characteristics of stars
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Characteristics of Stars. Astronomy Chapter 3.2 Pages 103-109. What is a Star?. A star is a sphere of super-hot gases Mostly Hydrogen and Helium 1 to 2 percent of a stars mass may consist of heavier elements. The Sun. Our solar system’s star The Sun is 150 million km away from Earth - PowerPoint PPT PresentationTRANSCRIPT
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Characteristics of Stars
Astronomy Chapter 3.2Pages 103-109
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• A star is a sphere of super-hot gases– Mostly Hydrogen and
Helium
• 1 to 2 percent of a stars mass may consist of heavier elements.
What is a Star?
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• Our solar system’s star
• The Sun is 150 million km away from EarthLight from the Sun
takes 8 minutes to reach Earth
The Sun
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• Billions of galaxies make up the universe
• All of space and everything in it make up the universe.
The Universe
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Massive cluster of stars is called a galaxy• It would take you 25,000 years to travel to the
center (250 million billion km) of our galaxy at the speed of light.
Milky Way Galaxy
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• Our neighboring galaxy
• Would take 2 million years to reach at the speed of light
• This galaxy is visible to the naked eye on a clear night.
Andromeda Galaxy
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4) Helium
2) Nitrogen
3) Hydrogen
1) Oxygen
What is the most abundant element in most stars?
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4) 25,000 years ago
2) 2 million years ago
3) 300,000 years ago
1) 10 million years ago
When did the light that you see actually leave the Andromeda galaxy?
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Distance to Stars• Earth is about 150 million km from the Sun
(93million miles)• That is equal to 1 Astronomical Unit (AU)
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Distance to Stars• Since Stars are so far
away:– A light year is used to
express great distances.– Light travels at 300,000
km/s– 1 light year = distance a
ray of light travels in 1 year (9.5 trillion km.)
Horsehead Nebula is 1,500 light years away)
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• The next closest star is 40 trillion km from the Sun (more than 260,000AU)
• Light takes 4.3 years to reach Earth
• Most stars are much further away
Proxima Centauri
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• Stars appear to be the same distance from Earth in the night sky
• How do we know that they are not?
Distance to Stars
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Parallax• Parallax: the apparent
change in position of an object when you look at it from different positions.
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• Only works for nearby stars (less than 1,000 light years away)
• Astronomers look at the star when Earth is on one side of the sun and again six months later.
Distance to Stars
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• They measure how much the star appears to move against the background of stars• The less the star appears to move the
further away it is.
Distance to Stars
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Distance to Stars
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What is the speed of light?
4) 25,000 m/s
2) 2 million m/s
3) 300,000km/s
1) 10 km/s
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Characteristics
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• Size (Mass)
• Color & Temperature
• Brightness
Classifying Stars
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Mass (size)• Mass is the total amount of
material in a body– How much “stuff” or matter
something contains
• Some stars are five, ten or more times the size of our Sun. Others are less massive.
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Medium Size Star - Our Sun
Types of Stars
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Giant Stars – are 10 to 100 times larger, having no more Hydrogen
Rigel
Types of Stars
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Super Giant – 10 to 70 times more massive V838 Monocerotis
Types of Stars
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White Dwarf - about the size of Earth, but with the mass of the Sun
Types of Stars
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Neutron Star – stars that are super small, super massive, and have become pure neutrons
Types of Stars
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4) Density
2) Gases present
3) Color
1) Temperature
If a star can differ in volume (size) and mass, what else will
differ as a result?
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Density of a Star• One teaspoon full of material from Sirius
(White Dwarf) is so dense that on Earth it would weigh a ton.
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4) Blue
2) Orange
3) Yellow
1) Red
What color would you expect a cool star to glow?
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3) Yellow
2) Orange
4) Blue
1) Red
What color would you expect a hot star to glow?
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Temperature
• How can the temperature of a star be determined?– By the color
• Red Stars = Cool• Blue Stars= Hot
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4) 50,000˚C
2) 5,500˚C
3) 10,000˚C
1) 3,900˚C
The Sun is a yellow star, what temperature would you expect
the sun to be close to?
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1. Red Stars ~ 3,000◦C (Betelgeuse)
2. Red-Orange Stars ~ 5,000 ◦C (Aldebaran)
3. Yellow Stars ~ 5,500◦C – 6,000 ◦C (Sun)
4. White Stars ~ 10,000◦C (Sirius)
5. Blue Stars ~ more than 15,000◦C (Rigel)
Temperatures & Colors
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• Stars are far from Earth
• As a result, what problem does this cause?– Cannot accurately determine the actual
brightness of a star from earth
• How bright a star appears from Earth depends on far away the star is.
Brightness (Luminosity)
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• Brightness depends on size and temperature
• Betelgeuse is large but cool. Its size makes it appear bright
• Rigel is smaller but is very hot so it shines brightly.
Brightness (Luminosity)
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Apparent Magnitude• The measure of how bright a star appears
to be from earth.– Less bright objects that are closer to you
could be seem brighter than objects that are far and actually brighter
• The lower the magnitude the brighter the star.
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• The brightness of a star if it was set at a standard distance from Earth.
– Astronomers calculate the star’s apparent magnitude and its distance from Earth.
– Then calculate the brightness if it were a standard distance from Earth.
Absolute Magnitude
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4) Size and temperature of a star
2) Brightness of a star at a set distance3) Temperature of a star
1) How bright a star appears to be
Absolute Magnitude determines…
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HR- Diagram
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• Herzsprung and Russell
• A graph used to find out if temperature and brightness are related.
• Plots Absolute Magnitude vs. Surface Temperature.
HR-Diagram
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• More than 90% of stars are Main Sequence, form a diagonal band.
HR- Diagram
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What to Work On• Read Section 3.2, pages 103-109• Answer the section review questions on
page 109 (#’s 1-4)
DUE: Friday, April 13th