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Supergugus Shapley - Riwayat revisi
2026-09-16T07:35:46Z
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Maintenance script: Presentation V4: sitasi, referensi, Math, Wikimedia Commons, dan atribusi
2026-08-26T18:00:47Z
<p>Presentation V4: sitasi, referensi, Math, Wikimedia Commons, dan atribusi</p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Revisi sebelumnya</td>
<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revisi per 26 Agustus 2026 18.00</td>
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<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">'''Supergugus Shapley''' (</del>[[<del style="font-weight: bold; text-decoration: none;">Bahasa Inggris</del>|<del style="font-weight: bold; text-decoration: none;">Inggris]]: ''</del>Shapley Supercluster<del style="font-weight: bold; text-decoration: none;">; SSC'') juga dikenal sebagai '''konsentrasi Shapley''' ('''SCI 124'''), adalah [[supergugus]] yang berjarak sekitar 650 juta </del>- <del style="font-weight: bold; text-decoration: none;">1 miliar tahun cahaya ([[pergeseran merah</del>]] <del style="font-weight: bold; text-decoration: none;">z = 0,037 dan 0,053).</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>[[<ins style="font-weight: bold; text-decoration: none;">File:Galaxies_in_the_Shapley_Supercluster_-_Flickr_-_geckzilla.png|thumb</ins>|<ins style="font-weight: bold; text-decoration: none;">right|280px|Galaxies in the </ins>Shapley Supercluster - <ins style="font-weight: bold; text-decoration: none;">Flickr - geckzilla</ins>]]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Supergugus Shapley <del style="font-weight: bold; text-decoration: none;">pertama kali ditemukan oleh astronom Amerika </del>[[<del style="font-weight: bold; text-decoration: none;">Harlow Shapley</del>]] <del style="font-weight: bold; text-decoration: none;">pada tahun 1930-an, </del>sebagai konsentrasi <del style="font-weight: bold; text-decoration: none;">galaksi yang luar biasa di rasi bintang [[Sentaurus </del>(<del style="font-weight: bold; text-decoration: none;">rasi bintang</del>)<del style="font-weight: bold; text-decoration: none;">|Centaurus]] di area langit 12° x 6° (asensio kanan x </del>[<del style="font-weight: bold; text-decoration: none;">[deklinasi]</del>]<del style="font-weight: bold; text-decoration: none;">)</del>. <del style="font-weight: bold; text-decoration: none;">Memiliki lebih dari 8</del>.<del style="font-weight: bold; text-decoration: none;">000 galaksi dan dengan total massa lebih dari </del>10 <del style="font-weight: bold; text-decoration: none;">juta miliar kali massa Matahari, ini </del>adalah <del style="font-weight: bold; text-decoration: none;">struktur paling masif dalam jarak </del>sekitar <del style="font-weight: bold; text-decoration: none;">satu </del>miliar tahun cahaya <del style="font-weight: bold; text-decoration: none;">dan nerupakan konsentrasi galaksi terkaya yang diketahui di </del>[[<del style="font-weight: bold; text-decoration: none;">alam semesta lokal</del>]]<del style="font-weight: bold; text-decoration: none;">. Terdapat setidaknya 25 gugus dengan tujuh gugus adalah gugus kekayaan 2 atau lebih tinggi</del>, <del style="font-weight: bold; text-decoration: none;">(secara kasar</del>) <del style="font-weight: bold; text-decoration: none;">yang berarti ada tujuh gugus yang sekaya [[gugus Perseus]] atau [[Gugus Coma|Coma]]</del>.