2 Pallas: Perbedaan antara revisi
Tampilan
Konten dihapus Konten ditambahkan
Luckas-bot (bicara | kontrib) k r2.7.1) (bot Menambah: be:(2) Палада |
Tidak ada ringkasan suntingan |
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Baris 1: | Baris 1: | ||
{{Infobox |
{{Infobox planet |
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| bgcolour=# |
| bgcolour=#BCD1F1 |
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| name=2 Pallas |
| name=2 Pallas |
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| symbol=[[ |
| symbol=[[Image:Pallas symbol.svg|25px]] |
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| physical_characteristics = |
| physical_characteristics = yes |
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| image= [[Image:PallasHST2007.jpg|275px]] |
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| image= |
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| caption= |
| caption= Citra ultraviolet dari Pallas yang diambil dari [[Teleskop Hubble]]. |
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| discovery= |
| discovery=yes |
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| discoverer=[[Heinrich Wilhelm Olbers]] |
| discoverer=[[Heinrich Wilhelm Olbers]] |
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| discovered=[[28 Maret]] |
| discovered=[[28 Maret]] [[1802]] |
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| pronounce = {{IPA-en|ˈpæləs|}} <ref group = note>In US dictionary transcription, {{USdict|păl′·əs}}. Or as {{Lang-el|''Παλλάς}}''.</ref> |
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| alt_names=''tidak ada'' |
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| |
| named_after = [[Athena|Pallas Athena]] |
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| note = yes |
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| epoch=[[26 November]] [[2005]] ([[hari Julian|HJ]] 2453700,5) |
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| mp_category=Keluarga Pallas |
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| semimajor=414,784 [[Giga|G]][[meter|m]] (2.773 [[satuan astronomi|AU]]) |
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| adjectives=Palladian<ref>[[OED]]</ref> |
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| perihelion=319,143 Gm (2,133 AU) |
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| orbit_ref=[ftp://ftp.lowell.edu/pub/elgb/astorb.html]<ref name="jpldata">{{cite web |
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| aphelion=510,425 Gm (3,412 AU) |
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|title=JPL Small-Body Database Browser: 2 Pallas |
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| eccentricity=0.231 |
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|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2 |
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| period=1686,333 [[hari|hr]] (4.62 [[hari Julian (astronomi)|a]]) |
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|accessdate=2009-09-12}}</ref> |
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| inclination=34,841[[derajat (sudut)|°]] |
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| epoch=[[22 Agustus]] [[2008]] ([[Hari Julian]] 2454700,5) |
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| asc_node=173,152° |
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| semimajor=2,772 SA (414,737 Gm) |
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| arg_peri=310,448° |
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| perihelion=2,132 SA (319,005 Gm) |
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| mean_anomaly=92,795° |
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| aphelion=3,412 [[Astronomical unit|SA]] (510,468 [[Giga|G]]m) |
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| avg_speed=17,65 km/[[detik|2]] |
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| eccentricity=0,231 |
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| dimensions=570×525×500 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> |
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| period=4,62 [[Tahun Julian|a]] (1686,044 [[hari|hr]]) |
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| mass=2.2×10<small><sup>20</sup></small> [[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> |
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| inclination=34,838[[Derajat (satuan sudut)|°]] ke [[Ekliptika]]<br>34,21° ke [[Bidang invariabel]]<ref name=meanplane>{{cite web |
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| density=2,8 g/[[senti|s]][[meter kubik|m³]] |
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|date=2009-04-03 |
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| surface_grav=0,18 m/s² |
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|title=The MeanPlane (Invariable plane) of the Solar System passing through the barycenter |
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| escape_velocity=0,32 km/s |
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|url=http://home.surewest.net/kheider/astro/MeanPlane.gif |
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| rotation=0,32555 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> |
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|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> |
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| 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> |
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| asc_node=173,134° |
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| magnitude = 6,4-10,6 |
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| arg_peri=310,274° |
