138 chapter five
that by the next TOV scientists would finally be able to measure the astro-
nomical unit (Sheehan and Westfall 2004 ).
Halley’s plans required sending scientific expeditions to the far corners
of the earth to observe the TOV. All this effort could be thwarted by a
few cloudy hours. A missed opportunity could result in more than a cen-
tury of delay before the next transit offered another chance to calculate
the astronomical unit. Increasing the number of expeditions improved the
probability of having successful observations. This opened the door to
international competition: Which country would support the largest num-
bers of expeditions to the most distant and inhospitable locations? Which
country would be the first to solve “the noblest problem in astronomy”?
The calculation of the astronomical unit is an example of pure basic
research. Within the context of the eighteenth and nineteenth centuries,
such measurement had no technological implications. A Times editorial
(September 22 , 1883 ) states this point explicitly.
The determination of the precise distance which separates the sun from the
earth would be an achievement which nearly every one would admit to be sur-
prising, but which would scarcely impress the mind of the average man with
the idea of eminent practical utility.... The business therefore is one which
States alone can undertake, and probably all the principal civilized nations of
the world will take their share in it.