For 4 millennia, the Great Pyramid of Cheops has been an architectural feat, with the hollowing of its faces in their middle. It is a silent message that has not been deciphered yet; this article will aim to do it.
The Great Step Pyramid of Djoser, at Saqqara, was already an achievement to build as it was the first gigantic pyramid ever built but being a step pyramid made it easy to properly erect the summit; from one step to the next, builders could rectify any drift in the orientation of the lower step without that being noticed once the construction finished.
From Meidum, builders took up a much more difficult challenge; not only were the pyramids bigger (100 meters, or 328.08 feet, high against 60 meters, or 196.85 feet, at Saqqara), but also the sharp edges had to be perfect straight lines and faultlessly oriented from the start to ensure that the four sides will all precisely meet at the summit, only visible at the very end of the construction. Any default in the construction would be as plain as the nose on one’s face, and moreover, it could not be rectified. But it is clear that all these great pyramids have perfect geometry, such as an almost perfect North-South orientation, which is proof that this issue has been brilliantly resolved.
This could not have been possible without precise measurement and survey tools compatible with the gigantic size of these pyramids to guarantee throughout the construction the perfect orientation of the pyramid and its faces toward the virtual summit and to rectify any occasional drifts in time.
This article will intend to explain the method of measurement that would have enabled builders to take on the challenge with the help of Ra, the guardian God of Ancient Egypt.
Orientation from circumpolar stars?
Every author has noticed the perfect North-South orientation of the six Great Pyramids, with smooth faces. Some authors have thought that the builders used the North Star at that millennia, Thuban, whose brightness is fragile though, for the orientation (2.5 times less bright than our current North Star), either by using it directly or by using its vertical alignment with two other nearby brighter stars, such as Mizar and Pherkad.
However, this hypothesis has several major weaknesses which, in my view, are disqualifying in view of the extreme precision obtained.
At the alleged time of construction, no stars marked the true North; the closest was Thuban, which circled a 9′ arc radius. The northern passage of these stars was therefore a transition that required two things: a prior measurement to determine the moment of northern passage and an association with a reference point in the sky, such as the vertical alignment of Mizar and Pherkad with Thuban, which deviated a little from true north. Therefore, the referential was a moving point that could only be used for a short period of time.
Because of the axial precession, the azimuth of these stars has changed over time, not to mention that the Egyptian chronology of the ancient empire is poorly established and differs by several centuries depending on the author. It is therefore risky to associate the orientation of a pyramid with a star.
Thuban shines dully, making it difficult to spot, so using it for angular measurements (sights) required dark nights. In addition, taking sight requires that it be done at a height of 30°, but there would remain the issue of adapting them on Earth, on a horizontal surface, and over a distance of approximately 200 m (656.16 ft.) on a perfectly dark night.
Assuming that the North-South axis could have been given from the stars, what about the East-West axis?
Orientation from the Sun
On the other hand, using the Sun was quite the opposite, and I will demonstrate how it could have intelligently been used, not only to orient the pyramid from the start, but also to monitor the alignment of the edges and the faces throughout the construction.
The Sun could be used to determine both axes, North-South and East-West, with great accuracy, provided the right method was used.
However, it should be well known that these axes remain nonetheless virtual because they are defined by the daily position of the Sun at its zenith for the South, but what about the East?
To determine the East direction, it should be understood that the Sun’s azimuth as its rising on an equinox day, does not precisely indicate the East as, every four years, the calendar takes an additional day. As a result, from one year to the next, the East shifts by 1/4 of a day (and so by a degree), and the accumulation of this drift over the years could reach one degree, but the accuracy of the pyramid’s orientation is within 3 minutes of arc. So another method had to be found.
The other reference point that could have been used to orientate the pyramids is the Sun’s azimuth at its zenith, but unfortunately, at this point, the sun’s trajectory is horizontal, making it impossible to determine the precise position by direct observation of its height. An indirect method was therefore required, unless a precise “mechanical” clock was available to determine solar noon, of which we have no proof in those days.
The ancient Egyptians therefore found a way of accurately determining solar noon, as evidenced by the Great Pyramid with its eight faces, and I’m about to show how. But in the meantime, I’d like to take stock of the ancient Egyptians’ degree of competence in measuring time.
