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<p><b>天囷增十五</b>，即<b>金牛座10</b>（10 Tauri），是一顆位於<a href="./%E9%87%91%E7%89%9B%E5%BA%A7" title="金牛座">金牛座</a>的<a href="./%E6%81%92%E6%98%9F" title="恆星">恆星</a>，它距離地球約45<a href="./%E5%85%89%E5%B9%B4" title="光年">光年</a>，<a href="./%E8%A7%86%E6%98%9F%E7%AD%89" title="視星等">視星等</a>為+4.28。
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<div class="pcs-collapse-table-collapsed-container pcs-collapse-table-expanded" style="display: block;"><strong class="pcs-table-infobox">快速預覽</strong><span class="pcs-collapse-table-collapse-text"> 觀測資料 曆元 J2000, 特性 ...</span><span class="pcs-collapse-table-aria" aria-labelledby="pcs-collapse-table-aria-expand" role="button" display="none"><span id="pcs-collapse-table-aria-expand" aria-label="展開表格"></span><span id="pcs-collapse-table-aria-collapse" aria-label="折疊表格"></span></span></div>
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<caption style="margin-left: inherit;"><b>天囷增十五（金牛座10） <br> 10 Tauri</b>
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<th style="background-color: #FFFFC0;" colspan="2" class="notheme">觀測資料<br><span style="font-size: small;"><a href="./%E6%9B%86%E5%85%83" title="曆元">曆元</a> J2000</span>
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<td><b><a href="./%E6%98%9F%E5%BA%A7" title="星座">星座</a></b>
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<td><a href="./%E9%87%91%E7%89%9B%E5%BA%A7" title="金牛座">金牛座</a>
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<td><b><a href="./%E6%98%9F%E5%AE%98" title="星官">星官</a></b>
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<td><a href="./%E8%83%83%E5%AE%BF" title="胃宿">胃宿</a> <a href="./%E5%A4%A9%E5%9B%B7" title="天囷">天囷</a>
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<td><b><a href="./%E8%B5%A4%E7%B6%93" class="mw-redirect" title="赤經">赤經</a></b>
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<td>03<sup>h</sup> 36<sup>m</sup> 52.38<sup>s</sup></td>
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<td><b><a href="./%E8%B5%A4%E7%B7%AF" class="mw-redirect" title="赤緯">赤緯</a></b>
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<td>+00° 24′ 06.0″
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<td><b><a href="./%E8%A6%96%E6%98%9F%E7%AD%89" class="mw-redirect" title="視星等">視星等</a><small>（V）</small></b>
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<td>4.28
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<th style="background-color: #FFFFC0; text-align: center;" colspan="2" class="notheme">特性</th>
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<td><b><a href="./%E6%81%92%E6%98%9F%E5%85%89%E8%B0%B1%E5%88%86%E7%B1%BB" class="mw-redirect" title="恆星光譜分類">光譜分類</a></b></td>
<td>F9 IV-V</td>
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<td><b>U−B <a href="./%E8%89%B2%E6%8C%87%E6%95%B0" class="mw-redirect" title="色指數">色指數</a></b></td>
<td>0.07</td>
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<td><b>B−V <a href="./%E8%89%B2%E6%8C%87%E6%95%B0" class="mw-redirect" title="色指數">色指數</a></b></td>
<td>0.57</td>
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<td><b><a href="./%E5%8F%98%E6%98%9F" class="mw-redirect" title="變星">變星類型</a></b></td>
<td>否</td>
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<th style="background-color: #FFFFC0; text-align: center;" colspan="2" class="notheme"><a href="./%E5%A4%A9%E4%BD%93%E6%B5%8B%E9%87%8F%E5%AD%A6" title="天體測量學">天體測定</a></th>
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<td><b><a href="./%E5%BE%91%E5%90%91%E9%80%9F%E5%BA%A6" title="徑向速度">徑向速度</a> <small>(R<sub>v</sub>)</small></b></td>
<td>+27.6 km/s</td>
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<td><b><a href="./%E8%87%AA%E8%A1%8C" title="自行">自行</a> <small>(μ)</small></b></td>
