Open in TheBrain

Points and Lines in the Affine Plane

Wild Egg mathematics courses

3.77K subscribers

SUBSCRIBED

This is the first lecture in the Algebraic Calculus One course, which will present an exciting new approach to calculus, sticking with rational numbers and high school algebra. The course will be carefully framed on careful definitions, explicit examples and concrete computations. In this first rather introductory lecture, we introduce the basic geometric framework of the affine grid plane, or Cartesian coordinate geometry, and review what hopefully should be familiar concepts around points and lines. But we will also introduce a perhaps novel point of view coming from projective geometry, employing the important ideas of proportions. This first lecture has two parts. The second part is given by Anna Tomskova and is Projective Points and Lines. ************************ Screenshot PDFs for my videos are available at the website http://wildegg.com. These give you a concise overview of the contents of the lectures for various Playlists: great for review, study and summary. My research papers can be found at my Research Gate page, at https://www.researchgate.net/profile/...My blog is at http://njwildberger.com/, where I will discuss lots of foundational issues, along with other things. Online courses will be developed at openlearning.com. The first one, already underway is Algebraic Calculus One at https://www.openlearning.com/courses/... Please join us for an exciting new approach to one of mathematics' most important subjects! If you would like to support these new initiatives for mathematics education and research, please consider becoming a Patron of this Channel at https://www.patreon.com/njwildberger Your support would be much appreciated.

00:01

[Music]

