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

this subtracted from th th time of opposition gives us ftle time of the middle of the eelip6se. Secondly, joining Ac (I)'ig. 5t:), not represented in the figrn)c, we calculate m.Ae, in fle triangle AreN; thelln A (:::::: mIA).M c..:.A(.. hec=::::. Ielnce, in tlhe triangle ACe, we can determine AC, and ttherefore.OAC AMl::::: MC, wllicl changlled into time as before, gives us, whlven subtracted firomtt the time of the middlle of the eclipse, the time of the beginntting of the ectipyse, or, whlen added to tlhat of the middle, the, ti'e of tthe en7d of the ecli2pse. The stlum of the two equals the ole ralion. Thllilrdly, by a similar metlhod -we calcuhlte the value of AMO'> which converted into time), and subtracted fr'om the time of tlte middle of the celipsc, gives the eommei cement.ofV totil (larkness, or when addelcd gives the end of total (artnc88. Their sum is the (d1'rattio)n of tottl (datkness. FIourthly, the qtaelutitdy qf the ectipse is determined by supposing the diameter of thle moon livided into twelve equal parts called Digits, and finding how many suchl parts lie'within the slhadow, at the time whlenl the centers of. the omoo n and tlhe shadow are nearest to each other. Even whenll the 3moonl lies whlolly Aithllil thle sladow, the quantity of the eclipse is still expressed by the iunlber of digits contained in that part of the line whlich joins the center of the shadow and fthe center of th0e 0 moo n, which is intercepted between the edge of the shadow and the inner edge of the Iloonl. Tillus ill figure no Ao...... An 54, thoe Inuber of digits eclipsed, equals............. - Ao..(Am.....) A...... (-.. an exprl'ession containing only known quantitles. 261. The for'cgoing will. serve as an explanation of tld ge~neral prinec)ies, on wlichl proceeds tfhe calculation of a lunar eclipse. AThe actual methotds practiced employ mlany expedients to facilitate the process, and to insure the greatest possible accuracy, the nature of wvhich arl explained and exemplified in M ason's Supplement to this work. 262. The leadling particulars respecting an ]eIEPwSI.: oF TIM}

/ 346
Pages

Actions

file_download Download Options Download this page PDF - Pages 153-157 Image - Page 153 Plain Text - Page 153

About this Item

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 153
Publication
New York,: Collins & brother,
1865.
Subject terms
Astronomy

Technical Details

Link to this Item
https://name.umdl.umich.edu/ajn0587.0001.001
Link to this scan
https://quod.lib.umich.edu/m/moa/ajn0587.0001.001/171

Rights and Permissions

These pages may be freely searched and displayed. Permission must be received for subsequent distribution in print or electronically. Please go to http://www.umdl.umich.edu/ for more information.

Manifest
https://quod.lib.umich.edu/cgi/t/text/api/manifest/moa:ajn0587.0001.001

Cite this Item

Full citation
"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.
Do you have questions about this content? Need to report a problem? Please contact us.