chapter 10- vector and geometry space
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The three coordinate axes determine the three
coordinate planes illustrated in the fi"ure &
The xy-plane is the plane that
contains the x- and y-axes'
the y#-plane contains the y-
and #-axes' and x#-plane
contains the x- and #-axes.These three coordinate
planes di%ide space into ei"ht
parts, called octant, in the
fore"round, is determined by
the positi%e axes.
Vectors in the plane
The term vectoris used by scientists to indicate a quantity
(such as displacement or %elocity or force) that has both
ma"nitude and direction. %ector is often represented by
an arrow or a directed line se"ment. The len"th of the
arrow represents the ma"nitude of the %ector and the arrow
points in the direction of the %ector. We denote a %ector by
printin" a letter in boldface ( v) or puttin" an arrow
abo%e the letter (
) .
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For instance , suppose a particle mo%es alon" a line
se"ment from point to point . The correspondin"
displacement vector v, shown in the fi"ure below , has
initial point ( the tail) and terminal point ( the tip) andwe indicate this by writin" % ()= .
*otice that the %ector u +,= has the same len"th and thesame direction as e%en thou"h it is in a different position.
We say that uand vare equivalent( or equal) and we
write u%. Thezero vector, denoted by ! , has len"th 0. t is
only %ector with no specific direction.
Combining Vectors
/uppose a particle mo%es from to , so its displacement
%ector is ( () ). Then the particle chan"es direction and
mo%es from to +, with displacement %ector ()+) as in
the fi"ure&
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n the followin" fi"ure
We start with the same %ectors u and % as in the pre%ious
one and draw another copy of v with the same initial
point as u. completin" the parallelo"ram , we see that u
+ v v + u. This also "i%es another way to construct the
sum& if we place u and % so they at the same point , then
u 0% lies alon" the dia"onal of the parallelo"ram with u
and v as sides . ( This is called the!arallelogram "a#)
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$%ample
raw the sum of the %ectors a and b shown in the
fi"ure &
Solution
First we translate b and place its tail at the tip of a, bein"
careful to draw a copy of b that has the same len"th and
direction. Then we draw the %ector ( a 0b) ( see the
fi"ure)
/tartin" the initial point of a and endin" at the terminalpoint of the copy of b.
lternati%ely , we could place b so it starts where a starts
and construct ( a 0b) by the parallelo"ram law as in the
fi"ure &
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Scalar &ultiplication
t is possible to multiply a %ector by a real number +. ( we
call the real number a scalar to distin"uish it from a %ector). For instance , we want 1% to be the same %ector as ( % 0
%), which has the same direction as % but is twice as lon".
n "eneral , we multiply a %ector by a scalar as follows&
efinition of scalar multiplication
f + is a scalar and vis a %ector, then the scalar multiple
cvis the %ector whose len"th is c times the len"th of vand
whose direction is the same as % if c2! and is opposite to %
if c3 ! . if c! or %! , then cv0
The definition is illustrated in the followin" fi"ure&
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we see that real numbers work like scalin" factors here'that is why we call them scalars. *otice that two non#ero
%ectors are parallel if they are scalar multiplies of one
another.
n particular, the %ector 4% (-5)% has the same len"th as %
but points in the opposite direction. We call it the negative
of %.
!osition vector
/ince the location of the initial point is irrele%ant, we
typically draw %ectors with their initial point located at the
ori"in. /uch a %ector is called a position %ector. For the
position %ector a with initial point at the ori"in and
terminal point at the point (a5,a1) we denote the %ector by
1 2,a 6( a a= = ( see the fi"ure)
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7a"nitude of position %ector a is &2 2
1 2a a a= +
f 0a = then 0a= this is called a #ero %ector. ny %ector
with ma"nitude of 5 i.e. 1u = is called a unit %ector. Wewill occasionally find it con%enient to write %ectors in
terms of some standard %ectors, we define the standard
basis %ectors i and 8 by 1, 0 , , 0,1i and 8= = and thiscan be extended to three dimensional case. *otice that
1i 8= = ( see the fi"ure)
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Difference of t#o vectorsy the difference ' u(v)of two %ectors we mean
u4 v u0 (-v) , so we can construct (u-%) by first drawin"
the ne"ati%e of %,-% , and then addin" it to u by the
parallelo"ram law in the followin" fi"ure&
lternati%ely, since % 0 ( u 4 % ) u, the %ector u 4 %,
when added to % "i%es u so we could construct u-% as infi"ure below by means of trian"le law
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$%ample
f a and b are the %ectors shown in the fi"ure below
,draw a(*b
SolutionWe first draw the %ector ( - 1 b) pointin" in the direction
opposite to b and twice as lon". We place it with its tail
at the tip of a and then use the trian"le law to draw a0(-
1b) as in the fi"ure below&
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Vectors in the space
/e%eral ideas can be extended from 1(91) to : space
(9:). ;oint in 9:is defined by (a,b,c), while x,y,# is the
ri"ht-handed coordinate system. (see the fi"ure )
7a"nitude of2 2 2
1 2 3 1 2 3, ,a a a a is a a a a= = + +
ector addition&
1 2 3 1 2 3
1 1 2 2 3 3, ,
a b a a a b b b
a b a b a b
+ = + + + + +
= + + +
/tandard basis %ectors &
1, 0, 0 , 0,1, 0 , 0, 0,1i 8 and k = = =ny %ector 1 2 3 1 2 3, ,a a a a a i a 8 a k = = + +Findin" the equation of a sphere of radius r centred at
(a,b,c) & the sphere consists of all points (x,y,#) whose
distance from (a,b,c) is r &
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2 2 2
2 2 2 2
( ) ( ) ( )
( ) ( ) ( )
x a y b # c r
x a y b # c r
+ + =
+ + =
,he Dot !roduct
/o far we ha%e added two %ectors and multiplied a %ector
by a scalar. The question arises ' s it possible to multiply
two %ectors so that their product is a useful quantity< 6ne
such product is the dot product, whose definition follows
(5)efinition
f { } 3,,,, 21321 bbbbandaaaa == , then the dot product of a and b
is the number a .b"i%en by&
a . b a5b50 a1b10 a:b:
Thus to find the dot product of a and b we multiply
correspondin" components and add. The result is not a
%ector. t is a real number, that is , a scalar, for this reason ,the dot product is sometimes called the scalar product ( or
inner product). lthou"h definition (5) is "i%en for three-
dimensional %ectors , the dot product of two-dimensional
%ectors is defined in a similar fashion&22112121 ,., bababbaa +=
=xample
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7)1)(3()2(2)0(12.32
6)2
1(4)2(7)6)(1(
2
1,2,6.4,7,1
2)1)(4()3(21,3.4,2
=++=+
=++=
=+=
k8k8i
The dot product obeys many of the laws that hold for
ordinary products of real numbers. These are stated in
the followin" theorem.
