September 8, 2024
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R3 – Rotation – Simple Examples

Tait-Bryan Angles

This post looks at simple R3 rotations that consist of 90o rotations around a single axis on the unit sphere. A 90^o axis-angle rotation around the x-axis is a z-y-x’’ rotation using the Tait-Bryan angles of φ = 90^o, θ = 0o and ψ= 0o. Rotation of 90^o around the x-axis moves the point Y^ to the location of Z^, and Z^ to Yv. As a result, the xy plane now intersects the YZ plane orthogonally through the y-axis to form the line of nodes called N. φ is the angle between  the N line and the Y-axis which is 90^o. This is the angle through which the Y^ point was rotated around the x-axis.

Unitary R3 Rotations

All the simple rotations looked at are rotations around either the x, y or z-axes and so have only one Tait-Bryan angle of 90o, the others being 0. The Orthogonal Rule from the Axioms of Rotation states that multiplication by a unitary is the equivalent of rotation around the unitary’s axis by 90^o. So, all the simple R3 rotations are the equivalent of multiplying by one of the unitaries  1^, 1v, i^, iv, j^ or jv.

Try out these rotations using the online calculator.

90o Rotations from (1^, 0, 0)

  1. π^/2 ↺z (1^,0, 0) = i^ or in multiplication j^*1^ = i^.
    • The point (1^,0, 0) on the x-axis rotates by  90^o counterclockwise or π^/2 around the z-axis. So, it moves to the point (0, i^,0), or i^ algebraically.
  2. π^/2 ↺y (1^,0, 0) = jv or in multiplication i^*1^ = jv.
    • The point (1^,0, 0) on the x-axis rotates by  90^o or π^/2 around the y-axis. So, it moves to the point (0, 0, jv), or jv algebraically.
  3. π^/2 ↺x (1^,0, 0) = 1^or in multiplication 1^*1^ = 1^.
    • The point (1^,0,0) on the x-axis rotates by  90^o counterclockwise or π^/2 around the x-axis but as the point is already on the x-axis, it stays at the point (1^,0, 0), or 1^ algebraically.
  4. πv/2 ↺z (1^,0, 0) = iv or in multiplication jv*1^ = iv.
    • The point (1^,0, 0) on the x-axis rotates by  90vo clockwise or πv/2 around the z-axis. So, it moves to the point (0, iv, 0), or iv algebraically.
  5. πv/2 ↺y (1^,0, 0) = j^ or in multiplication iv*1^ = j^.
    • The point (1^,0,0) on the x-axis rotates by  90vo clockwise or πv/2 around the y-axis. So, it moves to the point (0, 0, j^), or j^ algebraically.
  6. πv/2 ↺x (1^,0, 0) = 1^ or in multiplication 1v*1^ = 1^.
    • The point (1^,0, 0) on the x-axis rotates by  90vo clockwise or πv/2 around the x-axis but as the point is already on the x-axis, it stays at the point (1^,0, 0), or 1^ algebraically.
  7. πv/2 ↺z (2^,3iv, 4jv) = (3v, 2iv, 4jv) or in multiplication jv * (2^ + 3iv + 4jv) = (3v + 2iv + 4jv).
    • The point (2^,3iv, 4jv) rotates by  90vo clockwise or πv/2 around the z-axis. So, it moves to the point (3v, 2iv, 4jv), or (3v + 2iv + 4jv) algebraically.

Other Possible 90o or π?/2 rotations

Start PointRotationEnd PointAlgebra
    
1(1v,0,0)π^/2↺z(0, iv,0)j^*1v = iv
2(1v,0,0)π^/2↺y(0, 0, j^)i^*1v = j^
3(1v,0,0)π^/2↺x(1v,0,0)1^*1v = 1v
4(1v,0,0)πv/2↺z(0, i^,0)jv*1v = i^
5(1v,0,0)πv/2↺y(0, 0, jv)iv*1v = jv
6(1v,0,0)πv/2↺x(1v, 0, 0)1v*1v = 1v
     
7(0, i^,0)π^/2↺z(1v,0,0)j^*i^ = 1v
8(0, i^,0)π^/2↺y(0, i^,0)i^*i^ = i^
9(0, i^,0)π^/2↺x(0, 0 , j^)1^*i^ = j^
10(0, i^,0)πv/2↺z(1^,0,0)jv*i^ = 1^
11(0, i^,0)πv/2↺y(0, i^,0)iv*i^ = i^
12(0, i^,0)πv/2↺x(0, 0 , jv)1v*i^ = jv
     
13(0, iv,0)π^/2↺z(1^,0,0)j^*iv = 1^
14(0, iv,0)π^/2↺y(0, iv,0)i^*iv = iv
15(0, iv,0)π^/2↺x(0, 0, jv)1^*iv = jv
16(0, iv,0)πv/2↺z(1v,0,0)jv*iv = 1v
17(0, iv,0)πv/2↺y(0, iv,0)iv*iv = iv
18(0, iv,0)πv/2↺x(0, 0, j^)1v*iv = j^
     
19(0, 0, j^)π^/2↺z(0, 0, j^)j^*j^ = j^
20(0, 0, j^)π^/2↺y(1^,0,0)i^*j^ = 1^
21(0, 0, j^)π^/2↺x(0, iv,0)1^*j^ = iv
22(0, 0, j^)πv/2↺z(0, 0, j^)jv*j^ = j^
23(0, 0, j^)πv/2↺y(1v,0,0)iv*j^ = 1v
24(0, 0, j^)πv/2↺x(0, i^,0)1v*j^ = i^
     
25(0, 0, jv)π^/2↺z(0, 0, jv)j^*jv = jv
26(0, 0, jv)π^/2↺y(1v, 0, 0)i^*jv = 1v
27(0, 0, jv)π^/2↺x(0, i^,0)1^*jv = i^
28(0, 0, jv)πv/2↺z(0, 0, jv)jv*jv = jv
29(0, 0, jv)πv/2↺y(1^,0, 0)iv*jv = 1^
30(0, 0, jv)πv/2↺x(0, iv, 0)1v*jv = iv

Next: Multiplication Table

Previous: Euler and Tait-Bryan Angles

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