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1537 Transylvania

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1537 Transylvania
background#D6D6D6
imageFile:001537-asteroid shape model (1537) Transylvania.png
captionA lightcurve-derived shape model of Transylvania
discovery_ref
discovererG. Strommer
discovery_siteKonkoly Obs.
discovered27 August 1940
mpc_name(1537) Transylvania
alt_names1940 QA1940 QN
A903 VB
named_afterTransylvania
(region in Romania)
mp_categorymain-belt(outer)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc113.42 yr (41,428 days)
aphelion3.9677 AU
perihelion2.1361 AU
semimajor3.0519 AU
eccentricity0.3001
period5.33 yr (1,947 days)
mean_anomaly143.95°
mean_motion/ day
inclination3.8591°
asc_node230.07°
arg_peri148.20°
dimensions13.60 km (derived)
km
km
km
km
km
rotationh
albedo
0.1047 (derived)
spectral_typeC
abs_magnitude11.9012.3012.3212.4

A903 VB (region in Romania) km km km km km

0.1047 (derived)

1537 Transylvania (provisional designation ****) 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.

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.

Kristensen was able to show that Transylvania was first observed as 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.

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.

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.

Physical characteristics

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

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 (). As of 2017, no other lightcurve has been obtained, and Transylvania's period is still uncertain.

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.

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.

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). 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).

References

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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