(1) ;roperties of the ot ;roduct
f a, b, and c are %ectors in :and c is a scalar, then&
0.05
).().(4
..).(3
..2
.1 2
==
+=+==
a
cbabca
cabacba
abba
aaa
These properties are easily pro%ed usin" definition 5.
For instance , here are proofs of properties 5 and :&
caba
cacacabababa
cabacabacaba
cbacbacba
cbcbcbaaacba
aaaaaa
..
)()(
)()()(
,,.,,).(3
.1
332211332211
333322221111
333222111
332211321
22
3
2
2
2
1
+=
+++++=
+++++=
+++++=
+++=+
=++=
The dot product a .b can be "i%en a "eometric
interpretation in terms of the an"le > between a and b,
which is defined to be the an"le between the representation
of a and b that start at the ori"in, where ! ? > ? @ in other
words > is the an"le between the line se"ment 6( and6) in the fi"ure below &
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'-) ,heorem
f > is the an"le between the %ectors a and b, thencos. baba =
;roof
f we apply the law of cosines to trian"le 6 in the
fi"ure , we "et(A) cos2222
6)6(6)6(() +=
*ote that the law of cosine still applies in the limitin" cases
when > ! or @ or ( a! or b!) . but B6BBaB, B6BBbB
, and BB Ba-bB , so equation (A) becomes
(C) Ba-bB1 BaB1 0 BbB1-1BaBBbBcos>
$sin" properties of dot product we can rewrite the left side
of this equation as follows&
22
2
.2
....
)).((
bbaa
bbabbaaa
bababa
+=
+=
=
Therefore, equation (C) "i%es
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or
cos.
cos2.2
cos2.2 2222
baba
baba
bababbaa
=
=
+=+
=xample
f the %ectors a and b ha%e the len"th A and D, and the
an"le between them is @E:, find a . b.
/olution
$sin" theorem (:) , we ha%e
122
1.6.4)
3cos(. ===
baba
The formula in theorem : also enables us to find the
an"le between two %ectors.
+orollary & f > is an an"le between the non#ero
%ectors a and b , then
ba
ba+os
.=
$%ample
Find the an"le between %ectors 1,2,2 =a and
2,3,5=b .
/olution
3)1(22 222 =++=a and
382)3(5 222 =++=b
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and since a . b 1(C)01(-:)0(-5)11
We ha%e from the definition of the dot product&
. 2cos
(3)( 38)
a b
a b= = , so the an"le between a and b is
( )1 02
cos 1.46, 84(3)( 38)
or
=xample
(i)etermine the an"le between a and b if it is known
that 3, 4, 1 , 0,5, 2a and b= =(ii) +heck the ortho"onality of
1 12
2 4u i 8 and % i 8= = +r r
/olution(i)
. 3, 4, 1 0, 5, 2 3(0) (5)( 4) ( 1)(2) 22
9 16 1 26
0 25 4 29
a b
a
b
= = + + =
= + + =
= + + =
r
r
the an"le is then &
. 22cos 0.8011927
26 29
a b
a b
= = = r r that means >1.C
radians 5A:.1A!
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(ii)
1 1 1 5. 2, 1, 0 , , 0 12 4 4 4
u %= = = r r
( not ortho"onal)
55,
4u %= =r r
notice that1
4% u=r r
they
are parallel.
lso & 05 5
. 5. cos 1 1804 4
u % u % = = = = =r r r r
=xample
force is "i%en by the %ector F:i0A80Ck and mo%es a
particle from the point ;(1,5,!) to the point (A,D,1).
Find the work done.
/olution
The displacement %ector is
(2,5,2), ;F= = , so that work done is. 3, 4, 5 . 2,5, 2
6 20 10 36
W F ,= =
= + + =
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Components and !roections
For any two non#ero position %ectors a and b, let thean"le between the %ectors be >. f we drop a
perpendicular line se"ment from the terminal point of a
to the line containin" the %ector b, then from elementary
tri"onometry, the base of the trian"le ( in case where
(!3>3@E1) has the len"th "i%en by cosa ( see the
fi"ure)
6n the other hand, notice that if )2
(
, the len"th of
the base is "i%en by cosa ( see the fi"ure)
n either case, we refer to cosa as the component of a
alon" b, denoted +ompba . we can write this expression
as &
b
baa+omp
orbab
bab
b
baaa+omp
b
b
.
