Lectures on Experimental Philosophy, Astronomy, and Chemistry: Intended Chiefly for the Use of Students and Young Persons, Volume 2Longman, 1820 - Astronomy |
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Page 5
... equal time . The difference between mean and solar time depends upon three causes . 1st , The earth ( according to the third law o Kepler ) does not pass equal portions of its orbit in equal times . It proceeds sometimes quicker , and ...
... equal time . The difference between mean and solar time depends upon three causes . 1st , The earth ( according to the third law o Kepler ) does not pass equal portions of its orbit in equal times . It proceeds sometimes quicker , and ...
Page 6
... equal and regular ; and if the plane of the ecliptic were parallel to the equator , there would be no difference in the time marked by either of these circles , for fifteen degrees of each of these circles passing over any meridian ...
... equal and regular ; and if the plane of the ecliptic were parallel to the equator , there would be no difference in the time marked by either of these circles , for fifteen degrees of each of these circles passing over any meridian ...
Page 8
... equal times , the one in the circle of the ecliptic , and the other in that of the equator . 3dly , The orbit of the earth being an ellipsis , of which the sun occupies one of the foci , the portions of the ecliptic which the sun ...
... equal times , the one in the circle of the ecliptic , and the other in that of the equator . 3dly , The orbit of the earth being an ellipsis , of which the sun occupies one of the foci , the portions of the ecliptic which the sun ...
Page 10
... equal : and throughout the earth , ex- cept in the frigid zones , the longest and the shortest day together make 24 hours . Such is the duration of the artificial day to the different inhabitants of the earth , if we re- gard only the ...
... equal : and throughout the earth , ex- cept in the frigid zones , the longest and the shortest day together make 24 hours . Such is the duration of the artificial day to the different inhabitants of the earth , if we re- gard only the ...
Page 29
... equal parts , which are called digits ; and an eclipse is said to be so many digits , according to the number of those parts which are obscured . In total eclipses of the moon , it is often said to be eclipsed more than twelve digits ...
... equal parts , which are called digits ; and an eclipse is said to be so many digits , according to the number of those parts which are obscured . In total eclipses of the moon , it is often said to be eclipsed more than twelve digits ...
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Lectures on Experimental Philosophy, Astronomy, and Chemistry ..., Volume 1 G. (George) Gregory No preview available - 2012 |
Lectures on Experimental Philosophy, Astronomy, and Chemistry: Intended ... No preview available - 2019 |
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acid gas alkali alum ammonia animal appears applied atmosphere attraction for water becomes bodies boiling burning called caloric carbonat carbonic acid carbonic acid gas charcoal chemical chemistry chemists clay cold colour combined combustible compound condensed contain converted into vapour copper crystals degree of heat deliquescent dissolved distillation earth eclipse effect effervescence equator evaporation exposed fire flame fluid fluidity freezing furnace fusion glass Hence hydrogen hydrogen gas iron lecture lime liquor magnesia matter melted mercury metals mineral waters mixed mixture moon mucilage muriatic acid nitrat nitric acid nitrogen node obtained orbit oxide oxygen oxygen gas particles phænomenon phosphorus portion potass powder precipitated produced proportion pure resins rises saltpetre saturated sensible heat separated silver small quantity smell soda solid solution sometimes specific gravity spirit of wine stances strata strong substances sulphat sulphuric acid surface tains temperature tion transparent vegetable vessel volatile alkali
Popular passages
Page 1 - ... to the inclination of the axis of the earth to the plane of the ecliptic, and partly to the different positions in which a spectator is placed in different zones of the globe.
Page 22 - An eclipse of the sun can only take place when the moon is in conjunction with the sun, and when she is in one of her nodes, or very near it. Suppose the line EE (fig. 8) to be a portion of the ecliptic, and LL a portion of the orbit of the moon, cutting the ecliptic in the point N, at an angle of a little more than five degrees. Then, if in the moment of her conjunction the moon is found in the point F of her orbit, she will be too far from her node to intercept the sun's light, and cause an eclipse.
Page 86 - ... to combine with the oxygen of the atmosphere, and this oxygen during its combination lets go the caloric with which in the state of air or gas it was combined.
Page 86 - It is of course incombustible, because; its base being already saturated with oxygen, cannot combine with any more.
Page 26 - But the falling back of the line of conjunctions, or oppositions of the sun and moon 28' 12", with respect to the line of the nodes in every period, will wear it out in process of time; and after that it will not return again in less than 12,493 years.
Page 246 - When a sheet of pure tin is immersed in a solution of nitro-muriate of gold, the oxide of gold is precipitated of a purple colour; and, when scraped off and collected, forms the purple powder of Cassius, much employed in enamelling.
Page 25 - ... 225 days; in which time there would always be a regular period of eclipses, if any complete number of lunations were finished without a fraction. But this never happens ; for if both the Sun and Moon should start from a line of conjunction with either of the nodes in any point of the ecliptic, the Sun would perform 18 annual revolutions and 222 degrees over and above, and the Moon 230 lunations and 85...