The direct and reversed zenith angles observed by a theodolite are $56^\circ 00' 00''$ and $303^\circ 00' 00''$, respectively. What is the vertical collimation correction?
Step 1: Formula for vertical collimation error.
When direct and reversed zenith angles are observed, the condition for perfect collimation is:
\[
Z_d + Z_r = 360^\circ
\]
where $Z_d =$ direct reading, $Z_r =$ reversed reading.
If this sum is not exactly $360^\circ$, the deviation indicates collimation error.
Step 2: Apply the given data.
\[
Z_d = 56^\circ 00' 00'', Z_r = 303^\circ 00' 00''
\]
So,
\[
Z_d + Z_r = 56^\circ + 303^\circ = 359^\circ 00' 00''
\]
Step 3: Find the deviation.
For perfect collimation: $Z_d + Z_r = 360^\circ 00' 00''$.
Here, the actual sum is $359^\circ 00' 00''$.
Hence, there is a shortfall of:
\[
360^\circ - 359^\circ = 1^\circ 00' 00''
\]
Step 4: Correction formula.
Vertical collimation correction $= \dfrac{\text{error}}{2} = \dfrac{1^\circ 00' 00''}{2} = 0^\circ 30' 00''$.
Since the observed sum is less than $360^\circ$, the correction is taken as positive.
\[
\boxed{+0^\circ 30' 00''}
\]
Consider a five-digit number PQRST that has distinct digits P, Q, R, S, and T, and satisfies the following conditions:
1. \( P<Q \)
2. \( S>P>T \)
3. \( R<T \)
If integers 1 through 5 are used to construct such a number, the value of P is:


