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Nebulae &
    Galaxies

B y : J a s m i n e Ta m ,
 J e n n if e r L e e , &
What is a nebula?

A nebula is an interstellar cloud
 of dust, hydrogen, helium and
      other ionized gases
How do nebulae form stars?

Gas, dust, and other materials “clump” together
 to form masses
Gravity pulls other matter to the clump
Eventually, clump will become massive enough to
 form stars
How are nebulae formed?
Collapse of interstellar gas in space
 Ultraviolet rays from surrounding
   stars ionizes the surrounding gas
   making the nebula visible
Supernova explosions from stars of
 over 100 solar masses
When stars lose their outer layers of
 gases at the end of their lives
Types of Nebula:

      Diffuse Nebula           Supernova Remnant


Emission     Reflection    Dark
 Nebula       Nebula      Nebula



 Planetary
                H II Regions
  Nebula
Diffuse Nebula:
Nebulae which are extended and do
 not contain (visible) well-defined
 boundaries
Some diffuse nebula contain enough
 gas and dust to form about 100,000
 stars the size of the sun
May be positioned near a bright star
Diffuse Nebula – Emission Nebula
Light from a nearby star energizes the gas
atoms of the nebula causing this nebula to be
able to emit light
There are 2 types of emission nebulae
Planetary Nebula
H II Regions
Diffuse Nebula – Emission Nebula
Planetary Nebula               H II Regions
  Occurs during red giant        Newly formed stars emit
   phase of a star when           ultraviolet light which
   outer layers of star is        ionize the surrounding
   shed                           gases
  Ultraviolet radiation from
    exposed core ionizes
    shed layers


     Ring Nebula                 “Pillars of Creation”
                                    Eagle Nebula
Diffuse Nebula – Reflection Nebula
Do NOT emit light
Dust particles reflect
 light from stars
Usually blue in colour
 because dust grains
                           Witch Head   Trifid Nebula
 reflect more blue light
 than red light             Nebula
Supernova Remnant
Caused by the
 explosion of a star
Consists of the ejected
 matter from the
 explosion




                          Crab Nebula
Dark Nebula
Dark Nebula – What is it?

Interstellar cloud that is extremely dense with
  interstellar dust grains located in the
  coldest, darkest places of the nebula.
It is dark enough to block out ALL light! Even
   the neighbouring stars around the nebula!
Coal Sack Nebula
Brilliant example of a dark
 nebula, as it can easily be
 seen by human eyes.
On bright, starry nights, it’s
 seen as a dark patch on the
 night sky, clearly apparent
 from the background of
 Milky Way
Belongs to the constellation
 Crux, and can only be seen
 in the Southern Hemisphere
Snake Nebula
Dark Nebulae have no definite
 shape and boundaries
Many twist and turn into
 convulsing shapes. A good
 example is the Snake Nebula
Also known as Barnard 72, it is
  S-shaped and found in the
  constellation Ophiuchus
Part of the Great Dark Horse
 Nebula
Horse Head Nebula
Perhaps the most famous of the
  Dark Nebulae, also known as
  Barnard 33, is the Horse Head
  Nebula.
  Found in constellation Orion,
    and it lies behind the star
    Alnitak.
  Categorized and found by
    Edward Emerson
  About 1600 light years away
More apparent because the bright
 nebula, IC 434 is behind it,
 casting a larger shadow.
Bok Globules and New Stars

Small dark nebulae are often referred to as Bok
 Globules.
Cool clouds of gas and dust that are more
 spherical in shape, resembling drops of
 water
Named after Bart J. Bok (American astronomer)
Believed to create lower mass stars.
Dark Nebulae also site for creating new stars, as
 mentioned by Jen.
Planetary
 Nebula
What are they?
Type of emission nebulae
  Cloud of ionized gas that emit light in various colors
Lit up by a central star
  Looks like small planets through optical telescopes,
    which is why they are called PLANETary nebulae
Formed when a star is dying (in red giant stage)
  Outside layer of star dissipates and star shines
   brighter and hotter with out outer layer
  Can reach up to 25 000 to 200 000 degrees celsius
  Ultraviolet radiation from the core of the star ionizes
    the gas and plasma which creates the colorful
    lights
General
Help create new stars
                      Info :
  Star dies => metals in core sent across universe => metal
    able to create new stars
Only stars that are around the same mass of our sun
 (1 solar mass) can turn into a planetary nebula
  8 solar masses or more will turn into a supernova instead
Generally found in the plane of the Milky Way, but are
 more closely gathered in the centre of Milky Way
Not very bright compared to other nebulae, even
 thought their central star are some of the hottest
 known in the universe
  Because the hotter a star is, the more ultraviolet rays make
   it hard to see it in visible light
Bug Nebula
Found in constellation Scorpius
Outer structure (bipolar planetary nebula)
 considered to be the most complex of all known
 planetary nebulae.
Central star also considered to be hottest in the
 galaxy, but very faint to see on Earth -white
 dwarf that burns at 200 000 K
Cat's Eye Nebula   Found in constellation Draco
                    (3300 light years away)
                   Also contains highly
                     complicated structure that
                     contains a hot central star
                     that lost it’s outer layer
                     over 1000 years ago
                   Found by William Herschel
                   Shells that appear in the
                    photo are actually layers of
                    ionized gas from the dying
                    star
So What Happens When a Star Explodes?

