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	<id>https://arolstar52-zhtest.hf.space/index.php?action=history&amp;feed=atom&amp;title=WASP-49</id>
	<title>WASP-49 - 版本历史</title>
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	<updated>2026-07-14T03:14:23Z</updated>
	<subtitle>本wiki上该页面的版本历史</subtitle>
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	<entry>
		<id>https://arolstar52-zhtest.hf.space/index.php?title=WASP-49&amp;diff=3430823&amp;oldid=prev</id>
		<title>imported&gt;Yumeto：​Cat-a-lot：分类间移动：从Category:G-型主序星到Category:G型主序星 using Cat-a-lot</title>
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		<updated>2024-06-25T11:11:28Z</updated>

		<summary type="html">&lt;p&gt;&lt;a href=&quot;/wiki/Help:Cat-a-lot&quot; class=&quot;mw-redirect&quot; title=&quot;Help:Cat-a-lot&quot;&gt;Cat-a-lot&lt;/a&gt;：分类间移动：从&lt;a href=&quot;/wiki/Category:G-%E5%9E%8B%E4%B8%BB%E5%BA%8F%E6%98%9F&quot; title=&quot;Category:G-型主序星&quot;&gt;Category:G-型主序星&lt;/a&gt;到&lt;a href=&quot;/wiki/Category:G%E5%9E%8B%E4%B8%BB%E5%BA%8F%E6%98%9F&quot; title=&quot;Category:G型主序星&quot;&gt;Category:G型主序星&lt;/a&gt; using &lt;a href=&quot;/index.php?title=C:Help:Cat-a-lot&amp;amp;action=edit&amp;amp;redlink=1&quot; class=&quot;new&quot; title=&quot;C:Help:Cat-a-lot（页面不存在）&quot;&gt;Cat-a-lot&lt;/a&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{roughtranslation|time=2020-05-17T06:41:14+00:00}}&lt;br /&gt;
&lt;br /&gt;
{{Starbox begin}}&lt;br /&gt;
{{Starbox observe&lt;br /&gt;
| epoch = J2000&lt;br /&gt;
| constell = [[天兔座]]&lt;br /&gt;
| ra = {{RA|06|04|21.47346}}&amp;lt;ref name=DR2&amp;gt;{{cite DR2|2991284369063612928}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
| dec = {{DEC|-16|57|55.1088}}&amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
| appmag_v = 11.35&amp;lt;ref name=TYC2&amp;gt;{{cite journal|title=The Tycho-2 catalogue of the 2.5 million brightest stars|author1=Høg, E.|display-authors=etal|date=2000|journal=Astronomy and Astrophysics|volume=355|pages=L27–L30|bibcode=2000A&amp;amp;A...355L..27H}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox character&lt;br /&gt;
| class = G6V&amp;lt;ref name=wyttenbach2018/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox astrometry&lt;br /&gt;
| radial_v = 41.25&amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
| prop_mo_ra = 54.769&amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
| prop_mo_dec = -19.061&amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
| parallax = 5.1113&lt;br /&gt;
| p_error = 0.0314&lt;br /&gt;
| parallax_footnote = &amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox detail&lt;br /&gt;
| mass = 0.72&amp;lt;ref name=oza2019/&amp;gt;&lt;br /&gt;
| radius = 1.038&amp;lt;ref name=wyttenbach2018/&amp;gt;&lt;br /&gt;
| temperature = 5,600&amp;lt;ref name=oza2019/&amp;gt;&lt;br /&gt;
| luminosity = 0.884&amp;lt;ref name=DR2/&amp;gt;&lt;br /&gt;
| gravity = 4.5&amp;lt;ref name=wyttenbach2018/&amp;gt;&lt;br /&gt;
| rotation = &lt;br /&gt;
| age_gyr = 5.00&amp;lt;ref name=oza2019/&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox catalog&lt;br /&gt;
| names = {{odlist|TYC = 5936-2086-1|WDS= J06044-1658A | 2MASS = J06042146-1657550}}&amp;lt;ref name=SIMBAD&amp;gt;{{cite simbad|title=WASP-49|accessdate=2019-08-29}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox reference&lt;br /&gt;
