Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

6229 Tursachan

From Wikipedia, the free encyclopedia
Main-belt asteroid

6229 Tursachan
Discovery[1]
Discovered byB. A. Skiff
Discovery siteAnderson Mesa Stn.
Discovery date4 November 1983
Designations
(6229) Tursachan
Named after
"Standing Stones"[1]
(Gaelic language)
1983 VN7 · 1988 RC2
main-belt[1][2] · (outer)
Themis[3][4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc34.40yr (12,565 d)
Aphelion3.6472AU
Perihelion2.5155 AU
3.0814 AU
Eccentricity0.1836
5.41 yr (1,976 d)
142.06°
0° 10m 55.92s / day
Inclination1.6495°
146.28°
234.29°
Physical characteristics
8.61 km(calculated)[4]
10.34±2.69 km[5]
11.18±3.50 km[6]
11.603±0.070 km[7][8]
16.596±0.0167 h[9]
0.07±0.04[5]
0.076±0.012[7][8]
0.089±0.113[6]
0.08(assumed)[4]
C(assumed)[4]
13.00[6][8]
13.2[2]
13.236±0.003(R)[9]
13.39±0.24[10]
13.44[5]
13.69[4]

6229 Tursachan, provisional designation1983 VN7, is a Themistianasteroid from the outer regions of theasteroid belt, approximately 10 kilometers (6 miles) in diameter. It was discovered on 4 November 1983, by American astronomerBrian Skiff at Lowell'sAnderson Mesa Station near Flagstaff, Arizona, in the United States.[1] The presumedC-type asteroid has arotation period of 16.6 hours and is possibly elongated.[4] It was named after aGaelic word meaning "Standing Stones".[1]

Orbit and classification

[edit]

Tursachan is a Themistian asteroid that belongs to theThemis family (602),[3] a very largefamily of carbonaceous asteroids, named after24 Themis.[4][11]: 23 

It orbits the Sun in theouter main-belt at a distance of 2.5–3.6 AU once every 5 years and 5 months (1,976 days;semi-major axis of 3.08 AU). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[2] The body'sobservation arc begins with aprecovery taken atPalomar Observatory just 5 nights prior to its official discovery observation at Anderson Mesa.[1]

Physical characteristics

[edit]

Tursachan is an assumedC-type asteroid,[4] which agrees with the overallspectral type for members of the Themis family.[11]: 23 

Rotation period

[edit]

In September 2010, a rotationallightcurve ofTursachan was obtained fromphotometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 16.596 hours with a brightness amplitude of 0.57magnitude, indicative of an elongated shape (U=2).[4][9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Tursachan measures between 10.34 and 11.603 kilometers in diameter and its surface has analbedo between 0.07 and 0.089.[5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 8.61 kilometers based on anabsolute magnitude of 13.69.[4]

Naming

[edit]

Thisminor planet was named after the term "Tursachan", which means "Standing Stones" in theGaelic language (Tursachan is the plural form of Tursa, meaning in Gaelic "megalith, monolith, menhir"), and refers to the stones often placed in circles during theNeolithic (approximately 10,000 BC to 2000 BC) on theBritish Isles. These stones may have been used to follow the seasons and mark astronomical events.[1] The official naming citation was published by theMinor Planet Center on 11 February 1998 (M.P.C. 31296).[12]

References

[edit]
  1. ^abcdefg"6229 Tursachan (1983 VN7)".Minor Planet Center. Retrieved21 April 2018.
  2. ^abcd"JPL Small-Body Database Browser: 6229 Tursachan (1983 VN7)" (2018-03-25 last obs.).Jet Propulsion Laboratory. Retrieved21 April 2018.
  3. ^ab"Asteroid 6229 Tursachan – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  4. ^abcdefghij"LCDB Data for (6229) Tursachan". Asteroid Lightcurve Database (LCDB). Retrieved21 April 2018.
  5. ^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.
  6. ^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.
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.
  8. ^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.
  9. ^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.
  10. ^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.
  11. ^abNesvorný, 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.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved21 April 2018.

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=6229_Tursachan&oldid=1319063185"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp