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which we know to be the case from other and more direct principles.

508.

Let a and b be the semi-axes of the ellipse; then

the velocity at the extremity of the minor axis is

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a

× {√(ap — g3)
— ç') — 2. vers.-1. 2 p + C}

a

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the whole time of descent to the focus.

Again, by 484, the time of the body's moving from the nearer apside to the extremity of the axis minor is

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509.

Let R be the distance from the centre of force at

which the body is projected; then since

vdv= Fdę =

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dp

(4-4).

? = R, then

1

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N- 1 R-1

But since the velocity in any curve is that which would be ac

quired by the bodys's descent along chord of curvature (PV)

4

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510.

If the centre of force be any where about a circle,

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r being the radius of the circle, and a the distance of the centre of force from that of the circle.

Now when the force is in the circumference a=r, and p is positive

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511. Let the earth's radius be R, and

9 the space

fallen through in a second at its surface; also let p be the periodic time of the Moon. Then if ę be the distance of the moon from the earth, and F the force of the earth's attraction upon the moon, we have

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the distance required in feet, g being equal to 32

expressed in seconds.

512.

t=

1 feet, and p

Generally the time in the parabola is (see 484).

r being

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and the time of falling from rest through any space - z when

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22μ

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tit:: ç3 : √ 2 √ (ç − r) × (§ + 2r)

VOL. II.

2√2

3

2 A

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513. Let x be the angle between the tangent or direction of the body's motion and ę; then

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`v and v' being the velocities in a curve, and a circle at the same distance. Hence

dy

v2: v2 :: sin. : sin. ↓ : sin. ¥ + e cos. 4.

dz

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Hence, since

cannot exceed 90°, if de be considered positive, dis positive, or negative, or is increasing or decreasing, according as v' is> or < than v. If de be negative org be decreasing, then dy is positive or negative, that is, is increasing, or decreasing, according as v is> or <v'.

These results indicate a defect in the enunciation of the problem.

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Then since the velocity of a body revolving at the surface is

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