https://en.wikipedia.org/w/index.php?action=history&feed=atom&title=CD%E2%88%9234_8618
CD−34 8618 - Revision history
2025-10-08T11:56:36Z
Revision history for this page on the wiki
MediaWiki 1.45.0-wmf.21
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1299143102&oldid=prev
Lithopsian: new key for Category:Wide Angle Search for Planets: "167" using HotCat
2025-07-06T20:11:05Z
<p>new key for <a href="/wiki/Category:Wide_Angle_Search_for_Planets" title="Category:Wide Angle Search for Planets">Category:Wide Angle Search for Planets</a>: "167" using <a href="/wiki/Wikipedia:HC" class="mw-redirect" title="Wikipedia:HC">HotCat</a></p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 20:11, 6 July 2025</td>
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Lithopsian
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1299141588&oldid=prev
Lithopsian: added Category:Wide Angle Search for Planets using HotCat
2025-07-06T20:02:15Z
<p>added <a href="/wiki/Category:Wide_Angle_Search_for_Planets" title="Category:Wide Angle Search for Planets">Category:Wide Angle Search for Planets</a> using <a href="/wiki/Wikipedia:HC" class="mw-redirect" title="Wikipedia:HC">HotCat</a></p>
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Lithopsian
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1292419940&oldid=prev
Mike s: add ref for constellation
2025-05-26T21:08:13Z
<p>add ref for constellation</p>
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<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> | epoch = <del style="font-weight: bold; text-decoration: none;">[[</del>J2000.0<del style="font-weight: bold; text-decoration: none;">]] ([[International Celestial Reference System|ICRS]])</del></div></td>
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<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> | epoch = J2000.0</div></td>
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<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> | constell = [[Centaurus]]</div></td>
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<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> | constell = [[Centaurus]]<ins style="font-weight: bold; text-decoration: none;"><ref name="Roman1987"/></ins></div></td>
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<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><ref name = Tycho2000>{{cite journal | last1 = Høg | first1 = E. | last2 = Fabricius | first2 = C. | last3 = Makarov | first3 = V. V. | last4 = Urban | first4 = S. | last5 = Corbin | first5 = T. | last6 = Wycoff | first6 = G. | last7 = Bastian | first7 = U. | last8 = Schwekendiek | first8 = P. | last9 = Wicenec | first9 = A. | title = The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics | date = March 2000 | volume = 355 | pages = L27–L30 | bibcode = 2000A&A...355L..27H | issn = 0004-6361}}</ref></div></td>
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<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><ref name = Tycho2000>{{cite journal | last1 = Høg | first1 = E. | last2 = Fabricius | first2 = C. | last3 = Makarov | first3 = V. V. | last4 = Urban | first4 = S. | last5 = Corbin | first5 = T. | last6 = Wycoff | first6 = G. | last7 = Bastian | first7 = U. | last8 = Schwekendiek | first8 = P. | last9 = Wicenec | first9 = A. | title = The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics | date = March 2000 | volume = 355 | pages = L27–L30 | bibcode = 2000A&A...355L..27H | issn = 0004-6361}}</ref></div></td>
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Mike s
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1183280136&oldid=prev
112.120.56.105 at 09:19, 3 November 2023
2023-11-03T09:19:11Z
<p></p>
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<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>{{Short description|F-type dwarf with a planet<ins style="font-weight: bold; text-decoration: none;"> in</ins> Centaurus}}</div></td>
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<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> | name = [[Bonner Durchmusterung|CD]]−34°8618</div></td>
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112.120.56.105
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1154754226&oldid=prev
JJMC89 bot III: Moving :Category:Centaurus (constellation) to :Category:Centaurus per Wikipedia:Categories for discussion/Speedy
2023-05-14T13:03:40Z
<p>Moving <a href="/w/index.php?title=Category:Centaurus_(constellation)&action=edit&redlink=1" class="new" title="Category:Centaurus (constellation) (page does not exist)">Category:Centaurus (constellation)</a> to <a href="/wiki/Category:Centaurus" title="Category:Centaurus">Category:Centaurus</a> per <a href="/wiki/Wikipedia:Categories_for_discussion/Speedy" title="Wikipedia:Categories for discussion/Speedy">Wikipedia:Categories for discussion/Speedy</a></p>
