Sidebilder
PDF
ePub
[blocks in formation]

.916. Let L be the latitude of the place; then from the right-angled ▲ (L, 75°) we have (by the question)

[merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small][merged small]

917. If be the radius-vector of the comet's orbit, and r P its perihelion distance; then the time of its distance (from the sun) increasing from r top is (see 484)

[blocks in formation]

being the mass of the sun and comet.

In this formula let p = a, the mean distance of the earth from the sun. Then, by the question,

[merged small][merged small][ocr errors][merged small][merged small][merged small][merged small]

:)

[blocks in formation]

24)

Again, if T denote the length of the year; then (see 453), we

[merged small][ocr errors][merged small][merged small][merged small][merged small][merged small][merged small][merged small][ocr errors]

and the number of days in which the comet is moving within the earth's orbit, is, therefore, expressed by

[blocks in formation]
[merged small][merged small][merged small][merged small][ocr errors][ocr errors][merged small][merged small][ocr errors][ocr errors][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small]

919. The curve required is evidently the orthographic projection of the circular arch upon the surface of the water, and is, therefore, by the theory of projections, an ellipse, whose equation is

y' = cot.' I . (r2 = x2)

and semi-axes

r and r cot. I.

r being the radius of the arch, and I the meridian altitude of the

[blocks in formation]
[merged small][merged small][ocr errors][merged small][merged small][merged small][ocr errors][merged small]

Again the force at A being constant, we have

[merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][ocr errors][subsumed][ocr errors][merged small][merged small][merged small][merged small][merged small][merged small][merged small][merged small]

921.

a.

The right-ascension of the star, and time of the year, being given, the angular distances of the star and sun from Aries are known, and, consequently, the angle between them. Let this be denoted by Also the co-declinations of the star and sun are known, which call D, and D' respectively. Then if L be the latitude of the place or altitude of the Pole; from the right-angled spherical triangles, whose hypothenuses are D, D', we easily get two equations between the two unknown quantities, L and the angular distance of the star from the meridian.

922.

the density be

At any distance x from the centre of the sphere let

Ax",

+ being variable, and A and a certain constants not yet determined. Then if Q denote the quantity of matter in the sphere, whose radius is x, and M its magnitude, we have

[merged small][ocr errors][ocr errors][merged small][ocr errors][ocr errors][merged small][merged small][merged small][merged small]

Now if D be the mean density of a sphere whose radius is r, then by the question mD = the density at its surface; and we have, from the quantities of matter being the same in both hypotheses of density,

[merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][merged small][ocr errors][merged small][merged small][merged small][merged small][merged small][merged small][merged small]

923.

Let G be the magnitude of a guinea; bG represents its weight C. Also let P and G be the magnitudes of the platina and silver requisite to make the coin in question; then by the question we have

P+S G

and aP+cSbG.

.. aPaS = aG

and (ca) S (b − a) G

« ForrigeFortsett »