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





Birth of star
A star is “born” when the contracting
gas and dust become so hot that
nuclear fusion begins to occur.
How long a star lives depends on how
much mass it has. Stars with less mass
burn their fuel more slowly and last
longer than stars with more mass.
 star’s surface temperature
  determines the amount of
  visible light given off and the
  color we perceive the star to
  be.
 yellow stars produce light of
  all color.
 White   stars give off roughly
  equal amount of every kind of
  light, and blending of these
  colors makes them appear
  white.
 The    hottest type of star
  appears blue or white.
 The    coolest type of star
  appears red.
 Have  mass from 8
  to 100 times of our
  star.
 Luminosity is
  about 1000 to
  50000 times
  brighter than our
  sun
 Life-10 to 20
  million years
super giant
It is a Most massive star.
its mass is about 10 to70 solar mass

Its luminosity is from 30,000 to
100,000 times of solar luminosity

It has a short life time - about 3o
million years therefore it is called
tenuous stars.





o










 Have mass about 3.8
  times greater than our
  Sun.
 Diameter - 15 miles

 It lies very close to the
  minimum size predicted
  for black holes that
  originate from dying stars
lies in the Centre of nebula.
Having surface temperature up
to 250,000.
Is more than 30 times hotter and
250 times brighter than the Sun.
 Itis also known as the Dog
  Star.
 The sixth closest star to
  Earth.
 Magnitude-1.46.

 Is 8.7 light years distant.
V838 Monocerotis reveals
dramatic changes in the
illumination of surrounding dusty
cloud structures. The effect, called
a light echo, unbeiled never-
before-seen dust patterns when
the star suddenly brightened for
several weeks in early 2002.
 When    a star begins to run out of
  fuel, the center of the star
  shrinks and the outer part
  expands. The star becomes a
  red giant or supergiant
 When a star runs out of fuel it
  becomes a white dwarf, a
  neutron star, or a black hole.
All main sequence
 stars eventually
 become red giants
 or supergiants,
 what happens next
 depends on the
 mass of the star.
   www.space.com
   www.nasa.gov
   www.windows2universe.com
   www.google.com
   www.youtube.com
Stars Presentation

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Stars Presentation

  • 1.
  • 3. Birth of star A star is “born” when the contracting gas and dust become so hot that nuclear fusion begins to occur. How long a star lives depends on how much mass it has. Stars with less mass burn their fuel more slowly and last longer than stars with more mass.
  • 4.  star’s surface temperature determines the amount of visible light given off and the color we perceive the star to be.  yellow stars produce light of all color.
  • 5.  White stars give off roughly equal amount of every kind of light, and blending of these colors makes them appear white.  The hottest type of star appears blue or white.  The coolest type of star appears red.
  • 6.
  • 7.
  • 8.
  • 9.  Have mass from 8 to 100 times of our star.  Luminosity is about 1000 to 50000 times brighter than our sun  Life-10 to 20 million years
  • 10. super giant It is a Most massive star. its mass is about 10 to70 solar mass Its luminosity is from 30,000 to 100,000 times of solar luminosity It has a short life time - about 3o million years therefore it is called tenuous stars.
  • 12.  Have mass about 3.8 times greater than our Sun.  Diameter - 15 miles  It lies very close to the minimum size predicted for black holes that originate from dying stars
  • 13. lies in the Centre of nebula. Having surface temperature up to 250,000. Is more than 30 times hotter and 250 times brighter than the Sun.
  • 14.  Itis also known as the Dog Star.  The sixth closest star to Earth.  Magnitude-1.46.  Is 8.7 light years distant.
  • 15. V838 Monocerotis reveals dramatic changes in the illumination of surrounding dusty cloud structures. The effect, called a light echo, unbeiled never- before-seen dust patterns when the star suddenly brightened for several weeks in early 2002.
  • 16.  When a star begins to run out of fuel, the center of the star shrinks and the outer part expands. The star becomes a red giant or supergiant  When a star runs out of fuel it becomes a white dwarf, a neutron star, or a black hole.
  • 17. All main sequence stars eventually become red giants or supergiants, what happens next depends on the mass of the star.
  • 18. www.space.com  www.nasa.gov  www.windows2universe.com  www.google.com  www.youtube.com