 | 1833 - 634 pages
...Mean Time, the angular distances between the rentres of the Moon and certain heaven!; bodies, such as they would appear to an observer at the centre of the Earth. WheTi » Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | 1835 - 618 pages
...every third hour of Gì Time, the angular distances between the centres of the Moon and ce bodies, such as they would appear to an observer at the centre of the Ea Lunar Distance has been observed on the surface of the Earth, and centre, by clearing it of the... | |
 | 1841 - 630 pages
...Time, the angular distances between the apparent centres of the Moon and certain heavenly bodies, euch as they would appear to an observer at the centre of the Earth. When a Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | Janet Taylor - 1842 - 592 pages
...sun, and from the other celestial bodics above mentioned, for every third hour of Greenwich mean time, as they would appear to an observer at the centre of the earth. When, therefore, a lunar distanee has been observed at any distant place and reduced to the centre... | |
 | 1842 - 624 pages
...Time, the angular distances between the apparent centres of the Moon and certain heavenly bodies, such as they would appear to an observer at the centre of the Earth. When a Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | 1843 - 634 pages
...Time, the angular distances between the apparent centres of the Moon and cab: heavenly bodies, such as they would appear to an observer at the centre of the EirtL When a Lunar Distance has been observed on the surface of the Earth, and redasto the centre,... | |
 | 1845 - 404 pages
...Time, the angular distances between the apparent centres of the Moon and certain heavenly bodies, such as they would appear to an observer at the centre of the Earth. When a Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | 1845 - 396 pages
...Time, the angular distances between the apparent centres of the Moon and certain heavenly bodies, such as they would appear to an observer at the centre of the Earth. When a Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | 1846 - 646 pages
...Time, the angular distances between the apparent centres of the Moon and certain heavenly bodies, such as they would appear to an observer at the centre of the Earth. When a Lunar Distance has been observed on the surface of the Earth, and reduced to the centre, by... | |
 | George Coleman (F.R.A.S.) - 1846 - 488 pages
...being the angular distances between the apparent centres oí the moon and certain heavenly bodies, such as they would appear to an observer at the centre of the earth. When a lunar distance has been observed on the surface of the earth, and reduced to the centre, by... | |
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All the distances that can be observed on the same day, are grouped together under that date ; and the columns are read from left to right, across both pages of the same opening. 
