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68. (Prop. VI.) Investigations of formulæ for determining two
sides of a spherical triangle when there are given the other
side and two adjacent angles

69. Investigations of formulæ for expressing the relations between

an angle in any plane and its orthographical projection on

a plane inclined to that of the angle

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70. Reduction of an arc on any small circle to the corresponding
arc on a great circle parallel to it; and the converse
71. Two great circles making with each other a small angle at
their line of section, and from a point in one of these an
arc of a great circle being let fall perpendicularly on the
other, also from the same point an arc of a small circle
perpendicular to both being described; there are inves-
tigated approximative formulæ for the distance between
the two arcs and the difference of their lengths

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69

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trials
88. Process for determining the error of collimation by a micro-
meter, and the manner of correcting the observed time of
a transit on account of that error
89. Method of ascertaining that the meridional wire and those
which are parallel to it are in vertical positions, and that
the wire at right angles to them is horizontal

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89

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119. Employment of the micrometer with an equatorial, in mea-
suring angles of position, and small angular distances

120. Manner of deducing from thence the differences of declina-
tion and right ascension between two stars, and between

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123. Description of the floating collimator

124. Manner of using the horizontal and vertical collimators
125. The spirit level collimator, and manner of using it for find-
ing the error of collimation in a transit telescope or circle

126. Description of the repeating circle

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128. Manner of observing horizontal and oblique angles -
129. Hadley's reflecting octant, &c.

130. Manner in which, after two reflexions of light from an object,
the image of that object may be made to coincide with that
of an object seen by direct view

131. The parallax of a reflecting instrument

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144. Formula of Bradley : values of the constant, according to

Biot, Groombridge, and Atkinson

Page

108, 109

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169. The sun's declination goes through its changes during a year 129

170. The greatest observed declination of the sun is an ap-
proximate value of the obliquity of the ecliptic

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177. Designations of the rectangular co-ordinates of any point - 135

178. Transformation, when two of the co-ordinate planes turn
about their line of section, the latter remaining fixed

179. Application of spherical trigonometry in the case just men-

tioned

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