Approximate Length of Curves: Computing the Arclength of Functions, Study notes of Calculus

Notes from a university mathematics lecture on how to approximate the length of a curve using the arclength formula. The concept of interpreting the length as a limit of sums of lengths of simplest curves, and the use of right triangles to estimate the length of a subinterval. Examples of calculating the arclength of specific functions are included.

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Uploaded on 09/17/2009

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Jim Lambers
Math 2B
Fall Quarter 2004-05
Leture 25 Notes
These notes orrespond to Setion 9.1 in the text.
Ar Length
In this leture, we will learn how to use alulus to ompute the length of a urve that is desribed
by an equation of the form
y
=
f
(
x
), for some given funtion
f
(
x
). Just as we learned how to
ompute the area under suh a urve as the limit of a sum of areas of simpler regions (namely,
retangles), we an ompute the length of the urve by interpreting the length as a limit of a sum
of lengths of the simplest urves kno
wn, whih are line segments.
Suppose that we wish to ompute the length of the urve
y
=
f
(
x
) between
x
=
a
and
x
=
b
. We
an approximate this length by dividing the interval [
a; b
into subintervals of length
x
= (
b
a
)
=n
,
just as we did when we were trying to ompute the approximate area under
y
=
f
(
x
). Consider
any subinterval [
x
i
1
; x
i
℄. Then, if
x
is hosen to be suÆiently small, the length of the urve
y
=
f
(
x
) between
x
=
x
i
1
and
x
=
x
i
an be well approximated by the length of the line segment
between the points (
x
i
1
; f
(
x
i
1
)) and (
x
i
; f
(
x
i
)). This line segment is the hypotenuse of a right
triangle with legs of length
x
and
j
f
(
x
i
)
f
(
x
i
1
)
j
, and therefore the length
L
i
of the urve
y
=
f
(
x
) between
x
=
x
i
1
and
x
=
x
i
is approximately
L
i
p
x
2
+ (
f
(
x
i
)
f
(
x
i
1
))
2
=
x
s
1 +
f
(
x
i
)
f
(
x
i
1
)
x
2
:
(1)
It follows that the length
L
of the urve between
x
=
a
and
x
=
b
is approximated by
L
n
X
i
=1
L
i
=
n
X
i
=1
s
1 +
f
(
x
i
)
f
(
x
i
1
)
x
2
x
=
n
X
i
=1
s
1 +
f
(
x
i
)
f
(
x
i
1
)
x
i
x
i
1
2
x:
(2)
As
n
, the number of line segments, approahes
1
,
x
approahes zero, so the length of eah
subinterval [
x
i
1
; x
i
tends to zero. It follows from the denition of the derivative that
lim
x
!
0
f
(
x
i
)
f
(
x
i
1
)
x
i
x
i
1
= lim
x
!
0
f
(
x
i
1
+
x
)
f
(
x
i
1
)
x
=
f
0
(
x
i
1
) (3)
and therefore the sum onverges to the denite integral
L
= lim
n
!1
n
X
i
=1
L
i
=
Z
b
a
p
1 + [
f
0
(
x
)℄
2
dx:
(4)
1
pf3

Partial preview of the text

Download Approximate Length of Curves: Computing the Arclength of Functions and more Study notes Calculus in PDF only on Docsity!

Jim Lamb ers

Math 2B

Fall Quarter 2004-

Le ture 25 Notes

These notes orresp ond to Se tion 9.1 in the text.

Ar Length

In this le ture, we will learn how to use al ulus to ompute the length of a urve that is des rib ed

by an equation of the form y = f (x), for some given fun tion f (x). Just as we learned how to

ompute the area under su h a urve as the limit of a sum of areas of simpler regions (namely,

re tangles), we an ompute the length of the urve by interpreting the length as a limit of a sum

of lengths of the simplest urves known, whi h are line segments.

Supp ose that we wish to ompute the length of the urve y = f (x) b etween x = a and x = b. We

an approximate this length by dividing the interval [a; b℄ into subintervals of length x = (b a)=n,

just as we did when we were trying to ompute the approximate area under y = f (x). Consider

any subinterval [x i 1 ; x i ℄. Then, if x is hosen to b e suÆ iently small, the length of the urve

y = f (x) b etween x = x i 1

and x = x i

an b e well approximated by the length of the line segment

b etween the p oints (x i 1 ; f (x i 1 )) and (x i ; f (x i )). This line segment is the hyp otenuse of a right

triangle with legs of length x and jf (x i

) f (x i 1

)j, and therefore the length L i

of the urve

y = f (x) b etween x = x i 1

and x = x i

is approximately

L

i

p

x

  • (f (x i

) f (x i 1

= x

s

f (x i

) f (x i 1

x

It follows that the length L of the urve b etween x = a and x = b is approximated by

L 

n X

i=

L

i

n X

i=

s

f (x i

) f (x i 1

x

x =

n X

i=

s

f (x i

) f (x i 1

x i x i 1

x: (2)

As n, the numb er of line segments, approa hes 1 , x approa hes zero, so the length of ea h

subinterval [x i 1

; x i

℄ tends to zero. It follows from the de nition of the derivative that

lim

x! 0

f (x i

) f (x i 1

x i x i 1

= lim

x! 0

f (x i 1

  • x) f (x i 1

x

= f

(x i 1

and therefore the sum onverges to the de nite integral

L = lim

n!

n X

i=

L

i

Z

b

a

p

1 + [f

(x)℄

dx: (4)

The value of this integral is alled the ar length of the urve y = f (x) from x = a to x = b.

Similarly, if a urve is de ned by the equation x = f (y ) from y = to y = d, the ar length of the

urve is given by the de nite integral

Z

d p

1 + [f

(y )℄

dy : (5)

Example 1 Compute the ar length of the urve y = 2 x + 3, where 0  x  2.

Solution Sin e the urve is just a line segment, we an simply use the distan e formula to ompute

the ar length, sin e the ar length is the distan e b etween the endp oints of the segment. The

endp oints are (0; 3) and (2; 7), and therefore the ar length is

p

p

p

p

Using the ar length formula, we have y

= 2, and therefore the ar length is given by the integral

Z

p

dx =

Z

p

5 dx =

p

5 x

p

Example 2 Compute the ar length of the urve y = sin x from x = 0 to x = .

Solution Sin e y

= os x, the ar length is given by the integral

Z

p

1 + os

x dx: (8)

Unfortunately, this integral annot b e evaluated using the Fundamental Theorem of Cal ulus.

Using an approximation metho d su h as Simpson's Rule, the value of the integral is seen to b e

approximately 3.8202. 2

Example 3 Compute the ar length of the astroid des rib ed by the equation x

  • y

Solution We onsider only the p ortion of the astroid in the upp er quadrant x  0, y  0, whi h

has endp oints (0; 1) and (1; 0). In this quadrant, the astroid an b e des rib ed by the equation

y = (1 x

It follows that the ar length L of this segment of the astroid is given by the integral

L =

Z

p

1 + (y

dx