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argued the force of gravity is y proportional to the masses in 2 2 1 R m m F grav 2 2 1 R m m G F grav = a universal constant measured 6.67 10 -11 N·m 2 /kg 2 0.000 000 000 066 7 N·m 2 /kg 2
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We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67 10 -11 N·m 2 /kg.

Dec 21, 2015

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Page 1: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

We’ve argued the force of gravity is also directly proportional to the masses involved:

221

R

mmF

grav∝

221

R

mmGF

grav=

G is a universal constant measured to be6.67 10-11 N·m2/kg2

0.000 000 000 066 7 N·m2/kg2

Page 2: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Henry Cavendish (1731 – 1810)

Page 3: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

How irresistible is the gravitational force of attraction between a pair of us when 1 meter (center-to-center) apart?

G(80 kg) (70 kg)

(1 meter)2 = G 5600kg2

m2

= 0. 000 000 32 N

Fgrav

R

Page 4: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

2R

R

Rm mF F

R

R/2

Two objects of mass, m, separated by a center-to-center distance R are mutually

attracted to one another by a force F.How strong is the attractive force between

the other pairs of objects shown?

A. ¼ F C. F E. 4FB. ½ F D. 2F F. other

m m

m m

m 2m

2m 2m

Page 5: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Weight

How hard does earth’sgravity pull on me?

2R

MmGF earthDC=

distance to the center of the earth

If unbalanced by any normal force of support how fast would I be accelerated?

2R

MmGam earthDC

DC=

F = ma, so:

Page 6: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

How fast does the earthaccelerate me?

2R

MGa earth=

How fast does the earthaccelerate YOU?

2R

MmGam earthYOU

YOUYOU=

How fast does the earthaccelerate an apple?

2R

MmGam earthapple

appleapple=

Page 7: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

2R

MGa earth=

The earth accelerates ALL objects near its surface at exactly the same rate:

a = (6.67 10-11 N·m2/kg2) 5.98 1024 kg(6.38 106 m)2

= 9.800 m/sec2

Actually we’ve mixed up the historical order of events somewhat.

Newton’s ideas do in fact explain whyall objects fall to earth at the same rate

independent of their mass.

But notice calculating that the acceleration rate is exactly 9.8 m/sec2 required knowing the mass of the earth! How is THAT known?

Page 8: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Rearth = 6.38 106 meters

Navigators and surveyors had established a size for the earth:

3

3

4R V π= = 1.09 1021 m3

Density of some STUFF in the earth:

Granite 2.7 103 kg/m3

Iron 7.8 103 kg/m3

Water 1.0 103 kg/m3

Which would suggest the mass of the earth lies somewhere between

1 – 8 1024 kg

2R

MGa earth=

It was of course Cavendish who could take:

G

RmM

earth

22 )sec/8.9(=

Page 9: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

and for any moon orbiting any planet:

2

24

T

Ra

π=

For any planet (or star or asteroid)

2R

MGa planet=

the acceleration down toward its center is

which means:

2

2

2

4

T

R

R

MG planet π=

2

324

GT

RM

planet

π=

Page 10: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Which is how we’ve known the massof Mars, Jupiter and Saturn without

even going there!

How do we know the mass of Venus? Mercury?

How do we know the mass of the sun?

Page 11: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.
Page 12: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Johannes Kepler (1571-1630)

All planets move in ellipses, with the sun at one focus.

Page 13: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

The undefined concepts in GEOMETRY

collection of all points in a plane equidistant from a selected point

called the center.

Page 14: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

collection of every point in a plane whose distances from two fixed focii sums to the same constant total.

5 inches

3.5 in

ches

To build an ellipse, pick any two pointsand a number bigger than their distance apart.

3.5 inches

7 > 5

1 inch

Page 15: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

collection of every point in a plane whose distances from two fixed focii sums to the same constant total.

To build an ellipse, pick any two pointsand a number bigger than their distance apart.

7 > 5

3 + 4 = 7

3 inc

h

4 inch

2 + 5 = 7

Page 16: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

collection of every point in a plane whose distances from two fixed focii sums to the same constant total.

