Kenemu: Difference between revisions
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In ancient Egyptian cosmology, boats carried the sun god Ra, and the deceased pharaoh's soul on its journey through the afterlife. The WjA constellation symbolized these vital spiritual and solar voyages. | In ancient Egyptian cosmology, boats carried the sun god Ra, and the deceased pharaoh's soul on its journey through the afterlife. The WjA constellation symbolized these vital spiritual and solar voyages. | ||
Therefore constellation is also engraved on the granite sarcophagus lid of Djehapimu, the Royal Audit Officer, c. | Therefore constellation is also engraved on the granite sarcophagus lid of Djehapimu, the Royal Audit Officer and a relative of King Nectanebo II (Nakhthorheb, ''Nḫt-Ḥr-Ḥbt)'', c. 346-332 BCE, granite, displayed in the exhibition of the Neues Museum Berlin, Germany. | ||
== IAU WGSN star name discussion == | == IAU WGSN star name discussion == | ||
The name was proposed to WGSN in 2025. As Kenemu means something as "crew", we are not sure if it would be appropriate for a single star. Juan Belmonte suggests to look for any pair of closing stars or a star which is multiple (not to the naked eye) in the area east of Kaus Australis, as in that case, it may suit. Yet, Belmonte and Lull (2023) and Lull (2018) both identify ρ<sup>1</sup> Sgr at 3.93 mag in V. | The name was proposed to WGSN in 2025. As Kenemu means something as "crew", we are not sure if it would be appropriate for a single star. Juan Belmonte suggests to look for any pair of closing stars or a star which is multiple (not to the naked eye) in the area east of Kaus Australis, as in that case, it may suit. Yet, Belmonte and Lull (2023) and Lull (2018) both identify ρ<sup>1</sup> Sgr at 3.93 mag in V. | ||
In 2026, the name "Kenemu" was proposed for the star ρ1 Sgr (Rho1 Sagittarii, 44 Sgr, HR 7340, HD 181577, HIP 95168), a spectral type A9IV star with apparent magnitude V=3.92 that lies 40 parsecs away. The star is a Delta Scuti variable star that varies at the ~0.04 magnitude level on a timescale of ~1.2 hours. The star has a mass approximately 1.9x that of the Sun, and a luminosity of approximately 31x the Sun, placing it about ~1.5 magnitudes brighter than the main sequence, and making it a post-main sequence star. <gallery> | In 2026, the name "'''Kenemu'''" was proposed for the star [https://simbad.cds.unistra.fr/simbad/sim-id?Ident=44+Sgr ρ1 Sgr (Rho1 Sagittarii, 44 Sgr, HR 7340, HD 181577, HIP 95168)], a spectral type A9IV star with apparent magnitude V=3.92 that lies 40 parsecs away. The star is a Delta Scuti variable star that varies at the ~0.04 magnitude level on a timescale of ~1.2 hours. The star has a mass approximately 1.9x that of the Sun, and a luminosity of approximately 31x the Sun, placing it about ~1.5 magnitudes brighter than the main sequence, and making it a post-main sequence star. <gallery> | ||
File:Heryibwia profileCard SadeghFaghanpour-IAU-WGSN.jpg|link=|Heryibwia profile card (CC BY M.Sadegh Faghanpour for IAU-WGSN). | File:Heryibwia profileCard SadeghFaghanpour-IAU-WGSN.jpg|link=|Heryibwia profile card (CC BY M.Sadegh Faghanpour for IAU-WGSN). | ||
File:Heryibwia stickfigure SadeghFaghanpour-IAU-WGSN.jpg|link=|Heryibwia stick figure (CC BY M.Sadegh Faghanpour for IAU-WGSN). | File:Heryibwia stickfigure SadeghFaghanpour-IAU-WGSN.jpg|link=|Heryibwia stick figure (CC BY M.Sadegh Faghanpour for IAU-WGSN). | ||
Latest revision as of 03:28, 18 September 2026
Authors: Susanne M Hoffmann, Eric Mamajek, ASE Tech Team

