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His main work was in mathematical physics. In his study of the shape of the Earth he used the idea of minimising the sum of the absolute values of the deviations. His solution to this minimising problem took a geometric form. Boscovich was the first to give a procedure to compute a planet's orbit from 3 observations of its position and he also gave a procedure for determining the equator of a planet from 3 observations of a surface feature.
Boscovich became professor of mathematics at Pavia in 1764 and was director of Brera Observatory. He led an expedition to California in 1769 to observe a transit of Venus. From 1773 to 1783 he worked in Paris.
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