HD 164922 b: Perbedaan antara revisi

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{{Infobox planet|name=HD 164922 b
| name = HD 164922 b
<!-- DISCOVERY -->|discoverer=[[R. Paul Butler|Butler]] et al.<ref name="Butler20063"/>|discovery_site=[[California]], [[United States|USA]]|discovered=July 15, 2006|discovery_method=[[Kecepatan Radial]]
<!-- DISCOVERY -->
| discoverer = [[R. Paul Butler|Butler]] et al.<ref name="Butler2006">{{cite journal | title=Catalog of Nearby Exoplanets | last1=Butler | first1=R. P. | last2=Wright | first2=J. T. | last3=Marcy | first3=G. W. | last4=Fischer | first4=D. A. | last5=Vogt | first5=S. S. | last6=Tinney | first6=C. G. | last7=Jones | first7=H. R. A. | last8=Carter | first8=B. D. | last9=Johnson | first9=J. A. | last10=McCarthy | first10=C. | last11=Penny | first11=A. J. | display-authors=1 | journal=The Astrophysical Journal | volume=646 | issue=1 | pages=505–522 | year=2006 | arxiv=astro-ph/0607493 | bibcode=2006ApJ...646..505B | doi=10.1086/504701 }}</ref>
| discovery_site = [[California]], [[Amerika Serikat|AS]]
| discovered = 15 Juli 2006
| discovery_method = [[Kecepatan radial]]
<!-- DESIGNATIONS -->
<!-- ORBITAL -->
<!-- ORBITAL -->|apsis=astron|semimajor={{convert|2.11|±|0.13|AU|km|abbr=on}}|eccentricity=0.05 ± 0.14|period=1155 ± 23 [[hari|h]]|time_periastron=2,411,100 ± 280|arg_peri=195|semi-amplitude=7.3 ± 1.2|star=[[HD 164922]]
<!--| PHYSapsis CHARS -->|mean_radius= ~8 R⊕ = astron
| semimajor = {{convert|2.11|±|0.13|AU|km|abbr=on}}
|single_temperature={{convert|159|K|C F}}<ref name="New">{{Cite journal|arxiv=1607.00007|last1= Fulton|first1= Benjamin J.|title= Three Temperate Neptunes Orbiting Nearby Stars|journal= The Astrophysical Journal|volume= 830|issue= 1|pages= 46|last2= Howard|first2= Andrew W.|last3= Weiss|first3= Lauren M.|last4= Sinukoff|first4= Evan|last5= Petigura|first5= Erik A.|last6= Isaacson|first6= Howard|last7= Hirsch|first7= Lea|last8= Marcy|first8= Geoffrey W.|last9= Henry|first9= Gregory W.|last10= Grunblatt|first10= Samuel K.|last11= Huber|first11= Daniel|author12= Kaspar von Braun|last13= Boyajian|first13= Tabetha S.|last14= Kane|first14= Stephen R.|last15= Wittrock|first15= Justin|last16= Horch|first16= Elliott P.|last17= Ciardi|first17= David R.|last18= Howell|first18= Steve B.|last19= Wright|first19= Jason T.|last20= Ford|first20= Eric B.|year= 2016|doi= 10.3847/0004-637X/830/1/46|bibcode = 2016ApJ...830...46F }}</ref>
| eccentricity = 0,05 ± 0,14
| period = 1155 ± 23 [[hari|h]]
| time_periastron = 2.411.100 ± 280
| arg_peri = 195
| semi-amplitude = 7,3 ± 1,2
| star = [[HD 164922]]
<!-- PHYS CHARS -->
| mean_radius = ~8 {{Earth radius|link=y}}