| Simbad = WASP-49&lt;br /&gt;
}}&lt;br /&gt;
{{Starbox end}}&lt;br /&gt;
{{Infobox planet&lt;br /&gt;
| extrasolarplanet   = yes&lt;br /&gt;
| name               = WASP-49b&lt;br /&gt;
| image              = &amp;lt;!-- Use bare filename: Example.jpg --&amp;gt;&lt;br /&gt;
| image_size         = &amp;lt;!-- Overrides image size default of 225px --&amp;gt;&lt;br /&gt;
| image_alt          = &lt;br /&gt;
| caption            = &lt;br /&gt;
| apsis              = astron&lt;br /&gt;
| discovery_ref      = &amp;lt;ref&amp;gt;{{cite web |url=http://exoplanet.eu/catalog/wasp-49_b |title=European exoplanet catalog |accessdate=2019-08-29 |archive-date=2019-12-02 |archive-url=https://web.archive.org/web/20191202030259/http://exoplanet.eu/catalog/wasp-49_b/ }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
| discoverer         = 莫妮卡·倫德爾等人&lt;br /&gt;
| discovery_site     = &lt;br /&gt;
| discovered         = 2011&lt;br /&gt;
| discovery_method   = 主星凌&lt;br /&gt;
| alt_names          = &amp;lt;!--(Any alternative names for the body)--&amp;gt;&lt;br /&gt;
| periastron         = &lt;br /&gt;
| apoastron          = &lt;br /&gt;
| semimajor          = 0.0379±0.011 AU&lt;br /&gt;
| avg_speed          = &amp;lt;!--(Average orbital speed)--&amp;gt;&lt;br /&gt;
| eccentricity       = &lt;br /&gt;
| period             = 2.7817387 day&lt;br /&gt;
| inclination        = 84.89±0.19 deg&lt;br /&gt;
| angular_dist       = &lt;br /&gt;
| long_periastron    = &amp;lt;!--(Longitude of periastron)--&amp;gt;&lt;br /&gt;
| time_periastron    = &amp;lt;!--(Time of periastron)--&amp;gt;&lt;br /&gt;
| semi-amplitude     = &lt;br /&gt;
| mean_radius        = {{Jupiter radius|{{val|1.115|0.047|-0.047}}}}&lt;br /&gt;
| surface_area       = &lt;br /&gt;
| volume             = &lt;br /&gt;
| density            = &lt;br /&gt;
| mass               = {{Jupiter mass|{{val|0.378|0.027|-0.027}}}}&lt;br /&gt;
| surface_grav       = &amp;lt;!--Equatorial surface gravity--&amp;gt;&lt;br /&gt;
| moment_of_inertia_factor = &lt;br /&gt;
| escape_velocity    = &lt;br /&gt;
| albedo             = &lt;br /&gt;
| single_temperature = &lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;WASP-49&amp;#039;&amp;#039;&amp;#039;是一顆在主序帶的[[黃矮星]]，表面溫度是5,600K。WASP-49 缺乏重元素，相對於太陽的[[金屬量]]Fe/H指數為 -0.23，這意味著它含有的鐵是太陽的59%。&lt;br /&gt;
&lt;br /&gt;
== 行星系統 ==&lt;br /&gt;
在2011年，發現它有一顆行星，命名為WASP-49b。在2017年，發現它有一個廣泛的[[鈉]]包層&amp;lt;ref name=wyttenbach2018&amp;gt;{{cite journal|arxiv=1702.00448|doi=10.1051/0004-6361/201630063|title=Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS)|journal=Astronomy &amp;amp; Astrophysics|volume=602|pages=A36|year=2017|last1=Wyttenbach|first1=A.|last2=Lovis|first2=C.|last3=Ehrenreich|first3=D.|last4=Bourrier|first4=V.|last5=Pino|first5=L.|last6=Allart|first6=R.|last7=Astudillo-Defru|first7=N.|last8=Cegla|first8=H. M.|last9=Heng|first9=K.|last10=Lavie|first10=B.|last11=Melo|first11=C.|last12=Murgas|first12=F.|last13=Santerne|first13=A.|last14=Ségransan|first14=D.|last15=Udry|first15=S.|last16=Pepe|first16=F.}}&amp;lt;/ref&amp;gt;。在2019年，一項使用[[哈伯太空望遠鏡]]的[[紫外線|近紫外線]]數據的研究，發現包括[[鎂]]和[[鐵]]等金屬引起的明顯吸收特徵。鎂和鐵不是因為[[引力]]被行星拘束住，而可能是被行星的[[磁|磁性]]束縛著&amp;lt;ref&amp;gt;{{Cite journal|last=Sing|first=David K.