.1
cos1
coscos
=
==
==
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*otice that +ompba is a scalar and that we di%ide the
dot product by b and not by a . one way to keep this
strai"ht is to reco"ni#e that the components in fi"uresabo%e depend on how lon" a is but not on how lon" b is.
We can %iew the last formula as the dot product of the
%ector a and a unit %ector in the direction of b, "i%en by
b
b.
6nce a"ain, consider the case where the %ector a
represents a force. 9ather than the component of a alon"b, we are often interested in findin" a force %ector
parallel to b ha%in" the same component alon" b as a.
we call this %ector the pro8ection of a onto b, denoted by
;ro8ba , as indicated in the fi"ures below. /ince the
pro8ection has ma"nitude acompb and points in the
direction of b, for !3>3@E1 and opposite b , for
@E13>3@, we ha%e that
bb
baapro8
b
b
b
ba
b
bacompapro8
b
bb
2
.
.)(
=
==
Where bb
represents a unit %ector in the direction of b.
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=xample
For 5,1,3,2 == banda , find the component of a alon"
b and the pro8ection of a onto b.
/olution
We ha%e 2613
251
152
5,1
5,1.3,2.=
++
=
==
b
baacompb
/imilarly we ha%e
2
5,
2
15,1
2
15,1
26
13
26
5,1
26
13.
===
=
=
b
b
b
baapro8b
,he cross product
n this section , we define a second type of product of
%ectors, the cross product or %ector product. While the dot
product of two %ectors is a scalar, the cross product of two
%ectors is another %ector. The cross product has many
applications, from physics and en"ineerin" mechanics to
space tra%el.
/ome important definitions
efinition
The determinant of a 1 x 1 matrix of real numbers is
defined by
1 2
1 2 2 11 2
2 2x matrix
a a
a b a bb b = 14 2 43
=xample ' e%aluate the determinant1 2
3 4
From the abo%e definition we ha%e&
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2)3)(2()4)(1(43
21==
efinition
The determinant of a : x : matrix of real numbers isdefined as a combination of three 1 x 1 determinants, as
follows&
1 2 3
2 3 1 3 1 2
1 2 3 1 2 3
2 3 1 3 1 2
1 2 3
3 3x matrix
a a ab b b b b b
b b b a a ac c c c c c
c c c
= + +
1 4 2 4 3
this equation is referred to as an expansion of the
determinant alon" the first row. *otice that the multipliers
of each of the 1 x 1 determinants are the entries of the first
row of the : x : matrix. =ach 1 x 1 determinant is the
determinant we "et by eliminatin" the row and column in
which the correspondin" multiplier lies.
=xample
=%aluate the determinant
1 2 4
3 3 1
3 2 5
/olution
=xpandin" alon" the first row, we ha%e
[ ] [ ]
[ ]
1 2 4
3 1 3 1 3 33 3 1 (1) (2) (4)2 5 3 5 3 2
3 2 5
(1) (3)(5) (1)( 2) (2) ( 3)(5) (1)(3)
(4) ( 3)( 2) (3)(3) 41
= +
+ =
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we use the determinant notation as a con%enient de%ice for
definin" the cross product, as follows&
efinitionFor two %ectors 1 2 3 1 2 3, , , ,a a a a and b b b b= = in :,we define the cross product ( or %ector product) of a and b
to be &
2 3 1 3 1 2
1 2 3
2 3 2 3 1 2
1 2 3
i 8 ka a a a a a
axb a a a i 8 k b b b b b b
b b b
= = +
notice that a x b is also a %ector in :. To compute a x b ,
you must write the component of a in the second row and
the component of b in the third row' the order is important.
=xample
+ompute 1, 2, 3 4, 5, 6x
2 3 1 3 1 21, 2,3 4,5, 6 1 2 3
5 6 4 6 4 54 5 6
3 6 3 3, 6, 3
i 8 kx i 8 k
i 8 k
= = +
= + =
note that the cross product is defined only for %ectors in
:, there is no correspondin" operation for %ector in 1.
TheoremFor any %ector 3 , 0, 0 0a - axa and ax = =We pro%e the first one &
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2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
1 2 3
2 3 3 2 2 2 3 2 1 2 2 1( ) ( ) ( ) 0
i 8 ka a a a a a
axa a a a i 8 k a a a a a a
a a a
a a a a i a a a a 8 a a a a k
= = +
= + =
Theorem
For any %ectors a and b in :, a x b is ortho"onal to both a
and b.
;roof
9ecall that two %ectors are ortho"onal if and only if their
dot product is #ero.
[ ] [ ] [ ]
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
1 2 3 3 2 2 1 3 3 1 3 1 2 2 1
1 2 3 1 3 2 1 2 3 2 3 1 1 3 2 2 3 1
.( ) , , .
0
a a a a a aa axb a a a i 8 k
b b b b b b
a a a a a aa a a
b b b b b ba a b a b a a b a b a a b a b
a a b a a b a a b a a b a a b a a b
= +
= +
= +
= + +
=/o that a and (a x b ) are ortho"onal.
