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

129'THE MiooN. Iloonll, wVin full, t raversing that partt of ]ler orbit whic,11 lies nort]t of the equator, and of coturse above the htorizon of the( north pole, and traversing thte portioll thlat lies ssontll of I die eqvuator, and beloew thel polar hlorizon, whetn ntw. I )ur-int' th Ie )olat williter, thertefrel the t11oo1n, from tlle first to the la Ist quartelCr is colnlllnl>ly abti)oveizon, While the sntt is tabsentt; whereas, durin sulinmer, while tht s8tl is prcsetnt, tile lno00on is above thle horizon whjle describing ther first; and last q l ad ranl t-its. 216. About tlle time of the autumnal eqluinox, tlhe mooll wrtcl nletar the f,ell, l'is about; siiset ftor a nutllellr of niulits ilt suessiSClti; l and as tlis is, i lln Favrland th period tof lharvcst:, tile pll 0llcolltlo is called the li/i.'rve.'t./brn.. itll(ltcrstandt the reason of tlhis, silce t}he -110011 is never farl fr'om tlte ecliptic, w xe will suppose hleri Sio ss t)o be in til e ecliptie. if the itnoo moved in thtc equator, tithen, since ttils great ciircle is at rigltt anltes to tte axis of tlte etartlX, all p)at of it, as tlhe eartl rctlvolvcs, would cut the liorizoil at tute sallte cotlstant t anglle. ta11 the ]lltoon's lorblit, or t ile ecliptic, w\tich is here taken to reIrX'eseilt it, l)ein-I oblique to thle eqllator, cuflts the hol)izon at ditffterlnt aglcs i1 diffliereant parts', as will easily be sseen b)y rcftitret ce to an artificial globe. V'hltct tte filrst. of A\Aries, ol' ver.nal eqlinllox, is ill thle cIsterot horizoll, it will 1)e seell thlat t:le celiptic (and colsequently tthe 1oo0s18 orblit) mtakes its least aglle AwithI time orizoni. 2ow at tile autunltal equinox, thie 1sun beillg in. I,iblia, tile 110oo11 t t tlte full is inll.Aic, atd Irises \illcll thloe sun sets. O() thCe following Cvcittlilg, altlhola1gh she afts atlvan lced iln 1cr orbit aboutt 1t 3 (Art. 213), yet hcer progress l)cilgp ob)lique to tile horizon, adi at ia S11111 11atngle wvitlt it, she \vill be found at tt l tlhs t ime hlut a little way below tile ltrl'izoll, con(pltared with thIe point l\\Iere scie was \ t Stillset thle preceding evening. Site therefore rises but a little later eachl evea.lll tlanl s1he did o11 tite evening previous, but her Jpldace of' risinog moves rapidly northward. It sthould )tet ohservedt, tihat in uitlking leir r'evolultio llt'Ot1(1d tlt)o earth, trhe ilto011 ItluSt passl tlte first of Ariesi and therefore maltke tlhese,silliall diltter eces, ill the timle of risillg, every nonitll l. Btt as the mtool is not tfull at tile samile time, except iln autulmnl tlhe eircunsltaltee attracts 1no attenltiol.

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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 122
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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