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Gravitational repulsion and the Dipole Repeller

Ask Ethan: If Gravity Attracts, How Can The ‘Dipole Repeller’ Push The Milky Way?

Ethan Siegel, Contributor. Feb 4, 2017

Forbes.com Startswithabang 2017 Ask Ethan The Dipole Repeller

The relative attractive and repulsive effects of overdense and underdense regions on the Milky Way. Image credit: "The Dipole Repeller" by Yehuda Hoffman, Daniel Pomarède, R. Brent Tully, and Hélène Courtois, Nature Astronomy 1, 0036 (2017).

The relative attractive and repulsive effects of overdense and underdense regions on the Milky Way. Image credit: “The Dipole Repeller” by Yehuda Hoffman, Daniel Pomarède, R. Brent Tully, and Hélène Courtois, Nature Astronomy 1, 0036 (2017).

One of the most peculiar things about the Universe is how quickly the Milky Way appears to be moving. Despite having mapped out the cosmic masses nearby to unprecedented accuracy, there still doesn’t appear to be enough to cause the motion we actually experience. The idea of a “great attractor” doesn’t quite match up with what we see; what’s actually present isn’t quite “great” enough. But a new idea — that of a dipole repeller — might finally explain this longstanding conundrum. How would that work, and what it is, exactly? That’s what Darren Redfern wants to know:

What are the mechanics behind a dipole repeller? How can an area of space void of matter repulse galaxies to any meaningful extent (or at all?)?

If you were to look at all the galaxies accessible to us, you’d find, on average, that they were moving away from us at a specific rate: the Hubble rate. The farther away a galaxy is, the faster it appears to move away from us, and that’s a consequence of living in an expanding Universe governed by General Relativity. But that’s only on average. Each individual galaxy has an additional motion on top of that, known as peculiar velocity, and that’s due to the combined gravitational influence of every imperfection in the Universe on it.

The various galaxies of the Virgo Supercluster, grouped and clustered together. On the largest scales, the Universe is uniform, but as you look to galaxy or cluster scales, overdense and underdense regions dominate. Image credit: Andrew Z. Colvin, via Wikimedia Commons.

The various galaxies of the Virgo Supercluster, grouped and clustered together. On the largest scales, the Universe is uniform, but as you look to galaxy or cluster scales, overdense and underdense regions dominate. Image credit: Andrew Z. Colvin, via Wikimedia Commons.

The closest large galaxy to us, Andromeda, is actually moving towards us, thanks to the Milky Way’s gravitational pull. Galaxies in the closest giant cluster of galaxies — the Virgo cluster — get extra speeds of up to 2,000 km/s on top of the Hubble flow we see. And when we look at the Big Bang’s leftover glow, the Cosmic Microwave Background, we’re able to measure our own peculiar motion through the Universe.

The CMB dipole as measured by COBE, representing our motion through the Universe relative to the CMB's rest frame. Image credit: DMR, COBE, NASA, Four-Year Sky Map.

The CMB dipole as measured by COBE, representing our motion through the Universe relative to the CMB’s rest frame. Image credit: DMR, COBE, NASA, Four-Year Sky Map.

This “cosmic dipole” we see is redshifted in one direction (meaning we’re moving away from it) and blueshifted in the other (meaning we’re moving towards it), and we can reconstruct the motion of the entire local group as a result. Us, Andromeda, Triangulum and everything else is moving at a speed of 631 km/s relative to the Hubble flow, and we know that gravitation must be the cause of this. When we look out at where the galaxies are located, we can map out their masses and how much of an attractive force they exert.

 two-dimensional slice of the overdense (red) and underdense (blue/black) regions of the Universe nearby us. Image credit: Cosmic Flows Project/University of Hawaii, via http://www.cpt.univ-mrs.fr/.

two-dimensional slice of the overdense (red) and underdense (blue/black) regions of the Universe nearby us. Image credit: Cosmic Flows Project/University of Hawaii, via http://www.cpt.univ-mrs.fr/.

Thanks to the recent Cosmic Flows project, we’ve not only mapped out the nearby Universe to better precision than ever before, we discovered that the Milky Way lies on the outskirts of a giant collection of galaxies pulling us towards it: Laniakea. This is a significant contributor to our peculiar motion, but it isn’t enough to explain all of it on its own. Gravitational attraction is only half the story. The other half? It comes from gravitational repulsion. Let me explain.

Imagine you have a Universe where you have an equal number of masses evenly spaced everywhere you look. In all directions, at all locations, the Universe is filled with matter of even density. If you put an extra mass a certain distance to your left, you’ll be attracted towards your left, because of gravitational attraction.

But if you remove some of the mass that same distance to your right, you’ll also be attracted towards your left! In a perfectly uniform Universe, you’d be attracted to all directions equally, and that attractive force would cancel out. But if you remove some mass from one particular direction, it can’t attract you as strongly, and so you’re attracted preferentially in the other direction.

Dipoles are most common in electromagnetism, where we think of negative as attractive and positive as repulsive. If you thought of this gravitationally, negative would be 'extra mass' and therefore attractive, while positive would be 'less mass' and therefore, relative to everything else, repulsive. Image credit: Wikimedia Commons user Maschen.

Dipoles are most common in electromagnetism, where we think of negative as attractive and positive as repulsive. If you thought of this gravitationally, negative would be ‘extra mass’ and therefore attractive, while positive would be ‘less mass’ and therefore, relative to everything else, repulsive. Image credit: Wikimedia Commons user Maschen.

 

It’s not technically a gravitational repulsion, since gravitation is always attractive, but you’re less attracted to one direction than all the others, and so an underdense region effectively acts as a gravitational repeller. You can even imagine a situation where you have an overly dense region on one side of you with an underdense region on the other side. You’d experience the greatest magnitude of attraction and repulsion simultaneously. This is what the idea of the dipole repeller is.

The gravitational attraction (blue) of overdense regions and the relative repulsion (red) of the underdense regions, as they act on the Milky Way. Image credit: "The Dipole Repeller" by Yehuda Hoffman, Daniel Pomarède, R. Brent Tully, and Hélène Courtois, Nature Astronomy 1, 0036 (2017).

The gravitational attraction (blue) of overdense regions and the relative repulsion (red) of the underdense regions, as they act on the Milky Way. Image credit: “The Dipole Repeller” by Yehuda Hoffman, Daniel Pomarède, R. Brent Tully, and Hélène Courtois, Nature Astronomy 1, 0036 (2017).

It’s difficult to measure where an underdense region is, since regions of average density are fairly devoid of galaxies as well as the underdense ones. But a recently discovered cosmic void relatively nearby, and in the opposite direction to the large concentration of galaxies attracting us, seems to be responsible for roughly 50% of our peculiar motion, which is exactly the amount that was unaccounted for by the overdense regions alone.

Youtube video: The Dipole Repeller video, by Daniel Pomarède.  produced as part of the following publication: “The Dipole Repeller” by Yehuda Hoffman, Daniel Pomarède, R. Brent Tully, and Hélène Courtois, Nature Astronomy 1, 0036 (2017).

At long last, this could be the solution to why our Sun, galaxy and local group all exhibit the motion that they do. Gravity is never repulsive, but a less attractive force in one direction than all the others behaves indistinguishably from a repulsion. We might distinguish between a pull in one direction and a push in the opposite direction, but in astrophysics, it’s all the same thing: forces and acceleration. It doesn’t have anything to do with dark energy or a mysterious fifth force; it’s simply having an excess of matter in one direction and a dearth of matter in nearly the exact opposite direction. The result? We move through the Universe in our own particular, peculiar fashion.

Reference: The dipole repeller, Yehuda Hoffman, Daniel Pomarède, R. Brent Tully & Hélène M. Courtois, Nature Astronomy 1, Article number: 0036 (2017).

Ethan Siegel, Contributor. Feb 4, 2017

Forbes.com Startswithabang 2017 Ask Ethan The Dipole Repeller

 

Subtractive color

There are 2 ways to create color:

additive model/RGB:

Make new colors by adding beams of light

RGB: red, green, blue

subtractive model/CMYK:

Making new colors by adding pigments (dyes, inks, paints)

CMYK: Cyan, Magenta, Yellow, Black

This lesson is on the subtractive color model.

Additive and Subtractive primary colors

Paints/inks/dyes contain pigments, molecules that absorb some frequencies of light, but not others.

When paints/inks/dyes are mixed, the mixture absorbs all the frequencies that each individual one absorbs.

Examples:

Blue paint absorbs red, orange, and yellow light. It reflects the rest (blue, violet, some green)

Yellow paint absorbs blue & violent. It reflects mostly yellow, and some red, orange, and green.

Images by Paul Hewitt

Subtractive When blue and yellow paints are mixed Hewitt

Mixing colored light is called color mixing by addition.
When you cast lights on a stage, you use the rules of color addition, but when you mix paint, you use the rules of color subtraction.

The three colors most useful in color mixing by subtraction are:
• magenta (bluish red)
• yellow
• cyan (greenish blue)

Magenta, yellow, and cyan are the subtractive primary colors, used in printing illustrations in full color.

mixing-colored-pigments

Color printing is done on a press that prints each page with four differently colored inks (magenta, yellow, cyan, and black).

• Each color of ink comes from a different plate, which transfers the ink to the paper.

• The ink deposits are regulated on different parts of the plate by tiny dots.

• The overlapping dots of three colors plus black give the appearance of many colors.

colors-of-ink-used-for-color-illustrations

SlideShare on Color and Light

Learning Standards

SAT subject test in Physics: Waves and optics
• Physical optics, such as single-slit diffraction, double-slit interference, polarization, and color.

Massachusetts Arts Curriculum Framework: The Practice Of Creating
PreK- 4 Visual Arts Standards – Identify primary and secondary colors; predict and demonstrate the effects of blending or overlapping primary colors; demonstrate knowledge of making dark to light values of colors. Identify and use basic two-dimensional hollow and solid geometric shapes (circle, triangle, square, rectangle) and three-dimensional forms (sphere, pyramid, cube).

Grades 5-8 Visual Arts Standards – Create compositions that reflect knowledge of the elements and principles of art, i.e., line, color, form, texture; balance, repetition, rhythm, scale, and proportion. Demonstrate the ability to apply elements and principles of art to graphic, textile, product, and architectural design.

Massachusetts Arts Curriculum Framework
The Arts Disciplines: Visual Arts
PreK–12 STANDARD 2: Elements and Principles of Design

By the end of Grade 4: 2.1 Students will, for color, explore and experiment with the use of color in dry and wet media Identify primary and secondary colors and gradations of black, white and gray in the environment and artwork.
By the end of Grade 8: 2.7 Students will, for color, use and be able to identify hues, values, intermediate shades, tints, tones, complementary, analogous, and monochromatic colors. Demonstrate awareness of color by painting objective studies from life and freeform
abstractions that employ relative properties of color.

Additive color

There are 2 ways to create color:

additive model/RGB:

Make new colors by adding beams of light

RGB: red, green, blue

subtractive model/CMYK:

Making new colors by adding pigments (dyes, inks, paints)

CMYK: Cyan, Magenta, Yellow, Black

This lesson is on the additive color model.