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">'''</ins>Supergugus Shapley<ins style="font-weight: bold; text-decoration: none;">''' (</ins>[[<ins style="font-weight: bold; text-decoration: none;">Bahasa Inggris|Inggris</ins>]]<ins style="font-weight: bold; text-decoration: none;">: ''Shapley Supercluster; SSC'') juga dikenal </ins>sebagai <ins style="font-weight: bold; text-decoration: none;">'''</ins>konsentrasi <ins style="font-weight: bold; text-decoration: none;">Shapley''' </ins>(<ins style="font-weight: bold; text-decoration: none;">'''SCI 124'''</ins>)<ins style="font-weight: bold; text-decoration: none;">,<ref></ins>[<ins style="font-weight: bold; text-decoration: none;">https://www.oxfordreference.com/view/10.1093/oi/authority.20110803100459556 Shapley supercluster</ins>]. <ins style="font-weight: bold; text-decoration: none;">''Oxford Reference''</ins>. <ins style="font-weight: bold; text-decoration: none;">doi:</ins>10<ins style="font-weight: bold; text-decoration: none;">.1093/oi/authority.20110803100459556.</ref> </ins>adalah <ins style="font-weight: bold; text-decoration: none;">[[supergugus]] yang berjarak </ins>sekitar <ins style="font-weight: bold; text-decoration: none;">650 juta - 1 </ins>miliar tahun cahaya <ins style="font-weight: bold; text-decoration: none;">(</ins>[[<ins style="font-weight: bold; text-decoration: none;">pergeseran merah</ins>]] <ins style="font-weight: bold; text-decoration: none;">z = 0,037 dan 0</ins>,<ins style="font-weight: bold; text-decoration: none;">053</ins>).</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Gugus pusat </del>Shapley <del style="font-weight: bold; text-decoration: none;">adalah </del>[[<del style="font-weight: bold; text-decoration: none;">Abell 3558|A3558</del>]] <del style="font-weight: bold; text-decoration: none;">dengan massa sekitar 500 ~ 7.63E14 </del>[[<del style="font-weight: bold; text-decoration: none;">massa matahari</del>]]<del style="font-weight: bold; text-decoration: none;">. Di sekitar pusat supergugus, terdapat lima gugus yang sedang berinteraksi sebagai struktur koheren tunggal, dengan filamen (panjang ~ 7 Mpc) yang memanjang ke Utara </del>([[<del style="font-weight: bold; text-decoration: none;">Abell 3558|A3558</del>]]) <del style="font-weight: bold; text-decoration: none;">dari Inti </del>(<del style="font-weight: bold; text-decoration: none;">z = 0,17</del>). <del style="font-weight: bold; text-decoration: none;">Sistem tersebut terikat secara gravitasi </del>dan dalam <del style="font-weight: bold; text-decoration: none;">proses runtuh. Supergugus memancarkan sinar-X </del>yang <del style="font-weight: bold; text-decoration: none;">sangat tinggi yang berasal dari gas intragugus tinggi </del>di <del style="font-weight: bold; text-decoration: none;">setiap gugus, </del>[[<del style="font-weight: bold; text-decoration: none;">supergugus Laniakea</del>]] <del style="font-weight: bold; text-decoration: none;">terlalu lemah</del>, <del style="font-weight: bold; text-decoration: none;">hanya </del>[[gugus <del style="font-weight: bold; text-decoration: none;">Centaurus</del>]] <del style="font-weight: bold; text-decoration: none;">di </del>[[<del style="font-weight: bold; text-decoration: none;">supergugus Hydra-Centaurus</del>]] <del style="font-weight: bold; text-decoration: none;">(</del>[<del style="font-weight: bold; text-decoration: none;">[Penarik Besar</del>]<del style="font-weight: bold; text-decoration: none;">]) yang (hanya) lebih bercahaya daripada gugus terlemah yang terdeteksi di Supergugus Shapley</del>. <del style="font-weight: bold; text-decoration: none;">Di wilayah tersebut terdapat </del>[<del style="font-weight: bold; text-decoration: none;">[aliran Hubble</del>]<del style="font-weight: bold; text-decoration: none;">] dan gugus bergabung dengan kecepatan tinggi</del>.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Supergugus </ins>Shapley <ins style="font-weight: bold; text-decoration: none;">pertama kali ditemukan oleh astronom Amerika </ins>[[<ins style="font-weight: bold; text-decoration: none;">Harlow Shapley</ins>]] <ins style="font-weight: bold; text-decoration: none;">pada tahun 1930-an, sebagai konsentrasi galaksi yang luar biasa di rasi bintang </ins>[[<ins style="font-weight: bold; text-decoration: none;">Sentaurus (rasi bintang)|Centaurus</ins>]] <ins style="font-weight: bold; text-decoration: none;">di area langit 12° x 6° </ins>(<ins style="font-weight: bold; text-decoration: none;">asensio kanan x </ins>[[<ins style="font-weight: bold; text-decoration: none;">deklinasi</ins>]])<ins style="font-weight: bold; text-decoration: none;">.