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1171 Rusthawelia

From Wikipedia, the free encyclopedia
Main-belt asteroid

1171 Rusthawelia
Shape model ofRusthawelia from itslightcurve
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date3 October 1930
Designations
(1171) Rusthawelia
Named after
Shota Rustaveli
(Georgian poet)[2]
1930 TA · 1926 AD
1926 FH · 1927 FC
1949 BT · A904 EB
A913 TA
main-belt · (outer)[3]
background[4]
Orbital characteristics[5]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc113.85yr (41,584 d)
Aphelion3.7970AU
Perihelion2.5779 AU
3.1875 AU
Eccentricity0.1912
5.69 yr (2,079 d)
175.66°
0° 10m 23.52s / day
Inclination3.0731°
121.78°
290.57°
Physical characteristics
68.67±16.71 km[6]
70.13±2.3 km[7]
70.216±1.560 km[8]
70.98±2.42 km[9]
72.09±1.19 km[10]
72.38±20.19 km[11]
82.229±1.004 km[12]
Mass(1.81±0.20)×1018 kg[9]
9.66±1.45 g/cm3[9]
10.80±0.01 h[13]
10.98±0.01 h[14]
11.013±0.003 h[15]
0.029±0.003[12]
0.038±0.002[10]
0.0393±0.0051[8]
0.0394±0.003[7]
0.04±0.02[6][11]
Tholen =P[3][5] · P[8]
B–V = 0.678[5]
U–B = 0.255[5]
9.89[11]
9.90[3][5][6][7][8][10][12]
9.94±0.16[16]

1171 Rusthawelia, provisional designation1930 TA, is a large and darkbackground asteroid, approximately 72 kilometers (45 miles) in diameter, located in the outer regions of theasteroid belt. It was discovered on 3 October 1930, by Belgian astronomerSylvain Arend at theRoyal Observatory of Belgium in Uccle, and was an unnoticed rediscovery of alost minor planet then known as "Adelaide".[1] As the asteroid was already named for Georgian poetShota Rustaveli when the rediscovery was realized, its former designation was given to another asteroid instead, which is now known as525 Adelaide.[2]Rusthawelia is a primitiveP-type asteroid and has arotation period of 11 hours.

Unnoticed rediscovery of lost asteroid

[edit]

When Arend discoveredRusthawelia in 1930, it was not realized that he rediscovered the long-lost asteroid "525 Adelaide". It was already discovered 26 years earlier asA904 EB by German astronomerMax Wolf atHeidelberg Observatory in March 1904, who observed it for a short time during the discovery opposition before it became lost. Only decades later, in 1958, it was shown by French astronomerAndré Patry that both asteroid's discovered by Wolf and Arend were one and the same (M.P.C. 1831). It was then decided that this asteroid retains the number–name designation "1171 Rusthawelia", while525 Adelaide was vacated and given to another asteroid (which was the object1908 EKa, discovered byJoel Hastings Metcalf).[5][17]

Another confusion occurred in 1929, one year before Arend's discovery, when American astronomerAnne Sewell Young thought to have found long-lost "Adelaide", when in fact she mistook the asteroid for comet31P/Schwassmann–Wachmann that had a very similarorbital eccentricity.[18]

Orbit and classification

[edit]

Rusthawelia is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter main-belt at a distance of 2.6–3.8 AU once every 5 years and 8 months (2,079 days;semi-major axis of 3.19 AU). Its orbit has aneccentricity of 0.19 and aninclination of 3° with respect to theecliptic.[5] The body'sobservation arc begins asA904 EB at Heidelberg in March 1904, when it was discovered by Max Wolf(see above).[1]

Naming

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Thisminor planet was named for medieval Georgian poetShota Rustaveli (შოთა რუსთაველი, c. 1160 – after c. 1220). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 109).[2]

Physical characteristics

[edit]

Rusthawelia is a dark and primitiveP-type asteroid, as characterized by theWide-field Infrared Survey Explorer (WISE),[8] andclassified by Tholen.[5][3]

Rotation period

[edit]

In October and November 2003, two rotationallightcurves ofRusthawelia were obtained from photometric observations by John Menke at his observatory in Barnesville, Maryland, and by a group of American astronomers. Lightcurve analysis gave a well-definedrotation period of 10.80 and 10.98 hours and a brightness variation of 0.31 and 0.26magnitude, respectively (U=3/3).[13][14] A third, concurring period of 11.013 hours with an amplitude of 0.26 magnitude was obtained by French amateur astronomerRené Roy in February 2005 (U=3).[15]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Rusthawelia measures between 68.67 and 82.23 kilometers in diameter and its surface has analbedo between 0.029 and 0.04.[6][7][8][10][11][12] TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0394 and a diameter of 70.13 kilometers based on anabsolute magnitude of 9.90.[3]

References

[edit]
  1. ^abc"1171 Rusthawelia (1930 TA)".Minor Planet Center. Retrieved5 March 2018.
  2. ^abcSchmadel, Lutz D. (2007). "(1171) Rusthawelia".Dictionary of Minor Planet Names – (1171) Rusthawelia.Springer Berlin Heidelberg. pp. 98–99.doi:10.1007/978-3-540-29925-7_1172.ISBN 978-3-540-00238-3.
  3. ^abcde"LCDB Data for (1171) Rusthawelia". Asteroid Lightcurve Database (LCDB). Retrieved5 March 2018.
  4. ^ab"Asteroid 1171 Rusthawelia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved28 October 2019.
  5. ^abcdefgh"JPL Small-Body Database Browser: 1171 Rusthawelia (1930 TA)" (2018-01-20 last obs.).Jet Propulsion Laboratory. Retrieved5 March 2018.
  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. Retrieved5 March 2018.
  7. ^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.
  8. ^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.
  9. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009,S2CID 119226456 See Table 1.
  10. ^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)
  11. ^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.
  12. ^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. Retrieved5 March 2018.
  13. ^abMenke, John L. (September 2005)."Lightcurves and periods for asteroids 471 Papagena, 675 Ludmilla, 1016 Anitra, 1127 Mimi, 1165 Imprinetta, 1171 Rustahawelia, and 2283 Bunke"(PDF).Minor Planet Bulletin.32 (3):64–66.Bibcode:2005MPBu...32...64M.ISSN 1052-8091.
  14. ^abIvarsen, Kevin; Willis, Sarah; Ingleby, Laura; Matthews, Dan; Simet, Melanie (June 2004)."CCD observations and period determination of fifteen minor planets"(PDF).Minor Planet Bulletin.31 (2):29–33.Bibcode:2004MPBu...31...29I.ISSN 1052-8091.
  15. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1171) Rusthawelia". Geneva Observatory. Retrieved5 March 2018.
  16. ^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. Retrieved5 March 2018.
  17. ^Schmadel, Lutz D. (2007). "(525) Adelaide".Dictionary of Minor Planet Names – (525) Adelaide. Springer Berlin Heidelberg. p. 56.doi:10.1007/978-3-540-29925-7_526.ISBN 978-3-540-00238-3.
  18. ^"Long 'Lost' Planet Found Masquerading as Comet".Oakland Tribune. 21 June 1929. p. 31. Retrieved9 November 2017 – viaNewspapers.com.Open access icon

External links

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