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词条 1717 Arlon
释义

  1. Classification and orbit

  2. Binary system

      Primary    Secondary  

  3. Diameter and albedo

  4. Naming

  5. Notes

  6. References

  7. External links

{{Infobox planet
| minorplanet = yes
| name = 1717 Arlon
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  
| discovered = 8 January 1954
| discoverer = S. Arend
| discovery_site = Uccle Obs.
| mpc_name = (1717) Arlon
| alt_names = 1954 AC{{·}}1930 YU
1941 BJ{{·}}1946 UB
1951 GQ{{·}}1954 CE
{{mp|1977 FQ|3}}{{·}}{{mp|1978 PC|5}}
A915 CC
| named_after = {{nowrap|Arlon {{small|(Municipality of Belgium)}}[2]}}
| mp_category = main-belt{{·}}Flora [3]
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 85.66 yr (31,289 days)
| aphelion = 2.4797 AU
| perihelion = 1.9111 AU
| semimajor = 2.1954 AU
| eccentricity = 0.1295
| period = 3.25 yr (1,188 days)
| mean_anomaly = 224.11°
| mean_motion = {{Deg2DMS|0.3030|sup=ms}} / day
| inclination = 6.1881°
| asc_node = 340.49°
| arg_peri = 115.91°
| satellites = 1 {{small|(D: 4 km}}[5]{{·}}{{small|P: 18.2 h)}}[6][7]
| dimensions = {{val|8.484|0.183}}[8]
{{val|8.57|0.58}} km[9]
{{val|8.87|0.74}} km[10]
{{val|9.128|0.166}} km[11]
{{val|9.15|}} km[12]
| rotation = {{val|5.1082|0.0006}} h[13]
{{val|5.1477|0.00009}} h{{efn|name=LCDB-Prave-2011}}
{{val|5.148}} h[14]
{{val|5.148|0.001}} h[7][16]
{{val|5.1484|0.0004}} h{{efn|name=LCDB-Prave-2005}}
{{val|5.1484}} h[6]
{{val|5.261|0.005}} h[13]
| albedo = {{val|0.167|0.024}}[9]
{{val|0.225}}[12]
{{val|0.2492|0.0420}}[11]
{{val|0.287|0.048}}[8]
{{val|0.315|0.166}}[10]
| spectral_type = Tholen = S {{·}}S [3]
| abs_magnitude = {{val|11.94|0.08}} {{small|(R)}}{{efn|name=LCDB-Prave-2005}}{{·}}{{val|12.09|0.33}}[26]{{·}}12.13[10]{{·}}12.90[9]{{·}}12.3{{·}}12.33[11]{{·}}{{val|12.43|0.094}}[3][12]
}}

1717 Arlon, provisional designation {{mp|1954 AC}}, is a binary Florian asteroid from the inner regions of the asteroid belt, approximately 8.5 kilometers in diameter.

It was discovered on 8 January 1954, by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle, Belgium, and later named for the Belgian town and provincial capital, Arlon.[2][34]

Classification and orbit

Arlon is a member of the Flora family, a collisional family of S-type asteroids asteroids, and one of the largest populations of the main-belt. It orbits the Sun in the inner main-belt at a distance of 1.9–2.5 AU once every 3 years and 3 months (1,188 days). Its orbit has an eccentricity of 0.13 and an inclination of 6° with respect to the ecliptic. First identified as {{mp|A915 CC}} at Simeiz Observatory in 1915, Arlon{{'s}} first used observation was taken at Lowell Observatory in 1930, when it was identified as {{mp|1930 YU}}, extending the body's observation arc by 24 years prior to its official discovery observation.[34]

Binary system

Primary

A large number of rotational lightcurves of Arlon were obtained from photometric observations, giving a well-defined rotation period between 5.1477 and 5.1496 hours with a small brightness variation of 0.10 magnitude or less (also see infobox).[3]{{efn|name=LCDB-Prave-2011}}

Secondary

During one of these photometric observations in 2006, the binary nature of Arlon was revealed. The discovered asteroid moon orbits its primary once every 18.2 hours, at a distance of 16 kilometers. The moon itself measures approximately 4 kilometers in diameter.[5][6][7]

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Arlon measures between 8.48 and 9.15 kilometers in diameter and its surface has an albedo between 0.167 and 0.315.[8][9][12] The Collaborative Asteroid Lightcurve Link agrees with the revised WISE-results by Pravec, adopting an albedo of 0.225 and a diameter of 9.15 kilometers with an absolute magnitude of 12.43.[3]

Naming

This minor planet was named for the Belgian town, municipality and provincial capital, Arlon. It is located on a hill above the source of the Semois river. In ancient times, Arlon was known as Orolaunum by the Romans and served as a station on the Antoninian way linking the cities Trier with Reims.[2] The approved naming citation was published by the Minor Planet Center on 22 September 1983 ({{small|M.P.C. 8150}}).[46]

Notes

{{notelist|refs={{efn|name=LCDB-Prave-2005|1=Pravec (2005): rotation period {{val|5.1484|0.0004}} with a brightness amplitude of {{val|0.08}}. Summary figures for (1717) Arlon at Asteroid Lightcurve Database}}{{efn|name=LCDB-Prave-2011|1=Pravec (2011): Pravec (2011): rotation period of {{val|5.14822|0.00009}}, {{val|5.1496|0.0005}} and {{val|5.1477|0.0004}} with a corresponding brightness amplitude of {{val|0.07}}, {{val|0.09}} and {{val|0.10}} in magnitude. Summary figures at Asteroid Lightcurve Database for (1717) Arlon}}

}}

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (1717) Arlon |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 136 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1718 |chapter = (1717) Arlon }}
2. ^{{cite web |title = 1717 Arlon (1954 AC) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1717 |accessdate = 22 December 2016}}
3. ^{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 22 December 2016}}
4. ^{{cite web |title = Asteroids and comets rotation curves – (1717) Arlon |last = Behrend |first = Raoul |publisher = Geneva Observatory |url = http://obswww.unige.ch/~behrend/page4cou.html#001717 |accessdate = 22 December 2016}}
5. ^{{cite web |date = 13 October 2006 |title = (1717) Arlon |publisher = Johnston's Archive |author = Wm. Robert Johnston |url = http://www.johnstonsarchive.net/astro/astmoons/am-01717.html |accessdate = 22 December 2016}}
6. ^{{cite web |title = LCDB Data for (1717) Arlon |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1717%7CArlon |accessdate = 22 December 2016}}
7. ^{{cite journal |display-authors = 6 |first1 = Fumihiko |last1 = Usui |first2 = Daisuke |last2 = Kuroda |first3 = Thomas G. |last3 = Müller |first4 = Sunao |last4 = Hasegawa |first5 = Masateru |last5 = Ishiguro |first6 = Takafumi |last6 = Ootsubo |first7 = Daisuke |last7 = Ishihara |first8 = Hirokazu |last8 = Kataza |first9 = Satoshi |last9 = Takita |first10 = Shinki |last10 = Oyabu |first11 = Munetaka |last11 = Ueno |first12 = Hideo |last12 = Matsuhara |first13 = Takashi |last13 = Onaka |date = October 2011 |title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey |url = http://pasj.oxfordjournals.org/content/63/5/1117.full.pdf+html |journal = Publications of the Astronomical Society of Japan |volume = 63 |issue = 5 |pages = 1117–1138 |bibcode = 2011PASJ...63.1117U |doi = 10.1093/pasj/63.5.1117 |access-date= 22 December 2016}}
8. ^{{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 }}
9. ^{{Cite journal |first1 = Petr |last1 = Pravec |first2 = Alan W. |last2 = Harris |first3 = Peter |last3 = Kusnirák |first4 = Adrián |last4 = Galád |first5 = Kamil |last5 = Hornoch |date = September 2012 |title = Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012Icar..221..365P |journal = Icarus |volume = 221 |issue = 1 |pages = 365–387 |bibcode = 2012Icar..221..365P |doi = 10.1016/j.icarus.2012.07.026 |access-date= 22 December 2016}}
10. ^{{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 = C. |last6 = Nugent |first7 = M. S. |last7 = Cabrera |date = November 2012 |title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M |journal = The Astrophysical Journal Letters |volume = 759 |issue = 1 |page = 5 |bibcode = 2012ApJ...759L...8M |doi = 10.1088/2041-8205/759/1/L8 |arxiv = 1209.5794 |access-date= 22 December 2016}}
11. ^{{Cite journal |display-authors = 6 |first1 = W. |last1 = Cooney |first2 = J. |last2 = Gross |first3 = D. |last3 = Terrell |first4 = R. |last4 = Stephens |first5 = P. |last5 = Pravec |first6 = P. |last6 = Kusnirak |first7 = R. |last7 = Durkee |first8 = A. |last8 = Galad |date = January 2006 |title = (1717) Arlon |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006CBET..369....1C |journal = Central Bureau Electronic Telegrams |volume = 369 |issue = 369 |pages = 1 |bibcode = 2006CBET..369....1C |access-date= 22 December 2016}}
12. ^{{Cite journal |display-authors = 6 |first1 = W. |last1 = Cooney |first2 = J. |last2 = Gross |first3 = D. |last3 = Terrell |first4 = P. |last4 = Pravec |first5 = P. |last5 = Kusnirak |first6 = D. |last6 = Pray |first7 = Yu. |last7 = Krugly |first8 = L. |last8 = Kornos |first9 = J. |last9 = Vilagi |first10 = S. |last10 = Gajdos |first11 = A. |last11 = Galad |first12 = V. |last12 = Reddy |first13 = R. |last13 = Dyvig |first14 = S. |last14 = Nudds |first15 = Z. |last15 = Kanuchova |first16 = M. |last16 = Pikler |first17 = M. |last17 = Husarik |date = May 2006 |title = (1717) Arlon |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006CBET..504....1C |journal = Central Bureau Electronic Telegrams |volume = 504 |issue = 504 |pages = 1 |bibcode = 2006CBET..504....1C |access-date= 22 December 2016}}
13. ^{{Cite journal |author = Brinsfield, James W. |date = April 2009 |title = Asteroid Lightcurve Analysis at the Via Capote Observatory: 2008 4th Quarter |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009MPBu...36...64B |journal = The Minor Planet Bulletin |volume = 36 |issue = 2 |pages = 64–66 |issn = 1052-8091 |bibcode = 2009MPBu...36...64B |access-date= 22 December 2016}}
14. ^{{Cite journal |author = Oey, Julian |date = October 2014 |title = Lightcurve Analysis of Asteroids from Blue Mountains Observatory in 2013 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014MPBu...41..276O |journal = The Minor Planet Bulletin |volume = 41 |issue = 4 |pages = 276–281 |issn = 1052-8091 |bibcode = 2014MPBu...41..276O |access-date= 22 December 2016}}
15. ^{{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= 22 December 2016}}
16. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = T. |last2 = Grav |first3 = A. K. |last3 = Mainzer |first4 = C. R. |last4 = Nugent |first5 = J. M. |last5 = Bauer |first6 = R. |last6 = Stevenson |first7 = S. |last7 = Sonnett |date = August 2014 |title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M |journal = The Astrophysical Journal |volume = 791 |issue = 2 |page = 11 |bibcode = 2014ApJ...791..121M |doi = 10.1088/0004-637X/791/2/121 |arxiv = 1406.6645 |access-date= 22 December 2016}}
[1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16]

}}

External links

  • Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
  • 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 (1)-(5000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator |1716 Peter |number=1717 |1718 Namibia}}{{Small Solar System bodies}}{{DEFAULTSORT:Arlon}}

8 : Flora asteroids|Discoveries by Sylvain Arend|Minor planets named for places|Named minor planets|Binary asteroids|Arlon|S-type asteroids (Tholen)|Astronomical objects discovered in 1954

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