Arrange the following telescopes, where \( D \) is the telescope diameter and \( \lambda \) is the wavelength, in order of decreasing resolving power:
I. \( D = 100\,\text{m}, \lambda = 21\,\text{cm} \)
II. \( D = 2\,\text{m}, \lambda = 500\,\text{nm} \)
III. \( D = 1\,\text{m}, \lambda = 100\,\text{nm} \)
IV. \( D = 2\,\text{m}, \lambda = 10\,\text{mm} \)