The Complete Mathematical and General Navigation Tables: Including Every Table Necessary to be Used with the Nautical Almanac in Finding the Latitude and Longitude : with Their Description and Use, Comprising the Principles of Their Construction, and Their Direct Application to Plane and Spherical Trigonometry, Navigation, Nautical Astronomy, Dialling, Practical Gunnery, Mensuration, Guaging &c. &c, Volum 1

Baldwin and Cradock, 1828 - 664 sider

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Correction of the mean astronomical refraction
To find the latitude by the north polar star
Correction of the latitude deduced from the preceding table
Mean right ascension of the sun
Equations to equal altitudes of the sun part First
To reduce the suns longitude right ascension and declination and also the equation of time as given in the Nautical Almanac to any given time under ...
To reduce the moons longitude latitude right ascension declin ation semidiameter and horizontal parallax as given in the Nautical Almanac to any giv...
Equation of the second difference of the moons place
Correction of the moons apparent altitude
To reduce the true altitudes of the sun moon stars and planets to their apparent altitudes
Auxiliary angles
Correction of the auxiliary angle when the moons distance from a planet is observed
Error arising from a deviation of one minute in the parallelism of the surfaces of the central mirror of the circular instrument of reflection
Error arising from an inclination of the line of collimation to the plane of the sextant or to that of the circular instrument of re flection
Logarithmic difference
rent altitude
Logarithms of numbers
Logarithmic secants to every second in the semicircle
Logarithmic tangents to every second in the semicircle
Acceleration of the fixed stars or to reduce sidereal time into
latitude and the declination being of the same name
LIU The miles and parts of a mile in a degree of longitude at every
Table Page
Latitudes and longitudes of the principal seaports islands capes
Solution or Problems in Plane and Spherical Trigono

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Side 19 - Given two sides and the included angle, to find the third side and the remaining angles. The sum of the required angles is found by subtracting the given angle from 180°. The difference of the required angles is then found by Theorem II. Half the difference added to half the sum gives the greater angle, and, subtracted, gives the less angle.
Side 484 - AZIMUTH, in astronomy, an arch of the horizon, intercepted between the meridian of the place and the azimuth, or vertical circle passing through the centre of the object, which...
Side 212 - For the purpose of measuring angles, the circumference is divided into 360 equal parts, called degrees ; each degree into 60 equal parts, called minutes ; each minute into 60 equal parts called seconds.
Side 63 - And, if the logarithm of any number be divided by the index of its root, the quotient will be equal to the logarithm of that root. Thus the index or logarithm of 64 is 6 ; and, if this number be divided by 2, the quotient will be = 3, which is the logarithm of 8, or the square root of 64.
Side 63 - Also, between the mean, thus found, .and the nearest extreme, find another geometrical mean, in the same manner ; and so on, till you are arrived within the proposed limit of the number whose logarithm is sought.
Side 487 - ... reckoned from the north in north latitude, but from the south in south latitude. » In observations of the altitude of the sun'< loiter limb (by afore enervation) it is u«u»l to »<M 12' for tic cBecl of dip, parallax, ami sern diameter.
Side 159 - When there happens to be a remainder after the division ; or when the decimal places in the divisor are more than those in the dividend ; then ciphers may be annexed to the dividend, and the quotient carried on as far as required.
Side 681 - The Young Navigator's Guide to the Sidereal and Planetary Parts of Nautical Astronomy.
Side 649 - ... position with respect to a luminous body, can cast a circular shadow ; likewise all calculations of eclipses, and of the places of the planets, are made upon supposition that the earth is a sphere, and they all answer to the true times when accurately calculated. When an eclipse of the moon happens, it is observed sooner by those who live eastward than by those who live westward ; and, by frequent experience, astronomers have determined that, for every fifteen degrees difference of longitude,...
Side 183 - II. The sine of the middle part is equal to the product of the cosines of the opposite parts.

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