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Constellation
   and
  Galaxies

   Credit Given to:
    Ethan Vedder
Describe in writing (a few words) at least 10
      different things going on in this painting
                A tree
                                 The Twins
 A boat
          The watcher
                           A playful
                           man               The
                                                        A girl playing
                                             mother

A woman
                         A shy
fishing                                                                  A married
                         man
                                    A puzzling        The sisters        couple
                                    girl
    The thief



                                                                    The monkey?

    A man smoking                    The big dog
                                                   The running dog
Constellations
 Greek, Arab, Egyptian, and
  Babylonian constellations
 88 major ones (you don’t have to
  know all of them)
 North Circumpolar

 Winter, spring, summer, fall
  constellations
 Remember, these stars are only for
  the Northern Hemisphere
Winter Constellations
Summer Constellations
Galaxies




 http://www.galaxyphoto.com/high_res/hst_galaxy.JPG
Galaxies
 A large-scale group of stars
 100,000 light years across from one

  side to the other
 100-400 billion stars per galaxy

 Thought to be between 50 billion and

  1 trillion galaxies
       Quick math: 5,000,000,000,000,000,000
        to        400,000,000,000,000,000,000
        stars out there (5x1018-4x1020)
Galaxies
 Contain  gas and dust (nebulae)
 Brought together by gravity

 Bright and dark nebulae

 “Local Group”: the 17 galaxies

  within 3 million light years of the
  Milky Way
   Closest
          neighbors: Large and Small
   Magellanic Clouds
     (a   mere 150,000 light years away)
Types:
      Spiral galaxies                      Elliptical galaxies                   Irregular galaxies
   Huge; contain stars,                   Huge; contain stars,                  Huge; contain stars,
   gas, and dust                          gas, and dust                         gas, and dust
   Held together by gravity               Held together by gravity              Held together by gravity
   Pinwheel shape (see                    Round-to-oval shape                   No regular shape
   top view of Spiral 1,
   above)
   Bulge and thin disk;                   Bulge but no disk; halo May show signs of a
   halo is present (see                   is present              disk and/or a bulge;
   side view of Spiral 2,                                         halo is present
   above)
   Rich in gas and dust    Little cool gas and dust Usually rich in gas and
                                                    dust
   Young and old stars are Mainly old stars are     Young and old stars are
   present                 present                  present

http://amazing-space.stsci.edu/resources/organizers/galaxy.php.p=Astronomy+basics@eds.astronomy-basics.php
Spiral Galaxies
   Looks like a flattened disc
     Has a bulge/nucleus in the middle and
      spiral arms on the outside
     Spiral arms contain dust and gas and
      young stars
     Spiral (Sa, Sb, Sc) and,

     Barred Spiral (SBa, SBb, SBc)

     Ex. The Milky Way Galaxy
        A   barred spiral galaxy
Spiral Galaxy (Sa-Sc)




The Whirlpool Galaxy and its companion
http://en.wikipedia.org/wiki/Image:Messier51_sRGB.jpg
Barred Spiral Galaxy (SBa-
              SBc)
 There is a
 straight “bar”
 at the
 beginning of
 the galactic
 arms


  http://www.news.wisc.edu/newsphotos/images/Milky_Way_galaxy_sun05.jpg
Elliptical Galaxies
 Do not have “arms”, instead look like
  ellipses (flattened spheres)
 Symbols: E0-E7
 10-15% of known galaxies
 Are typically older stars and in the
  center of globular clusters
 No gas and dust (likely the dust has
  been used, collected, or blown away
  by the stars already)
Elliptical Galaxies (E0-E7)




                                http://cseligman.com/text/stars/
http://csep10.phys.utk.edu/as   messiergalaxies.htm
tr162/lect/galaxies/m87.gif
Irregular Galaxies
 These do not fit into spiral or elliptical
  galaxy descriptions
 Believed to be spiral or elliptical
  galaxies that were altered or distorted
  by gravity
 Or galaxies that were too small to
  organize themselves
 Generally small and faint

 25% of all galaxies
Computer models vs
  Hubble Pictures
Irregular Galaxies
http://starchild.gsfc.nasa.g
ov/Images/StarChild/unive
rse_level2/ngc6822.gif




                               http://en.wikipedia.org/wiki/Image:G
                               alaxyNGC1427A_HubbleImage.jpg
The Milky Way Galaxy (us!)
 We   are located on a spiral arm
  About    2/3 of the way out from the
   center
 100,000    light years across
Star groups
 Stars
      are more often found in
 groups than by themselves
   We’re   in the minority
 Open    and Globular clusters
   Open = less, loose, galactic arms
   Globular = more, spherical, center

 Binary   and triple star systems
   Revolve   around each other
Quasars
 Some    of the earliest things
  produced from the big bang 13.7
  billion years ago
 “Appear to be a faint small star”
  with the energy output much
  brighter than the brightest
  galaxies…
   Howcan something be so small and
   produce so much energy?
Star Journal Homework
 Go outside on a dark night with
  no clouds
 Find a safe place that is pretty

  dark (behind your house, a deck)
 Stay there for 10 minutes, but

  DO NOT look at any bright lights
 Answer the questions on the

  assignment sheet

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Constellations and galaxies 2013

