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2500 Alascattalo

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2500 Alascattalo
Discovery [1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date2 April 1926
Designations
(2500) Alascattalo
Named after
Alascattalo
(mythological creature)[2]
1926 GC · 1927 TA
1946 FB · 1981 VD
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc91.18 yr (33,303 days)
Aphelion2.4620AU
Perihelion2.0184 AU
2.2402 AU
Eccentricity0.0990
3.35yr (1,225 days)
78.867°
0° 17m 38.4s / day
Inclination6.9899°
48.004°
160.51°
Physical characteristics
Dimensions7.481±0.132 km[4]
7.947±0.037 km[5]
8.19 km(calculated)[3]
2.751±0.002 h[6]
2.754±0.007h[7]
0.2138±0.0580[5]
0.24(assumed)[3]
0.257±0.013[4]
S[3]
12.6[1][3] · 12.8[5] · 12.94±0.30[8]

2500 Alascattalo, provisional designation1926 GC, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter.

The asteroid was discovered on 2 April 1926, by German astronomerKarl Reinmuth atHeidelberg Observatory in southern Germany.[9] It was later named for the fictional moose–walrusAlascattalo creature.[2]

Orbit and classification

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Alascattalo is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,225 days). Its orbit has aneccentricity of 0.10 and aninclination of 7° with respect to theecliptic.[1] Noprecoveries were obtained prior to its discovery.[9]

Physical characteristics

[edit]

Alascattalo has been characterized as a common, stonyS-type asteroid.[3]

Rotation period

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A rotationallightcurve of this asteroid was obtained from photometric observations made by Junda Liu at the Lvye Observatory (P34), China, and at the iTelescope Observatory (Q62), at theSiding Spring Observatory site, Australia, in December 2015. The lightcurve gave a well-definedrotation period of2.751 hours with a brightness variation of 0.19 inmagnitude (U=3-).[6]

A previous lightcurve with a concurring period of2.754 hours and a similar amplitude of 0.15 was already obtained by French amateur astronomerPierre Antonini in March 2013 (U=2).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Alascattalo measures 7.5 and 7.9 kilometers in diameter and its surface has analbedo of 0.21 and 0.27, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – which derives from8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 8.2 kilometers with anabsolute magnitude of 12.6.[3]

Naming

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Thisminor planet was named after the mythological creature "Alascattalo", a fictionalchimera between a moose and a walrus.[2]

According to legend, it was genetically bred by miners during theKlondike Gold Rush in the late 19th century. The alascattalo also stands for the local people's unique sense of humor, dealing with tourists who ask naive questions, and is the mascot of the four-minute long, annual parade on "Alascattalo Day" held in November.[2] The official naming citation was published by theMinor Planet Center on 21 November 1991 (M.P.C. 19332).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2500 Alascattalo (1926 GC)" (2017-06-06 last obs.).Jet Propulsion Laboratory. Retrieved13 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(2500) Alascattalo".Dictionary of Minor Planet Names – (2500) Alascattalo.Springer Berlin Heidelberg. p. 204.doi:10.1007/978-3-540-29925-7_2501.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2500) Alascattalo". Asteroid Lightcurve Database (LCDB). Retrieved7 May 2016.
  4. ^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. Retrieved6 December 2016.
  5. ^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. Retrieved7 May 2016.
  6. ^abLiu, Junda (April 2016)."Rotation Period Analysis for 2500 Alascattalo".The Minor Planet Bulletin.43 (2):111–112.Bibcode:2016MPBu...43..111L.ISSN 1052-8091. Retrieved7 May 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2500) Alascattalo".Geneva Observatory. Retrieved7 May 2016.
  8. ^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. Retrieved7 May 2016.
  9. ^ab"2500 Alascattalo (1926 GC)".Minor Planet Center. Retrieved7 May 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 May 2016.

External links

[edit]
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