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2000 HSS/PSA Program 1 - History of Science Society

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<strong>HSS</strong> Abstracts<br />

the map projection, the mathematical graticule, betray the impossibility <strong>of</strong><br />

any transcendental orientation before or outside <strong>of</strong> experience? This proposition<br />

will be examined with respect to theories <strong>of</strong> map projection and the survey <strong>of</strong><br />

Hanover organized by Tobias Mayer and Georg Lichtenberg at Göttingen Georg<br />

Forster’s Göttingen-based compilations <strong>of</strong> travel literature his essay on “Cook<br />

der Entdecker” and his debate with Kant over the authority <strong>of</strong> travellers’ reports.<br />

David␣ H. DeVorkin Smithsonian Institution National Air and Space Museum<br />

Bringing Theory to Mount Wilson in the 1920s<br />

When George Ellery Hale established his Mount Wilson Solar Observatory in<br />

1904, his primary intellectual goal was to build a staff <strong>of</strong> astrophysicists fully<br />

acquainted with the latest developments and methodologies in physics. Over<br />

the next decade, as he built the two successively largest telescopes in the world,<br />

Hale remained firm in his conviction, but failed time and again to attract strong<br />

physics to his isolated Mount Wilson telescopes and laboratories in Pasadena.<br />

With the establishment in 1919 <strong>of</strong> the NRC postdoctoral fellowship program<br />

for physics and chemistry, and then in 1924 <strong>of</strong> the International Education<br />

Board (IEB) fellowships, all fuelled by Rockefeller money, a mechanism was<br />

in place to attract the best young theorists to Pasadena, where Hale had also<br />

transformed a small technical school into the California Institute <strong>of</strong> Technology<br />

and placed it in the hands <strong>of</strong> Robert A. Millikan. Thus what Hale set into<br />

motion for largely astrophysical motives resulted in the creation <strong>of</strong> a major<br />

new center for pure physics, where leading European physical theorists would<br />

visit, and send their students, to gain access to the best astrophysical data in<br />

the world. Here I discuss the impact upon Mount Wilson and upon theoretical<br />

astrophysics resulting from the residencies <strong>of</strong> European theorists, specifically<br />

Svein Rosseland, a student <strong>of</strong> Bohr, and Albrecht Unsöld, a student <strong>of</strong><br />

Sommerfeld, in the 1920s.<br />

72<br />

Nicholas Dew Cambridge University<br />

The Menagerie <strong>of</strong> Versailles and the Visualisation <strong>of</strong> Nature<br />

The project to rebuild the palace <strong>of</strong> Versailles got under way in the 1660s,<br />

and even before the court had arrived, the gardens were stocked with exotic<br />

birds and animals. The menagerie <strong>of</strong> Versailles presents a striking example<br />

<strong>of</strong> the marriage <strong>of</strong> ‘curiosity’ and ‘magnificence’, or the ways in which the<br />

practice <strong>of</strong> natural investigation in seventeenth-century Europe could pr<strong>of</strong>it<br />

from the spectacular culture <strong>of</strong> the princely court. The animals at the<br />

menagerie were dissected by members <strong>of</strong> the Académie royale des sciences<br />

and thereby became the stars <strong>of</strong> the sumptuous Memoires pour servir à

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