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]).