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1116 Catriona

From Wikipedia, the free encyclopedia
Main-belt asteroid

1116 Catriona
Shape model ofCatriona from itslightcurve
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date5 April 1929
Designations
(1116) Catriona
Named after
Catriona(novel by
Robert Louis Stevenson)
[2]
1929 GD · 1926 RQ
A908 AC
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc109.01 yr (39,815 days)
Aphelion3.5946AU
Perihelion2.2522 AU
2.9234 AU
Eccentricity0.2296
5.00yr (1,826 days)
348.27°
0° 11m 49.92s / day
Inclination16.523°
356.52°
82.666°
Physical characteristics
Dimensions36.71±0.53 km[6]
38.741±0.281 km[7]
39.02 km(derived)[8]
39.04 km[9]
39.12±0.7 km[10]
41.010±0.396 km[11]
8.83±0.01h[12]
8.832 h[a][b]
10.49 h[9]
12.06 h[c]
0.1395(derived)[8]
0.1397±0.0214[11]
0.1419[9]
0.1522±0.006[10]
0.155±0.025[7]
0.175±0.006[6]
C[8]
9.70[6][10][11] · 9.78[9] · 9.8[1][8]

1116 Catriona (prov. designation:1929 GD) is a carbonaceousasteroid from the outer regions of theasteroid belt, approximately 39 kilometers (24 miles) in diameter. It was discovered on 5 April 1929 by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[3] The asteroid was likely named after the 1893-novelCatriona byRobert Louis Stevenson.[2]

Classification and orbit

[edit]

Catriona is not a member of any identifiedasteroid family. It orbits the Sun in theouter main belt at a distance of 2.3–3.6 AU once every 5.00 years (1,826 days). Its orbit has aneccentricity of 0.23 and aninclination of 17° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Johannesburg.[3]

Naming

[edit]

Thisminor planet was probably named afterCatriona, the 1893-novel byRobert Louis Stevenson (1850–1894), who was a Scottish poet, novelist and travel writer.[2] The naming citation is based onLutz Schmadel's research including feedback from R. Bremer.[2]

Physical characteristics

[edit]

Catriona is an assumed carbonaceousC-type asteroid.[8]

Rotation period

[edit]

In December 2003, the best-rated rotationallightcurve ofCatriona was obtained from photometric observations by American astronomer John Menke at his Menke Observatory inBarnesville, Maryland (noobs. code). Lightcurve analysis gave a well-definedrotation period of 8.83 hours with a notably low brightness variation of 0.09magnitude, indicative of aspheroidal shape (U=3).[12] Additional photometric observations gave a concurring period of 8.832 hours, while others gave a longer period of 10.49 and 12.06 hours (U=2/2/2/2).[9][a][b][c]

Diameter and albedo

[edit]

According to observations by astronomers at theRozhen Observatory in Bulgaria, as well as the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Catriona measures between 36.71 and 41.010 kilometers in diameter and its surface has analbedo between 0.1397 and 0.175.[6][7][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1395 and a diameter of 39.02 kilometers based on anabsolute magnitude of 9.8.[8]

Notes

[edit]
  1. ^abCALL (2011): anonymous lightcurve submitted to Collaborative Asteroid Lightcurve Link. Rotation period8.832 hours with a brightness amplitude of0.10 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)
  2. ^abMenke (2011): rotation period8.832 hours with a brightness amplitude of0.10 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)
  3. ^abDenchev (1999; b) web: rotation period12.06 hours with a brightness amplitude of0.20 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL)

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1116 Catriona (1929 GD)" (2017-01-07 last obs.).Jet Propulsion Laboratory. Retrieved29 August 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1116) Catriona".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 95.doi:10.1007/978-3-540-29925-7_1117.ISBN 978-3-540-00238-3.
  3. ^abc"1116 Catriona (1929 GD)".Minor Planet Center. Retrieved29 August 2017.
  4. ^"Asteroid 1116 Catriona – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved13 March 2020.
  5. ^"Asteroid 1116 Catriona".Small Bodies Data Ferret. Retrieved13 March 2020.
  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. ^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. Retrieved29 August 2017.
  8. ^abcdef"LCDB Data for (1116) Catriona". Asteroid Lightcurve Database (LCDB). Retrieved29 August 2017.
  9. ^abcdefDenchev, P. (August 2000)."Photometry of 11 asteroids during their 1998 and 1999 apparitions".Planetary and Space Science.48 (10):987–992.Bibcode:2000P&SS...48..987D.doi:10.1016/S0032-0633(00)00067-2. Retrieved29 August 2017.
  10. ^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.
  11. ^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.
  12. ^abMenke, John (December 2005)."Asteroid lightcurve results from Menke Observatory"(PDF).Minor Planet Bulletin.32 (4):85–88.Bibcode:2005MPBu...32...85M.ISSN 1052-8091. Archived fromthe original(PDF) on 18 February 2020. Retrieved13 March 2020.

External links

[edit]
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