This chapter covers the development of western astronomy and modern science. I focus on the rise of modern science in Europe, from the ancient Greeks to Isaac Newton. Other cultures were also quite interested and skilled in astronomy (the Mayans, Egyptians, peoples of India and China come immediately to mind), but the Greeks were the first ones to try to explain how the universe worked in a logical, systematic manner using models and observations. Modern astronomy (and all of science) has its roots in the Greek tradition. If you would like a more thorough discussion of the history of astronomy than what I will present here, please take a look at Science and the Human Prospect by Ronald Pine. I will give dates of when certain persons lived and worked to give you some reference points in the long history of astronomy. Don't worry about memorizing the dates. What is more important is to see the development of ideas and methods of modern science.
I include images of world atlases from different time periods in this chapter and the next as another way to illustrate the advances in our understanding of our world and the universe. Links to the sites from which the photographs came are embedded in the images. Select the picture to go to the site. The vocabulary terms are in boldface.
By the 7th Century B.C.E. a common viewpoint had arisen in Greece that the Universe is a rational place following universal, natural laws and we are able to figure out those laws. Open inquiry and critical evaluation was highly valued. The emphasis was on the process of learning about the universe rather than attaining the goal. But people eventually got tired of learning and wanted absolute answers. Science is not able to give absolute, certain answers. There was disagreement among the experts and there came to be a crisis in confidence that led to the rise of the Sophists.
The Sophists taught that an absolute truth and morality are myths and are relative to the individual. Since truth and morality were just cultural inventions for the Sophists, they said a person should conform to the prevailing views, rather than resolutely holding to some belief as an absolute one. Socrates (lived 470--399 B.C.E.) disagreed with the Sophists, teaching that we can attain real truth through collaboration with others. By exploring together and being skeptical about ``common sense'' notions about the way things are, we can get a correct understanding of how our world and society operate. This idea of being skeptical so that a truer understanding of nature can be found is still very much a part of modern science.
Socrates' student, Plato(lived 427--347 B.C.E.), developed Socrates' ideas further. Plato taught that there are absolute truths---mathematics is the key. While statements about the physical world will be relative to the individual and culture, mathematics is independent of those influences: 2 + 2 = 4 always, here on Earth or on the far side of the galaxy. Plato had Four Basic Points:
Out of Plato's teachings grew the belief that when one studies mathematics, one studies the mind of God. Mathematical symmetries are the language of universal design and harmony. Their faith in order caused the Greeks to try to find explanation for the seemingly unordered planets (particularly retrograde motion). Their faith in an ordered universe compelled them to make precise observations and they were sustained by their belief in the power of reason. In one form or another, modern scientists have this faith in an ordered universe and the power of human reason.
The Greeks were guided by a paradigm that was first articulated by Pythagoras (picture on left) before Socrates' time. A paradigm is a general consensus of belief of how the world works. It is a mental framework we use to interpret what happens around us. It is what could be called ``common sense''. The Pythagorean Paradigm had three key points about the movements of celestial objects:
Some of the observations that convinced the Greeks that the Earth was not moving are
Plato taught that since an infinite number of theories can be constructed to account for the observations, we can never empirically answer what the universe is really like. He said that we should adopt an instrumentalist view: scientific theories are just tools or calculation devices and are not to be interpreted as real. Any generalizations we make may be shown to be false in the future and, also, some of our false generalizations can actually ``work''--an incorrect theory can explain the observations (see the scientific method page for background material on this).
Aristotle (lived 384--322 B.C.E.) was a student of Plato and had
probably the
most significant influence on many fields of studies (science, theology, philosophy,
etc.) of any single person in history. He thought that Plato had gone too far with
his instrumentalist view of theories. Aristotle taught a realist view:
scientific, mathematical tools are not merely tools---they characterize the way the
universe actually is. At most one model is correct. The model he chose was one
developed by another follower of Plato, Eudoxus. The planets and stars were on concentric
crystalline spheres centered on the Earth. Each planet, the Sun, and the Moon were on
their own sphere. The stars were placed on the largest sphere surrounding all of the rest.
Aristotle chose this model because most popular and observational evidence supported it
and his physics and theory of motion necessitated a geocentric
(Earth-centered) universe. In his theory of motion, things naturally move to the
center of the Earth and
the only way to deviate from that is to have a force applied to the object.
So a ball
thrown parallel to the ground must have a force continually pushing it along.
This idea was unchallenged for almost two thousand years until Galileo showed
experimentally that things will not move or change their motion unless a force
is applied. Also, the crystalline spheres model agreed with the Pythagorean paradigm of
uniform, circular motion (see the previous
section).
Astronomers continued working on models of
how the planets moved. In order to explain the retrograde motion some models used
epicycles---small circles attached to larger circles centered on the Earth. The
planet was on the epicycle so it executed a smaller circular motion as it moved around the
Earth. This meant that the planet's distance from us changed and if the epicyclic motion
was in the same direction (e.g., counter-clockwise) as the overall motion around the Earth,
the planet would be closer to the Earth as the epicycle carried the planet backward with
respect to the usual eastward motion. This explained why planets are brighter as they
retrogress.
Ptolemy's view of the world. Select the image to go to Jim Siebold's ancient
maps database from which this picture came.Ptolemy's geocentric universe
Ptolemy
(lived 85--165 C.E.) set out to
finally solve the problem of the planets motion.
He combined the best features of the geocentric models that used epicycles with the most
accurate observations of the planet positions to create a model that would last for
nearly 1500 years. He added some refinements to explain the
details of the observations: an ``eccentric'' for each planet that was the true center
of its motion (not the Earth!) and an ``equant'' for each planet moved uniformily in
relation to (not the Earth!). See the figure below for a diagram of this setup.
These refinements were incompatible with Aristotle's model and the Pythagorean paradigm---a planet on an epicycle would crash into its crystalline sphere and the motion is not truly centered on the Earth. So Ptolemy adopted an instrumentalist view---this strange model is only an accurate calculator to predict the planet motions but the reality is Aristotle's model. This apparent contradiction between reality and a calculation device was perfectly fine in his time. Our modern belief that models must characterize the way the universe actually is is a tribute to the even longer-lasting influence of Aristotle's realism. Ptolemy was successful in having people adopt his model because he gathered the best model pieces together, used the most accurate observations and he published his work in a large 13-volume series called the ``Almagest'', ensuring that his ideas would last long after he died.
Go to Renaissance Astronomy section
last updated 25 January 1999
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