1369 Ostanina

Last updated

1369 Ostanina
001369-asteroid shape model (1369) Ostanina.png
Shape model of Ostanina from its lightcurve
Discovery [1]
Discovered by P. Shajn
Discovery site Simeiz Obs.
Discovery date27 August 1935
Designations
(1369) Ostanina
Named after
 Ostanin [2]
(Discoverer's birthplace)
1935 QB ·1928 FE
main-belt [1] [3]  ·(outer)
Meliboea [4]
Orbital characteristics [3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc 90.58 yr (33,086 d)
Aphelion 3.7770 AU
Perihelion 2.4627 AU
3.1198 AU
Eccentricity 0.2106
5.51 yr (2,013 d)
110.16°
0° 10m 44.04s / day
Inclination 14.365°
180.46°
127.84°
Physical characteristics
Mean diameter
40.59±0.62  km [5]
41.24±4.1 km [6]
42.401±0.162 km [7] [8]
43.561±0.266 km [9]
8.4001±0.0002  h [10]
0.0490 [9]
0.052 [7] [8]
0.0545 [6]
0.061 [5]
Caa/Ch (S3OS2) [11]
C (SDSS-MOC) [12]
10.7 [1] [3] [5] [6] [7] [9]

    1369 Ostanina (prov. designation: 1935 QB) is a dark and elongated asteroid of the Meliboea family, located in the outer region of the asteroid belt. It was discovered on 27 August 1935, by Soviet astronomer Pelageya Shajn at the Simeiz Observatory on the Crimean peninsula. [1] The hydrated carbonaceous C-type asteroid has a rotation period of 8.4 hours and measures approximately 42 kilometers (26 miles) in diameter. [13] It was named for the Russian village of Ostanin, birthplace of the discoverer. [2]

    Contents

    Orbit and classification

    Ostanina orbits the Sun in the outer main-belt at a distance of 2.5–3.8  AU once every 5 years and 6 months (2,013 days; semi-major axis of 3.12 AU). Its orbit has an eccentricity of 0.21 and an inclination of 14° with respect to the ecliptic. [3]

    Based on the hierarchical clustering method (HCM) using the asteroid's proper orbital elements, Ostanina is a member of the Meliboea family ( 604 ), [4] a smaller asteroid family of a few hundred carbonaceous outer-belt asteroids. The family was named after its lowest-numbered member, 137 Meliboea. [14] : 23  In an alternative HCM-analysis, however, Ostanina is an asteroid of the main belt's background population. [15] The body's observation arc begins with its first observation as 1928 FE at the Heidelberg Observatory in March 1928, more than 7 years prior to its official discovery observation at Simeiz–Crimea. [1]

    Naming

    This minor planet was named after the small village of Ostanin, the birthplace of the discoverer, Pelageya Shajn. The village is located in Perm Krai, now part of the Russian Volga district. [2] The official naming citation was published by the Minor Planet Center in November 1952 ( M.P.C. 838; LDS ). [16]

    Physical characteristics

    In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Ostanina is a hydrated C-type asteroid (Caa and Ch), [4] [11] while in the SDSS-based taxonomy, the asteroid is a common C-type. [12]

    Rotation period

    In June 2011, a rotational lightcurve of Ostanina was obtained from photometric observations by French and Swiss astronomers Pierre Antonini, François Colas, Valery Lainey, Laurène Beauvalet and Raoul Behrend. Lightcurve analysis gave a rotation period of 8.4001±0.0002 hours with a very high brightness variation of 1.11 magnitude ( U=3 ). [10] A high brightness amplitude is indicative of a non-spheroidal, elongated shape. Other well defined rotation periods of 8.399 and 8.397 hours were obtained by Robert Stephens at the Center for Solar System Studies ( U81 ) in California in 2017, and by V. G. Shevchenko at the Kharkov Observatory ( 101 ) in 1996, respectively ( U=3/3 ). [17] [lower-alpha 1] [lower-alpha 2]