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JJMC89 bot III
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1136235518&oldid=prev
Usernamekiran (AWB): checkwiki error, fixed syntax, default sort
2023-01-29T11:05:39Z
<p>checkwiki error, fixed syntax, default sort</p>
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Usernamekiran (AWB)
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1115195004&oldid=prev
Dr vulpes: /* References */WP:CHECKWIKI HTML text style element, minor other wikitext edits
2022-10-10T07:27:19Z
<p><span class="autocomment">References: </span><a href="/wiki/Wikipedia:CHECKWIKI" class="mw-redirect" title="Wikipedia:CHECKWIKI">WP:CHECKWIKI</a> HTML text style element, minor other wikitext edits</p>
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<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><ref name = Stassun2019>{{cite journal | display-authors = 1 | last1 = Stassun | first1 = Keivan G. | last2 = Oelkers | first2 = Ryan J. | last3 = Paegert | first3 = Martin | last4 = Torres | first4 = Guillermo | last5 = Pepper | first5 = Joshua | last6 = Lee | first6 = Nathan De | last7 = Collins | first7 = Kevin | last8 = Latham | first8 = David W. | last9 = Muirhead | first9 = Philip S. | last10 = Chittidi | first10 = Jay | last11 = Rojas-Ayala | first11 = Bárbara | last12 = Fleming | first12 = Scott W. | last13 = Rose | first13 = Mark E. | last14 = Tenenbaum | first14 = Peter | last15 = Ting | first15 = Eric B. | last16 = Kane | first16 = Stephen R. | last17 = Barclay | first17 = Thomas | last18 = Bean | first18 = Jacob L. | last19 = Brassuer | first19 = C. E. | last20 = Charbonneau | first20 = David | last21 = Ge | first21 = Jian | last22 = Lissauer | first22 = Jack J. | last23 = Mann | first23 = Andrew W. | last24 = McLean | first24 = Brian | last25 = Mullally | first25 = Susan | last26 = Narita | first26 = Norio | last27 = Plavchan | first27 = Peter | last28 = Ricker | first28 = George R. | last29 = Sasselov | first29 = Dimitar | last30 = Seager | first30 = S. | last31 = Sharma | first31 = Sanjib | last32 = Shiao | first32 = Bernie | last33 = Sozzetti | first33 = Alessandro | last34 = Stello | first34 = Dennis | last35 = Vanderspek | first35 = Roland | last36 = Wallace | first36 = Geoff | last37 = Winn | first37 = Joshua N. | title = The Revised <ins style="font-weight: bold; text-decoration: none;">''</ins>TESS<ins style="font-weight: bold; text-decoration: none;">''</ins> Input Catalog and Candidate Target List | journal = The Astronomical Journal | date = 9 September 2019 | volume = 158 | issue = 4 | page = 138 | eissn = 1538-3881 | doi = 10.3847/1538-3881/ab3467 | bibcode = 2019AJ....158..138S | arxiv = 1905.10694 | doi-access = free}}</ref></div></td>
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<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><ref name = Temple2017>{{cite journal | display-authors = 1 | last1 = Temple | first1 = L. Y. | last2 = Hellier | first2 = C. | last3 = Albrow | first3 = M. D. | last4 = Anderson | first4 = D. R. | last5 = Bayliss | first5 = D. | last6 = Beatty | first6 = T. G. | last7 = Bieryla | first7 = A. | last8 = Brown | first8 = D. J. A. | last9 = Cargile | first9 = P. A. | last10 = Collier Cameron | first10 = A. | last11 = Collins | first11 = K. A. | last12 = Colón | first12 = K. D. | last13 = Curtis | first13 = I. A. | last14 = D'Ago | first14 = G. | last15 = Delrez | first15 = L. | last16 = Eastman | first16 = J. | last17 = Gaudi | first17 = B. S. | last18 = Gillon | first18 = M. | last19 = Gregorio | first19 = J. | last20 = James | first20 = D. | last21 = Jehin | first21 = E. | last22 = Joner | first22 = M. D. | last23 = Kielkopf | first23 = J. F. | last24 = Kuhn | first24 = R. B. | last25 = Labadie-Bartz | first25 = J. | last26 = Latham | first26 = D. W. | last27 = Lendl | first27 = M. | last28 = Lund | first28 = M. B. | last29 = Malpas | first29 = A. L. | last30 = Maxted | first30 = P. F. L. | last31 = Myers | first31 = G. | last32 = Oberst | first32 = T. E. | last33 = Pepe | first33 = F. | last34 = Pepper | first34 = J. | last35 = Pollacco | first35 = D. | last36 = Queloz | first36 = D. | last37 = Rodriguez | first37 = J. E. | last38 = Ségransan | first38 = D. | last39 = Siverd | first39 = R. J. | last40 = Smalley | first40 = B. | last41 = Stassun | first41 = K. G. | last42 = Stevens | first42 = D. J. | last43 = Stockdale | first43 = C. | last44 = Tan | first44 = T. G. | last45 = Triaud | first45 = A. H. M. J. | last46 = Udry | first46 = S. | last47 = Villanueva | first47 = S. | last48 = West | first48 = R. G. | last49 = Zhou | first49 = G. | title = WASP-167b/KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star | journal = Monthly Notices of the Royal Astronomical Society | date = 13 July 2017 | volume = 471 | issue = 3 | pages = 2743–2752 | issn = 0035-8711 | eissn = 1365-2966 | doi = 10.1093/mnras/stx1729 | bibcode = 2017MNRAS.471.2743T | arxiv = 1704.07771 | doi-access = free}}</ref></div></td>
