https://arolstar52-zhtest.hf.space/index.php?action=history&feed=atom&title=HIP_41378_f
HIP 41378 f - 版本历史
2026-07-16T03:24:57Z
在这个wiki上该页的修订历史
MediaWiki 1.43.9
https://arolstar52-zhtest.hf.space/index.php?title=HIP_41378_f&diff=4442347&oldid=prev
imported>InternetArchiveBot：补救2个来源，并将0个来源标记为失效。) #IABot (v2.0.9.5
2024-05-29T07:54:28Z
<p>补救2个来源，并将0个来源标记为失效。) #IABot (v2.0.9.5</p>
<p><b>新页面</b></p><div>{{Infobox planet<br />
| name = HIP 41378 f<br />
<!-- DISCOVERY --><br />
| discovered = 2016年6月<br />
| discovery_method = 凌日法<br />
<!-- DESIGNATIONS --><br />
<!-- ORBITAL --> <br />
| apsis = astron<br />
| period = 542.07975±0.00014<br />
| semimajor = 1.37±0.02 [[天文單位|au]]<br />
| star = [[HIP 41378]]<ref name=NASA>{{cite web<br />
| url=http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=HIP+41378+f&type=CONFIRMED_PLANET<br />
| title=HIP 41378 f CONFIRMED PLANET OVERVIEW PAGE<br />
| work=NASA Exoplanet Archive<br />
| access-date=2016-07-08<br />
| archive-date=2023-09-24<br />
| archive-url=https://web.archive.org/web/20230924105118/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=HIP+41378+f&type=CONFIRMED_PLANET<br />
| dead-url=no<br />
}}</ref><br />
<!-- PHYS CHARS --> <br />
| mean_radius = 9.2 ± 0.1 {{Earth radius|link=y}}<br />
| mass = 12 ± 3 {{Earth_mass|link=y}}<br />
| single_temperature = [[Planetary equilibrium temperature|''T''<sub>eq</sub>]]: {{convert|294|K|C F}}<br />
| density = 0.09 ± 0.02 [[Gram|g]] [[cubic centimeter|cm<sup>−3</sup>]]<br />
<!-- ATMOSPHERE --> <br />
<!-- NOTES --> <br />
}}<br />
'''HIP 41378 f'''（也稱為'''EPIC 211311380 f'''）是一顆圍繞[[F型主序星|F型]][[恆星]][[HIP 41378]]的[[系外行星]]。它是其系統的最外層行星。對於其大小和溫度的行星來說，它的半徑異常大（9.2 {{Earth radius|link=y}}），因此半徑實際上可能是一個光學厚環系統的半徑<ref>{{Cite journal|last1=Akinsanmi|first1=B.|last2=Santos|first2=N. C.|last3=Faria|first3=J. P.|last4=Oshagh|first4=M.|last5=Barros|first5=S. C. C.|last6=Santerne|first6=A.|last7=Charnoz|first7=S.|date=2020-03-01|title=Can planetary rings explain the extremely low density of HIP 41378 𝑓?|url=https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|journal=Astronomy & Astrophysics|language=en|volume=635|pages=L8|doi=10.1051/0004-6361/202037618|issn=0004-6361|doi-access=free|arxiv=2002.11422|access-date=2024-05-21|archive-date=2021-10-28|archive-url=https://web.archive.org/web/20211028001745/https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|dead-url=no}}</ref>。它位於其母星的[[適居帶]]內<ref>{{cite arXiv|eprint=1911.07355|last1=Santerne|first1=A.|title=An extremely low-density and temperate giant exoplanet|last2=Malavolta|first2=L.|last3=Kosiarek|first3=M. R.|last4=Dai|first4=F.|last5=Dressing|first5=C. D.|last6=Dumusque|first6=X.|last7=Hara|first7=N. C.|last8=Lopez|first8=T. A.|last9=Mortier|first9=A.|last10=Vanderburg|first10=A.|last11=Adibekyan|first11=V.|last12=Armstrong|first12=D. J.|last13=Barrado|first13=D.|last14=Barros|first14=S. C. C.|last15=Bayliss|first15=D.|last16=Berardo|first16=D.|last17=Boisse|first17=I.|last18=Bonomo|first18=A. S.|last19=Bouchy|first19=F.|last20=Brown|first20=D. J. A.|last21=Buchhave|first21=L. A.|last22=Butler|first22=R. P.|last23=Collier Cameron|first23=A.|last24=Cosentino|first24=R.|last25=Crane|first25=J. D.|last26=Crossfield|first26=I. J. M.|last27=Damasso|first27=M.|last28=Deleuil|first28=M. R.|last29=Delgado Mena|first29=E.|last30=Demangeon|first30=O.|display-authors=29|class=astro-ph.EP|year=2019}}</ref>。沒有像2022年那樣發現大氣特徵，進一步強化了不透明環的假設<ref>{{citation|arxiv=2201.02686|year=2022|title=The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System|doi=10.3847/2041-8213/ac559d |last1=Alam |first1=Munazza K. |last2=Kirk |first2=James |last3=Dressing |first3=Courtney D. |last4=López-Morales |first4=Mercedes |last5=Ohno |first5=Kazumasa |last6=Gao |first6=Peter |last7=Akinsanmi |first7=Babatunde |last8=Santerne |first8=Alexandre |last9=Grouffal |first9=Salomé |last10=Adibekyan |first10=Vardan |last11=Barros |first11=Susana C. C. |last12=Buchhave |first12=Lars A. |last13=Crossfield |first13=Ian J. M. |last14=Dai |first14=Fei |last15=Deleuil |first15=Magali |last16=Giacalone |first16=Steven |last17=Lillo-Box |first17=Jorge |last18=Marley |first18=Mark |last19=Mayo |first19=Andrew W. |last20=Mortier |first20=Annelies |last21=Santos |first21=Nuno C. |last22=Sousa |first22=Sérgio G. |last23=Turtelboom |first23=Emma V. |last24=Wheatley |first24=Peter J. |last25=Vanderburg |first25=Andrew M. |journal=The Astrophysical Journal Letters |volume=927 |issue=1 |pages=L5 |bibcode=2022ApJ...927L...5A |s2cid=245837282 |doi-access=free }}</ref>。<br />
<br />
== 相關條目 ==<br />
* [[行星列表]]<br />
* [[GJ 1132b]]：確認具有大氣層的岩石系外行星。<br />
* [[天壇座μc]]：天壇座μ的系外行星<br />
* [[行星系]]<br />
<br />
== 參考資料 ==<br />
{{Reflist}}<br />
<br />
{{HIP 41378}}<br />
{{2016 in space}}<br />
{{巨蟹座恆星}}<br />
{{Portal bar|天文學|恆星|航天|太空|太陽系}}<br />
<br />
{{DEFAULTSORT:HIP 41378 f}}<br />
[[Category: 2016年發現的系外行星]]<br />
[[Category:凌星現象]]<br />
[[Category:HIP 41378]]<br />
[[Category:巨蟹座]]<br />
[[Category:適居帶中的巨型行星]]<br />
<br />
<br />
{{Extrasolar-planet-stub}}</div>
imported>InternetArchiveBot