2 Pallas: Perbedaan antara revisi

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{{Infobox Planet
{{Infobox planet
| bgcolour=#FFFFC0
| bgcolour=#BCD1F1
| name=2 Pallas
| name=2 Pallas
| symbol=[[Berkas:PallasHST2007.jpg|25px]]
| symbol=[[Image:Pallas symbol.svg|25px]]
| physical_characteristics = ya
| physical_characteristics = yes
| image= [[Image:PallasHST2007.jpg|275px]]
| image=
| caption=Gambaran ultraviolet 2 Pallas yang menunjukkan bentuk oktahedron yang sepenuhnya datar
| caption= Citra ultraviolet dari Pallas yang diambil dari [[Teleskop Hubble]].
| discovery=ya
| discovery=yes
| discoverer=[[Heinrich Wilhelm Olbers]]
| discoverer=[[Heinrich Wilhelm Olbers]]
| discovered=[[28 Maret]] [[1802]]
| discovered=[[28 Maret]] [[1802]]
| pronounce = {{IPA-en|ˈpæləs|}} <ref group = note>In US dictionary transcription, {{USdict|păl′·əs}}. Or as {{Lang-el|''Παλλάς}}''.</ref>
| alt_names=''tidak ada''
| mp_category=[[Keluarga Pallas]]
| named_after = [[Athena|Pallas Athena]]
| note = yes
| epoch=[[26 November]]&nbsp;[[2005]] ([[hari Julian|HJ]]&nbsp;2453700,5)
| mp_category=Keluarga Pallas
| semimajor=414,784&nbsp;[[Giga|G]][[meter|m]] (2.773&nbsp;[[satuan astronomi|AU]])
| adjectives=Palladian<ref>[[OED]]</ref>
| perihelion=319,143&nbsp;Gm (2,133&nbsp;AU)
| orbit_ref=[ftp://ftp.lowell.edu/pub/elgb/astorb.html]<ref name="jpldata">{{cite web
| aphelion=510,425&nbsp;Gm (3,412&nbsp;AU)
|title=JPL Small-Body Database Browser: 2 Pallas
| eccentricity=0.231
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2
| period=1686,333&nbsp;[[hari|hr]] (4.62&nbsp;[[hari Julian (astronomi)|a]])
|accessdate=2009-09-12}}</ref>
| inclination=34,841[[derajat (sudut)|°]]
| epoch=[[22 Agustus]] [[2008]] ([[Hari Julian]] 2454700,5)
| asc_node=173,152°
| semimajor=2,772 SA (414,737 Gm)
| arg_peri=310,448°
| perihelion=2,132 SA (319,005 Gm)
| mean_anomaly=92,795°
| aphelion=3,412 [[Astronomical unit|SA]] (510,468 [[Giga|G]]m)
| avg_speed=17,65&nbsp;km/[[detik|2]]
| eccentricity=0,231
| dimensions=570×525×500&nbsp;km<ref name="Drummond1989">{{cite journal | author=Drummond, J. D.; Cocke, W. J. | title=Triaxial ellipsoid dimensions and rotational pole of 2 Pallas from two stellar occultations | journal=Icarus | year=1989 | volume=78 | pages=323-329 | url=http://adsabs.harvard.edu/abs/1989Icar...78..323D | accessdate=2007-03-15 }}</ref><ref name="Dunham1990">{{cite journal | author=D. W. Dunham ''et al'' | title=The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae | journal=Astronomical Journal | year=1990 | volume=99 | pages=1636-1662 | url=http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1990AJ.....99.1636D | accessdate=2007-03-14 }}</ref>
| period=4,62 [[Tahun Julian|a]] (1686,044 [[hari|hr]])
| mass=2.2×10<small><sup>20</sup></small>&nbsp;[[kilogram|kg]]<ref name="Pitjeva2004">{{cite conference | first = E. V. | last = Pitjeva | authorlink = Elena V. Pitjeva | title = Estimations of masses of the largest asteroids and the main asteroid belt from ranging to planets, Mars orbiters and landers | booktitle = 35th COSPAR Scientific Assembly. Held 18 - 25 July 2004, in [[Paris, France]] | pages= 2014 | year= 2004 | url= http://adsabs.harvard.edu/abs/2004cosp.meet.2014P}}</ref><ref name="Goffin2001">{{cite journal | last=Goffin | first=E. | title=New determination of the mass of Pallas | journal=Astronomy and Astrophysics | year=2001 | volume=365 | pages=627-630 | url=http://adsabs.harvard.edu/abs/2001A&A...365..627G | accessdate=2007-03-15 }}</ref>
| inclination=34,838[[Derajat (satuan sudut)|°]] ke [[Ekliptika]]<br>34,21° ke [[Bidang invariabel]]<ref name=meanplane>{{cite web
| density=2,8&nbsp;g/[[senti|s]][[meter kubik|m³]]
|date=2009-04-03
| surface_grav=0,18&nbsp;m/s²
|title=The MeanPlane (Invariable plane) of the Solar System passing through the barycenter
| escape_velocity=0,32&nbsp;km/s
|url=http://home.surewest.net/kheider/astro/MeanPlane.gif
| rotation=0,32555&nbsp;d<ref name="lc">{{cite web | last= Harris | first= A. W. | authorlink= | coauthors= Warner, B.D.; Pravec, P.; Eds. | title= Asteroid Lightcurve Derived Data. EAR-A-5-DDR-DERIVED-LIGHTCURVE-V8.0. | work= | publisher= [[Planetary Data System|NASA Planetary Data System]] | date= 2006 | url= http://www.psi.edu/pds/resource/lc.html | format= | doi= | accessdate= 2007-03-15}}</ref>
|accessdate=2009-04-10|archiveurl=http://www.webcitation.org/5glwILykY|archivedate=2009-05-14|deadurl=no}} (produced with [http://chemistry.unina.it/~alvitagl/solex/ Solex 10] written by Aldo Vitagliano; see also [[Invariable plane]]). Retrieved 2009-04-25.</ref>
| spectral_type=[[asteroid tipe B]]<ref name="tax">{{cite web | last= Neese | first= C. | authorlink= | coauthors= Ed. | title= Asteroid Taxonomy.EAR-A-5-DDR-TAXONOMY-V5.0. | work= | publisher= [[Planetary Data System|NASA Planetary Data System]] | date= 2005 | url= http://www.psi.edu/pds/resource/taxonomy.html | format= | doi= | accessdate= 2007-03-15}}</ref>
| asc_node=173,134°
| magnitude = 6,4-10,6
| arg_peri=310,274°
| abs_magnitude=4,13<ref name="iras">{{cite web | last= Tedesco | first= E.F. | authorlink= | coauthors= Noah, P.V.; Noah, M.; Price, S.D. | title= IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0. | work= | publisher= [[Planetary Data System|NASA Planetary Data System]] | date= 2004 | url= http://www.psi.edu/pds/resource/imps.html | format= | doi= | accessdate= 2007-03-15}}</ref>
| mean_anomaly=306,605°
| albedo=0.159 ([[albedo geometrik|geometrik]])<ref name="iras"/>
| avg_speed=17,65 km/[[detik|dtk]]
| angular_size = 0,59" <!-- Horizons 2014-Feb-24 --> hingga 0,17"
| p_orbit_ref = <ref name=Pallas-POE>{{cite web
| single_temperature=~164&nbsp;[[Kelvin|K]]{{br}}''max:'' ~265&nbsp;K (-8°&nbsp;[[Celsius|C]])}}
|title=AstDyS-2 Pallas Synthetic Proper Orbital Elements
|publisher=Department of Mathematics, University of Pisa, Italy
|url=http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.6&n=2
|accessdate=2011-10-01}}</ref>
| p_semimajor = 2,7709176
| p_eccentricity = 0,2812580
| p_inclination = 33,1988686°
| p_mean_motion = 78.041654
| perihelion_rate = -1,335344
| node_rate = −46,393342
| dimensions=582×556×500±18&nbsp;km<ref name="Hubble">
{{cite journal
|author=Schmidt, B. E., ''et al.''
|title=Hubble takes a look at Pallas: Shape, size, and surface
|journal=39th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXIX). Held March 10–14, 2008, in League City, Texas.
|year=2008 |volume=1391 |page=2502
|url=http://www.lpi.usra.edu/meetings/lpsc2008/pdf/2502.pdf
|format=PDF|accessdate=2008-08-24
}}</ref><br>544 km ([[Rata-rata geometrik|rata-rata]])<ref name=jpldata/>
| mass=(2,11±0,26){{e|20}}&nbsp;kg<ref name="Baer2007">
{{cite journal
|last=Baer |first=James
|coauthors=Steven R. Chesley
|title=Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris
|journal=Celestial Mechanics and Dynamical Astronomy
|volume=100 |issue=2008 |pages=27–42
|publisher=Springer Science+Business Media B.V. 2007
|url=http://www.springerlink.com/content/h747307j43863228/fulltext.pdf
|format=PDF
|doi=10.1007/s10569-007-9103-8
|accessdate=2008-11-11
|year=2008
|bibcode = 2008CeMDA.100...27B }}</ref>
| density=~2,8&nbsp;g/[[centi-|c]]m³<ref name="Hubble"/>
| surface_grav=~0,18&nbsp;m/s²
| escape_velocity=~0,32&nbsp;km/s
| axial_tilt=sekitar 78&nbsp;±&nbsp;13°<ref name="Torppa2003">{{cite journal
| author=Torppa, J.; ''et al.''
| title=Shapes and rotational properties of thirty asteroids from photometric data
| journal=Icarus | year=2003
| volume=164 | issue=2 | pages=346–383
| bibcode=2003Icar..164..346T
| doi=10.1016/S0019-1035(03)00146-5 }}</ref>
| rotation=0,325&nbsp;55&nbsp;hari<br>(7,8132 jam)<ref name="lc">
{{cite web
|last= Harris |first= A. W. |coauthors= Warner, B. D.; Pravec, P.; Eds.
|title= Asteroid Lightcurve Derived Data. EAR-A-5-DDR-Derived-Lightcurve-V8.0.
|publisher= [[Planetary Data System|NASA Planetary Data System]] |year= 2006
|url= http://www.psi.edu/pds/resource/lc.html
|accessdate= 2007-03-15 |archiveurl = http://web.archive.org/web/20070128183706/http://www.psi.edu/pds/resource/lc.html <!-- Bot retrieved archive --> |archivedate = 2007-01-28}}</ref>
| spectral_type=[[Asteroid tipe B]]<ref name="tax">
{{cite web
|last= Neese |first= C. |coauthors= Ed.
|title= Asteroid Taxonomy. EAR-A-5-DDR-Taxonomy-V5.0.
|publisher= [[Planetary Data System|NASA Planetary Data System]]
|year= 2005
|url= http://www.psi.edu/pds/resource/taxonomy.html
|accessdate= 2007-03-15 |archiveurl = http://web.archive.org/web/20070310220044/http://www.psi.edu/pds/resource/taxonomy.html <!-- Bot retrieved archive --> |archivedate = 2007-03-10}}</ref>
| magnitude = 6,4<ref name="Pasachoff1983">
{{cite book
| author=Menzel, Donald H.; Pasachoff, Jay M.
| year=1983
| title=A Field Guide to the Stars and Planets
| edition=2nd
| publisher=Houghton Mifflin
| page=391
| location=Boston, MA
| isbn=0-395-34835-8 }}</ref> hingga 10,6
| abs_magnitude=4,13<ref name="iras">
{{cite web
|last= Tedesco |first= E. F. |coauthors= Noah, P. V.; Noah, M.; Price, S. D.
|title= IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0.
|publisher= [[Planetary Data System|NASA Planetary Data System]] |year= 2004
|url= http://www.psi.edu/pds/resource/imps.html
|accessdate= 2007-03-15 |archiveurl = http://web.archive.org/web/20070311123634/http://www.psi.edu/pds/resource/imps.html <!-- Bot retrieved archive --> |archivedate = 2007-03-11}}</ref>
| albedo=0,159 ([[Albedo geometrik|geometrik]])<ref name="iras"/>
| angular_size = 0,59"<ref name=opp2014>Calculated with [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2 JPL Horizons] for 2014-Feb-24</ref> hingga 0,17"
| single_temperature=~164&nbsp;[[Kelvin|K]]<br>''max:'' ~265&nbsp;K (-8&nbsp;°C)
}}