    Additional period determinations: 6+ hours by Jean-Gabriel Bosch at the Collonges Observatory ( 178 ) ( U=2 ), [10] 6.145 hours at the Catania and Pino Torinese observatories in 2000 ( U=1 ), [18] 8.3945 hours by René Roy in 2016 ( U=3- ), [10] 8.397 hours by V. G. Chiorny in 2003 and 2007 ( U=n.a./2+ ), [19] [lower-alpha 3] and 8.4 hours by Roberto Crippa and Federico Manzini at the Sozzago Astronomical Station ( A12 ) in 2010 ( U=2+ ). [10]

    Diameter and albedo

    According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Ostanina measures between 40.6 and 43.6 kilometers in diameter and its surface has an albedo between 0.049 and 0.061. [5] [6] [7] [8] [9] The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0545 and diameter of 41.24 kilometers using an absolute magnitude of 10.7. [13]

    Notes

    1. ↑ Lightcurve plot of (1369) Ostanina by Robert Stephens at the Center for Solar System Studies ( U81 ) Quality code is 3. Summary figures at the LCDB and CS3.
    2. ↑ Shevchenko (1996) web: rotation period 8.397 hours with a brightness amplitude of 0.82 mag. Quality code is 3. Summary figures at the LCDB.
    3. ↑ Chiorny (2003) web: rotation period 8.397 hours with a brightness amplitude of 0.84 mag. Summary figures at the LCDB.

    Related Research Articles

    <span class="mw-page-title-main">2829 Bobhope</span>

    2829 Bobhope is a dark asteroid of the Meliboea family, from the outer region of the asteroid belt. It was discovered on 9 August 1948, by South African astronomer Ernest Leonard Johnson at Union Observatory in Johannesburg. The asteroid was later named after comedian Bob Hope. The asteroid has a rotation period of 6.1 hours and measures approximately 37 kilometers in diameter.

    460 Scania is a background asteroid and a slow rotator from the central regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 22 October 1900. The uncommon K-type asteroid has an exceptionally long rotation period of 164.1 hours and measures approximately 21 kilometers in diameter. It was named after the Swedish region of Scania, where a meeting was held by the Astronomische Gesellschaft in 1904.

    <span class="mw-page-title-main">834 Burnhamia</span>

    834 Burnhamia is a large background asteroid, approximately 61 kilometers in diameter, that is located in the outer region of the asteroid belt. It was discovered on 20 September 1916, by German astronomer Max Wolf at the Heidelberg Observatory in southwest Germany. The X-type asteroid (GS) has a rotation period of 13.9 hours. It was named after American astronomer Sherburne Wesley Burnham (1838–1921).

    927 Ratisbona is a large and dark background asteroid, approximately 76 kilometers in diameter, located in the outer region of the asteroid belt. It was discovered on 16 February 1920, by astronomer Max Wolf at the Heidelberg Observatory in southwest Germany. The carbonaceous C-type asteroid (CB) has a rotation period of 12.99 hours and is rather spherical in shape. It was named after the Bavarian city of Regensburg.

    946 Poësia is a Themis asteroid and slow rotator, approximately 39 kilometers in diameter, located in the outer regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 11 February 1921 and given the provisional designations A921 CD and 1921 JC. The F-type asteroid has a long rotation period of 108.5 hours. It was named after the goddess of poetry.

    1575 Winifred, provisional designation 1950 HH, is a stony Phocaea asteroid and slow rotator from the inner regions of the asteroid belt, approximately 9.5 kilometers in diameter.

    Lagrangea, provisional designation 1923 OU, is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 30 kilometers in diameter. It was discovered on 12 September 1923, by Russian astronomer Sergey Belyavsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named after Italian mathematician and astronomer Joseph-Louis Lagrange.