As mentioned before, if the star was less than 8
 solar masses, it will turn into a planetary
 nebulae
If more than 8 solar masses, it will turn into a
   supernova remnant!
Supernova remnant is the structure left behind
 after a supernova explosion (star goes BOOM)
Heats up interstellar medium and sends out
 important metals throughout universe
Types of Supernova Remnants (I)
2 main types: First type is the shell-type
  remnant (heats up interstellar medium
  during explosion)
   Interstellar medium: dust and gas
      between stars and galaxies (after
      supernova explosion becomes
      hot)
Cygnus Loop: example of a shell type
  remnant (show picture)
   Found in constellation Cygnus
     (extremely large for a supernova
     remnant)
   Scientists have found 4 smaller
     nebulae inside the Loop!
Types of Supernova Remnants (II)


                                             Crab Nebula
Second type is crab-type found in
  Famous Crab Nebula remnant.
 (also called pulsar wind (show
    constellation Taurus nebulae)
    picture)
  Contains neutron star that sends out
    regular pulses of radiation Crab
     Central neutron star called
        Pulsar
  These supernova remnants filled with
    high energy electrons from the neutron
     Spins 30.2 times per second
    starwhile emitting radiation
Galaxies
What are Spiral Galaxies?
Thin structures similar to a disk
Have arms of stars spiralled around the galaxy’s
 center.
Tightly wound spiral called “Sa” ; loose spiral is
  called “Sc.”
Consist of mainly young, new stars
Have interstellar matter in galaxy disk
 approximately 10,000 to almost 100,000 light
 years in diameter
What are Spiral Galaxies?
Center of the spiral galaxy  bulge (a dense
 concentration of stars)
Diameter of a few thousand light years
Extends above and below the disk.
Spiral arms & blue waves in the galaxy disk’s
 density hold high proportion of huge, hot stars
Stars shine longer & have brighter light than
 smaller, more common stars, eg. Sun
What are Barred-Spiral (SB) Galaxies?


 Very similar to spiral galaxies
 Have a bar of stars running through the middle
 Tightly wound barred-spiral galaxy is called “SBa”
    ; loosely wound barred-spiral galaxy
 Called “SBc.”
What are Barred-Spiral (SB) Galaxies?

Theories of bar fueling stars during its evolution.
Theories of bar created by density wave from the
 galaxy’s center
Caused the inner stars to reshape its orbit.
Those stars orbit further out T the structure of bar
Milky Way (aka Earth's Galaxy)
Part of the Local Group which contains over 24 other
  galaxies
  Contains many beautiful and important features
     Nebula in Orion’s sword.
         Birthing ground where powerful stars produced.
Created from swallowing other galaxies
  Stars from the Sagittarius Dwarf Galaxy
As old as the universe
  Milky Way: 13.6 billion yrs ; universe 13. 7 billion yrs.
      Galaxy’s disk and the bulge not created until 10-12
       billion yrs ago
Milky Way (aka Earth's Galaxy)
Has halo of approximately 150 globular clusters
 scattered around galactic center
  Globular clusters = thousands of millions of old stars tightly
    grouped together
     Only 20-30 light years across = concentrated in a swarm
     Stars so old  most less than two solar masses & glow yellow-
       red.
Dusty and gassy
  Only allow to see 6000 light years in visible spectrum
  Deflects visible light
  Infrared light can still pass through
     Use infrared telescope (Spitzer Space Telescope) and clearly see
      galaxy’s center and regions where stars form
Milky Way (aka Earth's Galaxy)
Have super massive black hole = Sagittarius A*
  Diameter 15x Sun’s
  Source of X-rays and radio waves from galaxy’s
   center
200 + billion stars
  Only 2500 seen from Earth
  Low # of stars because too far from center
     6000 light years closer, night sky = brighter!
Theory of having halo of dark matter
  Invisible but existence believed through simulations
The End (:

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Nebulae & Galaxies

  • 1. Nebulae & Galaxies B y : J a s m i n e Ta m , J e n n if e r L e e , &
  • 2. What is a nebula? A nebula is an interstellar cloud of dust, hydrogen, helium and other ionized gases
  • 3. How do nebulae form stars? Gas, dust, and other materials “clump” together to form masses Gravity pulls other matter to the clump Eventually, clump will become massive enough to form stars
  • 4. How are nebulae formed? Collapse of interstellar gas in space Ultraviolet rays from surrounding stars ionizes the surrounding gas making the nebula visible Supernova explosions from stars of over 100 solar masses When stars lose their outer layers of gases at the end of their lives
  • 5. Types of Nebula: Diffuse Nebula Supernova Remnant Emission Reflection Dark Nebula Nebula Nebula Planetary H II Regions Nebula
  • 6. Diffuse Nebula: Nebulae which are extended and do not contain (visible) well-defined boundaries Some diffuse nebula contain enough gas and dust to form about 100,000 stars the size of the sun May be positioned near a bright star
  • 7. Diffuse Nebula – Emission Nebula Light from a nearby star energizes the gas atoms of the nebula causing this nebula to be able to emit light There are 2 types of emission nebulae Planetary Nebula H II Regions
  • 8. Diffuse Nebula – Emission Nebula Planetary Nebula H II Regions Occurs during red giant Newly formed stars emit phase of a star when ultraviolet light which outer layers of star is ionize the surrounding shed gases Ultraviolet radiation from exposed core ionizes shed layers Ring Nebula “Pillars of Creation” Eagle Nebula
  • 9. Diffuse Nebula – Reflection Nebula Do NOT emit light Dust particles reflect light from stars Usually blue in colour because dust grains Witch Head Trifid Nebula reflect more blue light than red light Nebula
  • 10. Supernova Remnant Caused by the explosion of a star Consists of the ejected matter from the explosion Crab Nebula
  • 12. Dark Nebula – What is it? Interstellar cloud that is extremely dense with interstellar dust grains located in the coldest, darkest places of the nebula. It is dark enough to block out ALL light! Even the neighbouring stars around the nebula!
  • 13. Coal Sack Nebula Brilliant example of a dark nebula, as it can easily be seen by human eyes. On bright, starry nights, it’s seen as a dark patch on the night sky, clearly apparent from the background of Milky Way Belongs to the constellation Crux, and can only be seen in the Southern Hemisphere
  • 14. Snake Nebula Dark Nebulae have no definite shape and boundaries Many twist and turn into convulsing shapes. A good example is the Snake Nebula Also known as Barnard 72, it is S-shaped and found in the constellation Ophiuchus Part of the Great Dark Horse Nebula
  • 15. Horse Head Nebula Perhaps the most famous of the Dark Nebulae, also known as Barnard 33, is the Horse Head Nebula. Found in constellation Orion, and it lies behind the star Alnitak. Categorized and found by Edward Emerson About 1600 light years away More apparent because the bright nebula, IC 434 is behind it, casting a larger shadow.
  • 16. Bok Globules and New Stars Small dark nebulae are often referred to as Bok Globules. Cool clouds of gas and dust that are more spherical in shape, resembling drops of water Named after Bart J. Bok (American astronomer) Believed to create lower mass stars. Dark Nebulae also site for creating new stars, as mentioned by Jen.
  • 18. What are they? Type of emission nebulae Cloud of ionized gas that emit light in various colors Lit up by a central star Looks like small planets through optical telescopes, which is why they are called PLANETary nebulae Formed when a star is dying (in red giant stage) Outside layer of star dissipates and star shines brighter and hotter with out outer layer Can reach up to 25 000 to 200 000 degrees celsius Ultraviolet radiation from the core of the star ionizes the gas and plasma which creates the colorful lights
  • 19. General Help create new stars Info : Star dies => metals in core sent across universe => metal able to create new stars Only stars that are around the same mass of our sun (1 solar mass) can turn into a planetary nebula 8 solar masses or more will turn into a supernova instead Generally found in the plane of the Milky Way, but are more closely gathered in the centre of Milky Way Not very bright compared to other nebulae, even thought their central star are some of the hottest known in the universe Because the hotter a star is, the more ultraviolet rays make it hard to see it in visible light