'''2 Pallas''' ({{IPAEng|ˈpæləs}}, [[bahasa Yunani]]: ''Παλλάς'') merupakan [[asteroid]] besar yang terletak di [[sabuk asteroid]] [[sistem tata surya]] dan merupakan asteroid ke-2 yang ditemukan. Ditemukan dan dinamai oleh [[astronom]] [[Heinrich Wilhelm Matthaus Olbers]] pada tanggal [[28 Maret]] [[1802]]. 2 Pallas merupakan salah satu dari 4 asteroid besar ([[1 Ceres]], [[4 Vesta]], [[10 Hygiea]], dan Pallas). Asteroid besar tersebut tak termasuk [[704 Interamnia]]. Pallas berukuran sama seperti 4 Vesta.
'''2 Pallas''' ({{IPAEng|ˈpæləs}}, [[bahasa Yunani]]: ''Παλλάς'') merupakan [[asteroid]] besar yang terletak di [[sabuk asteroid]] [[sistem tata surya]] dan merupakan asteroid ke-2 yang ditemukan. Ditemukan dan dinamai oleh [[astronom]] [[Heinrich Wilhelm Matthaus Olbers]] pada tanggal [[28 Maret]] [[1802]]. 2 Pallas merupakan salah satu dari 4 asteroid besar ([[1 Ceres]], [[4 Vesta]], [[10 Hygiea]], dan Pallas). Asteroid besar tersebut tak termasuk [[704 Interamnia]]. Pallas berukuran sama seperti 4 Vesta.


