Days & Years
The length of a βdayβ and a βyearβ seem simple, but theyβre surprisingly complex. Multiple definitions exist, and theyβre all interconnected through Earthβs orbital mechanics and precession.
Types of Days
| Type | Definition | Duration | Connected To |
|---|---|---|---|
| Solar Day | Time for Sun to return to same position in sky | ~86,400 seconds | Solar Year |
| Sidereal Day | Time for stars to return to same position (relative to precessing equinox) | ~86,164.09 seconds | Solar Day |
| Stellar Day | Earthβs actual rotation period (relative to fixed stars) | ~86,164.10 seconds | Sidereal 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
Thereβs a small (~8-9 millisecond) difference between the stellar day and sidereal day:
| Measurement | Duration | Source |
|---|---|---|
| Sidereal day | 86,164.0905 seconds | IAU standard |
| Stellar day | 86,164.0989 seconds | Fixed 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 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
| Type | Definition | Duration | What Causes Variation |
|---|---|---|---|
| Solar Year | Solstice to solstice (or equinox to equinox) | ~365.2422 days | Obliquity, axial precession |
| Sidereal Year | Sun returns to same position relative to fixed stars | ~365.2564 days | Fixed |
| Anomalistic Year | Perihelion to perihelion | ~365.2597 days | Perihelion precession |
Why the Sidereal Year is Fixed
The sidereal year is fixed at 31,558,149.724 SI seconds because it measures Earthβs orbit relative to the fixed stars - an unchanging reference frame. Other year types fluctuate because theyβre 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 modelβs 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 Type | Duration | Difference |
|---|---|---|
| Sidereal Year | 31,558,149.724 seconds | β |
| 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 βbehindβ 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 1 sidereal yearThis is why the equinoxes βprecessβ 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 Earthβs orbital motion around the Sun adds one rotation per year.
Applied to Years (The Modelβs 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:
| Measurement | Count per Great Year |
|---|---|
| Solar years | ~25,684 |
| Sidereal years | ~25,683 |
| Difference | Exactly 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.
How the Years Connect
Starting from Earthβs perspective:
- Position 0: Sun and Earth aligned at the start
- After 1 Solar Year (~365.242 days): Sun returns to same seasonal position (Position A)
- 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:
| Property | Value |
|---|---|
| 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 Type | In Seconds | In Days | Depends On |
|---|---|---|---|
| Sidereal Year | Fixed (31,558,149.724 s) | Varies | Eccentricity (affects day count) |
| Solar Year | Varies | Varies | Obliquity (axial tilt) |
| Anomalistic Year | Varies | Varies | Perihelion precession |
The Critical Distinction
The sidereal year in seconds is fixed - itβs 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 secondsThis 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 Earthβs 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.
| Parameter | Current Value | Mean Value |
|---|---|---|
| Solar Day | ~86,400.0003 s | 86,399.989 s |
| Sidereal Day | ~86,164.09 s | 86,164.08 s |
| Stellar Day | ~86,164.10 s | 86,164.09 s |
| Solar Year | ~365.2422 days | 365.2422 days |
| Sidereal Year (seconds) | 31,558,149.724 s | (fixed) |
| Sidereal Year (days) | ~365.2564 days | Varies with eccentricity |
| Anomalistic Year | ~365.2597 days | 365.2597 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
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β COIN ROTATION PARADOX β
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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
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β DAY-YEAR CONNECTIONS β
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β Stellar Day βββββββββΊ Sidereal Year (fixed reference) β
β β β β
β βΌ βΌ β
β ~9.1ms difference ~1,228.7s difference β
β β β β
β βΌ βΌ β
β Sidereal Day ββββββββΊ Solar Year β
β β β β
β βΌ βΌ β
β Axial Precession Perihelion Precession β
β (~25,684 years) (~20,868 years) β
β β β
β βΌ β
β Anomalistic Year β
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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
- Three types of days and years exist, each measuring different reference points
- The sidereal year in seconds is fixed at 31,558,149.724 seconds - itβs the anchor point
- The sidereal year in days varies with eccentricity (day length changes)
- Solar year depends on obliquity - it measures equinox-to-equinox, which shifts with axial tilt
- Day length = sidereal year (seconds) / sidereal year (days) - everything derives from the fixed anchor
- 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
- All values are interconnected through Earthβs orbit around EARTH-WOBBLE-CENTER and PERIHELION-OF-EARTHβs orbit around the Sun
Continue to Invariable Plane to learn about the solar systemβs fundamental reference plane.