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Meteors, Meteorites, and Meteor Showers. Meteor Terminology Meteoroids - interplanetary debris Meteor - Also called “shooting star” When a meteorite has.

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Presentation on theme: "Meteors, Meteorites, and Meteor Showers. Meteor Terminology Meteoroids - interplanetary debris Meteor - Also called “shooting star” When a meteorite has."— Presentation transcript:

1 Meteors, Meteorites, and Meteor Showers

2 Meteor Terminology 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 Earth’s surface

3 Types of Meteorites Mostly made of iron with about 9% nickel IRONS: STONES: Primarily silicates similar to Earth rocks STONY-IRONS: Mixture of the above two types

4 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

5 Major Meteor Showers Often named for the constellation they fall from NameWhen# per hourConstellation Quadrantids Jan.30-40Bootes PerseidsAug.50-70Perseus LeonidsNov.50-70Leo GeminidsDec.40-50 (multi-colored) Gemini

6 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)

7 Comets Comet West

8 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.

9 Anatomy of a Comet Dust Tail Ion Tail Coma Direction of Comet’s Motion To Sun Nucleus Hydrogen Cloud

10 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

11 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

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

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

14 PLUTO God of the Underworld

15 Pluto Physical Data Discovered by Clyde W. Tombaugh in 1930 Diameter: 2294 km (0.18 D earth ) Mass: 1.2x10 25 g (0.002 M earth ) Density: 1.84 g/cm 3 Rotation Period: 6.39 days Tilt of Axis: 96 o (retrograde!) Surface Temperature: 43 K (-382 o F)

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

17 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

18 The Discovery of Planet X The Plates on which Clyde Tombaugh found Pluto January 23, 1930January 29, 1930

19 Pluto’s 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

20 Pluto’s 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

21 Pluto’s 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 Christy’s images

22 Pluto’s Moon As seen by Hubble Space Telescope 19,700 km Pluto Charon

23 Pluto’s Strange Orbit Pluto’s Orbit is highly eccentric (0.250), highly inclined to the plane of the solar system (17.2 o ), and its orbit crosses Neptune’s! Since Jan 23, 1979 and until March 15,1999 Pluto is closer to the Sun the Neptune!

24 Pluto’s Orgin Since Pluto and Charon are thought to have the same composition as Neptune’s 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

25 Asteroids

26 The Asteroid Belt Theory 1: Material between Jupiter and Mars tried to form a planet when the Solar System was forming, but Jupiter’s gravitational influence wouldn’t let it happen Theory 2: A planet did form between Jupiter and Mars (Asteroidia), and some catastrophic event destroyed the planet, leaving the asteroids

27 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

28 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

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

30 History of Comets m

31 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 Sun Horizon Zodiacal Light


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