    <span class="mw-page-title-main">1030 Vitja</span>

    1030 Vitja, provisional designation 1924 RQ, is a dark background asteroid from the outer regions of the asteroid belt, approximately 60 kilometers in diameter. It was discovered on 25 May 1924, by Soviet–Russian astronomer Vladimir Albitsky at the Simeiz Observatory on the Crimean peninsula. The asteroid was named in honor of Viktor Zaslavskij (1925–1944), a relative of the discoverer.

    1074 Beljawskya, provisional designation 1925 BE, is a Themistian asteroid from the outer region of the asteroid belt, approximately 48 kilometers in diameter.

    1517 Beograd, provisional designation 1938 FD, is a dark Paduan asteroid from the central region of the asteroid belt, approximately 36 kilometers in diameter. It was discovered on 20 March 1938, by Serbian astronomer Milorad Protić at Belgrade Astronomical Observatory in Serbia. It is named after the city Belgrade.

    1115 Sabauda is a carbonaceous Meliboean asteroid from the outer region of the asteroid belt, approximately 68 kilometers in diameter. Discovered in 1928 by Italian astronomer Luigi Volta, it was assigned the provisional designation 1928 XC. The asteroid was probably named after the House of Savoy, the former rulers of Italy.

    <span class="mw-page-title-main">1165 Imprinetta</span>

    1165 Imprinetta, provisional designation 1930 HM, is a carbonaceous Meliboean asteroid from the outer regions of the asteroid belt, approximately 49 kilometers (30 mi) in diameter. It was discovered on 24 April 1930 by Dutch astronomer Hendrik van Gent at the Union Observatory in Johannesburg, South Africa. The asteroid was named after Imprinetta Gent, wife of the discoverer.

    1712 Angola, provisional designation 1935 KC, is a dark asteroid from the outer regions of the asteroid belt, approximately 66 kilometers in diameter. It was discovered on 28 May 1935, by English-born South African astronomer Cyril Jackson at Johannesburg Observatory in South Africa. It is named after the Republic of Angola.

    <span class="mw-page-title-main">1241 Dysona</span>

    1241 Dysona, provisional designation 1932 EB1, is a dark background asteroid from the outer regions of the asteroid belt, approximately 77 kilometers in diameter. It was discovered on 4 March 1932, by English astronomer Harry Edwin Wood at the Union Observatory in Johannesburg, South Africa. The asteroid was named after English astronomer Frank Watson Dyson.

    1384 Kniertje, provisional designation 1934 RX, is a dark Adeonian asteroid from the central regions of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 9 September 1934, by Dutch astronomer Hendrik van Gent at the Union Observatory in Johannesburg, South Africa. The asteroid was named after a character in the Dutch play Op Hoop van Zegen by Herman Heijermans.

    <span class="mw-page-title-main">1841 Masaryk</span>

    1841 Masaryk (prov. designation: 1971 UO1) is a carbonaceous background asteroid from the outer region of the asteroid belt, approximately 46 kilometers in diameter. It was discovered on 26 October 1971, by Czech astronomer Luboš Kohoutek at Bergedorf Observatory in Hamburg, Germany. The asteroid was named after the first President of Czechoslovakia, Tomáš Garrigue Masaryk.

    1680 Per Brahe, provisional designation 1942 CH, is a bright background asteroid from the central region of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 12 February 1942, by Finnish astronomer Liisi Oterma at Turku Observatory in Southwest Finland. The stony S-type asteroid has a rotation period of 3.4 hours. It is named after Swedish count and governor Per Brahe the Younger.

    1405 Sibelius, provisional designation 1936 RE, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 12 September 1936, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland. The asteroid was named after composer Jean Sibelius.

    3345 Tarkovskij, provisional designation 1982 YC1, is a carbonaceous background asteroid from the inner regions of the asteroid belt, approximately 22 kilometers (14 miles) in diameter. It was discovered on 23 December 1982, by Russian astronomer Lyudmila Karachkina at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula, and named after filmmaker Andrei Tarkovsky. The C-type asteroid is a slow rotator with a rotation period of 187 hours.

