Kepler-11: Perbedaan antara revisi

Konten dihapus Konten ditambahkan
Tidak ada ringkasan suntingan
InternetArchiveBot (bicara | kontrib)
Rescuing 1 sources and tagging 0 as dead.) #IABot (v2.0.8.5
 
(33 revisi perantara oleh 18 pengguna tidak ditampilkan)
Baris 1:
{{inuse}}
{{Starbox begin
| name= Kepler-11
Baris 8 ⟶ 7:
}}
{{Starbox observe
| constell= [[Cygnus (rasi bintang)|Cygnus]]
| epoch= J2000
| ra= {{RA|19|48|27.62}}
| dec= {{DEC|+41|54|32.9}}
| appmag_v= 14.2<ref name="Ames">{{cite web|title=Kepler Discoveries|publisher=NASA Ames Research Center|url=http://kepler.nasa.gov/Mission/discoveries/|accessdate=4 February 2011|archive-date=2017-04-01|archive-url=https://web.archive.org/web/20170401080610/https://kepler.nasa.gov/MIssion/discoveries/|dead-url=yes}}</ref>
}}
{{Starbox astrometry
Baris 32 ⟶ 31:
{{Starbox end}}
 
'''Kepler-11''' adalah bintang seperti matahariMatahari yang dikitari oleh paling tidak enam [[planet luar surya|planet]]. Bintang ini terletak di rasi bintang [[Cygnus_(rasi bintang)|Cygnus]] dan berjarak sekitar 2.000 tahun cahaya dari Bumi.<ref name = "Lissauer">{{Cite journal | last=Lissauer | first=J. J. | authorlink=Jack J. Lissauer | coauthors = ''et al.'' | title=A closely packed system of low-mass, low-density planets transiting Kepler-11 | journal=Nature | volume=470 | issue= | pages=53–58 | date=3 February 2011 | url=http://arxiv.org/pdf/1102.0291v1.pdf | doi=10.1038/nature09760 | accessdate=4 February 2011}}</ref> Bintang ini ditemukan oleh [[Kepler (pesawat angkasa)|teleskop angkasa Kepler]], dan penemuannya diumumkan pada tanggal 2 Februari 2011.
 
Sistem bintang Kepler-11 sangat rapat dan memadati bintang induk. Lima planet tampak seperti mengumpul, sementara satu lainnya seperti "terpental".
 
== Planet ==
Planet-planet yang mengitari bintang ini dinamai secara alfabetis: ''b'', ''c'', ''d'', ''e'', ''f'', dan ''g''. Ukuran planet-planet tersebut berkisar antara ukuran [[Bumi]] dan [[Neptunus]]. Massa jenis mereka yang rendah menunjukkan bahwa tidak ada satu pun dari planet-planet itu yang komposisinya seperti Bumi.<ref name="Boyle">{{Cite news| last=Boyle | first=Alan | authorlink=Alan Boyle | title=Planetary six-pack poses a puzzle | work =MSNBC Cosmic Log | date=2 February 2011 | url=http://cosmiclog.msnbc.msn.com/_news/2011/02/01/5972312-planetary-six-pack-poses-a-puzzle | accessdate=4-02-2011|archive-date=2018-05-13|archive-url=https://web.archive.org/web/20180513081432/http://cosmiclog.msnbc.msn.com/_news/2011/02/01/5972312-planetary-six-pack-poses-a-puzzle|dead-url=yes}}</ref><!-- Atmosfer [[hidrogen]] aditemui significantpada [[hydrogen]] atmosphere is indicated for planetsplanet ''d'', ''e'' anddan perhapsmungkin ''f'', whilesementara ''b'' anddan ''c'' probably contain substantial amounts of [[Volatiles|ices]] and/ormengandung H/[[helium|He]].<ref name="Lissauer"/> The low densities likely result from large-volume extended atmospheres surrounding rocky/iron cores.<ref name="Naeye">{{Cite news | last=Naeye | first=Robert | title=Kepler's Outrageous System of Six Planets | work=Sky & Telescope | date=2 February 2011 | url=http://www.skyandtelescope.com/news/115102594.html | accessdate=4 February 2011}}{{Pranala mati|date=Februari 2021 |bot=InternetArchiveBot |fix-attempted=yes }}</ref>-->
 