*otice that since a x b is ortho"onal to both a and b, it is
also ortho"onal to e%ery %ector lyin" in the plane
containin" a and b. ut, "i%en a plane, out of which side ofthe plane does a x b point< We can "et an idea by
computin" some simple cross products.
*otice that
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0 0 1 0 1 01 0 0
1 0 0 0 0 10 1 0
i 8 k
ix8 i 8 k k = = + =
likewise 8 x k i
/ight(hand rule
There are illustrations of the ri"ht-hand rule& f you ali"n
the fin"ers of your ri"ht hand alon" the %ector a and bend
your fin"ers around in the direction of rotation from a
toward b ( throu"h an an"le of less than 5G!!), your thumb
will point in the direction ofa x b ( see the fi"ure )
*ow , followin" the ri"ht-hand rule , b x a will point in the
direction opposite a x b ( see the fi"ure )
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in particular, notice that
0 1 01 0 0
i 8 k
8xi k= =
efinition & Two non#ero %ectors 3,a b - parallel if andonly if a x b!
9ecall that a and b are parallel if and only if the an"le >
between them is either ! or @ . in either case , sin> ! and
so from one of the pre%ious theorems we ha%e that &
sin (0) 0axb a b a b= = =The result then follows from the fact that only %ector with
#ero ma"nitude is the #ero %ector.
The same theorem pro%ides us with the followin"
interestin" "eometric interpretation of the cross product.
For any two non#ero %ectors a and b, as lon" as a and b
are not parallel, they form two ad8acent sides of the
parallelo"ram , as seen in the fi"ure below
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notice that the area of the parallelo"ram is "i%en by the
product of the base and the altitude, we ha%e
rea ( base ) ( altitude )
sina b axb=
That is, the ma"nitude of the cross product of two %ectors"i%es the area of the parallelo"ram with two ad8acent sides
formed by the %ectors.
=xample
Find the area of the parallelo"ram with two ad8acent sides
formed by %ectors 1, 2, 3 , 4, 5, 6a and b= =/olution
First notice that&
2 3 1 3 1 21 2 3 3, 6, 3
5 6 4 6 4 54 5 6
i 8 k
axb i 8 k = = + =
from the formula for the area of the parallelo"ram we ha%ethat& 3, 6, 3 54 7.348(rea axb= = =
From the same theorem we can also find the distance from
a point to a line in 9:, as follows. Het d represent the
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For any three noncoplanar %ectors a,b, and c ( three
%ectors that do not lie in a sin"le plane), consider the
parallelepiped formed usin" %ectors as three ad8acent
ed"es ( see fi"ure )
9ecall that the %olume of such solid is "i%en by&
olume ( rea of base)(altitude)
Further , since two ad8acent sides of the base are formed
by the %ectors a and b, we know that the area of the base is
"i%en by axb . 9eferrin" to the fi"ure abo%e , notice that
the altitude is "i%en by&
.( )axb
c axbcomp c
axb= , the %olume of the parallelepiped is
then&.( )
.( )c axb
-olume axb c axbaxb
= =
the scalar c.(a x b) is called the scalar triple product of the%ectors a ,b , and c. it is possible to e%aluate the scalar
triple product by computin" a sin"le determinant. *ote that
for 1 2 3 1 2 3 1 2 3, , , , , , , ,a a a a b b b b and c c c c= = = ,we ha%e &
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1 2 3
1 2 3
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
1 2 3
1 2 3
1 2 3
.( ) .
, ,
i 8 k
c axb c a a a
b b b
a a a a a ac c c i 8 k
b b b b b b
a a a a a ac c c
b b b b b b
c c c
a a a
b b b
=
= +
= +
=
=xample
Find the %olume of the parallelepiped with three ad8acent
ed"es formed by three %ectors1, 2,3 , 4,5, 6 , 7,8, 0a b and c= = =
/olution
First , note that.( )-olume c axb= , we ha%e that
7 8 02 3 1 3 1 2
.( ) 1 2 3 7 8 05 6 4 6 4 5
4 5 6
( 3)(7) ( 6)(8) 21 48 27
c axb = = +
= = + =
so, the %olume of the parallelepiped is 1I
!roperties of cross product
f candba, are %ectors and e is a scalar, then&
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1. ( )
2. ( ) ( ) ( )
3. ( ) ( )
4. ( ) ( )
5. .( ) ( ). ( )
6. ( ) (
a xb bxa anticommuta%ity
ea xb e axb ax eb
a x b c axb axc distributi%e law
a b xc axc bxc distributi%e law
a bxc axb c scalar triple product
a x bxc a
=
= =
+ = ++ = +
=
=
r r r r r r
r r r r r r r
r r r r r r r
r r r r r r
r r r. ) ( . ) ( )c b a b c %ector triple product
r r r r r r
;roof (5)
We ha%e 1 2 3 1 2 3, , , , ,a a a a and b b b b= this can bewritten in form
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
1 2 3
2 3 1 3 1 2
2 3 1 3 1 2
( )
i 8 ka a a a a a
axb a a a i 8 k b b b b b b
b b b
b b b b b bi 8 k bxa
a a a a a a
= = +
= + =
since swappin" two rows in a 1x1 matrix ( or in a :x:
matrix, for this matter) chan"es the si"n of its determinant.