Additive and Subtractive primary colors

This lesson is from Apple Valley High School
http://www.district196.org/avhs/dept/science/physics/physicsweb04/AVHSPhysics/color-notes.html

Additive color: mixing beams of colored light

We start with no light, and add colors of light together to get the final result.

Complementary colors: These are two colors (one primary, one secondary) which, when added together, make white light. They are:

magenta and green
yellow and blue
cyan and red

Three projectors emit the 3 primary colors of light (red, green, blue) on a “white” screen.

Where two of the primary colors overlap you’ll find a secondary color.

Where all three overlap you’ll find white light.

Complementary colors are always across the white spot from each other in this “color wheel”.

light-boxes-make-white-light

Mixing colors of light

We have a white screen. It can reflect any color of light we shine on it.

Now shine red light on the surface – and hold up a hand so we cast a shadow.

The shadow will have no light hitting it so it will be black, while the rest of the screen would reflect the red light.

red-light-on-hand-hewitt

Now let’s add a green light on the right side of the picture.
Check out what happens now!

red-and-green-light-on-paper

Notice how the screen has both green and red which makes yellow.

The shadow on the left blocks the green light, so the red light is the only light that hits that particular shadow.

The right shadow is green for the same reason. Cool, huh?

Now let’s add blue in the center. Check it out!

red-blue-and-green-bulbs-on-paper

The screen has gone to white since it has red, green and blue striking it’s surface.

It reflects all 3 colors back to our eyes, so we see white.

The shadows are now the secondary colors (magenta, yellow, cyan).

This is because each shadow has 2 of the 3 primary colors hitting it, so it becomes one of the secondary colors.

Note: All of this is ONLY for mixing rays of light.
If you try mixing pigments (the colored chemicals in paints, crayons, dyes, markers, etc) we will get totally different results.

Looking at a white object in a white light

White objects in white light

.

White object in blue light

m

white object in red light

m

red object in red light

m

red object in blue light

m

red apple and green pear in white light

m

red apple and green pear in red light

m

red apple and green pear in blue light

 

Problems

When three colored lamps, red, blue and green, illuminate a physics instructor in front of a white screen in a dark room, three slightly overlapping shadows appear. Specify the colors in regions 1 through 6.

three-color-lamps-on-a-guys-face-additive-color

http://dev.physicslab.org/Document.aspx?doctype=5&filename=Compilations_NextTime_Shadows2.xml

External lessons

PhET lab color vision

Additive and Subtractive Color in early color movies

http://www.widescreenmuseum.com/oldcolor/oldcolor.htm

Learning Standards

SAT subject test in Physics: Waves and optics
• Physical optics, such as single-slit diffraction, double-slit interference, polarization, and color.

Massachusetts Arts Curriculum Framework: The Practice Of Creating
PreK- 4 Visual Arts Standards – Identify primary and secondary colors; predict and demonstrate the effects of blending or overlapping primary colors; demonstrate knowledge of making dark to light values of colors. Identify and use basic two-dimensional hollow and solid geometric shapes (circle, triangle, square, rectangle) and three-dimensional forms (sphere, pyramid, cube).

Grades 5-8 Visual Arts Standards – Create compositions that reflect knowledge of the elements and principles of art, i.e., line, color, form, texture; balance, repetition, rhythm, scale, and proportion. Demonstrate the ability to apply elements and principles of art to graphic, textile, product, and architectural design.

Massachusetts Arts Curriculum Framework
The Arts Disciplines: Visual Arts
PreK–12 STANDARD 2: Elements and Principles of Design

By the end of Grade 4: 2.1 Students will, for color, explore and experiment with the use of color in dry and wet media Identify primary and secondary colors and gradations of black, white and gray in the environment and artwork.
By the end of Grade 8: 2.7 Students will, for color, use and be able to identify hues, values, intermediate shades, tints, tones, complementary, analogous, and monochromatic colors. Demonstrate awareness of color by painting objective studies from life and freeform
abstractions that employ relative properties of color

Nuclear fusion

nuclear fusion

https://kaiserscience.wordpress.com/physics/modern-physics/quantum-mechanics/

https://kaiserscience.wordpress.com/physics/modern-physics/nuclear-physics-and-radioactivity/

Barns Are Painted Red Because of the Physics of Dying Stars

External links

It’s Not Cold Fusion… But It’s Something – Scientific American

Low Energy Nuclear Reactions Work And Could Supplant Fossil Fuels – Edge.Org

Can Cold Fusion Come Back From the Dead? – Popular Mechanics

The cold fusion horizon, Huw Price – Aeon.Com

Elastic and Inelastic collisions

This lesson assumes that you have already learned about momentum and the difference between kinetic energy and potential energy.

When two (or more) objects collide, what determines their subsequent behavior? What happens next? The result will depend on whether they collide in an elastic or inelastic fashion. (or, more often, in a partially elastic fashion.)

Let’s take a look at these different kinds of collisions with some short animation clips (GIFs.) We’ll figure out the basic principles.

Elastic collisions

Objects collide:

(a) without being deformed

(b) no kinetic energy (energy of motion) is lost

Example 1: Gas molecules bouncing off of each other

Example 2 Pool (pocket billiards )

pool-game-billiards

Example 3 car bouncing off of a truck

Example 4: Two cars colliding, without any (apparent) deformation or heating

elastic-collision-gif

Inelastic Collisions

Objects collide:

(a) and parts are deformed

(b) much kinetic energy (energy of motion) is lost, and turned into heat

Example 5: car hitting a truck, and they stick together

Example 6: car hitting a truck, and they stick together

completely-inelastic-collision-gif

Partially elastic collisions

Objects collide:

(a) and are slightly deformed

(b) some kinetic energy (energy of motion) is lost, and turned into heat

Example 7: Cars bounce after a collision

partially-inelastic-collision-gif

How can we tell if a collision is elastic or not?

.

How can we tell if a collision is elastic or not?

Take into account the kinetic energy (the energy of motion)

KE tr   =   KE translational

   = kinetic energy as stuff “translates”, or moves

Video GIFs from http://waiferx.blogspot.com/2011/10/physics-presentation-collisions.html

Collisions in two dimensions

Conservation of momentum in two dimensions:

2D cars colliding momentum

image from physicsclassroom

How can this kind of analysis be useful? In forensic accident reconstruction.

forensic reconstruction traffic accident 2d GIF

“Accident Reconstruction is the forensic science of determining how an accident occurred while assisting in the determination of the cause or why an accident or particular event during an accident happened using all available physical evidence.”

“This evidence can be in the form of tire marks, gouges, vehicle parts, vehicle damage, surveillance video, electronic vehicle information, occupant and pedestrian injuries, witness testimony, etc.”

“A collision reconstructionist takes all of the available evidence, like pieces in a puzzle, utilizes available tools and research, to put together the larger picture of the overall accident event.”

Excerpted from Collision research and analysis

Learning Standards

2016 Massachusetts Science and Technology/Engineering Curriculum Framework

HS-PS2-2. Use mathematical representations to show that the total momentum of a system of interacting objects is conserved when there is no net force on the system. Emphasis is on the qualitative meaning of the conservation of momentum and the quantitative understanding of the conservation of linear momentum in
interactions involving elastic and inelastic collisions between two objects in one dimension.

HS-PS2-3. Apply scientific principles of motion and momentum to design, evaluate, and refine a device that minimizes the force on a macroscopic object during a collision. Clarification Statement: Both qualitative evaluations and algebraic manipulations may be used.

Common Core Math

CCSS.MATH.CONTENT.7.EE.B.4 Use variables to represent quantities in a real-world or mathematical problem, and construct simple equations and inequalities to solve problems by reasoning about the quantities.

CCSS.MATH.CONTENT.8.EE.C.7 Solve linear equations in one variable

CCSS.MATH.CONTENT.HSA.SSE.B.3 Choose and produce an equivalent form of an expression to reveal and explain properties of the quantity represented by the expression. (including isolating a variable)

CCSS.MATH.CONTENT.HSA.CED.A.4 Rearrange formulas to highlight a quantity of interest, using the same reasoning as in solving equations. For example, rearrange Ohm’s law V = IR to highlight resistance R.

Kinematics in music videos

Kinematics is the study of objects in motion. One uses math to analyze distance, displacement, speed, velocity, and acceleration. It even finds a use in music videos

“The One Moment” is from OK Go’s 2014 full-length, Hungry Ghosts

New video on NPR.org

http://okgo.net/2016/11/23/background-notes-and-full-credits-for-the-one-moment-video/

https://www.youtube.com/user/OkGo/videos

Background notes and full credits for “The One Moment” Video by OK Go.
Damian Kulash, Jr. (director and singer)

The song “The One Moment” is a celebration of (and a prayer for) those moments in life when we are most alive. Humans are not equipped to understand our own temporariness; It will never stop being deeply beautiful, deeply confusing, and deeply sad that our lives and our world are so fleeting. We have only these few moments. Luckily, among them there are a few that really matter, and it’s our job to find them. (We had no idea when we wrote the song that we’d be releasing its video in such critical moment for our nation and the world. It’s one of those moments when everything changes, whether we like it or not, so the song feels particularly relevant)

For the video, we tried to represent this idea literally — we shot it in a single moment. We constructed a moment of total chaos and confusion, and then unraveled that moment, discovering the beauty, wonder, and structure within.

Most of our videos have sought to deliver wonder and surprise, and this one is no exception. But usually our tone has been more buoyant, more exuberant. For this song — our most heartfelt and sincere — we wanted the sense of wonder to be more intimate and contemplative…

How did you do that?

We used very precise digital triggers to set off several hundred events in extremely quick succession.

The triggers were synchronized to high speed robotic arms which whipped the cameras along the path of the action.

Though the routine was planned as a single event, currently no camera control systems exist which could move fast enough (or for many sections, change direction fast enough) to capture a movement this long and complex with a single camera, so the video you see connects seven camera movements.

How long did the routine take in real time?

The first three quarters of the video, from the beginning of the song until I pick up the umbrella at the a cappella breakdown, unfold over 4.2 seconds of real time. Then I lip sync in real time for about 16 seconds (we thought it was important to have a moment of human contact at this point in the song, so we returned to the realm of human experience) and we return to slow motion for the final chorus paint scene, which took a little longer than 3 seconds in real time.

How many things happen in it?

It sort of depends how you count “things,” but the there are 318 events (54 colored salt bursts behind Tim, 23 exploding paint buckets, 128 gold water balloons, etc.) that were synchronized to the music before the breakdown. After that there are only 9 digitally triggered events.

Just how slow is this, and is it all one speed?

It is not all one speed, but each section is at a constant rate, meaning that time does not “ramp” (accelerate or decelerate). We just toggle from one speed to another. When the guitars explode, we are 200x slower than reality (6,000 frames per second), but Tim and Andy’s short bursts of lip sync (Tim twice and Andy once) are only 3x slower than real life (90 frames per second). The watermelons are around 150x, and the spray paint cans are a little over 60x.

How did you plan all this?

