While any eyepiece can serve as a “planetary” eyepiece, an eyepiece which is best able to perform on lunar or planetary targets should naturally optimize its performance around those attributes which are peculiar to the target being observed. A planet as an observing target, when compared to the many other celestial targets available to the observer, has many attributes which are unique and can all occur simultaneously within the field of view. Arguably, the resulting major attributes of the primary planets (i.e., Jupiter, Saturn, Mars, Venus), and the importance these attributes become relative to selecting a planetary eyepiece, can be summarized as follows:
1 – Very Bright
Becomes important for the eyepiece to control internal reflections, glare, flare, scatter, and lateral color as these problems are usually accentuated by a very bright object either in the field of view, or just outside the field of view.
2 – Small in Angular Size
Becomes important for the eyepiece to be available in short focal lengths so higher magnifications are available without adding more components like a Barlow which may not be to the optimum level as your planetary eyepiece.
3 – Rich in Both Very High Contrast & Very Low Contrast Features
Becomes important for the eyepiece to have excellent transmission and contrast with minimal scatter so low contrast features are more easily visible and high contrast features are more brilliantly defined to impart a well defined three dimensional effect.
4 – Has Colored Features which are Easily Observable
Becomes important for the eyepiece to have excellent transmission so sufficient light is available to activate the color receptors in your eyes and a neutral image tone to preserve the true colors.
5 – Has Satellites (i.e., moons)
Becomes important for the eyepiece to have high transmission to better see dim satellites, high contrast so satellite shadows on a planet surface are more stark, and low scatter with a sharp field stop so dim moons are more easily detectable if you need to hide the planet behind the field stop and still have a field of view free from reflections and scatter in order to detect dim satellites close to the planet.