Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

1493 Sigrid

From Wikipedia, the free encyclopedia
Dark Nysian asteroid

1493 Sigrid
Shape ofSigrid modelled from itslightcurve
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date26 August 1938
Designations
(1493) Sigrid
Named after
Sigrid Strömgren[2]
(wife of astronomer)
Bengt Strömgren
1938 QB · 1934 NB1
1934 PW · 1957 UT
1961 TM1 · 1961 XL
1977 UN · A908 WA
A916 YD
main-belt · (inner)
Nysa[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc108.52 yr (39,636 days)
Aphelion2.9175AU
Perihelion1.9416 AU
2.4295 AU
Eccentricity0.2009
3.79yr (1,383 days)
318.09°
0° 15m 37.08s / day
Inclination2.5772°
330.58°
1.6890°
Physical characteristics
Dimensions22.111±0.200 km[5]
22.93±6.77 km[6]
23±2 km[7]
23.76±3.46 km[8]
24.03±2.1 km[3][9]
24.92±8.61 km[10]
25.10±0.42 km[11]
27.8±5.6 km[12]
28.905±0.401 km[13]
22.68±0.02 h[14]
43.179±0.005 h[15]
43.1795±0.0001 h[16]
43.296±0.048h[17]
0.034±0.007[13]
0.036±0.067[10]
0.0398±0.0028[5]
0.04±0.02[6][12]
0.04±0.03[8]
0.048±0.002[11]
0.0489±0.010[9]
0.05±0.01[7]
Tholen =F[1][3]
SMASS = Xc[1] · P[5]
B–V = 0.643[1]
U–B = 0.225[1]
11.99[1][3][5][6][7][9][11][12] · 12.24[8][10] · 12.35±0.23[18]

1493 Sigrid, provisional designation1938 QB, is a dark Nysianasteroid from the inner regions of theasteroid belt, approximately 24 kilometers in diameter. It was discovered on 26 August 1938, by Belgian astronomerEugène Delporte at theRoyal Observatory of Belgium in Uccle.[19] It was named after Sigrid Strömgren, wife of astronomerBengt Strömgren.[2]

Orbit and classification

[edit]

Sigrid is a member of theNysa family (405),[4] the largestasteroid family of the main belt, consisting of stony and carbonaceous subfamilies. The family, named after44 Nysa, is located in the inner belt near theKirkwood gap (3:1 orbital resonance with Jupiter), a depleted zone that separates the central main belt.[20]: 23 

It orbits the Sun in theinner main-belt at a distance of 1.9–2.9 AU once every 3 years and 9 months (1,383 days). Its orbit has aneccentricity of 0.20 and aninclination of 3° with respect to theecliptic.[1] The asteroid was first identified asA908 WA atHeidelberg Observatory in November 1908. The body'sobservation arc begins with its official discovery observation at Uccle in August 1938.[19]

Physical characteristics

[edit]

Spectral type

[edit]

In theTholen classification,Sigrid is anF-type asteroid (which agrees with the overallspectral type of the Polanian subgroup).[1][3] In theSMASS classification, it is a Xc-subtype, which transitions between theX- andC-type asteroids.[1] It has also been characterized as a primitiveP-type asteroid by theWide-field Infrared Survey Explorer (WISE).[5]

Photometry

[edit]

Rotation period an amplitude

[edit]

In August 2006, a rotationallightcurve ofSigrid was obtained from photometric observations at the Mount Tarana and Cecil Observatory in NSW, Australia. Lightcurve analysis gave arotation period of 43.296 hours with a brightness variation of 0.6magnitude (U=2).[17] In October 2010, Raymond Poncy found a period of 22.68 hours (or half the previous period solution) and an amplitude of 0.38 magnitude (U=2-).[14] While not being aslow rotator, the body's period is significantly longer than the typical 2 to 20 hours seen among the majority of asteroids.

Spin axis

[edit]

The asteroids lightcurve has also been modeled, using photometric data from the Lowell Photometric Database (LPD) and other sources. Modelling gave a concurring period of 43.179 and 43.1795 hours,[15][16] as well as two spin axis of (183.0°, 69°) and (350.0°, 69°) inecliptic coordinates (λ, β).[16]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Sigrid measures between 22.111 and 28.905 kilometers in diameter and its surface has a lowalbedo between 0.034 and 0.05.[5][6][7][8][9][10][11][12][13]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is an albedo of 0.0489 and a diameter of 24.03 kilometers based on anabsolute magnitude of 11.99.[3]

Naming

[edit]

Thisminor planet was named after Sigrid Strömgren, wife of the Danish-American astronomerBengt Strömgren, after whom the asteroid1846 Bengt was named. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 134;RI 2297).[2]

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 1493 Sigrid (1938 QB)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved19 October 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1493) Sigrid".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 119.doi:10.1007/978-3-540-29925-7_1494.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1493) Sigrid". Asteroid Lightcurve Database (LCDB). Retrieved19 October 2017.
  4. ^ab"Asteroid 1493 Sigrid – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^abcdefMainzer, 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.
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved19 October 2017.
  7. ^abcdAlí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013)."Physical properties of B-type asteroids from WISE data".Astronomy and Astrophysics.554: 16.arXiv:1303.5487.Bibcode:2013A&A...554A..71A.doi:10.1051/0004-6361/201220680. Retrieved19 October 2017.
  8. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  9. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  10. ^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. Retrieved19 October 2017.
  11. ^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)
  12. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids"(PDF).Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660. Retrieved19 October 2017.
  13. ^abcMasiero, 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. Retrieved19 October 2017.
  14. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1493) Sigrid".Geneva Observatory. Retrieved19 October 2017.
  15. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved19 October 2017.
  16. ^abcDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved19 October 2017.
  17. ^abBembrick, Colin; Byron, Jeff (March 2007)."A Rotation Period for 1493 Sigrid".The Minor Planet Bulletin.34 (1): 1.Bibcode:2007MPBu...34....1B.ISSN 1052-8091. Retrieved19 October 2017.
  18. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved19 October 2017.
  19. ^ab"1493 Sigrid (1938 QB)".Minor Planet Center. Retrieved19 October 2017.
  20. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=1493_Sigrid&oldid=1233136834"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp