IGY and the Antarctic Treaty

The development of IGY

The idea for more frequent programs was born in 1950, when it was proposed that scientists take advantage of increasing technological developments, interest in polar regions, and, not the least, the maximum sunspot activity expected in 1957–58. (The earlier, second polar year was a year of sunspot minimum.) As a vast intelligence gathering exercise, the idea also had covert political support. What was then called the International Council of Scientific Unions (ICSU; known as the International Science Council [ISC] as of July 2018) adopted the proposal, and in 1952 ICSU appointed a committee that was to become known as the Comité Spécial de l’Année Géophysique Internationale (CSAGI) to coordinate IGY planning. Plans widened to include the scientific study of the whole Earth, and eventually 67 nations showed interest in joining. Plans were laid for simultaneous observations, at all angles, of the Sun, weather, the aurora, the magnetic field, the ionosphere, and cosmic rays. An ICSU committee meeting in Rome in 1954 especially emphasized two programs, outer space and Antarctica. Whereas in the first polar year observations were confined to ground level and in the second to about 33,000 feet by balloon, IGY saw the Soviet Union launch the first artificial satellite Sputnik in 1957, an event that triggered the “space race” between the Soviet Union and the United States and started a new era in space exploration. Several international data centres were established to collect all observations and make them freely available for analysis to scientists of any nation.

Antarctica was emphasized because very few geophysical studies had yet been made on the continent, because the south geomagnetic pole focuses auroral and cosmic-ray activity in the Southern Hemisphere, and because on the eve of IGY almost half the continent had not yet even been seen by humans. The First Antarctic Conference was held in Paris in July 1955 to coordinate plans for expeditions, the advance parties of which were soon to set sail for the continent. Early tensions, due in part to overlapping political claims on the continent, were relaxed by the conference president’s statement that overall aims were to be entirely scientific. Plans were laid for extensive explorations: 12 nations were to establish more than 50 overwintering stations on the continent and sub-Antarctic islands; the first regular aircraft flights to the continent were to be inaugurated (by the United States); massive tractor traverses were to be run in order to establish inland stations in West Antarctica (Byrd Station for the United States), at the south geomagnetic pole (Vostok Station for the Soviet Union), and the pole of relative inaccessibility—that is, the point on the continent most remote from all coasts (at 82°06′ S, 54°58′ E)—which was first reached by the Soviets, on December 14, 1958; and an airlift by giant cargo aircraft was to be established in order to set up a station at the South Pole itself (Amundsen-Scott Station for the United States). Several major scientific programs were scheduled for Antarctica, dealing with the aurora and airglow, cosmic rays, geomagnetism, glaciology, gravity measurement, ionospheric physics, meteorology, oceanography, and seismology. Biology and geology were not primary studies of IGY.

Coastal bases were established in the summer of 1955–56 and inland stations the next summer for the official opening of IGY on July 1, 1957. For 18 months, until the end of IGY on December 31, 1958, a frenzy of activity not only in Antarctica but also all over the world and in space resulted in a multitude of discoveries that revolutionized concepts of Earth and its oceans, landmasses, glaciers, atmosphere, and gravitational and geomagnetic fields. The combination of a moratorium on territorial claims and the cooperative interchange between scientists of different nations during IGY also demonstrated that, as one historian put it, in Antarctica “science may be seen as a continuation of politics by other means.”