https://en.wikipedia.org/w/index.php?action=history&feed=atom&title=LyraLyra - Revision history2025-01-06T00:09:02ZRevision history for this page on the wikiMediaWiki 1.44.0-wmf.8https://en.wikipedia.org/w/index.php?title=Lyra&diff=1254072135&oldid=prevMonkbot: Task 20: replace {lang-??} templates with {langx|??} ‹See Tfd› (Replaced 1);2024-10-29T08:42:19Z<p><a href="/wiki/User:Monkbot/task_20" class="mw-redirect" title="User:Monkbot/task 20">Task 20</a>: replace {lang-??} templates with {langx|??} <a href="/wiki/Wikipedia:Templates_for_discussion/Log/2024_September_27#Replace_and_delete_lang-??_templates" title="Wikipedia:Templates for discussion/Log/2024 September 27">‹See Tfd›</a> (Replaced 1);</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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{<del style="font-weight: bold; text-decoration: none;">lang-</del>grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{<ins style="font-weight: bold; text-decoration: none;">langx|</ins>grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</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>[[Vega]], Lyra's brightest star, is [[list of brightest stars|one of the brightest stars in the night sky]], and forms a corner of the famed [[Summer Triangle]] [[Asterism (astronomy)|asterism]]. [[Beta Lyrae]] is the prototype of a class of [[binary star]]s known as [[Beta Lyrae variable]]s. These binary stars are so close to each other that they become egg-shaped and material flows from one to the other. [[Epsilon Lyrae]], known informally as the Double Double, is a complex multiple star system. Lyra also hosts the [[Ring Nebula]], the second-discovered and best-known [[planetary nebula]].</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>[[Vega]], Lyra's brightest star, is [[list of brightest stars|one of the brightest stars in the night sky]], and forms a corner of the famed [[Summer Triangle]] [[Asterism (astronomy)|asterism]]. [[Beta Lyrae]] is the prototype of a class of [[binary star]]s known as [[Beta Lyrae variable]]s. These binary stars are so close to each other that they become egg-shaped and material flows from one to the other. [[Epsilon Lyrae]], known informally as the Double Double, is a complex multiple star system. Lyra also hosts the [[Ring Nebula]], the second-discovered and best-known [[planetary nebula]].</div></td>
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</table>Monkbothttps://en.wikipedia.org/w/index.php?title=Lyra&diff=1253874704&oldid=prev80.232.221.188: /* Deep-sky objects */2024-10-28T10:11:06Z<p><span class="autocomment">Deep-sky objects</span></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;"><div>[[File:Messier 56 HST.jpg|right|thumb|[[Messier 56]] is composed of a large number of stars, tightly bound to each other by gravity.<ref>{{cite news|title=A Collection of Ancient Stars|url=http://www.spacetelescope.org/images/potw1234a/|access-date=20 August 2012|newspaper=ESA/Hubble Picture of the Week}}</ref> In Lyra are the objects M56, M57, and Kuiper&nbsp;90. [[Messier 56|M56]] is a rather loose [[globular cluster]] at a distance of approximately 32,900 [[light-year]]s, with a diameter of about 85 light-years. Its apparent brightness is 8.3m.]]</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>[[File:Messier 56 HST.jpg|right|thumb|[[Messier 56]] is composed of a large number of stars, tightly bound to each other by gravity.<ref>{{cite news|title=A Collection of Ancient Stars|url=http://www.spacetelescope.org/images/potw1234a/|access-date=20 August 2012|newspaper=ESA/Hubble Picture of the Week}}</ref> In Lyra are the objects M56, M57, and Kuiper&nbsp;90. [[Messier 56|M56]] is a rather loose [[globular cluster]] at a distance of approximately 32,900 [[light-year]]s, with a diameter of about 85 light-years. Its apparent brightness is 8.3m.]]</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>[[Ring Nebula|M57]], also known as the "Ring Nebula" and NGC 6720,<ref>{{cite book|first=David H.|last=Levy|title=Deep Sky Objects|date=2005|publisher=Prometheus Books|isbn=1-59102-361-0|url-access=registration|url=https://archive.org/details/deepskyobjects00davi|page=123}}</ref> at a distance of 2,<del style="font-weight: bold; text-decoration: none;">000</del> light-years from Earth is one of the best known [[planetary nebula]]e and the second to be discovered; its integrated magnitude is 8.8.