Exam 1 (Ch 1 & 2) Flashcards
Observing and understanding the natural
world
Science
The study of universal phenomena
Physics
4 steps of how science operates
Observe
Hypothesize
Test
If the hypothesis works, it is promoted to theory (a theory should predict phenomena that have not been observed yet)
Study of stars and other objects in space
Astronomy
“Physics” could best be described as the study of
The general principles underlying natural phenomena
Each sphere rotates at a uniform rate around Earth, roughly once a day. So the planets go in simple circles around the Earth
Greeks
Pythagoreans formed a cult that believed in the importance of abstract ideas -> mathematics
It was later observed that planetary motions are irregular and included retrograde motion. The theory was revised. Epicycles were added.
Pythagoras
Earth is spherical:
Ships appear sink little by little below the horizon as they travel out to sea as seen by someone on land
Noontime Sun was lower in the sky in northern lands
Shadow of the Earth on the Moon during a lunar eclipse was round
Aristotle
Sun at Center of Universe and other objects move around the sun in simple circles -> it was dismissed at the time
Aristarchus’ theory
Planets move in circles within circles (loop-the-loops) around Earth
Epicycle theory
Modified epicycle theory
His theory had > 80 epicycles
Ptolemy
Planets moved in simple circles around the sun and explained retrograde motion
A sun-centered universe
Once Galileo had used the telescope to observe the
heavens, he was able to observe the phases of Venus. These phases are totally incompatible with the earth-centered universe
Copernicus’s theory
The planet appears to move backwards on the sky as Earth overtakes the planet in its orbit. The apparent motion is caused by our line of sight to the planet changing. Planets appear brighter during this time since they are closer to us
Occurs when Earth overtakes another planet
Retrograde motion
After 20 years of observations, he found that neither Ptolemy nor Copernicus was right
Johannes Kepler was his disciple
Tycho Brahe
The orbital paths of the planets are elliptical (not circular) with the Sun at one focus
Each planet moves in an elliptical orbit around the sun with the sun occupying one foci of the ellipse (the other one is empty)
Kepler’s First Law
(Addressing the speed of a planet along it’s elliptical path) An imaginary line connecting the Sun to any planet sweeps out equal areas of the ellipse in equal intervals of time. Planet moves faster when closer to the Sun
The imaginary line connecting the planet to the sun sweeps out equal areas in equal times
Kepler’s Second Law
The square of any planet’s period of revolution is proportional to the cube of its mean distance from the sun
P2(in Earth years) = a3(in astronomical units)
Kepler’s Third Law
What is the eccentricity of a circle?
0
What is the eccentricity of a line?
1
The average distance between Earth and the Sun
Astronomical unit
A circle can be defined as the set of all points that are equidistant from the center point; all the points are the length of the radius away from the center
The separation of the two foci determines the eccentricity (or “out of round”) of this
Ellipse
Point of closest approach of a planetary orbit
Perihelion
Point at the greatest distance from the sun of a planetary orbit
Aphelion
Why do the seasons come about?
The seasons come about because of the tilt of the axis about which the Earth rotates every 24 hours. The tilt is about 23.5 degrees