;roof(:)
For 1 2 3, ,c c c c= , we ha%e
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1 1 2 2 3 3, ,b c b c b c b c+ = + + + , and so
1 2 3
1 1 2 2 3 3
( )
i 8 k
ax b c a a ab c b c b c
+ =+ + +
lookin" only at the i component of this, we ha%e
2 3
2 3 3 3 2 2
2 2 3 3
2 3 3 2 2 3 3 2
2 3 2 3
2 3 2 3
( ) ( )
( ) ( )
a aa b c a b c
b c b c
a b a b a c a c
a a a a
b b c c
= + + +
= +
= +
which is also the i component of a x b 0 a x c. similarly it
is possible to show that the 8 and k components also match.
"ines and planes in space*ormally , we specify a line in the xy-plane by selectin"
any two points on the line or a sin"le point on the line and
its direction, as indicated by the slope of the line. n three
dimensions, specifyin" two points on a line will still
determine the line. n alternati%e is to specify a sin"le
point on the line and its direction. n three dimensions,
direction should make you think about %ectors ri"ht away.HetJs look for the line that passes throu"h the point
;5(x5,y5,#5) and that is parallel to the position %ector
1 2 3, ,a a a a= ( see fi"ure).
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For any other point ;(x,y,#) on the line, obser%e that the
%ector 1; ;will be parallel to a. Further , two %ectors are
parallel if and only if one is a scalar multiple of the other,
so that& 1; ; ta= for some scalar t. The line then
coincides of all points ;(x,y,#) for which ( 1; ; ta= ) holds.
/ince1 1 1 1
, ,; ; x x y y # #= , we ha%e that&
1 1 1 1 2 3, , , ,x x y y # # ta t a a a = = , finally , since two%ectors are equal if and only if all of their components are
equal, we ha%e&
1 1 2 2 1 3, ,x x ta y y ta and # # ta = = =the last equation is called parametric equation for the line ,
where t is the parameter. s in two dimensional case , a
line in space can be represented by many different sets ofparametric equations. ;ro%ided none of a5,a1, and a:are
#ero., we can sol%e for the parameter in each of the three
equations, to obtain&
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1 1 1
1 2 3
x x y y # #
a a a
= =
we refer to the last equality as symmetric equations of the
line.
=xample
Find an equation of the line throu"h the point ( 5,C,1) and
parallel to the %ector 4,3,7 . lso, determine where the
line intersects the y#-plane.
/olution
From the pre%ious equations we know that the parametric
equations for the line are
1 4 , 5 3 , 2 7x t y t and # t = = =The symmetric equations of the line are &
1 5 2
4 3 7
x y # = =
The followin" fi"ure representin" the case&
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the line intersects the y#-plane where x!. settin" x!
yields that17 1
,4 4
y and #= =
alternati%ely, we could sol%e x-5At for t ( a"ain where
x!) and substitute this into the parametric equations for y
and # , so the line intersects the y#-plane at the point
( ! , 5IEA, 5EA ).
=xample
Find an equation of the line passin" throu"h the points
;(5,1,-5) and (C,-:,A).
/olution
First, a %ector that is parallel to the line is5,5,4))1(4,23,15( ==;F
pickin" either point will "i%e us equations for the line. Kere
we use ;, so that parametric equations for the line are&t#andtytx 51,52,41 =+== ,similarly , symmetric equations
of the line are
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1 2 1
4 5 5
x y # += =
the followin" fi"ure shows the "raph of the line
/ince we ha%e specified a line by choosin" a point on the
line and a %ector with the same direction , we can state the
followin" definition&
efinition
Het H5 and H1 be two lines in 9:, with parallel %ectors a
and b, respecti%ely, and let > be the an"le between a and b.
5-The lines H5and H1are parallel whene%er a and b are
parallel.
1-f H5and H1intersect, then
(i)The an"le between H5and H1is > and
(ii)The lines H5and H1are ortho"onal whene%er a and b
are ortho"onal.
n two dimensions, two lines are either parallel or they are
intersect. This is not true in three dimensions.
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$%ample& /how that the lines &t#andtytxl 25,21,2:1 === and
s#andsysxl 31,2,1:2 ===are not parallel, yet do notintersect.
/olution
We used different letters ( t and s )for the two lines as the
parameters . sol%in" the first parametric equation of each
line for the parameter in terms of x , we "etxt =2 , and 1= xs ,
respecti%ely , this means that the parameter representssomethin" different in each line' so we must use different
letters. *otice from the "raph below ,
that the lines are most certainly not parallel, but it is
unclear whether or not they intersect. Lou can read fromthe parametric equations that a %ector parallel to H5is
2,2,11 =a while the %ector parallel to H1is 3,1,12 =a .
/ince a5is not a scalar multiple of a1, the %ectors are not
parallel and so, the lines H5and H1 are not parallel'. The
lines intersect if there is a choice of the parameters s and t
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that produces the same point, that is, that produces the
same %alue for all x, y, and #. settin" the x-%alues equal, we
"etst += 12
, so thatts = 1. settin" that y-%alues equal andsettin" ts = 1 , we "et
tt
st
+===+
1)1(2
221
/ol%in" this for t yields 0=t , which further implies that 1=s
. settin" the #-components equal "i%es1325 +=+ st , but this equation is not satisfied when 0=t and
1=s, so, H5and H1are not parallel, yet do not intersect.
efinition
*onparallel, nonintersectin" lines are called skew lines.
*ote that itJs easy to %isuali#e skew lines. raw two planes
that are parallel and draw a line in each plane ( so that it
lies completely in the plane). s lon" as two lines are not
parallel, these are skew lines ( see the fi"ure below).
