Tepiamenit - Revision history

YoulaAzkarrula at 02:37, 17 August 2026

2026-08-17T02:37:30Z

← Older revision		Revision as of 02:37, 17 August 2026
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	{{Infobox constellation		{{Infobox constellation
	\| name = Tepiamenit		\| name = Tepiamenit
	\| native =		\| native = Tepiamenit
	\| translation = Predecessor of the Pole		\| translation = Predecessor of the Pole
	\| pronounce = ~~Tepiamenit~~		\| pronounce =
	\| IPA =		\| IPA =
	\| culture = ~~Egypt~~		\| culture = IAU
	\| RA = 206.8155757		\| RA = 206.8155757
	\| dec = 17.45689154		\| dec = 17.45689154

IanRidpath: Umlaut in Boötes, Deleted irrelevant ref

2026-07-23T21:09:13Z

Umlaut in Boötes, Deleted irrelevant ref

← Older revision		Revision as of 21:09, 23 July 2026
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	}}		}}
	[[File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|thumb\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).]]		[[File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|thumb\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).]]
	Tepiamenit, Predecessor of the Pole, is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is ancient Egyptian. It is the name of the star τ Boo (HIP 67275, HR 5185) in constellation [[Bootes]].		Tepiamenit, Predecessor of the Pole, is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is ancient Egyptian. It is the name of the star τ Boo (HIP 67275, HR 5185) in constellation [[Bootes\|Boötes]].

	==Concordance, Etymology, History==		==Concordance, Etymology, History==
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	* [[References\|References (general)]]		* [[References\|References (general)]]
	* [[References (Medieval and Early Modern)\|References (early modern)]]		* [[References (Medieval and Early Modern)\|References (early modern)]]
	* Ian Ridpath's website ([http://ianridpath.com/startales Star Tales] )

	[[Category:Single star-asterism‏‎]] [[Category:Asterism]]		[[Category:Single star-asterism‏‎]] [[Category:Asterism]]

Sushoff: /* Exoplanet */

2026-07-06T07:56:26Z

Exoplanet

← Older revision		Revision as of 07:56, 6 July 2026
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	Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets with >1373.03 M<sub>⨁</sub> discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>		Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets with >1373.03 M<sub>⨁</sub> discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>
	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium - version of "smaller" constellation as depicted in Dendera
	File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN).		File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, original huge constellation, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN)
	File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.
	File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).		File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).

Sushoff: /* Exoplanet */

2026-07-06T07:55:17Z

Exoplanet

← Older revision		Revision as of 07:55, 6 July 2026
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	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium
	File:~~Eg_const_pole1250BCE_stellarium~~.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN).
	File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg~~\|thumb~~\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).		File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.
			File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).
	</gallery>		</gallery>

Sushoff at 07:06, 6 July 2026

2026-07-06T07:06:37Z

← Older revision		Revision as of 07:06, 6 July 2026
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	\| bordering = Boo		\| bordering = Boo
	\| notes =		\| notes =
			\| cat = IAU-Star Name
	}}		}}
	[[File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|thumb\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).]]		[[File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|thumb\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).]]

Sushoff at 07:05, 6 July 2026

2026-07-06T07:05:22Z

← Older revision		Revision as of 07:05, 6 July 2026
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	The name was proposed as a candidate proper name for a naked eye star in the vicinity of Muphrid that would preserve the heritage of this ancient Egyptian asterism. The WGSN adopted the name '''Tepiamenit''' for the star τ Bootis and added it to the IAU-CSN on April 16, 2026.		The name was proposed as a candidate proper name for a naked eye star in the vicinity of Muphrid that would preserve the heritage of this ancient Egyptian asterism. The WGSN adopted the name '''Tepiamenit''' for the star τ Bootis and added it to the IAU-CSN on April 16, 2026.

	The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B. Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>		The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B.

			=== Exoplanet ===

			Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets with >1373.03 M<sub>⨁</sub> discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>
	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium

Sushoff at 07:01, 6 July 2026

2026-07-06T07:01:30Z

@@ Line 2: / Line 2: @@
 ----
 [[File:Tepiamenit profileCard SadeghFaghanpour-IAU-WGSN.jpg|thumb|Tepiamenit profile card (CC BY Sadegh Faghanpour, IAU WGSN).]]
 [[File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg|thumb|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).]]
 Tepiamenit, Predecessor of the Pole, is a modern star name adopted by the International Astronomical Union in the IAU-Catalog of Star Names (IAU-CSN). Its origin is ancient Egyptian. It is the name of the star τ Boo (HIP 67275, HR 5185) in constellation [[Bootes]].

