Orbital parameters
Three slow clocks behind every seasonal cycle
- Eccentricity
- 0.01670
- Obliquity
- 23.439°
- Longitude of perihelion ϖ (heliocentric)
- 102.9°
- Climatic precession e·sin ϖ̃
- -0.0163
- Perihelion date*
- 3 Jan
- Sun's longitude at perihelion
- 282.9°
Season lengths (Kepler's second law)
- NH spring92.8 d
- NH summer93.6 d
- NH autumn89.8 d
- NH winter89.0 d
*Calendar anchored to the March equinox on its modern date, the usual palaeoclimate convention. The unequal season lengths come from eccentricity alone: with a circular orbit every season would last 91.3 days.
La2004 orbital elements, 0–1000 ka
The vertical line marks the selected epoch
Eccentricity
Obliquity (°)
Climatic precession e·sin ϖ̃
65°N June-solstice insolation (W m⁻²)
Age (ka BP)
Conventions, stated once
La2004 distributes ϖ as the heliocentric longitude of perihelion measured from the moving equinox (102.9° today). The Sun's apparent longitude at perihelion is ϖ + 180°. The analysis pins this convention with a test: the present-day elements must place perihelion in early January, and an off-by-π error would place it in July.
Time runs as ka BP, thousands of years before 1950, positive into the past. La2004 stores it as negative kyr; the loader negates it and asserts the present-day elements (e = 0.01670, ε = 23.439°, ϖ = 102.92°) before any analysis proceeds.