https://wiki.unissula.ac.id/index.php?action=history&feed=atom&title=Bentuk_alam_semesta 2026-09-16T04:44:46Z Riwayat revisi halaman ini di wiki MediaWiki 1.46.0 https://wiki.unissula.ac.id/index.php?title=Bentuk_alam_semesta&diff=13902&oldid=prev 2026-08-26T09:12:05Z

<p>Presentation V4: sitasi, referensi, Math, Wikimedia Commons, dan atribusi</p> <table style="background-color: #fff; color: #202122;" data-mw-interface=""> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="id"> <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 09.12</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1">Baris 1:</td> <td colspan="2" class="diff-lineno">Baris 1:</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;">'''Bentuk alam semesta''' adalah salah satu pokok pembahasan dalam </del>[[<del style="font-weight: bold; text-decoration: none;">kosmologi fisik]]</del>. <del style="font-weight: bold; text-decoration: none;">Berdasarkan pengukuran yang dilakukan oleh [[Wilkinson Microwave Anisotropy Probe]] (</del>WMAP<del style="font-weight: bold; text-decoration: none;">), [[NASA</del>]] <del style="font-weight: bold; text-decoration: none;">menyatakan bahwa "Kita tahu alam semesta itu datar dengan batas kesalahan 0,4%." Dalam [[metrik Friedmann–Lemaître–Robertson–Walker|model Friedmann–Lemaître–Robertson–Walker]] (FLRW), bentuk alam semesta yang dianggap sesuai dengan data pengamatan adalah bentuk yang datar dan tak terbatas, sementara model FLRW lain yang cocok dengan data meliputi [[ruang dodekahedral Poincaré]] dan [[tanduk Picard]].</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:WMAP_2012</ins>.<ins style="font-weight: bold; text-decoration: none;">png|thumb|right|280px|</ins>WMAP <ins style="font-weight: bold; text-decoration: none;">2012</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;">== Catatan kaki ==</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;">'''Bentuk alam semesta''' adalah salah satu pokok pembahasan dalam [[kosmologi fisik]]. Berdasarkan pengukuran yang dilakukan oleh [[Wilkinson Microwave Anisotropy Probe]] (WMAP), [[NASA]] menyatakan bahwa "Kita tahu alam semesta itu datar dengan batas kesalahan 0,4%."&lt;ref&gt;http://map.gsfc.nasa.gov/universe/uni_shape.html&lt;/ref&gt; Dalam [[metrik Friedmann–Lemaître–Robertson–Walker|model Friedmann–Lemaître–Robertson–Walker]] (FLRW), bentuk alam semesta yang dianggap sesuai dengan data pengamatan adalah bentuk yang datar dan tak terbatas,&lt;ref&gt;Marek Demianski. [http://books.google.com/books?id=KhTJZG-U3ssC Topology of the universe and the cosmic microwave background radiation]. ''The Early Universe and the Cosmic Microwave Background: Theory and Observations. Proceedings of the NATO Advanced Study Institute''. Springer. 2003. Vol. 130. hlm. 161. ISBN 1-4020-1800-2., [http://books.google.com/books?id=KhTJZG-U3ssC&amp;pg=PA161 Extract of page 161]&lt;/ref&gt; sementara model FLRW lain yang cocok dengan data meliputi [[ruang dodekahedral Poincaré]]&lt;ref&gt;Jean-Pierre Luminet. ''Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background''. ''Nature''. 2003-10-09. Vol. 425 (6958). hlm. 593–5. doi:10.1038/nature01944.&lt;/ref&gt;&lt;ref&gt;Boudewijn Roukema. ''A test of the Poincare dodecahedral space topology hypothesis with the WMAP CMB data''. ''Astronomy and Astrophysics''. 2008. Vol. 482 (3). hlm. 747. doi:10.1051/0004-6361:20078777.&lt;/ref&gt; dan [[tanduk Picard]].&lt;ref&gt;Ralf Aurich. ''Hyperbolic Universes with a Horned Topology and the CMB Anisotropy''. ''Classical and Quantum Gravity''. 2004. Vol. 21 (21). hlm. 4901–4926. doi:10.1088/0264-9381/21/21/010.&lt;/ref&gt;</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>== Pranala luar ==</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>== Pranala luar ==</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>* [http://icosmos.co.uk Geometry of the Universe]</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>* [http://icosmos.co.uk Geometry of the Universe]  </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>* [http://physicsworld.com/cws/article/print/23009 A cosmic hall of mirrors]  – physicsworld (26 September 2005)</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>* [http://physicsworld.com/cws/article/print/23009 A cosmic hall of mirrors]  – physicsworld (26 September 2005)</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>* [http://news.nationalgeographic.com/news/2003/10/1008_031008_finiteuniverse.html Universe is Finite, &quot;Soccer Ball&quot;-Shaped, Study Hints.] Possible wrap-around dodecahedral shape of the universe</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>* [http://news.nationalgeographic.com/news/2003/10/1008_031008_finiteuniverse.html Universe is Finite, &quot;Soccer Ball&quot;-Shaped, Study Hints.] Possible wrap-around dodecahedral shape of the universe</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 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>*  </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>* Classification of [http://star-www.st-and.ac.uk/~kdh1/cos/cos.html possible universes] in the [[Lambda-CDM]] model.</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>* Classification of [http://star-www.st-and.ac.uk/~kdh1/cos/cos.html possible universes] in the [[Lambda-CDM]] model.</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>* [http://www.scielo.br/scielo.php?script=sci_arttext&amp;pid=S0103-97332002000500012&amp;lng=en&amp;nrm=iso Closed hyperbolic universe].</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>* [http://www.scielo.br/scielo.php?script=sci_arttext&amp;pid=S0103-97332002000500012&amp;lng=en&amp;nrm=iso Closed hyperbolic universe].</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>*</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>*</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;">&lt;references /&gt;</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;">Bentuk+alam+semesta&amp;oldid</ins>=<ins style="font-weight: bold; text-decoration: none;">20953259 Wikipedia bahasa Indonesia], revisi 20953259 (2022-04-09T01:10:19Z), 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=Bentuk+alam+semesta&amp;oldid=20953259 Wikipedia bahasa Indonesia], revisi 20953259 (2022</del>-<del style="font-weight: bold; text-decoration: none;">04</del>-<del style="font-weight: bold; text-decoration: none;">09T01:10:19Z), 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;">&lt;!</ins>-- <ins style="font-weight: bold; text-decoration: none;">WIKI_UNISSULA_PRESENTATION_V4 </ins>--<ins style="font-weight: bold; text-decoration: none;">&gt;</ins></div></td></tr> </table>

Maintenance script https://wiki.unissula.ac.id/index.php?title=Bentuk_alam_semesta&diff=13501&oldid=prev 2026-08-26T08:34:22Z

<p>Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 20953259; atribusi sumber disertakan.</p> <p><b>Halaman baru</b></p><div>&#039;&#039;&#039;Bentuk alam semesta&#039;&#039;&#039; adalah salah satu pokok pembahasan dalam [[kosmologi fisik]]. Berdasarkan pengukuran yang dilakukan oleh [[Wilkinson Microwave Anisotropy Probe]] (WMAP), [[NASA]] menyatakan bahwa &quot;Kita tahu alam semesta itu datar dengan batas kesalahan 0,4%.&quot; Dalam [[metrik Friedmann–Lemaître–Robertson–Walker|model Friedmann–Lemaître–Robertson–Walker]] (FLRW), bentuk alam semesta yang dianggap sesuai dengan data pengamatan adalah bentuk yang datar dan tak terbatas, sementara model FLRW lain yang cocok dengan data meliputi [[ruang dodekahedral Poincaré]] dan [[tanduk Picard]].<br /> <br /> == Catatan kaki ==<br /> <br /> <br /> == Pranala luar ==<br /> * [http://icosmos.co.uk Geometry of the Universe]<br /> * [http://physicsworld.com/cws/article/print/23009 A cosmic hall of mirrors] – physicsworld (26 September 2005)<br /> * [http://news.nationalgeographic.com/news/2003/10/1008_031008_finiteuniverse.html Universe is Finite, &quot;Soccer Ball&quot;-Shaped, Study Hints.] Possible wrap-around dodecahedral shape of the universe<br /> *<br /> * Classification of [http://star-www.st-and.ac.uk/~kdh1/cos/cos.html possible universes] in the [[Lambda-CDM]] model.<br /> * [http://www.scielo.br/scielo.php?script=sci_arttext&amp;pid=S0103-97332002000500012&amp;lng=en&amp;nrm=iso Closed hyperbolic universe].<br /> *<br /> <br /> <br /> <br /> == Sumber dan atribusi ==<br /> <br /> Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Bentuk+alam+semesta&amp;oldid=20953259 Wikipedia bahasa Indonesia], revisi 20953259 (2022-04-09T01:10:19Z), 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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