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1130 Skuld

From Wikipedia, the free encyclopedia
Florian asteroid

1130 Skuld
Modelled shape ofSkuld from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date2 September 1929
Designations
(1130) Skuld
Named after
Skuld(Norse mythology)[2]
1929 RC · 1928 FJ
1949 UD · 1962 LA
A906 VC
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.38 yr (40,316 days)
Aphelion2.6701AU
Perihelion1.7864 AU
2.2282 AU
Eccentricity0.1983
3.33yr (1,215 days)
173.35°
0° 17m 46.68s / day
Inclination2.1677°
216.13°
113.81°
Physical characteristics
Dimensions9.63±0.44 km[4]
9.99 km(derived)[3]
10.125±0.092 km[5]
10.24±0.64 km[6]
11.009±0.091 km[7]
4.73±0.02h[8]
4.807±0.002 h[9]
4.8079±0.0005 h[10]
4.810 h[a]
0.1995±0.0461[7]
0.24(assumed)[3]
0.244±0.033[6]
0.302±0.031[4]
S[3]
12.0[1][4] · 12.10[6] · 12.17[3][7] · 12.17±0.02[9]

1130 Skuld, provisional designation1929 RC, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 10 kilometers in diameter. It was named afterSkuld from Norse mythology.[2]

Discovery

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Skuld was discovered on 2 September 1929, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[11] The body was independently discovered by astronomers and fellow countrymenArnold Schwassmann andArno Wachmann at the HamburgerBergedorf Observatory ten nights later.[2]

It was first identified asA906 VC at Heidelberg in 1906, extending the asteroid'sobservation arc by 23 years prior to its official discovery observation.[11]

Orbit and classification

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Skuld is a member of theFlora family, one of the largest groups of stonyS-type asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,215 days). Its orbit has aneccentricity of 0.20 and aninclination of 2° with respect to theecliptic.[1]

Naming

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Thisminor planet was named afterSkuld, one of the three Norns inNorse mythology. The asteroids167 Urda and621 Werdandi are named after the other twoNorns.[2] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 110).[2]

Physical characteristics

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Rotation period

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In January 2004, the first rotationallightcurves ofSkuld were obtained by Henk de Groot and by a group of Polish and French astronomers. Lightcurve analysis gave arotation period of 4.73 and 4.8079 hours with a brightness variation of 0.46 and 0.40magnitude, respectively (U=2+/3-).[8][10]

In 2009 and 2011, astronomers Robert Buchheim andLarry Robinson obtained two well-defined lightcurves from photometric observations. They gave a refined period of 4.810 and 4.807 hours with an amplitude of 0.50 and 0.26 magnitude, respectively (U=3/3).[9][a]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Skuld measures between 9.63 and 11.009 kilometers in diameter and its surface has analbedo between 0.1995 and 0.302.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 9.99 kilometers with anabsolute magnitude of 12.17.[3]

Notes

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  1. ^abRobinson (2011) web: rotation period4.810 hours with a brightness amplitude of0.5 mag. Summary figures for (1130) Skuld at2=Collaborative Asteroid Lightcurve Link (CALL)

References

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  1. ^abcd"JPL Small-Body Database Browser: 1130 Skuld (1929 RC)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved26 July 2017.
  2. ^abcdeSchmadel, Lutz D. (2007). "(1130) Skuld".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 96.doi:10.1007/978-3-540-29925-7_1131.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1130) Skuld". Asteroid Lightcurve Database (LCDB). Retrieved12 February 2017.
  4. ^abcdMasiero, 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.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved12 February 2017.
  5. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved12 February 2017.
  6. ^abcdUsui, 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.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  7. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1130) Skuld".Geneva Observatory. Retrieved12 February 2017.
  9. ^abcBuchheim, Robert K. (April 2010)."Lightcurve and Phase Curve of 1130 Skuld".The Minor Planet Bulletin.37 (2):41–42.Bibcode:2010MPBu...37...41B.ISSN 1052-8091. Retrieved12 February 2017.
  10. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199. Retrieved12 February 2017.
  11. ^ab"1130 Skuld (1929 RC)".Minor Planet Center. Retrieved12 February 2017.

External links

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