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WASP-11/HAT-P-10 - Riwayat revisi
2026-09-15T22:41:44Z
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2026-08-27T14:05:20Z
<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 27 Agustus 2026 14.05</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>'''WASP-11/HAT-P-10''' adalah bintang biner. ''WASP-11/HAT-P-10'' adalah bintang katai oranye urutan utama. Sekunder ''WASP-11/HAT-P-10'' adalah tipe katai M dengan suhu 3494 ± 37 [[Kelvin|K]] dan diproyeksikan pemisahan 42 [[Satuan astronomi|SA]]. WASP-11/HAT-P-10 terletak sekitar 408 tahun cahaya dari [[Bumi]] <del style="font-weight: bold; text-decoration: none;"> </del>di rasi bintang [[Aries (constellation)|Aries]].</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>'''WASP-11/HAT-P-10''' adalah bintang biner. ''WASP-11/HAT-P-10'' adalah bintang katai oranye urutan utama. Sekunder ''WASP-11/HAT-P-10'' adalah tipe katai M dengan suhu 3494 ± 37 [[Kelvin|K]] dan diproyeksikan pemisahan 42 [[Satuan astronomi|SA]].<ins style="font-weight: bold; text-decoration: none;"><ref>''FRIENDS OF HOT JUPITERS III:AN INFRARED SPECTROSCOPIC SEARCH FOR LOW-MASS STELLAR COMPANIONS''. 2015.</ref> </ins>WASP-11/HAT-P-10 terletak sekitar 408 tahun cahaya dari [[Bumi]] <ins style="font-weight: bold; text-decoration: none;"><ref>[https://id.wikipedia.org/w/index.php?title=WASP-11%2FHAT-P-10&oldid=18073813 sumber pada Wikipedia bahasa Indonesia]</ref> </ins>di rasi bintang [[Aries (constellation)|Aries]].<ins style="font-weight: bold; text-decoration: none;"><ref>[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GSC02340-01714 SIMBAD query result: NAME HAT P-10 -- Star]. Centre de Données astronomiques de Strasbourg.</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 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;"><ref>M Mayor. ''The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets''. 2011.</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>== Referensi ==</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>== Referensi ==</div></td></tr>
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<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>== Sumber dan atribusi ==</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>== Sumber dan atribusi ==</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>Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=WASP-11%2FHAT-P-10&oldid=18073813 Wikipedia bahasa Indonesia], revisi 18073813 (2021-03-05T01:12:13Z), 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></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>Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=WASP-11%2FHAT-P-10&oldid=18073813 Wikipedia bahasa Indonesia], revisi 18073813 (2021-03-05T01:12:13Z), 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></td></tr>
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2026-08-27T13:34:03Z
<p>Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 18073813; atribusi sumber disertakan.</p>
<p><b>Halaman baru</b></p><div>'''WASP-11/HAT-P-10''' adalah bintang biner. ''WASP-11/HAT-P-10'' adalah bintang katai oranye urutan utama. Sekunder ''WASP-11/HAT-P-10'' adalah tipe katai M dengan suhu 3494 ± 37 [[Kelvin|K]] dan diproyeksikan pemisahan 42 [[Satuan astronomi|SA]]. WASP-11/HAT-P-10 terletak sekitar 408 tahun cahaya dari [[Bumi]] di rasi bintang [[Aries (constellation)|Aries]].<br />
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== Referensi ==<br />
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== Sumber dan atribusi ==<br />
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Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=WASP-11%2FHAT-P-10&oldid=18073813 Wikipedia bahasa Indonesia], revisi 18073813 (2021-03-05T01:12:13Z), 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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