Measuring time:
To determine the succession of days, the Egyptians of that period had no less than 3 calendars at their disposal: the civil or “vague” calendar, the ” scholar” or Sothiac calendar and the lunar calendar.
These calendars divided time into years, seasons, months, decades and days with a relentless precision that I won’t dwell on, but thanks to which it was impossible for them to lose a day even over millennia.
On the other hand, we know very little about the measurement of time during the day, other than that it was divided into 12 hours of daylight and 12 hours of night, but what about the measurement of the hour?
We did find the Clepsydra of Karnak, dating from Amenhotep III, whose regularly spaced subdivisions divided the night between 12 and 14 hours, depending on the month of the year, which suggests that they considered the hour to be of a fixed length.
Two or three rather “rustic” sundials have been found to measure the time during the day, so we can assume that the pyramid builders – and this was the least of their duties to Ra – knew how to design a sundial.
But these objects are far too imprecise to meet the specific needs of the pyramid builders. On the other hand, we can assume that they would have been able to design a specialized, ultra-precise sundial to meet their construction needs.
Turn the interaction of a scale model of the pyramid and the Sun into a compass and a clock:
For this purpose, I’m going to speculate that they could have built a reduced-scale wooden model of the pyramid, perhaps 1/28, to use as a sort of compass + sun clock combination.
By placing it on a perfectly level and horizontal terrace, and orienting NS as best they could to begin with, they would have had plenty of time, well in advance of starting work, to observe over the course of a year or even several, the play of light and shadow that the Sun made on the faces of this mini-pyramid.
From this observation, they were able to derive particular events, enabling them first to adjust the orientation of the model with near-absolute precision, and then to use it as a clock that gave, at certain times and on certain days of the year only, but unequivocally and with great precision, a visual signal giving the starting signal to take action, but not only for the orientation of the pyramid to be built, which only happens once, but also enabling them to check regularly that the pyramid was indeed rising straight towards its summit, which would remain invisible until the last day.
Analyzing the Sun’s light on the faces:

Every day of the year, the east, south and west faces go from shadow to sunlight within a variable time period. The North face, on the other hand, only emerges from shadow for a certain period of the year.
The phenomena described below have been repeated endlessly for millennia, and are visible to all. Thousands of visitors have stood before this pyramid, some of them seeing it every day, but apart from a vague mention here and there of the phenomenon often referred to as “lightning”, no one has yet described precisely what happens or what use the builders might have made of it.
We’re going to analyze the evolution of the shadow of the 4 NE, NW, SE and SW edges on the eight half-sides, observing the effect of the sun’s rays rotating around each edge.
In its daily course, the sun passes from West to East, taking an azimuth measured from North, i.e., 90° for East to 270° for West, passing through 180° for South. Its height on the horizon varies from zero at sunrise and sunset to a variable maximum every day as it passes over the zenith, with a maximum at the summer solstice and a minimum at the winter solstice, between around 83° and 36° at that time.
To illuminate a face, a ray of sunlight must shine on it with what I’ll call a positive incidence, whereas it is negative when the face is in the shadow of its edges. There is therefore, except at sunrise and sunset, a moment when the sun’s light shines on the half-faces, and it’s this moment that I’m going to study in detail in what follows.
The common case is therefore the moment when, for a given azimuth, the sun’s height equals and then exceeds the slope of the half-face, i.e., its illumination, and then falls below it, i.e., its transition to shadow. To describe this interaction properly, I’m going to start on any day of the year when all the pyramid’s faces will successively go from shadow to light, and vice versa.
https://videopress.com/v/CNt6s9Cj?preloadContent=metadata
Then, for the East, West and North faces, I’ll describe a special day that occurs only twice a year, giving the exact position of the Sun, due East, due West or due South…
On a graph, I’ll plot the slope of a straight line drawn on the half-face from a point on the edge of this half-face and/or the opposite half-face, having the same azimuth as that of the sun in its course, so that I can compare this slope with the height of the Sun.
The East face is passing into shadow:
As soon as the sun rises, it illuminates this face, and we’re going to examine how it passes into shadow.
On the graph below, we can see how the sun’s height varies with the hours for 4 particular days: the summer and winter solstices, any day close to the spring equinox, and finally the day when the sun passes due west with a height very close to 52.1°, which is the slope of the median line of the pyramid’s faces.

From noon to a given hour, a ray of sunlight passing over the ES edge meets the slope of this half-face, which increases as the sun moves westwards while its height decreases.
When the slope of the half-face is steeper than the height of the sun, the shadow of the edge covers it.
Let’s take the sun’s path on 05-04 (yellow curve): the East face is still entirely exposed to the Sun; at around 3:15 pm, the Sun’s height becomes equal to, then less than, the slope of the ES half-face, so the shadow of the ES ridge immediately covers the entire half-face.
However, at this moment, the slope of the other half-side EN is still slightly lower than the height of the sun, so the shadow of the ES edge sweeps across this half-side on its way from the EN edge to the median, and once this is reached, the East face is completely in shadow.
Because of the abrupt transition from light to shadow on the ES half-face, this phenomenon has been referred to as “lightning”, although the time taken to sweep the opposite half-face is of the order of a minute, slower when the Sun is low (around 2 min), and faster around the summer solstice (around 30 sec).
During the time it is swept by the shadow of the edge, the light is grazing, highlighting any defects in flatness and slope.
There are only two days in the year, around 15 days before and after the summer solstice, when at precisely 6 p.m. the Sun is due east at a height of just over 52.1° and the shadow of the ES edge, after having covered the ES half-face, no longer meets the EN half-face. A moment later, the shadow of the EN edge suddenly covers this half-face.
https://videopress.com/v/jxEsUcKD?preloadContent=metadata
This sudden event signals the right moment to exploit the Sun’s shadow, which is then exactly due West, to trace a perfectly aligned East-West axis.
Before that day, the shadow of the EN edge will first cover the EN half-side, then sweep across the ES half-side before covering it completely.
https://videopress.com/v/ptC5vmpT?preloadContent=metadata
Ultimately, the sun’s passage due west is an event “phoned in” in advance as the days go by, with an increasingly rapid sweep of the EN half-face, followed by a simultaneous “extinction” of both half-faces.
However, the sun’s ” due west ” was in relation to the scale model of the pyramid, which had been oriented “as best as possible ” using the north face a few months earlier. To be sure that this corresponded to a ” true ” due west of the sun, we had to observe the exactly symmetrical phenomenon on the west face 12 hours earlier, which translated into illumination rather than the face passing into shadow; if this were not the case, the scale model’s orientation would have to be rectified.
This symmetry could be precisely assessed on the days preceding the ” due west “, because then the sweep times of the face opposite the edge had to be exactly identical on the east and west faces, which was easy to measure over a duration of the order of a minute.
Illumination of the West face:
The West face illuminates symmetrically to the East face and goes out as the sun sets, whereas it used to be illuminated in the morning.
Before noon, as the Sun moves westward, its azimuth and height increase, while the slope of the west face decreases for the same azimuth.

Example of an “ordinary” sunny day 20 days before the equinox (blue curve):
At around 8:30 a.m., when the sun’s height exceeds the slope of the ON half-side, the shadow of the OS edge that covered it moves towards the median, gradually illuminating the ON half-side with a grazing light over a period of around 2 minutes. At the end of this movement, the sun’s height reaches the slope of the OS half-side, which is then suddenly illuminated in its entirety.
https://videopress.com/v/9XBailkj?preloadContent=metadata
Example when Sun is “due East”:
On the same day that the East face marks the Sun as “due West” by this face passing suddenly into the shadow, the symmetrical phenomenon occurs with the Sun being “due east”. When its height reaches 52.1° at around 6 a.m, the ON half-side suddenly lights up, followed a moment later by the OS half-side.
https://videopress.com/v/O8bGQTQS?preloadContent=metadata
As with the East face, this “full East” position of the sun is in relation to the model of the pyramid, so we trace the shadow of the same plumb line, which may be at an angle to the first trace. By taking the bisector of this angle, we obtain the true East-West axis, which will be used, if necessary, to rectify the orientation of the scale model before its next passage in about a month’s time.
