Page:Dictionary of National Biography volume 55.djvu/27

This page has been proofread, but needs to be validated.

desert of Tharr the absence of materials for building the necessary platforms, besides the need of providing a commissariat for two hundred men, taxed all the leader's resources. The triangulation of the section was completed on 22 April 1853. The series was 668 miles long, consisting of 173 principal triangles, and covering an area of 20,323 miles. After this work was ended, Strange joined the surveyor-general (Sir Andrew Scott Waugh [q. v.]) at his camp at Attock, and took part in measuring a verificatory base-line. He then bore the designation of ‘astronomical assistant.’ In 1855 he joined the surveyor-general's headquarters office, and in 1856 was placed in charge of the triangulation southwards from Calcutta to Madras, along the east coast. In 1859 he was promoted to the rank of major, and, in accordance with the regulations, retired from the survey. He received the special thanks of the government of India.

Returning home in January 1861, Strange retired from the army in December of the same year with the rank of lieutenant-colonel. As soon as he settled in England he persuaded the Indian government to establish a department for the inspection of scientific instruments for use in India, and was appointed to organise it, and to the office of inspector in 1862. Hitherto the system followed by the government in supervising the construction of scientific instruments for official use had been to keep a stock of patterns, invite tenders for copying them, and accept the lowest, thus preventing any chance of improvement in the type of instrument, and affording no guarantee for good workmanship or material. Strange abolished the patterns, encouraged invention, insured competition as to price by employing at least two makers for each class of instrument, and enforced strict supervision; a marked improvement in design and workmanship was soon evident, and the cost of the establishment was shown in his first decennial report to be only about .028 of one per cent. of the outlay on the works which the instruments were employed in designing or executing. For the trigonometrical survey he himself designed and superintended the construction of a set of massive standard instruments of the highest geodetic importance, viz. a great theodolite with a horizontal circle of three feet diameter, and a vertical circle of two feet diameter (these circles were read by means of micrometer microscopes); two zenith-sectors with arc of eighteen inch radius and telescope of four feet focal length; two five-feet transit instruments for the determination of longitude, with special arrangements for detecting flexure of the telescope; with others, which all exhibited very ingenious and important developments from previously accepted types.

Strange was elected a fellow of the Royal Geographical and Astronomical societies in 1861, and of the Royal Society on 2 June 1864. He took an active part in their proceedings. He served on the council of the Astronomical Society from 1863 to 1867, and as foreign secretary from 1868 to 1873. He contributed several papers to the society's ‘Memoirs’ (vol. xxxi.) and ‘Monthly Notices.’ In 1862 (Monthly Notices of Royal Astronomical Society, vol. xxiii.), he recommended the use of aluminium bronze in the construction of philosophical instruments. He was on the council of the Royal Society from 1867 to 1869. A lover of science for its own sake, he long preached the duty of government to support scientific research, especially in directions where discovery, though enriching the community, brings no benefit to the inventor. To this advocacy was mainly due the appointment in 1870 of the royal commission on this question (presided over by the Duke of Devonshire), which adopted and recommended many of his suggestions.

At the British Association at Belfast in 1874 he read a paper, which attracted much attention, on the desirability of daily systematic observations, preferably in India, of the sun as the chief source of cosmical meteorological phenomena.

Strange died in London on 9 March 1876. He married Adelaide, daughter of the Rev. William Davies, and left issue.

[Nature, xiii. 408–9; Times, 20 March 1876; Monthly Notices of Royal Astronomical Society, vol. xxxvii. No. 4; Markham's Memoirs on the Indian Surveys, 2nd ed. 1878.]

C. T.

STRANGE, Sir JOHN (1696–1754), master of the rolls, son and heir of John Strange of Fleet Street, London, was born in 1696, and was for some time a pupil of Mr. Salkeld of Brooke Street, Holborn, the attorney, in whose office Robert, viscount Jocelyn (lord chancellor of Ireland), Philip, earl of Hardwicke (lord chancellor of England), and Sir Thomas Parker (lord chief baron) all received their legal education. Strange used to carry his master's bag down to Westminster, and he witnessed Sir Joseph Jekyll's first appearance as master of the rolls in 1717, little dreaming ‘that he should have the option of being Sir Joseph Jekyll's immediate successor, and should actually fill the office eventually’ (Harris, Life of Lord