    1544 Vinterhansenia, provisional designation 1941 UK, is a dark asteroid from the inner regions of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 15 October 1941, by Finnish astronomer Liisi Oterma at Turku Observatory in Southwest Finland, and named for Danish astronomer Julie Vinter Hansen.

    References

    1. 1 2 3 4 5 "1369 Ostanina (1935 QB)". Minor Planet Center. Retrieved 14 December 2018.
    2. 1 2 3 Schmadel, Lutz D. (2007). "(1369) Ostanina". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 111. doi:10.1007/978-3-540-29925-7_1370. ISBN   978-3-540-00238-3.
    3. 1 2 3 4 "JPL Small-Body Database Browser: 1369 Ostanina (1935 QB)" (2018-10-18 last obs.). Jet Propulsion Laboratory . Retrieved 14 December 2018.
    4. 1 2 3 "Asteroid 1369 Ostanina – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 29 October 2019.
    5. 1 2 3 4 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
    6. 1 2 3 4 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0: IRAS–A–FPA–3–RDR–IMPS–V6.0. Bibcode:2004PDSS...12.....T . Retrieved 14 December 2018.
    7. 1 2 3 4 Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System: EAR–A–COMPIL–5–NEOWISEDIAM–V1.0. Bibcode:2016PDSS..247.....M . Retrieved 14 December 2018.
    8. 1 2 3 Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv: 1406.6645 . Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. S2CID   119293330.
    9. 1 2 3 4 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: 1109.6407 . Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID   118700974. (catalog)
    10. 1 2 3 4 5 Behrend, Raoul. "Asteroids and comets rotation curves – (1369) Ostanina". Geneva Observatory . Retrieved 12 January 2017.
    11. 1 2 Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004). "S3OS2: the visible spectroscopic survey of 820 asteroids" (PDF). Icarus. 172 (1): 179–220. Bibcode:2004Icar..172..179L. doi:10.1016/j.icarus.2004.06.006 . Retrieved 14 December 2018.
    12. 1 2 Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids". Astronomy and Astrophysics. 510: 12. Bibcode:2010A&A...510A..43C. doi: 10.1051/0004-6361/200913322 . Retrieved 30 October 2019. (PDS data set)
    13. 1 2 "LCDB Data for (1369) Ostanina". Asteroid Lightcurve Database (LCDB). Retrieved 14 December 2018.
    14. ↑ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv: 1502.01628 . Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN   9780816532131. S2CID   119280014.
    15. ↑ "Asteroid (1369) Ostanina – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 14 December 2018.
    16. ↑ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN   978-3-642-01964-7.
    17. ↑ Stephens, Robert D. (October 2017). "Asteroids Observed from CS3: 2017 April - June" (PDF). Minor Planet Bulletin. 44 (4): 321–323. Bibcode:2017MPBu...44..321S. ISSN   1052-8091 . Retrieved 15 March 2020.
    18. ↑ Blanco, C.; Di Martino, M.; Riccioli, D. (April 2000). "New rotational periods of 18 asteroids". Planetary and Space Science. 48 (4): 271–284. Bibcode:2000P&SS...48..271B. doi:10.1016/S0032-0633(99)00074-4.
    19. ↑ Chiorny, V. G.; Shevchenko, V. G.; Krugly, Yu. N.; Velichko, F. P.; Gaftonyuk, N. M. (May 2007). "Photometry of asteroids: Lightcurves of 24 asteroids obtained in 1993 2005". Planetary and Space Science. 55 (7–8): 986–997. Bibcode:2007P&SS...55..986C. doi:10.1016/j.pss.2007.01.001.
    This page is based on this Wikipedia article
    Text is available under the CC BY-SA 4.0 license; additional terms may apply.
    Images, videos and audio are available under their respective licenses.