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Efek pertentangan - Riwayat revisi
2026-09-16T07:59:15Z
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Maintenance script: Presentation V4: sitasi, referensi, Math, Wikimedia Commons, dan atribusi
2026-08-26T09:20:11Z
<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 09.20</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 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;">[[File:Armstrong_heiligenschein.jpg|thumb|right|280px|Armstrong heiligenschein]]</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;"></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;"><div>'''Efek pertentangan''' (kadang-kadang dikenal juga sebagai '''efek Seeliger''') adalah suatu peristiwa ketika permukaan kasar atau objek terentu yang mengandung banyak [[partikel]] terlihat lebih terang, ketika permukaan kasar atau objek tersebut disinari di belakang para pengamat. Istilah ini paling banyak digunakan dalam [[astronomi]], secara umum merujuk pada peningkatan yang nyata dalam kecerahan [[benda langit]] seperti [[planet]], [[satelit alami|satelit]], atau [[komet]] saat sudut fase pengamatan mendekati nol. Dinamakan demikian karena cahaya yang dipantulkan dari [[Bulan]] dan [[Mars]] muncul secara signifikan lebih terang daripada yang diprediksi oleh [[reflektansi Lambert]] sederhana ketika berada di [[oposisi (astronomi)|oposisi astronomis]]. Dua mekanisme fisik telah diusulkan untuk fenomena pengamatan ini: persembunyian bayangan dan hamburan balik yang koheren.</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>'''Efek pertentangan''' (kadang-kadang dikenal juga sebagai '''efek Seeliger''') adalah suatu peristiwa ketika permukaan kasar atau objek terentu yang mengandung banyak [[partikel]] terlihat lebih terang, ketika permukaan kasar atau objek tersebut disinari di belakang para pengamat. Istilah ini paling banyak digunakan dalam [[astronomi]], secara umum merujuk pada peningkatan yang nyata dalam kecerahan [[benda langit]] seperti [[planet]], [[satelit alami|satelit]], atau [[komet]] saat sudut fase pengamatan mendekati nol. Dinamakan demikian karena cahaya yang dipantulkan dari [[Bulan]] dan [[Mars]] muncul secara signifikan lebih terang daripada yang diprediksi oleh [[reflektansi Lambert]] sederhana ketika berada di [[oposisi (astronomi)|oposisi astronomis]]. Dua mekanisme fisik telah diusulkan untuk fenomena pengamatan ini: persembunyian bayangan dan hamburan balik yang koheren.</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-lineno" id="mw-diff-left-l6">Baris 6:</td>
<td colspan="2" class="diff-lineno">Baris 8:</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>* [[Albedo geometrik]]</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>* [[Albedo geometrik]]</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;">Referensi </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;">Sumber dan atribusi </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><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" 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" 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;">* Hapke, B. [http://adsabs.harvard.edu/abs/1990Icar...88..407H Coherent Backscatter: An Explanation for the Unusual Radar Properties of Outer Planet Satellites] ''Icarus'' '''88''': 407:417.</del></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;">*</del></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;">* Gehrels, T. (1956) "[http://adsabs.harvard.edu/abs/1956ApJ...123..331G Photometric Studies of Asteroids. V: The Light-Curve and Phase Function of 20 Massalia]". ''Astrophysical Journal'' '''195''': 331-338.</del></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;">* Gehrels, T.; Coffeen, T.; & Owings, D. (1964) "[http://adsabs.harvard.edu/abs/1964AJ.....69..826G Wavelength dependence of polarization. III. The lunar surface]". ''Astron. J.'' '''69''': 826-852.</del></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;">* Burrati, B. J.; Hillier, J. K.; & Wang, M. (1996) "[http://adsabs.harvard.edu/abs/1996Icar..124..490B The Lunar Opposition Surge: Observations by Clementine]". ''Icarus'' '''124''': 490-499.</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;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Efek+pertentangan&oldid=22826438 Wikipedia bahasa Indonesia], revisi 22826438 (2023-02-01T13:26:52Z), yang tersedia berdasarkan lisensi Creative Commons Atribusi-BerbagiSerupa (CC BY-SA). Gambar pada artikel ini bersumber dari Wikimedia Commons dan 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> </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>
<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 dan atribusi ==</del></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> </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;">Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Efek+pertentangan&oldid=22826438 Wikipedia bahasa Indonesia], revisi 22826438 (2023</del>-<del style="font-weight: bold; text-decoration: none;">02</del>-<del style="font-weight: bold; text-decoration: none;">01T13:26:52Z), 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 colspan="2" class="diff-side-added"></td></tr>
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Maintenance script: Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 22826438; atribusi sumber disertakan.
2026-08-26T08:44:28Z
<p>Impor teks terkontrol dari Wikipedia bahasa Indonesia; revisi 22826438; atribusi sumber disertakan.</p>
<p><b>Halaman baru</b></p><div>'''Efek pertentangan''' (kadang-kadang dikenal juga sebagai '''efek Seeliger''') adalah suatu peristiwa ketika permukaan kasar atau objek terentu yang mengandung banyak [[partikel]] terlihat lebih terang, ketika permukaan kasar atau objek tersebut disinari di belakang para pengamat. Istilah ini paling banyak digunakan dalam [[astronomi]], secara umum merujuk pada peningkatan yang nyata dalam kecerahan [[benda langit]] seperti [[planet]], [[satelit alami|satelit]], atau [[komet]] saat sudut fase pengamatan mendekati nol. Dinamakan demikian karena cahaya yang dipantulkan dari [[Bulan]] dan [[Mars]] muncul secara signifikan lebih terang daripada yang diprediksi oleh [[reflektansi Lambert]] sederhana ketika berada di [[oposisi (astronomi)|oposisi astronomis]]. Dua mekanisme fisik telah diusulkan untuk fenomena pengamatan ini: persembunyian bayangan dan hamburan balik yang koheren.<br />
<br />
== Lihat pula ==<br />
* [[Albedo]]<br />
* [[Fenomena Brocken]]<br />
* [[Albedo geometrik]]<br />
<br />
== Referensi ==<br />
*<br />
*<br />
* Hapke, B. [http://adsabs.harvard.edu/abs/1990Icar...88..407H Coherent Backscatter: An Explanation for the Unusual Radar Properties of Outer Planet Satellites] ''Icarus'' '''88''': 407:417.<br />
*<br />
* Gehrels, T. (1956) "[http://adsabs.harvard.edu/abs/1956ApJ...123..331G Photometric Studies of Asteroids. V: The Light-Curve and Phase Function of 20 Massalia]". ''Astrophysical Journal'' '''195''': 331-338.<br />
* Gehrels, T.; Coffeen, T.; & Owings, D. (1964) "[http://adsabs.harvard.edu/abs/1964AJ.....69..826G Wavelength dependence of polarization. III. The lunar surface]". ''Astron. J.'' '''69''': 826-852.<br />
* Burrati, B. J.; Hillier, J. K.; & Wang, M. (1996) "[http://adsabs.harvard.edu/abs/1996Icar..124..490B The Lunar Opposition Surge: Observations by Clementine]". ''Icarus'' '''124''': 490-499.<br />
<br />
<br />
<br />
== Sumber dan atribusi ==<br />
<br />
Konten artikel ini diadaptasi dari [https://id.wikipedia.org/w/index.php?title=Efek+pertentangan&oldid=22826438 Wikipedia bahasa Indonesia], revisi 22826438 (2023-02-01T13:26:52Z), 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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