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The Solar System

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Chapter 2 The Solar System Part 3 – PowerPoint PPT presentation

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Title: The Solar System


1
Chapter 2
  • The Solar System
  • Part 3

2
Asteroids (Minor Planets)
  • Objects in the solar system smaller than a planet
    that are made of rock.
  • The first asteroid in space, named Ceres, was
    discovered in 1801. Since then over 250,000
    asteroids have been discovered and that number
    continues to rapidly increase every year. This
    despite that probably many asteroids are too
    small to be seen from Earth.

3
Asteroids
  • Ceres is still by far the largest known asteroid
    with a diameter of 623 miles. Only 26 have been
    discovered larger than 120 miles. Most are
    smaller than a mile across.
  • Asteroids are referred to by a number and its
    name. The number represents the order in which it
    was discovered. For example, Ceres is referred by
    1 Ceres since it was the first one discovered.

4
Asteroids
  • The space probe Galileo provided the first close
    images of an asteroid when it passed near and
    photographed 951 Gaspra and 243 Ida in the Main
    Asteroid Belt.
  • Galileos pictures revealed that Ida has a
    natural satellite, Dactyl. Ida is about 35 miles
    long and 15 miles in diameter. Its tiny moon is
    about a mile in diameter and orbits about 60
    miles above Ida. Since then several other
    asteroids have been found to have companions,
    leading astronomers to believe that it may not be
    uncommon.

5
Asteroids
  • Most asteroids reside in the Main Asteroid Belt
    between Mars and Jupiter. It is hypothesized that
    they are bits of primordial solar system material
    that was unable to form a planet due to Jupiters
    large gravitational influence.

6
Near Earth Asteroids
  • Gravitational perturbations mostly from Jupiter
    cause asteroids to occasionally leave the Main
    Asteroid Belt and wander the solar system. Those
    that come near Earth are called Near Earth
    Asteroids.
  • Asteroid collisions with Earth are known to be
    common in its history. Until the 1990s though, it
    was not recognized that they could significantly
    change conditions on Earth. This was brought
    about by the theory that an asteroid impact 65
    million years ago was responsible for the
    extinction of some 85 of all species, including
    all of the dinosaurs.

7
Near Earth Asteroids
  • There are currently 3168 discovered near earth
    asteroids. They are classified into 3
    categories
  • Apollo Asteroids that cross the orbits of both
    Earth and Mars.
  • Amors Asteroids that cross the orbit of Mars
    but not Earth.
  • Atens Asteroids that cross the orbit of Earth
    but not Mars.
  • The last close encounter happened last year when
    the peanut-shaped 3-mile long asteroid named 4179
    Toutatis passed within a million miles of Earth.

8
NEAR (Near Earth Asteroid Rendezvous)-Shoemaker
  • Mission launched in February 1996 to study near
    earth asteroids 253 Mathilde and 433 Eros.
  • First attempt to insert NEAR-Shoemaker into Eros
    orbit failed in 1998. The second attempt in 2000
    was successful though.
  • NEAR-Shoemaker conducted the first long-term
    close-up study of an asteroid mass, structure,
    geology, composition, and gravity.

9
NEAR-Shoemaker
  • Near-Shoemaker discovered that Eros has an
    ancient surface covered with craters, grooves,
    layers, house-sized boulders, and other complex
    features. It also seems to be a fragment of a
    larger body.
  • In February 2001, the NEAR spacecraft landed on
    asteroid Eros, after transmitting 69 close-up
    images of the surface during its final descent.

10
Asteroid Collision Prevention
  • Efforts to find near earth asteroids stepped up
    in 1998 with highly efficient automated systems
    that consist of cameras and computers directly
    connected to telescopes. Since then a large
    majority of the asteroids have been discovered by
    such automated systems .
  • Several theories exist as to how to prevent a
    collision with an asteroid. The most popular is
    the one to deflect the asteroid such that it
    misses Earth. How to exactly accomplish this is
    not exactly known.

11
Comets
  • Unlike the other small bodies in the solar
    system, comets have been known since antiquity.
    There are Chinese records of Comet Halley going
    back to at least 240 BC.
  • Comets are sometimes called dirty snowballs. They
    are a mixture of ices (both water and frozen
    gases) and dust that for some reason didn't get
    incorporated into planets when the solar system
    was formed. This makes them very interesting as
    samples of the early history of the solar system.

12
Comets
  • Comet Machholz
  • Comet Hale-Bopp
  • Comet C 2003 K Linear
  • Comet Neat
  • Comet Bradfield
  • Comet Halley
  • Comet Wild 2
  • Comet Shoemaker-Levi 9

13
Comets
  • Comets have several distinct parts
  • nucleus relatively solid and stable, mostly ice
    and gas with a small amount of dust and other
    solids.
  • coma dense cloud of water, carbon dioxide and
    other neutral gases sublimed from the nucleus
  • hydrogen cloud large but very sparse envelope of
    hydrogen surrounding the comet and sometimes
    trailing it

14
Comets
  • dust tail very long white tail composed of
    smoke-sized dust particles driven off the nucleus
    by escaping gases this is the most prominent
    part of a comet to the unaided eye
  • ion tail very long bluish tail composed of
    ionized gas caused by interactions with the solar
    wind. It always points away from the Sun.

15
Comets
  • Since both the coma and the tails are composed of
    material driven off the nucleus by solar heating,
    comets are invisible except when they are near
    the Sun.
  • Most comets have highly eccentric orbits which
    take them far beyond the orbit of Pluto these
    are seen once and then disappear for millennia.
    Only the short- and intermediate-period comets
    (like Comet Halley), stay within the orbit of
    Pluto for a significant fraction of their orbits.

16
Comets
  • Short-period comets are believed to originate in
    the Kuiper Belt. Other comets are theorized to
    come from the Oort cloud or perhaps from outside
    our solar system.
  • After 500 or so passes near the Sun off most of a
    comet's ice and gas is lost leaving a rocky
    object very much like an asteroid in appearance.
    (Many of the near-Earth asteroids may be "dead"
    comets.) A comet whose orbit takes it near the
    Sun is also likely to either impact one of the
    planets or the Sun or to be ejected out of the
    solar system by a close encounter (esp. with
    Jupiter).

17
Meteor Showers
  • A meteor shower sometimes occurs when the Earth
    passes through the orbit of a comet. Some occur
    with great regularity the Perseid meteor shower
    occurs every year between August 9 and 13 when
    the Earth passes thru the orbit of Comet
    Swift-Tuttle. Comet Halley is the source of the
    Orionid shower in October.

18
Comet Machholz
  • Good views of Comet Machholz are in store for
    northern hemisphere comet watchers in January.
    Now making its closest approach to planet Earth,
    the comet passed near the Pleiades star cluster
    on January 7th and the double star cluster in
    Perseus on January 27th as Machholz moves
    relatively quickly through the evening sky.
    Currently just visible to the unaided eye from
    dark locations, the comet should be an easy
    target in binoculars or a small telescope.
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