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2090 Mizuho

From Wikipedia, the free encyclopedia
Stony asteroid

2090 Mizuho
Discovery[1]
Discovered byT. Urata
Discovery siteYakiimo Stn.
Discovery date12 March 1978
Designations
(2090) Mizuho
Named after
Mizuho Urata
(daughter of discoverer)[2]
1978 EA · 1937 RE
1942 PG · 1951 EH
1952 HA4 · 1953 RT
1953 TP · 1959 VD
1964 TE · 1970 WV
1978 EJ
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.14 yr (24,157 days)
Aphelion3.4819AU
Perihelion2.6635 AU
3.0727 AU
Eccentricity0.1332
5.39yr (1,967 days)
337.47°
0° 10m 58.8s / day
Inclination11.814°
339.85°
341.20°
Physical characteristics
Dimensions17.991±0.141[4]
18.185±0.117 km[5]
18.92±0.79 km[6]
35.28 km(calculated)[3]
5.47±0.01h[7]
0.057(assumed)[3]
0.207±0.019[6]
0.2154±0.0435[5]
0.219±0.029[4]
Tholen =S[1] · S[3]
B–V = 0.871[1]
U–B = 0.499[1]
10.99[1][3][5][6]

2090 Mizuho, provisional designation1978 EA, is a stonyasteroid from the outer region of theasteroid belt, approximately 18 kilometers in diameter.

The asteroid was discovered on 12 March 1978, by Japanese astronomerTakeshi Urata at theJCPM Yakiimo Station in Shimizu, Japan, who named it after his daughter, Mizuho Urata.[8]

Orbit and classification

[edit]

Mizuho orbits the Sun in theouter main-belt at a distance of 2.7–3.5 AU once every 5 years and 5 months (1,967 days). Its orbit has aneccentricity of 0.13 and aninclination of 12° with respect to theecliptic.[1]

The asteroid was first identified as1937 RE atSimeiz Observatory. The first used observation was obtained atHeidelberg Observatory in 1951, extending theMizuho'sobservation arc by 27 years prior to its official discovery observation.[8]

Physical characteristics

[edit]

In theTholen classification,Mizuho is characterized as a commonS-type asteroid.[1]

Rotation period

[edit]

In February 2010, a rotationallightcurve forMizuho was obtained from photometric observations by James W. Brinsfield at the Via Capote Observatory (G69) in California. It gave arotation period of 5.47 hours with a brightness variation of 0.30magnitude (U=2+).[7]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Mizuho measures between 18.0 and 18.9 kilometers in diameter and its surface has analbedo of between 0.207 and 0.219, which is typical for stony asteroids.[4][5][6] TheCollaborative Asteroid Lightcurve Link, however assumes a standard albedo for a carbonaceousC-type asteroid of 0.057 and correspondingly calculates a much larger diameter of 35.3 kilometers.[3]

Naming

[edit]

The discoverer named thisminor planet after his daughter, Mizuho Urata.[2] It was the first asteroid in over 50 years to be discovered by a non-professional astronomer, which set off a wave of interest in amateur asteroid discovery, especially in Japan.[9] The officialnaming citation was published by theMinor Planet Center on 1 September 1978 (M.P.C. 4482).[10]

References

[edit]
  1. ^abcdefgh"JPL Small-Body Database Browser: 2090 Mizuho (1978 EA)" (2017-05-02 last obs.).Jet Propulsion Laboratory. Retrieved10 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(2090) Mizuho".Dictionary of Minor Planet Names – (2090) Mizuho.Springer Berlin Heidelberg. p. 169.doi:10.1007/978-3-540-29925-7_2091.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2090) Mizuho". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2016.
  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. Retrieved7 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.
  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. ^abBrinsfield, James W. (October 2010)."Asteroid Lightcurve Analysis at the Via Capote Observatory: 2010 February-May".The Minor Planet Bulletin.37 (4):146–147.Bibcode:2010MPBu...37..146B.ISSN 1052-8091. Retrieved7 December 2016.
  8. ^ab"2090 Mizuho (1978 EA)".Minor Planet Center. Retrieved7 December 2016.
  9. ^Kosai, H.; Urata, T.; Nakamura, T. (December 1993)."Activities of Asteroid Studies by Amateur Astronomers in Japan".Seventy-five (75) Years of Hirayama Asteroid Families: The Role of Collisions in the Solar System History. Astronomical Society of the Pacific Conference Series.63: 297.Bibcode:1994ASPC...63..297K. Retrieved7 December 2016.
  10. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.


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