The Life Cycle of Stars: Chapter 8, Section 2 - PowerPoint PPT Presentation


PPT – The Life Cycle of Stars: Chapter 8, Section 2 PowerPoint presentation | free to view - id: 79a7f2-ZTQ2Y


The Adobe Flash plugin is needed to view this content

Get the plugin now

View by Category
About This Presentation

The Life Cycle of Stars: Chapter 8, Section 2


The Life Cycle of Stars: Chapter 8, Section 2 What we are going to learn today about the life cycle of Stars The different types of stars How to read an H-R diagram ... – PowerPoint PPT presentation

Number of Views:139
Avg rating:3.0/5.0
Slides: 20
Provided by: Susi59
Tags: chapter | cycle | life | rigel | section | star | stars


Write a Comment
User Comments (0)
Transcript and Presenter's Notes

Title: The Life Cycle of Stars: Chapter 8, Section 2

The Life Cycle of Stars Chapter 8, Section 2
What we are going to learn today about the life
cycle of Stars
  • The different types of stars
  • How to read an H-R diagram
  • How stars appear at different stages in their
    life cycle on the H-R diagram.

The Beginning and End of Stars
  • The Beginning A star enters the first stage of
    its life cycle as a ball of gas and dust. Gravity
    pulls the gas and dust together, and hydrogen
    changes to helium in a processes called nuclear
  • The End Stars usually lose material slowly, but
    sometimes they can lose material in a big
    explosion. Much of a stars material returns to
    space, where it sometimes forms new stars..
  • How many stars are estimated to
  • be in our Milky Way Galaxy?
  • 200,000,000,000

Different Types of Stars
  • Stars can be classified by their size, mass,
    brightness, color, temperature, spectrum, and
    age. A stars classification can change as it
  • Main-Sequence Stars After a star forms, it
    enters the second and longest stage of its life
    cycle known as the main sequence. Energy is
    generated in the core as hydrogen atoms fuse into
    helium atoms.
  • What kind of star is our sun??

Main Sequence Star System Alpha Centauri, 25
trillion miles away
Red Giants
  • A red giant is a large, reddish (usually main
    sequence) star late in its life cycle, or third
  • As the center of the star shrinks, the
    atmosphere of the star grows very large and
    cools to form a red giant or a red supergiant.
  • This is Betelgeuse, a red giant star
  • in the Milky Way. Who has seen
  • it through a telescope? In what
  • Constellation is it located?

Orion Constellation
White Dwarf Stars
  • In the final stage of its life cycle, a star that
    has the same mass as the sun (main sequence star)
    or smaller can be classified as a white dwarf.
  • A white dwarf is a small, hot dim star that is
    the leftover center of an old star.
  • It has no hydrogen left and cannot generate
    energy any more by nuclear fusion, but it can
    shine for billions of years before cooling
  • In what constellation is there
  • a white dwarf in our galaxy?
  • White Dwarf Stars

White Dwarf Sirius Blue Supergiant Rigel
H-R Diagram A graph for studying the stars
  • The H-R Diagram (Hertzprung-Russell diagram) is a
    graph that shows the relationship between a
    stars surface temperature and its absolute
  • Reading the H-R Diagram The diagonal pattern on
    the H-R diagram where most stars lie, is called
    the main sequence.
  • Where is our sun?
  • The main sequence
  • is the location on
  • the diagram where
  • most stars lie

H-R Diagram
  • How hot is the surface of the sun?
  • 5,000 6,000 C or 10,000 F

  • According to the H-R diagram, what types of
    stars have very low temperatures and high
    absolute magnitudes?
  • A blue stars
  • B red giants
  • C white dwarfs

When stars get old
  • When main sequence stars get old (such as our
    sun) they become red giants and then white dwarfs
    at the end of their life cycle.
  • Massive stars, however, generate much more energy
    and also dont last as long.
  • Massive stars may explode with such intensity
    that they may become supernovas, neutron stars,
    pulsars, or black holes.
  • What will our sun probably become in its next

  • A supernova is a gigantic explosion in which a
    massive star collapses and throws its outer
    layers into space.
  • Supernova NGC 6826
  • Its green gas is almost
  • half of its mass.

Neutron Star
  • After the supernova explosion, the center of the
    collapsed star contracts to form a new star. It
    has been smashed together so forcefully that all
    of its particles have become neutrons.

  • When a neutron star is rapidly spinning, it is
    called PULSAR. It emits rapid pulses of radio
    waves and optical energy.
  • This is Pulsar B1509. It is spinning so
    rapidly(7 rotations/sec), 12 miles wide, it
    creates a hand-shaped nebula

Black Holes
  • Sometimes the leftovers of a supernova are so
    massive that they collapse to form a black hole.
    A black hole is an object that is so massive
    that even light cannot escape its gravity.
  • Black Holes are invisible their extreme gravity
    can cause light to stretch their spinning can
    drag the very fabric of space around with it

Who took these pictures?
  • These images were taken from the ALMA telescope,
    CHANDRA satellite and the Hubble Space
  • ALMA is a radio telescope in Chile
  • CHANDRA is a satellite launched by NASA in 1999
  • The Hubble is an orbiting observatory that was
    launched by the Space Shuttle Discovery in 1990

Lets see how much you know about Stars now!
  • What are some different types of stars?
  • What does an H-R diagram tell us?
  • What can main sequence stars (like our sun) turn
    into as they get old?
  • What are some things massive stars become?