(3544) Borodino ( eng. 3544 Borodino , earlier 1977 RD 4 ) is a rocky asteroid of the inner region of the asteroid belt, the diameter is about 9 km. Discovered on September 7, 1977 by the Soviet astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory . [1] The form of the asteroid, presumably elongated, the circulation period is 5.44 hours. [3] The asteroid is named after the village of Borodino , in which the Battle of Borodino took place . [one]
| (3544) Borodino | |
|---|---|
| Asteroid | |
| Other names | 1977 FD 4 · 1936 QJ 1 1943 GM · 1947 LO 1951 RW 1 · 1951 SJ 1980 FM 11 · 1981 RN 5 |
| Category of small planets | main-belt asteroid [1] [2] · ( Kirkwood cracks ) [3] |
| Discovery [1] | |
| Discoverer | N. Chernykh |
| Place of discovery | CrAO |
| opening date | September 7, 1977 |
| Orbital characteristics [2] | |
| Epoch : March 23, 2018 ( JD 2458200.5) | |
| Perihelion | 1.8718 AU |
| Aphelion | 2,9302 AU |
| Semi-axis ( a ) | 2.4010 au |
| The eccentricity of the orbit ( e ) | 0,2204 |
| Sidereal period of circulation | 3.72 years (1359 days) |
| Average anomaly ( M o ) | 344.02 ° |
| Inclination ( i ) | 8.9017 ° |
| Ascending node longitude ( Ω ) | 147.61 ° |
| Pericenter Argument ( ω ) | 148.82 ° |
| Whose companion | |
| physical characteristics | |
| Dimensions | 6.11 ± 0.55 [4] 8.5002 ± 0.075 km [5] 8,688 ± 0,056 km [6] 9.84 km (estimated) [3] |
| Rotation period ( t ) | 5.43459 ± 0.00001 h [7] 5.43460 ± 0.00005 h [8] 5.435 ± 0.00005 h [9] 5.437 ± 0.001 h [10] 5.44 ± 0.01 h [11] 5.442 ± 0.002 h |
| Albedo | 0.20 (guess) [3] 0.2361 ± 0.0290 [6] 0,247 ± 0,027 [12] 0.474 ± 0.088 [4] |
| Spectral class | S (supposedly) [3] |
| Absolute magnitude | 12.23 ± 0.15 [13] 12.4 [2] [3] 12.50 [4] [6] |
Orbit and classification
Borodino is located in the asteroid belt, but does not belong to any family. [14] The asteroid orbits around the Sun in the inner part of the Main Belt at a distance of 1.9–2.9 AU. with a period of 3 years 9 months (1359 days, the semi-major axis is 2.4 AU). The eccentricity of the orbit is equal to 0.22, and the angle of inclination of the orbit relative to the plane of the ecliptic is 9 °. [2]
The asteroid was first observed as a 1936 QJ 1 object at the Johannesburg Observatory in August 1936. The observation arc begins with the observation of an asteroid as a 1943 GM object at the Turku Observatory in April 1943 more than 34 years before the official discovery. [one]
Physical characteristics
Borodino is assumed to be a S class stone asteroid, which is consistent with the measured albedo value (see below) according to the Wide-field Infrared Survey Explorer (WISE). [3]
Rotation period
Photometric observations from 2007 allowed us to construct several light curves . The high-resolution gloss curve was obtained by Australian amateur astronomer David Higgins at Hunters Hill Observatory; these data allowed us to determine the rotation period of 5.442 hours with a brightness change of 0.60 magnitude. Other observations by amateur French astronomer Patrick Masel, astronomers of the University of Texas A & M , and astronomers at the Oakley Observatory determined the period values of 5.435, 5.437, and 5.44 hours with a magnitude of 0.74, 0.65, and 0.63 stellar magnitudes, respectively. [9] [10] [11] The high brightness variability indicates a non-spherical shape of the asteroid.
Poles
Two light curves, published in 2016, were built using photometric models from the Lowell Photometric Database (LPD ) and other sources; the curves give estimates of the sidereal rotation period of 5.43459 and 5.43460 hours, respectively. Each simulated light curve also determines the position of the axes of rotation (104.0 °, −57.0 °) and (267.0 °, −53.0 °), and also (294.0 °, −60.0 °) and (157.0 °, −57.0 °) in the ecliptic coordinate system (λ, β) respectively. [7] [8]
Diameter and Albedo
According to the data of surveys conducted by Akari and WISE telescopes, Borodino has a diameter of from 6.11 to 8.688 km, the surface has an albedo from 0.2361 to 0.474. [4] [5] [6] [12]
The source of the Collaborative Asteroid Lightcurve Link indicates an albedo value of 0.20, which corresponds to a diameter of 9.84 km with an absolute magnitude of 12.4. [3]
Title
The minor planet is named after the Russian village of Borodino near Moscow, where the battle of Borodino took place in September 1812. [1] The official name was published by the Minor Planet Center on November 10, 1992 ( MPC 21130 ). [15]
See also
- List of asteroids ( 3501-3600 )
Notes
- ↑ 1 2 3 4 5 6 3544 Borodino (1977 RD4) . Minor Planet Center . The appeal date is May 15, 2018.