  • 1. Constellation and Galaxies Credit Given to: Ethan Vedder
  • 2. Describe in writing (a few words) at least 10 different things going on in this painting A tree The Twins A boat The watcher A playful man The A girl playing mother A woman A shy fishing A married man A puzzling The sisters couple girl The thief The monkey? A man smoking The big dog The running dog
  • 3.
  • 4.
  • 5. Constellations  Greek, Arab, Egyptian, and Babylonian constellations  88 major ones (you don’t have to know all of them)  North Circumpolar  Winter, spring, summer, fall constellations  Remember, these stars are only for the Northern Hemisphere
  • 9. Galaxies  A large-scale group of stars  100,000 light years across from one side to the other  100-400 billion stars per galaxy  Thought to be between 50 billion and 1 trillion galaxies  Quick math: 5,000,000,000,000,000,000 to 400,000,000,000,000,000,000 stars out there (5x1018-4x1020)
  • 10. Galaxies  Contain gas and dust (nebulae)  Brought together by gravity  Bright and dark nebulae  “Local Group”: the 17 galaxies within 3 million light years of the Milky Way  Closest neighbors: Large and Small Magellanic Clouds  (a mere 150,000 light years away)
  • 11. Types: Spiral galaxies Elliptical galaxies Irregular galaxies Huge; contain stars, Huge; contain stars, Huge; contain stars, gas, and dust gas, and dust gas, and dust Held together by gravity Held together by gravity Held together by gravity Pinwheel shape (see Round-to-oval shape No regular shape top view of Spiral 1, above) Bulge and thin disk; Bulge but no disk; halo May show signs of a halo is present (see is present disk and/or a bulge; side view of Spiral 2, halo is present above) Rich in gas and dust Little cool gas and dust Usually rich in gas and dust Young and old stars are Mainly old stars are Young and old stars are present present present http://amazing-space.stsci.edu/resources/organizers/galaxy.php.p=Astronomy+basics@eds.astronomy-basics.php
  • 12. Spiral Galaxies  Looks like a flattened disc  Has a bulge/nucleus in the middle and spiral arms on the outside  Spiral arms contain dust and gas and young stars  Spiral (Sa, Sb, Sc) and,  Barred Spiral (SBa, SBb, SBc)  Ex. The Milky Way Galaxy A barred spiral galaxy
  • 13. Spiral Galaxy (Sa-Sc) The Whirlpool Galaxy and its companion http://en.wikipedia.org/wiki/Image:Messier51_sRGB.jpg
  • 14. Barred Spiral Galaxy (SBa- SBc)  There is a straight “bar” at the beginning of the galactic arms http://www.news.wisc.edu/newsphotos/images/Milky_Way_galaxy_sun05.jpg
  • 15. Elliptical Galaxies  Do not have “arms”, instead look like ellipses (flattened spheres)  Symbols: E0-E7  10-15% of known galaxies  Are typically older stars and in the center of globular clusters  No gas and dust (likely the dust has been used, collected, or blown away by the stars already)
  • 16. Elliptical Galaxies (E0-E7) http://cseligman.com/text/stars/ http://csep10.phys.utk.edu/as messiergalaxies.htm tr162/lect/galaxies/m87.gif
  • 17. Irregular Galaxies  These do not fit into spiral or elliptical galaxy descriptions  Believed to be spiral or elliptical galaxies that were altered or distorted by gravity  Or galaxies that were too small to organize themselves  Generally small and faint  25% of all galaxies
  • 18. Computer models vs Hubble Pictures
  • 19. Irregular Galaxies http://starchild.gsfc.nasa.g ov/Images/StarChild/unive rse_level2/ngc6822.gif http://en.wikipedia.org/wiki/Image:G alaxyNGC1427A_HubbleImage.jpg
  • 20.
  • 21. The Milky Way Galaxy (us!)  We are located on a spiral arm  About 2/3 of the way out from the center  100,000 light years across
  • 22. Star groups  Stars are more often found in groups than by themselves  We’re in the minority  Open and Globular clusters  Open = less, loose, galactic arms  Globular = more, spherical, center  Binary and triple star systems  Revolve around each other
  • 23. Quasars  Some of the earliest things produced from the big bang 13.7 billion years ago  “Appear to be a faint small star” with the energy output much brighter than the brightest galaxies…  Howcan something be so small and produce so much energy?
  • 24. Star Journal Homework  Go outside on a dark night with no clouds  Find a safe place that is pretty dark (behind your house, a deck)  Stay there for 10 minutes, but DO NOT look at any bright lights  Answer the questions on the assignment sheet

Hinweis der Redaktion

  1. http://amazing-space.stsci.edu/resources/organizers/galaxy.php.p=Astronomy+basics@eds.astronomy-basics.php