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Luminosity = Brightness - Weebly

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Assignments Page # TC 1 ___ 1. Scientific Inquiry notes 2. Hypothesis Practice ___ 3. Control and Experiment groups ___ 4. Introduction to Forces notes ___ 5. Newton's Laws of Motion notes ___ 6. Newton's Laws Practice ___ 7. Birth of the Earth ___ 8. Solar system notes ___ 9. Planet Facts Notes ___ 10. Sunlight and Earth Notes ___ 12. Moon Notes part 2 ___ 13. Solar and Lunar Eclipses Notes ___ 14. Life Cycle of Stars Notes ___ Luminosity = Brightness
Transcript
Page 1: Luminosity = Brightness - Weebly

Assignments Page #

TC 1

___1. Scientific Inquiry notes2. Hypothesis Practice ___3. Control and Experiment groups ___

4. Introduction to Forces notes ___5. Newton's Laws of Motion notes ___

6. Newton's Laws Practice ___7. Birth of the Earth ___8. Solar system notes ___

9. Planet Facts Notes ___10. Sunlight and Earth Notes ___

12. Moon Notes part 2 ___

13. Solar and Lunar Eclipses Notes ___14. Life Cycle of Stars Notes ___

Luminosity = Brightness

Page 2: Luminosity = Brightness - Weebly

Coordinates on a graph are usually identified

Temperature (K) Luminosity(Lsun)

1 30,000 105

2 35,000 10-2

3 30,000 10-3

4 5,000 105

5 8,500 10-1

6 6,500 10-1

7 26,000 101

8 15,000 101

9 3,750 10-3

10 4,000 102

11 38,000 103

12 3,000 106

13 12,500 1

14 20,000 105

15 20,000 10-4

16 17,000 1

17 5,000 10-2

Page 3: Luminosity = Brightness - Weebly

1

7

14

10

17

12

2

169

65

4

13

-1

3,7507,50015,00030,000

(26,000 , 101

1

7

14

10

17

12

2

16

9

65

4

13

-1

3,7507,50015,00030,000

Page 4: Luminosity = Brightness - Weebly

Think-Ink-Pair-Share

Which part of the flame do you think is the

Think-Ink-Pair-Share

Which part of the flame do you think is the

Page 5: Luminosity = Brightness - Weebly

Look at the graph,What do you notice about

the temperatures of the stars compared to

the color? Think-Ink-Pair-Share

14

10

17

12

2

3 9

8

13

-3

-1

1

3

5

3,7507,50015,000

Page 6: Luminosity = Brightness - Weebly

Hertzsprung-Russell Diagram

Page 7: Luminosity = Brightness - Weebly

Hertzsprung and Russell were two

astronomers that plotted on a diagram the

doing so, they realized that there was a

pattern with the stars' colors and the

temperatures as well. They found out that

the color of a star determines how hot it is.

The diagram became known as the HR

diagram named after both astronomers.

The HR Diagram is used to categorize the

stars in our universe by temperature and

brightness (luminosity)

Page 8: Luminosity = Brightness - Weebly
Page 9: Luminosity = Brightness - Weebly

What is a nursery?

In relation to stars, what do you think a

stellar nursery is?

What are stellar nurseries?

Stellar nurseries are areas of space with

large clusters of space dust and clouds

made up of helium, hydrogen, and other

gases.

Page 10: Luminosity = Brightness - Weebly

Stars are created from Nebulas

which is another name for stellar

nurseries.

The word nebula is Latin for "cloud"

Page 11: Luminosity = Brightness - Weebly

Nebulas collapse due to gravity and

years, the nebula starts to form

protosuns and then spit them out.

simulation of a condensing nebula

Page 12: Luminosity = Brightness - Weebly

When the center of the protosun gets

hot enough (around 3,000 Kelvin), it

will turn into a sun.

The size of the sun depends on how

much hydrogen or fuel was present

when the sun formed.

Page 13: Luminosity = Brightness - Weebly

As the sun burns

hydrogen and helium it expands

outwards, but gravity pulls the

expansion back.

Page 14: Luminosity = Brightness - Weebly

3 types of stars can form from a nebula. Thetype of star they become depends on howbig the nebula was that formed the sun.

3 types of stars can form from a nebula. Thetype of star they become depends on howbig the nebula was that formed the sun.

1. Brown Dwarf

3. Massive star

Page 15: Luminosity = Brightness - Weebly

Stop and think

1. Brown Dwarf

3. Massive star

Which one of the 3 types of stars do you

think our sun is? Give 1 reason for your

answer

1. Brown dwarf star

Brown dwarf stars are formed

when the mass of the protosun is

too small.

about 10% the

size of our sun

The size means the sun cannot

go through nuclear fusion and

therefore does not shine.

Page 16: Luminosity = Brightness - Weebly

formed when a protosun heats

up to about 3,000 Kelvin.

about half our

sun's size to

about 140x

The energy of an average sun

These suns burn at a medium

heat and are usually orange or

about half our

sun's size to

about 140x

Page 17: Luminosity = Brightness - Weebly

3. Massive star

nebula.immense heat and the sun radiates a

about 150x or

bigger than our

sun

Page 18: Luminosity = Brightness - Weebly
Page 19: Luminosity = Brightness - Weebly

near the end of its life.

This happens because the sun

will burn all of the hydrogen at its

core and will start burning its

helium reserves (this gives it the

red color).

Page 20: Luminosity = Brightness - Weebly

Red Giant Stars will eventually burn out their

remaining helium fuel and collapse on itself

due to the extreme force of gravity and turn

into a white dwarf star

the star down to the point where there are

no space between atoms or electrons.

Basically the same mass but 1/100 the

size

Page 21: Luminosity = Brightness - Weebly

white dwarf star will turn into a black dwarf

after about 1 quadrillion years.

No one knows what happens after a black

dwarf because time hasn't allowed a black

dwarf to form.

Our solar system is only 14 billion years old.

No black dwarfs currently exist!!!

Page 22: Luminosity = Brightness - Weebly

3. Massive star

nebula.immense heat and the sun radiates a

about 150x or

bigger than our

sun

Near the end of a massive star's life (blue or

white), the star will burn all of its hydrogen

and start burning helium as fuel.

Page 23: Luminosity = Brightness - Weebly
Page 24: Luminosity = Brightness - Weebly

supernova at the end of its life and can

depends on the size of the supernova.

Page 25: Luminosity = Brightness - Weebly

black hole.

Black holes bend time and space. Not

even light can escape its gravitational

pull.

Page 26: Luminosity = Brightness - Weebly

star and a new nebula.

Page 27: Luminosity = Brightness - Weebly

neutrons. It sends out deadly

electromagnetic waves that can kill whole

planets and solar systems.

Neutron stars are the most dense objects

in the universe

it pulls another space object like another


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