  • 20. Bug Nebula Found in constellation Scorpius Outer structure (bipolar planetary nebula) considered to be the most complex of all known planetary nebulae. Central star also considered to be hottest in the galaxy, but very faint to see on Earth -white dwarf that burns at 200 000 K
  • 21. Cat's Eye Nebula Found in constellation Draco (3300 light years away) Also contains highly complicated structure that contains a hot central star that lost it’s outer layer over 1000 years ago Found by William Herschel Shells that appear in the photo are actually layers of ionized gas from the dying star
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  • 23. So What Happens When a Star Explodes? As mentioned before, if the star was less than 8 solar masses, it will turn into a planetary nebulae If more than 8 solar masses, it will turn into a supernova remnant! Supernova remnant is the structure left behind after a supernova explosion (star goes BOOM) Heats up interstellar medium and sends out important metals throughout universe
  • 24. Types of Supernova Remnants (I) 2 main types: First type is the shell-type remnant (heats up interstellar medium during explosion) Interstellar medium: dust and gas between stars and galaxies (after supernova explosion becomes hot) Cygnus Loop: example of a shell type remnant (show picture) Found in constellation Cygnus (extremely large for a supernova remnant) Scientists have found 4 smaller nebulae inside the Loop!
  • 25. Types of Supernova Remnants (II) Crab Nebula Second type is crab-type found in Famous Crab Nebula remnant. (also called pulsar wind (show constellation Taurus nebulae) picture) Contains neutron star that sends out regular pulses of radiation Crab Central neutron star called Pulsar These supernova remnants filled with high energy electrons from the neutron Spins 30.2 times per second starwhile emitting radiation
  • 27. What are Spiral Galaxies? Thin structures similar to a disk Have arms of stars spiralled around the galaxy’s center. Tightly wound spiral called “Sa” ; loose spiral is called “Sc.” Consist of mainly young, new stars Have interstellar matter in galaxy disk approximately 10,000 to almost 100,000 light years in diameter
  • 28. What are Spiral Galaxies? Center of the spiral galaxy  bulge (a dense concentration of stars) Diameter of a few thousand light years Extends above and below the disk. Spiral arms & blue waves in the galaxy disk’s density hold high proportion of huge, hot stars Stars shine longer & have brighter light than smaller, more common stars, eg. Sun
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  • 30. What are Barred-Spiral (SB) Galaxies? Very similar to spiral galaxies Have a bar of stars running through the middle Tightly wound barred-spiral galaxy is called “SBa” ; loosely wound barred-spiral galaxy Called “SBc.”
  • 31. What are Barred-Spiral (SB) Galaxies? Theories of bar fueling stars during its evolution. Theories of bar created by density wave from the galaxy’s center Caused the inner stars to reshape its orbit. Those stars orbit further out T the structure of bar
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  • 33. Milky Way (aka Earth's Galaxy) Part of the Local Group which contains over 24 other galaxies Contains many beautiful and important features Nebula in Orion’s sword. Birthing ground where powerful stars produced. Created from swallowing other galaxies Stars from the Sagittarius Dwarf Galaxy As old as the universe Milky Way: 13.6 billion yrs ; universe 13. 7 billion yrs. Galaxy’s disk and the bulge not created until 10-12 billion yrs ago
  • 34. Milky Way (aka Earth's Galaxy) Has halo of approximately 150 globular clusters scattered around galactic center Globular clusters = thousands of millions of old stars tightly grouped together Only 20-30 light years across = concentrated in a swarm Stars so old  most less than two solar masses & glow yellow- red. Dusty and gassy Only allow to see 6000 light years in visible spectrum Deflects visible light Infrared light can still pass through Use infrared telescope (Spitzer Space Telescope) and clearly see galaxy’s center and regions where stars form
  • 35. Milky Way (aka Earth's Galaxy) Have super massive black hole = Sagittarius A* Diameter 15x Sun’s Source of X-rays and radio waves from galaxy’s center 200 + billion stars Only 2500 seen from Earth Low # of stars because too far from center 6000 light years closer, night sky = brighter! Theory of having halo of dark matter Invisible but existence believed through simulations
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