<td> 赤經：-232.60 ± 0.59 <sup id="cite_ref-hipparcos_1-0" class="reference"><a href="#cite_note-hipparcos-1" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[1]</a></sup> <a href="./%E6%AF%AB%E8%A7%92%E7%A7%92" class="mw-redirect" title="毫角秒">mas</a>/<a href="./%E5%B9%B4" title="年">yr</a> <br> 赤緯：-481.92 ± 0.54 <sup id="cite_ref-hipparcos_1-1" class="reference"><a href="#cite_note-hipparcos-1" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[1]</a></sup> <a href="./%E6%AF%AB%E8%A7%92%E7%A7%92" class="mw-redirect" title="毫角秒">mas</a>/<a href="./%E5%B9%B4" title="年">yr</a> </td>
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<td><b><a href="./%E8%A7%86%E5%B7%AE" title="視差">視差</a> <small>(π)</small></b></td>
<td>71.62 ± 0.54<sup id="cite_ref-hipparcos_1-2" class="reference"><a href="#cite_note-hipparcos-1" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[1]</a></sup> <a href="./%E6%AF%AB%E8%A7%92%E7%A7%92" class="mw-redirect" title="毫角秒">mas</a></td>
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<td><b><a href="./%E5%AE%87%E5%AE%99%E8%B7%9D%E7%A6%BB%E5%B0%BA%E5%BA%A6" title="宇宙距離尺度">距離</a></b></td>
<td>45.5 ± 0.3 <a href="./%E5%85%89%E5%B9%B4" title="光年">ly</a> <br>(14 ± 0.1 <a href="./%E7%A7%92%E5%B7%AE%E8%B7%9D" title="秒差距">pc</a>)</td>
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<td><b><a href="./%E7%BB%9D%E5%AF%B9%E6%98%9F%E7%AD%89" class="mw-redirect" title="絕對星等">絕對星等</a> <small>(M<sub>V</sub>)</small></b></td>
<td>3.59</td>
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<th colspan="2" style="text-align: center"></th>
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<th style="background-color: #FFFFC0;" colspan="2" class="notheme">詳細資料 <sup></sup></th>
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<td><b><a href="./%E8%B3%AA%E9%87%8F" class="mw-redirect" title="質量">質量</a></b></td>
<td>1.6 <a href="./%E5%A4%AA%E9%98%B3%E8%B4%A8%E9%87%8F" title="太陽質量"><i>M</i><sub>☉</sub></a></td>
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<td><b><a href="./%E5%8D%8A%E5%BE%91" class="mw-redirect" title="半徑">半徑</a></b></td>
<td>1.6 <a href="./%E5%A4%AA%E9%98%B3%E5%8D%8A%E5%BE%84" title="太陽半徑"><i>R</i><sub>☉</sub></a></td>
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<td><b><a href="./%E4%BA%AE%E5%BA%A6" title="亮度">亮度</a></b></td>
<td>3 <a href="./%E5%A4%AA%E9%99%BD%E5%85%89%E5%BA%A6" title="太陽光度"><i>L</i><sub>☉</sub></a></td>
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<td><b><a href="./%E6%BA%AB%E5%BA%A6" class="mw-redirect" title="溫度">溫度</a></b></td>
<td>6037 ± 3.6 <sup id="cite_ref-2" class="reference"><a href="#cite_note-2" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[2]</a></sup> <a href="./%E7%86%B1%E5%8A%9B%E5%AD%B8%E6%BA%AB%E6%A8%99" class="mw-redirect" title="熱力學溫標">K</a></td>
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<td><b><a href="./%E9%87%91%E5%B1%AC%E9%87%8F" title="金屬量">金屬量</a></b></td>
<td>63–120 % Sun</td>
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<td><b><a href="./%E6%81%92%E6%98%9F#
%E5%B9%B4%E9%BD%A1年齡" title="恆星">年齡</a></b></td>
<td><span class="nowrap">4–8 × 10<sup>8</sup></span><sup id="cite_ref-apj687_3-0" class="reference"><a href="#cite_note-apj687-3" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[3]</a></sup> <a href="./%E5%B9%B4" title="年">年</a></td>
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<th style="background-color: #D3D3D3;" colspan="2" class="notheme"><a href="./%E6%98%9F%E8%A1%A8" title="星表">其他命名</a>
</th>
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<td colspan="2">
