A solar day is the interval between two successive returns of the sun to the same meridian. The sun moves through 360 degrees of longitude in one tropical year, or 365 days, 5 hours, 48 minutes, and 47 sec« onds. Hence the sun's mean daily motion in... A Treatise on Astronomy - Page 66by Elias Loomis - 1866 - 338 pagesFull view - About this book
| John Narrien - 1833 - 548 pages
...sensible, being, in fact, more than two days. It is also known that the length of the sidereal year, or the interval between two successive returns of the sun to the same fixed star, exceeds 365J days by a little more than nine minutes, and tliese, in about 150 years, make... | |
| William Augustus Norton - 1839 - 530 pages
...successive returns of the sun to the same equinox, or to the same longitude, is called a Tropical Year. And the interval between two successive returns of the sun to the same position with respect to the fixed stars, is called a Sidereal Year. 175. It appears from observation... | |
| Edward Bruce (bookseller.), John Bruce - 1846 - 398 pages
...is more than 1,100 miles per minute, or 18| m. per sec. The equinoctial, or tropical year, which is the interval between two successive returns of the sun to the same equinox, consists of 365 d. 5 hrs. 48 m. 49 sec. The difference between the equinoctial and the siderial,... | |
| Elias Loomis - 1855 - 514 pages
...between two successive returns of the vernal equinox to the same meridian is called a sidereal day. The interval between two successive returns of the sun to the same meridian is called a solar day. The sun completes an apparent revolution about the earth in one year, or 365 days... | |
| Elias Loomis - 1870 - 398 pages
...day, expressed in solar time, we have the proportion 360° 59' 8".3 : 59' 8".3 :: one day : 3m. 65.9s. Hence 24 hours of sidereal time are equivalent...and mean solar time, is called the equation of time. cate more than 12h. and sometimes less than 12h., the difference being equal to the equation of time.... | |
| Elias Loomis - 1870 - 274 pages
...thousand years. 114. Solar Time. — Solar time is time reckoned in solar days, hours, etc. A solar day is the interval between two successive returns of the sun to the same meridian. The sun moves through 360 degrees of longitude in one tropical year, or 365 days, 5 hours, 48 minutes,... | |
| Elias Loomis - 1893 - 374 pages
...another, but has not changed so much as the hundredth part of a second, in two thousand years. 117. Sohr Time. — The interval between two successive returns of the sun to the same meridian, is called a solar day. The sun passes through 360 degrees of longitude in one year, or 365 days 5 hours... | |
| Elias Loomis - 1897 - 264 pages
...thousand years. 114. Solar Time. — Solar time is time reckoned in solar days, hours, etc. A solar day is the interval between two successive returns of the sun to the same meridian. The sun moves through 360 degrees of longitude in one tropical year, or 365 days, 5 hours, 48 minutes,... | |
| Edward Singleton Holden - 1899 - 484 pages
...length is found by observation to be 365 (mean solar) days 6 hours 9 minutes 9 seconds = 365d. 25636. The interval between two successive returns of the Sun to the same equinox is called the equinoctial year. Its length is found by observation to be 365 (mean solar) days... | |
| Hamilton Scientific Association - 1903 - 924 pages
...accurately defined as the interval between two successive returns of that point to the same meridian. The interval between two successive returns of the sun to the same meridian is called a Solar day. Owing to the motion of the Earth in its orbit around the Sun it gives an apparent... | |
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