So, on the same day, the builders had two very precise visual cues to take advantage of the full west and full east orientation of the sun to first orient the model exactly and directly on the east-west axis, i.e., precisely but indirectly north-south.
South Face:
From the winter solstice to the equinoxes, this face remains illuminated from morning to evening; from the equinoxes to the summer solstice, we have to wait until after sunrise that the sun reaches a height equal to the slope of the south face, which happens for a variable azimuth depending on the day, which is represented on the diagram below for the summer solstice and an ordinary day limiting ourselves to the SE half-face.

When, on a given day, the height of the sun reaches the slope of the south face, the shadow of the SE edge of the SW half-face gradually moves towards the median of the face in about one minute, at which point the SE half-face is suddenly and totally illuminated.
12 hours later, the opposite phenomenon occurs, with the SW half-face suddenly and totally shaded by the SW edge, which then moves onto the SE half-face to cover it in about one minute.
Thus, for the East, South and West faces, every day between the equinoxes and the summer solstice, from sunrise to sunset, we can observe this phenomenon of illumination and shading of the faces, which, thanks to the hollowing of the faces, lasts for some time, during which the EN, SE, SW, WN half-faces remain in low-angled light long enough to inspect the flatness and slope.
The North face “engulfs” its shadow:
Starting from the winter solstice, when the north face is in shadow all day, there is one day in the year when the sun is at its zenith, with a height slightly exceeding the slope of the north face at its median 52. 1° begins to illuminate this face in low-angled light. At the time of construction, this day was situated around two decans before the vernal equinox and had its symmetrical counterpart two decans after the autumnal equinox, opening up a very short window of time during which the effects of shadow could be used to determine the sun’s passage to zenith with great precision.
To illustrate how this works, I’ve chosen the appropriate date in the year 2479 BC, which, according to some authors, could have been the starting year for the construction of the Great Pyramid.
In fact, the exact year doesn’t matter; changing the year only changes the day of the event. For example, this phenomenon will be observable on February 28, 2021, in the Julian calendar, i.e., March 13 in our calendar. However, the deterioration of the north face may slightly reduce the precision of the phenomenon.
The times given below are solar times.
To analyze the Sun’s effect on this north face, we need to consider the two half-faces, NE and NW, and analyze the Sun’s effect on each half-face.

On this particular day, at around 10 a.m., the Sun’s rays, rotating around the NW and NE edges, reach a height that a moment later equals the slope of the NW half-face, whereas for this azimuth, the NE half-face is steeper, and the NW face is suddenly illuminated (point A). Some time later, at around 10:35 a.m., the sun’s height exceeds the slope of the NE half-face, which in turn is suddenly illuminated.
As the Sun continues its course, reaching its zenith, its height falls below the slope of the NW half-face (point B), which suddenly falls into the shadow of the NW edge. Some time later, at around 2.05 p.m., the NE half-face falls into the shadow of the NE edge.
https://videopress.com/v/B4fbk3JY?preloadContent=metadata
As the graph shows, the duration of this phenomenon depends on the height difference between the Sun at its zenith and the 51.2° slope of the median. Whereas for the East and West faces, the phenomenon lasts only a short time.
From one day to the next, the Sun’s height at zenith varies by 0.37° of arc, which represents 45 minutes of sun movement. Therefore, for the sake of precision, it was crucial to be able to vary the model’s slope slightly by tilting it NS on its base, so that for the daytime sun, the slope of the rectified north face would be only slightly less than the Sun’s height.
We can imagine that there must have been a certain amount of trial and error involved in making this adjustment, and that this work on the scale model must have taken place well before construction began.
Nevertheless, although adjusted, the time between illumination and extinction of the north face could not have been less than a few minutes.
To obtain the precise zenith passage, it was therefore necessary to mark the shadow of a plumb line on the platform at point B and to mark the new shadow at point C, probably using a clepsydra to count the time between these two passages. Ultimately, the median of the two plots and the half-time of the count gave the precise NS axis, as well as the moment when the Sun’s south-facing shadow could be exploited.
