Chuhuiv Observational Station

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Chuhuiv Observational Station
Grakovo01.JPG
Dome of 70-cm telescope AZT-8
Organization Kharkiv National University
Observatory code 121 [1]
Location Chuhuiv Raion, Ukraine
Coordinates 49°38′34.6″N36°56′12.8″E / 49.642944°N 36.936889°E / 49.642944; 36.936889
Altitude156 m
Established1962  OOjs UI icon edit-ltr-progressive.svg
Website www.astron.kharkov.ua/grakovo/index.html
Telescopes
AZT-80.7 m reflector 
Reliefkarte Ukraine 2022.png
Red pog.svg
Location of Chuhuiv Observational Station
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Chuhuiv Observational Station (or Chuguev Observational Station) of the Institute of Astronomy of Kharkiv National University is an astronomical observatory founded in the early 1960s near the village of Ivanovka, Chuhuiv Raion, Kharkiv Oblast, Ukraine. The founder of the observatory was Nikolai P. Barabashov. [2] [3] The main instrument of the observatory is 70-cm reflector AZT-8. [4] The observational station hosted one of the first coherent optics processors used to reduce astronomical observations. [5] The main topics of the observations conducted on the observational station are photometric observations of asteroids and monitoring of space debris. In particular, the observations conducted here significantly contributed to the introduction of H-G1-G2 asteroid magnitude system [6] and to the discovery of the YORP effect for several asteroids [7] [8]

Related Research Articles

<span class="mw-page-title-main">1620 Geographos</span> Asteroid

1620 Geographos, provisional designation 1951 RA, is a highly elongated, stony asteroid, near-Earth object and potentially hazardous asteroid of the Apollo group, with a mean-diameter of approximately 2.5 km (1.6 mi). It was discovered on 14 September 1951, by astronomers Albert George Wilson and Rudolph Minkowski at the Palomar Observatory in California, United States. The asteroid was named in honor of the National Geographic Society.

<span class="mw-page-title-main">20 Massalia</span> Main-belt Massalian asteroid

Massalia, minor planet designation 20 Massalia, is a stony asteroid and the parent body of the Massalia family located in the inner region of the asteroid belt, approximately 145 kilometers in diameter. Discovered by Italian astronomer Annibale de Gasparis on 19 September 1852, it was named for the French city of Marseille, from which the independent discover Jean Chacornac sighted it the following night.

<span class="mw-page-title-main">YORP effect</span> Second-order variation on the Yarkovsky effect that changes the rotation rate of a small body

The Yarkovsky–O'Keefe–Radzievskii–Paddack effect, or YORP effect for short, changes the rotation state of a small astronomical body – that is, the body's spin rate and the obliquity of its pole(s) – due to the scattering of solar radiation off its surface and the emission of its own thermal radiation.

925 Alphonsina, provisional designation 1920 GM, is a stony Hansian asteroid from the central region of the asteroid belt, approximately 58 kilometers in diameter. It was discovered on 13 January 1920, by Catalan astronomer Josep Comas i Solà at the Fabra Observatory in Barcelona, Spain. The S-type asteroid has a rotation period of 7.88 hours. It was named for the Spanish Kings Alfonso X and Alfonso XIII.

<span class="mw-page-title-main">986 Amelia</span>

986 Amelia is a large background asteroid from the outer regions of the asteroid belt, approximately 50 kilometers in diameter. It was discovered on 19 October 1922, by Spanish astronomer Josep Comas i Solà at the Fabra Observatory in Barcelona. The L/D-type asteroid has a rotation period of 9.5 hours. It was named after the discoverer's wife, Amelia Solà.

<span class="mw-page-title-main">1627 Ivar</span>

1627 Ivar, provisional designation 1929 SH, is an elongated stony asteroid and near-Earth object of the Amor group, approximately 15×6×6 km. It was discovered on 25 September 1929, by Danish astronomer Ejnar Hertzsprung at Leiden Southern Station, annex to the Johannesburg Observatory in South Africa. It was named after Ivar Hertzsprung, brother of the discoverer. 1627 Ivar was the first asteroid to be imaged by radar, in July 1985 by the Arecibo Observatory.

2006 Polonskaya (provisional designation: 1973 SB3) is a stony Flora asteroid and asynchronous binary system from the inner regions of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. It was discovered on 22 September 1973, by Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula, and later named after Ukrainian astronomer Elena Kazimirtchak-Polonskaïa. Its one-kilometer-sized satellite was discovered by an international collaboration of astronomers in November 2005.

3309 Brorfelde, provisional designation 1982 BH, is a nearly spheroidal, binary Hungaria asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 28 January 1982, by Danish astronomers Kaare Jensen and Karl Augustesen at the Brorfelde Observatory near Holbæk, Denmark. It was named for the discovering observatory and the village where it is located.

<span class="mw-page-title-main">1111 Reinmuthia</span> Very elongated asteroid from the background population

1111 Reinmuthia is a very elongated asteroid from the background population, located in the outer region of the asteroid belt. It was discovered on 11 February 1927, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The F-type asteroid (FX) has a short rotation period of 4.02 hours and measures approximately 40 kilometers in diameter. It was later named in honor of Karl Reinmuth, the discoverer himself.

1128 Astrid, provisional designation 1929 EB, is a carbonaceous Astridian asteroid from the central region of the asteroid belt. It is the parent body of the Astrid family and measures approximately 40 kilometers in diameter.

14335 Alexosipov, provisional designation 1981 RR3, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered by Soviet–Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on 3 September 1981. The asteroid was named after astronomer Alexandr Osipov.

