11 Parthenope: Perbedaan antara revisi
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{{Infobox planet | discovery=yes | physical_characteristics = yes | bgcolour=#FFFFC0 |
name=11 Parthenope
| symbol=[[Berkas:
| image= [[Berkas:Parthenope-asteroid.jpg|200px]]
| discoverer=[[Annibale de Gasparis]]
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| surface_grav=0,0578 m/s²
| escape_velocity=0,0941 km/s
| rotation=0,3929 hr (9,43 jam)<ref name=jpldata/><ref>{{cite web |url=http://www.astrosurf.com/aude-old/map_files/AstVarMAP01-2003.htm |title=Lightcurves and Map Data on Numbered Asteroids N° 1 to 52225 |accessdate=2008-11-03 |publisher=AstroSurf |archiveurl=https://web.archive.org/web/20051127063200/http://www.astrosurf.com/aude-old/map_files/AstVarMAP01-2003.htm |archivedate=2005-11-27 |
| spectral_type=Asteroid tipe S<ref name=jpldata/>
| magnitude = 8,68<ref name=AstDys-Parthenope >{{cite web |title=AstDys (11) Parthenope Ephemerides |publisher=Department of Mathematics, University of Pisa, Italy |url=http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.3.1&n=11&oc=500&y0=2031&m0=7&d0=29&h0=00&mi0=00&y1=2031&m1=7&d1=29&h1=00&mi1=00&ti=1.0&tiu=days |accessdate=2010-06-26}}</ref> hingga 12,16
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| albedo=0,180 ([[albedo geometrik|geometrik]]) <ref name=jpldata/>
| angular_size = 0,178" <!-- Horizons 2008-Aug-07 --> hingga 0,057"
| single_temperature=~174 [[kelvin|K]]
}} '''11 Parthenope''' ({{IPAc-en
Parthenope ditemukan oleh [[Annibale de Gasparis]] pada 11 Mei 1850, asteroid kedua dari sembilan asteroid yang pernah dia temukan. Parthenope dinamai mengikuti salah satu [[Siren]] dalam [[mitologi Yunani]], yang dikatakan telah menemukan kota [[Napoli]]. De Gasparis "berusaha dengan sekuat tenaga untuk mewujudkan 'Parthenope' ada di surga (langit), nama yang disarankan oleh Sir [[John Herschel]] pada saat penemuan ''[[10 Hygiea|Hygeia]]'' pada tahun 1849".<ref>{{cite journal| bibcode=1850MNRAS..10..145.| last=De Gasparis| first= Annibale| title=The New Planet Parthenope| journal= Monthly notices of the Royal Astronomical Society| volume=10| pages=144–147| month=May| year= 1850}}</ref>
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|archive-date=2011-02-24
|archive-url=https://web.archive.org/web/20110224014158/http://www.springerlink.com/content/h747307j43863228/fulltext.pdf
|
}}</ref> dan massa jenisnya senilai 3.3 g/cm³.<ref name="Baer2007"/> Perkiraan yang dilakukan Baer pada tahun 2008 menyimpulkan bahwa massanya adalah 6,15{{e|18}}.<ref name=Baer>{{cite web
|year=2008
Baris 75 ⟶ 77:
|archive-date=2013-07-08
|archive-url=https://www.webcitation.org/6HxBzMsli?url=http://home.earthlink.net/~jimbaer1/astmass.txt
|
}}</ref> Perkiraan oleh Viateau dan Rapaport pada tahun 1997 dan 2001 menyimpulkan bahwa massanya mendekati nilai 5{{e|18}} kg dengan massa jenis 2.7 g/cm³.<ref name="Baer2007"/>
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* [http://lunar-occultations.com/iota/iotandx.htm IOTA] (International Occultation Timing Association) occultation database
* [http://www.asteroidoccultation.com/observations/Results/Data2011/20110126_Parthenope_InversionModel.jpg 2011-Jan-26 Occultation] {{Webarchive|url=https://web.archive.org/web/20140108170353/http://www.asteroidoccultation.com/observations/Results/Data2011/20110126_Parthenope_InversionModel.jpg |date=2014-01-08 }} / [http://www.asteroidoccultation.com/observations/Results/index2011.html (2011 Asteroidal Occultation Results for North America)]
* {{cite web |title=Elements and Ephemeris for (11) Parthenope |publisher=Minor Planet Center |url=http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=b2011&o=00011 |access-date=2012-03-07 |archive-date=2016-03-04 |archive-url=https://web.archive.org/web/20160304023625/http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=b2011&o=00011 |
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