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GALAXIES GALAXIES Pages 639-642 Pages 639-642

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Page 1: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

GALAXIESGALAXIES

Pages 639-642Pages 639-642

Page 2: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

GalaxiesGalaxies

Def: large scale groups of stars (approx. Def: large scale groups of stars (approx. 100 billion) bound by gravitational 100 billion) bound by gravitational attraction- rotates around a centerattraction- rotates around a center

Also contain nebulae, planets, dark matter Also contain nebulae, planets, dark matter (90%), space, etc..(90%), space, etc..

Page 3: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Is the center of every galaxy a Is the center of every galaxy a supermassive black hole?supermassive black hole?

Page 4: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Small Magellanic Cloud

Nearest galaxy 150,000 lyNearest galaxy 150,000 ly

Page 5: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Andromeda (M31)Andromeda (M31)

A large galaxy neighborA large galaxy neighbor2,900,000 ly2,900,000 ly

Page 6: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Milky WayMilky Way

• StructureStructure• Barred spiral galaxy Barred spiral galaxy

• About 100,000 About 100,000 light-years widelight-years wide

• Sun is 30,000 light-Sun is 30,000 light-years from the center years from the center

• Rotates every 200 Rotates every 200 million years around million years around “galactic center”“galactic center”

Page 7: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Milky WayMilky Way

Page 8: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Face-on view of the Face-on view of the Milk Way GalaxyMilk Way Galaxy

Page 9: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Edge-on view of the Edge-on view of the Milk Way GalaxyMilk Way Galaxy

Page 10: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Galaxy SongGalaxy Songfrom Monty Pythonfrom Monty Python

http://www.youtube.com/watch?v=vIy76M-4txo&feature=related&safety_mode=true&persist_safety_mode=1&safe=active

Page 11: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Types of GalaxiesTypes of Galaxies

Page 12: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

M105

NGC 3384

Page 13: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Elliptical galaxyElliptical galaxy

60% of all galaxies60% of all galaxiesContain older starsContain older starssmallsmall

Page 14: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

LMC

Large Magellanic cloud

Page 15: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

NCG 6946

Spiral galaxiesSpiral galaxies

30% of all galaxies30% of all galaxiesOlder in center; younger in armsOlder in center; younger in arms

Page 16: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

A barred spiral galaxyA barred spiral galaxy

Page 17: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Merger of two Spirals to form an Elliptical

Page 18: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Irregular galaxyIrregular galaxy

10% of all galaxies10% of all galaxiesContain young starsContain young stars

Page 19: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

M104 (The Sombrero Galaxy)

Page 20: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Hubble’s LawHubble’s Law

Galaxies are receding at a speed Galaxies are receding at a speed proportional to their distanceproportional to their distance

Farther galaxies are moving faster than Farther galaxies are moving faster than nearby galaxiesnearby galaxies

Page 21: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

http://hyperphysics.phy-astr.gsu.edu/hbase/astro/hubble.html#c3

Page 22: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Raisin bread analogy of an Raisin bread analogy of an expanding universeexpanding universe

Page 23: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

What would cause this?What would cause this?

EXPANDING EXPANDING UNIVERSE!UNIVERSE!

Cosmological red Cosmological red shift- supports thisshift- supports this

Page 24: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Local groupLocal group

Local Group Local Group • Milky way and nearest Milky way and nearest

galaxiesgalaxies• Contains at least 28 Contains at least 28

galaxiesgalaxies

Page 25: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

What pattern do galaxies form What pattern do galaxies form in the universe?in the universe?

Page 26: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

AMAZING FACTAMAZING FACT

Our known Universe contains at least Our known Universe contains at least 1,000,000 billions ( Thats One Million, 1,000,000 billions ( Thats One Million, Billions) of other Galaxies...Billions) of other Galaxies...like our like our own Milky Way.own Milky Way. There is no doubt that There is no doubt that there are other vast Universes in there are other vast Universes in existence on top of our Universeexistence on top of our Universe

Page 27: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

What is your galactic addressWhat is your galactic address

Page 28: GALAXIES Pages 639-642. Galaxies Def: large scale groups of stars (approx. 100 billion) bound by gravitational attraction- rotates around a center Def:

Power of TenPower of Ten

http://micro.magnet.fsu.edu/primer/java/http://micro.magnet.fsu.edu/primer/java/scienceopticsu/powersof10/index.htmlscienceopticsu/powersof10/index.html