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!lanes in /-
6bser%e the followin" fi"ure &
*ote that the y#-plane is a set of points in space such that
e%ery %ector connectin" two points in the set is ortho"onal
to i. Kowe%er, e%ery plane parallel to the y#-plane satisfies
this criterion . n order to select the one that corresponds
to the y#-plane, you need to specify a point throu"h which it
passes ( any one will do).
n "eneral, a plane in space is determined by specifyin" a
%ector 1 2 3, ,a a a a= that is normal to the plane ( i.e.,ortho"onal to e%ery %ector lyin" in the plane) and a point
;5(x5,y5,#5) lyin" in the plane ( see the fi"ure)
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n order to find an equation of the plane, let ;(x,y,#)
represent any point in the plane. Then, since ; and ;5are
both points in the plane , the %ector
1 1 1 1, ,;; x x y y # #= lies in the plane and so, must beortho"onal to a. y theorem that we used earlier we ha%e
1 1 2 3 1 1 1
1 1 2 1 3 1
0 . , , . , ,
0 ( ) ( ) ( )
a ;; a a a x x y y # # or
a x x a y y a # #
= =
= + +
the last equation is equation for the plane passin" throu"h
the point ( x5,y5,#5) with normal %ector 1 2 3, ,a a a .
$%ample
Find an equation of the plane containin" the point (5,1,:)
with normal %ector (A,C,D) and sketch the plane.
/olution
From the equation of the plane we ha%e
!A(x-5)0C(y-1)0D(#-:) , which is the equation of the
plane. To draw the plane, we locate three points lyin" in
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the plane, n this case , the simplest way to do this is to
look at the intersections of the plane with each of the
coordinate axes. . when y#!, we "et that &
!A(x-5)0C(!-1)0D(!-:)Ax-A-5!-5G, so that Ax:1 andxG . the intersection of the plane with the x-axis is the
point ( G,!,!) , similarly we can find the intersections of the
plane with y- and #-axes& (!,:1EC , !) and ( !,!,5DE:)
respecti%ely. $sin" these three points , we can draw the
plane seen in fi"ure below&
we start by drawin" the trian"le with %ertices at the three
points' the plane we want is the one containin" this
trian"le. *otice that since the plane intersects all three of
the coordinate axes, the portion of the plane in the firstoctant is the indicated trian"le.
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1inding the equation of a plane given three points
*ot that we can expand the equation of the plane
1 1 2 1 3 10 ( ) ( ) ( )a x x a y y a # # = + + to the followin" form&1 2 3 1 1 2 2 3 3
tan
0 ( )
cons t
a x a y a # a x a x a x= + + + 1 4 44 2 4 4 43
we refer to the last equation as a linear equation in the
three %ariables x, y,and #. n particular, this says that e%ery
linear equation of the form
!ax0by0c#0d is the equation of a plane with normal
%ector , ,a b c , where a,b,c,and d are constants.We noticed earlier that three points determine a plane, but
how can we find an equation of a plane "i%en only three
points< We need first to find a normal %ector then proceed
easily as in the example
$%ample
Find the plane containin" three points ;(5,1,1), (1,-5,A)
and 9(:,C,-1).
/olution
First, we will need to find a %ector normal to the plane.
*otice that two %ectors lyin" in the plane are
1, 3, 2 , 1, 6, 6;F and F9= = , consequently, a
%ector ortho"onal to both of ,;F and F9 is the cross
product
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1 3 2 6,8,9
1 6 6
i 8 k
;x9= =
uuur uuur
since ,; and 9 are not parallel, ;FxF9 must be
ortho"onal to the plane, as well an equation for the plane
is then 0 6( 1) 8( 2) 9( 2)x y #= + + , in the followin"fi"ure we can see the trian"le with %ertices at the three
points. The plane in question is the one containin" the
indicated trian"le.
,he equation of a plane given a point and a parallel
plane
n three dimensions, two planes are either parallel or they
intersect in a strai"ht line.. suppose that two planes ha%in"
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normal %ectors a and b , respecti%ely, intersect. Then the
an"le between the planes is the same as the an"le between
a and b ( see the fi"ure)
With this in mind, we say that the two planes are parallelwhene%er their normal %ectors are parallel and the planes
are ortho"onal whene%er their normal %ectors are
ortho"onal.
$%ample
Find an equation for the plane throu"h the point (5,A,-C)
and parallel to the plane defined by 1x-Cy0I#51
/olution
First, notice that a normal %ector to the "i%en plane is
2, 5,7 . /ince the two planes are to be parallel, this%ector is also normal to new plane, then we can write down
the equation of the plane as follows&
!1(x-5)-C(y-A)0I(#0C)
1inding intersection of t#o planes
The intersection of two nonparallel planes should be a line
$%ample
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Find the intersection of the planes 32 =++ #yx and534 =+ #yx .
/olution & sol%in" both equations for x , we "et#yx = 23 and #yx 345 +=
settin" these expressions for x equal "i%es us#y#y 34523 +=
sol%in" for # "i%es us262 += y# or 13 += y#
returnin" to either plane equations , we can sol%e for x
( also in terms of y) , we ha%e18)13(223223 +=+== yyy#yx
Takin" y as the parameter ( i.e., lettin" ty= ) , we obtain
parametric equations for the line of intersection&13,,18 +==+= t#andtytx
/ee the fi"ure below
Distance bet#een parallel planes
The distance from the plane ax0by0c#! to a point ;!
