 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 Elements of the Theory of Astronomy - Page 312by John Hymers - 1840 - 354 pagesFull view - About this book
 | Ephemerides - 1842 - 624 pages
...contain, for every third hour of Greenwich Mean 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... | |
 | Ephemerides - 1843 - 634 pages
...hour of Greenwich Me«i 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... | |
 | Almanacs, American - 1845 - 404 pages
...contain, for every third hour of Greenwich Mean 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... | |
 | 1845 - 396 pages
...contain, for every third hour of Greenwich Mean 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... | |
 | Ephemerides - 1846 - 646 pages
...contain, for every third hour of Greenwich Mein 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... | |
 | George Coleman (F.R.A.S.) - 1846 - 488 pages
...every third hour of Greenwich meantime; 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... | |
 | Ephemerides - 1850 - 668 pages
...contain, for every third hour of Greenwich Mean 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... | |
 | Great Britain. Nautical Almanac Office - 1852 - 676 pages
...contain, for every third hour of Greenwich Mean 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... | |
 | Ephemerides - 1860 - 568 pages
...contain, for every third hour of Greenwich mean time, the íhgular 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... | |
 | Ephemerides - 1861 - 564 pages
...contain, for every third hour of Greenwich mean 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... | |
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