<GetPassage xmlns:tei="http://www.tei-c.org/ns/1.0" xmlns="http://chs.harvard.edu/xmlns/cts">
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                <requestUrn>urn:cts:latinLit:stoa0023.stoa001.perseus-eng2:20.3.2-20.3.4</requestUrn>
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            <reply>
                <urn>urn:cts:latinLit:stoa0023.stoa001.perseus-eng2:20.3.2-20.3.4</urn>
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                    <TEI xmlns="http://www.tei-c.org/ns/1.0"><text><body><div xml:lang="lat" type="translation" n="urn:cts:latinLit:stoa0023.stoa001.perseus-eng2"><div type="textpart" subtype="book" n="20"><div type="textpart" subtype="chapter" n="3"><div type="textpart" subtype="section" n="2"><p>This phenomenon never takes place so clearly as when the moon, after its shifting courses,<note type="footnote" resp="editor">See note 2, p. 10, § 4, below.</note> brings back its monthly journey to the same starting-point after fixed intervals of time; that is to say, when the entire moon,<note type="footnote" resp="editor">I.e. the full moon; cf. § 7, below.</note> in the abode of the same sign of the zodiac, is found in a perfectly straight line directly under the sun, and for a brief time stands still in the minute points which the science of geometry calls parts of parts.<note type="footnote" resp="editor">I.e. parts of degrees, or minutes; cf. Pliny, <title rend="italic">N.H.</title> ii. 48, <foreign xml:lang="lat" rend="italic">scripulis partium.</foreign> </note></p></div><div type="textpart" subtype="section" n="3"><p>And although the revolutions and movements of both heavenly bodies, as the searchers<note type="footnote" resp="editor">The natural philosophers.</note> for intelligible causes had observed, after the course of the moon is completed,<note type="footnote" resp="editor">At the end of each lunar month.</note> meet at one and the same point always at the same distance from each other,<note type="footnote" resp="editor">I.e. are in conjunction.</note> yet the sun is not always eclipsed at such times, but only when the moon (by a kind of fiery plumb-line)<note type="footnote" resp="editor">According to Clark’s punctuation, based upon metrical <foreign xml:lang="lat" rend="italic">clausulae</foreign> (Introd., p. xxii); but <foreign xml:lang="lat" rend="italic">igneo</foreign> seems to be more naturally taken with <foreign xml:lang="lat" rend="italic">orbi.</foreign> </note> is directly opposite the sun and interposed between its orb and our vision.</p></div><div type="textpart" subtype="section" n="4"><p>In short, the sun is hidden and his brightness suppressed, when he himself and the orb of the moon, the lowest of all the heavenly bodies, accompanying <pb n="v2.p.11"/> each other and each keeping its proper course, maintaining the relation of height between them and being in conjunction, as Ptolemy wisely and elegantly expresses it<note type="footnote" resp="editor"><foreign xml:lang="grc">μαθνηατικὴ σύνταξις,</foreign> vi. 6.</note> have come to the points which in Greek we call <foreign xml:lang="grc">ἀναβιβάζοντας</foreign> and <foreign xml:lang="grc">καταβιβάζοντας</foreign> <foreign xml:lang="grc">ἐκλειπτικοὶ σύνδεσμοι</foreign><note type="footnote" resp="editor"><q>Ascending and descending ecliptic nodes.</q> The moon in its course shifts from one side to the other of the ecliptic, or sun’s course (see § 2, above). The nodes are the points where the moon passes the ecliptic; the node where she passes from the south to the north side is called <q>ascending,</q> that where she changes from north to south, <q>descending.</q> </note> (that is, eclipse nodes). And if they merely graze the spaces adjacent to these nodes, the eclipse will be partial.</p></div></div></div></div></body></text></TEI>
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