166

3
166 Author(s): Marcus Baker Source: The American Mathematical Monthly, Vol. 10, No. 1 (Jan., 1903), pp. 14-15 Published by: Mathematical Association of America Stable URL: http://www.jstor.org/stable/2971135 . Accessed: 13/05/2014 17:23 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. . Mathematical Association of America is collaborating with JSTOR to digitize, preserve and extend access to The American Mathematical Monthly. http://www.jstor.org This content downloaded from 193.105.154.47 on Tue, 13 May 2014 17:23:31 PM All use subject to JSTOR Terms and Conditions

Upload: marcus-baker

Post on 05-Jan-2017

212 views

Category:

Documents


0 download

TRANSCRIPT

166Author(s): Marcus BakerSource: The American Mathematical Monthly, Vol. 10, No. 1 (Jan., 1903), pp. 14-15Published by: Mathematical Association of AmericaStable URL: http://www.jstor.org/stable/2971135 .

Accessed: 13/05/2014 17:23

Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at .http://www.jstor.org/page/info/about/policies/terms.jsp

.JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range ofcontent in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new formsof scholarship. For more information about JSTOR, please contact [email protected].

.

Mathematical Association of America is collaborating with JSTOR to digitize, preserve and extend access toThe American Mathematical Monthly.

http://www.jstor.org

This content downloaded from 193.105.154.47 on Tue, 13 May 2014 17:23:31 PMAll use subject to JSTOR Terms and Conditions

14

Hence there are six sets of solutions:

X-0,j y-0; X, - W3 p - 02 m m

(2) Solution of the sinmultaneous equations

mx4 +py=O, my3 +px3 =0.

In addition to the solutions x=y=O, there are exactly nine sets of solutions

xiphr9Mnt-4)ho f yu-n4p7/9M(-7)/t,

wvhere e is an arbitrary niinth root of ninity.

165. Proposed byJ. K. ELLWOOD, A. M., Principal of Colfax School, Pittsburg, Pa.

Solve X4 -x= 14, by quadratics.

Solution by G. B. M. ZERR, A.M., Ph.D., Professor of Cbemistry and Physics, The Temple College. Pbiladel- phia, Pa.

X4-x=14 or $'-16=x--2.

___x _ x 2

2 _- _ 2 1 . 4 X2- +s 4 + 2+

x8 +4+ 4(x2 +4)2 = 4 2+4? 4(xe + 4)

1 x--2 or x=-2 + 4

x-=2 or x? + 2x2 +4x+7=0.

.x2 or---1l nearly, or - 1 ?1?//(-843)] nearly.

166. Proposed by MARCUS BAKER. U. S. Geological Survey, Washington, D. C.

Solve ax + by -zx ....(1). cy+dz=-2xy .... (2). ez+fx-2yz .... (3).

Solution by the PROPOSER,

From (1), (2), and (3), respectively,

(2z-a)x dz ez +fx Y b 2x-c 2z

whence x(2x-c)(2z-a)=zbdz .... (4), fx(2x-c) +ez(2x-c) =2dz? .... (5).

This content downloaded from 193.105.154.47 on Tue, 13 May 2014 17:23:31 PMAll use subject to JSTOR Terms and Conditions

From (4), z=2xa (2x ) bd which substituted in (5), gives, after reduction,

x' + 1 (ae-2cf)x8 + [fc?-a2d d-2(ace + bdf )]xi

2f 4f

-1 8j [ac(ad+ce) +bd(2cf-ae)]x +tj!bd(ace + bdf ) -O.

Similarly,

Y + 21 (ac-2be)y3 + -[f Uc?-e2b-2(ace+ bdf )]y2

1 ~~~1 + 8b [ce(ae+cf ) + df(2be-ac)]y+16 lb df(ace+bdf )=0.

Z+2d (ce-2ad)z3+4d [a2d-e2b-2(ace+ibdf)]z2

1 1 + 81 [ac(ae+be) + bf(2ad-ce)]z +16d bf(ace +Ibdf ) O.

Also solved by LON C. WALKER.

GEOMETRY.

REMARXS ON No. 187, GEOMETRY, BY J. R. IIITT, Goss, Miss.

There seems to be an error in (4) of Professor Zerr's demonstration of

No. 187, Geometry. The result given is not correct. For t== 1 bsinCoosC, t

= 1 -boosC, t -7 = bsinC, from which it is seen that in general P cannot equal I/ 2bcoC,t /2

t,t2. It is also easilyseen that if t: t _t: tt, then must DI=b, whereas DI cannot be >kb.

CALCULUS.

154. Proposed by B. R. DOWNER, HopkinBville, Ky.

At the equinox, when the sun is on the celestial equator, a mat starts driving on a perfectly level plain at six o'clock in the morning, and continues, going always from the sun, at the uniform rate of six nmiles per hour, until six o'clock in the eveninig. Required the path he will travel and the distance in a str aight linie from starting point to stopping point.

This content downloaded from 193.105.154.47 on Tue, 13 May 2014 17:23:31 PMAll use subject to JSTOR Terms and Conditions