Global InformationChuhuiv Observational Station information
 | You can help expand this article with text translated from the corresponding article in Ukrainian. (May 2024) Click [show] for important translation instructions.
|
 Dome of 70-cm telescope AZT-8 | |||
| Organization | Kharkiv National University | ||
|---|---|---|---|
| Observatory code | 121[1] | ||
| Location | Chuhuiv Raion, Ukraine | ||
| Coordinates | 49°38′34.6″N 36°56′12.8″E / 49.642944°N 36.936889°E | ||
| Altitude | 156 m | ||
| Established | 1962  | ||
| Website | www | ||
| Telescopes | |||
| |||
  Location of Chuhuiv Observational Station | |||
 Related media on Commons | |||
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]
- ^ List Of Observatory Codes, Minor Planet Center.
- ^ 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.
- ^ 200 лет астрономии в Харьковском университете (PDF) (500 экз ed.). Харьков: ХНУ. 2008.
{{cite book}}: Unknown parameter|agency=ignored (help) - ^ 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) - ^ 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) - ^ 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. 209 (2) (Icarus ed.): 542–555. Bibcode:2010Icar..209..542M. doi:10.1016/j.icarus.2010.04.003.
{{cite journal}}: Unknown parameter|agency=ignored (help) - ^ 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.
- ^ 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.