reply to post by fraterormus
I am aware of this but precession of the equinox is irrelevant to Earth's plane of the ecliptic. The orbital plane for Earth and all the other
planets in our solar system remain the same overall. The orbits of the planets are titled (orbit inclination) and eccentric, I am also aware that the
respective orbit nodes and perihelions change as well. None of these motions, however, effect our edge on tilt of 60 degrees to the Milky Way.
There are other motions underway that could effect this alignment, like our galactic rotation or stellar oscillations but I don't know if it changes.
My guess is that it does change as we rotate around the galactic center and this edge on alignment happens twice for every galactic orbit, once on
each side.
Earth's axis is tilted to the ecliptic (orbital path around the Sun) by around 23.5 degrees. Precession is the slow circular motion of the Earth's
axis that advances our alignment by around 1 degree every 72 years. Every tropical year for Earth (equinox to equinox) comes about 50.3 arc seconds
early due to the slow circular motion of the axis. A sidereal year is actually a little bit longer than what we consider an Earth year, Earth has more
than one length for a year.
Tropical (equinox to equinox)----------------365.2421897 days
Sidereal (fixed star to fixed star)------------365.256365741 days
Anomalistic (perihelion to perihelion)--------365.259641204 days
Eclipse (Moon's node to Moon's node)-------346.620046296 days
Gaussian (Kepler's law for a = 1)------------365.2569 days
Julian (based on Julian calendar)-------------364.25 days
Gregorian (based on Gregorian calendar)---365.2425 days
[edit on 10/9/2009 by Devino]