Introduction to the Solar System


APAS 1110 Summer 1996

Lecture 17 -- Uranus-Neptune: Icy Realms Beyond the Wanderers

Thursday, June 27



  • Uranus and Neptune --What you see

    Can't see them at all without a telescope
    They were not part of the wanderers of the ancients
    OH: Right now, Neptune is behind Uranus, which is behind Jupiter
    Almost in a straight line
    Uranus to me looks like a green dot in a powerful telescope
    Neptune looks like a smaller blue dot, but you can see the disk
    There are so far out that you know that they have to be big to see a disk


  • Discovery of Uranus and Neptune

    William Herschel was a musician, who turned to astronomy
    He was trying to map all the bright stars in the sky, and discovered Uranus
    There are supposed to be only 2 kinds of true geniuses in the world -- mathematicians and music, but the aptitudes are very related
    So Herschel discovered Uranus in 1781, well after the establishment of Newton's laws of gravitation and motion
    Uranus is 2 billion km from the Sun, and goes around once every 84 years
    So it has gone around the Sun only 2.5 times since its discovery
    Uranus is the mythological grandfather of Jupiter (Zeus in Greek)
    Saturn is the father of Jupiter
    Uranus was watched for a few years until they could figure out its orbit
    The problem is, it had some irregularities in its orbit that apparently couldn't be explained by Newton's Laws
    It was a crisis in science -- some people suspected that Newton's laws were wrong
    French mathematician Leverrier, in 1846 used Newton's laws to try and predict (with pencil and paper) where another large body might be to explain the discrepancies
    It took some German astronomers only and hour of searching to find Neptune
    This was cited as a great victory for Newtonian physics, and probably ushered in the great era of rationalistic thinking that characterized the Victorian era


  • Uranus' Ring

    In 1977, before Voyager got to Uranus, the planet passed in front of a star
    This is called an occultation
    Stellar occultations are important in planetary astronomy, because it allows you to figure out whether a planet has an atmosphere
    If the star dims and flickers a little when it disappears behind a planet, you know the planet has an atmosphere
    But with Uranus, the star dimmed before it got to the edge of the planet
    We concluded that it had some rings around it


  • Voyager at Uranus

    It took Voyager 6 years to cross the deep space between Saturn and Uranus, and it arrived there in 1986
    What Voyager saw was a featureless bluish-green disk
    The atmosphere of Uranus was made of H2 and He, just like Jupiter and Saturn
    It has clouds of methane, at -320 F
    Uranus and Neptune formed in the same way as Jupiter and Saturn
    First a rocky core, several times the size of the Earth accreted from the planetesimals in the outer solar system
    When the core got big enough, it began to gravitationally attract the gas in the solar nebula
    It got lots of H2 and He, like Jupiter and Saturn, but it got lots of other frozen gases, too, like CH4
    Because they are all almost the same, Jupiter, Saturn, Uranus and Neptune are called the Gas Giants
    But on Jupiter and Saturn, we have yellow clouds and lots of turbulent weather
    Why is Uranus blue-green, and why don't we see bands of clouds and weather?
    Recall what drives the weather on Jupiter and Saturn
    On the Earth, it is the Sun's energy
    On Jupiter and Saturn, it is the energy coming up from the interior, the left over heat from the compression due to gravity
    Because Uranus is smaller, it doesn't have as much compressional energy, and there is less heat from the interior to drive cloud motions
    And why is Uranus blue-green?
    On Uranus, the clouds are made of methane, rather than the sulfur and ammonia clouds of Jupiter and Saturn
    Methane absorbs red and orange light, and Uranus looks blue-green
    Voyager also discovered the shepherd moons that are necessary to keep the rings in place


  • Uranus' Interior

    Small rock core
    mantle of liquid water and methane mixture -- an enormous ocean
    Atmosphere of H2 and He
    Clouds of methane, topped with a haze layer that may be a little like Titan's
    Because Uranus it further out from the sun, the conversion of methane to heavier hydrocarbons takes place slower (it takes sunlight)
    Uranus lacks the mantle of metallic and liquid hydrogen that Jupiter has, because it doesn't compress hydrogen enough


  • Uranus's tilt

    The most amazing thing about Uranus is that it is tilted onto its side
    The north pole is pointing straight at the sun
    The angle that the rotation axis makes with the axis of the solar system (same as the Sun's rotational axis) is called the planet's obliquity
    Uranus' obliquity is about 90 degrees
    As Uranus goes around the Sun, the equator points at the sun, and then it's south pole, and then the equator again, and then the north pole again
    But the planet spins once every 17 hours
    What it means is that the concept of years and days is really mixed up
    The best explanation is that by a huge planetesimal, and that it wound up on its side
    But why did its moons and rings get knocked over, too?
    Tidal forces would have forced the moons to eventually orbit in the same plane as Uranus' rotation.


  • Neptune

    Voyager got to Neptune in 1989
    Neptune actually violates Bodes' law -- it isn't as far out as you would expect
    Uranus is 20 AU from the Sun, twice as far as Saturn. But Neptune is 30 AU from the Sun
    What we saw there really surprised us
    We expected another Uranus
    Neptune is the same size as Uranus, so we don't expect much heating of the atmosphere due to compression
    But what we saw were cloud features and storms, like on Jupiter
    Neptune is a striking blue color, but it has noticeable clouds and storms
    We know the sun is even dimmer there than at Uranus, so what drives the weather
    We have no idea
    Neptune may be bluer than Uranus because of N2 in the atmosphere
    Maybe this has something to do with the weather and storms
    Neptune has a blue storm, just like the Great Red Spot on Jupiter, rotating counter clockwise
    It also has smaller features, like Jupiter, that rotate in the upper clouds
    One feature seems to zip around the planet, a mini storm, called scooter
    When we looked really closely at Neptune, we saw bands of cumulus clouds, like thunderstorms on the Earth
    If Neptune was a basketball, Voyager flew 1/4" off the surface of the cloud tops
    Before Voyager got to Neptune, in the 1980's, people tried to use occultations to show that Neptune had rings
    The problem was that sometimes they saw the star dim before it passed behind Neptune, and sometimes they didn't
    They concluded that Neptune didn't have rings, it had ring-arcs
    Voyager saw that Neptune truly had rings all the way around the planet, but that they got thinner and thicker as you go around the planet
    They are still called ring-arcs, and they are difficult to explain

    VIDEO: NEPTUNE'S COLD FURY, NOVA (First half) 6/27/96