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Honey, I Shrunk the Solar System

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Orbit strange- tilted 17 from plane of the solar system ... A third class, Small Solar System Bodies, was defined as all other objects except satellites. ... – PowerPoint PPT presentation

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Title: Honey, I Shrunk the Solar System


1
Honey, I Shrunk the Solar System
  • or
  • Pluto We Barely Knew Ye as a Planet

Image credit JPL
2
The Way it Was
Image from JPL
3
And Then There Were Eight
Image from JPL
4
From Where Did the Word Planet Come?
  • The word planet is derived from the Greek word
    for wanderer and was traditionally applied to
    any heavenly body that moved with respect to the
    stars. In this sense the Sun and Moon were also
    planets.
  • Dictionary says that a planet is any one of the
    nine large bodies that orbit the Sun.
  • But some objects have been found that are larger
    than Pluto- so are they planets?

5
Who Discovered the First Planets?
  • Ancient cultures knew that some objects were not
    fixed in the sky like the stars.
  • The Greeks knew of five such objects Mercury,
    Venus, Mars, Jupiter and Saturn
  • By 800 B.C.E. Babylonian astronomers had records
    of planetary motion for Venus, Jupiter and Mars.

6
The Solar System Until 1781Mercury, Venus,
Earth, Mars, Jupiter and Saturn
Images from NASA
7
The Solar System Grows What to Name a New
Planet?
  • March 13, 1781 William Herschel discovers what he
    thinks is a comet, but he has discovered a new
    planet- the seventh in our Solar System.
  • Herschel wanted to name the new planet George
    after King George III of England.
  • It was decided to continue with the Roman god
    names that had been used for the other planets,
    thus it was named Uranus.
  • This set the standard for the convention of using
    Roman god names for the planets.

8
Uranus- The First New Planet
  • Distance 19.1 AU Doubled the size of the Solar
    System
  • Diameter 4 Earth diameters

Image courtesy of NASA
9
Another New World Neptune
  • The orbit of Uranus was not as expected.
  • John Couch Davies, a 24 year old Cambridge grad,
    thought that this might be caused by another
    unknown planet
  • In 1845 he submitted his calculations to the
    Astronomer Royal of England. English star charts
    not good enough.
  • At nearly the same time French astronomer Urbain
    Jean Joseph de Verrier did the same calculations.
    The Berlin Observatory was given his data and
    the planet was found the first night due to
    better star maps.

10
Neptune
  • Following the Roman god theme the planet was
    named Neptune, for the sea god since it was blue
  • 30 AU from the Sun
  • Diameter 3.9 Earth diameters

Image by Hubble Space Telescope
11
A Ninth Planet?
  • Speculations about a ninth planet date back to
    the late 1800s.
  • Percival Lowell urged that a special camera be
    built to look for Planet X.
  • In 1929 the camera was finished and installed at
    Lowell Observatory in Flagstaff, AZ
  • Clyde Tombaugh discovered Pluto on February 18,
    1930 after looking at over one million stars
  • Name Pluto suggested by Venetia Burney, an 11
    year old girl. Pluto was the Roman god of the
    underworld.

12
Clyde Tombaugh 1906-1997
13
Finding Pluto
Pluto images by Nathan Twining Observatory
14
Here it is!
Pluto images by Nathan Twining Observatory
15
Pluto
  • 39.5 AU from Sun
  • Diameter about 0.18 Earth diameter (about 1400
    miles)
  • Pluto and Charon essentially a double system
  • NASA New Horizons mission will reach Pluto in
    2015

Image by Hubble Space Telescope
16
The Arguments for and Against Planethood for Pluto
  • Pluto very small
  • Doesnt fit into any other categories of planets-
    terrestrial or gas giants
  • Orbit strange- tilted 17 from plane of the solar
    system
  • May be typical of thousands of icy objects found
    far from the Sun
  • It is round like a planet and it orbits the Sun.

Image by JPL
17
The Kuiper Belt
John Hopkins University
18
Orbital Paths of Planets and Pluto
19
Orbit of UB 313 (Known as Xena)
NASA
20
Kuiper Belt Object Sizes
21
The International Astronomical Union Resolution
  • A planet is for the first time defined
    scientifically. A planet orbits a star, has
    sufficient gravity to become round, and has
    cleared the neighborhood around its orbit.
  • A Dwarf Planet orbits a star, is not a satellite,
    has sufficient gravity to become round and has
    not cleared the neighborhood of its orbit. Pluto
    is the prototype of this class and currently
    includes Ceres and UB 313. Others will be
    decided upon later.
  • A third class, Small Solar System Bodies, was
    defined as all other objects except satellites.
    This includes most asteroids, most comets and
    most trans Neptune objects.

22
So Long Planet Pluto and Hello Dwarf Planet
Pluto!
International Astronomical Union
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