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	<title>HD 212771 b - 版本历史</title>
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		<title>imported&gt;Willy1018-bot：​BOTR：批量替換所有lang-xx模板為langx模板</title>
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		<summary type="html">&lt;p&gt;&lt;a href=&quot;https://en.wikipedia.org/wiki/%E6%9C%BA%E5%99%A8%E4%BA%BA/%E4%BD%9C%E4%B8%9A%E8%AF%B7%E6%B1%82#.E8.AB.8B.E6.B1.82.E6.89.B9.E9.87.8F.E6.9B.BF.E6.8F.9B.E6.89.80.E6.9C.89lang-xx.E6.A8.A1.E6.9D.BF.E7.82.BAlangx.E6.A8.A1.E6.9D.BF&quot; class=&quot;extiw&quot; title=&quot;wikipedia:机器人/作业请求&quot;&gt;BOTR&lt;/a&gt;：批量替換所有lang-xx模板為langx模板&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{redirect-distinguish|太平山|太平山 (disambiguation){{!}太平山}}&lt;br /&gt;
{{Infobox planet&lt;br /&gt;
| name = HD 212771 b /太平山&lt;br /&gt;
&amp;lt;!-- DISCOVERY --&amp;gt;| discovery_ref = &amp;lt;ref name=&amp;quot;Johnson2010&amp;quot;/&amp;gt;&lt;br /&gt;
| discoverer = 約翰等人&lt;br /&gt;
| discovery_site = [[凱克天文台]]&lt;br /&gt;
| discovered = 2010-03-17&lt;br /&gt;
| discovery_method = [[都卜勒光譜學|都卜勒光譜]]&lt;br /&gt;
&amp;lt;!-- DESIGNATIONS --&amp;gt;&lt;br /&gt;
&amp;lt;!-- ORBITAL --&amp;gt;| orbit_ref = &amp;lt;ref name=&amp;quot;Luhn2019&amp;quot;/&amp;gt;&lt;br /&gt;
| semimajor = {{val|1.19|0.13|ul=AU}}&lt;br /&gt;
| eccentricity = {{val|0.076|0.051}}&lt;br /&gt;
| period = {{val|380.7|1.4|u=days}}&lt;br /&gt;
| time_periastron = {{val|2454920|52|ul=JD}}&lt;br /&gt;
| arg_peri = {{val|29|65|u=º}}&lt;br /&gt;
| semi-amplitude = {{val|50.0|5.8|ul=m/s}}&lt;br /&gt;
| star = [[HD 212771]]&lt;br /&gt;
&amp;lt;!-- PHYS CHARS --&amp;gt;| physical_ref = &amp;lt;ref name=&amp;quot;Luhn2019&amp;quot;/&amp;gt;&lt;br /&gt;
| mass = {{val|2.39|0.27|p=≥|ul=Jupiter mass}}&lt;br /&gt;
&amp;lt;!-- ATMOSPHERE --&amp;gt;&lt;br /&gt;
&amp;lt;!-- NOTES --&amp;gt;}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;HD 212771 b&amp;#039;&amp;#039;&amp;#039;是在星座[[寶瓶座]]&amp;lt;ref name=&amp;quot;Johnson2010&amp;quot;/&amp;gt;的一顆圍繞[[恆星光譜#G型|G型]]恆星[[HD 212771]]運行的[[太陽系外行星]]，距離大約364光年&amp;lt;ref name=&amp;quot;Gaia2016&amp;quot;/&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
== 名稱 ==&lt;br /&gt;
HD 212771 b的名稱是&amp;#039;&amp;#039;&amp;#039;太平山&amp;#039;&amp;#039;&amp;#039;（{{langx|en|&amp;#039;&amp;#039;&amp;#039;Victoriapeak&amp;#039;&amp;#039;&amp;#039;}}）。[[太平山 (香港)|太平山]]（{{langx|en|&amp;#039;&amp;#039;&amp;#039;Victoria peak&amp;#039;&amp;#039;&amp;#039;}}）是[[香港島]]上的最高點，在[[國際天文學聯合會|IAU]]成立100周年的[[IAU100太陽系外世界命名活動]]由[[香港]]地區的活動中，選出以之命名為「太平山」&amp;lt;ref&amp;gt;{{Cite web|url=http://www.nameexoworlds.iau.org/final-results|title=Approved names|website=NameExoworlds|language=en|access-date=2020-01-02|archive-date=2019-12-19|archive-url=https://web.archive.org/web/20191219084750/http://www.nameexoworlds.iau.org/final-results|dead-url=no}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite web|url=https://www.iau.org/news/pressreleases/detail/iau1912/|title=International Astronomical Union {{!}} IAU|website=www.iau.org|access-date=2020-01-02|archive-date=2020-04-08|archive-url=https://web.archive.org/web/20200408020100/https://www.iau.org/news/pressreleases/detail/iau1912/|dead-url=no}}&amp;lt;/ref&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
== 性質 ==&lt;br /&gt;
&lt;br /&gt;
=== 軌道 ===&lt;br /&gt;
HD 212771 b的軌道週期和距離都與[[地球]]相似，分別為380天和1.19[[天文單位|AU]]。與長週期氣態巨星相比，它的軌道幾乎是完美的圓形軌道。&lt;br /&gt;
&lt;br /&gt;
=== 特徵 ===&lt;br /&gt;
{{Planetary radius|align=right|Exoplanet=HD 212771 /太平山|radius=118}}&lt;br /&gt;
&lt;br /&gt;
由於軌道參數未知，這顆行星的真實質量尚不清楚，估計其質量至少是[[木星]]質量的2.39倍。HD 212771 b的半徑也未知，所以[[NASA]]的「系外行星之眼」給出的估計半徑是木星的1.18倍&amp;lt;ref&amp;gt;{{Cite web|title=Eyes On Exoplanets – Exoplanet Exploration: Planets Beyond our Solar System|url=https://exoplanets.nasa.gov/eyes-on-exoplanets/#/planet/HD_212771_b/|access-date=2021-06-06|website=exoplanets.nasa.gov|archive-date=2024-03-24|archive-url=https://web.archive.org/web/20240324092547/https://exoplanets.nasa.gov/eyes-on-exoplanets/#/planet/HD_212771_b/|dead-url=no}}&amp;lt;/ref&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