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| 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> |
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| mean_anomaly=306,605° |
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| albedo=0.159 ([[albedo geometrik|geometrik]])<ref name="iras"/> |
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| avg_speed=17,65 km/[[detik|dtk]] |
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| angular_size = 0,59" <!-- Horizons 2014-Feb-24 --> hingga 0,17" |
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| p_orbit_ref = <ref name=Pallas-POE>{{cite web |
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| single_temperature=~164 [[Kelvin|K]]{{br}}''max:'' ~265 K (-8° [[Celsius|C]])}} |
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|title=AstDyS-2 Pallas Synthetic Proper Orbital Elements |
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|publisher=Department of Mathematics, University of Pisa, Italy |
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|url=http://hamilton.dm.unipi.it/astdys/index.php?pc=1.1.6&n=2 |
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|accessdate=2011-10-01}}</ref> |
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| p_semimajor = 2,7709176 |
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| p_eccentricity = 0,2812580 |
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| p_inclination = 33,1988686° |
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| p_mean_motion = 78.041654 |
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| perihelion_rate = -1,335344 |
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| node_rate = −46,393342 |
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| dimensions=582×556×500±18 km<ref name="Hubble"> |
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{{cite journal |
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|author=Schmidt, B. E., ''et al.'' |
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|title=Hubble takes a look at Pallas: Shape, size, and surface |
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|journal=39th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXIX). Held March 10–14, 2008, in League City, Texas. |
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|year=2008 |volume=1391 |page=2502 |
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|url=http://www.lpi.usra.edu/meetings/lpsc2008/pdf/2502.pdf |
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|format=PDF|accessdate=2008-08-24 |
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}}</ref><br>544 km ([[Rata-rata geometrik|rata-rata]])<ref name=jpldata/> |
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| mass=(2,11±0,26){{e|20}} kg<ref name="Baer2007"> |
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{{cite journal |
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|last=Baer |first=James |
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|coauthors=Steven R. Chesley |
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|title=Astrometric masses of 21 asteroids, and an integrated asteroid ephemeris |
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|journal=Celestial Mechanics and Dynamical Astronomy |
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|volume=100 |issue=2008 |pages=27–42 |
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|publisher=Springer Science+Business Media B.V. 2007 |
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|url=http://www.springerlink.com/content/h747307j43863228/fulltext.pdf |
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|format=PDF |
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|doi=10.1007/s10569-007-9103-8 |
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|accessdate=2008-11-11 |
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|year=2008 |
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|bibcode = 2008CeMDA.100...27B }}</ref> |
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| density=~2,8 g/[[centi-|c]]m³<ref name="Hubble"/> |
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| surface_grav=~0,18 m/s² |
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| escape_velocity=~0,32 km/s |
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| axial_tilt=sekitar 78 ± 13°<ref name="Torppa2003">{{cite journal |
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| author=Torppa, J.; ''et al.'' |
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| title=Shapes and rotational properties of thirty asteroids from photometric data |
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| journal=Icarus | year=2003 |
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| volume=164 | issue=2 | pages=346–383 |
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| bibcode=2003Icar..164..346T |
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| doi=10.1016/S0019-1035(03)00146-5 }}</ref> |
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| rotation=0,325 55 hari<br>(7,8132 jam)<ref name="lc"> |
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{{cite web |
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|last= Harris |first= A. W. |coauthors= Warner, B. D.; Pravec, P.; Eds. |
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|title= Asteroid Lightcurve Derived Data. EAR-A-5-DDR-Derived-Lightcurve-V8.0. |
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|publisher= [[Planetary Data System|NASA Planetary Data System]] |year= 2006 |
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|url= http://www.psi.edu/pds/resource/lc.html |
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|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> |
