A Treatise on Astronomy, Descriptive, Physical and Practical: Designed for Schools, Colleges, and Private Students |
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Page vi
... noon ,. 91 What is meant by sun slow and sun fast ,. 94 Use of the equation of time , .... 96 CHAPTER VI . Apparent motions of the planets ,. 97 The morning and evening star , .. 98 Motion of Venus in respect to the fixed stars , .. 101 ...
... noon ,. 91 What is meant by sun slow and sun fast ,. 94 Use of the equation of time , .... 96 CHAPTER VI . Apparent motions of the planets ,. 97 The morning and evening star , .. 98 Motion of Venus in respect to the fixed stars , .. 101 ...
Page ix
... noon , .. Results taken from the projection , ...... Results from trigonometrical computations ,. 286 287 288 CHAPTER V. Local eclipses , & c . , ..... 291 How to construct a local solar eclipse , .. 291 How to find the time of greatest ...
... noon , .. Results taken from the projection , ...... Results from trigonometrical computations ,. 286 287 288 CHAPTER V. Local eclipses , & c . , ..... 291 How to construct a local solar eclipse , .. 291 How to find the time of greatest ...
Page 9
... noon , and about 23 ° in alti- tude ; and is nearly west at 6 in the afternoon . ( 11. ) In the southern hemisphere , there is no prominent star near the south pole ; that is , no southern polar star ; but , of course , there are ...
... noon , and about 23 ° in alti- tude ; and is nearly west at 6 in the afternoon . ( 11. ) In the southern hemisphere , there is no prominent star near the south pole ; that is , no southern polar star ; but , of course , there are ...
Page 18
... noon to noon , when we take the average of the whole year , is 24 hours of solar time , or 24 h . 3 m . 56.5554 s . of sidereal time ; but , as we have just observed , these intervals are not uniform ; for instance , about the 20th of ...
... noon to noon , when we take the average of the whole year , is 24 hours of solar time , or 24 h . 3 m . 56.5554 s . of sidereal time ; but , as we have just observed , these intervals are not uniform ; for instance , about the 20th of ...
Page 33
... noon , local solar time . By merely inspecting these observations , it will be perceived that the sun must have crossed the equator between the 20th and 21st ; for at the apparent noon of the 20th , the declina- tion was 11 ' 29 " .4 ...
... noon , local solar time . By merely inspecting these observations , it will be perceived that the sun must have crossed the equator between the 20th and 21st ; for at the apparent noon of the 20th , the declina- tion was 11 ' 29 " .4 ...
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Common terms and phrases
altitude apogee apparent diameter argument argument of latitude ascending node astronomers attraction axis called celestial celestial equator central eclipse CHAP circle clock comet compute conceive conjunction corresponding declination degrees determine difference Digits eclipsed earth earth's orbit eccentricity equa equal equator equinox Evection fixed stars full moon give gravity greater greatest Greenwich heavens Hence horizon horizontal parallax inferior planet interval Jupiter Kepler's Kepler's third law less lunar orbit magnitude mass Mean Anomaly mean distance measure Mercury meridian altitude miles minutes MOON'S HOURLY MOTION moon's motion moon's path nearly node nutation observations opposite perigee period planet pole position proportion radial force radius refraction represent result revolution right angles right ascension round satellites Saturn semidiameter sidereal sine solar sun and moon suppose tance tangent telescope tion transit triangle true tude Uranus variation velocity Venus zenith
Popular passages
Page 144 - Jupiter a moderate-sized orange, in a circle nearly half a mile across; Saturn a small orange, on a circle of four-fifths of a mile; Uranus a full-sized cherry, or small plum, upon the circumference of a circle more than a mile and a half, and Neptune a good-sized plum on a circle about two miles and a half in diameter.
Page 139 - ... appearances of spots seen upon them, render it extremely probable that they subsist in the atmosphere of the planet, forming tracts of comparatively clear sky, determined by currents analogous to our trade-winds, but of a much more steady and decided character, as might indeed be expected from the immense velocity of its rotation. That it is the comparatively darker body of the planet which appears in the belts is evident from this, — that they do not come up in all their strength to the edge...
Page 143 - Venus a pea, on a circle 284 feet in diameter; the Earth also a pea, on a circle of 430 feet; Mars a rather large pin's head, on a circle of 654 feet; Juno, Ceres, Vesta, and Pallas, grains of sand, in orbits of from 1000 to 1200 feet; Jupiter a moderate-sized orange, in a circle nearly half a mile across...
Page 80 - For, by the first of Kepler's laws, the areas described by the radius vector are proportional to the times, and when this is the case, by Art.
Page 118 - The squares of the times of revolution are to each other as the cubes of the mean distances from the sun.
Page 144 - As to getting correct notions on this subject by drawing circles on paper, or, still worse, from those very childish toys called orreries, it is out of the question.
Page 141 - ... and less strongly marked than those of Jupiter, and owing doubtless to a similar cause. That the ring is a solid opake substance, is shown by its throwing its shadow on the body of the planet on the side nearest the sun, and on the other side receiving that of the body.
Page 154 - ... is leaving behind, must seem gradually to approach, in the same manner as when we walk through a forest, the ranges of trees to which we advance are constantly widening in their apparent distance from each other, while the distance of those we leave behind is gradually contracting.
Page 147 - Gregorius, of Constantinople, in June, 1337, whose course he describes very accurately. Comets do not all move from west to east, like the planets. Some have a direct, and some a retrograde motion. Their orbits are not comprehended within a narrow zone of the heavens, like those of the principal planets ; they vary through all degrees of inclination. There are some whose plane is nearly coincident with that of the ecliptic, and others have their planes perpendicular to it. Indeed, a slight inclination...
Page 89 - Whenever the sun is above the horizon of any place, that place is receiving heat; when below, parting with it, by the process called radiation ; and the whole quantities received and parted with in the year...