3.5 completed star evolution module - harrisonburg...

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Notes: 3.5 STAR EVOLUTION Name: ________ Part 3: Re-read the highlighted information in your notes. Construct quiz questions using this information. Write the questions next to the paragraph where the answers can be found. Part 1: Fill in the blanks during the class discussion. Star Evolution Background “Evolve” or “Evolution” means to CHANGE. All stars change into different STAGES or phases throughout their life. What a star ends as depends on its MASS. A low mass star will evolve DIFFERENTLY than a high mass star. Stages of Star Evolution 1. Nebula: The BIRTH of a star. A nebula is CLOUD of dust and gas that is not a star yet. HYDROGEN is most common gases in a nebula. A nebula is also called a “Stellar NURSERY”. 2. Protostar: The material in a nebula CONDENSES and the star starts to come together. CONDENSE means the gases that will form the star begin to collect in the middle. The bright spots in Nebulas are PROTOSTARS will eventually become STARS. 3. Main Sequence star: This is the stage where the star “ SWITCHES ON”. The gravity in the core of the star is enough that FUSION begins. Fusion powers the star and turns the HYDROGEN gas into HELIUM. The equation for fusion is: H 1 + H 1 = He 2 + ENERGY. Unit 3.5 Star Evolution Nebula (the cloud) Protostars (bright spots)

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Notes: 3.5 STAR EVOLUTION Name: ________  Part 3: Re-read the highlighted information in your notes. Construct quiz questions using this information. Write the questions next to the paragraph where the answers can be found.  

Part 1: Fill in the blanks during the class discussion. Star Evolution Background

Ø “Evolve” or “Evolution” means to CHANGE. Ø All stars change into different STAGES or phases throughout their

life. Ø What a star ends as depends on its MASS. Ø A low mass star will evolve DIFFERENTLY than a high mass star.

Stages of Star Evolution 1. Nebula:

The BIRTH of a star. Ø A nebula is CLOUD of dust and gas

that is not a star yet. Ø HYDROGEN is most common

gases in a nebula. Ø A nebula is also called a “Stellar

NURSERY”. 2. Protostar: The material in a nebula CONDENSES and the star starts to come together.

Ø CONDENSE means the gases that will form the star begin to collect in the middle.

Ø The bright spots in Nebulas are PROTOSTARS will eventually become STARS.

3. Main Sequence star: Ø This is the stage where the star “

SWITCHES ON”. Ø The gravity in the core of the star is

enough that FUSION begins. Ø Fusion powers the star and turns the

HYDROGEN gas into HELIUM. Ø The equation for fusion is: H1 + H1=

He2 + ENERGY.

Unit    3.5      Star  Evolution    

Nebula  (the  cloud)  

Protostars  (bright  spots)    

4. Giant/SuperGiant Star: Ø Happens when the star runs out of HYDROGEN FUEL. Ø The star INCREASES in size Ø Small to average size stars become GIANT stars Ø Large Mass stars become SUPERGIANT.

5. Star Destruction-Planetary Nebula OR Supernova Once the star runs out of fuel for good it will be destroyed.

Ø A PLANETARY NEBULA is when a Giant star begins to fall apart and the outer layer of gas float out into space.

Ø A supernova is big EXPLOSION that happens when a Supergiant runs out of fuel

6. End of Stars Life. (White Dwarf, Neutron Star, or Black Hole Depending on its MASS a star will end its life as one of three things.

Ø White Dwarf: what SMALL or AVERAGE stars end as. • White Dwarf stars are SMALL, and DIM,

but hot.

Ø Neutron Stars. what MEDIUM LARGE stars end as. • Neutron stars emit RADIO WAVES instead of light.

Ø Black Holes: what the VERY LARGEST

stars end as. • Black holes have so much

GRAVITY that LIGHT cannot escape.

• Black holes may be located in the center of THE GALAXIES and may even hold the galaxies together.

• We could never travel to a black hole because of the distance, but if we could it IS possible it may be a path to another UNIVERSE.

The Life Cycle of our Sun

Ø The sun is currently 4.6 BY old. Ø At 10 BY of age, our sun will become a RED GIANT. Ø Our sun will end its life as a WHITE DWARF after 13 BY.

Part 2. Re-read your notes. Highlight the most important information