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The ModelDays & Years

Days & Years

The length of a β€œday” and a β€œyear” seem simple, but they’re surprisingly complex. Multiple definitions exist, and they’re all interconnected through Earth’s orbital mechanics and precession.


Types of Days

TypeDefinitionDurationConnected To
Solar DayTime for Sun to return to same position in sky~86,400 secondsSolar Year
Sidereal DayTime for stars to return to same position (relative to precessing equinox)~86,164.09 secondsSolar Day
Stellar DayEarth’s actual rotation period (relative to fixed stars)~86,164.10 secondsSidereal Year

Why Solar Day is Longer

A solar day is ~4 minutes longer than a sidereal day because Earth moves along its orbit while rotating. After one full rotation relative to the stars, Earth must rotate a bit more for the Sun to return to the same position.

The 8-9 Millisecond Difference

There’s a small (~8-9 millisecond) difference between the stellar day and sidereal day:

MeasurementDurationSource
Sidereal day86,164.0905 secondsIAU standard
Stellar day86,164.0989 secondsFixed star reference
Difference~8.4 milliseconds

This difference has been debated for decades without official scientific consensus. The model proposes that this difference is caused by axial precession: as Earth wobbles on its axis over ~25,684 years, the reference point for the sidereal day (the precessing equinox) shifts slightly each day relative to the fixed stars.

The connection: 8.4 milliseconds per day Γ— 365.25 days β‰ˆ 3,068 seconds per year. This relates to the ~1,224.5 second difference between solar and sidereal years through the precession mechanics.


Types of Years

TypeDefinitionDurationWhat Causes Variation
Solar YearSolstice to solstice (or equinox to equinox)~365.2422 daysObliquity, axial precession
Sidereal YearSun returns to same position relative to fixed stars~365.2564 daysFixed
Anomalistic YearPerihelion to perihelion~365.2597 daysPerihelion precession

Why the Sidereal Year is Fixed

The sidereal year is fixed at 31,558,149.724 SI seconds because it measures Earth’s orbit relative to the fixed stars - an unchanging reference frame. Other year types fluctuate because they’re measured relative to moving reference points:

  • Solar year: Measured from equinox to equinox, but the equinox position shifts due to axial precession
  • Anomalistic year: Measured from perihelion to perihelion, but perihelion shifts due to perihelion precession

The sidereal year is the model’s anchor point from which other values are derived.


The Difference Between Solar and Sidereal Years

The solar year is ~1,224.5 seconds shorter than the sidereal year. This difference is the source of axial precession.

Year TypeDurationDifference
Sidereal Year31,558,149.724 secondsβ€”
Solar Year~31,556,925.2 seconds~1,224.5 seconds shorter

In our current epoch every year, the Sun appears ~1,224.5 seconds β€œbehind” its previous position relative to the fixed stars when measured at the equinox. Over ~25,684 years, this accumulates to a full 360Β° shift - one complete precession cycle.

~1,224.5 seconds/year Γ— ~25,772 years = 31,558,149.724 seconds β‰ˆ 1 sidereal year

This is why the equinoxes β€œprecess” through the zodiac constellations.


The Coin Rotation Paradox

The coin rotation paradoxΒ  is key to understanding these relationships:

When a coin rolls around another coin of equal size, it rotates twice - once for the orbit, plus once for its own rotation.

Applied to Days

In one year, Earth rotates:

  • ~365.25 solar days (rotations relative to the Sun)
  • ~366.25 sidereal days (rotations relative to the stars)

The difference is exactly 1 extra rotation - because Earth’s orbital motion around the Sun adds one rotation per year.

Diagram showing the coin rotation paradox at the start of the Great Year, illustrating how Earth's orbital motion adds one extra sidereal day per year

Applied to Years (The Model’s Insight)

The same paradox applies to the Great Year:

  • Earth orbits the EARTH-WOBBLE-CENTER clockwise over ~25,684 years
  • The PERIHELION-OF-EARTH orbits the Sun counter-clockwise over ~111,296 years

Because these motions are in opposite directions, the coin rotation paradox works in reverse:

MeasurementCount per Great Year
Solar years~25,684
Sidereal years~25,683
DifferenceExactly 1 less

Just as there is exactly 1 more sidereal day than solar days per year, there is exactly 1 fewer sidereal year than solar years per Great Year.

End of Great Year cycle showing 1 fewer sidereal year

How the Years Connect

Diagram showing relationship between different year types

Starting from Earth’s perspective:

  1. Position 0: Sun and Earth aligned at the start
  2. After 1 Solar Year (~365.242 days): Sun returns to same seasonal position (Position A)
  3. After 1 Sidereal Year (~365.256 days): Sun aligns with the same fixed star again (Position B)

The angular difference between A and B is the annual precession shift (~50 arcseconds/year).


