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1556 Wingolfia

Metallic main-belt asteroid


Metallic main-belt asteroid

FieldValue
minorplanetyes
name1556 Wingolfia
background#D6D6D6
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered14 January 1942
mpc_name(1556) Wingolfia
alt_names1942 AA
pronounced
named_afterWingolf (student fraternity)
mp_categorymain-belt(outer)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc75.20 yr (27,468 days)
aphelion3.7979 AU
perihelion3.0531 AU
semimajor3.4255 AU
eccentricity0.1087
period6.34 yr (2,316 days)
mean_anomaly99.491°
mean_motion/ day
inclination15.750°
asc_node91.594°
arg_peri269.34°
dimensionskm
km
rotationh
albedo
spectral_typeTholen XC
XM
B–V 0.708
U–B 0.202
abs_magnitude10.55

km

XM B–V 0.708 U–B 0.202

1556 Wingolfia (provisional designation ****) is a metallic asteroid from the outer regions of the asteroid belt, approximately 30 kilometers in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 14 January 1942. The asteroid was named after Wingolf, a student fraternity in Heidelberg.

Orbit and classification

Wingolfia is a non-family asteroid from the background population of the asteroids belt. It orbits the Sun in the outer main belt at a distance of 3.1–3.8 AU once every 6 years and 4 months (2,316 days). Its orbit has an eccentricity of 0.11 and an inclination of 16° with respect to the ecliptic. The body's observation arc begins at Heidelberg with its official discovery observation in January 1942.

Physical characteristics

In the Tholen classification, Wingolfia has an ambiguous spectral type, similar to the X-types (which includes the M-type asteroids) with some resemblance to the carbonaceous C-types. It has also been characterized as an M- and X-type, by direct photometric observations and by PanSTARRS photometric survey, respectively. The Lightcurve Data Base adopts an M-type.

Rotation period

In October 1990, a rotational lightcurve of Wingolfia was obtained from photometric observations by Italian astronomers at ESO's La Silla Observatory using the ESO 1-metre telescope. Lightcurve analysis gave a rotation period of 10 hours with a brightness variation of 0.15 magnitude ().

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS and the Japanese Akari satellite, Wingolfia measures 28.65 and 33.88 kilometers in diameter and its surface has an albedo of 0.093 and 0.1297, respectively. The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS. All diameter measurements are based on an absolute magnitude of 10.55.

Naming

This minor planet was named by the discoverer after Wingolf, which is one of Germany's long-standing Christian student fraternity in Heidelberg, that was prohibited during Nazi Germany, and reinstalled after WWII. The official was published by the Minor Planet Center in May 1955 (M.P.C. 1221). The asteroid's name was announced on 17 June 1955, during the celebration of the fraternity's 104th anniversary. The discoverer's original citation reads:

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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