Warm Up What causes day and night? Why do we experience season’s? What divides the Earth into...
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Transcript of Warm Up What causes day and night? Why do we experience season’s? What divides the Earth into...
Warm Up What causes day and night?
Why do we experience season’s?
What divides the Earth into northern and southern hemispheres?
What is a revolution?
If the northern hemisphere is experiencing spring, what is the southern hemisphere experiencing?
Explain the difference between nutation and precession.
Activating
stratgegy1. 1) How many Earths do you think
would fit inside the Sun?2. 2) How hot do you think the Sun is?3. 3) How much longer do you think the
Sun will last? 4. 4) How many stars do you think
there are in our Milky Way?5. 5) How many stars do you think
there are in the whole universe?
Quote of the Day
Life is not about waiting for the storm to subside. It’s about learning to dance in the rain!
Objective & LEQ Objective: SWBAT analyze the
life cycle of stars and apply it to the Hertzsprung-Russell diagram.
LEQ: What determines the life cycle of a star and how is it applied to the Hertzsprung-Russell diagram?
Table of ContentsLeft Side Item Page Right Side Items Page
T-Chart Planets 0 Solar System Formation CN
1
Kepler 22b Article 0 Planetary Motion CN 3
Universe Venn Diagram
0 Star CN 5
Season’s Foldable 2
Season’s Graphic Organizer
2
HR Diagram 4
Star Foldable 4
Science GEMS of Wisdom
Page Avid Strategy W I C O R
0 T-Chart Planets
0 Kepler 22b Article
0 Universe Venn Diagram
2 Season’s Foldable
2 Season’s Graphic Organizer
4 HR Diagram
4 Star Foldable
Warm Up ANSWERS
1. 1 million (1,000,000!) Earths!
2. 10,000°million F!
3. About 7 billion more years
4. 200-400 billion
5. 100,000,000,000,000,000,000,000!
Quiz! You may use your notes
ABSOLUTELY NO TALKING First time, verbal warning and -5 points Second time, zero on your quiz
Once you are finished, hold up your quiz and I will collect it.
You have 3 things to finish: Make sure you have a SUMMARY written for your
notes yesterday (**remember, the summary answers the LEQ)!
Finish chunking/coloring notes Finish the worksheet and foldable (it was HW)
*Stages of a Star
A-Large star B-Crab NebulaC-Orion Nebula
D-Betelgeuse
E-Supernova
F-Nova Cygni
G-SupernovaH-Embryonic Star
Black Hole Video Clip
http://www.youtube.com/watch?v=h1iJXOUMJpg
Scientist Neil Degrasse Tyson
*What are the different ways that death would result from a black hole?
Characteristics of Stars Apparent magnitude: (a stars brightness as it appears
from EARTH) 1. how big it is 2. how hot it is 3. how far away it is
Absolute magnitude: how bright a star actually is.
(ex: 2 stars with equal absolute magnitudes may have difference apparent magnitudes because one is farther away!)
Luminosity measures absolute magnitude.
Surface temperature: how hot a star is (measured in Kelvins)
Characteristics of Stars HR Diagram:
A graph that shows the relationship between the absolute magnitude and temperature of stars.
The hottest main sequence stars are the brightest
The coolest main sequence stars are the dimmest.
Use the information on luminosity and apparent
magnitude to make a Hertzsprung-Russell diagram
(pg. 704)!Draw your own HR Diagram
using the chart on page 704 as an example!!
You have 20 minutes…work smart!
Depending on how big a star is, it will follow a certain life
path.
What determines the life cycle of a star?
FAST FACT In a few billion years, the sun’s core will run out
of hydrogen fuel, triggering nuclear fusion in the surrounding shell. As a result, the sun’s outer envelope will expand, producing a red giant hundreds of times larger and brighter. Intense solar radiation will boil Earth’s oceans, and solar winds will drive away Earth’s atmosphere.
Directions Complete the star foldable and
lifecycle diagram using pages 707-711 in your textbook for:
A) low-mass stars
B) medium-mass stars (sun-like)
C) massive stars
*Draw the life cycle stages for the 3 types of stars
This will be glued/taped onto page 6 of your notebook!
http://www.youtube.com/watch?v=YU6X3SPZAJo
Protostar the beginning stages of star formation when
gravity pulls in the gas and dusts from the star nursery and it begins to shine!
Red Giants a large bright star with a cool surface. It is
formed during the later stages of the evolution of a star like the Sun, as it runs out of hydrogen fuel at its center
White DwarfThought to be the final evolutionary state of all stars whose mass is not too high—over 97% of the stars in our Galaxy; when its nuclear energy is gone, I begin to contract and appear very bright
Black DwarfOver a very long time, a white dwarf will cool to temperatures at which it is no longer visible and become a cold black dwarf; become a lump of coal in the sky when all its nuclear energy is gone
Supernova type of death for Massive and Giant Blue Stars. They
are a stellar explosion of its content material with a burst of radiation that are very luminous
Blackholea region of space in which the gravitational field is so powerful that nothing, including light, can escape its pull. The black hole has a one-way surface, called an event horizon, into which objects can fall, but out of which nothing can come (form of death for massive stars)
Neutron staralso known as a Pulsar star because of its ‘pulsating’ effect that can be seen when viewed at a specific angle. The Pulsar Star is a result of the gravitational collapse of a Giant Blue Star
Stellar Match!
Cut out the star stages and definitions
Match the start stage with the correct definition
Glue it into your notebook on page 6
Using pages 704-714, match the type of star with its description.
You have 10 minutes to complete this activity.
Star Story: Write a short story following a star from birth to
death. Beginning At least 3 descriptive sentences about each stage. End
OR
Illustrate a comic book following a star from birth to death. Must have drawings AND text (speech/thought bubbles). Beginning At least 3 panels for each life stage. End
Textbook Activities
Read pages 703 – 704 and 706. Answer questions 4 – 5 on page 706.
Read pages 707 – 714. Answer questions 1-4 on page 714.
Read pages 622 – 624: Answer questions 1 and 2 on page 629.
Read pages 644 – 647: Answer questions 1-6 on page 648.