Baris 46: Baris 126:
* {{cite web | last=Dunn | first=Tony | year=[[2006]] | url=http://orbitsimulator.com/gravity/articles/ceres.html | title=Ceres, Pallas Vesta and Hygeia | publisher=GravitySimulator.com | accessdate=2007-3-15}}
* {{cite web | last=Dunn | first=Tony | year=[[2006]] | url=http://orbitsimulator.com/gravity/articles/ceres.html | title=Ceres, Pallas Vesta and Hygeia | publisher=GravitySimulator.com | accessdate=2007-3-15}}
* {{cite web | last = Yeomans | first = Donald K. | url = http://ssd.jpl.nasa.gov/?horizons | title = Horizons system | publisher = [[NASA]] [[JPL]] | accessdate = 2007-3-20 }} — Horizons can be used to obtain a current ephemeris.
* {{cite web | last = Yeomans | first = Donald K. | url = http://ssd.jpl.nasa.gov/?horizons | title = Horizons system | publisher = [[NASA]] [[JPL]] | accessdate = 2007-3-20 }} — Horizons can be used to obtain a current ephemeris.

{{Minor planets navigator|1 Ceres|3 Juno}}


{{Astronomi-stub}}
{{Astronomi-stub}}

Revisi per 24 Februari 2012 18.06

2 Pallas
Citra ultraviolet dari Pallas yang diambil dari Teleskop Hubble.
Penemuan
Ditemukan olehHeinrich Wilhelm Olbers
Tanggal penemuan28 Maret 1802
Penamaan
Pelafalan[ˈpæləs] [note 1]
Asal nama
Pallas Athena
Keluarga Pallas
Kata sifat bahasa InggrisPalladian[1]
Ciri-ciri orbit[1][3]
Epos 22 Agustus 2008 (Hari Julian 2454700,5)
Aphelion3,412 SA (510,468 Gm)
Perihelion2,132 SA (319,005 Gm)
2,772 SA (414,737 Gm)
Eksentrisitas0,231
4,62 a (1686,044 hr)
Kecepatan orbit rata-rata
17,65 km/dtk
306,605°
Inklinasi34,838° ke Ekliptika
34,21° ke Bidang invariabel[2]
173,134°
310,274°
Elemen orbit tetap[4]
2,7709176 AU
0,2812580
Inklinasi tetap
33,1988686°
78.041654 ° / tahun
4.61292 tahun
(1684.869 hari)
Presesi perihelion
-1,335344 arcsec / tahun
Presesi node menaik
−46,393342 arcsec / tahun
Ciri-ciri fisik
Dimensi582×556×500±18 km[5]
544 km (rata-rata)[3]
Massa(2,11±0,26)×1020 kg[6]
Massa jenis rata-rata
~2,8 g/cm³[5]
~0,18 m/s²
~0,32 km/s
0,325 55 hari
(7,8132 jam)[7]
sekitar 78 ± 13°[8]
Albedo0,159 (geometrik)[9]
Suhu~164 K
max: ~265 K (-8 °C)
Pola spektrum
Asteroid tipe B[10]
6,4[11] hingga 10,6
4,13[9]
0,59"[12] hingga 0,17"

