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The Birth and Death of Stars By Moira Whitehouse PhD
What are Stars?
[object Object],[object Object],[object Object],[object Object]
What are Galaxies?
•  Stars form groupings called galaxies.  •  There are about 80-100 billion galaxies in that part of the Universe we can observe. •   There may be more in the Universe beyond what we are able to detect. •  Each galaxy has billions or trillions of stars. •  Many astronomers believe that stars in a galaxy orbit around a black hole.
Hubble Ultra Deep Field image with a huge number of galaxies.
5 galaxies Hickson Compact Gp 52
interacting Galaxy Pair Arp 8
[object Object],[object Object],[object Object]
NASA /JPL-Caltech Artist’s image of the Milky Way
Infrared image of the Milky Way—Cosmic Background Explorer (COBE) satellite  NASA
Spiral  Galaxy M7
How  Are Stars “Born”?
[object Object],[object Object],The Great Orion Nebula
A nebula called NGC 6302.  What resembles butterfly wings are actually boiling cauldrons of gases heated to more than 36,000 degrees F.
 
• Sometimes part of the cloud shrinks and forms a ball as gravity pulls the   gas and dust particles closer and closer together. • The gas and dust inside the ball bump into one another causing the temperature to rise.
[object Object],[object Object]
•  The heated gases expand balancing the inward pull of gravity. gravity hot gases expanding
•  The energy moves through the outer layers of the ball and into space as electromagnetic radiation. •  The visible light causes the ball to glow ••••••• and
………  a new star is born!
Embryonic stars in the Eagle Nebula
Stars bursting into life in Carina nebula
A firestorm of stars being  born in Galaxy NGC 604
Intense bursts of stars that have formed over the last few tens of million years. •  The Hodge Cluster 301 Many stars  forming in the Tarantula Cluster in the Large Magellanic Cloud galaxy
What Happens During the “Life”  of a Star
[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
[object Object],[object Object],[object Object]
How does a Star “Die”?
[object Object],[object Object],[object Object]
[object Object],[object Object],[object Object]
[object Object]
 
[object Object],[object Object],[object Object]
•  The star then sheds its outer layers of gas and dust and  becomes  planetary nebulae. •  When a planetary nebular forms, there is only about 20% of the original star left.
Twin jet nebula Ant nebula Two planetary nebula
•  The planetary nebula spends the rest of its life cooling and shrinking until it becomes a few thousand miles in diameter.  •  Finally it becomes a……
•  white dwarf-- a very dense ball. •  It continues to give off heat for billions of years until it finally becomes a black  dwarf and ceases to shine--you can no longer see it.
Image from the Liverpool Telescope Here you can see a planetary nebula called M57 with its White Dwarf in the middle.
 
[object Object],[object Object]
[object Object],As the core shrinks, the outer layers swell into a Red Super Giant (a very big Red Giant).
Red Supergiant Star V838 Monocerotis
Betelgeuse a red supergiant nearing its end.
Upper section of the picture is the bluish color of hot stars newly formed stars reflected by a cloud of cool gases and dust.  The lower red section is Antares, a super red giant which is gradually shedding layers.
Antares – a Red Super Giant Anatares, a Red Super Giant in the Milky Way Galaxy in the process of dying.
[object Object],•  Inside the core of a Super Giant Red Star, new nuclear fusions begin causing the star to expand once more.  •  When the fuel for nuclear fusion finally runs out core is made of iron. •  The temperature of the core rises to 100 billion degrees Celsius and the star explodes as a supernova.
 
Crab Nebula with remnants of a star’s supernova explosion.
•  huge stars 1.5 to 3 times the mass of the Sun shrink and form a neutron star. After the supernova explosion: •  giant stars 3 times the mass of the Sun shrink and form a black hole.
Neutron star
This deep Chandra X-ray Observatory image shows the supernova remnant Kes. The explosion of a massive star created the supernova remnant, along with a pulsar-- a rapidly spinning neutron star.
Eta-Carinae supernova with a neutron star
A NASA image illustration of a supermassive black hole ripping apart a star and consuming part of it.
This black hole has about 3.8 times the mass of our sun, and is orbited by a companion star, as shown in this illustration.  Credit: NASA/CXC/A. Hobar
The debris from a supernova explosion is blown away and forms a glowing cloud called  a supernova remnant.
Remnants of a supernova
Supernova Remnant from Palomar
Remnants of a supernova and pulsar in the middle of the remnants
http://www.valdosta.edu/~cbarnbau/astro_demos/frameset_moon.html
[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
 