00:13

hello everyone I'm Norman Wahlberg and

00:15

welcome to the algebraic calculus so in

00:18

this lecture we're going to be looking

00:20

at the geometrical underpinnings of the

00:22

subject which is basically sort of

00:24

linear algebra or affine geometry and

00:27

also the corresponding algebraic set up

00:30

that captures those geometrical notions

00:34

logically it's usually the algebraic

00:36

setup which is primary for us but we

00:41

like to have pictures in mind as well

00:42

and notably the pictures are not those

00:45

of Euclidean geometry so the usual

00:48

pictures that you find in most calculus

00:50

textbooks are not exactly in the

00:53

direction where to thinking we're

00:54

adopting rather a more I find geometry

00:58

point of view and I want to explain that

00:59

because it might not be that familiar to

01:01

you so roughly what we're doing is we're

01:04

thinking about geometry in the plane

01:05

with a notion of parallelism first and

01:09

foremost in our minds so the

01:10

perpendicularity is not actually going

01:13

to play a role ok so here is a picture

01:18

of an XY plane maybe a little bit

01:20

different from what you're used to

01:22

because these axes don't appear exactly

01:24

perpendicular to you and you can see

01:27

that the spacing in the X directions and

01:29

the spacings and the Y directions are

01:31

not exactly the same

01:33

although along the x direction we have

01:35

equal spacing and along the Y direction

01:37

we have equal spacing but this

01:39

separation here in this separation here

01:41

are not really cool corresponding ok so

01:44

that's the the basic set up we might

01:46

call that the affine plane and a natural

01:48

question is you know how do you organize

01:50

such a thing and you know it turns out

01:53

there's a a Renaissance artist kind of

01:57

point of view that allows one to create

02:00

such a thing if you just have a

02:01

draftsman stool that allows you to

02:03

create parallel lines so suppose we have

02:06

such a kind of a fine grid then we can

02:08

talk about points and lines which are at

02:11

least the

02:11

first fundamental objects of study so a

02:14

point for us will be something like this

02:17

a equals 3 2 that represents the point

02:20

which is 3 in the X Direction 2 in the y

02:22

direction

02:22

there it is there so what we do is we go

02:25

to the x position here that's labeled by

02:28

3 and then we draw a line through that

02:31

which is parallel to the y axis and we

02:34

simultaneously go up to the position on

02:36

the y axis corresponding to 2 and draw

02:39

through that a line parallel to the x

02:42

axis okay and then it's the meet of

02:44

these two lines that determines that

02:47

point a the other kind of ingredient

02:50

that we'll need is that of a line ok and

02:54

a line for us is an equation like this X

02:57

plus 2y equal to this equation describes

02:59

this line maybe the name of this line is

03:02

L ok it passes through the point 0 1 it

03:07

also passes through the point 2 0 and of

03:10

course through many other points so

03:13

we've already become sort of familiar

03:14

first with this basic setup where we do

03:17

not assume perpendicular kind of

03:19

standard Euclidean graph paper kind of

03:24

framework ok this is somewhat more

03:26

general all right so now let's make an

03:29

official definition basically an

03:31

algebraic definition we'll say that an

03:34

affine point is a pair of numbers in

03:37

square brackets for example this thing

03:40

here

03:40

there's square brackets and there's two

03:43

numbers 1 and 5 over 2 and they're

03:46

separated by a comma there's a left

03:48

bracket on the side and a right bracket

03:50

on this line these are square brackets

03:51

ok so this is an affine point and in

03:55

this case it's name is capital a so we

03:57

say a equals the point 1 5 over 2 now in

04:02

this course when we refer to numbers the

04:05

default is usually rational numbers

04:08

because this is a very algebraic

04:11

approach so for us real numbers are

04:14

highly problematic and we're going to

04:17

avoid them almost entirely surprisingly

04:19

but we are going to allow the

04:21

possibility of extending our

04:24

considerations to other fields also in

04:27

particular later on to finite fields so

04:31

ultimately the same kinds of definitions

04:33

will also work if we replace our notion

04:36

of number with the notion of a finite

04:38

field number whatever that is you don't

04:40

need to understand what that is at this

04:41

stage okay but currently the default

04:44

when I say number is it's a rational

04:46

number like a fraction now this point is

04:51

a purely expression oriented object but

04:56

it can be interpreted geometrically in a

04:58

wide variety of ways so here is one

05:01

possible interpretation here is one kind

05:03

of representation of an affine plain and

05:06

then the point here a is one five over

05:10

two here's another representation a

05:12

different kind of affine plain one and

05:16

five - there's the point a in this

05:18

scenario so both of these are correct

05:20

and illustrate this idea that it's not

05:25

really the geometry that's primary it's

05:27

the algebra that's primary and a given

05:30

algebraic object will have many

05:32

different geometrical manifestations or

05:35

interpretations okay so that's that's

05:40

our rough orientation to things okay

05:42

we're gonna start with the algebraic

05:44

thing we're gonna say precisely what we

05:46

mean when we write something down

05:47

typically as an expression involving

05:49

certain symbols and then we're going to

05:51

interpret that in perhaps a different

05:54

number of ways geometrically alright and

05:58

our second definition is that of an

06:00

affine line okay so a line for us is an

06:04

equation in the variables x and y of the

06:07

following form ax + b y equals C where a

06:12

