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
- Bartosz Ciechanowskiciechanow.ski
- Diurnal motion - Wikipediaen.wikipedia.org
- The Copernican Revolution from the Insidejacoblagerros.wordpress.com
- GPS – Bartosz Ciechanowskiciechanow.ski
- Bicycle – Bartosz Ciechanowskiciechanow.ski
- Solar time - Wikipediaen.wikipedia.org
- arXiv:gr-qc/0202090v1 26 Feb 2002arxiv.org
- The Structure of Scientific Revolutions - Wikipediaen.wikipedia.org
- How do rockets really get to where they're headed? - Orbital Mechanics — Steemitsteemit.com
- 行星机制及其概念开显-萃嶺网cuilingmag.com
- Mach's principle - Wikipediaen.wikipedia.org