Download WebQuest-The-Life-Cycle-of-Stars-1

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Chinese astronomy wikipedia , lookup

Star of Bethlehem wikipedia , lookup

History of astronomy wikipedia , lookup

Formation and evolution of the Solar System wikipedia , lookup

History of Solar System formation and evolution hypotheses wikipedia , lookup

Aries (constellation) wikipedia , lookup

International Ultraviolet Explorer wikipedia , lookup

Serpens wikipedia , lookup

Observational astronomy wikipedia , lookup

Constellation wikipedia , lookup

Corona Borealis wikipedia , lookup

Auriga (constellation) wikipedia , lookup

Canis Minor wikipedia , lookup

Corona Australis wikipedia , lookup

Boötes wikipedia , lookup

Cassiopeia (constellation) wikipedia , lookup

Canis Major wikipedia , lookup

Type II supernova wikipedia , lookup

Cygnus (constellation) wikipedia , lookup

Perseus (constellation) wikipedia , lookup

Ursa Major wikipedia , lookup

CoRoT wikipedia , lookup

Lyra wikipedia , lookup

Hipparcos wikipedia , lookup

Star catalogue wikipedia , lookup

Star wikipedia , lookup

Stellar classification wikipedia , lookup

Future of an expanding universe wikipedia , lookup

Aquarius (constellation) wikipedia , lookup

H II region wikipedia , lookup

Astronomical spectroscopy wikipedia , lookup

Ursa Minor wikipedia , lookup

Stellar kinematics wikipedia , lookup

Timeline of astronomy wikipedia , lookup

Corvus (constellation) wikipedia , lookup

Stellar evolution wikipedia , lookup

Star formation wikipedia , lookup

Transcript
The Life Cycle of Stars
Name
When finished – email to me (or share it with me via google docs) : [email protected]
Purpose:
1. In this webquest, you will learn how to identify stars by their magnitude, color, temperature, and spectral
class.
2. You will investigate the process of nuclear fusion explained by Einstein's famous equation
E = MC2 and learn how mass in the form of hydrogen atoms is converted to helium and causes a release of
energy that makes stars shine.
3. You will also begin to understand the forces involved in stars that maintain this nuclear reaction and how
these forces change as the star ages.
4. You will explore the stages stars progress through from birth to death and how the death of a star
depends on its initial mass.
Task #1: Lights in the Sky
Go to the website http://www.seasky.org/cosmic/sky7a01.html and answer the following questions:
1. What are constellations?
2. What is a star's brightness
known as?
3. How do astronomers rate
the magnitude of a star?
4. What is the brightest star
in the known universe?
5. Are the brightest stars low
magnitude or high
magnitude?
6. Stars are identified by their
color; what does the color
indicate?
7. What color is the hottest
star?
8. What color is the coolest
star?
9. What color is our sun?
Task #2: A Nuclear Furnace
Continue to read on to the section “A Nuclear Furnace” on the same webpage
http://www.seasky.org/cosmic/sky7a01.html and answer the following questions:
1. The nuclear reactions
inside a star, such as our sun,
convert hydrogen into
helium by means of a process
known as.
2. What gives a star its
energy?
3. How many protons does a
standard hydrogen atom
have in its nucleus?
4. How many neutrons does
a standard hydrogen atom
have in its nucleus?
5. The animation shows how
stars fuse the hydrogen
deuterium and hydrogen
tritium to form helium. Use
colored pencil to draw a
diagram that shows this
nuclear reaction. Label the
names of the atoms and
draw arrows showing the
progression of the reaction
.
Task #3: The Circle of Life
Continue to read on to the section “The Circle of Life” on the same webpage
http://www.seasky.org/cosmic/sky7a01.html and answer the following questions:
1. Stars begin their lives as clouds of
dust and gas called.
2. What is a protostar?
3. When does nuclear fusion begin?
4. The life span of a star depends on
5. Very large, massive stars burn
their fuel much ___________ than
smaller stars.
6. The life span of smaller stars are
much __________ than that of large,
massive stars
7. When will a star become a red
giant?
8. Why do some stars become super
red giant?
9. What will happen when a star
exhausts its remaining fuel?
10. What is a planetary nebula?
11. What is a white dwarf?
12. What produces all of the heavy
elements required for life?
13. What are we made of?
14. Using colored pencils (if you have some) , draw a diagram of the life cycle of a star:
Task #4: Types of Stars
Continue to read on to the section “Types of Stars” on the same webpage
http://www.seasky.org/cosmic/sky7a01.html and answer the following questions:
1. What does the main
sequence represent?
2. Is our sun a main sequence
star?
3. What will decide the
amount of time a star spends
in the main sequence phase?
4. Large, massive stars will have a _____________ main sequence stage while less
massive stars will
have a _________ main sequence stage.
5. What is a red giant?
6. What is a white dwarf?
Task #5: Life Cycle of Stars
Go to the website http://map.gsfc.nasa.gov/universe/rel_stars.html. Read the short section on “Where are stars born”
and see pictures of the protostars of M16: The Eagle Nebula and other nebulae on this page. Continue by reading up
on Main Sequence Stars and find out how our sun compares in mass to other stars.
1) Compare the mass of our sun to
Sirius? To Proxima Centauri?
2) Based on its mass, will our sun be
around for a while?
3) What will our Sun become when it
runs out of hydrogen fuel and has
exhausted its ability to fuse other
elements like carbon and oxygen?
4) Approximately how long before our
sun grows large and consumes the
inner planets of our solar system?
5) - Which size of stars has longer life
spans, ones with more mass or less
mass?