B and C are numbers with the crucial

06:16

condition that a and B these two numbers

06:19

here are not both 0 one of them can be 0

06:24

but not both of them that's what a line

06:31

will be for us so for us a line is not a

06:33

set of points

06:37

is not a set of points even were a set

06:39

of points that we would have to worry

06:41

about you know how to encode this set of

06:43

points onto our hard drive which is

06:45

basically an impossibility unless you're

06:48

working over a finite field then you can

06:49

do it but over the rationals you can't

06:51

describe all the all the points on this

06:54

and that doesn't even have any meaning

06:55

to me because there's all these

06:57

difficulties associated with dealing

06:59

with numbers which are so big that they

07:00

don't fit into the universe okay so I

07:02

don't want to go there so it's much

07:04

better if we just think about a line not

07:07

as a set of points but actually it's

07:08

just an equation now however we do have

07:12

to say that there's some there's some

07:14

ambiguity here because a given equation

07:16

can be expressed in alternate ways so we

07:20

could perform algebraic manipulations

07:21

for example the line X plus 3 y equals 2

07:24

okay we can multiply that equation by 2

07:27

to get the line 2x plus 6 y equals 4 and

07:30

we would want these two to be the same

07:32

line or maybe we could bring them two to

07:36

the other side here get minus 2 plus X

07:38

plus 3 y equals 0 or maybe we could

07:41

solve for y bring the X to the other

07:43

side and divide by 3 to get y equals

07:45

minus 1/3 X plus 2/3 so these are all

07:49

the same line for us now maybe that's a

07:53

little bit unsatisfactory and I hope you

07:56

do feel that a little bit okay that it's

07:59

a little bit ambiguous because now how

08:01

is our computer going to tell whether

08:03

this line is equal to this line and that

08:07

in fact will motivate the short well

08:10

talking about an alternate form of

08:12

describing lines involving projective

08:14

ideas okay so we're going to get to that

08:16

but at least at this stage here with

08:18

this connect with standard high school

08:20

terminology so we now have points and we

08:23

have lines as linear equations in X and

08:25

y so we know what a point is we know

08:29

what a line is now we have to describe

08:30

the relationship between them we say

08:32

that a point a which is say x0 y0 lies

08:36

on the line L given by the equation ax

08:41

plus B y equals C precisely when a x0

08:46

plus b y0 equals c in other words

08:51

the equation is satisfied if you plug in

08:54

the values of x0 y0 let define a into

09:00

X&Y there's alternate notation or

09:06

terminology for this we equivalently say

09:09

that the line L passes through a or

09:13

sometimes we say that the point a is

09:15

incident with the line L great ok

09:20

another important definition is this

09:22

basic idea of parallelism which I said

09:24

was at the heart of affine geometry so

09:26

we should say when two lines are

09:28

parallel so the line l1 say with

09:33

equation a 1 X plus B 1 y equal C 1 and

09:36

the line l2 which is a 2 X plus B 2 y

09:40

equals C 2 they are parallel precisely

09:43

when the following relation is satisfied

09:49

when a 1 times B 2 minus a 2 times B 1

09:54

equals 0 now in this situation we will

10:00

sometimes write that l1 is parallel to

10:02

l2 by using two vertical bars to

10:05

represent parallelism this is a very

10:09

important kind of expression that we're

10:11

gonna be seeing quite a lot in this

10:13

course alright so this is our first

10:15

example of it it's describing

10:18

parallelism of two lines and I've

10:22

arranged the indices here so instead of

10:25

having a B and C and D E and F it's

10:28

maybe a little bit easier to remember

10:30

this if we go to the additional work of

10:33

using indices so ones for this first

10:37

line and twos for the second line it

10:39

somehow makes things consistent and

10:41

reduces the number of variables

10:43

altogether even at the cost of a slight

10:46

amount of extra work with the indices so

10:49

that's something that would have to play

10:51

off against each other quite a lot in

10:54

the course you know

10:55

so anyway I just point that out that

10:57

sometimes it's nice to use indices to

10:59

sort of organize or book keep the

11:02

objects that we're interested in okay so

11:05

there is the definition of parallelism

11:07

for lines a few more hopefully familiar

11:11

definitions will say that points a B and

11:13

C are collinear precisely when they all

11:16

lie on a given line L and we'll say that

11:20

lines K L and M say are concurrent

11:24

precisely when they all pass through a

11:27

given point a so for example here's a

11:30

picture of three collinear points they

11:33

all happen to lie on this line so the

11:35

point a point B Point C it's a point on

11:38

a here is the y intercept of this line

11:42

it's the point 0 2 at the point B here

11:45

is the x intercept of this line it's the

11:47

point 3 comma 0 and here's another point

11:50

on it say C which has x-coordinate 1 and

11:54

then to find the y coordinate we would

11:56

sort of plug x equals 1 here and solve

11:58

for y and get 4 over 3 here is an

12:02

example of a point with 3 lines through

12:05

it so these are three concurrent lines

12:07

the point is to 1 and lines are well

12:12

here's the line x equals 2 yeah that's a

12:15

valid line here's the line y equals 1

12:19

which is a valid line and here's some

12:22

other line it happens to be X plus y

12:25

equals 3 and we can check that that

12:28

actually does pass through a because 2

12:31

plus 1 does equal 3

12:33

okay so we have collinear points and

12:35

concurrent lines now we want to augment

12:40

our number system a little bit think

12:42

about numbers in not just an absolute

12:45

way but in a kind of a relative way so

12:48