After this measurement, if necessary, the orientation of the pyramid scale model could be rectified thanks to the NS axis traced on the platform.
One minute of arc equals to a sun passage of 4 seconds, so time counting over a few minutes had to be accurate to the nearest second – a far cry from the precision of Swiss chronometers – and it’s likely that a clepsydra would have done the trick for this short duration.
We now fully understand the mute “message” of the hollowed median, which is to create a predictable visual effect on certain days – a kind of lightning, instantaneous and significant, observable by all—which marks unequivocally and precisely the passage of the sun due south as well as due east and west.
It’s possible that this 8-face scale model was developed for the pyramids preceding Cheops, but that the builders at the time didn’t see fit to leave any trace of it on the actual pyramid, so as not to complicate the already immense task of building a gigantic, perfect pyramid.
Precision of the method:
It took at least one year with 5 days of measurement, and perhaps one or two more inclining the model slightly, to obtain a “perfect” orientation of the pyramid model.
If, at the end of this year, the result obtained on the last day was not satisfactory, the builders have to wait for the following year to start the operation again to reach the perfection that would enable the exact orientation tops to be given for the base of the pyramid when the time came.
However, the sun is not a punctual source of light but a disc whose apparent size is half a degree of arc, or a passage time of 120 sec.
In the above method, it was not the center of the sun, but the middle of the NW or NE quarter of the periphery of the solar disk that first lit up or extinguished a face. Since both shadows were symmetrical, the bisector indicated the exact NS orientation of the sun’s axis.
Depending on the method used by the builders to align the base of the pyramid with the Sun, for the sake of precision, they had to make a time correction to take account of any offset caused by the method used. They had to be fast: every 4 seconds, the sun drifted by one minute of arc.
This may explain why the alignment “error” between the 6 great smooth-sided pyramids ranged from 3 to 20 arc minutes, which could have been the consequence of varying speeds in exploiting the sun’s shadow.
Orienting the base of the future pyramid:
The SE angle could have served as the starting point, as the Sun’s shadow from there pointed towards the NE angle at noon and SW at 8 o’clock.
While we’ll probably never know the exact method they used to make such an alignment, I’ll simply suggest one that combines simplicity with accuracy and is fully compatible with the technology of the time.
They could have used the shadow cast by a plumb bob suspended from a tripod a few meters high, leaving a shadow on the ground whose exact direction is NS at noon, and EO at 8 o’clock.
But since this shadow is only a few meters long, whereas the distance to be covered was 440 cubits, they could have aligned several of these tripods along one side, connected by a cord, giving a perfectly straight shadow on the ground, which would have covered the shadows cast by the plumb bobs connecting them. Such a cast shadow is centered on the center of the solar disc.
Workers could have prepositioned this device to a satisfactory approximation using an “ordinary” estimate of solar noon and 8 o’clock, then used the five days of year zero from the start of construction to rectify the alignment with the ultra-precise signal given by the model. If the result hadn’t been satisfactory, they would have had to wait for the following year to start again.
Surveying the faces and edges during the construction:
While these faces were being illuminated with low-angled light, it was possible for the builders to ensure that the slope of the faces under construction was identical to that of the scale model based on its lighting. On the pyramid under construction, on the same day at the same time, the faces had to be lit or darkened at the same time as on the scale model.
However, even though the grazing light highlights any defects in flatness, this phenomenon had a limit because the shadow cast by an edge could only partially sweep a half-side when that edge was also partially completed. For the rest of the half-face, builders had to make do with the short time provided by the sun’s grazing light.
The builders only had short periods of time in which to carry out these checks, which could nevertheless be carried out over many days of the year.
Pointed at the top of the model, the builders could have left a plumb line, which, by projecting its shadow, gave the exact azimuth of the sun, thus enabling them to check the direction of the edges on the pyramid under construction, again using a plumb line, particularly for azimuths 135° and 225°, where this shadow fell on the NW and NE edges.
As a conclusion, thanks to the model and the Sun, the pyramid was perfectly oriented from the very start, with its faces and edges pointing exactly towards the summit, which would remain virtual until the very last day!