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| spectral_type=[[Asteroid tipe B]]<ref name="tax"> |
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{{cite web |
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|last= Neese |first= C. |coauthors= Ed. |
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|title= Asteroid Taxonomy. EAR-A-5-DDR-Taxonomy-V5.0. |
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|publisher= [[Planetary Data System|NASA Planetary Data System]] |
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|year= 2005 |
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|url= http://www.psi.edu/pds/resource/taxonomy.html |
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|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> |
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| magnitude = 6,4<ref name="Pasachoff1983"> |
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{{cite book |
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| author=Menzel, Donald H.; Pasachoff, Jay M. |
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| year=1983 |
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| title=A Field Guide to the Stars and Planets |
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| edition=2nd |
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| publisher=Houghton Mifflin |
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| page=391 |
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| location=Boston, MA |
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| isbn=0-395-34835-8 }}</ref> hingga 10,6 |
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| abs_magnitude=4,13<ref name="iras"> |
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{{cite web |
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|last= Tedesco |first= E. F. |coauthors= Noah, P. V.; Noah, M.; Price, S. D. |
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|title= IRAS Minor Planet Survey. IRAS-A-FPA-3-RDR-IMPS-V6.0. |
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|publisher= [[Planetary Data System|NASA Planetary Data System]] |year= 2004 |
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|url= http://www.psi.edu/pds/resource/imps.html |
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|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> |
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| albedo=0,159 ([[Albedo geometrik|geometrik]])<ref name="iras"/> |
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| 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" |
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| single_temperature=~164 [[Kelvin|K]]<br>''max:'' ~265 K (-8 °C) |
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}} |
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'''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. |
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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}} |
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* {{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. |
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{{Minor planets navigator|1 Ceres|3 Juno}} |
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{{Astronomi-stub}} |
{{Astronomi-stub}} |
Revisi per 24 Februari 2012 18.06
![]() Citra ultraviolet dari Pallas yang diambil dari Teleskop Hubble. | |
Penemuan | |
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Ditemukan oleh | Heinrich Wilhelm Olbers |
Tanggal penemuan | 28 Maret 1802 |
Penamaan | |
Pelafalan | [ˈpæləs] [note 1] |
Asal nama | Pallas Athena |
Keluarga Pallas | |
Kata sifat bahasa Inggris | Palladian[1] |
Ciri-ciri orbit[1][3] | |
Epos 22 Agustus 2008 (Hari Julian 2454700,5) | |
Aphelion | 3,412 SA (510,468 Gm) |
Perihelion | 2,132 SA (319,005 Gm) |
2,772 SA (414,737 Gm) | |
Eksentrisitas | 0,231 |
4,62 a (1686,044 hr) | |
Kecepatan orbit rata-rata | 17,65 km/dtk |
306,605° | |
Inklinasi | 34,838° ke Ekliptika 34,21° ke Bidang invariabel[2] |
173,134° | |
310,274° | |
Elemen orbit tetap[4] | |
Sumbu semimayor tetap | 2,7709176 AU |
Eksentrisitas tetap | 0,2812580 |
Inklinasi tetap | 33,1988686° |
Pergerakan rata-rata tetap | 78.041654 ° / tahun |
Periode orbit tetap | 4.61292 tahun (1684.869 hari) |
Presesi perihelion | -1,335344 arcsec / tahun |
Presesi node menaik | −46,393342 arcsec / tahun |
Ciri-ciri fisik | |
Dimensi | 582×556×500±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] | |
Albedo | 0,159 (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
- ^ OED
- ^ "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.
- ^ a b "JPL Small-Body Database Browser: 2 Pallas". Diakses tanggal 2009-09-12.
- ^ "AstDyS-2 Pallas Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Diakses tanggal 2011-10-01.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ Calculated with JPL Horizons for 2014-Feb-24
Pranala luar
- "2 Pallas". JPL Small-Body Database Browser. Diakses tanggal 2007-3-29.
- Tedesco, Edward F.; Noah, Paul V.; Noah, Meg; Price, Stephan D. (2002). "The Supplemental IRAS Minor Planet Survey". The Astronomical Journal. 123 (2): 1056–1085. Diakses tanggal 2007-3-15.
- Hilton, James L. (April 1, 1999). "U.S. Naval Observatory Ephemerides of the Largest Asteroids". U.S. Naval Observatory. Diakses tanggal 2007-3-14.
- Dunn, Tony (2006). "Ceres, Pallas Vesta and Hygeia". GravitySimulator.com. Diakses tanggal 2007-3-15.
- Yeomans, Donald K. "Horizons system". NASA JPL. Diakses tanggal 2007-3-20. — Horizons can be used to obtain a current ephemeris.
Navigasi planet minor
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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