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Samuel Foster

From Wikipedia, the free encyclopedia

Samuel Foster (c. 1600 – July 1652) was an English mathematician and astronomer. He made several observations of eclipses, both of the sun and moon, at Gresham College and in other places; and he was known particularly for inventing and improving planetary instruments.[1]

Life

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A native of Northamptonshire, he was admitted a sizar at Emmanuel College, Cambridge on 23 April 1616, as a member of which he proceeded B.A. in 1619, and M.A. in 1623.[2] On the death of Henry Gellibrand, he was elected Gresham Professor of Astronomy on 2 March 1636, but resigned later in the year and was succeeded by Mungo Murray. In 1641, Murray having vacated the professorship by his marriage, Foster was re-elected on 26 May.

During the civil war and Commonwealth he was one of the society of gentlemen who met in London for cultivating the 'new philosophy,' in the group around Charles Scarburgh. In 1646 John Wallis received from Foster a theorem on spherical triangles (two antipodal triangles, that is two triangles formed from corresponding antipodal vertices, are congruent) which he afterwards published in his Mechanica.[3] Wallis's retrospective account of the origins of the Royal Society made Foster's lectures a rendezvous of the London-based Scarburgh-Jonathan Goddard group; but it is disputed to what extent this connection was with Gresham College and its tradition, rather than simply the location.[4][5]

Foster died at Gresham College in May 1652, and was buried in the church of St. Peter the Poor in Broad Street.

Works

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He published little himself, but many treatises written by him were printed after his death, though John Twysden and Edmund Wingate, his editors, state that long illness caused them to be left very imperfect, and Twysden complains that some people had taken advantage of his liberality by publishing his works as their own (Preface to Foster's Miscellanies). In the following list of Foster's works, only the first two were published before his death:

Foster left numerous manuscript treatises in addition to those printed by his friends. Of these two were in the possession of William Jones, F.R.S.: The Uses of a General Quadrant, and Select Uses of the Quadrant, dated 1649.

Notes

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  1. ^ Frost 2006.
  2. ^ "Foster, Samuel (FSTR616S)". A Cambridge Alumni Database. University of Cambridge.
  3. ^ Wallis, John (1670). Mechanica (in Latin). Guliemi Godbid. p. 475, also plate 6, fig. 192. Exponatur jam, in superficie Sphaericâ, Tringulum Sphaericum ABD, circulorum Maximorum arcubus comprehensum. Qui quidem arcus continuati, intelligantut circulos integros absolvere. Hi Circuli cum sint in Sphaera maximi; se mutuo bisecabunt bini quilibet. Et, propter aequales angulos tum qui sunt oppositi verticales, tum qui sunt in eodem Bilineo oppositi, (puta A=α, & a = a, & sic ubique;) aequalia invincem erunt quae sunt in contrariis Hemisphaeriis Bilinea, (eorundem Circulorum contrariis Semicirculis interjecta;) puta αα, & (quod, in Schemate disruptum est & replicatum, set in Sphaerâ continuari intelligendum est,) AA; & similiter BB, & ββ; item DD, & δδ. Sed &, eâdem ratione, Opposita Triangula ABD, αβδ, (propter Latera lateribus, & Angulos angulis, respective sumptis aequalia,) erunt invincem aequalia. (Quae est etiam Samuelis Fosteri nostratis demonstratio, in Collegio Greshamensi Londini Astronomiae non ita predem Professoris.)
  4. ^ Margery Purver, The Royal Society: Concept and Creation (1967), pp. 184–5.
  5. ^ Christopher Hill, Intellectual Origins of the English Revolution (1965), p. 100.

References

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