An Elementary Treatise on Plane & Spherical Trigonometry: With Their Applications to Navigation, Surveying, Heights, and Distances, and Spherical Astronomy, and Particularly Adapted to Explaining the Construction of Bowditch's Navigator, and the Nautical Almanac |
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Page 213
... at the distance from P , PM PM will appear to describe the circumference MHMH . It will rise in the east at H and set at H ' , if the distance PM Sideral time . from the pole is greater than the $ 22 . ] 213 DIURNAL MOTION .
... at the distance from P , PM PM will appear to describe the circumference MHMH . It will rise in the east at H and set at H ' , if the distance PM Sideral time . from the pole is greater than the $ 22 . ] 213 DIURNAL MOTION .
Page 214
... sideral day , that is , literally , a star - day . This day is divided into 24 hours , and clocks regulated to this time are said to denote sideral time . [ B. p . 147. ] 24. Each point of the celestial equator passes the meridian once ...
... sideral day , that is , literally , a star - day . This day is divided into 24 hours , and clocks regulated to this time are said to denote sideral time . [ B. p . 147. ] 24. Each point of the celestial equator passes the meridian once ...
Page 215
... sideral time since the passage of the star over the meridian . 26. Corollary . The difference of the right ascensions of the star and of the meridian is the hour angle of the star . 27. The distance of a star from the east or west ...
... sideral time since the passage of the star over the meridian . 26. Corollary . The difference of the right ascensions of the star and of the meridian is the hour angle of the star . 27. The distance of a star from the east or west ...
Page 226
... superior and inferior passage of a star over the meridian is just half of a sideral day . If , then , a telescope Meridian determined by circumpolar stars . were placed so as 226 [ CH . III . SPHERICAL ASTRONOMY . The Meridian.
... superior and inferior passage of a star over the meridian is just half of a sideral day . If , then , a telescope Meridian determined by circumpolar stars . were placed so as 226 [ CH . III . SPHERICAL ASTRONOMY . The Meridian.
Page 227
... sideral time of its description . Let then T = the sideral time of describing the arc S M , t = the sideral time of describing the arc s m , I interval from the observation at S to that at s , i = interval from the observation at s to ...
... sideral time of its description . Let then T = the sideral time of describing the arc S M , t = the sideral time of describing the arc s m , I interval from the observation at S to that at s , i = interval from the observation at s to ...
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Common terms and phrases
A₁ aberration altitude and azimuth angle given ascension and declination azimuth celestial equator celestial sphere centre circle computed Corollary corr correct central altitude corresponding cosec cosine cotan diff difference of latitude difference of longitude dist earth eclipse of April equal to 90 formula gives Greenwich Hence horizon horizontal parallax hour angle hypothenuse included angle interval latitude and longitude lunar distance mean meridian altitude method middle latitude moon's motion N₁ Napier's Rules Nautical Almanac Navigator Nutation obliquity obtuse perpendicular plane polar triangle prime vertical Problem R₁ radius reduced right ascension sailing Scholium second member semidiameter sideral sideral day solar eclipse Solution solve the triangle spherical right triangle spherical triangle star's sun's Table XXIII tang tangent Theorem transit triangle ABC Trig true latitude tude vernal equinox whence
Popular passages
Page 156 - I. The sine of the middle part is equal to the product of the tangents of the adjacent parts.
Page 145 - A spherical triangle is a portion of the surface of a sphere, bounded by three arcs of great circles.
Page 48 - As the sine of the angle opposite the given side is to the sine of the angle opposite the required side, so is the given side to the required side. Thus, if a (fig.
Page 50 - The third side is found by the proportion. As the sine of the given angle is to the sine of the angle opposite the required side, so is the side opposite the given angle to the required side.
Page 41 - Since, when an angle is acute its supplement is obtuse, it follows from the preceding proposition, that the sine and cosecant of an obtuse angle are positive, while its cosine, tangent, cotangent, and secant, are negative.
Page 53 - The sum of any two sides of a triangle is to their difference, as the tangent of half the sum of the angles opposite to those sides, to the tangent of half their difference.
Page 182 - But a' = 180° - A, b' = 180° - ß, c' = 180° - C. and A' = 180° - a. Therefore, — cos A = (— cos B)(— cos C) + sin B sin C(— cos a...