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Mrkos
Mrkos may refer to: * Antonín Mrkos (1918, Střemchoví, Dolní Loučky Dolní Loučky is a municipality and village in Brno-Country District in the South Moravian Region of the Czech Republic. It has about 1,300 inhabitants. Dolní Loučky lies approximately north-west of Brno and south-east of Prague. Administrat ... - 1996), a Czech astronomer ** 143P/Kowal-Mrkos, a periodic comet ** 18D/Perrine-Mrkos, a periodic comet ** 1832 Mrkos (provisional designation 1969 PC), an outer main belt asteroid discovered in 1969 by L. Chernykh ** 45P/Honda-Mrkos-Pajdušáková, a periodic comet discovered on 1948 ** Comet Mrkos (other) {{surname, Mrkos, Mrkosová Czech-language surnames ...
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Antonín Mrkos
Antonín Mrkos () (27 January 1918 – 29 May 1996) was a Czech astronomer. Biography Mrkos entered the University in Brno in 1938. His studies were interrupted by the onset of World War II, and in 1945 he became a staff member at the Skalnaté Pleso Observatory in Czechoslovakia (now in Slovakia). It was from here that he carried out his extremely active cometary programme and became the discoverer of several unusual comets, the most famous of them the bright Comet 1957d. He was the second Czech in Antarctica and the first Czechoslovak to reach the Southern Pole of Inaccessibility as a member of the 3rd Soviet Antarctic Expedition (1957–1959). The Czechoslovak flag was the second flag raised after the flag of the USSR. He returned to Antarctica as the head of the four-member Czechoslovak crew in the seventh Soviet Antarctic Expedition (1961–1963). He was studying auroras among other things.
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1832 Mrkos
1832 Mrkos, provisional designation , is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 30 kilometers in diameter. It was discovered on 11 August 1969 by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. It was named after Czech astronomer Antonín Mrkos. Orbit and classification The C-type asteroid orbits the Sun in the outer main-belt at a distance of 2.9–3.5  AU once every 5 years and 9 months (2,104 days). Its orbit has an eccentricity of 0.10 and an inclination of 15 ° with respect to the ecliptic. ''Mrkos'' was first observed and identified as at Yerkes Observatory in 1937, extending the body's observation arc by 32 years prior to its official discovery observation. Physical characteristics Rotation period In October 2004, a rotational lightcurve for ''Mrkos'' was obtained from photometric observations taken by American astronomer Brian D. Warner, Brian W ...
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