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1098 Hakone

From Wikipedia, the free encyclopedia
Asteroid

1098 Hakone
Modelled shape ofHakone from itslightcurve
Discovery[1]
Discovered byO. Oikawa
Discovery siteTokyo Astronomical Obs.
Discovery date5 September 1928
Designations
(1098) Hakone
PronunciationJapanese:[hakone]
Named after
Mount Hakone
(Japanese volcanic mountain)[2]
1928 RJ · 1926 EC
1950 QH1 · 1952 BE1
A906 RD · A917 DD
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc110.19 yr (40,247 days)
Aphelion3.0081AU
Perihelion2.3686 AU
2.6884 AU
Eccentricity0.1189
4.41yr (1,610 days)
13.741°
0° 13m 24.96s / day
Inclination13.377°
329.00°
80.805°
Physical characteristics
24.44 km(derived)[6]
24.73±1.1 km[7]
24.90±0.57 km[8]
26.684±0.397 km[9]
29.567±0.135 km[10]
7.14±0.01 h[11]
7.14117±0.00001 h[12]
7.142±0.002 h[13]
7.16±0.050 h[14]
(40.0°, 43.0°) (λ11)[5]
0.1745±0.0334[10]
0.1865(derived)[6]
0.206±0.009[9]
0.2404±0.022[7]
0.245±0.013[8]
SMASS =Xe[3] · M[10] · X[6]
10.20[7][8][10] · 10.350±0.120(R)[14] · 10.5[3][6]

1098 Hakone (prov. designation:1928 RJ) is abackground asteroid from the central regions of theasteroid belt. TheX-type asteroid has arotation period of 7.1 hours and measures approximately 25 kilometers (16 miles) in diameter. Discovered by Japanese astronomerOkuro Oikawa at Tokyo Observatory in 1928, the asteroid was later named after the volcanicMount Hakone in Japan.

Orbit and classification

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Located in the orbital region of the stonyEunomia family,[6]Hakone is a non-family asteroid from the main belt'sbackground population when applying thehierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in thecentral asteroid belt at a distance of 2.4–3.0 AU once every 4 years and 5 months (1,610 days). Its orbit has aneccentricity of 0.12 and aninclination of 13° with respect to theecliptic.[3]

Discovery

[edit]

Hakone was discovered by Japanese astronomerOkuro Oikawa at the old Tokyo Astronomical Observatory (389) on 5 September 1928.[1] It was independently discovered by German astronomerMax Wolf atHeidelberg Observatory and Soviet astronomerGrigory Neujmin at theSimeiz Observatory on the Crimean peninsula on 9 and 11 September 1928, respectively.[2] TheMinor Planet Center, however, only acknowledges the first discoverer.[1] The asteroid was first observed asA906 RD at Taunton Observatory (803) on 16 September 1906. The body'sobservation arc begins the following month at theU.S. Naval Observatory, almost 22 years prior to its official discovery observation at Tokyo.[1]

Naming

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Thisminor planet was named after the volcanicMount Hakone, located 80 kilometers from the discovering Tokyo Astronomical Observatory and near the Japanese town ofHakone. The mountain resort is known for its hot springs,Lake Ashi and its view ofMount Fuji, after which the asteroid1584 Fuji was named. The official naming citation was prepared by astronomerKōichirō Tomita.[2]

Physical characteristics

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In theSMASS classification,Hakone is a Xe-subtype, that transitions from theX-type the very brightE-type asteroids.[3] It has also been characterized as a metallicM-type asteroid, by theWide-field Infrared Survey Explorer.[10]

Rotation period

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Several rotationallightcurves ofHakone were obtained fromphotometric observations. Analysis of the best-rated lightcurve by French amateur astronomerLaurent Bernasconi gave arotation period of 7.142 hours with a brightness amplitude of 0.35magnitude (U=3/3/2).[11][13][14]

Spin axis

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A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 7.14117 hours, as well as a spin axis of (40.0°, 43.0°) inecliptic coordinates (λ, β).[12]

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,Hakone measures between 24.73 and 29.567 kilometers in diameter and its surface has analbedo between 0.1745 and 0.245.[7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1865 and a diameter of 24.44 kilometers based on anabsolute magnitude of 10.5.[6]

References

[edit]
  1. ^abcde"1098 Hakone (1928 RJ)".Minor Planet Center. Retrieved25 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1098) Hakone".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 93.doi:10.1007/978-3-540-29925-7_1099.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 1098 Hakone (1928 RJ)" (2016-12-21 last obs.).Jet Propulsion Laboratory. Retrieved25 September 2017.
  4. ^ab"Asteroid 1098 Hakone – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved13 March 2020.
  5. ^abc"Asteroid 1098 Hakone".Small Bodies Data Ferret. Retrieved13 March 2020.
  6. ^abcdef"LCDB Data for (1098) Hakone". Asteroid Lightcurve Database (LCDB). Retrieved25 September 2017.
  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. ^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)
  9. ^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. Retrieved25 September 2017.
  10. ^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.
  11. ^abLecrone, Crystal; Addleman, Don; Butler, Thomas; Hudson, Erin; Mulvihill, Alex; Reichert, Chris; et al. (September 2005)."2004-2005 winter observing campaign at Rose-Hulman Institute: results for 1098 Hakone, 1182 Ilona, 1294 Antwerpia, 1450 Raimonda, 2251 Tikhov, and 2365 Interkosmos"(PDF).Minor Planet Bulletin.32 (3):46–48.Bibcode:2005MPBu...32...46L.ISSN 1052-8091.
  12. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573. Retrieved25 September 2017.
  13. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1098) Hakone".Geneva Observatory. Retrieved25 September 2017.
  14. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved25 September 2017.

External links

[edit]
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