<span class="mw-page-title-main">1338 Duponta</span>

1338 Duponta, provisional designation 1934 XA, is a stony Florian asteroid and synchronous binary system from the inner regions of the asteroid belt, approximately 7.8 kilometers in diameter.

<span class="mw-page-title-main">1251 Hedera</span>

1251 Hedera is a background asteroid from the central regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 25 January 1933, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The asteroid was named for the climbing plant Hedera, commonly known as "ivy".

5905 Johnson, provisional designation 1989 CJ1, is a Hungaria asteroid and synchronous binary system from the innermost regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 11 February 1989, by American astronomer Eleanor Helin at Palomar Observatory in California, United States. Its satellite measures approximately 1.6 km (1 mi) in diameter and orbits its primary every 21.8 hours. It was named after American astronomer and engineer Lindley N. Johnson.

21509 Lucascavin, provisional designation 1998 KL35, is a small asteroid from the inner regions of the asteroid belt, approximately 2.5 kilometers (1.6 miles) in diameter. It is the namesake of the tiny Lucascavin family located within the Flora clan. It was discovered on 22 May 1998, by astronomers with the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico. The presumed S-type asteroid has a rotation period of 5.8 hours. It was named for the 2005-ISEF awardee Lucas James Cavin.

1376 Michelle, provisional designation 1935 UH, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 29 October 1935, by French astronomer Guy Reiss at the North African Algiers Observatory in Algeria. It is named for the discoverer's daughter, Michelle Reiss.

<span class="mw-page-title-main">1512 Oulu</span>

1512 Oulu, provisional designation 1939 FE, is a dark Hildian asteroid, slow rotator and possibly the largest known tumbler orbiting in the outermost region of the asteroid belt. With a diameter of approximately 80 kilometers, it belongs to the fifty largest asteroids in the outer main-belt. The body was discovered on 18 March 1939, by Finnish astronomer Heikki Alikoski at Turku Observatory in Southwest Finland and named for the Finnish town Oulu.

2169 Taiwan, provisional designation 1964 VP1, is a carbonaceous Astridian asteroid from the central regions of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 9 November 1964, by astronomers at the Purple Mountain Observatory near Nanking, China. It was named for Taiwan.

2044 Wirt, provisional designation 1950 VE, is a binary Phocaea asteroid and Mars-crosser, approximately 6.7 kilometers in diameter. The minor-planet moon has an estimated diameter of 1.89 kilometer.

<span class="mw-page-title-main">Kharkiv Observatory</span> Observatory

Institute of Astronomy of Kharkiv National University, or Kharkiv Astronomical Observatory — is a scientific institution at Kharkiv University. The institution was founded in 1808 as the astronomy laboratory of the university, and in 1888, mainly due to the efforts of Gregory Levitsky, a fully equipped observatory in a separate house was created.

References

  1. List Of Observatory Codes, Minor Planet Center.
  2. Нещерет И. (2019-07-31). "Начальник Чугуевской наблюдательной станции НИИ астрономии рассказал об истории станции и поделился новостями из космоса" (in Russian). Медиа Группа Объектив.
  3. 200 лет астрономии в Харьковском университете (PDF) (500 экз ed.). Харьков: ХНУ. Шкуратов Ю. Г. (ред.). 2008.
  4. Tereshchenko IA, Shevchenko VG, Kruglyy YN (2010). "Исследование фотометрической системы телескопа АЗТ-8 и ПЗС-камеры IMG 1024S" (PDF). 26 (2) (Кинематика и физика небесных тел ed.): 74–80.{{cite journal}}: Cite journal requires |journal= (help)
  5. Dudinov VN, Tsetkova VS, Krishtal VA, Gurenko AN, Shpilsky LF (1977). "Когерентно-оптический вычислитель Харьковского университета" (160. Физика Луны и планет. Фундаментальная астрономия) (Вестник Харьковского государственного университета ed.): 65–76.{{cite journal}}: Cite journal requires |journal= (help)
  6. Karri Muinonen; Irina N. Belskaya; Alberto Cellino; Marco Delbò; Anny Chantal Levasseur-Regourd; Antti Penttilä; Edward F. Tedesco (2010). "A three-parameter magnitude phase function for asteroids". Icarus (Icarus ed.). Elsevier. 209 (2): 542–555. Bibcode:2010Icar..209..542M. doi:10.1016/j.icarus.2010.04.003.
  7. Ďurech, J.; Vokrouhlický, D.; Kaasalainen, M.; Higgins, D.; Krugly, Yu. N.; Gaftonyuk, N. M.; Shevchenko, V. G.; Chiorny, V. G.; Hamanowa, H.; Hamanowa, H.; Reddy, V.; Dyvig, R. R. (2008). "Detection of the YORP effect in asteroid (1620) Geographos". Astronomy and Astrophysics. 489 (2): L25–L28. Bibcode:2008A&A...489L..25D. doi:10.1051/0004-6361:200810672.
  8. Durech, J.; Vokrouhlický, D.; Baransky, A. R.; Breiter, S.; Burkhonov, O. A.; Cooney, W.; et al. (November 2012). "Analysis of the rotation period of asteroids (1865) Cerberus, (2100) Ra-Shalom, and (3103) Eger - search for the YORP effect". Astronomy and Astrophysics. 547: 9. arXiv: 1210.2219 . Bibcode:2012A&A...547A..10D. doi:10.1051/0004-6361/201219396. S2CID   54496050.