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Birth & death of stars (teach)

  • 1. The Birth and Death of Stars By Moira Whitehouse PhD
  • 3.
  • 5. • Stars form groupings called galaxies. • There are about 80-100 billion galaxies in that part of the Universe we can observe. •   There may be more in the Universe beyond what we are able to detect. • Each galaxy has billions or trillions of stars. • Many astronomers believe that stars in a galaxy orbit around a black hole.
  • 6. Hubble Ultra Deep Field image with a huge number of galaxies.
  • 7. 5 galaxies Hickson Compact Gp 52
  • 9.
  • 10. NASA /JPL-Caltech Artist’s image of the Milky Way
  • 11. Infrared image of the Milky Way—Cosmic Background Explorer (COBE) satellite NASA
  • 13. How Are Stars “Born”?
  • 14.
  • 15. A nebula called NGC 6302. What resembles butterfly wings are actually boiling cauldrons of gases heated to more than 36,000 degrees F.
  • 16.  
  • 17. • Sometimes part of the cloud shrinks and forms a ball as gravity pulls the gas and dust particles closer and closer together. • The gas and dust inside the ball bump into one another causing the temperature to rise.
  • 18.
  • 19. • The heated gases expand balancing the inward pull of gravity. gravity hot gases expanding
  • 20. • The energy moves through the outer layers of the ball and into space as electromagnetic radiation. • The visible light causes the ball to glow ••••••• and
  • 21. ……… a new star is born!
  • 22. Embryonic stars in the Eagle Nebula
  • 23. Stars bursting into life in Carina nebula
  • 24. A firestorm of stars being born in Galaxy NGC 604
  • 25. Intense bursts of stars that have formed over the last few tens of million years. • The Hodge Cluster 301 Many stars forming in the Tarantula Cluster in the Large Magellanic Cloud galaxy
  • 26. What Happens During the “Life” of a Star
  • 27.
  • 28.
  • 29. How does a Star “Die”?
  • 30.
  • 31.
  • 32.
  • 33.  
  • 34.
  • 35. • The star then sheds its outer layers of gas and dust and becomes planetary nebulae. • When a planetary nebular forms, there is only about 20% of the original star left.
  • 36. Twin jet nebula Ant nebula Two planetary nebula
  • 37. • The planetary nebula spends the rest of its life cooling and shrinking until it becomes a few thousand miles in diameter. • Finally it becomes a……
  • 38. • white dwarf-- a very dense ball. • It continues to give off heat for billions of years until it finally becomes a black dwarf and ceases to shine--you can no longer see it.
  • 39. Image from the Liverpool Telescope Here you can see a planetary nebula called M57 with its White Dwarf in the middle.
  • 40.  
  • 41.
  • 42.
  • 43. Red Supergiant Star V838 Monocerotis
  • 44. Betelgeuse a red supergiant nearing its end.
  • 45. Upper section of the picture is the bluish color of hot stars newly formed stars reflected by a cloud of cool gases and dust. The lower red section is Antares, a super red giant which is gradually shedding layers.
  • 46. Antares – a Red Super Giant Anatares, a Red Super Giant in the Milky Way Galaxy in the process of dying.
  • 47.
  • 48.  
  • 49. Crab Nebula with remnants of a star’s supernova explosion.
  • 50. • huge stars 1.5 to 3 times the mass of the Sun shrink and form a neutron star. After the supernova explosion: • giant stars 3 times the mass of the Sun shrink and form a black hole.
  • 52. This deep Chandra X-ray Observatory image shows the supernova remnant Kes. The explosion of a massive star created the supernova remnant, along with a pulsar-- a rapidly spinning neutron star.
  • 53. Eta-Carinae supernova with a neutron star
  • 54. A NASA image illustration of a supermassive black hole ripping apart a star and consuming part of it.
  • 55. This black hole has about 3.8 times the mass of our sun, and is orbited by a companion star, as shown in this illustration. Credit: NASA/CXC/A. Hobar
  • 56. The debris from a supernova explosion is blown away and forms a glowing cloud called a supernova remnant.
  • 57. Remnants of a supernova
  • 59. Remnants of a supernova and pulsar in the middle of the remnants
  • 61.
  • 62.