- 2 1 2 3 4 JPL Small-Body Database Browser: 3544 Borodino (1977 RD4) Undefined . Jet Propulsion Laboratory . The appeal date is May 15, 2018.
- ↑ 1 2 3 4 5 6 7 8 LCDB Data for (3544) Borodino Unc . Asteroid Lightcurve Database (LCDB). The appeal date is May 15, 2018.
- ↑ 1 2 3 4 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G .; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; Ishihara, Daisuke; Kataza, Hirokazu; Takita, Satoshi; Oyabu, Shinki; Ueno, Munetaka; Matsuhara, Hideo; Onaka, Takashi. Asteroid Catalog Using Akari: AKARI / IRC Mid-Infrared Asteroid Survey (Eng.) // Publications of the Astronomical Society of Japan : journal. - Astronomical Society of Japan, 2011. - October ( vol. 63 , no. 5 ). - P. 1117-1138 . - DOI : 10.1093 / pasj / 63.5.1117 . - . Online catalog
- ↑ 1 2 Masiero, Joseph R .; Grav, T .; Mainzer, AK; Nugent, CR; Bauer, JM; Stevenson, R .; Sonnett, S. Main-belt Asteroids with WISE / NEOWISE: Near-infrared Albedos (English) // The Astrophysical Journal : journal. - IOP Publishing , 2014. - August ( vol. 791 , no. 2 ). - P. 11 . - DOI : 10.1088 / 0004-637X / 791/2/121 . - . - arXiv : 1406.6645 .
- ↑ 1 2 3 4 Mainzer, A .; Grav, T .; Masiero, J .; Hand, E .; Bauer, J .; Tholen, D .; McMillan, RS; Spahr, T .; Cutri, RM; Wright, E .; Watkins, J .; Mo, W .; Maleszewski, C. NEOWISE Studies of the Classified Asteroids: Preliminary Results (Eng.) // The Astrophysical Journal : journal. - IOP Publishing , 2011. - November ( vol. 741 , no. 2 ). - P. 25 . - DOI : 10.1088 / 0004-637X / 741/2/90 . - . - arXiv : 1109.6407 . ( catalog )
- ↑ 1 2 Durech, J .; Hanus, J .; Oszkiewicz, D .; Vanco, R. Asteroid models from the Lowell photometric database (Eng.) // Astronomy and Astrophysics : journal. - EDP Sciences , 2016. - March ( vol. 587 ). - P. 6 . - DOI : 10.1051 / 0004-6361 / 201527573 . - . - arXiv : 1601.02909 .
- ↑ 1 2 Hanus, J .; Durech, J .; Oszkiewicz, DA; Behrend, R .; Carry, B .; Delbo, M .; Adam, O .; Afonina, V .; Anquetin, R .; Antonini, P .; Arnold, L .; Audejean, M .; Aurard, P .; Bachschmidt, M .; Baduel, B .; Barbotin, E .; Barroy, P .; Baudouin, P .; Berard, L .; Berger, N .; Bernasconi, L .; Bosch, J.-G .; Bouley, S .; Bozhinova, I .; Brinsfield, J .; Brunetto, L .; Canaud, G .; Caron, J .; Carrier, F .; Casalnuovo, G .; Casulli, S .; Cerda, M .; Chalamet, L .; Charbonnel, S .; Chinaglia, B .; Cikota, A .; Colas, F .; Coliac, J.-F .; Collet, A .; Coloma, J .; Conjat, M .; Conseil, E .; Costa, R .; Crippa, R .; Cristofanelli, M .; Damerdji, Y .; Debackè; re, A .; Decock, A .; Déhais, Q .; Déléage, T .; Delmelle, S .; Demeautis, C .; Drózdz, M .; Dubos, G .; Dulcamara, T .; Dumont, M .; Durkee, R .; Dymock, R .; Escalante del Valle, A .; Esseiva, N .; Esseiva, R .; Esteban, M .; Fauchez, T .; Fauerbach, M .; Fauvaud, M .; Fauvaud, S .; Forné, E .; Fournel, C .; Fradet, D .; Garlitz, J .; Gerteis, O .; Gillier, C .; Gillon, M .; Giraud, R .; Godard, J.-P .; Goncalves, R .; Hamanowa, Hiroko; Hamanowa, Hiromi; Hay, K .; Hellmich, S .; Heterier, S .; Higgins, D .; Hirsch, R .; Hodosan, G .; Hren, M .; Hygate, A .; Innocent, N .; Jacquinot, H .; Jawahar, S .; Jehin, E .; Jerosimic, L .; Klotz, A .; Koff, W .; Korlevic, P .; Kosturkiewicz, E .; Krafft, P .; Krugly, Y .; Kugel, F .; Labrevoir, O .; Lecacheux, J .; Lehký, M .; Leroy, A .; Lesquerbault, B .; Lopez-Gonzales, MJ; Lutz, M .; Mallecot, B .; Manfroid, J .; Manzini, F .; Marciniak, A .; Martin, A .; Modave, B .; Montaigut, R .; Montier, J .; Morelle, E .; Morton, B .; Mottola, S .; Naves, R .; Nomen, J .; Oey, J .; Ogloza, W .; Paiella, M .; Pallares, H .; Peyrot, A .; Pilcher, F .; Pirenne, J.