Plutarch De Facie Quae in orbe Lunae Apparet 20

Harold Cherniss (Translator), William C. Helmbold (Translator)

De Facie Quae in orbe Lunae Apparet. Plutarch. Harold Cherniss (Translator), William C. Helmbold (Translator). Cambridge, MA. 1957.

Sponsored by Perseus Project, Tufts University.

Funding provided by The National Endowment for the Humanities.

Current edition Perseus

Concerning the Face which Appears in the Orb Of the Moon (English) (Plutarch. Moralia, Vol. XII. Cherniss, Harold and William Clark Helmbold translators. Cambridge, MA: Harvard University Press; London: William Heinemann Ltd., 1957 (printing).)

Editions (1)
Περὶ τοῦ ἐμφαινομένου προσώπου τῷ κύκλῳ τῆς σελήνης Perseus (Plutarch. Plutarchi Chaeronensis Moralia, Vol. V. Vernardakēs, Grēgorios N., editor. Leipzig: Teubner, 1893.) — 20 focus
Translations (1)
Of the Face Appearing Within the Orb Of the Moon Perseus (Plutarch. Plutarch's Morals, Vol. V. Goodwin, William W., editor; G., A., translator. Boston: Little, Brown, and Company; Cambridge: Press of John Wilson and Son, 1874.) — 20 focus

Notes on the current edition

Concerning the Face which Appears in the Orb Of the Moon

1. The argument that the moon is earthy, which at the beginning of chap. 19 (931 D) Lucius stated in the form of a proportion.
2. cf. Cleomedes, ii. 6. 115 (p. 208. 9-12 [Ziegler]) for the eclipse of the moon and ii. 4. 106 (p. 192, 14-20) for the eclipse of the sun; cf. also Theon of Smyrna, p. 193. 23 ff, and p. 197. 22 ff. (Hiller); Geminus, viii. 14 (p. 104. 23 ff. [Manitius]).
3. See notes a and b on 923 B supra.
4. cf. Cleomedes, ii. 6. 118 (p. 214. 2-12 [Ziegler]); Aristotle, Caelo, 297 B 23-30.
5. i.e. the intersecting lines are always arcs of a circle because the degree of curvature of each of the two surfaces is at every point similar. For this interpretation cf Class. Phil. xlvi (1951), p. 144.
6. cf. Class. Phil. xlvi (1951), p. 144; Cleomedes, ii. 6. 116 (p. 210. 6-19 [Ziegler]), 117 (p. 212. 1-12) on the lunar eclipse; ii. 5. 113-114 (p. 204. 27 ff.) on the solar eclipse; Geminus, xii. 5-13 (pp. 138-140 [Manitius]) on the eastward motion of sun and moon.
7. cf. Communibus Notitiis, 1080 B : αὐταὶ γάρ δήπουθεν αἱ τῶν κωνικῶν τμημάτων ἐπιφάνειαι. κύκλοι εἰσίν.
8. cf. Cleomedes, ii. 6. 119 (pp. 214. 13-216. 8 [Ziegler]); for the observation that the planets appear to move most swiftly when they are nearest to the earth and most slowly when they are farthest away cf. Cleomedes, ii. 5. 112-114 (pp. 202. 26-206. 27), and Theon of Smyrna, p. 135. 6-11 and p. 157. 2-12 (Hiller). Plutarch’s language, however, implies that the moon makes a conscious exertion to accelerate her motion when she is near the earth, and in the myth at 944 A s.v. it is stated that she increases her speed in order to escape the shadow of the earth. Kepler in note 51 to his translation declares that, contrary to what Lucius here says, perigee eclipses even when central are briefer than apogee eclipses; and Prickard ( Plutarch on the Face of the Moon [1911], p. 11) says that ceteris paribus an eclipse of a distant moon should be longer by about one fifteenth. Prof. Neugebauer informs me that, using the Ptolemaic figures for the apparent diameter of the moon and of the earth’s shadowand the classical figures given by Geminus for the velocity, the maximum totality in apogee should be 4; 3, 23ʰʳ and in perigee 3; 20, 0ʰʳ.
9. Probably a reference to such matters as are discussed by Geminus, ix (pp, 124-130 [Manitius]), With τὰς φάσεις καὶ διαφορήσεις cf. species diversitatesque Lunae, Martianus Capella, viii. 871 (p. 459. 15-16 [Dick]).
10. It is impossible to give an exhaustive and accurately scientific explanation of physical phenomena, for they are involved in the indeterminateness of matter. cf. Aristotle, Anal. Post. 87 a 31-37 and Metaphysics, 995 A 14-17, 1078 A 9-13 ( cf. Zeller, Die Philosophie der Griechen, ii. 2, p. 166, n. 3); and for Plato’s more extreme attitude cf. especially Timaeus, 29 B - C, Philebus, 56 and 59. Plutarch appears to have Philebus, 56 C in mind at Quaest. Conviv 744 e-f, where he makes astronomy attendant upon geometry, as he has Philebus, 66 a-b in mind at 720 C ( cf. R. M. Jones, Class. Phil. vii [1912], pp. 76 f.). For the notion of the necessary lack of accuracy of the physical sciences cf. further Plat. Quaest. 1001 E ff. and Quaest. Conviv 699 B.
11. cf. note a on 932 D supra.
12. cf. Cleomedes, ii. 3. 99 (p. 180. 11-13 [Ziegler]) and ii. 6. 120-121 (p. 218. 2-3).
13. cf. Quomodo Adul. ab Amico Internosc. 57 C, Herodoti Malignitate, 863 E.
14. cf. Aristotle, Caelo, 305 A 9-13; [Alexander], Anima Libri Mantissa, p. 128. 2-7 (Bruns), and the explanation of the moon’s phases ascribed to Antiphon in Placitis, 891 D = Aëtius, ii. 28. 4 ( Dox. Graeci, p. 358).
15. See 928 D supra with note d there and 935 B s.v.. Reference to the present passage is omitted in S. V. F.
16. αἰθήρ is here used in the Stoic sense as in 922 B and 928 c-d supra.
17. For this period of 465 ecliptic full moons cf. Class. Phil. xlvi (1951), p. 145.
18. For this argument cf. Cleomedes, ii. 4. 103 (p. 182. 10-16 [Ziegler]).