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Dr vulpes
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1110668686&oldid=prev
Lithopsian: overly large lead
2022-09-16T19:31:46Z
<p>overly large lead</p>
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 19:31, 16 September 2022</td>
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<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>'''CD−34°8618''', also known as '''KELT-13''' or '''WASP-167''', is a yellowish-white hued [[star]] located in the southern [[constellation]] of [[Centaurus]]. It has an [[apparent magnitude]] of 10.52,<ref name = Tycho2000/> making it readily visible in medium sized [[telescope]]s, but not to the [[naked eye]]. Based on [[parallax]] measurements from the [[Gaia spacecraft]], the object is estimated to be approximately 1,350 [[light year]]s away from the [[Solar System]].<ref name = GaiaDR3/> It appears to be drifting closer to it, having a [[radial velocity]] of {{val|-0.53|ul=km/s}}.<ref name = GaiaDR2/></div></td>
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<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>'''CD−34°8618''', also known as '''KELT-13''' or '''WASP-167''', is a yellowish-white hued [[star]] located in the southern [[constellation]] of [[Centaurus]]. It has an [[apparent magnitude]] of 10.52,<ref name = Tycho2000/> making it readily visible in medium sized [[telescope]]s, but not to the [[naked eye]]. Based on [[parallax]] measurements from the [[Gaia spacecraft]], the object is estimated to be approximately 1,350 [[light year]]s away from the [[Solar System]].<ref name = GaiaDR3/> It appears to be drifting closer to it, having a [[radial velocity]] of {{val|-0.53|ul=km/s}}.<ref name = GaiaDR2/></div></td>
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<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>
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<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>==Description==</div></td>
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<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>WASP-167 has a [[stellar classification]] of F1 V,<ref name = Temple2017/> indicating that it is an ordinary [[F-type main-sequence star]] that is generating energy via [[hydrogen]] fusion at its core. At present it has 1.59 times the [[mass of the Sun]]<ref name = Temple2017/> and 1.94 times the [[radius of the Sun]].<ref name = Stassun2019/> It radiates 8.34 times the [[luminosity of the Sun]]<ref name = McDonald2017/> from its [[photosphere]] at an [[effective temperature]] of {{val|6909|ul=K|fmt=commas}}.<ref name = McDonald2017/> WASP-167 has an [[iron]] abundance 26% above solar levels,<ref name = Temple2017/> making it metal enriched — common among planetary hosts. The object has completed 63% of its [[main sequence]] lifetime<ref name = GaiaDR3/> at an age of 1 [[billion years]].<ref name = Temple2017/> Like many hot stars, WASP-167 spins rapidly, having a [[projected rotational velocity]] of {{val|52|ul=km/s}},<ref name = Saffe2021/> meaning it completes a rotation under 2 [[days]].<ref name = Temple2017/></div></td>
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<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>WASP-167 has a [[stellar classification]] of F1 V,<ref name = Temple2017/> indicating that it is an ordinary [[F-type main-sequence star]] that is generating energy via [[hydrogen]] fusion at its core. At present it has 1.59 times the [[mass of the Sun]]<ref name = Temple2017/> and 1.94 times the [[radius of the Sun]].<ref name = Stassun2019/> It radiates 8.34 times the [[luminosity of the Sun]]<ref name = McDonald2017/> from its [[photosphere]] at an [[effective temperature]] of {{val|6909|ul=K|fmt=commas}}.<ref name = McDonald2017/> WASP-167 has an [[iron]] abundance 26% above solar levels,<ref name = Temple2017/> making it metal enriched — common among planetary hosts. The object has completed 63% of its [[main sequence]] lifetime<ref name = GaiaDR3/> at an age of 1 [[billion years]].<ref name = Temple2017/> Like many hot stars, WASP-167 spins rapidly, having a [[projected rotational velocity]] of {{val|52|ul=km/s}},<ref name = Saffe2021/> meaning it completes a rotation under 2 [[days]].<ref name = Temple2017/></div></td>
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Lithopsian
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1110668307&oldid=prev