Sushoff: /* IAU Working Group on Star Names */

2026-07-03T19:40:09Z

IAU Working Group on Star Names

← Older revision		Revision as of 19:40, 3 July 2026
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	The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B. Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>		The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B. Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>
	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus ~~Neues Mus~~. ~~Berlin~~		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium
	File:Eg_const_pole1250BCE_stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Eg_const_pole1250BCE_stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.

Sushoff at 19:38, 3 July 2026

2026-07-03T19:38:33Z

← Older revision		Revision as of 19:38, 3 July 2026
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	[[Category:Africa]] [[Category:North Africa]]		[[Category:Africa]] [[Category:North Africa]]
	[[Category:Egyptian]]		[[Category:Egyptian]]
			[[Category:Boo]]

Sushoff: /* IAU Working Group on Star Names */

2026-07-03T19:14:33Z

IAU Working Group on Star Names

← Older revision		Revision as of 19:14, 3 July 2026
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	The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B. Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>		The name was assigned specifically to the bright (V=4.50 magnitude) F7V-type star τ Boo A (HD 120136, GJ 527A, HR 5185, HIP 67275) , which is in a binary system with a faint red dwarf companion τ Boo B. Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>
	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus Neues Mus. Berlin
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium
	File:Eg_const_pole1250BCE_stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Eg_const_pole1250BCE_stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.

← Older revision		Revision as of 07:56, 6 July 2026
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	Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets with >1373.03 M<sub>⨁</sub> discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>		Orbiting τ Boo A / Tepiamenit on a very close-in 3.3-day orbital period orbit is the famous exoplanet τ Boo Ab, which was one of the first 'hot Jupiter' type exoplanets with >1373.03 M<sub>⨁</sub> discovered (by [https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.115B/abstract Paul Butler and collaborators 1997)]. τ Boo Ab and its host star were one of the initial exoplanetary systems selected for public naming in the first IAU NameExoWorlds (2015) campaign, however the top vote-getting selection was disqualified, and the system went unnamed ([https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/iau-from-new-worlds-to-exoworlds-recollections-of-a-mandate/3169A64226F084E3BF80B30F2FDBB4D5 Montmerle 2019]). <gallery>
	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium - version of "smaller" constellation as depicted in Dendera
	File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN).		File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, original huge constellation, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN)
	File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.
	File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).		File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).

← Older revision		Revision as of 07:55, 6 July 2026
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	File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).		File:Rrt-hippoGoddess sarcophagus NeuesMusBerlin.jpg\|Rrt at sarcophagus of Nectanebo (Staatliche Museen zu Berlin – Ägyptisches Museum und Papyrussammlung, ÄM 7).
	File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium		File:Reret+Menit stellarium.jpg\|Reret and Menit (Berlin) mapped to Stellarium
	File:~~Eg_const_pole1250BCE_stellarium~~.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.		File:Rrt+mnt IAUstarNames stellarium.jpg\|Reret and Menit on Stellarium map, with the two IAU-star names Khepdenreret and Tepiamenit (CC BY WGSN).
	File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg~~\|thumb~~\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).		File:Eg const pole1250BCE stellarium.jpg\|Egyptian constellation of the late (Roman time) Dendera Zodiac with the precession circle and the circumpolar circle for Northern Egypt in 1250 BCE. Simulation with Stellarium<ref>Zotti, Georg; Hoffmann, Susanne M.; Wolf, Alexander; Chéreau, Fabien & Chéreau, Guillaume, "The Simulated Sky: Stellarium for Cultural Astronomy Research", ''Journal of Skyscape Archaeology'', '''6(2)''' (2020), 221--258 <nowiki>https://doi.org/10.1558/jsa.17822</nowiki>.</ref>.
			File:Tepiamenit stickfigure SadeghFaghanpour-IAU-WGSN.jpg\|Tepiamenit stick figure (CC BY Sadegh Faghanpour, IAU WGSN).
	</gallery>		</gallery>