for example if I have two objects and I

12:50

want to sort of compare them let's say I

12:52

want to compare their weights one way is

12:54

to sort of weigh this one and get a

12:56

number and then weigh this one and get a

12:58

number and then compare those two

12:59

numbers but another way is to not worry

13:02

about the actual absolute measurements

13:06

of those weights of the two things but

13:07

just the relative weights

13:09

so maybe we can establish that this one

13:11

weighs twice as much as this one without

13:14

actually individually weighing them both

13:17

so we get a proportion the weights are

13:19

in the proportion two to one so this

13:22

kind of relative notion of numbers was

13:24

very important to the Greeks who thought

13:27

geometrically okay rather than

13:30

arithmetic li primarily but so they had

13:32

maybe one segment like this and maybe

13:34

another segment

13:35

you know half the size and they would

13:37

say well this the proportion this

13:39

segment to this segment is two to one

13:41

that kind of thing so we want to allow

13:45

ourselves some flexibility in terms of

13:47

being able to use this kind of notion of

13:50

number sometimes okay so we're gonna

13:53

introduce the idea of a proportion here

13:55

okay so what is a proportion well there

14:00

are different kinds of proportions the

14:01

simplest ones are the two proportion so

14:03

a two proportion is an expression A to B

14:08

where there's a colon here okay so a

14:11

colon B where a and B are numbers in

14:15

other words typically rational numbers

14:17

not both zero one of them could be zero

14:21

a could be zero but then B cannot be 0

14:24

or B could be 0 in which case a could

14:27

not be 0 with the following convention

14:30

that we agree that a certain proportion

14:33

is equal to another proportion in a

14:35

certain situation we say that a to B

14:37

equals C to D precisely when ad minus BC

14:43

equals zero hopefully that looks a

14:46

little bit familiar ok so this is the

14:50

fundamental notion of equality between

14:52

proportions

14:53

a three proportion is something similar

14:57

but we are comparing three things not

15:01

two things

15:02

so it's an expression a 1 to a 2 to a 3

15:06

where now a 1 a 2 and a 3 are numbers

15:10

not all 0 with the corresponding

15:14

convention that 1/3 proportion say a 1 a

15:17

2 a 3 equals a 2nd 3 proportion B 1 B 2

15:21

2 B 3

15:22

precisely when a1 b2 minus a2 b1 equals

15:29

0 and a2 b3 minus a3 b2 equals 0 and a1

15:36

b3 minus a3 b1 equals 0 so the same

15:42

kinds of relations occurring in a2

15:45

proportion are occurring here but three

15:48

different ways corresponding to pairing

15:50

the ones and the twos the twos and the

15:53

threes and the ones and the threes no

16:00

proportions are kind of close to my

16:02

heart because I wrote a book called

16:04

divine proportions k this is my book on

16:07

rational trigonometry which I hope

16:09

you've all heard of and I hope that

16:11

maybe some of you have read or if you

16:12

haven't that you will read it at some

16:14

point because then you'll learn the very

16:16

important new geometrical understanding

16:18

of rational trigonometry and the the

16:22

notion of proportion encoded here plays

16:24

a kind of a central role in setting up

16:26

this entire new theory of trigonometry

16:29

ok so it's a quite a useful thing even

16:33

though it goes back to antiquity we'll

16:36

see that it's very useful for us so the

16:41

proportions satisfy some nice little

16:43

propositions the first one captures the

16:46

idea of an equivalence relation okay

16:48

that that proportions really provide us

16:51

with an example of the equivalence

16:52

relation that amounts to three sort of

16:55

simple properties that proportions

16:57

satisfy the first one is very simple

16:59

that a to b equals a to b now you may

17:04

think well why do we have to check that

17:06

house that a proposition is that obvious

17:08

well kind of but maybe not entirely

17:12

because remember we defined equality in

17:15

a very precise way we say that this

17:17

proportion is equal to this proportion

17:19

when ad minus BC equals zero so there's

17:22

something to check before we can state

17:24

that two proportions are equal in this

17:26

case you have to check that this number

17:29

times this number minus this number of

17:31

times this number is equal to zero okay

17:33

and obviously it is

17:35

but that's still something that you have

17:38

to check if you had some more convoluted

17:40

notion of equality then maybe this

17:43

property wouldn't actually be satisfied

17:45

and you might wonder why you're actually

17:48

considering that so but anyway that's an

17:51

important problem here's another kind of

17:53

obvious property that a to B equals C to

17:56

D is really the same as C to D equals a

17:59

to B so in other words if these two

18:01

proportions are equal then the Easter

18:03

proportions are also equal and the last

18:06

one transitivity that is a to b equals C

18:09

to D and C to D equals E to F then we

18:15

can conclude that a to B equals E to F

18:20

you might like to prove this for

18:24

yourself

18:26

okay the corresponding facts also hold

18:28

for three proportions so there's a

18:30

corresponding set of statements for

18:33

three proportions and here's another

18:35

useful way of thinking about this

18:38

equality of proportions that a to B

18:41

equals C to D precisely when C is lambda

18:46

a and D is lambda B for some nonzero

18:52

number lambda so in other words this

18:55

proportions obtained from this one by

18:57

scaling up both of the numbers by the

19:00

same nonzero amount because it's another

19:04

way of thinking about what equality of

19:06

proportions means that it's invariant

19:09

under nonzero scaling so that's great so

19:15

we've learned a little bit about basic a

19:17

prior geometry and proportions

19:21

[Music]

Attachments