<ref>H. Quintana. [http://dx.doi.org/10.1086/301476 The Shapley Supercluster. II. Spectroscopic Observations in a Wide Area and General Morphology]. ''The Astronomical Journal''. 2000-08. Vol. 120 </ins>(<ins style="font-weight: bold; text-decoration: none;">2</ins>). <ins style="font-weight: bold; text-decoration: none;">hlm. 511–522. doi:10.1086/301476.</ref> Memiliki lebih dari 8.000 galaksi </ins>dan <ins style="font-weight: bold; text-decoration: none;">dengan total massa lebih dari 10 juta miliar kali massa Matahari, ini adalah struktur paling masif </ins>dalam <ins style="font-weight: bold; text-decoration: none;">jarak sekitar satu miliar tahun cahaya dan nerupakan konsentrasi galaksi terkaya </ins>yang <ins style="font-weight: bold; text-decoration: none;">diketahui </ins>di [[<ins style="font-weight: bold; text-decoration: none;">alam semesta lokal</ins>]]<ins style="font-weight: bold; text-decoration: none;">.<ref>Jeffrey O. Breen. [http://dx.doi.org/10.1063/1.46689 ROSAT PSPC observations of the Shapley Supercluster]. ''AIP Conference Proceedings''. AIP. 1994. doi:10.1063/1.46689.</ref> Terdapat setidaknya 25 gugus dengan tujuh gugus adalah gugus kekayaan 2 atau lebih tinggi</ins>, <ins style="font-weight: bold; text-decoration: none;">(secara kasar) yang berarti ada tujuh gugus yang sekaya </ins>[[gugus <ins style="font-weight: bold; text-decoration: none;">Perseus</ins>]] <ins style="font-weight: bold; text-decoration: none;">atau </ins>[[<ins style="font-weight: bold; text-decoration: none;">Gugus Coma|Coma</ins>]]<ins style="font-weight: bold; text-decoration: none;">.<ref></ins>[<ins style="font-weight: bold; text-decoration: none;">http://www.atlasoftheuniverse.com/superc/shapley.html The Shapley Supercluster</ins>]. <ins style="font-weight: bold; text-decoration: none;">''www.atlasoftheuniverse.com''.</ref><ref></ins>[<ins style="font-weight: bold; text-decoration: none;">https://sci.esa.int/web/planck/-/57952-shapley-supercluster ESA Science & Technology - Shapley Supercluster</ins>]. <ins style="font-weight: bold; text-decoration: none;">''sci.esa.int''.</ref></ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Ada juga </del>struktur <del style="font-weight: bold; text-decoration: none;">penghubung yang terkait </del>dengan <del style="font-weight: bold; text-decoration: none;">kompleks gugus Abell </del>~ [[Abell <del style="font-weight: bold; text-decoration: none;">3571</del>|<del style="font-weight: bold; text-decoration: none;">3571</del>]] <del style="font-weight: bold; text-decoration: none;">yang sedikit lebih dekat </del>(<del style="font-weight: bold; text-decoration: none;">v ~ 12</del>.<del style="font-weight: bold; text-decoration: none;">000 km</del>/<del style="font-weight: bold; text-decoration: none;">s</del>). <del style="font-weight: bold; text-decoration: none;">Galaksi</del>-<del style="font-weight: bold; text-decoration: none;">galaksi ini tampaknya menghubungkan dua lembaran galaksi, dan cenderung mengisi celah galaksi antar latar Hydra</del>-<del style="font-weight: bold; text-decoration: none;">Centaurus dan SSC yang lebih jauh</del>. <del style="font-weight: bold; text-decoration: none;">SSC bergerak dengan kecepatan </del>(<del style="font-weight: bold; text-decoration: none;">9</del>.<del style="font-weight: bold; text-decoration: none;">000 km</del>/<del style="font-weight: bold; text-decoration: none;">s </del><<del style="font-weight: bold; text-decoration: none;">cz</del>< <del style="font-weight: bold; text-decoration: none;">18</del>.