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词条 9971 Ishihara
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation and poles    Diameter and albedo  

  3. Naming

  4. References

  5. External links

{{short description|Asteroid}}{{Infobox planet
| minorplanet = yes
| name = 9971 Ishihara
| background = #D6D6D6
| image = AnimatedOrbitOf9971Ishihara.gif
| image_size = 180
| caption = {{longitem|Orbit of Ishihara (blue), inner planets and Jupiter (outermost)}}
| discovery_ref =  
| discovered = 16 April 1993
| discoverer = K. Endate
K. Watanabe
| discovery_site = Kitami Observatory
| mpc_name = (9971) Ishihara
| alt_names = 1993 HS{{·}}{{mp|1991 YC|2}}
{{mp|1996 EU|1}}
| pronounced =
| named_after = Takahiro Ishihara
{{small|(Japanese astronomer)}}[2]
| mp_category = main-belt{{·}}Flora [3]
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 24.91 yr (9,097 days)
| aphelion = 2.4465 AU
| perihelion = 1.9164 AU
| semimajor = 2.1814 AU
| eccentricity = 0.1215
| period = 3.22 yr (1,177 days)
| mean_anomaly = 158.69°
| mean_motion = {{Deg2DMS|0.3059|sup=ms}} / day
| inclination = 2.7482°
| asc_node = 20.550°
| arg_peri = 246.01°
| dimensions = 3.74 km {{small|(calculated)}}[3]
{{val|4.986|0.053}} km[6]
{{val|5.012|0.069}} km[7]
| rotation = {{val|6.715|0.0036}} h[8]
{{val|6.71574|0.00001}} h[9]
| albedo = {{val|0.2328|0.0281}}[7]
{{val|0.235|0.027}}[6]
0.24 {{small|(assumed)}}[3]
| spectral_type = S [3]
| abs_magnitude = 13.7[7]{{·}}13.9{{·}}{{val|13.852|0.006}} {{small|(R)}}[8]{{·}}{{val|14.26|0.22}}[17]{{·}}14.3[3]
}}9971 Ishihara, provisional designation {{mp|1993 HS}}, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 4 to 5 kilometers in diameter. It was discovered by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on 16 April 1993,[19] and named after Takahiro Ishihara, president of the astronomical society at Hiroshima.[2]

Orbit and classification

Ishihara is a member of the Flora family, one of the largest families of stony asteroids in the asteroid belt. It orbits the Sun in the inner main-belt at a distance of 1.9–2.4 AU once every 3 years and 3 months (1,177 days). Its orbit has an eccentricity of 0.12 and an inclination of 3° with respect to the ecliptic. It was first identified as {{mp|1991 YC|2}} at Karl Schwarzschild Observatory in 1991, extending the body's observation arc by approximately 2 years prior to its official discovery at Kitami.[19]

Physical characteristics

Rotation and poles

In January 2012, a rotational lightcurve of Ishihara was obtained from photometric observations by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 6.715 hours with a brightness amplitude of 1.06 in magnitude, which indicates that the body has a non-spheroidal shape ({{small|U=2}}).[8]

A 2016-published lightcurve, using modeled photometric data from the Lowell Photometric Database (LPD), gave a concurring period of 6.71574 hours ({{small|U=n.a.}}), as well as a spin axis of (42.0°, 76.0°) in ecliptic coordinates (λ, β).[9]

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Ishihara measures 4.986 and 5.012 kilometers in diameter and its surface has an albedo of 0.235 and 0.2328, respectively.[6][7] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, a S-type asteroid and the family's largest member and namesake – and calculates a diameter of 3.74 kilometers with an absolute magnitude of 14.3.[3]

Naming

This minor planet was named after Takahiro Ishihara (born 1961), an observer of comets, communicator of astronomy, and former president of the astronomical society at Hiroshima (1987–1997).[2] The official naming citation was published by the Minor Planet Center on 6 January 2003 ({{small|M.P.C. 47298}}).[29]

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (9971) Ishihara, Addendum to Fifth Edition: 2003–2005 |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 49 |date = 2006 |isbn = 978-3-540-34361-5 |doi = 10.1007/978-3-540-34361-5_391 |chapter = (9971) Ishihara [2.18, 0.12, 2.7] }}
2. ^{{cite web |title = 9971 Ishihara (1993 HS) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=9971 |accessdate = 10 April 2017}}
3. ^{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 10 April 2017}}
4. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 10 April 2017}}
5. ^{{cite web |title = LCDB Data for (9971) Ishihara |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=9971%7CIshihara |accessdate = 10 April 2017}}
6. ^{{cite journal |display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 }}
7. ^{{cite journal |first1 = J. |last1 = Durech |first2 = J. |last2 = Hanus |first3 = D. |last3 = Oszkiewicz |first4 = R. |last4 = Vanco |date = March 2016 |title = Asteroid models from the Lowell photometric database |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016A&A...587A..48D |journal = Astronomy and Astrophysics |volume = 587 |page = 6 |bibcode = 2016A&A...587A..48D |doi = 10.1051/0004-6361/201527573 |arxiv = 1601.02909 |access-date= 10 April 2017}}
8. ^{{cite journal |display-authors = 6 |first1 = Adam |last1 = Waszczak |first2 = Chan-Kao |last2 = Chang |first3 = Eran O. |last3 = Ofek |first4 = Russ |last4 = Laher |first5 = Frank |last5 = Masci |first6 = David |last6 = Levitan |first7 = Jason |last7 = Surace |first8 = Yu-Chi |last8 = Cheng |first9 = Wing-Huen |last9 = Ip |first10 = Daisuke |last10 = Kinoshita |first11 = George |last11 = Helou |first12 = Thomas A. |last12 = Prince |first13 = Shrinivas |last13 = Kulkarni |date = September 2015 |title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W |journal = The Astronomical Journal |volume = 150 |issue = 3 |page = 35 |bibcode = 2015AJ....150...75W |doi = 10.1088/0004-6256/150/3/75 |arxiv = 1504.04041 |access-date= 10 April 2017}}
9. ^{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 10 April 2017}}
[1][2][3][4][5][6][7][8][9]

}}

External links

  • Asteroid Lightcurve Database (LCDB), query form (info)
  • [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator|(9970) 1992 ST1|number=9971|9972 Minoruoda}}{{Small Solar System bodies}}{{DEFAULTSORT:Ishihara}}

6 : Flora asteroids|Discoveries by Kazuro Watanabe|Discoveries by Kin Endate|Minor planets named for people|Named minor planets|Astronomical objects discovered in 1993

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