-F .; Piron, P .; Polinska, M .; Polotto, M .; Poncy, R .; Previt, JP; Reignier, F .; Renauld, D .; Ricci, D .; Richard, F .; Rinner, C .; Risoldi, V .; Robilliard, D .; Romeuf, D .; Rousseau, G .; Roy, R .; Ruthroff, J .; Salom, PA; Salvador, L .; Sanchez, S .; Santana-Ros, T .; Scholz, A .; Séné, G .; Skiff, B .; Sobkowiak, K .; Sogorb, P .; Soldán, F .; Spiridakis, A .; Splanska, E .; Sposetti, S .; Starkey, D .; Stephens, R .; Stiepen, A .; Stoss, R .; Strajnic, J .; Teng, J.-P .; Tumolo, G .; Vagnozzi, A .; Vanoutryve, B .; Vugnon, JM; Warner, BD; Waucomont, M .; Wertz, O .; Winiarski, M .; Wolf, M. New and updated convex shape from a large collaboration ( http://www.ustech.org/ ) communication / / Astronomy and Astrophysics : journal. - EDP Sciences , 2016. - February ( vol. 586 ). - P. 24 . - DOI : 10.1051 / 0004-6361 / 201527441 . - . - arXiv : 1510.07422 .
- 2 1 2 Behrend, Raoul Asteroids and comets rotation curves - (3544) Borodino Unreferenced (not available link) . Geneva Observatory. The appeal date is May 15, 2018. Archived December 14, 2018.
- ↑ 1 2 Cantu, Sara; Adolphson, Max; Montgomery, Kent; Renshaw, Thomas. Lightcurves of Asteroids 2007 McCuskey, 2669 Shostakovich 3544 Borodino, and 7749 Jackschmitt (Eng.) // The Minor Planet Bulletin : journal. - Association of Lunar and Planetary Observers , 2015. - January ( vol. 42 , no. 1 ). - P. 28-29 . - ISSN 1052-8091 . - .
- ↑ 1 2 Torno, Steven; Oliver, Robert Lemke; Ditteon, Richard. Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory - October 2007 (Eng.) // The Minor Planet Bulletin : journal. - Association of Lunar and Planetary Observers , 2008. - June ( vol. 35 , no. 2 ). - P. 54-55 . - ISSN 1052-8091 . - .
- ↑ 1 2 Masiero, Joseph R .; Mainzer, AK; Grav, T .; Bauer, JM; Cutri, RM; Dailey, J .; Eisenhardt, PRM; McMillan, RS; Spahr, TB; Skrutskie, MF; Tholen, D .; Walker, RG; Wright, EL; DeBaun, E .; Elsbury, D .; Gautier, T., IV; Gomillion, S .; Wilkins, A. Main Belt. Asteroids with WISE / NEOWISE. I. Preliminary Albedos and Diameters (English) // The Astrophysical Journal : journal. - IOP Publishing , 2011. - November ( vol. 741 , no. 2 ). - P. 20 . - DOI : 10.1088 / 0004-637X / 741/2/68 . - . - arXiv : 1109.4096 .
- ↑ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; Chastel, Serge; Wainscoat, Richard J .; Burgett, William S .; Chambers, Kenneth C .; Flewelling, Heather; Kaiser, Nick; Magnier, Eugen A .; Morgan, Jeff S .; Price, Paul A .; Tonry, John L .; Waters, Christopher. Pan-STARRS PS1 - Preliminary results (Eng.) // Absolute magnitudes and slope parameters for 250,000 asteroids : journal. - Elsevier , 2015. - November ( vol. 261 ). - P. 34-47 . - DOI : 10.1016 / j.icarus.2015.08.007 . - . - arXiv : 1506.00762 .
- ↑ Small Bodies Data Ferret . Nesvorny HCM Asteroid Families V3.0 . The appeal date is May 15, 2018.
- ↑ MPC / MPO / MPS Archive . Minor Planet Center . The appeal date is May 15, 2018.
Links
- Archived October 25, 2010.
- Asteroid Lightcurve Database (LCDB) , request form ( info )
- Dictionary of Minor Planet Names , Google books
- Asteroids and comets rotation curves, CdR - Geneva Observatory, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1) - (5000) - Center for Small Planets
- (3544) Borodino on AstDyS-2, Asteroids — Dynamic Site