|last2=Lavvas|first2=Panayotis|last3=Ballester|first3=Gilda E.|last4=Etangs|first4=Alain Lecavelier des|last5=Marley|first5=Mark S.|last6=Nikolov|first6=Nikolay|last7=Ben-Jaffel|first7=Lotfi|last8=Bourrier|first8=Vincent|last9=Buchhave|first9=Lars A.|last10=Deming|first10=Drake L.|last11=Ehrenreich|first11=David|display-authors=etal|date=2019-08-01|title=The HST PanCET Program: Exospheric Mg II and Fe II in the Near-UV transmission spectrum of WASP-121b using Jitter Decorrelation|journal=The Astronomical Journal|volume=158|issue=2|pages=91|doi=10.3847/1538-3881/ab2986|arxiv=1908.00619|issn=1538-3881|hdl=10150/634666|hdl-access=free}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite web|url=http://hubblesite.org/contents/news-releases/2019/news-2019-19|title=Hubble Uncovers a &amp;#039;Heavy Metal&amp;#039; Exoplanet Shaped Like a Football|website=HubbleSite.org|language=en|access-date=2020-01-01|archive-date=2021-11-09|archive-url=https://web.archive.org/web/20211109225919/https://hubblesite.org/contents/news-releases/2019/news-2019-19}}&amp;lt;/ref&amp;gt;。WASP-49b周圍的鈉包層可能來自類似[[木衛一|埃歐]]的[[系外衛星]] &amp;lt;ref name=oza2019&amp;gt;{{Cite journal|last=Oza|first=Apurva V.|last2=Johnson|first2=Robert E.|last3=Lellouch|first3=Emmanuel|last4=Schmidt|first4=Carl|last5=Schneider|first5=Nick|last6=Huang|first6=Chenliang|last7=Gamborino|first7=Diana|last8=Gebek|first8=Andrea|last9=Wyttenbach|first9=Aurelien|last10=Demory|first10=Brice-Olivier|last11=Mordasini|first11=Christoph|first12=Prabal|last12=Saxena|first13=David |last13=Dubois|first14=Arielle |last14=Moullet|first15=Nicolas |last15=Thomas|date=2019-08-28|title=Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets|arxiv=1908.10732 |bibcode=2019ApJ...885..168O |doi=10.3847/1538-4357/ab40cc |journal=[[The Astrophysical Journal]]|volume=885|issue=2|pages=168}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite web|url=https://www.unibe.ch/news/media_news/media_relations_e/media_releases/2019/medienmitteilungen_2019/hints_of_a_volcanically_active_exomoon/index_eng.html|title=Hints of a volcanically active exomoon|date=2019-08-29|website=Portal|access-date=2020-01-01|archive-date=2021-11-09|archive-url=https://web.archive.org/web/20211109224843/https://www.unibe.ch/news/media_news/media_relations_e/media_releases/2019/medienmitteilungen_2019/hints_of_a_volcanically_active_exomoon/index_eng.html}}&amp;lt;/ref&amp;gt;。這個新想法很有趣，但也頗具投機性&amp;lt;ref&amp;gt;{{Cite web|url=https://wasp-planets.net/2019/09/02/hints-of-volcanic-exo-moons/|title=Hints of volcanic exo-moons?|last=waspplanets|date=2019-09-02|website=WASP Planets|language=en|access-date=2020-01-01|archive-date=2021-05-08|archive-url=https://web.archive.org/web/20210508130738/https://wasp-planets.net/2019/09/02/hints-of-volcanic-exo-moons/}}&amp;lt;/ref&amp;gt;。&lt;br /&gt;
&lt;br /&gt;
== 參考資料 ==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
{{Sky|6|4|21.462|-|16|57|55.06|470}}&lt;br /&gt;
&lt;br /&gt;
{{Stars of Lepus}}&lt;br /&gt;
&lt;br /&gt;
[[Category:天兔座]]&lt;br /&gt;
[[Category:行星凌變星]]&lt;br /&gt;
[[Category:G型主序星]]&lt;/div&gt;</summary>
		<author><name>imported&gt;Yumeto</name></author>
	</entry>
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