Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Euler angles
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
==Properties== {{See also|Charts on SO(3)|Quaternions and spatial rotation}} The Euler angles form a [[chart (topology)|chart]] on all of [[SO(3)]], the [[special orthogonal group]] of rotations in 3D space. The chart is smooth except for a polar coordinate style singularity along {{Nowrap|1=''Ξ²'' = 0}}. See [[charts on SO(3)]] for a more complete treatment. The space of rotations is called in general "The [[Quaternions and spatial rotation#Quaternion rotation operations|Hypersphere of rotations]]", though this is a misnomer: the group [[Spin group|Spin(3)]] is [[isometric embedding|isometric]] to the hypersphere ''S''<sup>3</sup>, but the rotation space SO(3) is instead isometric to the [[real projective space]] '''RP'''<sup>3</sup> which is a 2-fold [[Quotient space (topology)|quotient space]] of the hypersphere. This 2-to-1 ambiguity is the mathematical origin of [[Spin (physics)|spin in physics]]. A similar three angle decomposition applies to [[SU(2)]], the [[special unitary group]] of rotations in complex 2D space, with the difference that ''Ξ²'' ranges from 0 to 2{{pi}}. These are also called Euler angles. The [[Haar measure]] for SO(3) in Euler angles is given by the Hopf angle parametrisation of SO(3), <math>\textrm{d}V \propto \sin \beta \cdot \textrm{d}\alpha \cdot \textrm{d}\beta \cdot \textrm{d}\gamma</math>,<ref>{{cite journal|at=Section 8 β Derivation of Hopf parametrisation |pmc=2896220 |year=2010 |last1=Yershova |first1=A. |last2=Jain |first2=S. |last3=Lavalle |first3=S. M. |last4=Mitchell |first4=J. C. |title=Generating Uniform Incremental Grids on SO(3) Using the Hopf Fibration |journal=The International Journal of Robotics Research |volume=29 |issue=7 |doi=10.1177/0278364909352700 |pmid=20607113 }}</ref> where <math>(\beta, \alpha)</math> parametrise <math>S^{2}</math>, the space of rotation axes. For example, to generate uniformly randomized orientations, let ''Ξ±'' and ''Ξ³'' be uniform from 0 to 2{{pi}}, let ''z'' be uniform from −1 to 1, and let {{nowrap|1=''Ξ²'' = arccos(''z'')}}. ===Geometric algebra=== Other properties of Euler angles and rotations in general can be found from the [[geometric algebra]], a higher level abstraction, in which the quaternions are an even subalgebra. The principal tool in geometric algebra is the rotor <math> \mathbf{R} = [ \cos(\theta / 2) - I u \sin(\theta / 2) ] </math> where <math>\theta =</math>[[angle of rotation]], <math>\mathbf{u} </math> is the rotation axis (unitary vector) and <math>\mathbf{I}</math> is the pseudoscalar (trivector in <math>\mathbb{R}^3</math>) ===Higher dimensions=== It is possible to define parameters analogous to the Euler angles in dimensions higher than three.<ref>{{Citation |last = Hoffman |first = D. K. |title = Generalization of Euler Angles to N-Dimensional Orthogonal Matrices |journal = Journal of Mathematical Physics |publisher = [J. Math. Phys. 13, 528β533] |year = 1972 |volume = 13 |issue = 4 |pages = 528β533 |doi = 10.1063/1.1666011 |bibcode = 1972JMP....13..528H |url = https://pubs.aip.org/aip/jmp/article/13/4/528/440286/Generalization-of-Euler-Angles-to-N-Dimensional |url-access = subscription}}</ref> <ref>{{in lang|it}} [http://ansi.altervista.org A generalization of Euler Angles to ''n''-dimensional real spaces]</ref>{{unreliable source?|date=December 2022}} In four dimensions and above, the concept of "rotation about an axis" loses meaning and instead becomes "rotation in a plane." The number of Euler angles needed to represent the group {{math|SO(''n'')}} is {{math|''n''(''n'' β 1)/2}}, equal to the number of planes containing two distinct coordinate axes in ''n''-dimensional Euclidean space. In [[SO(4)]] a rotation matrix [[Rotation (mathematics)#In four dimensions|is defined by two unit quaternions]], and therefore has six degrees of freedom, three from each quaternion.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)