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6247 Amanogawa

From Wikipedia, the free encyclopedia
Main-belt asteroid

6247 Amanogawa
Discovery[1]
Discovered byK. Endate
K. Watanabe
Discovery siteKitami Obs.
Discovery date21 November 1990
Designations
(6247) Amanogawa
Named after
Amanogawa River[1]
(Japanese river)
1990 WY3 · 1992 FR1
main-belt[1][2] · (inner)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc27.45yr (10,025 d)
Aphelion2.5286AU
Perihelion2.2604 AU
2.3945 AU
Eccentricity0.0560
3.71 yr (1,353 d)
168.98°
0° 15m 57.6s / day
Inclination8.5728°
105.57°
287.33°
Physical characteristics
6.722±0.098 km[4][5]
11.63 km(calculated)[6]
12.369±0.0107 h[7]
12.38±0.02 h[8]
0.057(assumed)[6]
0.165±0.018[4][5]
C(assumed)[6]
X(SDSS-MOC)[9]
13.2[5]
13.288±0.006(R)[7]
13.3[2]
13.4[6]

6247 Amanogawa, provisional designation1990 WY3, is a backgroundasteroid from the inner regions of theasteroid belt, approximately 7 kilometers (4 miles) in diameter. It was discovered on 21 November 1990, by Japanese amateur astronomersKin Endate andKazuro Watanabe at theKitami Observatory.[1] TheX-type asteroid has arotation period of 12.38 hours.[6] It was named after theAmanogawa River on the island of Hokkaido, Japan.[1]

Orbit and classification

[edit]

Amanogawa is a non-family asteroid from the main belt'sbackground population.[3] It orbits the Sun in theinner asteroid belt at a distance of 2.3–2.5 AU once every 3 years and 9 months (1,353 days;semi-major axis of 2.39 AU). Its orbit has aneccentricity of 0.06 and aninclination of 9° with respect to theecliptic.[2] The body'sobservation arc begins with aprecovery atPalomar Observatory on 14 November 1990, just one week prior to its official discovery observation at Kitami.[1]

Physical characteristics

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In theSDSS-based taxonomy,Amanogawa has been characterized as anX-type asteroid.[9] It is also a generically assumedC-type asteroid.[6]

Rotation period

[edit]

In September 2008, a rotationallightcurve ofAmanogawa was obtained fromphotometric observations at theOakley Southern Sky Observatory andOakley Observatory. Lightcurve analysis gave a well-definedrotation period of 12.38 hours with a brightness variation of 0.48magnitude (U=3).[8] In February 2014, astronomers at thePalomar Transient Factory measured a similar period of 12.369 hours and an amplitude of 0.38 magnitude in the R-band (U=2).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Amanogawa measures 6.722 kilometers in diameter and its surface has analbedo of 0.165.[4][5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for acarbonaceous asteroid of 0.057 and calculates a diameter of 11.63 kilometers based on anabsolute magnitude of 13.4.[6]

Naming

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Thisminor planet was named after the JapaneseAmanogawa River that through the town ofKaminokuni on the island of Hokkaido. "Amanogawa" also means "Milky Way" in Japanese.[1] The official naming citation was published by theMinor Planet Center on 22 February 1997 (M.P.C. 29146).[10]

References

[edit]
  1. ^abcdefg"6247 Amanogawa (1990 WY3)".Minor Planet Center. Retrieved28 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 6247 Amanogawa (1990 WY3)" (2018-04-26 last obs.).Jet Propulsion Laboratory. Retrieved28 May 2018.
  3. ^ab"Asteroid 6247 Amanogawa".Small Bodies Data Ferret. Retrieved28 May 2018.
  4. ^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.S2CID 118745497.
  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.S2CID 118700974. (catalog)
  6. ^abcdefg"LCDB Data for (6247) Amanogawa". Asteroid Lightcurve Database (LCDB). Retrieved28 May 2018.
  7. ^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.
  8. ^abCarbo, Landy; Kragh, Katherine; Krotz, Jonathan; Meiers, Andrew; Shaffer, Nelson; Torno, Steven; et al. (July 2009). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory and Oakley Observatory: 2008 September and October".The Minor Planet Bulletin.36 (3):91–94.Bibcode:2009MPBu...36...91C.ISSN 1052-8091.
  9. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved28 May 2018.

External links

[edit]
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