An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ...

J UPITel 48at.:197 of tlle olcs is indeed quite pc)rccptible by the telescope, anld is ol)\ious to th eye in a correct drawing of the planet. (See I:'rontispiece.) Such a figure might naturally be expected firom the rapidity of his diurnal revolution, which is accolnplishllc inl about 10 hours (9h. 551n. 21.s.3).* A. place oni the cquator of Jupiter must revolve 450 miles per minlute, or 27 times as fast as a place on the terrestrial cquator. Th'.le distance of Jupiter ftom the sunl is 495,000,000 ]ilcs (4195,81Y7,00).[ Illis plane of rotation is but slightlyt ilnclinel to the plane of Ilis orbit (only about 30), and consequeltly his climato expericnccs bu)t a slight change of seasons. 329.''The view of Jupiter thllouigh a good tclescope is one of.tllhc ost mIlaglificent alnd interesting spectacles amlong the hceavenly bodies..1The disk expands into a large and bright orb like the full moon; tlhe spheroidal figure which theory assinlls to revolill.n worlds is herle pa)iblyr cxhibited to the c'e; across the disk, arranged in parallel stripes, are discerned several dusky bandls, called belts; and four lrightl satellites, always it att-cndancee but ever varyilng their )ositions) colmpose a: splcn(did retinulll. IndlCed, astrononm10'rs gaze -with pecuiliar illterest on Jupiter and his moons, as affording a miniature representation of the whole solar system; repeating, oln a smaller scale, thle saiame revolutions, and ecxmplifyting, iln a mannmer more witliln the comlpass of our observation, tlhe same laws as recgulate the entire assemblage of siun and planets. 330. The?Belts f J apriter, are variable in their number and dimensions. AWith smaller telescopes only one or two are scem across the equatorial regions; but with mIolr powerfull inlstlrulnments the nl1luber is increasecd, coNvering a great part o tllhe disk. Occasionallay these belts retain nearly the same formt alnd positiolIs for rmanly montlhs together, while at other times they undergo great and sudden changes, and il One or two ilntances, t.ey lhave been obscrved to break up and spread themselves ov\er tle whole face of thle planet. The prevailing opinion almongl astronomers in reference to ithe nature of these belts is, tllhat they are piroduclcd by disturbances in tlhe plact's at.nos. - Ahy.' Ilind.,

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Title
An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ...
Author
Olmsted, Denison, 1791-1859.
Canvas
Page 197
Publication
New York,: Collins & brother,
1865.
Subject terms
Astronomy

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"An introduction to astronomy: designed as a text-book for the use of students in college. By Denison Olmsted ..." In the digital collection Making of America Books. https://name.umdl.umich.edu/ajn0587.0001.001. University of Michigan Library Digital Collections. Accessed June 7, 2025.
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