| Asterism Info | |
| Native | Knmw |
|---|---|
| Translation | crew |
| Position (2000) | |
| Right ascension | 290.4181661 |
| Declination | -17.84719859 |
| Area | 0 sq. deg. |
| Stars | |
| Bright stars | 1 |
| Bayer/Flamsteed stars | 1 |
| Stars brighter than 3.00m | 0 |
| Brightest star | Kenemu (3.93m) |
| Taxonomy | |
| category of asterism | IAU-Star Name |
| IAU- constellations | Sgr |
Kenemu (knmw), Crew, is an Egyptian constellation of three stars ρ1 Sgr = 44 Sgr.[1][2] (Stars of) Kenmu, 17th decan in Egyptian astral science, has its heliacal rise in month Peret, represented by a small group of stars around ρ1 Sgr.
Concordance, Etymology, History

Origin of Constellation

Kenemu is the name of a decan (possibly form by several stars as its name indicate, the Crew) of the constellation Wia, The Boat, which is formed by several stars expanding from before the Red of the Prow (Antares) to the end of Sagittarius. It is sailing the Milky Way.

Lull (2018)[1] dedicates an entire research paper to the discussion, cultural embedding and astronomical identification of Wia, The Boat, with Knmw, The Crew. He concludes on the identification of Knmw with the area between the stars ρ1 Sgr (44 Sgr).
Previous Identification: Leitz (1995, 91)[3] reads knm and translates The Dark One, which he interprets as a reference to fainter stars. His identification with λ Aql is refuted by Belmonte and Lull (2023),[2] who also adopt another reading of the original hieroglyphs.
Transfer and Transformation of the Constellation

Religion/ Tales/ Mythology
In ancient Egyptian cosmology, boats carried the sun god Ra, and the deceased pharaoh's soul on its journey through the afterlife. The WjA constellation symbolized these vital spiritual and solar voyages.
Therefore constellation is also engraved on the granite sarcophagus lid of Djehapimu, the Royal Audit Officer and a relative of King Nectanebo II (Nakhthorheb, Nḫt-Ḥr-Ḥbt), c. 346-332 BCE, granite, displayed in the exhibition of the Neues Museum Berlin, Germany.
IAU WGSN star name discussion
The name was proposed to WGSN in 2025. As Kenemu means something as "crew", we are not sure if it would be appropriate for a single star. Juan Belmonte suggests to look for any pair of closing stars or a star which is multiple (not to the naked eye) in the area east of Kaus Australis, as in that case, it may suit. Yet, Belmonte and Lull (2023) and Lull (2018) both identify ρ1 Sgr at 3.93 mag in V.
In 2026, the name "Kenemu" was proposed for the star ρ1 Sgr (Rho1 Sagittarii, 44 Sgr, HR 7340, HD 181577, HIP 95168), a spectral type A9IV star with apparent magnitude V=3.92 that lies 40 parsecs away. The star is a Delta Scuti variable star that varies at the ~0.04 magnitude level on a timescale of ~1.2 hours. The star has a mass approximately 1.9x that of the Sun, and a luminosity of approximately 31x the Sun, placing it about ~1.5 magnitudes brighter than the main sequence, and making it a post-main sequence star.
-
Heryibwia profile card (CC BY M.Sadegh Faghanpour for IAU-WGSN). -
Heryibwia stick figure (CC BY M.Sadegh Faghanpour for IAU-WGSN). -
Babylonian "River Boat" constellation: see Magur. -
Kenemu profile card (CC BY M.Sadegh Faghanpour for IAU-WGSN). -
Kenemu stick figure (CC BY M.Sadegh Faghanpour for IAU-WGSN). -
Qedty profile card (CC BY M.Sadegh Faghanpour for IAU-WGSN). -
Qedty stick figure (CC BY M.Sadegh Faghanpour for IAU-WGSN).
Weblinks
References
- References (general)
- ↑ 1.0 1.1 Lull, José (2018). Ancient Egyptian constellation of WjA (Boat) and its link to Sagittarius in the Ptolemaic and Roman era. Aula Orientalis 36/2, 257-277
- ↑ 2.0 2.1 Belmonte, Juan Antonio and Lull, José (2023). Astronomy of Ancient Egypt - A Cultural Perspective, Springer
- ↑ Leitz, Ch., 1995. Altägyptische Sternuhren. OLA, 62. Leuven: Peeters.







