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11066 Sigurd
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Near-Earth asteroid
October 2019
yes 11066 Sigurd #FFC2E0 11066 Sigurd.jpg An image of 11066 Sigurd as seen by the Arecibo and Goldstone radar observatories 9 February 1992 C. Shoemaker
E. Shoemaker
Palomar Obs. (11066) Sigurd 1992 CC 1
1987 GE
Sigurd (Norse mythology) NEO
Apollo
4 September 2017 (JD 2458000.5) 0 41.22 yr (15,057 days) 1.9138 AU 0.8691 AU 1.3915 AU 0.3754 1.64 yr (600 days) 314.05° 0.6005 ms / day 36.883° 349.25° 22.006° 0.1183 AU (46.1 LD) 2.10 0.09 km
2.778 0.115 km
2.86 km (calculated)
8.4958 h
8.496 h
8.51 0.01 h
0.18 (assumed)
0.190 0.033
0.29 0.04
0.38 0.31
SMASS K
Sr
S
K
15.00
15.2
15.36
15.51 0.31
11066 Sigurd (provisional designation 1992 CC 1) is a stony contact binary asteroid classified as a near-Earth object of the Apollo group of asteroids, approximately 2.5 kilometers in diameter.
It was discovered on 9 February 1992 by American astronomer couple Carolyn and Eugene Shoemaker at Palomar Observatory, California, and named after Sigurd, a hero from Norse mythology.
Orbit and classification
Sigurd orbits the Sun in the inner main-belt at a distance of 0.9–1.9 AU once every 1 years and 8 months (600 days). Its orbit has an eccentricity of 0.38 and an inclination of 37° with respect to the ecliptic. A first precovery was taken at the Australian Siding Spring Observatory in 1978, and it was identified as 1987 GE at Palomar in 1987. Both observations remained unused. The body's observation arc begins with its official discovery observation at Palomar in 1992.
It has an Earth minimum orbital intersection distance of 0.1183 AU km on off 3, which corresponds to 46.1 lunar distances.
Physical characteristics
In the SMASS taxonomy, Sigurd is a relatively rare K-type asteroid, which fall into the broader stony S-complex. It has also been grouped into the common S-type asteroid. The ExploreNEOs Warm Spitzer program, using the NASA Infrared Telescope Facility on Mauna Kea Observatory in Hawaii, classifies Sigurd as a Sr-type, which transitions to the R-type asteroids.
Contact binary
Radiometric observations at Arecibo Observatory revealed that Sigurd is a contact binary, composed of two lobes in contact with each other. The more or less ellipsoidal lobes are elongated and joined on their long axis. The body has an axial tilt of 50° to 130°. The observing astronomers also note, that more than 10% of all larger (> 200 meters) near-Earth objects observed by radar are such contact binaries.
Photometry
Rotational lightcurves obtained from photometric observations by Petr Pravec, Brian Warner and by a group of German and Ukrainian astronomers, gave a well-defined rotation period of 8.4958 to 8.51 hours. The analysis of the constructed lightcurves also gave a high brightness amplitude between 0.97 and 1.15 magnitude, which is indicative that Sigurd has a non-spheroidal shape (U=3/3/3).
Diameter and albedo
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Sigurd measures between 2.10 and 2.778 kilometers in diameter and its surface has an albedo of 0.190 and 0.29, respectively. Observations by the ExploreNEOs survey give a higher albedo of 0.38. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.18 and calculates a diameter of 2.86 kilometers with an absolute magnitude of 15.2, while radiometric observations of Sigurd gave a maximum dimensions of 4.2 kilometers.
Naming
This minor planet was named after Sigurd, a legendary hero in Norse mythology. In the Völsunga saga, Sigurd rides through a ring of fire to awaken the shieldmaiden Brynhild (123 123 Brunhild), and later dies in a fight with Odin (3989 3989 Odin). Sigurd is also known as the dragon-slayer Siegfried in the German poem The Song of the Nibelungs. The approved naming citation was published by the Minor Planet Center on 23 May 2000 (M.P.C. 40706).
References
30em 2017-06-22 last obs.
JPL Small-Body Database Browser: 11066 Sigurd (1992 CC1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2011066
Jet Propulsion Laboratory
5 July 2017
Dictionary of Minor Planet Names – (11066) Sigurd
Schmadel Lutz D.
Springer Berlin Heidelberg
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10.1007/978-3-540-29925-7_8204 (11066) Sigurd
11066 Sigurd (1992 CC1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=11066
5 April 2017
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
5 April 2017
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P. A. Taylor
E. Howell
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J. D. Giorgini
October 2012
Radar Imaging Of 11066 Sigurd, 2000 YF29, And 2004 XL14 And The Obliquity Distribution Of Contact Binary Near-Earth Asteroids
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American Astronomical Society
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External links
IAUC 5459 (discovery 1992 CC 1), Central Bureau for Astronomical Telegrams, 27 February 1992
Contact Binary Asteroids and Comets, Robert Johnston, list at jonstonsarchive.net, 25 March 2017
Binary and Ternary near-Earth Asteroids detected by radar, Lance A. M. Benner, ASA/JPL Asteroid Radar Research
(11066) Sigurd at NEODyS-2
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 Observatoire de Genève, Raoul Behrend
11066
11066 Sigurd
(11065) 1991 XE2 11066 11067 Greenancy
011066
Category:Discoveries by Eugene Merle Shoemaker
Category:Discoveries by Carolyn S. Shoemaker
Category:Named minor planets
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