Step 1: Understanding the Rayleigh Criterion. The limit of resolution (θ) of a telescope is given by Rayleigh's criterion: \[ \theta = \frac{1.22 \lambda}{D} \] where: - \( \lambda \) is the wavelength of light (540 nm = \( 540 \times 10^{-9} \) m), - \( D \) is the diameter of the telescope’s objective (3.6 m), - The factor \( 1.22 \) is derived from diffraction theory.
Step 2: Substituting the values. \[ \theta = \frac{1.22 \times 540 \times 10^{-9}}{3.6} \] \[ \theta = \frac{658.8 \times 10^{-9}}{3.6} \] \[ \theta = 1.83 \times 10^{-7} \text{ rad} \] Final Answer: \[ \boxed{1.83 \times 10^{-7} \text{ rad}} \]
Observe the following data given in the table. (\(K_H\) = Henry's law constant)
Gas | CO₂ | Ar | HCHO | CH₄ |
---|---|---|---|---|
\(K_H\) (k bar at 298 K) | 1.67 | 40.3 | \(1.83 \times 10^{-5}\) | 0.413 |
The correct order of their solubility in water is
For a first order decomposition of a certain reaction, rate constant is given by the equation
\(\log k(s⁻¹) = 7.14 - \frac{1 \times 10^4 K}{T}\). The activation energy of the reaction (in kJ mol⁻¹) is (\(R = 8.3 J K⁻¹ mol⁻¹\))
Note: The provided value for R is 8.3. We will use the more precise value R=8.314 J K⁻¹ mol⁻¹ for accuracy, as is standard.