Lecture 19 Flashcards

Saturn and its rings and moons

1
Q

Cassini Huygens Mission

A

2 Probes: Cassini and Huygens
Went to Saturn and Titan
17 Nation Venture
Operated by NASA

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2
Q

Purpose of Cassini’s Instruments

A

To see beneath Titan’s cloud cover
Map Titans Surface
Get atmospheric informtation
Detect UV light from clouds

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3
Q

Uses of Huygens Instruments

A

Getting Density, T, and pressure of atmosphere
Images of landing sight and surroundings
Measuring chemicals in atmosphere
Getting properties of surface

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4
Q

Purpose of the Cassini Huygens Mission for Saturn?

A

Determine the temperature field, cloud properties and composition of Saturn’s Atmosphere
Determine Internal Structure and rotation of deep atmosphere
Determine Heat Flux and radiation environment present during formation and evolution

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5
Q

Purpose of the Cassini Huygens Mission for the Rings?

A

Composition and size of ring material
Investigate the interrelation of the the rings and moons

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6
Q

Purpose of the Cassini Huygens Mission for the Satellites?

A

Determining geological history
Define different physical processes that have created surfaces crusts and sub surfaces
Determining bulk compositions and internal structures of moons

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7
Q

Purpose of the Cassini Huygens Mission for Titan?

A

Determine abundant elements
Search for complex molecules
Determine physical state, topography and composition of surface
Determine surface state of matter (solid or liquid)

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8
Q

How are Saturn’s Rings divided?

A

By the order they were discovered
Each distinct from its neighbor

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9
Q

Origin of the Rings

A

3 Hypotheses
1. Gravitational disruption of a satellite or comet
2. Fragmentation of satellites by impact
3. Accretionary Remnant

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10
Q

What is the Roche Limit

A

The orbit closest to a planet that a satellite can withstand Tidal Forces

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11
Q

Clues for the Origins of Saturn’s Rings

A

Some rings are made from the debris of inner satellites
Saturn’s rings are disappearing

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12
Q

Titan’s Geologic History

A

Accretion from materials rich in water, methane and ammonia
Differentiation
Dissociation of NH3

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13
Q

Titan Atmosphere

A

Ethane based weather cycle

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14
Q

Titans Lakes

A

Located near polar regions
Made up of liquid methane and ethane

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15
Q

Winds on Titan

A

Blow West to East globally

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16
Q

Titan’s Dunes Composition

A

Dunes are made up of grains of ice and organic matter

17
Q

Evidence of Titan’s geological activity

A

Wind erosion
Flowing Liquid
Cryovolcanism
Impact Cratering
Potential Tectonic Activity

18
Q

Titan’s Climate

A

Humid conditions at the poles for lakes seas and rivers
Dry conditions at the equator for dunes and dry river beds

19
Q

Titan Interior Characteristics

A

Organic Rich Atmosphere
Decoupled Outer shell
Global Subsurface ocean
High pressure Ice VI shell
Hydrous Silicate Core

20
Q

Geological Activity on Enceladus

A

Liquid Water is present in Enceladus
Tidal Heating
Salt-water mixtures

21
Q

Shepherd Moons of Saturn

A

Enceladus
Pandora
Hyperion
Mimas
Dione
Phoebe
Iapetus