atmospheres of the giant planets

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SECRETS OF SECRETS OF THE SOLAR SYSTEM THE SOLAR SYSTEM S S 3 3 - - 05 05 Wladimir (Wlad) Lyra Wladimir (Wlad) Lyra Brian Levine Brian Levine AMNH After-School Program AMNH After-School Program

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Page 1: Atmospheres of the Giant Planets

SECRETS OF SECRETS OF THE SOLAR SYSTEM THE SOLAR SYSTEM

SS33--0505Wladimir (Wlad) LyraWladimir (Wlad) Lyra

Brian LevineBrian Levine

AMNH After-School ProgramAMNH After-School Program

Page 2: Atmospheres of the Giant Planets

From last class

The Sun is by far the dominant object of the Solar System

Jupiter has more than twice the mass of all planets combined.And the Sun is more than 1000x more massive than Jupiter.

The Sun accounts for 99.9% of the mass of the solar system

The Sun

Page 3: Atmospheres of the Giant Planets

From last class

Magnetic Fields

Page 4: Atmospheres of the Giant Planets

Magnetic Reconnection

Magnetic Field lines store energy

Upon cancellation, the energy is explosively released

From last class

Page 5: Atmospheres of the Giant Planets

The chemical composition of the SunThe chemical composition of the Sun

Chemical Composition

Most abundant elements, in order: H (71%) He (27%)

0 (1.04%) C (0.46%) Ne (0.13%) Fe (0.11%) N (0.1%) Si (0.06%), Mg (0.05%), S (0.04%)

From last class

Page 6: Atmospheres of the Giant Planets

From last class

H H H H H He H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H O H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H C H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H O H H H H H H H H H H H H H H H H H He H H H H H O H H H H H H H H H H H H H H H H H H H H H Ne H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H He H H H O H H H H H H H H H H H H H H He H H H H H H H O H H H H H H He H H H HH H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H He H H H H H C H H H H H H H H H H H H H H H H H H H H O H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H

He H H H H H H H H H H H H H H H H H H H H H C H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H H H H H H H H He H H H H He H H H H H H H H H H H HH H H H H H H N H H H H H H H H H H H H H H H H H H H H H H H H H H H H He H H H H H H O H H H H H H H H H H H H H O H H H H H H H H H H H H H H He H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H H O H H H H H H H H H H H C H H H H H H H H H He H H H H H H H H H H H H H H H H H H H H HH H H H H H H H H H H H H H H H H H H H H H O H H H H H H He H H He H H H H H H H H H H H H H Fe H H H

H H H H H H H H H H H H H H H H H H H H H H H H H H

H2 He

H

20 CH

4 NH

3

Fe, Si

Gas

Ices

Rock

Chemistry

Page 7: Atmospheres of the Giant Planets

From last class

Inward of snowline

Accreting rocky cores

(small)

Outward of snowline

Ice comes to aid! Growing big

icy/rocky cores.

Formation

Page 8: Atmospheres of the Giant Planets

Outline

Classes of Planets

Giant Planets

- Interiors- Atmospheres

- Rings

Page 9: Atmospheres of the Giant Planets

The Snowline

Colder than ~150K, the volatiles (H20, CH

4, NH

3)

condense into icesices.

Volatiles in gas phase Volatiles in solid phase

Page 10: Atmospheres of the Giant Planets

Classes of planets

EarthJupiter Saturn Uranus/Neptune

Rocky Planets Gas Giants Ice Giants

Rock Gas Ice

Page 11: Atmospheres of the Giant Planets

Formation

Page 12: Atmospheres of the Giant Planets

Formation

Inward of snowline

Accreting rocky cores

(small)

Outward of snowline

Ice comes to aid! Growing big

icy/rocky cores.

Page 13: Atmospheres of the Giant Planets

Formation

Inward of snowline

Accreting rocky cores

(small)

Outward of snowline

Ice comes to aid! Growing big

icy/rocky cores.

These guys got so big they started accreting gas from the nebula!

These ones never did. They are just the icy/rocky cores.

Page 14: Atmospheres of the Giant Planets

Gas Giants

Page 15: Atmospheres of the Giant Planets

Activity

Page 16: Atmospheres of the Giant Planets

Interior of Jupiter

Pressure = weight/area

Pressure at center70 million atmospheres

Temperature at center17.000 K

Page 17: Atmospheres of the Giant Planets

Phase diagram

Page 18: Atmospheres of the Giant Planets

Phase diagram

Page 19: Atmospheres of the Giant Planets

A lot more happens at high pressures

Page 20: Atmospheres of the Giant Planets

Hydrogen under pressure

Page 21: Atmospheres of the Giant Planets

Interior of Jupiter

Pressure = weight/area

Pressure at center70 million atmospheres

Temperature at center17.000 K

Cloud topsMolecular Hydrogen

Liquid Hydrogen

Fluid Metallic Hydrogen

Rock/Ice core

Page 22: Atmospheres of the Giant Planets

Interior of the giant planets

Page 23: Atmospheres of the Giant Planets

Activity

Page 24: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Page 25: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Page 26: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Bands and Storms

Page 27: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Bands and Storms

Page 28: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Bands and Zones

Large scale windsof alternate direction

Page 29: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Wind Speeds

Page 30: Atmospheres of the Giant Planets

Clouds of the Giant Planets

Page 31: Atmospheres of the Giant Planets

Molecules condense at different temperatures

H20 ~300K

NH3

~140KCH

4 ~80K

Atmospheric Temperatures

Page 32: Atmospheres of the Giant Planets

Ammonia and Methane Clouds

Jupiter and Saturn have ammonia cloudsColder Uranus and Neptune have methane clouds

Page 33: Atmospheres of the Giant Planets

Clouds of Jupiter

Bright ZonesZonesDark BeltsBelts

Dark brown color: compounds of sulfur (S) and phosphorus (P)

Bright zones:High ammonia clouds

shielding brown stuff below

Page 34: Atmospheres of the Giant Planets

Clouds of Jupiter

Bright ZonesZonesDark BeltsBelts

Dark brown color: compounds of sulfur (S) and phosphorus (P)

Bright zones:High ammonia clouds

shielding brown stuff below

In Jupiter

Hot gas rises, cools, ammonia condenses -> Zones.