The Anomalistic Year

The anomalistic year measures the time from perihelion to perihelion:

PropertyValue
Current duration~365.2597 days
Difference from solar year~25 minutes longer
Perihelion date shift~1 day every 57 years
Full cycle (perihelion precession)~20,868 years

The anomalistic year is longer because perihelion shifts forward in time due to perihelion precession.


What Each Year Type Depends On

This is a key insight of the model: each year type depends on different orbital parameters.

Year TypeIn SecondsIn DaysDepends On
Sidereal YearFixed (31,558,149.724 s)VariesEccentricity (affects day count)
Solar YearVariesVariesObliquity (axial tilt)
Anomalistic YearVariesVariesPerihelion precession

The Critical Distinction

The sidereal year in seconds is fixed - it’s the time for Earth to complete one orbit relative to the fixed stars. This never changes.

But the sidereal year in days varies with eccentricity:

Sidereal Year (days) = Sidereal Year (seconds) / Day Length (seconds)

As eccentricity changes over the 20,868-year cycle, day length changes, which changes how many days fit into the fixed number of seconds.

The Day Length Formula

From the fixed sidereal year, we can derive day length:

Day Length = Sidereal Year (seconds) / Sidereal Year (days) = 31,558,149.724 s / 365.256363 days = 86,400.002 seconds

This connects everything: the sidereal year in seconds is the anchor, and all other time measurements are derived from it.

Why Solar Year Depends on Obliquity

The solar year measures equinox-to-equinox (or solstice-to-solstice). These points are defined by Earth’s axial tilt relative to its orbit. As obliquity changes over the 41,736-year cycle, the exact timing of equinoxes shifts slightly, affecting the solar year length.


Current vs Mean Values

The model proposes that all measurements have mean (average) values over the full precession cycles. Current values fluctuate around these means.

ParameterCurrent ValueMean Value
Solar Day~86,400.0003 s86,399.989 s
Sidereal Day~86,164.09 s86,164.08 s
Stellar Day~86,164.10 s86,164.09 s
Solar Year~365.2422 days365.2422 days
Sidereal Year (seconds)31,558,149.724 s(fixed)
Sidereal Year (days)~365.2564 daysVaries with eccentricity
Anomalistic Year~365.2597 days365.2597 days

The sidereal year in seconds is fixed. The sidereal year in days varies because day length depends on eccentricity. All other values fluctuate within each precession cycle.


Summary: How Everything Connects

β”Œβ”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β” β”‚ COIN ROTATION PARADOX β”‚ β”œβ”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€ β”‚ 366.25 sidereal days = 365.25 solar days (1 more rotation) β”‚ β”‚ 25,683 sidereal years = 25,684 solar years (1 fewer orbit) β”‚ β””β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”˜ β”‚ β–Ό β”Œβ”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β” β”‚ DAY-YEAR CONNECTIONS β”‚ β”œβ”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€ β”‚ Stellar Day ────────► Sidereal Year (fixed reference) β”‚ β”‚ β”‚ β”‚ β”‚ β”‚ β–Ό β–Ό β”‚ β”‚ ~9.1ms difference ~1,228.7s difference β”‚ β”‚ β”‚ β”‚ β”‚ β”‚ β–Ό β–Ό β”‚ β”‚ Sidereal Day ───────► Solar Year β”‚ β”‚ β”‚ β”‚ β”‚ β”‚ β–Ό β–Ό β”‚ β”‚ Axial Precession Perihelion Precession β”‚ β”‚ (~25,684 years) (~20,868 years) β”‚ β”‚ β”‚ β”‚ β”‚ β–Ό β”‚ β”‚ Anomalistic Year β”‚ β””β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”€β”˜

Calculate Day & Year Lengths at Any Year

To calculate solar year, sidereal year, day length, and precession durations for any year, see the Formulas page which provides the complete Excel formulas.


Key Takeaways

  1. Three types of days and years exist, each measuring different reference points
  2. The sidereal year in seconds is fixed at 31,558,149.724 seconds - it’s the anchor point
  3. The sidereal year in days varies with eccentricity (day length changes)
  4. Solar year depends on obliquity - it measures equinox-to-equinox, which shifts with axial tilt
  5. Day length = sidereal year (seconds) / sidereal year (days) - everything derives from the fixed anchor
  6. The coin rotation paradox explains why counts differ by exactly 1:
    • 366.25 sidereal days = 365.25 solar days per year
    • 25,683 sidereal years = 25,684 solar years per Great Year
  7. All values are interconnected through Earth’s orbit around EARTH-WOBBLE-CENTER and PERIHELION-OF-EARTH’s orbit around the Sun

Continue to Invariable Plane to learn about the solar system’s fundamental reference plane.

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