| single_temperature = {{convert|159|K|C F}}<ref name="New">{{Cite journal|arxiv=1607.00007|last1= Fulton|first1= Benjamin J.|title= Three Temperate Neptunes Orbiting Nearby Stars|journal= The Astrophysical Journal|volume= 830|issue= 1|pages= 46|last2= Howard|first2= Andrew W.|last3= Weiss|first3= Lauren M.|last4= Sinukoff|first4= Evan|last5= Petigura|first5= Erik A.|last6= Isaacson|first6= Howard|last7= Hirsch|first7= Lea|last8= Marcy|first8= Geoffrey W.|last9= Henry|first9= Gregory W.|last10= Grunblatt|first10= Samuel K.|last11= Huber|first11= Daniel|author12= Kaspar von Braun|last13= Boyajian|first13= Tabetha S.|last14= Kane|first14= Stephen R.|last15= Wittrock|first15= Justin|last16= Horch|first16= Elliott P.|last17= Ciardi|first17= David R.|last18= Howell|first18= Steve B.|last19= Wright|first19= Jason T.|last20= Ford|first20= Eric B.|year= 2016|doi= 10.3847/0004-637X/830/1/46|bibcode = 2016ApJ...830...46F }}</ref>
<!-- ATMOSPHERE -->
<!-- NOTES -->|image=
}}
'''HD 164922 b''' adalah [[Planet luar tata suryaEksoplanet|planet luar suryaekstrasurya]] bermassa Saturnus yang mengorbit bintang [[HD 164922]], sekitar 72 tahun [[Tahun cahaya|cahaya]] dari Bumi di konstelasi [[Herkules (rasi bintang)|Hercules]]. <span data-segmentid="85" class="cx-segment">[[Inklinasi]]nya tidak diketahui, dan [[Massa sejati|massa minimalnya]] dapat secara signifikan lebih besar dari batas bawah kecepatan radial massa Jupiter 0,36.</span> <span data-segmentid="88" class="cx-segment">Planet ini juga memiliki eksentrisitas rendah, yang hampir sama dengan [[Yupiter|Jupiter]] dan [[Saturnus]], yaitu 0.05.<ref name="Butler20063"><cite class="citation journal">Butler, R. P.; et al. (2006). [http://iopscience.iop.org/0004-637X/646/1/505/fulltext/ "Catalog of Nearby Exoplanets"]. ''The Astrophysical Journal''. '''646''' (1): 505–522. [[arXiv]]:<span class="cs1-lock-free" title="Freely accessible">[//arxiv.org/abs/astro-ph/0607493 astro-ph/0607493]</span>. [[Bibcode]]:[[bibcode:2006ApJ...646..505B|2006ApJ...646..505B]]. [[Digital object identifier|doi]]:[[doi:10.1086/504701|10.1086/504701]].</cite></ref></span> <span data-segmentid="92" class="cx-segment">Planet ini ditemukan pada tahun 2006 dengan menggunakan teknik [[kecepatan radial]] melalui pengamatan [[Efek Doppler|pergeseran Doppler]] dalam [[spektrum]] [[HD 164922|bintang induk]] planet.</span><ref>{{Cite web|url=http://www.openexoplanetcatalogue.com/planet/HD%20164922%20b/|title=Open Exoplanet Catalogue - HD 164922 b|last=|first=|date=|website=|access-date=}}</ref>
 
== Karakteristik ==
 
=== Massa, Radius, dan Suhu ===
<span data-segmentid="100" class="cx-segment">HD 164922 b adalah [[raksasa gas]] yang memilik</span><span data-segmentid="104" class="cx-segment">i memiliki suhu {{Convert|159|K|C F}}.</span> <span data-segmentid="105" class="cx-segment">Berdasarkan massanya yang mirip Saturnus (yang terukur sekitar 0,36 M<sub>J)</sub>, radius potensialnya sekitar 8 R⊕{{Earth radius}}</span>
 
=== Bintang Induk ===
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== Referensi ==
<references />
{{Sky|18|02|30.86|+|26|18|46.81}}
[[Kategori:Eksoplanet]]
[[Kategori:Hercules (Rasi bintang)]]