James Bradley (September 1692?-July 13, 1762)

James Bradley was the third Royal Astronomer. His date of borth is uncertain, but there is a baptism document of October 3, 1792 (see e.g. Wikipedia); this gives evidence for his birth in September 1792. School and college education provided him with the degrees of a Bachelor of Arts and a Master of Arts, and proceeded to a short ecclesial career as a vicar. Besides, he started astronomical observing with his uncle, James Pound, a skilled astronomer; their joint observations included the opposition of Mars in 1719, the transit of Mercury of October 29, 1723, and measurements of double star Gamma Virginis. Bradley was elected a Fellow of the Royal Society in 1718, resigned from his ecclesial duties in 1721, and was appointed as astronomer in Oxford, to the Savilian Chair of Astronomy. In 1742, he succeeded Edmond Halley as third Astronomer Royal, a post held for the rest of his life. He retired in 1761 and died on July 13, 1762.

His most fundamental discoveries were that of the aberration of light (1725-1728) from observations of Gamma Draconis, and the nutation of the Earth's axis (1728-1748).

Bradley discovered M48 and observed M41, both on February 16, 1727. These observations, noted as "Nebulous Stars," were noted in his observation notes, but not immediately published, and thus unnoticed. Only over a century later, in 1832, Rigaud published a clollection of Bradley's work Bradley and Rigaud (1832), which still was not widely recognized.

Bradley's descriptions are printed in under "Astronomical Observations, Miscellaneus Observations":

[M41]
16. 10h.1/2 a nebulos: about 4deg to the south of Sirius contiguous to a small star.
[M48]
Another [nebulous star] near the middle of an isosceles triangle formed by three stars, the brightest and northermost has two small ones contiguous, being in a line with it, the equal and longest sides of the triangle are about 5deg f[ollowing]. The stars lie almost in the midway between Procyon and Cor Hydrae.

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