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Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
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Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Dec 18, 2015

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Page 1: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Unit 47

Comets

Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Page 2: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

The Structure of Comets

• Comets have two primary parts, the head and the tail

• The head consists of– The nucleus, a lump of

frozen gas mixed with loose rock and dust

• Only about 10 km across

• Dark in color, probably from dust and other materials

– The coma, the cloud of evaporated ices and gases streaming from the surface of the nucleus

• May be 100,000 km wide!

• The tail can be hundreds of millions of km long, and streams directly away from the Sun

Page 3: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Visiting Comets

Comet Halley, visited by Giotto

Comet Wild 2, visited by Stardust

Comet Tempel 1, visited by Deep Impact

Page 4: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

The Origin of Comets

• Comets may originate in either the Oort Cloud or the Kuiper Belt– Oort cloud is a cloud of

comet-like planetesimals more than 100,000 AU from the Sun

– Oort cloud objects may have formed near the giant planets and then were tossed outwards by gravitational forces

• Passing stars or other gravitational influences nudge the comets into the inner Solar System

Page 5: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

How a comet becomes visible

• As a comet moves into the inner solar system, it is warmed by the sun

– Ices on the surface sublimate (go from solid to gas) and stream away from the comet nucleus

– The sublimated gases form the coma

– Escaping gas carries dust particles outward

• Solar photons strike the dust particles, pushing them away

– Process is called radiation pressure

– This forms the dust tail!

• Gas and ions in the coma are pushed away from the nucleus by the solar wind

– This forms the ion tail, and usually points directly away from the Sun

• Gas in the coma and tail are lit up by the Sun, making them visible (fluorescence)

Page 6: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

The Two Tails of a Comet

Page 7: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Another View of the Process

Page 8: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Meteor Showers

• As a comet orbits the sun, it leaves a trail of dust behind it.

• Occasionally, the Earth passes through one of these dust trails– Dust particles enter

Earth’s atmosphere and burn up

– We see them as meteors, in a meteor shower

• The meteors all appear to be coming from the same point in the sky called the radiant

Page 9: Unit 47 Comets Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

The Names of Meteor Showers

• We name the meteor shower after what constellation the radiant is located in

• Perseus – Perseids

• Leo - Leonids

and so on