2000 HSS/PSA Program 1 - History of Science Society
2000 HSS/PSA Program 1 - History of Science Society
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