Emergence of Science
Lecture #2, by I. Bars
As we saw in Travel
across the Universe, powers of ten, we know an awful lot about the Universe
from the very small to the very large. How did we develop this knowledge,
when did it happen, who are the heroes? In this lecture we discuss the
evolution of our understanding of our closest part of the universe, Earth,
Moon, Sun, and the role that measurement and the scientific method played
in establishing the facts.
Credit for graphics: http://www.seds.org/nineplanets/nineplanets/
"Science is a way of trying not to fool yourself." -- Richard Feynman
Science : organize knowledge, condense to
testable theories, predict new phenomena that are (or can be)
verified.
Science does not concern itself with questions that cannot be tested (e.g.
spiritual issues). However, at the frontiers of science there are plenty of
questions in a very fuzzy state, and scientists keep harping at them to turn
them into testable hypotheses (story about the drunk at the lamp post).
Why do we do it? 1) we are curious, 2) we find it useful (through
this knowledge we can harness Nature and put it to use through numerous technological
applications - but that is mainly the realm of Technology).
Scientific method: 1) question or puzzle, 2) hypothesis and prediction,
3) verification or nullification by experiment and measurement, 4) formulation
of a theory or a law of nature that explains and interprets the facts
as simply (and as beautifully) as possible and that makes further testable
predictions.
In science measurement that is continuously refined plays an essential
role. When new facts or measurements do not fit a theory, the theory is evolved
or refined to a better theory, or sometimes completely overthrown. As an example,
consider the evolution of the concepts and theories about the universe we
live in:
- The correct full explanation of planetary motion is due to Newton
who proposed the law of universal gravity
(to be explained later, see simulation1
, simulation2
and simulation3
).
- But there is a lot more beyond the solar system, as discovered through
large telescopes, in prticular by Hubble in the 1920's: The solar system
is only a tiny part of the Milky Way galaxy, and there are billions of galaxies
in the universe. The universe is in motion and in a state of expansion. We
are far from being special or being at the center of the universe. Furthermore,
as interpreted through Einstein's theory of General Relativity, it all was
created in a Big Bang (a theory which makes predictions that are verified).
Video: Stephen Hawking's Universe, Seeing is believing (first 25 minutes,
up to Newton).
Text: Seeing
is believing (first 3 pages and links).
Project (Homework #1, part a): Measure the
size of the sun by doing a rough experiment
(question #2).
Homework (#1, part b): Developing an appreciation of the sizes of planets and their orbits.
Do not e-mail your work to the TA or Professor. Print your
homework and hold on to it.
You will return all parts of Homework #1 simultaneously on
9/25/01.
Reading assignment: Read the full text of "Seeing is believing"
and the related links.
More reading for those interested: Galileo1
, Galileo2, Newton
More reading on the solar system and the planets,A planetary
tour.
Next time questions: from physicsplace.com, ch.2
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