric) angular momentum conserving flow to wave driven flow

Page 44: Angular Momentum in Planetary Atmospheres

SummaryAngular momentum is a unifying concept in

atmospheric dynamics.

Mars• Mars’ Hadley Cell is much more angular momentum

conserving than Earth’s but is still not “rings of fluid”• Angular momentum conserving theories accurately

predict width of the cells on Mars as well• A type of dry Monsoons may be driving non-

axisymmetric transport of H2O, CO2 and dust

Page 45: Angular Momentum in Planetary Atmospheres

SummaryAngular momentum is a unifying concept in

atmospheric dynamics.

Venus and Titan• Super-rotation in both atmospheres• Several mechanisms are possible causes but none are

certain (and may be different for each atmosphere)• Titan’s atmosphere may be exchanging significant

angular momentum with the surface, causing spin rate changes

Page 46: Angular Momentum in Planetary Atmospheres

SummaryAngular momentum is a unifying concept in

atmospheric dynamics.

Jupiter• Multiple jets and macroturbulence• Equatorial super-rotation as well• Angular momentum transport can form jets, while

a planet’s size, rotation rate and atmospheric wind speeds determine their width/number

Page 47: Angular Momentum in Planetary Atmospheres

THANK YOU!