The whole point of the video is to explore a time scale that we can’t normally experience, but because it’s so inaccessible to us, our tools for dealing with it are indirect. The only way we can really communicate with that realm is through math. The choreography for this video was a big web of numbers — I made a motherfucker of a spreadsheet. It had dozens of connected worksheets feeding off of a master sheet 25 columns wide and nearly 400 rows long. It calculated the exact timing of each event from a variety of data that related the events to one another and to the time scale in which they were being shot. Here’s a screen shot of just the first few lines, to give you a sense.

the-one-moment-video-by-ok-go-spreadsheet

____________________

Example of a high speed robotic camera arm

http://www.8k-47.com/technologies/bolt-highspeed-cinebot/

http://www.roboticgizmos.com/spike-robotic-motion-control-camera-system/

http://www.mrmoco.com/thebolt/

https://www.youtube.com/watch?v=HRvnYmxcMOY

 

 

 

 

Internal reflection

Physics is a deeply conceptual class. It’s not like English or History, where everyone already knows vast amounts of content before even entering. Students entering high school already knowing what a story is, what characters are, what a theme is, and what a moral is.

The human themes discussed by Shakespeare or Homer are universal. They are intuitively understood by even the least prepared of readers. Students may not know much about Elizabethan England, or ancient Greece, but they know what it means to be happy, sad, angry, or jealous. They know what it means for a character to fall in love, or to flee from their home.

When they read about a King entering a castle, and making a pronouncement to the citizens, students get it right away. Does any student ever erroneously think that “the pronouncement” is a person? That “the King” is a large object built out of wood and stone that someone lives in? That “the Castle” is a letter to be read? Of course not.

This is not so, however, with concepts in physics. Student entering a physics class often have no meaningful understanding of conservation laws, or Newton’s laws of motion. Most don’t understand why it is essential to differentiate between conservation of energy and conservation of momentum. When someone doesn’t know if a problem requires conservation of energy concepts, or kinematic equation concepts to solve a problem, that’s a like a person not knowing the difference between a King and a Castle. It is that basic.

Outside of AP Physics we usually are teaching from the ground level upwards.

No teaching method, homework assignment, or pedagogical technique has much effect on student performance – unless that student takes time to engage in internal mental reflection.

When students review at home what we learned in class,

When students think about what happened, and why it happened,

When students compare their preconceptions to what they have observed

only they are engaging in internal mental reflection.

If a student chooses not do this, then there is little a teacher can add. We can explain it for you, but we can’t understand it for you.

This is one reason why some students struggle. Doing classwork has only limited usefulness, unless one internally reflects on the subject.

How to be a good student

Chapter 12. Learning Through Reflection, by Arthur L. Costa and Bena Kallick

Learning Through Reflection

Google Scholar Search

Scholar.google.com Learning internal reflection

Scholar Google: Mental reflection

Aristotle’s laws of motion

Aristotle (Ἀριστοτέλης) 384–322 BCE was a Greek philosopher and scientist born in the city of Stagira, in classical Greece.

Aristotle bust

At 17 years of age, he joined Plato’s Academy in Athens and remained there until the age of thirty-seven (c. 347 BCE)

ancient-athens-map

His writings cover many subjects – including physics, biology, zoology, logic, ethics, poetry, theater, music, linguistics, and politics. They constitute the first comprehensive system of Western philosophy.

Shortly after Plato died, Aristotle left Athens and, at the request of Philip of Macedon, tutored Alexander the Great beginning in 343 BC.

Aristotle’s views on physical science profoundly shaped medieval scholarship. Their influence extended from Late Antiquity and the Early Middle Ages into the Renaissance, and were not replaced systematically until the Enlightenment and theories such as classical mechanics.

  • excerpted and adapted from Aristotle. (2016, October 20). Wikipedia, The Free Encyclopedia.

___________________________

Aristotle’s laws of motion

Aristotle bust
Aristotle set out 3 laws of motion, based on observations (but not on experiment)

* objects fall at a constant rate, that depends on their size and weight.

* there is a difference between “violent motion” versus “natural motion”

* objects in the heavens (the celestial sphere) move in circular motion, without any external force compelling them to do so.
objects on Earth (the terrestrial sphere) move in straight lines, unless forced to move in a circular motion.

Here is the modern, correct view of how gravity accelerates objects of different masses.

(Does the mass and size affect the speed at which they fall?)

Yet here is Aristotle’s view of how gravity accelerates objects of different masses.

(How does this differ from the previous animation?)

Aristotles view of gravity

What about pushing and pulling?

Natural vs Unnatural Motion

For objects on Earth, Aristotle thought that objects moved by people (“unnatural motion”) would move in a straight line, and when that “unnatural force” ran out, then natural motion would take over.

So what would happen if a canon fired a cannonball? Aristotle supposed that it would move in a straight line (due to the unnatural force), and then would fall straight down (due to a different, natural force.)

aristotle-idea-of-cannonball-not-projectile-motion

For Aristotle, once “violent motion” (from people) extinguished itself, natural motion takes over, and then the cannon ball falls to its natural place, the earth.

An animation of what this would look like.

However, as Galielo showed in the 1500’s, Aristotle’s view isn’t correct at all.  Anyone who watches an archer fire an arrow into the air, and carefully observes, would see that this doesn’t happen.

Galileo showed that the vertical motion (up/down) and horizontal motion (size-to-side) are independent.

When you fire an arrow, cannonball, or pop-fly in baseball, into the air, what happens?

The vertical motion slowly decreases, reaches zero (at the peak), and then increases in the opposite (downward) direction.

The horizontal motion actually stays constant (doesn’t speed up, or slow down.)

projectile-motion-canon-on-cliff

Heavenly forces vs terrestrial forces

Aristotle thought that heavenly (celestial) objects, by their nature, forever moved in circles – without any external force acting on them.

