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Aristarkh Belopolsky

From Wikipedia, the free encyclopedia
Russian astronomer (1854–1934)
"Belopol'skiy" redirects here. For the lunar crater, seeBelopol'skiy (crater).
In this name that followsEast Slavic naming customs, thepatronymic is Apollonovich and thefamily name is Belopolsky.
Aristarkh Belopolsky
Аристарх Белопольский
Born(1854-07-01)July 1, 1854
DiedMay 16, 1934(1934-05-16) (aged 79)
EducationAcademician
Alma materImperial Moscow University (1840)
Scientific career
FieldsAstronomy
InstitutionsPulkovo Observatory

Aristarkh Apollonovich Belopolsky (Аристарх Аполлонович Белопольский; July 13 [O.S. July 1] 1854 – 16 May 1934) was a Russian and later Sovietastronomer. He was born inMoscow but his father's ancestors are from aSerbian town called Belo Polje.[1]Adjunct professor since 1900, extraordinary (1903) and ordinary (1906)academician of theImperial Academy of Sciences.

Life

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Belopolsky got his degree atMoscow University in 1876, and in 1878, he became the assistant toFyodor Aleksandrovich Bredikhin atMoscow Observatory. In 1888, he joined the staff ofPulkovo Observatory.

He worked inspectroscopy and discovered a number ofspectroscopic binaries. Among others, he discovered thatCastor B was a spectroscopic binary with a period of 2.92 days.

Belopolsky was known for his fine instrument making, and in 1900 he built an apparatus with which he managed to experimentally detect Doppler shift of light reflected from a moving object.[2] This was a breakthrough, since before this experiment the possibility of Doppler shift in light - as opposed to matter waves like sound - was still a controversial matter.[3] He pioneered the use of optical Doppler shift to measure the rotational rates of distant objects. He was the first to discover that the equator of Jupiter rotates more rapidly than higher latitudes, and that the rings of Saturn do not rotate as a solid mass, proving that they were made up of individual small objects.

He attempted twice to measure the rotational rate of Venus, suggesting 24 hours in 1900 and 35 hours in 1911—one of countless unsuccessful attempts by astronomers of that time to measure the length of the Venusian day.[4]

He was a good friend ofOskar Backlund, and when the latter died in 1916, he succeeded him as director of Pulkovo Observatory. However he resigned in 1918, because he did not like the administrative burden.

The craterBelopol'skiy on theMoon, the asteroid1004 Belopolskya andan award of theRussian Academy of Sciences are named after him.

Belopolsky at the Fourth Conference International Union for Cooperation in Solar Research atMount Wilson Observatory, 1910

References

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  1. ^Hockey, Thomas (2009).The Biographical Encyclopedia of Astronomers.Springer Publishing.ISBN 978-0-387-31022-0. RetrievedAugust 22, 2012.
  2. ^Belopolsky, Aristarh (1901). "On an apparatus for the laboratory demonstratian of the Doppler-Fizeau principle".Astrophysical Journal.13: 15.Bibcode:1901ApJ....13...15B.doi:10.1086/140786.
  3. ^Nolte, David D. (2020)."The fall and rise of the Doppler effect".Physics Today.73 (3):30–35.doi:10.1063/PT.3.4429.
  4. ^"Аристарх Аполлонович Белопольский — Bourabai Research". Archived fromthe original on 2011-07-22. Retrieved2010-04-30.

Bibliography

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  • Imperial Moscow University: 1755-1917: encyclopedic dictionary. Moscow: Russian political encyclopedia (ROSSPEN). 2010. pp. 61–63.ISBN 978-5-8243-1429-8 – via A. Andreev, D. Tsygankov.

External links

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