 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 - Pàgina 312per John Hymers - 1840 - 354 pàginesVisualització completa - Sobre aquest llibre
 | 1842 - 624 pàgines
...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... | |
 | 1843 - 634 pàgines
...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... | |
 | 1845 - 404 pàgines
...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 pàgines
...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... | |
 | 1846 - 646 pàgines
...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 pàgines
...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... | |
 | 1850 - 668 pàgines
...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 pàgines
...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... | |
 | 1860 - 568 pàgines
...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... | |
 | 1861 - 564 pàgines
...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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