{| class="toccolours sortable" border=1 cellspacing=0 cellpadding=2 align=center style="text-align:center; border-collapse:collapse; margin-left: 0; margin-right: auto;"
|- bgcolor="#a0b0ff"
! [[Planet]]
! [[Massa]]<br /><small>([[Massa Bumi|M<sub>E</sub>]])</small>
! [[Jari-jari]]<br /><small>([[Jari-jari Bumi|R<sub>E</sub>]])</small>
! [[Massa jenis]]<br /><small>(g/cm<sup>3</sup>)</small>
! [[Periode orbit]]<br /><small>([[hari]])</small>
! [[Aksis semimayor]]<br /><small>([[Satuan astronomi|AU]])</small>
! [[Eksentrisitas (orbit)|Eksentrisitas orbit.]]
! [[Inklinasi]]<br /><small>([[derajat (sudut)|°]])</small>
! Tahun<br />penemuan
|-
! [[de:Kepler-1111b|b]]
|| 4.3 (2.3 - 6.5) || 1.97 ± 0.19 || 3.1 (1.6 - 5.2) ||10.30375 || 0.091 || 0 || 88.5 || 2011<ref name="EPE2">{{cite web |title=Star : Kepler-11 |work=Extrasolar Planets Encyclopaedia |url=http://exoplanet.eu/star.php?st=Kepler-11#a_publi |accessdate=4 February 2011 |archive-date=2012-06-16 |archive-url=https://web.archive.org/web/20120616124459/http://exoplanet.eu/star.php?st=Kepler-11#a_publi |dead-url=yes }}</ref>
|-
! [[es:Kepler-1111c|c]]
|| 13.5 (7.4 - 18.3) || 3.15 ± 0.30 || 2.3 (1.2 - 3.6) ||13.02502 || 0.106 || 0 || 89 || 2011<ref name="EPE2"/>
|-
! [[fr:Kepler-1111d|d]]
|| 6.1 (4.4 - 9.2) || 3.43 ± 0.32 || 0.9 (0.6 - 1.4) ||22.68719 || 0.159 || 0 || 89.3 || 2011<ref name="EPE2"/>
|-
! [[it:Kepler-1111e|e]]
|| 8.4 (6.5 - 10.9) || 4.52 ± 0.43 || 0.5 (0.3 - 0.7) ||31.9959 || 0.194 || 0 || 88.8 || 2011<ref name="EPE2"/>
|-
! [[no:Kepler-1111f|f]]
|| 2.3 (1.1 - 4.5) || 2.61 ± 0.25 || 0.7 (0.3 - 1.4) ||46.68876 || 0.25 || 0 || 89.4 || 2011<ref name="EPE2"/>
|-
! [[pl:Kepler-1111g|g]]
|| < 300 (0.95 [[Jupiter mass|M<sub>J</sub>]]) || 3.66 ± 0.35 || ||118.37774 || 0.462 || 0 || 89.8 || 2011<ref name="EPE2"/>
|-
|colspan=10|[[Berkas:Kepler11 system sideview.png|640px]]<br />Posisi enam planet yang mengitari Kepler-11
|-
|colspan=10|[[Berkas:Kepler-11 sideview withsolarsystem.png|640px]]<br />Perbandingan dengan [[Tata Surya]]
|}
 
== Catatan kaki ==
{{reflist}}
 
== Pranala luar ==
Baris 41 ⟶ 80:
* [http://www.nasa.gov/mission_pages/kepler/news/new_planetary_system.html Official release: NASA's Kepler Spacecraft Discovers Extraordinary New Planetary System]
* [http://www.youtube.com/watch?v=c8Ipowj6X5s YouTube: Animation of Kepler-11 planetary system]
{{astronomibintang-stub}}
 
[[Kategori:Rasi bintang Cygnus]]
{{astronomi-stub}}
 
[[cs:Kepler 11]]
[[de:Kepler-11]]
[[es:Kepler-11]]
[[fa:کپلر-۱۱]]
[[fr:Kepler-11]]
[[ko:케플러-11]]
[[it:Kepler-11]]
[[he:קפלר-11]]
[[ja:ケプラー11]]
[[no:Kepler-11]]
[[pl:Kepler-11]]
[[pt:Kepler 11]]
[[ru:Kepler-11]]
[[sl:Kepler 11]]
[[ta:கெப்லர்-11]]
[[uk:Кеплер-11]]
[[zh:開普勒11]]