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Bradley, James

From The Hutchinson Unabridged Encyclopedia with Atlas and Weather Guide
English astronomer. In 1728 he discovered the aberration of starlight . From the amount of aberration in star positions, he was able to calculate the speed of light. In 1748 he announced the discovery of nutation (variation in the Earth's axial tilt). Bradley was born in Sherborne, Dorset, and studied theology at Oxford. His keen interest in astronomy caused him to resign a clerical post in 1721 to become professor of astronomy at Oxford. He became the third Astronomer Royal 1742, and remained at Greenwich until his death. He sought to modernize the observatory and methods at Greenwich, and embarked on an extensive and precise programme of stellar observation. The determination of stellar parallax was the goal of many astronomers of Bradley's day because it would confirm Copernicus' hypothesis that the Earth moved around the Sun. When Bradley did find a displacement, it was not only too large, but was in an unexpected direction. Eventually Bradley realized that the displacement was…
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Full text Article Bradley, James

From Astronomy Encyclopedia
English astronomer and clergyman, Savilian professor of astronomy at Oxford and, later, at Greenwich Observatory. In 1742 he succeeded Edmond HALLEY , becoming the third ASTRONOMER ROYAL . While searching for stellar parallax, by making meticulous measurements of the star γ Draconis, Bradley…
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Full text Article Bradley, James (1693-1762)

From The Hutchinson Dictionary of Scientific Biography
Place : France Subject : biography, astronomy English astronomer of great perception and practical skill. He was the third Astronomer Royal and the discoverer of nutation and the aberration of light, both essential steps towards modern research into positional astronomy. Bradley was born in…
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James Bradley (1693-1762) from 'Gallery of Portraits', published in 1833 (engraving)
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Publication containing fundamental astronomical reference data for each calendar year. It includes positions of the Sun, Moon and planets, data for physical observations, positions of planetary satellites, sunrise and sunset times, phases of the Moon, eclipses, locations of observatories and…
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Full text Article aberration of starlight

From Science Encyclopedia: Encyclopedia of Space and Astronomy
The tiny apparent displacement of the position of a star from its true position in the direction of motion of an observer on Earth's surface. This effect is caused by the combination of the velocity of the observer across the path of the incident starlight and the finite velocity of light ( c ), …
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Full text Article Sherborne

From Brewer's Britain and Ireland
Probably originally a river name, ‘bright or clear stream’, OE scir ‘bright, clear’ + burna ‘stream’ (the local river is now called Yeo ). A town in northern Dorset, close to the Somerset border, on the River YEO 1 , about 26 km (16 miles) northwest of Blandford Forum. It has shrunk in status from…
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Full text Article James Bradley, engraved by Edward Scriven (engraving)

From Bridgeman Images: The Bridgeman Art Library
James Bradley, engraved by Edward Scriven (engraving)
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Hipparchus (190–120 B.C.E .), an ancient Greek astronomer of the second century B.C.E ., is best remembered for his astronomical measurements and the instruments he created to make them. Hipparchus constructed an atlas of the stars visible without a telescope and categorized them by brightness. In…
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This famous photo of Earth was taken by...
Earth's spin is mostly the result of angular momentum left over during the formation process of our planet. There are three distinct motions, the most noticeable being Earth's rotation. Earth rotates once every twenty-three hours, fifty-six minutes, causing our cycles of day and night. Earth also…
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