<ref name="objects"/> It was discovered in 1779 by [[Antoine Darquier]], 15 years after [[Charles Messier]] discovered the [[Dumbbell Nebula]].{{sfn|Levy|2005|p=125}} Astronomers have determined that it is between 6,000 and 8,000 years old;<ref name="objects"/> it is approximately one light-year in diameter.{{sfn|Levy|2005|p=124}} The outer part of the nebula appears red in photographs because of emission from [[ionized hydrogen]]. The middle region is colored green; [[doubly ionized oxygen]] emits greenish-blue light. The hottest region, closest to the central star, appears blue because of emission from [[helium]]. The central star itself is a [[white dwarf]] with a temperature of 120,000 [[kelvin]]s. In telescopes, the nebula appears as a visible ring with a green tinge; it is slightly elliptical because its three-dimensional shape is a [[torus]] or [[cylinder (geometry)|cylinder]] seen from a slight angle.<ref name="objects">{{cite book |title=300 Astronomical Objects: A Visual Reference to the Universe |first1=Jamie |last1=Wilkins |first2=Robert |last2=Dunn |publisher=Firefly Books |date=2006 |location=Buffalo, New York |isbn=978-1-55407-175-3}}</ref> It can be found halfway between [[Gamma Lyrae]] and Beta Lyrae.{{sfn|Levy|2005|p=124}}</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>[[Ring Nebula|M57]], also known as the "Ring Nebula" and NGC 6720,<ref>{{cite book|first=David H.|last=Levy|title=Deep Sky Objects|date=2005|publisher=Prometheus Books|isbn=1-59102-361-0|url-access=registration|url=https://archive.org/details/deepskyobjects00davi|page=123}}</ref> at a distance of 2,<ins style="font-weight: bold; text-decoration: none;">550</ins> light-years from Earth is one of the best known [[planetary nebula]]e and the second to be discovered; its integrated magnitude is 8.8.<ref name="objects"/> It was discovered in 1779 by [[Antoine Darquier]], 15 years after [[Charles Messier]] discovered the [[Dumbbell Nebula]].{{sfn|Levy|2005|p=125}} Astronomers have determined that it is between 6,000 and 8,000 years old;<ref name="objects"/> it is approximately one light-year in diameter.{{sfn|Levy|2005|p=124}} The outer part of the nebula appears red in photographs because of emission from [[ionized hydrogen]]. The middle region is colored green; [[doubly ionized oxygen]] emits greenish-blue light. The hottest region, closest to the central star, appears blue because of emission from [[helium]]. The central star itself is a [[white dwarf]] with a temperature of 120,000 [[kelvin]]s. In telescopes, the nebula appears as a visible ring with a green tinge; it is slightly elliptical because its three-dimensional shape is a [[torus]] or [[cylinder (geometry)|cylinder]] seen from a slight angle.<ref name="objects">{{cite book |title=300 Astronomical Objects: A Visual Reference to the Universe |first1=Jamie |last1=Wilkins |first2=Robert |last2=Dunn |publisher=Firefly Books |date=2006 |location=Buffalo, New York |isbn=978-1-55407-175-3}}</ref> It can be found halfway between [[Gamma Lyrae]] and Beta Lyrae.{{sfn|Levy|2005|p=124}}</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>Another planetary nebula in Lyra is [[Abell 46]]. The central star, [[V477 Lyrae]], is an eclipsing [[Post common envelope binary|post-common-envelope binary]], consisting of a white dwarf primary and an oversized secondary component due to recent accretion. The nebula itself is of relatively low surface brightness compared to the central star,<ref name="PollaccoBell1994">{{cite journal |last1=Pollacco |first1=D. L. |last2=Bell |first2=S. A. |title=A preliminary analysis of the planetary nebula central star V477 Lyrae |journal=Monthly Notices of the Royal Astronomical Society |volume=267 |issue=2 |pages=452–464 |date=1994 |bibcode=1994MNRAS.267..452P |doi=10.1093/mnras/267.2.452|doi-access=free }}</ref> and is undersized for the primary's mass for reasons not yet fully understood.<ref name="CorradiGarcía-Rojas2015">{{cite journal |last1=Corradi |first1=Romano L. M. |last2=García-Rojas |first2=Jorge |last3=Jones |first3=David |last4=Rodríguez-Gil |first4=Pablo |title=Binarity and the Abundance Discrepancy Problem in Planetary Nebulae |journal=The Astrophysical Journal |volume=803 |issue=2 |date=2015 |pages=99 |bibcode=2015ApJ...803...99C |doi=10.1088/0004-637X/803/2/99 |arxiv=1502.05182 |s2cid=118565181 }}</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>Another planetary nebula in Lyra is [[Abell 46]]. The central star, [[V477 Lyrae]], is an eclipsing [[Post common envelope binary|post-common-envelope binary]], consisting of a white dwarf primary and an oversized secondary component due to recent accretion. The nebula itself is of relatively low surface brightness compared to the central star,<ref name="PollaccoBell1994">{{cite journal |last1=Pollacco |first1=D. L. |last2=Bell |first2=S. A. |title=A preliminary analysis of the planetary nebula central star V477 Lyrae |journal=Monthly Notices of the Royal Astronomical Society |volume=267 |issue=2 |pages=452–464 |date=1994 |bibcode=1994MNRAS.267..452P |doi=10.1093/mnras/267.2.452|doi-access=free }}</ref> and is undersized for the primary's mass for reasons not yet fully understood.<ref name="CorradiGarcía-Rojas2015">{{cite journal |last1=Corradi |first1=Romano L. M. |last2=García-Rojas |first2=Jorge |last3=Jones |first3=David |last4=Rodríguez-Gil |first4=Pablo |title=Binarity and the Abundance Discrepancy Problem in Planetary Nebulae |journal=The Astrophysical Journal |volume=803 |issue=2 |date=2015 |pages=99 |bibcode=2015ApJ...803...99C |doi=10.1088/0004-637X/803/2/99 |arxiv=1502.05182 |s2cid=118565181 }}</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;"><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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{lang-grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{lang-grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</div></td>
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</table>HirowoWikihttps://en.wikipedia.org/w/index.php?title=Lyra&diff=1226351024&oldid=prevLumiel777 at 02:25, 30 May 20242024-05-30T02:25:52Z<p></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="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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{lang-grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</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>{{langnf|la|'''Lyra'''|[[lyre]]|paren=left}}, from {{lang-grc|λύρα}}; pronounced: {{IPAc-en|ˈ|l|aɪ|r|ə}} {{respell|LY|rə}})<ref>Lesley Brown: The New Shorter Oxford English Dictionary. Vol.&nbsp;1:&nbsp;A−M.'' [[Oxford University Press|Clarendon Press]]'', Oxford 1993, p.&nbsp;1651</ref> is a small [[constellation]]. It is one of the 48 listed by the 2nd century astronomer [[Ptolemy]], and is one of the modern 88 constellations recognized by the [[International Astronomical Union]]. Lyra was often represented on star maps as a [[vulture]] or an [[eagle]] carrying a lyre, and hence is sometimes referred to as '''Vultur Cadens''' or '''Aquila Cadens''' ("Falling Vulture"<ref>{{cite book|last1=Bistue|first1=Belen|title=Collaborative Translation and Multi-Version Texts in Early Modern Europe|date=May 23, 2016|publisher=Routledge|isbn=978-1317164357|pages=72–73|url=https://books.google.com/books?id=Nlc3DAAAQBAJ|ref=Bistue}}</ref> or "Falling Eagle"), respectively. Beginning at the north, Lyra is bordered by [[Draco (constellation)|Draco]], [[Hercules (constellation)|Hercules]], [[Vulpecula]], and [[Cygnus (constellation)|Cygnus]]. Lyra is nearly overhead in temperate northern latitudes shortly after midnight at the start of summer. From the equator to about the [[40th parallel south]] it is visible low in the northern sky during the same (thus winter) months.</div></td>
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</table>Lumiel777https://en.wikipedia.org/w/index.php?title=Lyra&diff=1224754234&oldid=prevCaspian Rehbinder: /* See also */ Aniara is mainly a work of poetry, which also revolves around Lyra2024-05-20T07:39:11Z<p><span class="autocomment">See also: </span> Aniara is mainly a work of poetry, which also revolves around Lyra</p>
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</table>Caspian Rehbinderhttps://en.wikipedia.org/w/index.php?title=Lyra&diff=1223299886&oldid=prevGünniX: v2.05 - Fix errors for CW project (Reference list duplication)2024-05-11T05:18:54Z<p>v2.05 - Fix errors for <a href="/wiki/Wikipedia:WCW" class="mw-redirect" title="Wikipedia:WCW">CW project</a> (Reference list duplication)</p>
