Lecture 27: Jupiter and Saturn cont.
Overview of Jupiter and Saturn
- Study Chapter 6 (The Giant Planets) in detail.
- Review online resources:
Thermal Emission and Energy Balance
- Jupiter and Saturn emit radiation similar to a black body.
- Total energy emitted by these planets is greater than the energy they receive from the Sun.
- Both planets appear warmer than expected based on their distance from the Sun, suggesting internal heat sources.
Differentiation and Internal Heat
- Differentiation leads to a planet's layered structure, with denser materials sinking.
- This process releases gravitational potential energy, converted into heat.
- Jupiter: Helium and hydrogen currently undergoing differentiation, causing helium to separate and settle, releasing further energy.
Helium and Hydrogen Behavior
- Inside Jupiter and Saturn, helium and hydrogen exist as two immiscible liquids, forming an emulsion-like state.
- As helium droplets sink, gravitational energy is released, potentially explaining the depletion of neon in Jupiter’s atmosphere.
Atmospheric Dynamics of Jupiter
- Jupiter’s atmosphere shows a clear banding structure due to convection:
- Warm air rises, cools, and condenses, forming clouds.
- Rapid rotation (9.9-hour day) disrupts convection, causing alternating wind systems and impacting storm dynamics (e.g., Great Red Spot).
- Equatorial wind speeds can reach approximately 150extm/s or 540extkm/hr.
Cloud Bands and Composition
- Cloud Layers: Two main types of bands –
- Zones: Light-colored due to high altitudes and ammonia concentration.
- Belts: Darker areas where ammonia clouds dissipate, revealing deeper layers made of ammonium hydrosulfide ice.
The Great Red Spot
- A long-lived anti-cyclone located in the southern hemisphere, characterized by its vast size (over twice the diameter of Earth).
- First recorded in 1665 and still evolving, demonstrating dynamic atmospheric changes.
Coriolis Effect and Storm Systems
- The Coriolis effect causes rotation patterns in atmospheric systems:
- Low pressure systems (cyclones) spin counterclockwise in the northern hemisphere and clockwise in the southern hemisphere.
- High-pressure zones show the opposite spin.
Saturn’s Characteristics and Exploration
- Saturn appears less colorful than Jupiter, with less pronounced cloud bands.
- Major insights into Saturn came from the Cassini-Huygens mission, launched in 1997 and orbiting Saturn from 2004 to 2017.
Energy Sources for Space Probes
- RTGs (radioisotope thermoelectric generators) are used for spacecraft power, notably in Cassini, which used plutonium pellets to generate electricity.
Magnetic Fields of Jupiter and Saturn
- Jupiter’s magnetic field is tilted; Saturn’s field is closely aligned with its rotation axis.
- Both planets emit radio waves related to their magnetic fields and rotation, which can vary across regions.
Differential Rotation in Saturn
- Saturn shows slight differences in its rotation rate measurements, illustrating the complexity of planetary dynamics.
- Variations may be influenced by atmospheric plasma interactions with the magnetic field.
Dynamic Atmosphere of Saturn
- Like Jupiter, Saturn possesses a dynamic, banded atmosphere, frequently changing due to storm activity driven by convection.
Overview of Galilean Moons of Jupiter
- Discovered by Galileo Galilei in 1610, the four largest moons (Io, Europa, Ganymede, Callisto) exhibit diverse features:
- Callisto: Heavily cratered, suggesting inactivity and possible differentiation with a rocky core.
- Ganymede: Fully differentiated with a layered structure and potentially a subsurface ocean beneath ice.
Differentiation Factors in Ganymede and Callisto
- Ganymede's greater differentiation likely arises from faster accretion rates and increased tidal heating compared to Callisto.
Future Study Directions
- Further exploration into icy moons and their potential subsurface oceans, as well as volcanic activity, is suggested for next meetings.
- Study related articles on Moons of Jupiter (EUROPA, IO, GANYMEDE) and their implications.
Useful References
- For further details on the moons: