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{{Infobox planet
{{Infobox planet
| discovery=yes
| minorplanet = yes
| name = 692 Hippodamia
| physical_characteristics = yes
| bgcolour=#FFFFC0
| background = #FFFFC0
| image =
| name=692 Hippodamia
| caption =
| alt_names= 1901 HD
| discovery_ref = &thinsp;<ref name="jpldata" />
| discoverer= [[Max Wolf]]<br/>[[August Kopff]]
| discovered= November 5, 1901
| discovered = 5 November 1901
| discoverer = [[Max Wolf|M. Wolf]] and [[August Kopff|A. Kopff]]
| discovery_site= [[Heidelberg]]
| discovery_site = [[Heidelberg-Königstuhl State Observatory|Heidelberg Observatory]]
| epoch=August 18, 2005 ([[Julian day|JDCT]] 2453600.5)
| mp_name = 692 Hippodamia
| eccentricity= 0.171
| alt_names = 1901 HD{{·}}1941 HK
| semimajor= 3.382 [[Astronomical unit|AU]]
| named_after = [[Hippodamia]]<br />{{small|([[Greek mythology]])}}<ref name="springer" />
| perihelion= 2.802 [[Astronomical unit|AU]]
| mp_category = [[main-belt|main-belt (outer)]]{{·}}[[Cybele family]]
| aphelion= 3.961 [[Astronomical unit|AU]]
| orbit_ref = &thinsp;<ref name="jpldata" />
| period= 6.219 [[Julian year (astronomy)|a]]
| epoch = 27 June 2015 ([[Julian day|JD]] 2457200.5)
| inclination= 26.104°
| uncertainty = 0
| asc_node= 63.561°
| observation_arc = {{nowrap|113.83 yr (41,575 days)}}
| arg_peri= 55.753°
| aphelion = 3.9572 [[Astronomical unit|AU]]
| mean_anomaly= 231.734°
| perihelion = 2.8079 AU
| semimajor = 3.3825 AU
| eccentricity = 0.1698
| period = 6.22 [[Julian year (astronomy)|yr]] (2,272 days)
| mean_anomaly = 83.918[[degree (angle)|°]]
| inclination = 26.083°
| asc_node = 63.488°
| arg_peri = 54.237°
| dimensions = {{val|45.90|1.8}} km<ref name="SIMPS" /><br />{{val|45.34|0.68}} km<ref name="AKARI" /><br />{{val|44.309|0.609}} km<ref name="WISE" />
| rotation = 8.98 [[hour|h]]<ref name="Zappala-1989" /><br />{{val|8.998|0.007}} h<ref name="geneva-obs" /><br />{{val|8.99690|0.00005}} h<ref name="Hanus-2011" /><br />{{val|8.99690|0.00005}} h<ref name="Hanus-2015b" />
| albedo = {{val|0.1785|0.015}}<ref name="SIMPS" /><br />{{val|0.185|0.006}}<ref name="AKARI" /><br />{{val|0.1950|0.0194}}<ref name="WISE" />
| spectral_type = [[Asteroid color indices|B–V]] = 0.860<br />[[Asteroid color indices|U–B]] = 0.435<br />[[Tholen classification|Tholen]] = [[S-type asteroid|S]]<br />[[S-type asteroid|S]]&thinsp;<ref name="lcdb" />
| abs_magnitude = 9.18<ref name="jpldata" />
}}
}}


'''692 Hippodamia''', provisional designation 1901 HD, is a stony [[asteroid]] from the outer region of the [[asteroid belt]], about 45 kilometers in diameter. It was discovered on 5 November 1901, by the German astronomers [[Max Wolf]] and [[August Kopff]] at [[Heidelberg-Königstuhl State Observatory|Heidelberg Observatory]] in southern Germany.<ref name="MPC-Hippodamia" /> Nine years later, the body was rediscovered by August Kopff at its apparition in 1910.<ref name="springer" />
'''692 Hippodamia''' is a [[minor planet]] orbiting the [[Sun]].


The [[S-type asteroid|S-type]] asteroid orbits the Sun at a distance of 2.8–4.0&nbsp;[[Astronomical unit|AU]] once every 6 years and 3 months (2,272 days). Its orbit is [[orbital inclination|tilted]] by 26 degrees to the plane of the [[ecliptic]] and shows an [[orbital eccentricity|eccentricity]] of 0.17.<ref name="jpldata" /> Based on its orbital elements, it is a member of the [[Cybele family]]. Named after the [[65 Cybele]], the group consists of relatively low-eccentric asteroids, which have a [[semi-major axis]] around 3.4&nbsp;AU, dwelling in-between the [[Hungaria family|Hungaria]] and the outermost [[Hilda family|Hilda]] family of asteroids.<ref name="Cybele-family" />
==External links==

* [http://cfa-www.harvard.edu/iau/lists/NumberedMPs.txt Discovery Circumstances: Numbered Minor Planets]
According to the surveys carried out by the Infrared Astronomical Satellite, [[IRAS]], the Japanese [[Akari (satellite)|Akari]] satellite, and the [[Wide-field Infrared Survey Explorer]] with its subsequent [[NEOWISE]] mission, the body has an [[astronomical albedo|albedo]] between 0.18 and 0.20,<ref name="SIMPS" /><ref name="AKARI" /><ref name="WISE" /> and several independent and concurring photometric [[light-curve]] analysis rendered a well-defined [[rotation period]] of 8.99 hours.<ref name="Zappala-1989" /><ref name="geneva-obs" /><ref name="Hanus-2011" /><ref name="Hanus-2015b" />

The minor planet was named after [[Hippodamia]], a figure from [[Greek mythology]]. It is conjectured, that the naming might be influenced by the two letters of the [[Provisional designation in astronomy#Minor planets|provisional designation]] "1901 HD". Hippodamia is the daughter of King [[Oenomaus]] of Pisa and wife of [[Pelops]]. She bribed Myrtilus, her father's charioteer, to remove a spoke from the royal chariot wheels so that Pelops could win her. Oenomaus had already defeated and killed 13 other suitors whom he had challenged to chariot races. After killing Oenomaus, Pelops murdered Myrtilus. These murders were primal sins, all paid for later by the many troubles of the house of Atreus.<ref name="springer" />

== References ==
{{reflist
|refs=

<ref name="geneva-obs">{{cite web
|title=Asteroids and comets rotation curves – (692) Hippodamia
|last=Behrend |first=Raoul
|publisher=Geneva Observatory
|url=http://obswww.unige.ch/~behrend/page2cou.html#000692
|accessdate=December 2015}}</ref>

<ref name="lcdb">{{cite web
|title=LCDB Data for (692) Hippodamia
|publisher=Asteroid Lightcurve Database (LCDB)
|url=http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=692%7CHippodamia
|accessdate=December 2015}}</ref>

<ref name="jpldata">{{cite web
|type=2015-09-03 last obs.
|title=JPL Small-Body Database Browser: 692 Hippodamia (1901 HD)
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000692
|publisher=Jet Propulsion Laboratory
|accessdate=December 2015}}</ref>

<ref name="springer">{{cite book
|url=http://link.springer.com/referenceworkentry/10.1007/978-3-540-29925-7_693
|title=Dictionary of Minor Planet Names – (692) Hippodamia
|last=Schmadel |first=Lutz D.
|publisher=Springer Berlin Heidelberg
|page=67
|date=2003
|isbn=978-3-540-29925-7
|accessdate=December 2015}}</ref>

<ref name="MPC-Hippodamia">{{cite web
|title=692 Hippodamia (1901 HD)
|work=Minor Planet Center
|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=692
|accessdate=December 2015}}</ref>

<ref name="SIMPS">{{cite journal
|authors = Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D.
|date = October 2004
|title = IRAS Minor Planet Survey V6.0
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2004PDSS...12.....T
|journal = NASA Planetary Data System
|bibcode = 2004PDSS...12.....T
|access-date= December 2015}}</ref>

<ref name="AKARI">{{cite journal
|authors = Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; Ishihara, Daisuke; Kataza, Hirokazu; Takita, Satoshi; Oyabu, Shinki; Ueno, Munetaka; Matsuhara, Hideo; Onaka, Takashi
|date = October 2011
|title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011PASJ...63.1117U
|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= December 2015}}</ref>

<ref name="WISE">{{cite journal
|authors = Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; McMillan, R. S.; Spahr, T.; Cutri, R. M.; Wright, E.; Watkins, J.; Mo, W.; Maleszewski, C.
|date = November 2011
|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M
|journal = The Astrophysical Journal
|volume = 741
|issue = 2
|page = 25
|bibcode = 2011ApJ...741...90M
|doi = 10.1088/0004-637X/741/2/90
|access-date= December 2015}}</ref>

<ref name="Zappala-1989">{{cite journal
|authors = Zappala, V.; di Martino, M.; Cellino, A.; de Sanctis, G.; Farinella, P.
|date = December 1989
|title = Rotational properties of outer belt asteroids
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1989Icar...82..354Z
|journal = Icarus
|pages = 354–368.ResearchsupportedbyCNRandMPI
|issn = 0019-1035
|bibcode = 1989Icar...82..354Z
|doi = 10.1016/0019-1035(89)90043-2
|access-date= December 2015}}</ref>

<ref name="Hanus-2011">{{cite journal
|authors = Hanuš, J.; Ďurech, J.; Brož, M; Warner, B. D.; Pilcher, F.; Stephens, R.; Oey, J.; Bernasconi, L.; Casulli, S.; Behrend, R.; Polishook, D.; Henych, T.; Lehký, M; Yoshida, F.; Ito, T.
|date = June 2011
|title = A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011A&A...530A.134H
|journal = Astronomy and Astrophysics
|volume = 530
|page = 16
|bibcode = 2011A&A...530A.134H
|doi = 10.1051/0004-6361/201116738
|access-date= December 2015}}</ref>

<ref name="Hanus-2015b">{{cite journal
|authors = Hanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo', M.; Adam, O.; Afonina, V.; Anquetin, R.; Antonini, P.; Arnold, L.; Audejean, M.; Aurard, P.; Bachschmidt, M.; Badue, B.; Barbotin, E.; Barroy, P.; Baudouin, P.; Berard, L.; Berger, N.; Bernasconi, L.
|date = October 2015
|title = New and updated convex shape models of asteroids based on optical data from a large collaboration network
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015arXiv151007422H
|journal = eprint arXiv:1510.07422
|bibcode = 2015arXiv151007422H
|access-date= December 2015}}</ref>

<ref name="Cybele-family">{{cite web
|url=https://books.google.ch/books?id=K-0xBsMsursC&pg=PA96&dq=Cybele+asteroid&hl=en&ei=IkjITJ-vI8KB8gbelP3mDw&sa=X&oi=book_result&ct=result&redir_esc=y#v=onepage&q=Cybele%20asteroid&f=false
|title=Asteroids, Meteorites, and Comets
|author= Linda T. Elkins-Tanton
|accessdate=December 2015}}</ref>

}} <!-- end of reflist -->

== External links ==
* [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html info])
* [https://books.google.se/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
* [http://obswww.unige.ch/~behrend/page_cou.html Asteroids and comets rotation curves, CdR] – Observatoire de Genève, Raoul Behrend
* [http://www.minorplanetcenter.net/iau/lists/NumberedMPs000001.html Discovery Circumstances: Numbered Minor Planets (1)-(5000)] – Minor Planet Center
* {{JPL small body|title=692 Hippodamia (1901 HD)|id=2000692}}


{{MinorPlanets Navigator|691 Lehigh|693 Zerbinetta}}
{{MinorPlanets Navigator|691 Lehigh|693 Zerbinetta}}
{{Small Solar System bodies}}
{{MinorPlanets_Footer}}


{{DEFAULTSORT:000692}}
{{DEFAULTSORT:Hippodamia}}
[[Category:Cybele asteroids]]
[[Category:Main-belt asteroids|000692]]
[[Category:Cybele asteroids|000692]]
[[Category:Numbered asteroids|000692]]
[[Category:Minor planets named from Greek mythology|Hippodamia]]
[[Category:Minor planets named from Greek mythology|Hippodamia]]
[[Category:Discoveries by Max Wolf]]
[[Category:Discoveries by Max Wolf|000692]]
[[Category:Discoveries by August Kopff]]
[[Category:Discoveries by August Kopff|000692]]
[[Category:Astronomical objects discovered in 1901|19011105]]
[[Category:Astronomical objects discovered in 1901|19011105]]
[[Category:Main-belt asteroids]]
[[Category:Numbered asteroids]]



