Theme 4 – Newton and Gravity ASTR 101 Prof. Dave Hanes.
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Transcript of Theme 4 – Newton and Gravity ASTR 101 Prof. Dave Hanes.
![Page 1: Theme 4 – Newton and Gravity ASTR 101 Prof. Dave Hanes.](https://reader036.fdocuments.in/reader036/viewer/2022062322/5697bf901a28abf838c8dd33/html5/thumbnails/1.jpg)
Theme 4 – Newton and Gravity
ASTR 101Prof. Dave Hanes
![Page 2: Theme 4 – Newton and Gravity ASTR 101 Prof. Dave Hanes.](https://reader036.fdocuments.in/reader036/viewer/2022062322/5697bf901a28abf838c8dd33/html5/thumbnails/2.jpg)
Newton – The Laws of Mechanics
[Forces and Motions]
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His Objective
To develop a quantitative, mathematical and predictable understanding of how objects move when they are influenced by forces.
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Newton’s First Law(Inertia)
A body in any state of motion (including
a body at rest) will stay in that state ofmotion unless an unbalanced force is acting on it.
Unlike Galileo, hegot this completely right!
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“Acceleration” defined
In physics, Acceleration is any change in the state of motion of an objectThis includes speeding up, slowing down, and/or changing direction.
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Newton’s Second Law (in words!)
If an unbalanced force acts on a body, it will accelerate (its state of motion will change)
The degree to which it does so depends on the size of the force (obviously!) but also on the mass of the object (how much material it contains, its sluggishness or resistance to motion).
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The Colloquial Meaning of Mass
Massive headache Massive amount of work
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But in Physics
Mass is a measure of an object’s resistance to being pushed around, and depends on how many atoms it contains in total.
May be unrelated to size!
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The Law as an Equation (not essential here!):
F = m a, or equivalently a = F / m.
In other words (looking at the right-hand version):
For a given object of mass “m,” a bigger force (“F”) produces a greater acceleration (“a” = change in the state of motion)
but for a given force (“F”), a more massive object (larger “m”) is accelerated less (smaller “a”) than a lower-mass object
Try it! -- throw a baseball, then a shot put!
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Newton’s Third Law
Every force (‘action’) is matched by a force
of the same size but in the oppositedirection (‘reaction’).
Often used metaphorically
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Push the Wall; It Pushes Back
http://www.astro.queensu.ca/~hanes/ASTR101-Fall2015/ANIMS/THIRD-LAW.mp4
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Car Breakdown
Why must you get out? If you don’t: You push the
dashboard It pushes back on you You are pushed into
the seatback That pushes the car
itself towards the rear So nothing moves! No
‘unbalanced’ force!
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Note That Everything Moves[although perhaps imperceptibly!]
You push the car – and so the car pushes you, and through your feet, the Earth itself. (What would happen if you were on glare ice?)
As the car moves forward, the Earth moves back – but only a microscopic amount, as it’s so massive!
Likewise pushups – you go up, the Earth goes down!
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GravityA New, Very Special Force
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As Envisaged by Newton
‘action at a distance’ – no contact required, no strings, no pushing or pulling
universal (acts between any two lumps of matter in the Universe)
inverse-square (e.g. weaker with distance, in a very precise way. Two objects 2 metres apart feel just ¼ of the force they would feel if they were 1 metre apart)
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Why Inverse-Square? Analogy to the Intensity of
Light
…or to a paint sprayer!
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Like an Apple, the Moon is Continuously
Falling!
Its sideways motion keeps it
from landing on our heads!
For every 1 km of sidewaysmotion, it falls about 1.3 mmtowards the Earth. So it
movesat a nearly constant distanceaway, in a near-circular orbit.
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Calculating the Force of
AttractionHow do you add up the tug every atom in one body exerts on every atom in the other body?
Very challenging, especially for irregularly-shaped objects.
Newton’s solution: invent calculus.
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An Amazing Simplification
Consider a “spherically symmetric body” -- one that
looks the same no matter what direction you drill into it
Not this But this
And this
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…and These Astronomical Objects!
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As If by a Miracle!
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So All You Need to Know:
What is the total mass closer to the centre than you are? (i.e. add up all those atoms)
How far are you from the precise centre?
Bingo: out pops the force in question.
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Why This Simplicity?(Nature’s Gift to Us!)
It’s because
1. Gravity obeys an inverse-square law; and
2. Big objects are spherical
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Not Vacuum Cleaners!
If the sun became a black hole (which it won’t, by the way!):
Its gravitational effect on the Earth would be unchanged: we would not be ‘sucked into’ it.
We would continue to orbit it, once a year, just as before – but in perpetual darkness!
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Planning Space Flight Made Easy!
We coast past planets, in rockets and space probes
Calculating the forces, and the motions, is sublimely easy!
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How Do Things Move Under Gravity’s Influence?
A ‘gedanken’ [thought] experiment, not easily implemented in practice.
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One Problem:The cannonball will hit the ground!
Solution: Shrink the Earth right afterwards!
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Low-Speed Cannonball
The cannonball fallstowards the (shrunken)Earth, picking up speed. It whips around it,
movingreally fast, then climbsback to the starting
point,losing speed.
This orbit repeats! It’s asmall ellipse, with theshrunken Earth at the farfocus, the former centre.
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High-Speed Cannonball!
The cannonball moves away
from the blue Earth alongthe curved path shown,losing speed all the while.After reaching a maximumdistance (at the bottom ofthe figure) it starts to fall back, picking up
speed.
The orbit repeats. This time,
it’s a huge ellipse, with the earth at the near (top)
focus.
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At the “Just Right” Speed
The cannonball movesaround the Earth in a
perfectcircle (a special kind ofellipse!) at constant
speed.
This is what the ISS(International Space
Station)does, by our design.
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A Full Understanding
The planets are orbiting the Sun under theinfluence of its gravitational attraction.
They are obeying Newton’s laws of motion,accelerating and moving because of thegravitational forces they feel.
Newton was able to explain all three of Kepler’s
Laws!
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Beyond Kepler’s First Law
Newton asked: What would happen if we shoot the cannonball really really fast?
There are two answers to this.
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“Escape Velocity”
If we launch it at just the rightspeed, the cannonball coasts
offalong a curve known as a
parabola,never to return.
Eventually it will be barely inching
along, having lost essentially all of
its speed. It has only just enough
energy to escape, will never quite
stop, and will never return to the
Earth.
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Faster Still?
If we give it more thanbare escape speed, thecannonball moves offalong a curve knownas a hyperbola.
In this case, it will still be moving with considerablespeed even when far away.
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Putting These All Together
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Planning the Path!
The final path or orbit depends on the speed with which you launch (that is, the energy) and the initial location and direction.
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Are You Geometrically Perplexed?
Kepler discovered elliptical orbits (including circles) for bound objects (those in repeating paths).
Now Newton has introduced parabolas and hyperbolas for unbound objects (those that will escape to infinite distance).
No problem! they are mathematically related in a very direct way, as Newton showed. The details needn’t concern us. (See the next panel if keen.)
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Conic Sections
Make a cross-sectional cut through a cone.
The curve that results depends on the angle at which you make the cut.
These curves are closely related mathematically.