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:



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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