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Maximilianus Hell (1720-1792) - Munin

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II.1.4 above. However, prior to 1770 he seems not to have been engaged in any disputes with<br />

the man whom Jean-Claude Pecker characterises as “the most important French astronomer of<br />

the eighteenth century” – Lalande. 114 For all its fragmentary status, the epistolary evidence to<br />

hand suggests that <strong>Hell</strong> and Lalande remained close allies during the 1760s. That changed<br />

with Lalande’s reaction to the Vardø report.<br />

Around the year 1761, Father <strong>Hell</strong> and Lalande were both ‘shooting stars’ in the European<br />

Republic of Letters. Lalande waited impatiently behind the back of Delisle to become the<br />

main nodal astronomer on the international stage of contemporary astronomy. Father <strong>Hell</strong> was<br />

almost as ambitious, but Vienna was hardly any great power in matters of astronomy. As a<br />

nodal astronomer, <strong>Hell</strong>’s main ‘capital’ was Central Europe and its surroundings, along with<br />

certain Jesuit connections in China. It was from from these regions that he was able to<br />

assemble exclusive data sets and theoretical expositions for his Ephemerides.<br />

Lalande considered himself a nodal astronomer for more than France. In his own eyes at least,<br />

he was the world wide coordinator of the entire Venus transit enterprise. The first seed of<br />

discontent was probably sown when neither <strong>Hell</strong> nor Denmark-Norway asked for his advice<br />

in the planning of the Vardø expedition. But their independent behaviour went beyond that.<br />

The data sets from Vardø were not shared with Lalande immediately – he had to wait in line<br />

behind the Danish King, along with every astronomer except the few Copenhagen-based<br />

savants that attended oral presentations given in the sessions of the Danish Society of<br />

Sciences in November and December 1769 (see Section II.3.2). A third element that annoyed<br />

Lalande was the peculiar method in calculating the coordinates of Vardø, especially the pole<br />

height method described above. The fourth issue at stake was of course the conclusions drawn<br />

concerning the solar parallax itself. Unlike the previous occasion, Lalande and <strong>Hell</strong> disagreed<br />

fundamentally here. Instead of standing on the side-lines, the two stepped forward to become<br />

main characters in a heated scientific controversy.<br />

When calculating the solar parallax, contemporaneous astronomers could choose between two<br />

strategies. One option was to wait for all observations to be published and then undertake a<br />

thorough survey of all the available data. Ideally, such a survey would lead to a decisive<br />

conclusion, ‘the author’s final word’ on the matter. Another modus operandi was to make<br />

114 Pecker 2007, p. 3: “Lalande fut en effet sans doute le plus important astronome français du XVIII e siècle.”<br />

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