( x!,y!,#!) not on the plane is measures alon" a line
se"ment connectin" the point to the plane that is
ortho"onal to the plane ( see the fi"ure)
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To compute this distance, pick any point ;5( x5y5#5) lyin"
in the plane and let , ,a a b c= denote a %ector normal tothe plane. From the fi"ure notice that the distance from ;!
to the plane is simply 1 0acomp ;; , where&
1 0 0 1 0 1 0 1, ,;; x x y y # #=
from the rule of distance we ha%e that the distance is
1 0 1 0
0 1 0 1 0 1
2 2 2
0 0 0 1 1 1
2 2 2
0 0 0
2 2 2
.
, ,, , .
, ,
( ) ( ) ( )
( )
a
a
comp ; ; ; ; a
a b cx x y y # #
a b c
a x x b y y c # #
a b c
ax by c# ax by c#
a b c
ax by c# d
a b c
=
=
+ + =
+ ++ + + +
= + ++ +
=+ +
uuuur uuuur
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since (x5, y5,#5) lies in the plane and ax0by0c#-d, for
e%ery point (x,y,#) in the plane
$%ampleFind the distance between the parallel planes
1
2
: 2 3 6
: 4 6 2 8
; x y #
; x y #
+ = + =
/olution
First, obser%e that the planes are parallel, since their
normal %ectors 2, 3,1 , 4, 6, 2and are parallel.Further, since planes are parallel, the distance from the
plane ;5to e%ery point in the plane ;1is the same , so ,
pick any point in ;1, say )4,0,0( . The distance d from the
point )4,0,0( to the plane ;5is then "i%en by&
2 2 2
(2)(0) (3)(0) (1)(4) 6 2
142 3 1d
+ = =
+ +
Surface in spacen this section we take a first look at functions of two
%ariables and their "raphs, which are surfaces in three-
dimensional space.
2uadric surface
The "raph of a second-de"ree equation in three %ariables
x,y,and # is called quadric surface. The "raph of theequation &2 2 2 0ax by c# dxy ey# fx# "x hy 8# k + + + + + + + + + =
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n three-dimensional space ( where a,b,c,d,e,f,",h,8,and k
are all constants and at least one of a,b,c,d,e or f is
non#ero) is referred to as a quadric surface.
The most familiar quadric surface is the sphere&2222 )()()( rc#byax =++ , of radius r centred at the point),,( cba , to draw the sphere centred at )0,0,0( , first draw a
circle of radius r, centred at the ori"in in the planey# .
Then, to "i%e the surface its three-dimensional look, draw
circles of radius r centred at the ori"in, in both the planex#
and planexy , as in the fi"ure
*ote that due to the perspecti%e, these circles will look like
ellipses and will be only partially %isible ( the hidden parts
of the circles will be represented by dashed lines)
"enerali#ation of the sphere is the ellipsoid&2 2 2
2 2 2
( ) ( ) ( )1
x a y b # c
d e f
+ + =
notice that when def, the surface is a sphere.
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$%ample
Mraph the ellipsoid2 2 2
11 4 9
x y #
+ + =
/olution
first draw the traces in the three coordinate planes. n the
y#-plane, x ! , which "i%es us the ellipse&2 2
14 9
y #+ =
shown in the fi"ure below&
*ext, add to the last fi"ure the traces in the xy- and x#-
planes, these are&2 2 2 2
1, 11 4 1 9
x y x #and+ = + = , which are both ellipses
(see the fi"ure)
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To sketch the problem in the hand for instance we can sol%e
for # and plot the two functions&2 2
2 23 1 , 3 14 4
y y# x and # x= = , to obtain surface
S3etching a paraboloid
raw a "raph of the quadric surface
2 2x y #+ =To "et an idea of what the "raph looks like, first draw its
traces in the three coordinate planes. n the planey# , we
ha%e0=xand so
#y =2
( a parabola). n the planex#
, we ha%e0=y and so, #x =2 ( a parabola) . n the planexy , we ha%e0=# and so, 022 =+ yx ( a point- the ori"in). We sketch the
traces in the fi"ure below
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Finally since the trace in the xy-plane is 8ust a point, weconsider the traces in the planes )0( >= kk# . *otice that these
are the circles kyx =+ 22 , where for lar"er %alues of # ( i.e.,
lar"er %alues of k) , we "et circles of lar"er radius.. we
sketch the surface as in the fi"ure below
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/uch surface is called paraboloids and since the traces in
planes parallel to the xy-plane are circles, this is called a
circular paraboloid.Mraphin" utilities with three-dimensional capabilities
"enerally produce a "raph like the fi"ure below&
For 22 yx# += . *otice that the parabolic traces are %isible,
but not the circular across sections we draw in the second
fi"ure. The four peaks %isible in the last fi"ure are due tothe rectan"ular domain used to plot ( in this case
55 x and 55 y ).
This can be impro%ed by restrictin" #-%alues.
With 150 # , we can clearly see the circular cross section
in the plane 15=# in the followin" fi"ure
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We can plot the parametric surface to the same problem ,
we ha%e tx cos= , and ty sin= and 2s#= , with 50 s and20 t . The fi"ure below shows the circular cross
sections in the plane k#= for 0>k .
S3etching an elliptic cone
raw a "raph of quadric surface2
2 2
4
yx #+ =
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while this equation may look a lot like that of an ellipsoid,
there is a si"nificant difference ( look where the #1is), we
start by lookin" at the traces in the coordinate planes. For
theplaney#
, we ha%e0=xand so &2
2
4
x#= or 22 4#y = , so that #y 2= . That is, the trace is a
pair of lines & #y 2= and #y 2= ( see the fi"ure)
Hikewise, the trace in the planex# is a pair of lines& #x 2= .