Lithopsian: Lithopsian moved page CD-34 8618 to CD−34 8618: that's a minus sign
2022-09-16T19:28:55Z
<p>Lithopsian moved page <a href="/wiki/CD-34_8618" class="mw-redirect" title="CD-34 8618">CD-34 8618</a> to <a href="/wiki/CD%E2%88%9234_8618" title="CD−34 8618">CD−34 8618</a>: that's a minus sign</p>
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<td colspan="1" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 19:28, 16 September 2022</td>
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Lithopsian
https://en.wikipedia.org/w/index.php?title=CD%E2%88%9234_8618&diff=1110668254&oldid=prev
Lithopsian: no space in the designation
2022-09-16T19:28:20Z
<p>no space in the designation</p>
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<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>
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<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;">CD −34</del>°8618''', also known as '''KELT-13''' or '''WASP-167''', is a yellowish-white hued [[star]] located in the southern [[constellation]] of [[Centaurus]]. It has an [[apparent magnitude]] of 10.52,<ref name = Tycho2000/> making it readily visible in medium sized [[telescope]]s, but not to the [[naked eye]]. Based on [[parallax]] measurements from the [[Gaia spacecraft]], the object is estimated to be approximately 1,350 [[light year]]s away from the [[Solar System]].<ref name = GaiaDR3/> It appears to be drifting closer to it, having a [[radial velocity]] of {{val|-0.53|ul=km/s}}.<ref name = GaiaDR2/></div></td>
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<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;">CD−34</ins>°8618''', also known as '''KELT-13''' or '''WASP-167''', is a yellowish-white hued [[star]] located in the southern [[constellation]] of [[Centaurus]]. It has an [[apparent magnitude]] of 10.52,<ref name = Tycho2000/> making it readily visible in medium sized [[telescope]]s, but not to the [[naked eye]]. Based on [[parallax]] measurements from the [[Gaia spacecraft]], the object is estimated to be approximately 1,350 [[light year]]s away from the [[Solar System]].<ref name = GaiaDR3/> It appears to be drifting closer to it, having a [[radial velocity]] of {{val|-0.53|ul=km/s}}.<ref name = GaiaDR2/></div></td>
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<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>
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<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>WASP-167 has a [[stellar classification]] of F1 V,<ref name = Temple2017/> indicating that it is an ordinary [[F-type main-sequence star]] that is generating energy via [[hydrogen]] fusion at its core. At present it has 1.59 times the [[mass of the Sun]]<ref name = Temple2017/> and 1.94 times the [[radius of the Sun]].<ref name = Stassun2019/> It radiates 8.34 times the [[luminosity of the Sun]]<ref name = McDonald2017/> from its [[photosphere]] at an [[effective temperature]] of {{val|6909|ul=K|fmt=commas}}.<ref name = McDonald2017/> WASP-167 has an [[iron]] abundance 26% above solar levels,<ref name = Temple2017/> making it metal enriched — common among planetary hosts. The object has completed 63% of its [[main sequence]] lifetime<ref name = GaiaDR3/> at an age of 1 [[billion years]].<ref name = Temple2017/> Like many hot stars, WASP-167 spins rapidly, having a [[projected rotational velocity]] of {{val|52|ul=km/s}},<ref name = Saffe2021/> meaning it completes a rotation under 2 [[days]].<ref name = Temple2017/></div></td>
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<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>WASP-167 has a [[stellar classification]] of F1 V,<ref name = Temple2017/> indicating that it is an ordinary [[F-type main-sequence star]] that is generating energy via [[hydrogen]] fusion at its core. At present it has 1.59 times the [[mass of the Sun]]<ref name = Temple2017/> and 1.94 times the [[radius of the Sun]].<ref name = Stassun2019/> It radiates 8.34 times the [[luminosity of the Sun]]<ref name = McDonald2017/> from its [[photosphere]] at an [[effective temperature]] of {{val|6909|ul=K|fmt=commas}}.<ref name = McDonald2017/> WASP-167 has an [[iron]] abundance 26% above solar levels,<ref name = Temple2017/> making it metal enriched — common among planetary hosts. The object has completed 63% of its [[main sequence]] lifetime<ref name = GaiaDR3/> at an age of 1 [[billion years]].<ref name = Temple2017/> Like many hot stars, WASP-167 spins rapidly, having a [[projected rotational velocity]] of {{val|52|ul=km/s}},<ref name = Saffe2021/> meaning it completes a rotation under 2 [[days]].<ref name = Temple2017/></div></td>
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Lithopsian