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Section 1.3 Pages 384-391 Distribution of Matter in Space

Distribution of Matter in Space

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Distribution of Matter in Space. Section 1.3 Pages 384-391. Stars. A star is a hot , glowing ball of gas (mainly hydrogen) that gives off light energy . Very hot stars look blue , while cooler stars look red . - PowerPoint PPT Presentation

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Page 1: Distribution of Matter in Space

Section 1.3Pages 384-391

Distribution of Matter in Space

Page 2: Distribution of Matter in Space

Stars A star is a hot, glowing

ball of gas (mainly hydrogen) that gives off light energy.

Very hot stars look blue, while cooler stars look red.

In the 1920's, Ejnar Hertzsprung and Henry Norris Russell compared the surface temperature of stars with its brightness (luminosity).

Stars fall into distinct groupings.

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Birth of Stars

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Birth of Stars

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SupernovaAn enormous explosion

that marks the death of a massive star.

Fusion has stopped and the star runs out of fuel.

Gravity causes the star to collapse upon its self.

The outer part of the star explodes with a shock wave.

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Black HolesA highly dense remnant

of a star in which gravity is so strong that not even light from radiation going on inside the remnant can escape.

Event horizon – point at which light cannot escape.

Invisible to telescopes.

This shows how the path of a beam of light bends in the vicinity of a non-rotating black hole.

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Star Groups Constellations are the

groupings of stars we see as patterns in the night sky.

There are 88 constellations and many are explained in Greek Mythology.

Asterisms are also groupings of stars but are not officially recognized as constellations.

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Galaxies A galaxy is a grouping of

millions or billions of stars, gas and dust.

Held together by gravity.

The Milky Way Galaxy is the galaxy our solar system is a part of.

It is shaped like a flattened pinwheel, with arms spiralling out from the center.

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Milky Way Galaxy

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Types of GalaxiesSpiral – long curved

arms radiating out from a bright central core – older to younger at the arms

Elliptical – football or egg – mostly old stars

Irregular – no notable shape – smaller size – mixture of young and old stars

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Section 1.4Pages 392-400

Our Solar Neighbourhood

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The SunThe Sun

emits charged particles in all directions.

This solar wind bombards the Earth at 400km/s, but the magnetic field of the Earth protects us.

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Protoplanet hypothesis1. A cloud of gas &

dust in space begin swirling

2. Most of the matter (more than 90% of it) accumulates in the center - forming the Sun

3. The remaining materials accumulate (forming planets) and circle the Sun

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The Planets: MercuryClosest planet to the

Sun

Surface similar to our moon

No atmosphere

High temperature – 400oC sunny side

- 180oC dark side

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The Planets: VenusSimilar in size, mass, and

gravity to earth

High surface temperature – 450oC (melt lead)

90 x atmospheric pressure to Earth

CO2 cloud cover

Rotates opposite to other planets – east to west

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The Planets: EarthOnly planet where water

exists in solid, liquid, and gas

Only planet to support life

Atmosphere provides protection from the Sun

70% surface covered in water

Active volcanism

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The Planets: MarsRed planet – orangish –

caused by iron oxides on surface

Two polar ice caps (One of Co2 + H2O and one of CO2)

Extremely cold surface temperature

Varied surface topography

2 moons

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The Planets: JupiterLargest of all planets

Twice the mass of all other planets combined

Composed of mainly hydrogen and helium

Great Red Spot – atmospheric storm

Three thin rings

28 moons

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The Planets: Saturn19 moons

Second largest planet

1000+ rings surround equator

Composed mostly of hydrogen and helium

High wind speeds over 1800 km/h due to fast rotation

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The Planets: UranusUnusual axis of rotation –

tilted toward the plane of its orbit –making it appear to roll its orbit

Composed mostly of hydrogen and helium

Methane in atmosphere gives it its blue colour

Large ring system

17 moons

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The Planets: Neptune Composed mostly of

hydrogen and helium, and methane

Methane in atmosphere gives it its blue colour

Little light reaches this planet

Fastest wind speed – 2500 km/h

Own ring system

8 moons

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The Planets: Pluto Cold frozen ball of methane

Disqualified as a Planet due to its obit around the sun at 17.2o – more elliptical

Rotates east to west rather than west to east

Some astronomers believe it and Charon (moon) are comets that have been captured by the gravity of the sun

Originated from the Kuiper Belt

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Other Celestial BodiesAsteroids – rocky ,

metallic bodies ranging in size of a few meters to hundreds of kilometres

Comets – dirty snowballs – dust and ice and heat up when they come close to the sun, releasing gas

Comets have predictable paths – large ellipses

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Other Celestial BodiesMeteoroids – small

pieces of rock flying through space with not particular path

Meteor – a meteoroid that gets pulled into the atmosphere by gravity – heats up and gives off light

Meteorite – a meteor that hits the surface

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Section 1.5Pages 401-407

Describing the Position of

Objects in Space

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AltitudeAltitude gives you the

"how above the horizon it is”

The point straight overhead has an altitude of +90 degrees

Straight underneath, an altitude of -90 degrees.

Points on the horizon have 0 degree altitudes.

An object halfway up in the sky has an altitude of 45 degrees.

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AzimuthAzimuth determines

"which compass direction it can be found in the sky."

An azimuth of zero degrees puts the object in the North.

An azimuth of 90 degrees puts the object in the East.

An azimuth of 180 degrees puts the object in the South, and one of 270 degrees puts the object in the west.

Zenith is the position in the sky directly overhead.

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Motion of Objects in SpaceThe path in the sky

along which the Sun takes is called the ecliptic.

The Celestial Sphere is the name given to the very large imaginary 'sphere of sky' surrounding the Earth.

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Assess Your LearningPage 406

Questions 2-3, 5-7, 10- 11, 13-15, 17

Read Section 2 pages 408-433