<div style="width: 250px;"> <a href="./Gliese-Jahreiss_catalogue" class="mw-redirect" title="Gliese-Jahreiss catalogue">GJ</a> 147, <a href="./Harvard_Revised_catalogue" class="mw-redirect" title="Harvard Revised catalogue">HR</a> 1101, <a href="./Bonner_Durchmusterung" class="mw-redirect" title="Bonner Durchmusterung">BD</a> -00°572, <a href="./Henry_Draper_catalogue" class="mw-redirect" title="Henry Draper catalogue">HD</a> 22484, <a href="./Luyten_Half-Second_catalogue" class="mw-redirect" title="Luyten Half-Second catalogue">LHS</a> 1569, <a href="./Luyten_Two-Tenths_catalogue" class="mw-redirect" title="Luyten Two-Tenths catalogue">LTT</a> 11194, <a href="./General_Catalogue_of_Trigonometric_Parallaxes" class="mw-redirect" title="General Catalogue of Trigonometric Parallaxes">GCTP</a> 753.00, <a href="./Smithsonian_Astrophysical_Observatory_Star_Catalog" class="mw-redirect" title="Smithsonian Astrophysical Observatory Star Catalog">SAO</a> 111292, <span class="new">FK5</span> 1101, <a href="./Hipparcos_catalogue" class="mw-redirect" title="Hipparcos catalogue">HIP</a> 16852. </div>
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<div class="pcs-collapse-table-collapsed-bottom pcs-collapse-table-icon" style="display: none;">關閉</div>
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<p>天囷增十五是質量和亮度比<a href="./%E5%A4%AA%E9%98%B3" title="太陽">太陽</a>稍大，年齡和太陽差不多或稍老。<a href="./%E6%81%92%E6%98%9F%E5%85%89%E8%B0%B1" title="恆星光譜">光譜分型</a>顯示它介於<a href="./%E7%9F%AE%E6%98%9F" class="mw-redirect" title="矮星">矮星</a>和<a href="./%E6%AC%A1%E5%B7%A8%E6%98%9F" title="次巨星">次巨星</a>之間，因此它可能是充分進化的恆星，已經接近<a href="./%E4%B8%BB%E5%BA%8F%E6%98%9F" title="主序星">主序星</a>階段的末期。天囷增十五可能是一顆分光雙星，但現在沒有被確認。從望遠鏡上觀測這顆恆星時，可以看到一個在同一視線中的伴星。
</p>
<p>通過IRAS/ISO的紅外輻射探測，已經確定在天囷增十五周圍有一個岩質圓盤<sup id="cite_ref-4" class="reference"><a href="#cite_note-4" class="reference-link" style="margin: -4px -16px -16px -16px; padding: 4px 16px 16px 16px;">[4]</a></sup>。
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参考资料.E5.8F.82.E8.80.83.E8.B5.84.E6.96.99" class="pcs-edit-section-title">參考資料</h
26><span class="pcs-edit-section-link-container"><a href="/w/index.php?title=天囷增十五&action=edit&section=1" data-id="1" data-action="edit_section" aria-labelledby="pcs-edit-section-aria-normal" class="pcs-edit-section-link"></a></span>
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<h2><span class="mw-headline" id="参考资料">參考資料</span></h2>
<div class="reflist" style="list-style-type: decimal;">
<div class="mw-references-wrap" about="#mwt_present">
<ol class="references mw-references">
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<div class="pcs-ref">
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<div class="pcs-ref-body"><span class="reference-text"><cite class="citation web">van Leeuwen, F. <a rel="nofollow" class="external text" href="http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=16810">HIP 16852</a>. Hipparcos, the New Reduction. 2007 <span class="reference-accessdate"> [<span class="nowrap">2009-12-15</span>]</span>. （原始內容<a rel="nofollow" class="external text" href="//web.archive.org/web/20160303174943/http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I%2F311%2Fhip2&recno=16810">存檔</a>於2016-03-03）.</cite></span></div>
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<div class="pcs-ref-body"><span class="reference-text"><cite class="citation journal">Kovtyukh; Soubiran, C.; Belik, S. I.; Gorlova, N. I.; 等. <a rel="nofollow" class="external text" href="http://www.aanda.org/articles/aa/full/2003/46/aa3944/aa3944.html">High precision effective temperatures for 181 F-K dwarfs from line-depth ratios</a>. <a href="./Astronomy_and_Astrophysics" class="mw-redirect" title="Astronomy and Astrophysics">Astronomy and Astrophysics</a>. 