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Transcript
23.3 The Outer Planets
Pluto: Planet X
‹ Pluto’s orbit is highly eccentric, causing it
to occasionallyy travel inside the orbit of
Neptune, where it resided from 1979
through February 1999.
23.4 Minor Members of the Solar System
Asteroids: Microplanets
‹ An asteroid is a small, rocky body whose
diameter can range
g from a few hundred
kilometers to less than a kilometer.
‹ Most asteroids lie between the orbits of
Mars and Jupiter. They have orbital periods
of three to six years.
Irregular Orbits of Asteroids
23.4 Minor Members of the Solar System
Comets
‹ Comets are small bodies made of rocky
and metallic p
pieces held together
g
by
y frozen
gases. Comets generally revolve about the
sun in elongated orbits.
23.4 Minor Members of the Solar System
Comets
‹ Coma
• A coma is the fuzzy, gaseous component of a
comet’s head.
• A small glowing nucleus with a diameter of only
a few kilometers can sometimes be detected
within a coma. As comets approach the sun,
some, but not all, develop a tail that extends for
millions off kilometers.
Comet’s Tail Points Away from the Sun
23.4 Minor Members of the Solar System
Comets
‹ Kuiper Belt
• Like the asteroids in the inner solar system,
y
most
Kuiper belt comets move in nearly circular orbits
that lie roughly in the same plane as the planets.
‹ Oort Cloud
• Comets with long orbital periods appear to be
distributed
d
st buted in all
a directions
d ect o s from
o tthe
e su
sun,, forming
o
g
a spherical shell around the solar system called
the Oort cloud.
23.4 Minor Members of the Solar System
Comets
‹ Halley’s Comet
• The most famous short-period
p
comet is Halley’s
y
comet. Its orbital period is 76 years.
23.4 Minor Members of the Solar System
Meteoroids
‹ A meteoroid is a small, solid particle that
travels through
g space.
p
‹ A meteor is the luminous phenomenon
observed when a meteoroid enters Earth’s
atmosphere and burns up, popularly called
a shooting star.
‹ A meteorite
t
it is
i any portion
ti off a meteoroid
t
id
that reaches Earth’s surface.
23.4 Minor Members of the Solar System
Meteoroids
‹ Most meteoroids originate from any one of
the following
g three sources: ((1))
interplanetary debris that was not
gravitationally swept up by the planets
d i th
during
the fformation
ti off the
th solar
l system,
t
(2)
material from the asteroid belt, or (3) the
solid remains of comets that once traveled
near Earth’s orbit.
Meteor Shower
These meteorites broke off from the
Comet Swift-Tuttle
Swift Tuttle
Major Meteor Showers