2. Rayleigh criterion at H band
θ_H = 1.22×1.65µm/10m = 41.5 mas, coarser than the V-band value (13.9 mas), consistent with the direct proportionality of resolution to wavelength.
| Criterion | Points |
|---|
| Correct arithmetic | 10 |
| Correct direction (coarser at longer wavelength) | 5 |
3. Seeing-limited versus diffraction-limited
Ratio = 0.8″/0.0415″ = 19 -- still far larger than 1, so an uncorrected Keck H-band image remains strongly seeing-limited, not diffraction-limited, even though the gap is smaller than at V band.
| Criterion | Points |
|---|
| Correct ratio | 8 |
| Correct seeing-limited conclusion | 7 |
4. Focal-station reasoning
The Cassegrain focus is compact but mass- and space-constrained (it moves with the telescope through its full range of motion); Nasmyth and Coudé foci route light to a stationary or slower-moving platform with far more room and weight capacity for large cryostats, optical benches, and vibration-sensitive components, which is why the heaviest instruments are placed there rather than at Cassegrain.
| Criterion | Points |
|---|
| Correct identification of the weight/space trade-off | 12 |
| Correct connection to instrument type | 8 |