Astronomy:1537 Transylvania

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1537 Transylvania
001537-asteroid shape model (1537) Transylvania.png
Discovery[1]
Discovered byG. Strommer
Discovery siteKonkoly Obs.
Discovery date27 August 1940
Designations
(1537) Transylvania
Named afterTransylvania[2]
(region in Romania)
1940 QA · 1940 QN
A903 VB
Minor planet categorymain-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc113.42 yr (41,428 days)
|{{{apsis}}}|helion}}3.9677 AU
|{{{apsis}}}|helion}}2.1361 AU
3.0519 AU
Eccentricity0.3001
Orbital period5.33 yr (1,947 days)
Mean anomaly143.95°
Mean motion0° 11m 5.64s / day
Inclination3.8591°
Longitude of ascending node230.07°
148.20°
Physical characteristics
Dimensions13.60 km (derived)[3]
13.77±1.5 km[4]
17.48±1.16 km[5]
20.288±0.256 km[6]
20.29±0.26 km[6]
21.49±1.58 km[7]
Rotation period12 h[8]
Geometric albedo0.05±0.00[5]
0.052±0.006[6]
0.067±0.010[7]
0.1047 (derived)[3]
0.1619±0.041[4]
C[3][9]
Absolute magnitude (H)11.90[7][4] · 12.12±0.49[9] · 12.30[6] · 12.32[5] · 12.4[1][3]


1537 Transylvania, provisional designation 1940 QA, is a carbonaceous asteroid and long-lost minor planet from the outer regions of the asteroid belt, approximately 17 kilometers in diameter. Discovered by Gyula Strommer in 1940, it was later named after region of Transylvania, where the discoverer was born.[10]

Discovery and rediscovery

Transylvania was discovered on 27 August 1940, by Hungarian astronomer Gyula Strommer at the Konkoly Observatory near Budapest, Hungary. Observations of the asteroid continued at Konkoly until February 1942. It became a lost minor planet until Spring 1981, when astronomer Leif Kahl Kristensen at the University of Aarhus rediscovered it based on contemporary observations at Palomar Observatory.[10][11]

Kristensen was able to show that Transylvania was first observed as A903 VB at Heidelberg Observatory in October 1903, and, after its observations at Konkoly in the early 1940s, it was again observed at Goethe Link Observatory in December 1962, and at Palomar in February 1981.[10][11]

Remaining lost minor planets

At the same time, Kristensen also rediscovered 452 Hamiltonia. With these two rediscoveries in 1981, only nine numbered minor planets remained unobserved since their discoveries: 330 Adalberta, 473 Nolli, 719 Albert, 724 Hapag, 843 Nicolaia, 878 Mildred, 1009 Sirene, 1026 Ingrid, and 1179 Mally.[11]

Orbit and classification

Transylvania is a non-family asteroid of the main belt's background population. It orbits the Sun in the outer main-belt at a distance of 2.1–4.0 AU once every 5 years and 4 months (1,947 days). Its orbit has an eccentricity of 0.30 and an inclination of 4° with respect to the ecliptic.[1]

Physical characteristics

Transylvania has been characterized as a carbonaceous C-type asteroid by PanSTARRS photometric survey.[9]

Rotation period

In September 2004, a rotational lightcurve of Transylvania was obtained from photometric observations by French amateur astronomer Laurent Bernasconi. Analysis of the fragmentary lightcurve gave a rotation period of 12 hours with a brightness amplitude of 0.15 magnitude ({{{1}}}).[8] As of 2017, no other lightcurve has been obtained, and Transylvania's period is still uncertain.[3]

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, Transylvania measures between 13.77 and 21.49 kilometers in diameter and its surface has an albedo between 0.05 and 0.1619.[4][5][6][7]

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1047 and a diameter of 13.60 kilometers based on an absolute magnitude of 12.4.[3]

Naming

This minor planet was named after the historical region of Transylvania, located in what is now Romania. Formerly, it was part of the Austro-Hungarian Empire. Transylvania is also the birthplace of the discoverer Gyula Strommer (1920–1995).[2] Transylvania was his only minor-planet discovery. The official naming citation was published by the Minor Planet Center on 1 February 1980 (M.P.C. 5182).[12]

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1537 Transylvania (1940 QA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001537. Retrieved 20 September 2017. 
  2. ↑ 2.0 2.1 Schmadel, Lutz D. (2007). "(1537) Transylvania". Dictionary of Minor Planet Names – (1537) Transylvania. Springer Berlin Heidelberg. p. 122. doi:10.1007/978-3-540-29925-7_1538. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 "LCDB Data for (1537) Transylvania". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1537%7CTransylvania. Retrieved 20 September 2017. 
  4. ↑ 4.0 4.1 4.2 4.3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019. 
  5. ↑ 5.0 5.1 5.2 5.3 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T. et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal 152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. 
  6. ↑ 6.0 6.1 6.2 6.3 6.4 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C. et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 20 September 2017. 
  7. ↑ 7.0 7.1 7.2 7.3 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  8. ↑ 8.0 8.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1537) Transylvania". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001537. Retrieved 20 September 2017. 
  9. ↑ 9.0 9.1 9.2 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 20 September 2017. 
  10. ↑ 10.0 10.1 10.2 "1537 Transylvania (1940 QA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1537. Retrieved 20 September 2017. 
  11. ↑ 11.0 11.1 11.2 Kristensen, L. K.; Gibson, J.; Shao, C.-Y.; Bowell, E.; Marsden, B. G. (April 1981). "(1537) Transylvania and (452) Hamiltonia". IAU Circ. 3595 (3595): 1. Bibcode: 1981IAUC.3595....1K. http://www.cbat.eps.harvard.edu/iauc/03500/03595.html#Item1. Retrieved 20 September 2017. 
  12. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. Retrieved 20 September 2017. 

External links



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