936 Kunigunde
Template:Short description Template:Use dmy dates Script error: No such module "infobox".Script error: No such module "Check for unknown parameters".
936 Kunigunde (prov. designation: Template:Mp or Template:Mp) is a dark Themistian asteroid from the outer regions of the asteroid belt, approximately Script error: No such module "convert". in diameter. It was discovered on 8 September 1920, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory.[1] The carbonaceous B-type asteroid has a rotation period of 9.4 hours. It was named "Kunigunde", a common German female name unrelated to the discoverer's contemporaries, that was taken from the almanac Lahrer Hinkender Bote.[2]
Orbit and classification
Kunigunde is a core member of the Themis family (602Script error: No such module "Check for unknown parameters".), when applying the hierarchical clustering method to its proper orbital elements. The very large family of carbonaceous asteroids is named after 24 Themis.[3][4][5]Template:Rp Kunigunde orbits the Sun in the outer main-belt at a distance of 2.6–3.7 AU once every 5 years and 6 months (2,025 days; semi-major axis of 3.13 AU). Its orbit has an eccentricity of 0.18 and an inclination of 2° with respect to the ecliptic.[6] The asteroid was first observed as Template:Mp (Template:Mp) at Simeiz Observatory on 27 April 1913. The body's observation arc begins at Heidelberg with its official discovery observation on 8 September 1920.[1]
Naming
This minor planet was named "Kunigunde", after a female name picked from the Lahrer Hinkender Bote, published in Lahr, southern Germany.[2][7] A Hinkender Bote (lit. "limping messenger") was a very popular almanac, especially in the Alemannic-speaking region from the late 17th throughout the early 20th centuries. The calendar section contains feast days, the dates of important fairs and astronomical ephemerides. For 3 March, the calendar gives "Kunigund" as the German name day analogue next to Kunigunde and Titian, the protestant and catholic entries in the calendar of saints, likely referring to Cunigunde of Luxembourg and Titian of Brescia.[8]
Reinmuth's calendar names
As with 22 other asteroids—starting with 913 Otila, and ending with 1144 Oda—Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries. Lutz Schmadel, the author of the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]
Physical characteristics
In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Kunigunde is a B-type asteroid, a somewhat brighter spectral type than the common C type typical for Themistian asteroids.[4][9]
Rotation period and poles
In March 2018, a rotational light curve of Kunigunde was obtained from photometric observations by French amateur astronomer René Roy. Light-curve analysis gave a well-defined rotation period of Script error: No such module "val". hours with a brightness variation of Script error: No such module "val". magnitude (U=3Script error: No such module "Check for unknown parameters".).[10] Richard Ditteon at the Oakley Southern Sky Observatory Template:Obscode determined a period of Script error: No such module "val". with an amplitude of Script error: No such module "val". magnitude (U=2Script error: No such module "Check for unknown parameters".).[11] Photometry by Angeli and Guimarães at observatories in Brazil and Argentina gave a similar period of Script error: No such module "val". hours (U=2Script error: No such module "Check for unknown parameters".).[12] In 2013, an international study modeled a light curve with a sidereal period of 8.82653 hours and found two spin axes at (47.0°, 57.0°) and (234.0°, 50.0°) in ecliptic coordinates (λ, β) (U=n.a.Script error: No such module "Check for unknown parameters".).[13]
Diameter and albedo
According to the survey carried out by the Japanese Akari satellite, the Infrared Astronomical Satellite IRAS, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Kunigunde measures (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".) kilometers in diameter and its surface has an albedo of (Script error: No such module "val".), (Script error: No such module "val".) and (Script error: No such module "val".), respectively.[14][15][16]
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0792 and a diameter of 39.29 kilometers based on an absolute magnitude of 10.4.[12] Further published mean-diameters and albedos by the WISE team include (Script error: No such module "val".) and (Script error: No such module "val".) with corresponding albedos of (Script error: No such module "val".) and (Script error: No such module "val".).[4][12] An asteroid occultation on 21 November 2004, gave a best-fit ellipse dimension of 39.0 × 39.0 km.[4] These timed observations are taken when the asteroid passes in front of a distant star. However, the quality of the measurement is poorly rated.[4]
References
<templatestyles src="Reflist/styles.css" />
- ↑ a b Script error: No such module "citation/CS1".
- ↑ a b c Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1".
- ↑ a b c d e Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1". Lahrer Bote archive
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "Citation/CS1".
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "Citation/CS1".
- ↑ a b c Script error: No such module "citation/CS1".
- ↑ Script error: No such module "Citation/CS1".
- ↑ Script error: No such module "Citation/CS1". (online, AcuA catalog p. 153)
- ↑ Script error: No such module "Citation/CS1".
- ↑ Script error: No such module "Citation/CS1".
Script error: No such module "Check for unknown parameters".
External links
- Lightcurve Database Query (LCDB), at www.minorplanet.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) – Minor Planet Center
- Template:AstDys
- Template:PAGENAMEBASE at the JPL Small-Body DatabaseTemplate:EditAtWikidata
Script error: No such module "Navbox". Script error: No such module "Navbox". Template:Authority control