Earthly (terrestrial) objects were believed to have a separate set of laws of motion. Earthly objects supposedly would always stop moving, of their own accord, on their own.

As we will learn, there aren’t really 2 sets of laws (heavenly and earthly); rather, the laws of nature are the same everywhere:

* objects naturally travel only in straight lines.
* for objects to have a circular motion requires some external force, keeping them pulled into a circular path

How could one of the greatest thinkers of the classical world be in error? The ancient Greeks had a preference for attempting to find truth through logic alone. Greeks viewed observations of the physical world as a valid way  to learn, but held this to be inferior to intellect.

Also, Aristotle never ran experiments, so he was very limited in what he could observe. In the medieval era, Galileo (and others) ran controlled experiments. The results of these experiments were analyzed with math.

Their findings ended the acceptance of Aristotelian physics.

Galileo learned critical thinking skills from his father, Vincenzo

Galileo and Einstein: History of Physics – Prof Michael Fowler

Vincenzo Galilei, father of Galileo.

Vincenzo Galilei, father of Galileo.

Galileo continued his father’s tradition of critical inquiry

Galileo rolled balls along surfaces tilted at different angles.

a. When ball rolls downward, it moves with Earth’s gravity, and its speed increases.

b. When ball rolls upward, it moves against gravity and loses speed.

c. When ball rolls on level plane, it doesn’t move with or against gravity.

 Galileo rolls balls slope

a. The ball rolls down the incline, and then up the opposite incline,
and reaches its initial height.

b. As the angle of the upward incline is reduced, the ball rolls a greater distance before reaching its initial height.

c. If there is no friction, then the ball will never stop – unless it hits something.

Galileo rolls balls no friction never stops

Galileo’s conclusion was supported by another line of reasoning.

He described two inclined planes facing each other.

A ball released to roll down one plane would roll up the other to reach nearly the same height.

The smoother the planes were, the more nearly equal would be the initial and final heights.

He noted that the ball tended to attain the same height, even when the second plane was longer and inclined at a smaller angle than the first plane.

Always, the ball went farther and tended to reach the same height.

Inclined Plane – Galileo’s Battle for the Heavens PBS NOVA

Video clip: Galileo’s inclined plane PBS media

Advanced: Similar studies with the moment of inertia

Rolling balls, cylinders and tubes down inclined plane: Moment of Inertia

http://makeagif.com/i/sWbNgM

 

Something special: The brachistochrone – curve of quickest descent. And the tautochrone- the curve for which the time taken by an object sliding without friction in uniform gravity to its lowest point is independent of its starting point.

brachistochrone-and-tautochrone-curve

 

Aristotle’s laws of motion

Excerpted from a lecture by Professor Michael Fowler, U. Va. Physics, 9/3/2008

http://galileoandeinstein.physics.virginia.edu/lectures/aristot2.html

What Aristotle achieved in those years in Athens was to begin a school of organized scientific inquiry on a scale far exceeding anything that had gone before. He first clearly defined what was scientific knowledge, and why it should be sought. In other words, he single-handedly invented science as the collective, organized enterprise it is today. Plato’s Academy had the equivalent of a university mathematics department, Aristotle had the first science department, truly excellent in biology, but, as we shall see, a little weak in physics.

After Aristotle, there was no comparable professional science enterprise for over 2,000 years, and his work was of such quality that it was accepted by all, and had long been a part of the official orthodoxy of the Christian Church 2,000 years later. This was unfortunate, because when Galileo questioned some of the assertions concerning simple physics, he quickly found himself in serious trouble with the Church.
Aristotle’s method of investigation:

defining the subject matter

considering the difficulties involved, by reviewing the generally accepted views on the subject, and suggestions of earlier writers

presenting his own arguments and solutions

This is the pattern modern research papers follow, Aristotle was laying down the standard professional approach to scientific research.

Aristotle often refuted an opposing argument by showing that it led to an absurd conclusion, this is called reductio ad absurdum (reducing something to absurdity). As we shall see later, Galileo used exactly this kind of argument against Aristotle himself, to the great annoyance of Aristotelians [people who fully agreed with Aristotle] 2,000 years after Aristotle.

[Aristotle himself likely would not have minded later thinkers disagreeing with him;
in his lifetime Aristotle would change his mind if he found new information or a more logical argument.]

In contrast to Plato, who felt the only worthwhile science to be the contemplation of abstract forms, Aristotle practiced detailed observation and dissection of plants and animals, to try to understand how each fitted into the grand scheme of nature, and the importance of the different organs of animals.

It is essential to realize that the world Aristotle saw around him in everyday life was very different indeed from that we see today. Every modern child has since birth seen cars and planes moving around, and soon finds out that these things are not alive, like people and animals. In contrast, most of the motion seen in fourth century Greece was people, animals and birds, all very much alive. This motion all had a purpose, the animal was moving to someplace it would rather be, for some reason, so the motion was directed by the animal’s will.

For Aristotle, this motion was therefore fulfilling the “nature” of the animal, just as its natural growth fulfilled the nature of the animal.

To account for motion of things obviously not alive, such as a stone dropped from the hand, Aristotle extended the concept of the “nature” of something to inanimate matter. He suggested that the motion of such inanimate objects could be understood by postulating that elements tend to seek their natural place in the order of things:

So earth moves downwards most strongly, water flows downwards too, but not so strongly, since a stone will fall through water. In contrast, air moves up (bubbles in water), and fire goes upwards most strongly of all, since it shoots upward through air.

This general theory of how elements move has to be elaborated, of course, when applied to real materials, which are mixtures of elements. He would conclude that wood has both earth and air in it, since it does not sink in water.

Natural Motion and Violent Motion

Things also move because they are pushed. A stone’s natural tendency, if left alone and unsupported, is to fall, but we can lift it, or even throw it through the air.

