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1323 Tugela

From Wikipedia, the free encyclopedia
Dark background asteroid

1323 Tugela
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date19 May 1934
Designations
(1323) Tugela
Named after
Tugela River[2]
(South Africanriver)
1934 LD · 1974 HR3
1974 KM · 1974 KO
A908 UB · A911 HC
main-belt · (outer)[1][3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.02 yr (39,818 days)
Aphelion3.7100AU
Perihelion2.7510 AU
3.2305 AU
Eccentricity0.1484
5.81yr (2,121 days)
234.50°
0° 10m 10.92s / day
Inclination18.787°
45.241°
136.10°
Physical characteristics
Dimensions58.44±3.4 km[5]
58.50 km(derived)[3]
62.00±19.32 km[6]
63.45±0.94 km[7]
67.76±25.28 km[8]
78.295±0.511 km[9]
90.557±0.542 km[10]
110.11±1.73 km[11]
19.50±0.02h[12][a]
19.777±0.0365 h[13]
0.018±0.004[11]
0.0236±0.0044[10]
0.04±0.02[6]
0.04±0.03[8]
0.048±0.002[7]
0.0567±0.007[5]
0.0620(derived)[3]
SMASS =Xc[1]
P[10] · C(assumed)[3]
9.56±0.62[14] · 9.80[3][11] · 9.84[8] · 9.90[1][5][6][7][10] · 10.245±0.001(S)[13]

1323 Tugela, provisional designation1934 LD, is a dark backgroundasteroid from the outer regions of theasteroid belt, approximately 60 kilometers in diameter. It was discovered on 19 May 1934, by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[15] The asteroid was named for theTugela River in western South Africa.[2]

Orbit and classification

[edit]

Tugela is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter main-belt at a distance of 2.8–3.7 AU once every 5 years and 10 months (2,121 days;semi-major axis of 3.23 AU). Its orbit has aneccentricity of 0.15 and aninclination of 19° with respect to theecliptic.[1]

The body'sobservation arc begins with its first identification asA908 UB atHeidelberg Observatory in October 1908, almost 26 years prior to its official discovery observation at Johannesburg.[15]

Physical characteristics

[edit]

In theSMASS classification,Tugela is an Xc-subtype that transitions from theX-type to the carbonaceousC-type asteroids.[1] TheWide-field Infrared Survey Explorer (WISE) characterized it as a primitiveP-type asteroid, while theCollaborative Asteroid Lightcurve Link (CALL) assumes it to be a C-type.[3][10]

Rotation period

[edit]

Observations performed by American astronomerBrian Warner at thePalmer Divide Observatory in Colorado Springs, Colorado, during February 2007 produced alightcurve with a period of 19.50 ± 0.02 hours and an amplitude of 0.25 ± 0.02 inmagnitude (U=3).[12][a] In September 2011, photometry in the S-band at thePalomar Transient Factory gave a similar period of 19.777 hours with a brightness variation of 0.18 magnitude (U=2).[13]

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,Tugela measures between 58.44 and 110.11 kilometers in diameter and its surface has analbedo between 0.018 and 0.0567.[5][6][7][8][9][10][11]

CALL largely agrees with IRAS and derives an albedo of 0.0620 with a diameter of 58.50 kilometers based on anabsolute magnitude of 9.8.[3]

Naming

[edit]

Thisminor planet was named after theTugela River, the largest river in theKwaZulu-Natal Province of western South Africa. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 121).[2]

Notes

[edit]
  1. ^abLightcurve plot of 1323 Tugela, Palmer Divide Observatory, B. D. Warner (2007). Summary figures at theLCDB

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 1323 Tugela (1934 LD)" (2017-11-02 last obs.).Jet Propulsion Laboratory. Retrieved30 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1323) Tugela".Dictionary of Minor Planet Names – (1323) Tugela.Springer Berlin Heidelberg. p. 108.doi:10.1007/978-3-540-29925-7_1324.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1323) Tugela". Asteroid Lightcurve Database (LCDB). Retrieved30 November 2017.
  4. ^ab"Asteroid 1323 Tugela – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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.
  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.S2CID 9341381. Retrieved30 November 2017.
  7. ^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)
  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. ^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.S2CID 119293330.
  10. ^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.S2CID 35447010.
  11. ^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.S2CID 46350317. Retrieved30 November 2017.
  12. ^abWarner, Brian D. (September 2007)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory - December 2006 - March 2007".The Minor Planet Bulletin.34 (3):72–77.Bibcode:2007MPBu...34...72W.ISSN 1052-8091. Retrieved30 November 2017.
  13. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929. Retrieved30 November 2017.
  14. ^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.S2CID 53493339. Retrieved30 November 2017.
  15. ^ab"1323 Tugela (1934 LD)".Minor Planet Center. Retrieved30 November 2017.

External links

[edit]
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