2003, <b>411</b> (3): 559–564 <span class="reference-accessdate"> [<span class="nowrap">2011-10-19</span>]</span>. <a rel="nofollow" class="external text" href="//ui.adsabs.harvard.edu/abs/2003A&A...411..559K"><span>Bibcode:2003A&A...411..559K</span></a>. <span class="plainlinks"><a rel="nofollow" class="external text" href="//arxiv.org/abs/astro-ph/0308429"><span>arXiv:astro-ph/0308429</span></a> <img alt="可免費查閱" src="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png" decoding="async" title="可免費查閱" width="9" height="14" srcset="//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/14px-Lock-green.svg.png 1.5x, //upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/18px-Lock-green.svg.png 2x" data-file-width="512" data-file-height="813"></span>. <a rel="nofollow" class="external text" href="//dx.doi.org/10.1051%2F0004-6361%3A20031378"><span>doi:10.1051/0004-6361:20031378</span></a>. （原始內容<a rel="nofollow" class="external text" href="//web.archive.org/web/20190516001408/https://www.aanda.org/articles/aa/full/2003/46/aa3944/aa3944.html">存檔</a>於2019-05-16）.</cite><span class="citation-comment" style="display:none; color:#33aa33"> 引文格式1維護：顯式使用等標籤 (<a href="./Category:%E5%BC%95%E6%96%87%E6%A0%BC%E5%BC%8F1%E7%BB%B4%E6%8A%A4%EF%BC%9A%E6%98%BE%E5%BC%8F%E4%BD%BF%E7%94%A8%E7%AD%89%E6%A0%87%E7%AD%BE" title="Category:引文格式1維護：顯式使用等標籤">link</a>)</span></span></div>
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<div class="pcs-ref-body"><span class="reference-text"><cite class="citation journal">J.S. Greaves, D.A. Fischer, M.C. Wyatt. <a rel="nofollow" class="external text" href="http://www.astro.washington.edu/courses/astro421/SciPapers/StarFormation/metallicity_debrisdisks.pdf">Metallicity, Debris Discs and Planets</a> <span style="font-size:85%;">(PDF)</span>. Monthly Notices of the Royal Astronomical Society. 2006, <b>366</b>: 283–286 <span class="reference-accessdate"> [<span class="nowrap">2011-10-19</span>]</span>. <a rel="nofollow" class="external text" href="//ui.adsabs.harvard.edu/abs/2006MNRAS.366..283G"><span>Bibcode:2006MNRAS.366..283G</span></a>. <a rel="nofollow" class="external text" href="//dx.doi.org/10.1111%2Fj.1365-2966.2005.09848.x"><span>doi:10.1111/j.1365-2966.2005.09848.x</span></a>. （原始內容<a rel="nofollow" class="external text" href="//web.archive.org/web/20120229212459/http://www.astro.washington.edu/courses/astro421/SciPapers/StarFormation/metallicity_debrisdisks.pdf">存檔</a> <span style="font-size:85%;">(PDF)</span>於2012-02-29）.</cite></span></div>
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外部链接.E5.A4.96.E9.83.A8.E9.93.BE.E6.8E.A5" class="pcs-edit-section-title">外部連結</h
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<h2><span class="mw-headline" id="外部链接">外部連結</span></h2>
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<li><cite class="citation web"><a rel="nofollow" class="external text" href="http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=HD+22484&NbIdent=1&Radius=10&Radius.unit=arcmin&CooFrame=FK5&CooEpoch=2000&CooEqui=2000&output.max=all&o.catall=on&output.mesdisp=N&Bibyear1=1983&Bibyear2=2006&Frame1=FK5&Frame2=FK4&Frame3=G&Equi1=2000.0&Equi2=1950.0&Equi3=2000.0&Epoch1=2000.0&Epoch2=1950.0&Epoch3=2000.0">HD 22484 -- High proper-motion Star</a>. SIMBAD. <span class="reference-accessdate"> [<span class="nowrap">2006-08-10</span>]</span>.</cite></li>
<li><cite class="citation web"><a rel="nofollow" class="external text" href="//web.archive.org/web/20110607164810/http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c00315.htm">4C00315</a>. ARICNS. 1998-03-04 <span class="reference-accessdate"> [<span class="nowrap">2006-08-10</span>]</span>. （<a rel="nofollow" class="external text" href="http://www.ari.uni-heidelberg.de/datenbanken/aricns/cnspages/4c00315.htm">原始內容</a>存檔於2011-06-07）.</cite></li>
<li><cite class="citation web"><a rel="nofollow" class="external text" href="//web.archive.org/web/20070928160150/http://www.stellar-database.com/Scripts/search_star.exe?ID=25500">10 Tauri</a>. Internet Stellar Database. <span class="reference-accessdate"> [<span class="nowrap">2006-08-10</span>]</span>. （<a rel="nofollow" class="external text" href="http://www.stellar-database.com/Scripts/search_star.exe?ID=25500">原始內容</a>存檔於2007-09-28）.</cite></li>
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