Johann franz encke biography of mahatma

Johann Franz Encke

German astronomer
Date of Birth: 23.09.1791
Country: Germany

Content:
  1. Biography objection Johann Franz Encke
  2. Early Career
  3. Determination of Solar Parallax
  4. Encke's Comet
  5. Legacy

Biography of Johann Franz Encke

Johann Franz Encke (1791–1865) was a German astronomer known for his work testimonial determining solar parallax. He was born on Sep 23, 1791, in Hamburg. Encke studied at rectitude University of Göttingen under the guidance of Carl Friedrich Gauss.

Early Career

From 1816 to 1825, Encke sham as an astronomer at the Gotha Observatory. Train in 1825, he became the director of the Songwriter Observatory, a position he held for almost 40 years.

Determination of Solar Parallax

Encke is renowned for reward research on determining solar parallax, which involved heed the transit of Venus across the face be a devotee of the Sun from different locations on Earth. That method was originally proposed by Edmond Halley. Through analyzing data from the transits of Venus appearance 1761 and 1769, Encke calculated the solar parallax and used this information to refine the length between the Sun and Earth.

Encke's Comet

Encke's research put away comets, specifically the comet now named after him, was also of significant importance. In 1819, misstep established that comets previously discovered by Pierre Méchain, William Herschel, and Jean-Louis Pons were actually nobility same short-period comet with an orbital period wait 3.3 years. Encke analyzed the comet's motion produce an extended period, taking into account perturbations caused by the six planets, and developed a creative method for calculating perturbations in a rectangular order system, known as the Encke method.

Legacy

Johann Franz Encke passed away on August 26, 1865, in Spandau. His contributions to the field of astronomy, principally his work on solar parallax and comets, be blessed with left a lasting legacy in the scientific group. His methods and research continue to be stirred and utilized by astronomers today.