Physics 311 General Relativity Lecture 14: Gravity: Galileo, Newton, Einstein.
PHY134 Introductory Astronomy Galileo – and Newton!! 1.
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Transcript of PHY134 Introductory Astronomy Galileo – and Newton!! 1.
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PHY134Introductory Astronomy
Galileo – and Newton!!
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So Which is it?• Both models produce predictions matching observations of
apparent motion• Culturally difference is huge: does Earth move? Is it central?• Scientifically difference is in motion of planets in 3d.• Other things change in the heavens: Comets come and go and
their motion does not fit well with either model• Real determination: better observations with new technology• Leads to new understanding of fundamental laws that are
universal. That is the scientific revolution
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Kepler’s Laws• 1. Orbit of a planet is an
ellipse with Sun at one focus
• What’s at other focus? Nothing, not even the same for all planets
• Eccentricity small: 0.017 for Earth, 0.2 for Mercury.
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• 2. Line from Sun to planet sweeps out equal areas in equal times
• Planet moves faster near perihelion, slower near aphelion
• Comets in highly eccentric orbits – dramatic effect
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Kepler’s Third• 3. Square of sidereal
period proportional to cube of semimajor axis
Same for all planets!
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Galileo’s Smoking Scope• New technology: Galileo
(1610) turns telescope up• Finds
– phases of Venus showing it orbits Sun
– Galilean moons orbiting Jupiter
– Mountains on Moon, spots on Sun, ears on Saturn
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This is Progress• Galileo studies heavens as a physical system to be observed• Kepler’s laws predict planetary motion with unprecedented accuracy
from simple model• They are universal. In fact, they govern orbiting systems from Solar
System to Saturn’s Moons to…electrons in an Atom (with different K)• Such universality is a hint of underlying fundamental laws• Galileo also studied mechanics (science of motion) and formulated
principle of inertia: An object will retain its state of motion unless disturbed externally
• It took Newton and new math to find them
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Motion• State of motion is velocity - speed and
direction in • Rate of change of is acceleration in
• Acceleration can be speeding, slowing, or turning and is directed in direction of change
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Circular motion• We found that directed to center and of
constant magnitude. If radius is and speed what is magnitude of ?
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Mechanics• Acceleration due to a force applied by another
object:• is a property of object mass - in • is measured – in • When object A applies a force to B, then B
applies a force to A
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Weight and Mass• Weight of an object is the force gravity applies
to it• We know objects fall with acceleration
so force of gravity is• is property of Earth• My mass is . My weight on Earth is
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This is Everything• . The rest is details• If we can figure out forces this is a way to
predict from where things are today where they will be in future (or were in past):positions, velocities
forces accelerations
advance t