<del style="font-weight: bold; text-decoration: none;">000 km</del>/<del style="font-weight: bold; text-decoration: none;">s) dan ditemukan bahwa </del>[[<del style="font-weight: bold; text-decoration: none;">galaksi antargugus</del>]] <del style="font-weight: bold; text-decoration: none;">membentuk 48% galaksi</del>, yang <del style="font-weight: bold; text-decoration: none;">berkonstribusi hampir dua kali lipat massa </del>gugus.</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Gugus pusat Shapley adalah [[Abell 3558|A3558]] dengan massa sekitar 500 ~ 7.63E14 [[massa matahari]].<ref>P. Merluzzi. [http://dx.doi.org/10.1093/mnras/stu2085 Shapley Supercluster Survey: Galaxy evolution from filaments to cluster cores]. ''Monthly Notices of the Royal Astronomical Society''. 2014-11-13. Vol. 446 (1). hlm. 803–822. doi:10.1093/mnras/stu2085.</ref> Di sekitar pusat supergugus, terdapat lima gugus yang sedang berinteraksi sebagai </ins>struktur <ins style="font-weight: bold; text-decoration: none;">koheren tunggal, </ins>dengan <ins style="font-weight: bold; text-decoration: none;">filamen (panjang </ins>~ <ins style="font-weight: bold; text-decoration: none;">7 Mpc) yang memanjang ke Utara (</ins>[[Abell <ins style="font-weight: bold; text-decoration: none;">3558</ins>|<ins style="font-weight: bold; text-decoration: none;">A3558</ins>]]<ins style="font-weight: bold; text-decoration: none;">) dari Inti </ins>(<ins style="font-weight: bold; text-decoration: none;">z = 0,17).<ref>Yuchi Higuchi. [http://dx.doi.org/10</ins>.<ins style="font-weight: bold; text-decoration: none;">1093</ins>/<ins style="font-weight: bold; text-decoration: none;">mnras/staa1766 Shapley supercluster survey: mapping the dark matter distribution]. ''Monthly Notices of the Royal Astronomical Society''. 2020-06-19. Vol. 497 (1</ins>). <ins style="font-weight: bold; text-decoration: none;">hlm. 52–66. doi:10.1093/mnras/staa1766.</ref> Sistem tersebut terikat secara gravitasi dan dalam proses runtuh.<ref>C P Haines. [http://dx.doi.org/10.1093/mnras/sty2338 Shapley Supercluster Survey: mapping the filamentary network connecting the clusters]. ''Monthly Notices of the Royal Astronomical Society''. 2018</ins>-<ins style="font-weight: bold; text-decoration: none;">08</ins>-<ins style="font-weight: bold; text-decoration: none;">25. Vol</ins>. <ins style="font-weight: bold; text-decoration: none;">481 </ins>(<ins style="font-weight: bold; text-decoration: none;">1). hlm. 1055–1074. doi:10</ins>.<ins style="font-weight: bold; text-decoration: none;">1093</ins>/<ins style="font-weight: bold; text-decoration: none;">mnras/sty2338.</ins><<ins style="font-weight: bold; text-decoration: none;">/ref> Supergugus memancarkan sinar-X yang sangat tinggi yang berasal dari gas intragugus tinggi di setiap gugus,</ins><<ins style="font-weight: bold; text-decoration: none;">ref>Jeffrey O. Breen. [http://dx.doi</ins>.<ins style="font-weight: bold; text-decoration: none;">org</ins>/<ins style="font-weight: bold; text-decoration: none;">10.1063/1.46689 ROSAT PSPC observations of the Shapley Supercluster]. ''AIP Conference Proceedings''. AIP. 1994. doi:10.1063/1.46689.</ref> </ins>[[<ins style="font-weight: bold; text-decoration: none;">supergugus Laniakea</ins>]] <ins style="font-weight: bold; text-decoration: none;">terlalu lemah</ins>, <ins style="font-weight: bold; text-decoration: none;">hanya [[gugus Centaurus]] di [[supergugus Hydra-Centaurus]] ([[Penarik Besar]]) yang (hanya) lebih bercahaya daripada gugus terlemah </ins>yang <ins style="font-weight: bold; text-decoration: none;">terdeteksi di Supergugus Shapley. Di wilayah tersebut terdapat [[aliran Hubble]] dan </ins>gugus <ins style="font-weight: bold; text-decoration: none;">bergabung dengan kecepatan tinggi.<ref>Somak Raychaudhury. [http://dx</ins>.<ins style="font-weight: bold; text-decoration: none;">doi.org/10.1093/mnras/248.1.101 X-ray and optical observations of the Shapley supercluster in Hydra–Centaurus]. ''Monthly Notices of the Royal Astronomical Society''. 