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98. If in (48) x = log. b in any system, x': L. b,* in the naperian system, and M': '= modulus of naperian system =1, we have

log. b: L. b :: M: 1,
log. b MxL. b.

whence

(49)

That is, the logarithm of a number in any system is equal to the modulus of that system multiplied by the naperian logarithm of the number.

99. If b=a= base of the system whose modulus is M, then log. b=1, and (49) becomes

1=MXL. a,

1

L. a

whence

(50)

That is, the modulus of any system is the reciprocal of the naperian logarithm of the base of the system.

If in (50) a=10, we shall have the value of the modulus of the common system, or

M=

M

=

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The naperian logarithm of 10, as will be shown hereafter, (Art. 113,) is 2.30258,50930. Therefore

Briggs' modulus

1
L. 10

1 2.30258,50930

log. b

-.43429,44819,

which

agrees with the value found by another method in Art. 93. 100. If we substitute in (49) the value of M given by (50), we

have

L. b
L. a

·

=

(51)

That is, the logarithm of a number to any given base is equal to the naperian logarithm of that number divided by the naperian logarithm of the given base.

* We here designate naperian logarithms by the letter L., to distinguish them from other logarithms.

101. If we make be in (49), we have

log. e = M× L. e= = M.

(52)

That is, the logarithm of Napier's base in any system is equal to the modulus of that system.

Hence, Briggs' modulus is the common logarithm of Napier's base, or

log. 2.718281828 &c. = .4342944819 &c.

102. With the aid of these principles, we can construct as many systems of logarithms as we please after having calculated a table of naperian logarithms; for, by (49), we have only to multiply all the logs. of this table by the modulus of the new system, in order to obtain the logarithms in this system; or, by (51), we have only to divide each naperian logarithm by the naperian logarithm of the new base, to obtain the logarithms to that base.

103. We may now suppose the modulus to be known, since it may be determined for any base by formula (42). We are not, however, yet prepared to construct a table, for (34) is not convergent unless b is less than 2. Various transformations have been proposed, by which it is rendered very convergent and expeditious in practice. The most useful of these we proceed to explain.

log. (n+d)—log. n=.

TRANSFORMATIONS OF THE LOGARITHMIC FORMULA.

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104. Since (34) will converge when b<2, let b=1+ d

n

n

whence b-1=-, and log. b= log. (n+d)— log. n, (Art. 61.) The formula becomes

n

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=M

d5

d d2 d3 d4
i+
ท 2n1 3n3 4n4 5n5

+

d

Again, let b=1—

whence b-1

n

n

log. (n-d)- log. n. The formula becomes

n

d

log. (nd) - log. n=M M (-22.

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d ds (3 d4 d5
n 2no 3n3 4n4 5n5

d n+d

-=

&c.) (53)

and log. b

xc.) (54)

Add (54) to (53); we have

log.(n+d)−2 log.n+log. (n–d)=M ( —

2d

log. (n+d) log. (n−d)=M(~ +

or transposing and reducing,
log. (n+d)= log. (n− d) +2 M (

2d = p―1, log. 1=0)

or transposing and reducing,

log.(n+d)=2 log.n—log.(n-d)-M(+++ &c.) (56)

Subtract (54) from (53); we have

and

n

log. p=2M

p-1

P+1

=

d

n

These formulæ will always converge when is a proper fraction; that is, when d <n. In using (53) log. n must be known before log. (n+d) can be determined. From (54) we find log. n when log. (n-d) is given; from (56) we find log. (n+d) when log. n and log. (nd) are given; and from (58) we find log. (n+d) when log. (n-d) is given.

ds d4

no 2n1

105. In (58) let n+d=p, n-d=1, whence 2n=p+1,

d

d4

2d3
3n3

d d3

ds

M(C + + + &c.) (58)

3n3

5n5

1

2n

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de

3n6

+

&c.) (55)

+ + &c.) (57)

2d5
5n5

; then we have (since log. (n-d)=

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This formula requires no logarithms to be given, but converges slowly unless p is a small number.

106. In formulæ (53, 54, 56, 58) let d=1; then we have

1

1

log. (n+1)= log. n+M (1

1
3na 4n1 5n5

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(59)

+ &c.) (60)

1

4n1+5ns+ &c.) (61)

1

log. (n+1)=2 log. n—log. (n-1)-M (+

2n1

log. (n + 1) = log. (n−1) + 2 M (1 + 3/

1

3n3

+

1

1

3n6

whence we find n-p3-3p, d=2, and

In (58) substitute n+d=p+1, n-d-p, whence we have

d

1

2n=2p+1, 2d=1, and

-1

; the formula becomes

n 2p+1

These values substituted in (58) give

log.(p+1)=log.p+2M(2p+1+3(2p+1)=+5(2p+1)3

+ &c. (64)

These formula will be found convenient in calculating the logarithm of a number, when that of a number greater or less by unity is given.

1

+5n+ &c.) (63) Sere! We

;+

55

1

+ &c.) (62)

n+d=(p—1)3 (p+2)=p3—3p+2
n―d=(p+1)3 (p-2)=p3-3p-2

107. The above would suffice for the computation of a table, but other formulæ have been found, in which the series are more rapidly convergent. That of BORDA may be thus derived. In (58) let

log. (n+d)=2 log. (p-1)+log. (p+2)
log. (n―d)= 2 log. (p+1)+log. (p—2)

log. (p+2) — 2 log. (p+1)+2 log. (p-1) — log. (p-2)=

2

1

2 3 1

2 5

2M

" [p = 3 p + = ( p = sp)" + ( p2 = 3p)'+ &c.] (65)

3 3 -3p. 5

By this formula we may obtain log. (p+2) when the logarithms of p+1, p-1 and p-2 are given. The series is so convergent that when p=50 the first significant figure of the second term is in the 15th place of decimals.

108. A still more convergent formula, but requiring more logarithms to be known, is that of HAROS. In (58) let

n+d=(p—3)(p+3)(p−4)(p+4)=p*—25p3+144

n—d=p2(p—5)(p+5)

=p*-25p3

whence we have n=p1- 25p3+72, d=72, and the formula becomes

log. (p+5)-log. (p+4)—log. (p+3)+2 log. p-log. (p—3)— log. (p-4)+log. (p—5)—

72

1

+ 33 (‚'_2532)2+72)*+ &c.] (66)

p*—25p2+72

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-2M

This formula expresses the relation between seven logarithms, and the series is very convergent.

109. In (64) let p+1=q2, p=q3—1=(q—1)(q+1); the formula becomes

2 log. q = log. (4 — 1) + log. (q + 1) +

1

1

2 M (22 + (2q1—1) + &c.)

-1

from which we derive

log. q = [ log. (q − 1) + log. (q + 1) ] +

1

3(2qo—1)® + &c.)

M

1 (292-1

(67) which is a very convenient formula, requiring but two logarithms to be given.

+

110. An unlimited number of formulæ may be derived from (53) and (54) by a peculiar combination, the law of which will be perceived in the following examples.

, In (53) let d=3, 2, 1, and in (54) let d=1, 2, 3, successively; we shall thus obtain the six following formulæ :

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