Earth, which is g5 millions of miles from the sun, performs its revolution round it in 365 days, 5 hours, 48 minutes, and 48 seconds. This is called its annual revolution, and causes the difference in the length of the days and nights, and the various... Elementary geography for beginners - Page 26by Richard Hiley - 1872Full view - About this book
| Thomas Hogg - 1806 - 130 pages
...annual revolution round the sun in a year, from, west to east, in the ecliptic; this motion produces the difference in the length of the days and nights, and the regular succession of the *. seasons. 78. The ecliptic is an astronomical circle, and peculiar to the... | |
| C T. Watkins - 1810 - 1056 pages
...end uf Ucceoibcr, wbcm Ve begins to 'move forward as before. This change in the sun's place occasions the difference in the length of the days and nights, and the vicissitude* of ine •MBM. The ecliptic is that path or great circle which the sun is suppose.! to... | |
| Jedidiah Morse - Geography - 1814 - 378 pages
...48 seconds. In its annual course, the earth moves at the rate of 75,222 miles an hour ; which motion causes the difference in the length of the days and nights, and the agreeable succession of the seasons. The Earth has one sate/lite, the MOON, which revolves in an elliptical... | |
| Jedidiah Morse - Geography - 1814 - 382 pages
...feconds. In its annual courfe, the earth moves at the rate of 75,222 miles an hour ; which motion cauies the difference in the length of the days and nights, and the agreeable fucceffion cf the feafons. The Earth has one fatellite, the MOON, which revolves in an elliptical... | |
| Jedidiah Morse - Geography - 1818 - 384 pages
...48 seconds. In its annual course, the earth moves at the rate of 75,222 mites an hour ; which motion causes the difference in the length of the days and nights, and the agreeable succession of the seasons. The earth has one satellite, the MOON, which revolves in an elliptical... | |
| Jacob Willetts - Geography - 1823 - 236 pages
...carried 1043 miles in an hour. It completes its revolution round tbe sun once in a vea- and occasions the difference in the length of the days and nights, and the agreeable •variety of the seasons. '3 rie diameter of the earth'* orbit is about '88000,948 miles,... | |
| Jesse Olney - Geography - 1835 - 298 pages
...many motions has the Earth ? It completes its revolution round the sun once in a year, and occasions the difference in the length of the days and nights, and the agreeable variety in the seasons. The earth is not a perfect sphere, but an oblate spheroid, elevated... | |
| Jesse Olney - Geography - 1836 - 294 pages
...heavenly bodies from east to west. It completes its revolution round the sun once in a year, and occasions the difference in the length of the days and nights, and the agreeable variety in the seasons. The earth is not a perfect sphere, but an oblate spheroid, elevated... | |
| Thomas Ewing (of Edinburgh.) - 1839 - 348 pages
...alternation of day and night ; another, round the sun, in 365 days 6 hours, called its annual motion, which causes the difference in the length of the days and nights, and the various seasons, (k) Mercury, about 7 times greater than at our earth ; while at our earth they are about 360 times... | |
| James Ferguson (schoolmaster.) - 1840 - 48 pages
...APPARENT MOTION OF THE SUN, REDUCED TO TIME. The Annual motion of the earth round the sun, is the cause of the difference in the length of the days and nights, and the various seasons. 360° or 12 signs =365d. 6h. nearly. 30° or 1 do = 30d. do. 1° = Id. do. Note. — I. The Earth in... | |
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