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Small Bodies of the Solar System

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Small Bodies of the Solar System. Pluto, Comets, Asteroids, Meteors and ... God of the Underworld. Pluto Physical Data. Discovered by Clyde W. Tombaugh in 1930 ... – PowerPoint PPT presentation

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Title: Small Bodies of the Solar System


1
Small Bodies of the Solar System
  • Pluto, Comets, Asteroids,
  • Meteors and Zodiacal Light

2
PLUTOGod of the Underworld
3
Pluto Physical Data
  • Discovered by Clyde W. Tombaugh in 1930
  • Diameter 2294 km (0.18 Dearth)
  • Mass 1.2x1025 g (0.002 Mearth)
  • Density 1.84 g/cm3
  • Rotation Period 6.39 days
  • Tilt of Axis 96o (retrograde!)
  • Surface Temperature 43 K (-382o F)

4
Pluto Physical Data
  • Orbital Semi-Major Axis 39.44 AU
  • Orbital Period 247.7 years
  • Orbital Inclination 17.2o
  • Orbital Eccentricity 0.250
  • Surface Gravity 0.06 Earth gravity
  • Satellites 1
  • Magnetic Field unknown

5
The Discovery of Planet X
  • Discovered Feb 8, 1930 by then 24-year old Clyde
    Tombaugh
  • Its existence was predicted by Percival Lowell
    using the same techniques that Leverrier used to
    find Neptune

6
The Discovery of Planet X
January 23, 1930
January 29, 1930
The Plates on which Clyde Tombaugh found Pluto
7
Plutos Surface
  • This image was taken by the Hubble Space
    Telescope and is the best surface map yet made
  • Only contrasts are seen, no features
  • Pluto has not yet been visited by spacecraft

8
Plutos Atmosphere
  • Very thin atmosphere (when closest to Sun)
  • Envelopes its moon too
  • Mostly made of Nitrogen and Methane
  • Atmosphere condenses and snows to the surface of
    Pluto and its moon when they are farther from the
    Sun

9
Plutos Moon
  • CHARON
  • Discovered by James Christy in 1978
  • Saw a bump move from one side of Pluto to the
    other about every six days
  • About half the size of Pluto, orbits retrograde

One of Christys images
10
Plutos Moon
  • As seen by Hubble Space Telescope

Charon
Pluto
19,700 km
11
Plutos Strange Orbit
  • Plutos Orbit is highly eccentric (0.250), highly
    inclined to the plane of the solar system
    (17.2o), and its orbit crosses Neptunes!
  • Since Jan 23, 1979 and until March 15,1999 Pluto
    is closer to the Sun the Neptune!

12
Plutos Orgin
  • Since Pluto and Charon are thought to have the
    same composition as Neptunes Triton, it is
    suggested that they might be escaped satellites
    of Neptune (dynamicists say no)
  • Or Triton, Pluto and Charon all formed near
    Neptune and only Triton was captured

13
Asteroids
14
The Asteroid Belt
  • Theory 1
  • Material between Jupiter and Mars tried to form a
    planet when the Solar System was forming, but
    Jupiters gravitational influence wouldnt let it
    happen
  • Theory 2
  • A planet did form between Jupiter and Mars
    (Asteroidia), and some catastrophic event
    destroyed the planet, leaving the asteroids

15
The Discovery of Asteroids
  • On the first day of the 19th C. (Jan 1,1801),
    Ceres (the largest known asteroid) was discovered
    by Giuseppe Piazzi
  • By the end of the 19th C., several hundred were
    known
  • We now know of more than 7000


16
Particular Asteroids
  • CERES
  • The largest asteroid by far
  • Diameter 914 km
  • Contains 25 of the mass of all the asteroids
    combined
  • The next largest are Pallas, Vesta, and Hygiea
    which are between 400 and 525 km in diameter
  • All other known asteroids are less than 340 km
    across

17
Particular Asteroids
IIDA and DACTYL
  • Ida was encountered by the Galileo spacecraft in
    1993
  • Ida was found to have a small satellite, Dactyl
  • Dactyls size is 1.6 x 1.2 km, and orbits 90 km
    above Ida

18
Comets
Comet West
19
Comet Basics
  • Comets are mostly (50) water ice
  • Comets are referred to as dirty snowballs
  • They are a mixture of water ice, frozen gases,
    and silicate materials
  • Comets have very eccentric orbits
  • They only have tails when close to the Sun
  • The tails are made of gas and dust released by
    the comet.

20
Anatomy of a Comet

Ion Tail
Direction of Comets Motion
Coma
Nucleus
Hydrogen Cloud
Dust Tail
To Sun
21
History of Comets
m
22
Comet Halley
  • Orbits Sun every 76 years
  • Furthest point in its orbit is just beyond the
    orbit of Neptune
  • Nucleus 15 x 8 x 8 km
  • Rotates every 7.6 days

23
Recent Comets
  • Comet Hyakutake in March of 1996

Image taken by J. De Buizer and J. Radomski of
the University of Florida Department of Astronomy
24
Recent Comets
  • Comet Hale-Bopp in March 1997
  • Image taken by J. DeBuizer and J.Radomski of
    the University of Florida Department of Astronomy

25
Meteors, Meteorites, and Meteor Showers
26
Meteor Nomenclature
  • Meteoroids - interplanetary debris
  • Meteor - Also called shooting star
  • When a meteorite has entered the
  • atmosphere creating a streak of
    light
  • Meteorite - Those few meteoroids that make
  • it to the Earths surface

27
Types of Meteorites
IRONS
  • Mostly made of iron with about 9 nickel

STONES
  • Primarily silicates similar to Earth rocks

STONY-IRONS
  • Mixture of the above two types

28
Meteor Showers
  • Associated with debris left behind by comets
  • Typically very small meteoroids, so no meteorites
    are produced during a shower
  • Can be as many as 100 meteors per hour in a good
    shower


29
Meteor Impacts
  • One catastrophic meteor impact every 26 million
    years
  • Might have been responsible for dinosaur
    extinction

Barringer crater in Arizona (1200 m in diameter,
200 m deep)
30
Zodiacal Light and Gegenschein
  • Zodiacal light is due to dust, concentrated in
    the plane of the solar system, that reflects the
    light of the Sun towards our eyes
  • Reflection from the dust also causes a patch of
    light directly opposite the Sun, called the
    gegenschein

Ecliptic
Zodiacal Light
Horizon
Sun
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