Eris (planet katai): Perbedaan antara revisi

| bgcolour = #FFA0FF

| name = Eris

| symbol = <!--[[Berkas:FFHoE.svg|25px]] is there a source that clearly makes this official? -->

| image = [[Berkas:Eris and dysnomia2.jpg|240px|Eris (centre) and Dysnomia (left of centre), taken by the [[Hubble Space Telescope]].]]

| caption = Eris (Tengah) and [[Dysnomia (moon)|Dysnomia]] (kiri dari tengah).{{br}}[[Teleskop luar angkasa Hubble]].

| discovery = yes

| discoverer = [[Michael E. Brown|M. E. Brown]],{{br}}[[Chad Trujillo|C. A. Trujillo]],{{br}}[[David L. Rabinowitz|D. L. Rabinowitz]]<ref name="discovery">{{cite web

| author=Staff

| date=2007-05-01

| url=http://www.cfa.harvard.edu/iau/lists/NumberedMPs.html

| title=Discovery Circumstances: Numbered Minor Planets

| publisher=IAU: Minor Planet Center

| accessdate=2007-05-05 }}</ref>

| discovered = [[21 Oktober]] [[2003]]<ref name="discovery" />

| mp_name = '''136199 Eris'''

| alt_names = {{mp|2003 UB|313}}<ref name="designation">{{cite web

| author=Staff

| date=2004-02-29

| url=http://www.cfa.harvard.edu/iau/MPDes.html

| title=Minor Planet Designations

| publisher=IAU: Minor Planet Center

| accessdate=2007-05-05

| mp_category = [[Planet katai]],{{br}}[[Obyek trans-Neptunus|TNO]],{{br}}[[plutoid]],{{br}} dan [[Piringan tersebar|SDO]]<ref name=MPC>{{cite web

| epoch = [[6 Maret]], [[2006]]{{br}}([[Julian day|JD]] 2453800.5)<ref><!---[http://hamilton.dm.unipi.it/cgi-bin/astdys/astibo?list_objects:0;main AstDyS database] ---> [http://asteroid.lowell.edu/ Asteroid Observing Services]<!--- Actual page is ftp://ftp.lowell.edu/pub/elgb/astorb.html ---></ref>

| adjectives = Eridian

| aphelion = 97,56&nbsp;[[satuan astronomi|SA]]{{br}}14.60{{e|9}}km

| perihelion = 37,77&nbsp;SA {{br}}5.65{{e|9}} km

| semimajor = 67,6681&nbsp;SA {{br}}10.12{{e|9}} km

| eccentricity = 0,44177

| period = 203.600&nbsp;days{{br}}557&nbsp;[[julian year (astronomy)|tahun]]

| avg_speed = 3,436&nbsp;km/s

| mean_anomaly = 197,63427°

| inclination = 44,187°

| asc_node = 35,8696°

| arg_peri = 151,4305°

| satellites = 1

| physical_characteristics= yes

| mean_radius = 1.300 +200 -100&nbsp;km<ref name=spitzer>{{cite web|title=Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope|author=John Stansberry, Will Grundy, Mike Brown, John Spencer, David Trilling, Dale Cruikshank, Jean-Luc Margot | work= University of Arizona, Lowell Observatory, California Institute of Technology, NASA Ames Research Center, Southwest Research Institute, Cornell University|url=http://arxiv.org/abs/astro-ph/0702538v1|year=2007|accessdate=2007-05-18}}</ref>

| mass = (1,67 ± 0,02){{e|22}}&nbsp;kg<ref name=mass>{{cite journal

|url=http://www.sciencemag.org/cgi/content/abstract/316/5831/1585| pages=1585

| surface_grav = ~0,8 [[Acceleration|m/s²]]

| sidereal_day = >&nbsp;8&nbsp;h?

| albedo = 0,86&nbsp;±&nbsp;0,07

| temperatures = yes

| temp_name1 = (sekitar)

| min_temp_1 = 30&nbsp;[[Kelvin|K]]

| mean_temp_1 = 42,5&nbsp;K

| max_temp_1 = 55&nbsp;K

| magnitude = 18,7

| abs_magnitude = −1,12&nbsp;±&nbsp;0,01

| angular_size = 40 [[milliarcsecond|milli-arcsec]]<ref name="nature">

| title = The trans-Neptunian object {{mp|UB|313}} is larger than Pluto

| author =Bertoldi F., Altenhoff W., Weiss A., Menten K. M., Thum C.

| journal = Nature

| year = 2006

| volume =439

| issue = 7076

| pages = 563–564

| doi = 10.1038/nature04494

| pmid = 16452973