Chapter 3 Flashcards

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1
Q

The Greeks

A
  • Named “moving stars”, PLANETS from the Greek word meaning “wanderers”
  • had a GEOMETRIC (geo for earth) view of the solar system- thought the earth was the center of revolving planets.
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2
Q

Ptolemy’s view

A

He thought that as each planet revolved the earth they moved in different directions in big and little circles.

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3
Q

Nicolaus Copernicus

A
  • a polish astronomer
  • in 1543 developed a HELIOCENTRIC (sun centered) view of the solar system which he explained the movements of the 6 known planets.
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4
Q

Galileo Galilei

A
  • made 2 discoveries to support the heliocentric view in the 1600’s
  • saw 4 moons revolving around Jupiter
  • observed that Venus appeared to go through phases like the Moon
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5
Q

Tycho Brahe and Johannes Kepler

A
  • Brahe made careful planetary observations in the late1500’s that Kepler, his assistant, analyzed in the early 1600’s.
  • Kepler was the first person to determine that planets had elliptical orbits.
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6
Q

Sun’s gravity

A

the most powerful force in the solar system

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7
Q

Sun’s mass

A

99.8% of solar system mass

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8
Q

Sun composition

A

Ball of glowing gas ¾ hydrogen, ¼ helium, very small amounts of other elements

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9
Q

Sun facts

A
  • The Sun rotates on its axis

* The Sun has an atmosphere

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10
Q

Nuclear fusion

A

The Sun’s energy comes from nuclear fusion – under extremely high temperatures and pressure hydrogen atoms join together to form helium (mass is converted to energy)

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11
Q

Three Parts of the Sun

A
  1. Core
  2. Radiation Zone
  3. Convection Zone
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12
Q

Sun’s Core

A
  • central region
  • temperature = 15 million degrees Celsius
  • produces the energy
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13
Q

Sun’s Radiation Zone

A
  • middle layer
  • Consists of very tightly packed gas where the energy from the core is transferred in the form of electromagnetic radiation
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14
Q

Sun’s Convection Zone

A

outermost layer

•The gases travel in circular convection currents here

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15
Q

The Sun’s Atmosphere

3 Layers

A
  1. Photosphere
  2. Chromosphere
  3. Corona
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16
Q

Photosphere

A

inner sphere
•Photos means “light” in Greek
•Gives off visible light

17
Q

Chromosphere

A

middle layer (color)
•Chroma means “color” in Greek
•Visible during solar eclipse (reddish color)

18
Q

Corona

A

outer layer
•Corona means “crown” in Latin
•Visible during solar eclipse (looks like a halo)
•Extends into space for millions of km
•Sends out a stream of electrically charged particles – solar wind, which on Earth is blocked by our magnetic field, except at the poles.

19
Q

Solar wind

A

Corona sends out a stream of electrically charged particles – solar wind, which on Earth is blocked by our magnetic field, except at the poles.
We see northern and southern lights.

20
Q

Sunspots

A
  • areas of gas that are cooler than the gases around them in the photosphere
  • Can be the larger than the size of the Earth
  • Number of sunspots vary over a period of about 11 years.
21
Q

Prominences

A

reddish loops of gas that link pairs/groups of sunspots

22
Q

Comets

A

chunks of ice and dust whose orbits are usually very long, narrow ellipses

23
Q

Comet parts

A

•When close to the Sun, solar energy turns the ice into gas, releasing dust forming an outer layer called the coma.
•The inner layer is called the nucleus
The brightest part is the head which is made of the nucleus and the coma.
•Solar wind pushes the gas from the comet away from the Sun forming the tail (can be hundreds of millions of km long)
•Actually have 2 tails (one gas and one dust)
•Comet means “long-haired star” in Greek

24
Q

Edmond Halley

A

(1705) calculated orbits of 24 comets

25
Q

Asteroids

A

small rocky objects that orbit the Sun

most revolve around the Sun between the orbits of Mars and Jupiter (this region is known as the asteroid belt)

26
Q

Meteoroid

A

a chunk of rock or dust IN SPACE that usually comes from comets or asteroids

27
Q

Meteor

A

when a meteoroid enters the EATHS ATMOSPHERE friction makes it burn up and produce a streak of light.
SHOOTING STAR 💫

28
Q

Meteorites

A

when meteoroids are large enough to pass through the atmosphere and hit the EARTHS SURFACE