structure and evolution of the universe workshop

18
Structure and Evolution of the Universe Workshop

Post on 18-Dec-2015

249 views

Category:

Documents


1 download

TRANSCRIPT

Page 1: Structure and Evolution of the Universe Workshop

Structure and Evolution of the Universe Workshop

Page 2: Structure and Evolution of the Universe Workshop

2nd Century: Claudius Ptolemy (physics of Aristotle)

View: Geostatic cosmology

Big Idea: Different laws for Earth and the cosmos

We can describe a model as a Paradigm, or our “World View”Astronomy has seen 3 major paradigms.

16th Century: Nicolaus Copernicus (physics of Newton)View: Heliocentric cosmology

Big Idea: Universal physics; same laws everywhere

20th Century: Edwin Hubble (physics of Einstein)View: Big Bang Cosmology

Big Idea: universe is changing, evolving

Page 3: Structure and Evolution of the Universe Workshop

Model

Observation

Success!Prediction

Failure!

Refine

How to use your model of the Universe:

Page 4: Structure and Evolution of the Universe Workshop

Model

Observation

Success!Prediction

Failure! Crisis!

How to use your model of the Universe:

Page 5: Structure and Evolution of the Universe Workshop

“The heavens are perfect and unchanging in Time.”

Aristotle

Claudius Ptolemy 100-170 AD Geostatic cosmology

Page 6: Structure and Evolution of the Universe Workshop

Prediction: Future planetary positions

Observation: retrograde motion of planets

Refine: epicycles

Success! For 1500 years

Page 7: Structure and Evolution of the Universe Workshop

Prediction: Phases of Venus

Observation: Full set of phases (Galileo) Crisis!

Page 8: Structure and Evolution of the Universe Workshop

Nicolaus Copernicus 1473-1543 Heliocentric cosmology

Page 9: Structure and Evolution of the Universe Workshop

Prediction: Future planetary positions

Observation: No better than Ptolemy

Refine: elliptical orbits (Johannes Kepler 1571-1630)

Page 10: Structure and Evolution of the Universe Workshop

Prediction: Observed shift in position of stars (parallax) as the earth Moves around the Sun.

Observation: No shift.

Crisis? No, but we had to wait until 1838 (Friedrich Bessel)

Page 11: Structure and Evolution of the Universe Workshop

Prediction: Sun at center of Cosmos

Observation: Sun is not at center of universe (1918)

The galaxy is not the entire universe (1923)

The universe is expanding (1929)

Crisis!

Page 12: Structure and Evolution of the Universe Workshop

Albert Einstein (1879-1955) Big Bang Cosmology

Page 13: Structure and Evolution of the Universe Workshop

Prediction: If denser, hotter, in past, should see evidence of left-over heat from early universe. Observation: Left-over heat from the early universe.

Page 14: Structure and Evolution of the Universe Workshop

Prediction: A dense, hot expanding universe, should be predominantly hydrogen, helium.

The Sun: 74.5% H, 24% He by mass Cecelia Payne 1900-1979

Observation: universe is ~75% hydrogen, ~25% helium by mass

Page 15: Structure and Evolution of the Universe Workshop

Prediction: An expanding universe is evolving over time. If we look at the early universe, it should appear different.

Observation: Distant galaxies less evolved, physically and chemically.

Page 16: Structure and Evolution of the Universe Workshop

Observation: 90% of matter is an unknown form: Dark Matter.

Refine: A new and unknown form of matter exists. But its gravity works the same way, and its presence is needed to explain how the universe looks.

Page 17: Structure and Evolution of the Universe Workshop

Observation: Expansion is accelerating.

Refine: Extra energy content (dark energy). A recent discovery and of unknown origin,the concept of dark energy is actually an integral part of Einstein’s theory of gravity.

Page 18: Structure and Evolution of the Universe Workshop

Conclusions• Big Bang model is our current paradigm or

“world view” of the universe.

• Anomalies, such as dark matter and accelerating expansion (dark energy), lead us to refine our model, but there is no crisis (yet).

• Science is an ongoing process - forcing us to test our model through prediction and observation. The more tests it passes, the greater is our confidence in it.