astro.wikisort.org - Asteroid2423 Ibarruri, provisional designation 1972 NC, is an eccentric, tumbling and rare-type asteroid, classified as slow rotator and sizable Mars-crosser from the inner regions of the asteroid belt, approximately 5 kilometers in diameter.
2423 Ibarruri|
Discovered by | L. Zhuravleva |
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Discovery site | Crimean Astrophysical Obs. |
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Discovery date | 14 July 1972 |
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MPC designation | (2423) Ibarruri |
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Named after | Rubén Ibárruri (Hero of the Soviet Union)[2] |
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Alternative designations | 1972 NC · 1930 SV 1943 TB · 1956 VC 1972 PB |
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Minor planet category | Mars-crosser [3][4] |
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Epoch 4 September 2017 (JD 2458000.5) |
Uncertainty parameter 0 |
Observation arc | 60.59 yr (22,129 days) |
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Aphelion | 2.8068 AU |
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Perihelion | 1.5702 AU |
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Semi-major axis | 2.1885 AU |
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Eccentricity | 0.2825 |
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Orbital period (sidereal) | 3.24 yr (1,183 days) |
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Mean anomaly | 315.42° |
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Inclination | 4.0571° |
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Longitude of ascending node | 264.96° |
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Argument of perihelion | 80.645° |
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Dimensions | 4.899±1.085[5] 6.50 km (calculated)[3] |
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Synodic rotation period | 73.08±0.10 h[6] 139.79±0.04 h[lower-alpha 1] 139.9±0.2 h[7] 139.92±0.01 h[8] |
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Geometric albedo | 0.20 (assumed)[3] 0.330±0.167[5] |
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Spectral type | SMASS = A [1][9] L [10] · S [11] · C [3] |
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Absolute magnitude (H) | 13.3[1] · 13.44±1.15[10] · 13.20[11] · 13.3[3] |
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The asteroid was discovered by Russian–Ukrainian astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauchnyj, on 14 July 1972.[4] It was named after Spanish communist Rubén Ruiz Ibárruri.[2]
Orbit and classification
Ibarruri orbits the Sun in the inner main-belt at a distance of 1.6–2.8 AU once every 3 years and 3 months (1,183 days). Its orbit has an eccentricity of 0.28 and an inclination of 4° with respect to the ecliptic.[1]
Physical characteristics
The spectral type of the asteroid is that of a rare A-type in the SMASS taxonomy, with its surface consisting of almost pure olivine, which gives the body a very reddish color. As of November 2015, only 17 minor planets of this type are known.[12]
As a spectroscopic A-type asteroid, it belongs to the larger group of bodies with a silicaceous composition. However, the Collaborative Asteroid Lightcurve Link classifies the asteroid into the carbonaceous group, despite the fact that is assumes a relatively high geometric albedo of 0.20,[3] which is rather typical for stony asteroids.
Slow rotator and tumbler
Ibarruri has a notably slow rotation period of 140 hours,[lower-alpha 1][7] and seems to be in a non-principal axis rotation (NPAR), colloquially called as "tumbling".[13]
Naming
This minor planet was named after Rubén Ruiz Ibárruri (1920–1942), son of Spanish communist leader Dolores Ibárruri and a posthumous Hero of the Soviet Union. He enlisted in the Soviet army and died in the early stage of the Battle of Stalingrad in September 1942.[2] The official naming citation was published by the Minor Planet Center on 8 February 1982 (M.P.C. 6649).[14]
Notes
References
- "JPL Small-Body Database Browser: 2423 Ibarruri (1972 NC)" (2017-06-05 last obs.). Jet Propulsion Laboratory. Retrieved 13 June 2017.
- Schmadel, Lutz D. (2007). "(2423) Ibarruri". Dictionary of Minor Planet Names – (2423) Ibarruri. Springer Berlin Heidelberg. p. 198. doi:10.1007/978-3-540-29925-7_2424. ISBN 978-3-540-00238-3.
- "LCDB Data for (2423) Ibarruri". Asteroid Lightcurve Database (LCDB). Retrieved 7 December 2016.
- "2423 Ibarruri (1972 NC)". Minor Planet Center. Retrieved 7 December 2016.
- Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. Retrieved 7 December 2016.
- Vander Haagen, Gary A. (April 2012). "Lightcurves of 724 Hapag, 2423 Ibarruri, 4274 Karamanov 4339 Almamater, and 5425 Vojtech". The Minor Planet Bulletin. 39 (2): 48–50. Bibcode:2012MPBu...39...48V. ISSN 1052-8091. Retrieved 7 December 2016.
- Buchheim, Robert K. (October 2012). "Lightcurves of 2423 Ibarruri and 8345 Ulmerspatz". The Minor Planet Bulletin. 39 (4): 209–211. Bibcode:2012MPBu...39..209B. ISSN 1052-8091. Retrieved 7 December 2016.
- Ferrero, Andrea (April 2012). "Lightcurve Determination at the Bigmuskie Observatory from 2011 July-December". The Minor Planet Bulletin. 39 (2): 65–67. Bibcode:2012MPBu...39...65F. ISSN 1052-8091. Retrieved 7 December 2016.
- Xu, Shui; Binzel, Richard P.; Burbine, Thomas H.; Bus, Schelte J. (May 1995). "Small main-belt asteroid spectroscopic survey: Initial results". Icarus. 115 (1): 1–35. Bibcode:1995Icar..115....1X. doi:10.1006/icar.1995.1075. ISSN 0019-1035. Retrieved 25 November 2015.
- Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 7 December 2016.
- Carry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry". Icarus. 268: 340–354. arXiv:1601.02087. Bibcode:2016Icar..268..340C. doi:10.1016/j.icarus.2015.12.047. Retrieved 7 December 2016.
- "JPL Small-Body Database Search Engine: spec. type = A (SMASSII)". JPL Solar System Dynamics. Retrieved 25 November 2015.
- Pravec, P.; Scheirich, P.; Durech, J.; Pollock, J.; Kusnirák, P.; Hornoch, K.; et al. (May 2014). "The tumbling spin state of (99942) Apophis". Icarus. 233: 48–60. Bibcode:2014Icar..233...48P. doi:10.1016/j.icarus.2014.01.026. Retrieved 25 November 2015.
- "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 7 December 2016.
External links
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- 2422 Perovskaya
- 2423 Ibarruri
- 2424 Tautenburg
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На других языках
[de] (2423) Ibarruri
(2423) Ibarruri (1972 NC; 1930 SV; 1943 TB; 1956 VC; 1972 PB) ist ein ungefähr fünf Kilometer großer Asteroid des inneren Hauptgürtels, der am 14. Juli 1972 von der ukrainischen (damals: Sowjetunion) Astronomin Ljudmyla Schurawlowa am Krim-Observatorium (Zweigstelle Nautschnyj) auf der Halbinsel Krim (IAU-Code 095) entdeckt wurde.
- [en] 2423 Ibarruri
[ru] (2423) Ибаррури
(2423) Ибаррури (лат. Ibarruri) — небольшой астероид, который относится к группе астероидов пересекающих орбиту Марса и принадлежащий к редкому спектральному классу A. Он был открыт 14 июля 1972 года советским астрономом Людмилой Журавлёвой в Крымской обсерватории и назван в честь Героя Советского Союза испанского коммуниста Рубена Ибаррури[1].
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