To build an ellipse, pick any two pointsand a number bigger than their distance apart.

7 > 5

2 inch

5 inch

2 + 5 = 7

Page 17: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

speed just right

speed too highspeed too

low

The second (far) focus is empty!

The second (near) focus is empty!

Page 18: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

Oops! Speedway too slow!

Page 19: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

A popgun fires a standard 40mm (2.7 gram) ping pong ball at the back of a stationary wagon.

mv

mv

The ball ricochets back with almost the same speed.

A. zero momentum D. momentum 2mv.B. momentum ½mv. E. momentum 3mv.C. momentum mv. F. momentum 4mv.

The wagon must recoil with

Page 20: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

mv

mv

Now compare the case where the tennis ballsolidly rebounds

Page 21: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

mv

…to the case where the tennis ball smashes into but imbeds itself

Page 22: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

mv

?

?

Which collision sends the wagon rolling forward with the greater speed?

A.

B.

C. Either collision gives the wagon the same speed.

Page 23: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

mv

?

?

60 gram tennis ball initially at 10 m/sec60 kg wagon initially at rest

wagonwagonballballballballvmvmvm ′+′=+0

wagonvkgsmkgsmkg ′+⋅−=⋅ )60(/60.0/60.0

wagonvkgsmkg ′=⋅ )60(/20.1

wagonvsm ′=/02.0

vmmsmkgwagonball

′+=⋅ )(/60.0vkgsmkg ′=⋅ )060.60/()/60.0(

vsm ′=/00999.0

Page 24: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

A spray of rapid fire will provide a steady pressure that can levitate this block, holding it back in place.

Page 25: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

v = 500 m/sec

A ball rebounds from the ground straight up at 500 m/sec.

How high can it climb? (How high had it been dropped from?)

mghmv =221

gtvv −=0

tsmsm )/8.9(/5000 2−=

2/8.9

/500

sm

smt

−−

= sec51=

2

21 gtd =

22

21 )51)(/8.9( ssm=

So:

meters 745,12=Or just:

hg

v =2

2

meters h 745,12=

Page 26: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

v = 500 m/sec

A 500 m/sec projectile traveling straight up, is in the air 102 seconds

and reaches a 12.745 km altitude.

v = 500 m/sec

A 500 m/sec projectile traveling horizontally can cross a 12 meter lecture hall in:

ssmmt 004.0)/500/(12 ==

dropping only2

21 atd =

22

21 )004.0)(/8.9( ssm=

meters 0000784.0=mm 0784.0=

Crosses the room in nearly a straight line!

][ 2

21 mvmgh Δ=Rising h=1 meter:

reduces its speed by ~4 cm/sec.

Page 27: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

CO2 molecules of a refrigerator-cold bubble in a can of soda pop 887 mph

Room temperature nitrogen N2 molecules

1160 mph

An enormous number of these invisibly small particles exert a ~constant pressure outward, against all the surfaces

of their container:

The round shapecharacteristic of a balloonconfirms that this pressure is exerted in all directions.

Page 28: We’ve argued the force of gravity is also directly proportional to the masses involved: G is a universal constant measured to be 6.67  10 -11 N·m 2 /kg.

A. just as hard as

Answers to Clicker QuestionsJust another example of Newton’s law: Interactions always involve mutually equal but opposite forces.

Slide 2 presents an argument as to why.

R/2m m

2Rm m

Rm 2m

R2m 2m

Compare each to: 2

2

R

mG

RR

mmGF =

××

=

⎥⎦

⎤⎢⎣

⎡×== 2

2

4/22

2

42

)2/( R

mGmG

R

mG

R

⎥⎦

⎤⎢⎣

⎡×== 2

2

22

2

4

14

2

)2( R

mG

RmG

R

mG

⎥⎦

⎤⎢⎣

⎡×=×

2

2

2 2)2(

R

mG

R

mmG

⎥⎦

⎤⎢⎣

⎡×=×

2

2

2 4)2()2(

R

mG

R

mmG