the gas giants l.
Skip this Video
Loading SlideShow in 5 Seconds..
The Gas Giants PowerPoint Presentation
Download Presentation
The Gas Giants

Loading in 2 Seconds...

play fullscreen
1 / 24

The Gas Giants - PowerPoint PPT Presentation

  • Uploaded on

The Gas Giants. Astronomy 311 Professor Lee Carkner Lecture 16. Upcoming Events. Thursday, October 21 Nelson Lecture in Astronomy Dr. Jason Steffen, “ Kepler Mission’s Search for Planets Around Other Stars: Finding Other Earths” Saturday, October 23 Planetarium Open House

I am the owner, or an agent authorized to act on behalf of the owner, of the copyrighted work described.
Download Presentation

PowerPoint Slideshow about 'The Gas Giants' - MartaAdara

An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.

- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -
Presentation Transcript
the gas giants
The Gas Giants

Astronomy 311

Professor Lee Carkner

Lecture 16

upcoming events
Upcoming Events
  • Thursday, October 21
    • Nelson Lecture in Astronomy
    • Dr. Jason Steffen, “Kepler Mission’s Search for Planets Around Other Stars: Finding Other Earths”
  • Saturday, October 23
    • Planetarium Open House
    • See planetarium show and look through telescopes
  • 10 points extra credit on observing project for each
gas giant basics
Gas Giant Basics
  • Sometimes called Jovian or Outer planets
    • Does not include Pluto
  • The gas giants have no real surface, all we see is atmosphere
missions to the outer planets
Missions to the Outer Planets
  • 1972 Pioneer 10 -- Jupiter flyby
  • 1973 Pioneer 11 -- Jupiter/Saturn flyby
  • 1977 Voyager 2 --Jupiter/Saturn/Uranus/ Neptune flyby
  • 1997 Cassini -- Saturn orbiter and Titan probe (Huygens)
    • arrived 2004, currently taking data
voyager 2
Voyager 2
  • Took advantage of favorable alignment of outer planets to visit them all
  • Used gravity of each planet to change orbit to get to the next
    • Is still taking data on the edge of the solar system
gas giant facts

Diameter: 11.21

Mass: 317.83

Orbital Radius: 5.20


Diameter: 9.42

Mass: 95.16

Orbital Radius: 9.54


Diameter: 4.01

Mass: 14.50

Orbital Radius: 19.19


Diameter: 3.88

Mass: 17.20

Orbital Radius: 30.06

Gas Giant Facts
  • Numbers are relative to the Earth
  • Orbital radii for the outer planets range from ~5-30 AU
    • The outer planets cover a much larger region
    • Gas giants don’t move much in the sky from our viewpoint
sizes of the gas giants
Sizes of the Gas Giants
  • Jupiter and Saturn about 10 Earth diameters
  • Uranus and Neptune about 4 Earth diameters
  • The gas giants contain 99% of the mass of the solar system (not including the Sun)
    • Volume and mass go as radius cubed
  • Average density (kg/m3)
    • Jupiter:
    • Saturn:
    • Uranus:
    • Neptune:
  • For comparison Earth’s density is 5515
    • Saturn is less dense than water (it floats)
  • The gas giants have a low density because they are made up mostly of hydrogen and helium, the 2 lightest elements
    • Hydrogen is the lightest and most abundant element in the universe (1 proton + 1 electron)
  • Total composition
    • ~5% heavier elements (methane, ammonia, water vapor etc.)
atmospheric features
Atmospheric Features
  • Clouds
    • small amounts of trace elements may produce the colors
  • Bands
    • adjacent bands move in opposite directions
  • Storms
    • some are very long lived (e.g. Great Red Spot)
continuous boost
Continuous Boost
  • Rate of change of speed is called the acceleration, a
  • Solution: turn around halfway and decelerate to a stop
time to get to planet
Time to get to Planet
  • Find time to get half way there and double it
  • In general, distance equals ½at2
  • As a simple estimation, we will assume a direct boost at opposition
    • In reality we would have to take into account the orbital velocities of the planets
odyssey to jupiter
Odyssey to Jupiter

Jupiter at Conjunction

Spaceship Direct Boost



Least Energy Orbit

Jupiter at Opposition

  • Degree of oblateness depends on mass distribution
  • Models indicate that gas giants have a small, dense, rock-ice core
    • Must have conducting liquid interiors
  • Number of satellites (larger than ~10 km)
    • Jupiter -- 16
    • Saturn -- 26
    • Uranus -- 27
    • Neptune -- 13
    • Including the very small ones, about 170 total
moon properties
Moon Properties
  • Satellites tend to be composed of rock and ice
  • Many have rocky cores and icy surfaces
    • Io is very active and covered with volcanoes
    • Europa may have a liquid water ocean
  • All of the gas giants have rings of small particles
    • The rings of the other planets are made of smaller darker particles and were only discovered by spacecraft
    • This is the region where the tidal force from the planet is greater than the gravitational force holding the object together
differences between the gas giants
Differences Between the Gas Giants
  • Uranus and Neptune are smaller, cooler and have less distinct cloud features
next time
Next Time
  • Read 11.1-11.4, 11.6
  • Size: ~4-11 times Earth diameter
  • Mass: ~15-318 Earth masses
  • Composition: mostly hydrogen and helium
  • Atmosphere: clouds of methane and ammonia
    • also have large, long-lived storm systems and oppositely moving bands
summary the jovian systems
Summary: The Jovian Systems
  • The gas giants have extensive satellite systems
    • Many moons have icy exteriors with rocky cores
    • Some are very large (~size of Earth’s Moon)
  • All of the outer planets (not just Saturn have ring systems)
    • rings composed of small particles
    • Ring properties different for each planet