Aristotle termed such forced motion “violent” motion as opposed to natural motion.

The term “violent” just means that some external force is applied to it.

Aristotle was the first to think quantitatively about the speeds involved in these movements. He made two quantitative assertions about how things fall (natural motion):

Heavier things fall faster, the speed being proportional to the weight.

The speed of fall of a given object depends inversely on the density of the medium it is falling through.

So, for example, the same body will fall twice as fast through a medium of half the density.

Notice that these rules have a certain elegance, an appealing quantitative simplicity. And, if you drop a stone and a piece of paper, it’s clear that the heavier thing does fall faster, and a stone falling through water is definitely slowed down by the water, so the rules at first appear plausible.

The surprising thing is, in view of Aristotle’s painstaking observations of so many things, he didn’t check out these rules in any serious way.

It would not have taken long to find out if half a brick fell at half the speed of a whole brick, for example. Obviously, this was not something he considered important.

From the second assertion above, he concluded that a vacuum cannot exist, because if it did, since it has zero density, all bodies would fall through it at infinite speed which is clearly nonsense.

For violent motion, Aristotle stated that the speed of the moving object was in direct proportion to the applied force.

This means first that if you stop pushing, the object stops moving.

This certainly sounds like a reasonable rule for, say, pushing a box of books across a carpet, or an ox dragging a plough through a field.

This intuitively appealing picture, however, fails to take account of the large frictional force between the box and the carpet. If you put the box on a sled and pushed it across ice, it wouldn’t stop when you stop pushing. Centuries later, Galileo realized the importance of friction in these situations.

Learning Standards

2016 Massachusetts Science and Technology/Engineering Curriculum Framework
HS-PS2-1. Analyze data to support the claim that Newton’s second law of motion is a
mathematical model describing change in motion (the acceleration) of objects when
acted on by a net force.

HS-PS2-10(MA). Use free-body force diagrams, algebraic expressions, and Newton’s laws of motion to predict changes to velocity and acceleration for an object moving in one dimension in various situations

Massachusetts History and Social Science Curriculum Framework

The roots of Western civilization: Ancient Greece, C. 800-300 BCE.
7.34 Describe the purposes and functions of development of Greek institutions such as the lyceum, the gymnasium, and the Library of Alexandria, and identify the major accomplishments of the ancient Greeks.

WHI.33 Summarize how the Scientific Revolution and the scientific method led to new theories of the universe and describe the accomplishments of leading figures of the Scientific Revolution, including Bacon, Copernicus, Descartes, Galileo, Kepler, and Newton.

A FRAMEWORK FOR K-12 SCIENCE EDUCATION: Practices, Crosscutting Concepts, and Core Ideas
PS2.A: Forces and motion – How can one predict an object’s continued motion, changes in motion, or stability?

Interactions of an object with another object can be explained and predicted using the concept of forces, which can cause a change in motion of one or both of the interacting objects… At the macroscale, the motion of an object subject to forces is governed by Newton’s second law of motion… An understanding of the forces between objects is important for describing how their motions change, as well as for predicting stability or instability in systems at any scale.

Math is the language of physics

 

Mathematics is the language of physics

Natural philosophy [i.e., physics] is written in this grand book – I mean the universe – which stands continually open to our gaze, but it cannot be understood unless one first learns to comprehend the language and interpret the characters in which it is written.

[The universe] cannot be read until we have learned the language and become familiar with the characters in which it is written. It is written in mathematical language, and the letters are triangles, circles and other geometrical figures, without which means it is humanly impossible to comprehend a single word.

  • Galileo, Opere Il Saggiatore p. 171

Mathematics is the language of physics. Physical principles and laws, which would take two or even three pages to write in words, can be expressed in a single line using mathematical equations. Such equations, in turn, make physical laws more transparent, interpretation of physical laws easier, and further predictions based on the laws straightforward.

  • Mesfin Woldeyohannes, Assistant Professor, Western Carolina University

ἀεὶ ὁ θεὸς γεωμετρεῖ – Aei ho theos geōmetreî. God always geometrizes.

  • Plato, 400 BCE, classical Greece, as quoted by Plutarch in his The Moralia, Quaestiones convivales. (circa 100 CE)

Math is so useful in the real world that it’s eerie

There is a classic paper, The Unreasonable Effectiveness of Mathematics in the Natural Sciences, that it should be read even by high school students.

Wigner begins his paper with the belief, common among those familiar with mathematics, that mathematical concepts have applicability far beyond the context in which they were originally developed.

Based on his experience, he says “it is important to point out that the mathematical formulation of the physicist’s often crude experience leads in an uncanny number of cases to an amazingly accurate description of a large class of phenomena.”

Wigner then invokes the fundamental law of gravitation as an example. Originally used to model freely falling bodies on the surface of the earth, this law was extended on the basis of what Wigner terms “very scanty observations” to describe the motion of the planets, where it “has proved accurate beyond all reasonable expectations”.

Another oft-cited example is Maxwell’s equations, derived to model the elementary electrical and magnetic phenomena known as of the mid 19th century. These equations also describe radio waves, discovered by David Edward Hughes in 1879, around the time of James Clerk Maxwell’s death.

Wigner sums up his argument by saying that “the enormous usefulness of mathematics in the natural sciences is something bordering on the mysterious and that there is no rational explanation for it”. He concludes his paper with the same question with which he began:

The miracle of the appropriateness of the language of mathematics for the formulation of the laws of physics is a wonderful gift which we neither understand nor deserve. We should be grateful for it and hope that it will remain valid in future research and that it will extend, for better or for worse, to our pleasure, even though perhaps also to our bafflement, to wide branches of learning.

