Full Pinhole Camera Projection
Project a 3D world point onto 2D image coordinates using the full pinhole camera model with both intrinsic and extrinsic parameters.
The full projection is:
x=K[R∣t]Xw​
Where:
- K is the 3×3 intrinsic matrix
- R is the 3×3 rotation matrix (world to camera)
- t is the 3×1 translation vector
- Xw​ is the 3D world point in homogeneous coordinates [X,Y,Z,1]T
Steps:
- Form the 3×4 extrinsic matrix [R∣t]
- Compute the 3×4 projection matrix P=K[R∣t]
- Project: x′=P⋅Xw​
- Normalize: [u,v]=[x′/w′,y′/w′]
Return [u,v] rounded to 2 decimal places.
Example:
world_point = [10.0, 5.0, 20.0] intrinsic_lambda = [[1000, 0, 500], [0, 1000, 400], [0, 0, 1]] rotation_omega = [[1, 0, 0], [0, 1, 0], [0, 0, 1]] # Identity translation_tau = [0, 0, 5]
[900.0, 600.0]
- Form extrinsic [R∣t] as 3×4 matrix
- Compute P=K⋅[R∣t]
- Project: x′=P⋅[5,3,10,1]T
- Normalize by the third component
Constraints:
- The world point w will always result in a non-zero lambda after projection
- Lambda is a valid 3x3 intrinsic matrix
- Omega is a 3x3 rotation matrix
- Tau is a 3x1 translation vector
- All inputs are floating-point numbers
- Output must be rounded to 4 decimal places
1. Background Knowledge
The pinhole camera model is the foundational geometric model in computer vision for projecting 3D world points onto a 2D image plane, assuming light rays pass through a single point (pinhole) without distortion. It separates intrinsic parameters (internal camera properties) and extrinsic parameters (camera pose in world space).
- Intrinsic matrix K (3×3):
where fx​,fy​ are focal lengths in pixels, and cx​,cy​ is the principal point.
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Extrinsic parameters: R (3×3 rotation matrix, world-to-camera) and t (3×1 translation vector).
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Homogeneous coordinates: World point Xw​=[X,Y,Z,1]T, projected to image point x′=[x′,y′,w′]T, then normalized to [u,v]=[x′/w′,y′/w′].
This model assumes perspective projection where parallel lines converge, valid for standard cameras but extended in variants like fisheye.
2. Algorithm Approach
The standard algorithm computes the projection matrix P=K[R∣t] (3×4), then applies linear transformation followed by perspective division:
- Form extrinsic matrix: [R∣t] by concatenating R (columns 1-3) and t (column 4).
- P=K⋅[R∣t].
- x′=P⋅Xw​.
- u=x′/w′, v=y′/w′.
Matrix multiplication is O(1) for fixed 3×4×4 dimensions. Libraries like NumPy (Python) or Eigen (C++) handle this efficiently. No iterative optimization needed due to closed-form nature.
3. Step-by-Step Strategy
import numpy as np
def project_point(K, R, t, Xw):
# Step 1: Form extrinsic matrix [R | t] (3x4)
extrinsic = np.hstack((R, t.reshape(3, 1)))
# Step 2: Compute projection matrix P = K @ extrinsic (3x4)
P = K @ extrinsic
# Step 3: Project homogeneous point (4x1)
x_prime = P @ Xw # [x', y', w']
# Step 4: Perspective division and round to 4 decimals
u = x_prime / x_prime
v = x_prime / x_prime
return np.round([u, v], 4)
Input assumptions: K ("Lambda"), R ("Omega"), t ("Tau"), Xw​ as 4×1 vector. Constraints guarantee wâ€²î€ =0.
4. Common Pitfalls
- Homogeneous coordinates: Forgetting to append 1 to Xw​=[X,Y,Z].
- Matrix dimensions: K (3×3) × [R∣t] (3×4) → P (3×4); P × Xw​ (4×1) → 3×1. Shape mismatches cause errors.
- Perspective division: Dividing by zero (prevented by constraints); use w′ not z.
- Rounding: Problem specifies 4 decimal places (not 2 as initially stated); use np.round(..., 4).
- Coordinate systems: R transforms world-to-camera; verify convention (row-major vs column-major).
- Floating-point precision: Use double precision; small numerical errors amplify in division.
5. Time & Space Complexity
- Time: O(1) constant time. Dominant operations: two 3×3×3 multiplications (K⋅R) + 3×1×4 (⋅t,⋅Xw​) + 2 divisions = ~100 FLOPs.
- Space: O(1) constant. Matrices: K (9 floats), R (9), t (3), Xw​ (4), P (12), temporary vectors (~20 floats total).
Scalability: For n points, becomes O(n) via batch matrix multiplication P@Xw​ (3×4 × 4×n). Ideal for real-time vision pipelines.