Cold air sinks, heatsheats, dry in ammonia - > BeltsBelts.

Page 35: Atmospheres of the Giant Planets

Atmospheres of the Giant Planets

Storms !!

Page 36: Atmospheres of the Giant Planets

Merging Storms

Page 37: Atmospheres of the Giant Planets

Jupiter's Red Spots

Page 38: Atmospheres of the Giant Planets

Uranus

Featureless...

Page 39: Atmospheres of the Giant Planets

Not quite featureless...

Uranus in false color: Bands ! Recently seen by Hubble: Storms !

Due to the extreme axial tilt,weather in Uranus may be highly seasonal, being more Neptune-like in the equinoxes.

Page 40: Atmospheres of the Giant Planets

Mission to Jupiter: Galileo

Page 41: Atmospheres of the Giant Planets
Page 42: Atmospheres of the Giant Planets

Mission to Saturn: Cassini

Page 43: Atmospheres of the Giant Planets
Page 44: Atmospheres of the Giant Planets
Page 45: Atmospheres of the Giant Planets

Cassini orbiting Saturn

Page 46: Atmospheres of the Giant Planets

Ringshine

Page 47: Atmospheres of the Giant Planets

Planetary Rings

Page 48: Atmospheres of the Giant Planets

Planetary Rings

Galileo's drawing, 1610.

“I do not know what to say in a case so surprising, so unlooked for, so novel.”

Page 49: Atmospheres of the Giant Planets

Planetary Rings

Huygens's drawings, 1659.

“Saturn is surrounded by a thin flat disk, nowhere touching the planet”

Page 50: Atmospheres of the Giant Planets

Planetary Rings

Other drawings from the 17th century

Galileo, 1610

Gassendi, 1634

Fontana, 1646

Riccioli, 1648

Huygens, 1655

Cassini, 1676

Page 51: Atmospheres of the Giant Planets

Planetary Rings

What are these rings???

Solid? Liquid? Particulate?

Page 52: Atmospheres of the Giant Planets

Planetary Rings

Maxwell's proof

James Clerk Maxwell (1831-1879)

Page 53: Atmospheres of the Giant Planets

Planetary Rings

Maxwell's proof There are some questions in Astronomy, to which we are attracted

rather on account of their peculiarity, […] than from any direct advantage which their solution would afford to mankind.

[…] I am not aware that any practical use has been made of Saturn's Rings […]

But when we contemplate the Rings from a purely scientific point of view, they become the most remarkable bodies in the heavens. [..] When we have actually seen that great arch swung over the equator of the planet without any visible connection, we cannot bring out minds to rest. […] We must explain its motion on the principles of mechanics.

[...]60 pages of calculations

[...]

[…] We conclude, therefore, that the rings must consist of disconnected particles; these may be either solid or liquid, but they must be independent. […] The final result, therefore, of the mechanical theory is, that the only system of rings which can exist is one composed of an indefinite number of unconnected particles, revolving around the planet with different velocities according to their respective distances.

Maxwell's proof

Page 54: Atmospheres of the Giant Planets

Planetary Rings

Why only Saturn has rings?

Carl Sagan

Page 55: Atmospheres of the Giant Planets

Rings of Uranus

Occultations Uranus occults a star

Page 56: Atmospheres of the Giant Planets

Rings of Uranus

Page 57: Atmospheres of the Giant Planets

Rings of Jupiter

A very faint ring systemdiscovered by Voyager 1.

Page 58: Atmospheres of the Giant Planets

Rings of Jupiter

Viewed with Keck, with a methane filter.

Page 59: Atmospheres of the Giant Planets

Rings of Neptune

A very faint ring system, similar to Jupiter's ringsdiscovered by Voyager 2.

Page 60: Atmospheres of the Giant Planets

Rings of Neptune

Arcs!!!

Page 61: Atmospheres of the Giant Planets

Ring Systems

Jupiter Saturn Uranus Neptune

Fine, diffuse dust,very dark.

Icy boulders,very bright.

Rocky boulders,dark.

Pebbles (?)Dark and reddish (?)

Page 62: Atmospheres of the Giant Planets

Tides

Page 63: Atmospheres of the Giant Planets

Tides

The side closer to the Moon experiences a greater pull than the side further out.

The effective result is adifferential force

we call Tidal Force.

Page 64: Atmospheres of the Giant Planets

Roche Limit

Limit where the tidal force is stronger than the internal forces

holding the body together

Page 65: Atmospheres of the Giant Planets

All ring systems are inside their planet's Roche limit

Page 66: Atmospheres of the Giant Planets

Ring formation: Competing theories

1). Moon that got too close 2). Leftover material that could not coalesce into moons