{{beltasteroid-stub}}
{{Beltasteroid-stub}}

Revision as of 06:46, 15 December 2015

692 Hippodamia
Discovery [1]
Discovered byM. Wolf and A. Kopff
Discovery siteHeidelberg Observatory
Discovery date5 November 1901
Designations
692 Hippodamia
Named after
Hippodamia
(Greek mythology)[2]
1901 HD · 1941 HK
main-belt (outer) · Cybele family
Orbital characteristics[1]
Epoch 27 June 2015 (JD 2457200.5)
Uncertainty parameter 0
Observation arc113.83 yr (41,575 days)
Aphelion3.9572 AU
Perihelion2.8079 AU
3.3825 AU
Eccentricity0.1698
6.22 yr (2,272 days)
83.918°
Inclination26.083°
63.488°
54.237°
Physical characteristics
Dimensions45.90±1.8 km[3]
45.34±0.68 km[4]
44.309±0.609 km[5]
8.98 h[6]
8.998±0.007 h[7]
8.99690±0.00005 h[8]
8.99690±0.00005 h[9]
0.1785±0.015[3]
0.185±0.006[4]
0.1950±0.0194[5]
B–V = 0.860
U–B = 0.435
Tholen = S
S[10]
9.18[1]

692 Hippodamia, provisional designation 1901 HD, is a stony asteroid from the outer region of the asteroid belt, about 45 kilometers in diameter. It was discovered on 5 November 1901, by the German astronomers Max Wolf and August Kopff at Heidelberg Observatory in southern Germany.[11] Nine years later, the body was rediscovered by August Kopff at its apparition in 1910.[2]

The S-type asteroid orbits the Sun at a distance of 2.8–4.0 AU once every 6 years and 3 months (2,272 days). Its orbit is tilted by 26 degrees to the plane of the ecliptic and shows an eccentricity of 0.17.[1] Based on its orbital elements, it is a member of the Cybele family. Named after the 65 Cybele, the group consists of relatively low-eccentric asteroids, which have a semi-major axis around 3.4 AU, dwelling in-between the Hungaria and the outermost Hilda family of asteroids.[12]

According to the surveys carried out by the Infrared Astronomical Satellite, IRAS, the Japanese Akari satellite, and the Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the body has an albedo between 0.18 and 0.20,[3][4][5] and several independent and concurring photometric light-curve analysis rendered a well-defined rotation period of 8.99 hours.[6][7][8][9]

The minor planet was named after Hippodamia, a figure from Greek mythology. It is conjectured, that the naming might be influenced by the two letters of the provisional designation "1901 HD". Hippodamia is the daughter of King Oenomaus of Pisa and wife of Pelops. She bribed Myrtilus, her father's charioteer, to remove a spoke from the royal chariot wheels so that Pelops could win her. Oenomaus had already defeated and killed 13 other suitors whom he had challenged to chariot races. After killing Oenomaus, Pelops murdered Myrtilus. These murders were primal sins, all paid for later by the many troubles of the house of Atreus.[2]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 692 Hippodamia (1901 HD)" (2015-09-03 last obs.). Jet Propulsion Laboratory. Retrieved December 2015. {{cite web}}: Check date values in: |accessdate= (help)
  2. ^ a b c Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (692) Hippodamia. Springer Berlin Heidelberg. p. 67. ISBN 978-3-540-29925-7. Retrieved December 2015. {{cite book}}: Check date values in: |accessdate= (help)
  3. ^ a b c "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. October 2004. Bibcode:2004PDSS...12.....T. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  4. ^ a b c "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. October 2011. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  5. ^ a b c "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. November 2011. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  6. ^ a b "Rotational properties of outer belt asteroids". Icarus: 354–368.ResearchsupportedbyCNRandMPI. December 1989. Bibcode:1989Icar...82..354Z. doi:10.1016/0019-1035(89)90043-2. ISSN 0019-1035. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  7. ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (692) Hippodamia". Geneva Observatory. Retrieved December 2015. {{cite web}}: Check date values in: |accessdate= (help)
  8. ^ a b "A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method". Astronomy and Astrophysics. 530: 16. June 2011. Bibcode:2011A&A...530A.134H. doi:10.1051/0004-6361/201116738. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  9. ^ a b "New and updated convex shape models of asteroids based on optical data from a large collaboration network". eprint arXiv:1510.07422. October 2015. Bibcode:2015arXiv151007422H. Retrieved December 2015. {{cite journal}}: Check date values in: |access-date= (help); Cite uses deprecated parameter |authors= (help)
  10. ^ "LCDB Data for (692) Hippodamia". Asteroid Lightcurve Database (LCDB). Retrieved December 2015. {{cite web}}: Check date values in: |accessdate= (help)
  11. ^ "692 Hippodamia (1901 HD)". Minor Planet Center. Retrieved December 2015. {{cite web}}: Check date values in: |accessdate= (help)
  12. ^ Linda T. Elkins-Tanton. "Asteroids, Meteorites, and Comets". Retrieved December 2015. {{cite web}}: Check date values in: |accessdate= (help)

External links