What is Precession?
allthescience.org · 434 words · saved by 1 readers
Precession is any alteration in the position of a celestial body's rotation axis. Common examples of precession include...
Any alteration in the position of a celestial body's rotation axis is known as precession. Astronomical bodies naturally feature slow changes in both their rotational rate and orbital status around other gravitationally-strong bodies. Two types of precession exist within the realm of astronomy: torque-free and torque-induced. According to the mathematical principles of torque-free precession, the rotating axis is different from the ellipse of an object. In the case of torque-induced precession, the object maintains an alternating rotation. The most common example of this phenomenon can be…
saved by
related reading
- Foucault pendulum - Wikipediaen.wikipedia.org
- Diurnal motion - Wikipediaen.wikipedia.org
- Bartosz Ciechanowskiciechanow.ski
- The Copernican Revolution from the Insidejacoblagerros.wordpress.com
- Mach's principle - Wikipediaen.wikipedia.org
- GPS – Bartosz Ciechanowskiciechanow.ski
- Hysteresis - Wikipediaen.wikipedia.org
- Solar time - Wikipediaen.wikipedia.org
- Tide - Wikipediaen.wikipedia.org
- N-body problemen.wikipedia.org
- Tautochrone curve - Wikipediaen.wikipedia.org
- Circular Restricted Three-Body Problem — Orbital Mechanics & Astrodynamicsorbital-mechanics.space