  • The Unreasonable Effectiveness of Mathematics in the Natural Sciences. (2016, September 11). In Wikipedia, The Free Encyclopedia

The Unreasonable Effectiveness of Mathematics in the Natural Sciences

Math is different from physics

Mathematics does not need to bother itself with real-world observations. It exists independently of any and all real-world measurements. It exists in a mental space of axioms, operators and rules.

Physics depends on real-world observations. Any physics theory could be overturned by a real-world measurement.

None of maths can be overturned by a real-world measurement. None of geometry can be.

Physics starts from what could be described as a romantic or optimistic notion: that the universe can be usefully described in mathematical terms; and that humans have the mental ability to assemble, and even interpret, that mathematical description.

Maths need not concern itself with how the universe actually works. Perhaps there are no real numbers, one might think it is likely that there is only a countable number of possible measurements in this universe, and nothing can form a perfect triangle or point.

Maths, including geometry, is a perfect abstraction that need bear no relation to the universe as it is.
Physics, to have any meaning, must bear some sort of correspondence to the universe as it is.

Why-is-geometry-mathematics-and-not-physics? Physics StackExchange, by EnergyNumbers

Related articles

What is mathematics, really? Is it made by humans or a feature of the universe? Math in art & poetry.

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Thanks for reading. While you’re here see our articles on astronomybiologychemistryEarth sciencephysicsthe scientific method, and making connections to science through reading, books, TV and movies.

Discovery of conservation of momentum

You can explore this history-oriented lesson by Prof. Michael Fowler.

Momentum, Work and Energy Michael Fowler, U. Va. Physics

In 530 A.D., working in Alexandria, Byzantine philosopher John Philoponus developed a concept of momentum in his commentary to Aristotle’s Physics. Aristotle had claimed that everything that is moving must be kept moving by something. For example, a thrown ball must be kept moving by motions of the air.

Aristotle bust

Most writers continued to accept Aristotle’s theory until the time of Galileo, but a few were skeptical.

Philoponus pointed out the absurdity in Aristotle’s claim that motion of an object is promoted by the same air that is resisting its passage.

He proposed instead that an impetus was imparted to the object in the act of throwing it.

Ibn Sina (Arabic ابن سینا‎) (known by his Latinized name, Avicenna) read Philoponus and published his own theory of motion in The Book of Healing in 1020. He agreed that an impetus is imparted to a projectile by the thrower – but unlike Philoponus, who believed that it was temporary, and would decline even in a vacuum – Ibn Sina viewed it as a persistent. He understood that it required external forces – such as air resistance – to dissipate it.

Avicenna

These ideas were refined by European philosophers Peter Olivi and Jean Buridan. Buridan, who in about 1350 was made rector of the University of Paris, referred to impetus as proportional to the weight times the speed.

Like Ibn Sīnā, Buridan held that impetus (momentum) would not go away by itself; it could only dissipate if it encountered air resistance, friction, etc.

http://www.slideshare.net/StephenKwong1/part-1-world-in-motion

http://www.slideshare.net/StephenKwong1/part-1-world-in-motion

http://www.slideshare.net/StephenKwong1/part-1-world-in-motion

http://www.slideshare.net/StephenKwong1/part-1-world-in-motion

René Descartes believed that the total “quantity of motion” in the universe is conserved: quantity of motion = size and speed.

But Descartes didn’t distinguish between mass and volume, so this is not a specific equation.

Leibniz, in his “Discourse on Metaphysics”, gave an experimental argument against Descartes’ idea of “quantity of motion”.

Leibniz dropped blocks of different sizes, different distances.

He found that [size speed] did not yield a conserved quantity.

Gottfried_Wilhelm_von_Leibniz

The first correct statement of conservation of momentum:
English mathematician John Wallis, 1670
Mechanica sive De Motu, Tractatus Geometricus:

Isaac Newton’s Philosophiæ Naturalis Principia Mathematica, 1687

Defined “quantity of motion”, as “arising from the velocity and quantity of matter conjointly”
-> mass x velocity – which identifies it as momentum.

Isaac Newton

Adapted from “Momentum.” Wikipedia, The Free Encyclopedia. 2 Oct. 2015.

External resources

The cause of motion from Aristotle to Philoponus

The cause of motion Descartes to Newton

Learning Standards

2016 Massachusetts Science and Technology/Engineering Curriculum Framework

HS-PS2-2. Use mathematical representations to show that the total momentum of a system of interacting objects is conserved when there is no net force on the system. Emphasis is on the qualitative meaning of the conservation of momentum and the quantitative understanding of the conservation of linear momentum in
interactions involving elastic and inelastic collisions between two objects in one
dimension.
HS-PS2-3. Apply scientific principles of motion and momentum to design, evaluate, and refine a device that minimizes the force on a macroscopic object during a collision. Clarification Statement: Both qualitative evaluations and algebraic manipulations may be used.

Common Core Math

  • CCSS.MATH.CONTENT.7.EE.B.4  Use variables to represent quantities in a real-world or mathematical problem, and construct simple equations and inequalities to solve problems by reasoning about the quantities.
  • CCSS.MATH.CONTENT.8.EE.C.7  Solve linear equations in one variable
  • CCSS.MATH.CONTENT.HSA.SSE.B.3  Choose and produce an equivalent form of an expression to reveal and explain properties of the quantity represented by the expression. (including isolating a variable)
  • CCSS.MATH.CONTENT.HSA.CED.A.4  Rearrange formulas to highlight a quantity of interest, using the same reasoning as in solving equations. For example, rearrange Ohm’s law V = IR to highlight resistance R.
  • http://www.corestandards.org/Math/