The trace in the planexy is simply the ori"in(why)< Finally,
the traces in the planes )0( = kk# , parallel to the planexy ,
are the ellipses &2
2 2
4
yx k+ = . ddin" these to the drawin" "i%es us the
double-cone seen in the fi"ure below&
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/ince the traces in planes parallel to the xy-plane are
ellipses, we refer to this as an elliptic cone. 6ne way toplot this with a +/ is to "raph the two functions&
2 22 2
4 4
y y# x and # x= + = + .
in the followin" fi"ure
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We restrict the #-ran"e to 1010 # to show the elliptical
cross sections. *otice that this plot shows a "ap between
the two hal%es of the cone. lternati%ely, the parametric
plot shown in the followin" fi"ure
With 2 2cos , 2 sinx s t y s t= = and s# = , with 55 s
and 20 t , shows the full cone with its elliptical and
linear traces.
S3etching a hyperboloid of one sheet
raw a "raph of the quadric surface
2 22 14 2
x #y+ =
/olution
The traces in the coordinate plane are as follows&
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22
22
2 2
( 0) : 1 ( )2
( 0) : 1 ( )4
( 0) : 1 ( )4 2
#y# plane x y hyperbola
xxy plane # y ellipse
x #and x# plane y hyperbola
= =
= + =
= =
( see the fi"ure )
Further notice that the trace of the surface in each planek#= ( parallel to the planexy ) is also an ellipse&
2 22 1
4 2
x ky+ = +
Finally, obser%e that the lar"er k is, the lar"er the axes ofthe ellipses are. ddin" this information to the last fi"ure ,
we draw the surface seen in the followin" fi"ure
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We call this surface a hyperboloid of one sheet.
$sin" the +/ , we can "raph the two functions &2 2
2 22 1 2 14 4
x x# y and # y
= + = +
as in the fi"ure below&
(where we ha%e restricted the #-ran"e to1010 # , to show the elliptical cross sections.)
lternati%ely , the parametric plot seen in the fi"ure
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with 2 cos cosh , sin cosh , 2 sinhx s t y s t and # t= = = ,with 0 2 5 5s and t , shows the fullhyperboloid with its elliptical and hyperbolic trace
S3etching a hyperboloid of t#o sheets
raw a "raph of the quadric surface&2 2
2 14 2
x #y =
/olution
*otice that this is the same equation as in the last example,
except for the si"n of the termy . s we ha%e done before,
we first look at the traces in the three coordinate planes.The trace in the )0( = xplaney# is defined by&
22
12
#y = , since it is clearly impossible for two ne"ati%e
numbers to add up to somethin" positi%e, this is a
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contradiction and there is no trace in the planey# . That is ,
the surface does not intersect the planey# . The traces in the
other two coordinate planes are as follows&2
2
2 2
( 0) : 1 ( )4
( 0) : 1 ( )4 2
xxy plane # y hyperbola
x #x# plane y hyperbola
= =
= =
we show these traces in the followin" fi"ure '
Finally, notice that for kx= , we ha%e that2 2
2 12 4
# ky + =
so that the traces in the plane kx= are ellipses for 42 >k . t
is important to notice here that if 42
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sheets. ;uttin" this all to"ether , we ha%e the surface seen
in the fi"ure below&
we call this surface a hyperboloid of two sheets.
We can plot this on +/ by "raphin" the two functions
2 22 2
2 1 2 14 4
x x# y and # y
= = , as in
the fi"ure '
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where we ha%e restricted the #-ran"e to 1010 # , to show
the elliptical cross sections. This plot shows lar"e "aps
between the two hal%es of the hyperboloid.
The parametric plot with
2 cosh , sinh cos 2 sinh sin ,x s y s t and # s t= = =for 4 4 0 2s and t , produces the left half of
the hyperboloid with its elliptical and hyperbolic traces.The ri"ht half of the hyperboloid has parametric equations
2 cosh , sinh cos , 2 sinh sinx s y t and # s t= = = ,
with 4 4 0 2s and t . s shown in thefi"ure
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S3etching a hyperbolic paraboloid
/ketch the "raph of the quadric surface defined by theequation
2 22# y x=
/olution
We consider first the traces in planes parallel to each of the
coordinate planes&
;arallel to kxyk#planexy == 222:)( ( hyperbola , for )0( k .
;arallel to 22
2:)( kx#kyplanex# +== (parabola openin"down).
and parallel to 222:)( ky#kxplaney# == ( parabola openin"
up).
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first we start by drawin" the traces in the x#-planes as seen
in the fi"ure
/ince the trace in the xy-plane is the de"enerate hyperbola
)2( 22 xy =
( two lines & 2x y=m
), we instead draw thetrace in se%eral of the planes k#= . For )0( >k ), these are
hyperbolas openin" toward the positi%e and ne"ati%e y-
direction and for )0(
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We refer to this fi"ure as a hyperbolic paraboloid
wireframe "raph of 222 xy# = is shown in the fi"ure below
with )5555( yandx where we limited the #-ran"e to128 # .
*ote that only the parabolic cross sections are drawn, but
the "raph shows all the features of the fi"ure. ;lottin" this
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surface parametrically is fairly tedious because it requires
four different sets of equations) and does not impro%e the
"raph noticeably .