1991-01. Vol. 248 (1). hlm. 101–111. doi:10.1093/mnras/248.1.101.</ref></ins></div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div> </div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">== Referensi ==</del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Ada juga struktur penghubung yang terkait dengan kompleks gugus Abell ~ [[Abell 3571|3571]] yang sedikit lebih dekat (v ~ 12.000 km/s). Galaksi-galaksi ini tampaknya menghubungkan dua lembaran galaksi, dan cenderung mengisi celah galaksi antar latar Hydra-Centaurus dan SSC yang lebih jauh. SSC bergerak dengan kecepatan (9.000 km/s <cz< 18.000 km/s) dan ditemukan bahwa [[galaksi antargugus]] membentuk 48% galaksi, yang berkonstribusi hampir dua kali lipat massa gugus.<ref>Dominique Proust. [http://dx.doi.org/10.1017/s1743921304000225 Structure and dynamics of the Shapley supercluster]. ''Proceedings of the International Astronomical Union''. 2004-03. Vol. 2004 (IAUC195). doi:10.1017/s1743921304000225.</ref></ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Lihat pula ==</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>== Lihat pula ==</div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2" class="diff-side-added"></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Gugus Norma]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Gugus Norma]]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Supergugus]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Supergugus]]</div></td></tr>
<tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l20">Baris 20:</td>
<td colspan="2" class="diff-lineno">Baris 18:</td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Void (astronomi)]]</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[Void (astronomi)]]</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">== Referensi ==</ins></div></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"><references /></ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">== Sumber dan atribusi ==</ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>== <del style="font-weight: bold; text-decoration: none;">Sumber </del>dan <del style="font-weight: bold; text-decoration: none;">atribusi ==</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title</ins>=<ins style="font-weight: bold; text-decoration: none;">Supergugus+Shapley&oldid</ins>=<ins style="font-weight: bold; text-decoration: none;">28884893 Wikipedia bahasa Indonesia], revisi 28884893 (2026-01-23T15:46:32Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Gambar pada artikel ini bersumber dari Wikimedia Commons </ins>dan <ins style="font-weight: bold; text-decoration: none;">mengikuti ketentuan lisensi masing-masing berkas. Mohon gunakan konten dan media secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</ins></div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Supergugus+Shapley&oldid=28884893 Wikipedia bahasa Indonesia], revisi 28884893 (2026</del>-<del style="font-weight: bold; text-decoration: none;">01</del>-<del style="font-weight: bold; text-decoration: none;">23T15:46:32Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi</del>-<del style="font-weight: bold; text-decoration: none;">BerbagiSerupa (CC BY</del>-<del style="font-weight: bold; text-decoration: none;">SA). Mohon gunakan konten ini secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;"><!</ins>-- <ins style="font-weight: bold; text-decoration: none;">WIKI_UNISSULA_PRESENTATION_V4 </ins>--<ins style="font-weight: bold; text-decoration: none;">></ins></div></td></tr>
</table>
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https://wiki.unissula.ac.id/index.php?title=Supergugus_Shapley&diff=14966&oldid=prev
Maintenance script: Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 28884893; atribusi sumber disertakan.
2026-08-26T17:20:01Z
<p>Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 28884893; atribusi sumber disertakan.</p>
<p><b>Halaman baru</b></p><div>'''Supergugus Shapley''' ([[Bahasa Inggris|Inggris]]: ''Shapley Supercluster; SSC'') juga dikenal sebagai '''konsentrasi Shapley''' ('''SCI 124'''), adalah [[supergugus]] yang berjarak sekitar 650 juta - 1 miliar tahun cahaya ([[pergeseran merah]] z = 0,037 dan 0,053).<br />
<br />
Supergugus Shapley pertama kali ditemukan oleh astronom Amerika [[Harlow Shapley]] pada tahun 1930-an, sebagai konsentrasi galaksi yang luar biasa di rasi bintang [[Sentaurus (rasi bintang)|Centaurus]] di area langit 12° x 6° (asensio kanan x [[deklinasi]]). Memiliki lebih dari 8.000 galaksi dan dengan total massa lebih dari 10 juta miliar kali massa Matahari, ini adalah struktur paling masif dalam jarak sekitar satu miliar tahun cahaya dan nerupakan konsentrasi galaksi terkaya yang diketahui di [[alam semesta lokal]]. Terdapat setidaknya 25 gugus dengan tujuh gugus adalah gugus kekayaan 2 atau lebih tinggi, (secara kasar) yang berarti ada tujuh gugus yang sekaya [[gugus Perseus]] atau [[Gugus Coma|Coma]].<br />
<br />
Gugus pusat Shapley adalah [[Abell 3558|A3558]] dengan massa sekitar 500 ~ 7.63E14 [[massa matahari]]. Di sekitar pusat supergugus, terdapat lima gugus yang sedang berinteraksi sebagai struktur koheren tunggal, dengan filamen (panjang ~ 7 Mpc) yang memanjang ke Utara ([[Abell 3558|A3558]]) dari Inti (z = 0,17). Sistem tersebut terikat secara gravitasi dan dalam proses runtuh. Supergugus memancarkan sinar-X yang sangat tinggi yang berasal dari gas intragugus tinggi di setiap gugus, [[supergugus Laniakea]] terlalu lemah, hanya [[gugus Centaurus]] di [[supergugus Hydra-Centaurus]] ([[Penarik Besar]]) yang (hanya) lebih bercahaya daripada gugus terlemah yang terdeteksi di Supergugus Shapley. Di wilayah tersebut terdapat [[aliran Hubble]] dan gugus bergabung dengan kecepatan tinggi.<br />
<br />
Ada juga struktur penghubung yang terkait dengan kompleks gugus Abell ~ [[Abell 3571|3571]] yang sedikit lebih dekat (v ~ 12.000 km/s). Galaksi-galaksi ini tampaknya menghubungkan dua lembaran galaksi, dan cenderung mengisi celah galaksi antar latar Hydra-Centaurus dan SSC yang lebih jauh. SSC bergerak dengan kecepatan (9.000 km/s <cz< 18.000 km/s) dan ditemukan bahwa [[galaksi antargugus]] membentuk 48% galaksi, yang berkonstribusi hampir dua kali lipat massa gugus.<br />
<br />
== Referensi ==<br />
<br />
<br />
== Lihat pula ==<br />
<br />
* [[Gugus Norma]]<br />
* [[Supergugus]]<br />
* [[Aliran gelap]]<br />
* [[Penarik Besar]]<br />
* [[Supergugus Hydra-Centaurus]]<br />
* [[Struktur berskala besar]]<br />
* [[Void (astronomi)]]<br />
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<br />
<br />
== Sumber dan atribusi ==<br />
<br />
Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Supergugus+Shapley&oldid=28884893 Wikipedia bahasa Indonesia], revisi 28884893 (2026-01-23T15:46:32Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Mohon gunakan konten ini secara bijak serta sesuai dengan ketentuan lisensi yang berlaku.</div>
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