12
PHY134 Introductory Astronomy Galileo – and Newton!! 1

PHY134 Introductory Astronomy Galileo – and Newton!! 1

Embed Size (px)

Citation preview

Page 1: PHY134 Introductory Astronomy Galileo – and Newton!! 1

1

PHY134Introductory Astronomy

Galileo – and Newton!!

Page 2: PHY134 Introductory Astronomy Galileo – and Newton!! 1

2

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

Page 3: PHY134 Introductory Astronomy Galileo – and Newton!! 1

3

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.

Page 4: PHY134 Introductory Astronomy Galileo – and Newton!! 1

4

• 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

Page 5: PHY134 Introductory Astronomy Galileo – and Newton!! 1

5

Kepler’s Third• 3. Square of sidereal

period proportional to cube of semimajor axis

Same for all planets!

Page 6: PHY134 Introductory Astronomy Galileo – and Newton!! 1

6

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

Page 7: PHY134 Introductory Astronomy Galileo – and Newton!! 1

7

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

Page 8: PHY134 Introductory Astronomy Galileo – and Newton!! 1

8

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

Page 9: PHY134 Introductory Astronomy Galileo – and Newton!! 1

9

Circular motion• We found that directed to center and of

constant magnitude. If radius is and speed what is magnitude of ?

Page 10: PHY134 Introductory Astronomy Galileo – and Newton!! 1

10

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

Page 11: PHY134 Introductory Astronomy Galileo – and Newton!! 1

11

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

Page 12: PHY134 Introductory Astronomy Galileo – and Newton!! 1

12

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