Astronomy:2055 Dvořák
| Discovery [1] | |
|---|---|
| Discovered by | L. Kohoutek |
| Discovery site | Bergedorf Obs. |
| Discovery date | 19 February 1974 |
| Designations | |
| (2055) Dvořák | |
| Pronunciation | /dəˈvɔːrʒɑːk, ˈdvɔːr-, -ʒæk/ d-VOR-zha(h)k |
| Named after | Antonín Dvořák (Czech composer)[2] |
| 1974 DB | |
| Minor planet category | Mars-crosser [1][3][4] |
| Orbital characteristics [1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 42.37 yr (15,475 days) |
| |{{{apsis}}}|helion}} | 3.0297 AU |
| |{{{apsis}}}|helion}} | 1.5909 AU |
| 2.3103 AU | |
| Eccentricity | 0.3114 |
| Orbital period | 3.51 yr (1,283 days) |
| Mean anomaly | 101.49° |
| Mean motion | 0° 16m 50.52s / day |
| Inclination | 21.488° |
| Longitude of ascending node | 340.44° |
| 244.12° | |
| Physical characteristics | |
| Dimensions | 8.18 km (calculated)[4] |
| Rotation period | 4.405±0.001 h[5] 4.4106±0.0001 h[6] |
| Geometric albedo | 0.20 (assumed)[4] |
| S [4] | |
| Absolute magnitude (H) | 12.8[1][4] · 12.81±0.05[5] · 13.27±0.65[7] |
2055 Dvořák (/dəˈvɔːr.ʒɑːk/ or /ˈdvɔːr-, -ʒæk/ d-VOR-zha(h)k), provisional designation 1974 DB, is an eccentric asteroid and sizable Mars-crosser from the innermost regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 19 February 1974, by Czech astronomer Luboš Kohoutek at the Bergedorf Observatory in Hamburg, Germany.[3] It was named after Czech composer Antonín Dvořák.[2]
Classification and orbit
Dvořák is a Mars-crossing asteroid, as it crosses the orbit of Mars at 1.666 AU. It orbits the Sun at a distance of 1.6–3.0 AU once every 3 years and 6 months (1,283 days). Its orbit has an eccentricity of 0.31 and an inclination of 21° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation at Bergedorf in 1974.[3]
Physical characteristics
Lightcurves
In July 2013, two rotational lightcurves of Dvořák were obtained from photometric observations by Julian Oey at the Blue Mountain Observatory (Q68), Australia, and by a collaboration of astronomers in Argentina. Lightcurve analysis gave a concurring rotation period of 4.405 and 4.4106 hours, respectively, both with a brightness variation of 0.17 magnitude ({{{1}}}).[5][6]
Diameter and albedo estimates
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.18 kilometers based on an absolute magnitude of 12.8.[4] Dvořák has not been surveyed by any of the space-based telescopes such as IRAS, Akari and WISE.[1][4]
Naming
This minor planet was named after Czech composer Antonin Dvořák (1841–1904), one of the worldwide known Czech composers along with Bedřich Smetana.[2] The official naming citation was published by the Minor Planet Center on 1 July 1979 (M.P.C. 4786).[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "JPL Small-Body Database Browser: 2055 Dvorak (1974 DB)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002055. Retrieved 29 June 2017.
- ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(2055) Dvořák". Dictionary of Minor Planet Names – (2055) Dvořák. Springer Berlin Heidelberg. p. 166. doi:10.1007/978-3-540-29925-7_2056. ISBN 978-3-540-00238-3.
- ↑ 3.0 3.1 3.2 "2055 Dvorak (1974 DB)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2055. Retrieved 29 June 2017.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 "LCDB Data for (2055) Dvořák". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2055%7CDvořák. Retrieved 29 June 2017.
- ↑ 5.0 5.1 5.2 Mazzone, Fernando; Colazo, Carlos; Mina, Federico; Melia, Raul; Spagnotto, Julio; Bernal, Alejandro (January 2014). "Collaborative Asteroid Photometry and Lightcurve Analysis at Observatories OAEGG, OAC, EABA, and OAS". The Minor Planet Bulletin 41 (1): 17–19. ISSN 1052-8091. Bibcode: 2014MPBu...41...17M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014MPBu...41...17M. Retrieved 29 June 2017.
- ↑ 6.0 6.1 Oey, Julian (October 2014). "Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2013". The Minor Planet Bulletin 41 (4): 276–281. ISSN 1052-8091. Bibcode: 2014MPBu...41..276O. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014MPBu...41..276O. Retrieved 29 June 2017.
- ↑ 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 29 June 2017.
- ↑ 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. https://archive.org/details/dictionaryminorp2008schm.
External links
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 2055 Dvořák at AstDyS-2, Asteroids—Dynamic Site
- 2055 Dvořák at the JPL Small-Body Database
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