the jovian planets
Download
Skip this Video
Download Presentation
The Jovian Planets

Loading in 2 Seconds...

play fullscreen
1 / 19

The Jovian Planets - PowerPoint PPT Presentation


  • 330 Views
  • Uploaded on

The Jovian Planets. Chapter 7. Topics. Jupter, Saturn, Uranus, Neptune How do we know? Why do we care? What is common about the outer planets? What is peculiar to each of these planets?. Jovian planets (Jupiter-like). Size. radius is about 1/10 of the radius of the Sun.

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

PowerPoint Slideshow about 'The Jovian Planets' - tamas


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
topics
Topics
  • Jupter, Saturn, Uranus, Neptune
  • How do we know?
  • Why do we care?
  • What is common about the outer planets?
  • What is peculiar to each of these planets?
slide4
Size

radius is about 1/10 of the radius of the Sun

distance from the sun
Distance from the Sun

Jovian

Terrestrial

slide6
Terrestrial

Jovian

small--1/100 radius of the Sun

large --1/10 radius of the Sun

Size

orbit at 0.4 to 1.5 AU

orbit at 5 to 30 AU

Location

few

many (# growing)

Moons

none

all have rings

Rings

Composition

rocks and metals

gasses and ice

composition
Composition

0.71 to 1.67 g/cm3

So what are they made of?

mostly gasses (hydrogen, helium) and ice

jupiter
Jupiter
  • largest planet
  • Great Red Spot
  • studied by Pioneer, Voyager 1 & 2, Galileo spacecraft
  • liquid interior (very high pressure and temperature)
  • 16 moons (4 largest are the Galilean moons)
slide9
Io
  • Active volcanoes
europa
Europa
  • subsurface ocean
  • cracked ice
ganymeade
Ganymeade
  • lots of faults
  • strong magnetic field
callisto
Callisto
  • old surface (meaning that it’s not undergoing lots of change except for impact craters)
saturn
Saturn
  • Large, thin rings
  • Rings are held together by the gravitational attraction of “shepharding” satellites
  • Major Gaps: The Cassini and Enke divisions
titan
Titan
  • larger than Mercury
  • has an atmosphere
  • probably has oceans of methane
uranus
Uranus
  • discovered in 1781
  • shows no cloud banding
  • axis of rotation is only tilted 8 degrees from the ecliptic
  • 84 year orbital period
  • rings originally discovered during occultation of a star
  • young rings (what’s the source of dust?)
neptune
Neptune
  • noted by Galileo
  • the exact path of Uranus could not be explained by the gravitational pulls of the Sun, and the other planets. What does this mean?
  • discovered in 1846
  • 164 year orbital period
  • strong magnetic field
triton
Triton
  • density 2.1 g/cm3
  • atmosphere (nitrogen)
  • impact craters due to comets
  • ice made of water
  • active ice volcanoes
  • retrograde orbit (it’s going the wrong way)
  • probably captured by Neptune
extrasolar planets
Extrasolar planets
  • How many planets have we discovered besides those in our solar system?
  • I’m starting to lose count, but it’s now over 100.
  • Planets are even found in binary star systems.
  • We analyze the wobble in a star by studying the Doppler shift in its spectrum and determine the approximate masses and distances of the orbiting planets.
how do we know
How do we know?
  • How do we know that the outer planets are mostly gas and mostly made up of hydrogen and helium?
  • How do we know that the atmosphere of a planet has methane?
  • How do we know the period of rotation of the outer planets? (Note: we use a different technique of measuring rotational period of the terrestrial planets.)
  • How do we know that a moon’s surface is ice?
  • How do we know the size of matter within the rings?
  • How do we know that a moon has an “old” surface and that the moon has little geologic activity?
ad