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What is this? PH1600: Introductory Astrono Lecture 21: Geometry of the Univer

What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

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Page 1: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

What is this?

PH1600: Introductory AstronomyLecture 21: Geometry of the Universe

Page 2: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

PH1600: Introductory AstronomyLecture 21: Geometry of the Universe

Next Lecture: In the Beginning …

School: Michigan Technological UniversityProfessor: Robert Nemiroff

Online Course WebCT pages: http://courses.mtu.edu/

This class can be taken online ONLY, class attendance is not required!

Page 3: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

You are responsible for… Lecture material

Listed wikipedia entries But not higher math

APODs posted during the semester APOD review every week during lecture

Completing the Quizzes Homework quizzes 1 - 10. HW 11 released later today (Wed) by 4 pm See WebCT at http://courses.mtu.edu/

Page 4: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Wikipedia entries:

Shape of the universe redshift Dark matter Dark energy Age of the universe

Page 5: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Considering Our Universe as a Whole

The Cosmological Principle Universe Homogeneous & Isotropic

Homogeneous Smooth when averaged out Example: jello, even fruity jello

Isotropic Same in every direction Example: room with the lights out

Page 6: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Possible Geometries of the Universe

Flat 2D: Circles have area = π r2

3D: Spheres have volume = 4/3 π r3

Negative curvature 2D: Circles have area > π r2

3D: Spheres have volume > 4/3 π r3

Positive curvature 2D: Circles have area < π r2

3D: Spheres have volume < 4/3 π r3

Page 7: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

http://imagine.gsfc.nasa.gov/docs/features/exhibit/map_shape.html

Page 8: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Example: 2D: The Earth

Draw a small circle on your paper It’s area is very close to π r2

Draw a circle the size of Houghton Area still close to π r2

Draw a circle around the Earth Area NOT π r2

Area actually 2 π R2, where R is the distance to the center of the Earth

Page 9: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

http://map.gsfc.nasa.gov/m

_mm

/mr_content.htm

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Page 10: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Average Universe Density Determines Universe Curvature

ρcrit = 3 Ho2/(8 pi G)

Ω = ρ / ρcrit

Flat Geometry: Ω = 1 Negative curvature: Ω < 1 Positive curvature: Ω > 1

Page 11: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

A Simple Example Universe Made Only of Matter: Ω = ΩM

Open: ΩM > 1 Universe infinite in size Universe will expand forever

Closed: ΩM < 1 Universe finite in size

Can circle the universe! Universe will expand for a while Universe will eventually end in a Big Crunch

Flat: ΩM = 1 Universe infinite in size, always was, always will be Universe will expand forever but stop an infinity

Page 12: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

http://physics.uoregon.edu/~courses/BrauImages/Chap26/FG26_009.jpg

Page 13: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Our Accelerating Universe

Supernova cosmology Microwave background Ω = 1

ΩM = 0.3; Ωλ = 0.7

Universe geometry is flat Universe will expand forever Universe expansion rate is

increasing

Page 14: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Possible fates of the universe

Big Freeze (current favorite) Big Crunch Big Rip

Page 15: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Breaking Distant LightCredit: VIMOS, VLT, ESO APOD: 2002 March 19

Page 16: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Rumors of a Strange UniverseCredit: Adam G. Riess (STScI) et al., NASA APOD: 2004 February 27

Page 17: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

http://casa.colorado.edu/~ajsh/astr5770_06/sn.htm

l

Page 18: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

http://en.wikipedia.org/wiki/Image:Cosmological_composition.jpg

Page 19: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Dark Matter: What is it?

Makes up about 30% of universe energy

Not seen directly Indicated by the way visible matter

moves Spiral galaxies rotate too quickly Clusters of Galaxies would evaporate Clusters of Galaxies show smooth lens

effect Composition unknown

Page 20: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Hot Gas and Dark MatterCredit: Richard Mushotzky (GSFC/NASA),

ROSAT, ESA, NASA APOD: April 4, 1999

Page 21: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

The Matter of the Bullet ClusterComposite Credit: X-ray: NASA/CXC/CfA/ M.Markevitch et al.;Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/ D.Clowe et al.Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.;APOD: 2006 August 24

Page 22: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Giant Cluster Bends, Breaks ImagesCredit: W. N. Colley (U. Virginia) et al., HST, NASA APOD: 2004 August 7

Page 23: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Dark Energy: What is it?

Dark Matter is NOT Dark Energy Makes up about 70% of Universe

energy Repulsive gravitational affects seen

Universe accelerating, larger than previously thought

Supernova appear too dim to be close Nature and composition unknown

Page 24: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Future of the Universe

Stellifereous Era Present day: universe filled with stars

Degenerate Era Universe filled with degenerate stellar

remnants Black Hole Era

Universe filled with black holes Dark Era

Universe filled with reshifting light

Page 25: What is this? PH1600: Introductory Astronomy Lecture 21: Geometry of the Universe

Will the Universe End in a Big Rip?Illustration Credit & Copyright: Lynette Cook APOD: 2007 October 21