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</table>GünniXhttps://en.wikipedia.org/w/index.php?title=Lyra&diff=1222515993&oldid=prevYodin: /* History */ copy edit2024-05-06T11:54:12Z<p><span class="autocomment">History: </span> copy edit</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>The Roman book {{lang|la|[[De astronomia]]}}, attributed to [[Hyginus]], also records another myth about Lyra, which said that it belonged to [[Theseus]] "for he was skilful in all the arts and seems to have learned the lyre as well". The book reports that the neighbouring constellation now known as [[Hercules (constellation)|Hercules]] was said to depict many different mythical figures, including Theseus, Orpheus, or the musician [[Thamyris]].<ref name=Kneeler>{{cite web | first=Mary | last=Grant | title=Hyginus, Astronomica: 2.6 'The Kneeler' | website=[[Theoi Project]] | access-date=2017-12-24 | url=http://www.theoi.com/Text/HyginusAstronomica.html#6 | archive-date=2017-12-24 | archive-url=https://web.archive.org/web/20171224042241/http://www.theoi.com/Text/HyginusAstronomica.html#6 }}</ref> The proximity <del style="font-weight: bold; text-decoration: none;">between</del> these two constellations and [[Corona Borealis]] (perhaps a symbol of Theseus' royalty) could indicate that the three constellations were invented as a group.<ref>{{cite book | translator-first=Robin | translator-last=Hard | chapter=Hercules, originally known as Engonasin, the Kneeler | title=Constellation Myths | year=2015 | isbn=9780191026539 | publisher=Oxford University Press }}</ref></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>The Roman book {{lang|la|[[De astronomia]]}}, attributed to [[Hyginus]], also records another myth about Lyra, which said that it belonged to [[Theseus]] "for he was skilful in all the arts and seems to have learned the lyre as well". The book reports that the neighbouring constellation now known as [[Hercules (constellation)|Hercules]] was said to depict many different mythical figures, including Theseus, Orpheus, or the musician [[Thamyris]].<ref name=Kneeler>{{cite web | first=Mary | last=Grant | title=Hyginus, Astronomica: 2.6 'The Kneeler' | website=[[Theoi Project]] | access-date=2017-12-24 | url=http://www.theoi.com/Text/HyginusAstronomica.html#6 | archive-date=2017-12-24 | archive-url=https://web.archive.org/web/20171224042241/http://www.theoi.com/Text/HyginusAstronomica.html#6 }}</ref> The proximity <ins style="font-weight: bold; text-decoration: none;">of</ins> these two constellations and [[Corona Borealis]] (perhaps a symbol of Theseus' royalty) could indicate that the three constellations were invented as a group.<ref>{{cite book | translator-first=Robin | translator-last=Hard | chapter=Hercules, originally known as Engonasin, the Kneeler | title=Constellation Myths | year=2015 | isbn=9780191026539 | publisher=Oxford University Press }}</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;"><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>
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<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>Vega and its surrounding stars are also treated as a constellation in other cultures. The area corresponding to Lyra was seen by the Arabs as a [[vulture]] or an [[eagle]] diving with folded wings.<ref name="Ridpath">{{cite web |last1=Ridpath |first1=Ian |title=Star Tales - Lyra |work=Star Tales |url=http://www.ianridpath.com/startales/lyra.html |publisher=self-published |access-date=3 September 2021}}</ref> In [[Wales]], Lyra is known as King Arthur's Harp (''Talyn Arthur''), and King David's harp. The Persian [[Hafiz Shirazi|Hafiz]] called it the Lyre of Zurah.</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>Vega and its surrounding stars are also treated as a constellation in other cultures. The area corresponding to Lyra was seen by the Arabs as a [[vulture]] or an [[eagle]] diving with folded wings.<ref name="Ridpath">{{cite web |last1=Ridpath |first1=Ian |title=Star Tales - Lyra |work=Star Tales |url=http://www.ianridpath.com/startales/lyra.html |publisher=self-published |access-date=3 September 2021}}</ref> In [[Wales]], Lyra is known as King Arthur's Harp (''Talyn Arthur''), and King David's harp. The Persian [[Hafiz Shirazi|Hafiz]] called it the Lyre of Zurah.</div></td>
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</table>Yodin