2 Pallas (pengucapan bahasa Inggris: [ˈpæləs], bahasa Yunani: Παλλάς) merupakan asteroid besar yang terletak di sabuk asteroid sistem tata surya dan merupakan asteroid ke-2 yang ditemukan. Ditemukan dan dinamai oleh astronom Heinrich Wilhelm Matthaus Olbers pada tanggal 28 Maret 1802. 2 Pallas merupakan salah satu dari 4 asteroid besar (1 Ceres, 4 Vesta, 10 Hygiea, dan Pallas). Asteroid besar tersebut tak termasuk 704 Interamnia. Pallas berukuran sama seperti 4 Vesta.

Rujukan

  1. ^ OED
  2. ^ "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". 2009-04-03. Diarsipkan dari versi asli tanggal 2009-05-14. Diakses tanggal 2009-04-10.  (produced with Solex 10 written by Aldo Vitagliano; see also Invariable plane). Retrieved 2009-04-25.
  3. ^ a b "JPL Small-Body Database Browser: 2 Pallas". Diakses tanggal 2009-09-12. 
  4. ^ "AstDyS-2 Pallas Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Diakses tanggal 2011-10-01. 
  5. ^ a b Schmidt, B. E.; et al. (2008). "Hubble takes a look at Pallas: Shape, size, and surface" (PDF). 39th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXIX). Held March 10–14, 2008, in League City, Texas. 1391: 2502. Diakses tanggal 2008-08-24. 
  6. ^ Baer, James (2008). "Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris" (PDF). Celestial Mechanics and Dynamical Astronomy. Springer Science+Business Media B.V. 2007. 100 (2008): 27–42. Bibcode:2008CeMDA.100...27B. doi:10.1007/s10569-007-9103-8. Diakses tanggal 2008-11-11. 
  7. ^ Harris, A. W. (2006). "Asteroid Lightcurve Derived Data. EAR-A-5-DDR-Derived-Lightcurve-V8.0". NASA Planetary Data System. Diarsipkan dari versi asli tanggal 2007-01-28. Diakses tanggal 2007-03-15. 
  8. ^ Torppa, J.; et al. (2003). "Shapes and rotational properties of thirty asteroids from photometric data". Icarus. 164 (2): 346–383. Bibcode:2003Icar..164..346T. doi:10.1016/S0019-1035(03)00146-5. 
  9. ^ a b Tedesco, E. F. (2004). "IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0". NASA Planetary Data System. Diarsipkan dari versi asli tanggal 2007-03-11. Diakses tanggal 2007-03-15. 
  10. ^ Neese, C. (2005). "Asteroid Taxonomy. EAR-A-5-DDR-Taxonomy-V5.0". NASA Planetary Data System. Diarsipkan dari versi asli tanggal 2007-03-10. Diakses tanggal 2007-03-15. 
  11. ^ Menzel, Donald H.; Pasachoff, Jay M. (1983). A Field Guide to the Stars and Planets (edisi ke-2nd). Boston, MA: Houghton Mifflin. hlm. 391. ISBN 0-395-34835-8. 
  12. ^ Calculated with JPL Horizons for 2014-Feb-24

Pranala luar


Navigasi planet minor
Didahului oleh:
1 Ceres
2 Pallas Diikuti oleh:
3 Juno


Kesalahan pengutipan: Ditemukan tag <ref> untuk kelompok bernama "note", tapi tidak ditemukan tag <references group="note"/> yang berkaitan