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Saturn

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First viewed through a telescope by Galileo ... Dropped a probe (Huygens) into Titan's atmosphere. Path of Cassini. Saturn's Atmosphere ... – PowerPoint PPT presentation

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Title: Saturn


1
Saturn
  • Astronomy 311
  • Professor Lee Carkner
  • Lecture 18

2
Which of the following is a major component of
Jupiters clouds?
  • Water
  • Ammonia
  • Molecular hydrogen
  • a and b only
  • a, b, and c

3
In what region does Jupiter generate its strong
magnetic field?
  • Rock/ice core
  • Liquid metallic hydrogen mantle
  • Molecular hydrogen atmosphere
  • Dust ring
  • Alternating cloud bands

4
Saturn -- King of the Titans
  • He was overthrown by Jupiter who became king of
    the gods
  • Saturns symbol is the sickle

5
Viewing Saturn from Earth
  • First viewed through a telescope by Galileo
  • Modern telescopes reveal a series of rings and
    cloud patterns in Saturns atmosphere

6
Saturn Facts
  • Size 9.5 Earth diameters
  • Orbit 9.5 AU
  • Description smaller, more distant Jupiter with
    rings

7
Viewing Saturn from Space
  • Hubble Space Telescope has provided many images
  • Orbiting Saturn to study it long term
  • Dropped a probe (Huygens) into Titans atmosphere

8
Path of Cassini
9
Saturns Atmosphere
  • Saturn has belts, zones, ovals and storms, but
    they are less distinct than on Jupiter
  • Colors tend to be yellow, white and brown
  • Saturn sometimes has storms that burst up from
    below

10
Composition of Atmosphere
  • Top layer of Ammonia (NH3)
  • Middle layer of Ammonium Hydrosulfide (NH4SH)
  • We dont see all of the layers as clearly as we
    do on Jupiter

11
Saturns Dullness
  • The temperature of Saturns atmosphere increases
    more slowly with depth than Jupiter because
  • Due to weaker gravity the layers are more spread
    out
  • As a result
  • Upper layers obscure the deeper layers

12
Saturn and Jupiters Atmospheric Structure
13
Saturns Heat
  • Saturn is smaller than Jupiter and should have
    radiated much of its heat away by now
  • Theory the helium condensed into droplets and
    fell towards the core liberating gravitational
    energy
  • Calculations seem to support this

14
Saturns Interior
  • Saturn is also the most oblate planet
  • The density is low due to a much smaller liquid
    metallic hydrogen mantle
  • Saturn has a magnetosphere but it is not as
    strong as Jupiters
  • Due to slower rotation, less liquid hydrogen and
    blocking of charged particles by the rings

15
Internal Structure of Jupiter and Saturn
16
HST Views the Rings Edge-On
17
Rings and Tides
  • This is the region where the tidal force pulling
    the material apart is stronger than the
    gravitational force holding it together

18
Structure of the Rings
  • Rings are separated by gaps or divisions with
    relatively few particles
  • The size and composition of particles vary from
    ring to ring
  • F ring has many small, dark particles

19
Diagram of Saturns Rings
20
Moons and the Rings
  • Several moons have orbits within the rings
  • Moons may also be a source of ring material
  • Examples of moons effecting the rings
  • The Encke gap has a small moon, Pan, in it

21
Next Time
  • Read Chapter 13.1-13.6

22
Summary
  • Saturn is the second largest planet and the
    second closest gas giant to Earth
  • Saturn is similar to Jupiter with key exceptions
    mostly due to less mass and smaller gravity
  • cloud layers are more spread out in depth
  • less distinct cloud bands
  • larger core
  • less liquid metallic hydrogen

23
Summary Rings
  • Made up of many distinct rings and ringlets
  • Composed mostly of icy particles of various sizes
    and reflectivity
  • Ring structure shaped by moons
  • Rings cannot form a larger body due to tidal
    forces
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