== 相關條目 ==&lt;br /&gt;
* [[HD 4313 b]]&lt;br /&gt;
* [[HD 181342 b]]&lt;br /&gt;
* [[HD 206610 b]]&lt;br /&gt;
* [[HD 180902 b]]&lt;br /&gt;
* [[HD 136418 b]]&lt;br /&gt;
&lt;br /&gt;
== 參考資料 ==&lt;br /&gt;
{{reflist|refs=&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Gaia2016&amp;quot;&amp;gt;{{cite journal | title=Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties | url=https://www.aanda.org/articles/aa/full_html/2016/11/aa29512-16/aa29512-16.html | last1=Brown | first1=A. G. A. | last2=Vallenari | first2=A. | last3=Prusti | first3=T. | last4=De Bruijne | first4=J. H. J. | last5=Mignard | first5=F. | last6=Drimmel | first6=R. | last7=Babusiaux | first7=C. | last8=Bailer-Jones | first8=C. A. L. | last9=Bastian | first9=U. | last10=Biermann | first10=M. | last11=Evans | first11=D. W. | last12=Eyer | first12=L. | last13=Jansen | first13=F. | last14=Jordi | first14=C. | last15=Katz | first15=D. | last16=Klioner | first16=S. A. | last17=Lammers | first17=U. | last18=Lindegren | first18=L. | last19=Luri | first19=X. | last20=o&amp;#039;Mullane | first20=W. | last21=Panem | first21=C. | last22=Pourbaix | first22=D. | last23=Randich | first23=S. | last24=Sartoretti | first24=P. | last25=Siddiqui | first25=H. I. | last26=Soubiran | first26=C. | last27=Valette | first27=V. | last28=Van Leeuwen | first28=F. | last29=Walton | first29=N. A. | last30=Aerts | first30=C. | display-authors=1 | journal=Astronomy and Astrophysics | volume=595 | at=A2 | year=2016 | arxiv=1609.04172 | bibcode=2016A&amp;amp;A...595A...2G | doi=10.1051/0004-6361/201629512 | s2cid=1828208 | access-date=2024-04-27 | archive-date=2020-10-15 | archive-url=https://web.archive.org/web/20201015143930/https://www.aanda.org/articles/aa/abs/2016/11/aa29512-16/aa29512-16.html | dead-url=no }}[http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&amp;amp;-source=I/337/tgas&amp;amp;recno=733014 Gaia Data Release 1 catalog entry] {{Wayback|url=http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&amp;amp;-source=I/337/tgas&amp;amp;recno=733014 |date=20220626113942 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Johnson2010&amp;quot;&amp;gt;{{cite journal | title=Retired a Stars and Their Companions. IV. Seven Jovian Exoplanets from Keck Observatory | last1=Johnson | first1=John Asher | last2=Howard | first2=Andrew W. | last3=Bowler | first3=Brendan P. | last4=Henry | first4=Gregory W. | last5=Marcy | first5=Geoffrey W. | last6=Wright | first6=Jason T. | last7=Fischer | first7=Debra A. | last8=Isaacson | first8=Howard | display-authors=1 | journal=Publications of the Astronomical Society of the Pacific | volume=122 | issue=892 | pages=701–711 | year=2010 | arxiv=1003.3445 | bibcode=2010PASP..122..701J | bibcode-access=free | doi=10.1086/653809 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;ref name=&amp;quot;Luhn2019&amp;quot;&amp;gt;{{cite journal | title=Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts | last1=Luhn | first1=Jacob K. | last2=Bastien | first2=Fabienne A. | last3=Wright | first3=Jason T. | last4=Johnson | first4=John A. | last5=Howard | first5=Andrew W. | last6=Isaacson | first6=Howard | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=149 | year=2019 | arxiv=1811.03043 | bibcode=2019AJ....157..149L | doi=10.3847/1538-3881/aaf5d0 | s2cid=102486961 | doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
== 外部連結 ==&lt;br /&gt;
* {{cite encyclopedia | url=https://exoplanet.eu/catalog/hd_212771_b--659/ | encyclopedia=[[Extrasolar Planets Encyclopaedia]] | title=HD 212771 b | date=1995 | access-date=2024-04-27 | archive-date=2024-05-01 | archive-url=https://web.archive.org/web/20240501152101/https://exoplanet.eu/catalog/hd_212771_b--659/ | dead-url=no }}&lt;br /&gt;
&lt;br /&gt;
{{Sky|22|27|03|-|17|15|49}}&lt;br /&gt;
{{寶瓶座}}&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:HD 212771 b}}&lt;br /&gt;
[[Category:2009年發現的系外行星]]&lt;br /&gt;
[[Category:徑向速度法發現的系外行星]]&lt;br /&gt;
[[Category:寶瓶座]]&lt;br /&gt;
[[Category:巨行星]]&lt;br /&gt;
[[Category:有專有名稱的系外行星]]&lt;/div&gt;</summary>
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