Tomb of Seti I The tomb of Seti I, also known as KV17, is located in the Valley of the Kings. The pharaoh Seti I died in 1279 BC. His tomb was discovered by the archaeologist and explorer Giovanni Belzoni in 1817. Coordinates 25.740031, 32.601998 Description Seti I had many buildings built, which included the Temple of Seti I in Abydos. The tomb KV17 consists of 17 chambers, corridors, and side rooms and is considered one of the largest. There is a well near the entrance of the tomb; the corridor descends into the tomb and is designed similarly to other tombs. Decorations are found throughout most of the tomb. The tomb and side chambers are on the level of the well, with a further corridor that ends in a room at a lower level. (The measurements used are given in official documents) Total area of tomb: 649.04 sq m / 2373 sq cubits Burial chamber width: 13.19 ft / 25.22 cubits Distance to burial chamber: 290 ft / 88.382 m / 169 cubits Distance to the end of the tomb: 570 ft / 173.74...
Mulfra Quoit
Mulfra Quoit stands on Mulfra Hill to the north of the hamlet of Mulfra, Penzance, Cornwall. It is considered similar to the Chûn Quoit monument, which is located about five kilometres away.
Coordinates
50.163352,-5.569343
Description
The monument is made up of three supporting stones and one much larger capstone.
Although it appears as if the capstone has fallen, it is possible it was built this way. As a building used as a gnomon or winter solstice marker, it is angled lengthwise at 40° toward the northeast and 50° toward the northwest as a gnomon.
Analysis
Mulfra Quoit as a gnomon at 50° would suggest a celestial object, but its gnomon is quite large. The angle off the surface could be suggested as 45°.
It is also possible that it marks a date and rather than being used as a gnomon, it was used so that light would illuminate an inner surface. The date would be when light aligned to reach the inner surface.
When applying the angles to the surface, the following would apply:
Its gnomon entrance would track at 67.5° toward the north or 67.5° + 23.5°, which is 91°.
Although this seems like it aligns with the star Polaris in the constellation Ursa Minor, a building date in the 3rd millennium BCE should be considered. This would give it a 7° tilt. A possible star would then be Epsilon Ursae Minoris.
82° 02′ 14.1233
82.037256°
82.037256 - 89 = 6.962
6.962 ÷ 1.55 = 4.492
4.492 x 1000 = 4492.092
4492.092 - 1985 = 2507 BCE
Conclusion
It has been shown in other articles that the planet currently tilts at 23.256° according to the latest measurements, although 23.5° is also commonly used. It also has a 7.155° tilt to the Sun's equator. If a gnomon were to track an object, it would vary by about 7.155° and trace a looped path. However, this has been shown not to be the case, and the object would instead be measured at variable times throughout the year or align once during its 20° tilt.
If the monument was built recently, as if from land clearing, then it aligns with Polaris. A more likely alignment would be with Epsilon Ursae Minoris in 2507 BCE.
It is also quite wide, so it could be considered centered on the constellation.
Mulfra Quoit (no changes)
Archeology77 ©
Mulfra Quoit stands on Mulfra Hill to the north of the hamlet of Mulfra, Penzance, Cornwall. It is considered similar to the Chûn Quoit monument, which is located about five kilometres away.
Coordinates
50.163352,-5.569343
Description
The monument is made up of three supporting stones and one much larger capstone.
Although it appears as if the capstone has fallen, it is possible it was built this way. As a building used as a gnomon or winter solstice marker, it is angled lengthwise at 40° toward the northeast and 50° toward the northwest as a gnomon.
Analysis
Mulfra Quoit as a gnomon at 50° would suggest a celestial object, but its gnomon is quite large. The angle off the surface could be suggested as 45°.
It is also possible that it marks a date and rather than being used as a gnomon, it was used so that light would illuminate an inner surface. The date would be when light aligned to reach the inner surface.
When applying the angles to the surface, the following would apply:
Its gnomon entrance would track at 67.5° toward the north or 67.5° + 23.5°, which is 91°.
Although this seems like it aligns with the star Polaris in the constellation Ursa Minor, a building date in the 3rd millennium BCE should be considered. This would give it a 7° tilt. A possible star would then be Epsilon Ursae Minoris.
82° 02′ 14.1233
82.037256°
82.037256 - 89 = 6.962
6.962 ÷ 1.55 = 4.492
4.492 x 1000 = 4492.092
4492.092 - 1985 = 2507 BCE
Conclusion
It has been shown in other articles that the planet currently tilts at 23.256° according to the latest measurements, although 23.5° is also commonly used. It also has a 7.155° tilt to the Sun's equator. If a gnomon were to track an object, it would vary by about 7.155° and trace a looped path. However, this has been shown not to be the case, and the object would instead be measured at variable times throughout the year or align once during its 20° tilt.
If the monument was built recently, as if from land clearing, then it aligns with Polaris. A more likely alignment would be with Epsilon Ursae Minoris in 2507 BCE.
It is also quite wide, so it could be considered centered on the constellation.
Mulfra Quoit (no changes)
Archeology77 ©
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