1 The Birth of Science - MSRI
1 The Birth of Science - MSRI
1 The Birth of Science - MSRI
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78 3. Other Hellenistic Scientific <strong>The</strong>ories<br />
the sphere <strong>of</strong> the fixed stars loses its function. It is not an accident that<br />
both Aristotle and Ptolemy, who believed in the earth’s immobility, also<br />
believed in a rigid sidereal sphere, and that the first person to challenge<br />
the notion <strong>of</strong> that sphere was apparently the same who first asserted that<br />
the earth rotates — Heraclides <strong>of</strong> Pontus, who maintained that the universe<br />
is infinite and that every celestial body is a world in itself (and even<br />
has its own atmosphere). 118 An interesting argument in favor <strong>of</strong> an infinite<br />
universe is reported by Lucretius. 119<br />
Aristarchan heliocentrism brought to bear a new argument that increased page 115<br />
enormously the traditional dimensions <strong>of</strong> the cosmos. <strong>The</strong> supporters <strong>of</strong><br />
heliocentrism, indeed, had to explain why ever our motion around the<br />
sun causes no observable parallax effects — that is, why the appearance<br />
<strong>of</strong> the constellations does not change as our vantage point moves relative<br />
to them throughout the year. According to Archimedes, Aristarchus overcame<br />
that objection by assuming that the radius <strong>of</strong> the earth’s orbit is to the<br />
radius <strong>of</strong> the sphere <strong>of</strong> fixed stars as a sphere’s center is to its radius. This<br />
wording, which appears more or less unchanged in Geminus, Cleomedes,<br />
Ptolemy and other authors, 120 is criticized by Archimedes, who says that<br />
the ratio between two lengths is necessarily nonzero. 121<br />
This issue calls perhaps for a mathematical parenthesis. <strong>The</strong> aim <strong>of</strong> the<br />
Arenarius may have been precisely to defend the “Archimedean postulate”<br />
(see page 45 in Section 2.7), by showing that one can assign a finite,<br />
nonzero ratio to any two nonzero lengths (or other homogeneous magnitudes).<br />
To accomplish this it was necessary to work out a numbering<br />
system able to express even the largest imaginable ratio between homogeneous<br />
magnitudes, such as the ratio between the volume <strong>of</strong> the sidereal<br />
sphere and that <strong>of</strong> a grain <strong>of</strong> sand; this is what Archimedes does in his<br />
tract. <strong>The</strong> triumph <strong>of</strong> Archimedes’ views on commensurability took away<br />
the rationale for the task undertaken in the Arenarius and rendered the<br />
work hard to understand (it has always been felt to be strange). Obviously,<br />
what Aristarchus (and the other authors mentioned) intended in<br />
saying that two lengths are in the same ratio as a point is to a circumfer-<br />
118 [DG], 328b, 4–6; 343, 15. <strong>The</strong> same opinions were attributed by Aetius also to “Pythagoreans”;<br />
these may have been the same Pythagoreans, such as Hicetas and Ecphantus (page 74), who<br />
asserted that the earth moves.<br />
119 Lucretius states that if the universe were finite, all masses would already be concentrated in its<br />
center. Thus he supposes that gravity affects all bodies, not just “heavy” ones (Lucretius, De rerum<br />
natura, I, 984–997).<br />
120 For example, Geminus, Eisagoge eis ta phainomena, XVII, 16; Cleomedes, Caelestia, I, 8, 1–5 (ed.<br />
Todd); Ptolemy, Almagest, V, xi, 401, 22–402, 1. Aristarchus likewise postulates that the ratio between<br />
the earth and the orbit <strong>of</strong> the moon is equal to the ratio between a point and a circumference<br />
(On the sizes and distances <strong>of</strong> the sun and moon, hypothesis 2 = [Heath: Aristarchus], p. 352).<br />
121 Arenarius, 135, 19–22 (ed. Mugler, vol. II).<br />
Revision: 1.13 Date: 2002/10/16 19:04:00