2002 PY152: Perbedaan antara revisi

Konten dihapus Konten ditambahkan
Wagino Bot (bicara | kontrib)
k Rujukan: replaced: The International Astronomical Union Minor Planet Center → ''The International Astronomical Union Minor Planet Center''
HsfBot (bicara | kontrib)
k Bot: Penggantian teks otomatis (-{{astronomi-stub}}; +{{CentaurTNO-stub}})
 
(12 revisi perantara oleh 2 pengguna tidak ditampilkan)
Baris 1:
{{Infobox Planet
| minorplanet = yes
| width = 25em
| bgcolour =
| apsis =
| name = 2002 PY152
| symbol =
| image =
| caption =
| discovery = yes
| discovery_ref =
| discoverer =M. J. Holman;J. J. Kavelaars; T. Grav; W. Fraser
| discovery_site =807
| discovered = 2002/08/15
| designations = yes
| mp_name =
| alt_names =
| mp_category =
| orbit_ref =
| epoch =
| aphelion =43.892
| perihelion =43.337
| semimajor =43.614
| eccentricity =0.006
| period =
| avg_speed =
| inclination =5.2
| asc_node =131.1
| mean_anomaly =0.0
| arg_peri =178.6
| satellites =
| physical_characteristics = yes
| dimensions =
| mass =
| density =
| surface_grav =
| escape_velocity =
| sidereal_day =
| axial_tilt =
| pole_ecliptic_lat =
| pole_ecliptic_lon =
| albedo =
| temperatures=
| temp_name1 =
| mean_temp_1 =
| max_temp_1 =
| temp_name2 =
| max_temp_2 =
| spectral_type =
| abs_magnitude =9.4
}}
'''2002 PY152''' adalah sebuah [[objek trans-Neptunus]]. Seperti objek trans-Neptunus pada umumnya, benda ini mengorbit Matahari dari jarak yang lebih jauh dari planet [[Neptunus]].
Baris 54:
[[Eksentrisitas orbit]] objek ini tercatat sebesar 0.006, sementara [[magnitudo mutlak]]nya adalah 9.4.
 
== RujukanReferensi ==
 
* [http://www.minorplanetcenter.net/iau/lists/t_tnos.html Daftar Objek Transneptunus] - ''''''''The International Astronomical Union Minor Planet Center''''''.''
* {{cite journal|last=Remo|first=John L.|title=Classifying Solid Planetary Bodies|year=2007|journal=AIP Conference Proceedings|volume=886|pages=284–302|bibcode=2007AIPC..886..284R|doi=10.1063/1.2710063}}
{{astronomiCentaurTNO-stub}}
 
[[Kategori:Objek trans-Neptunus]]
 
 
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