I used to use a 2.5mm BO/TMB on planets all the time in my 100mm f/6 so I can see a use for the 2.4 if it has improved resolution or contrast but since replacing that with a 2-4mm Nagler Zoom, I haven't found the 2mm end of the NZ to be useful yet. Mars is quite good at 2.5mm in my 127 f/7.5 but nothing else can tolerate that small of an exit pupil. And of course the atmosphere needs to cooperate which, for instance, it wasn't doing last night even at 4mm in the shorter focal length 100mm f/6.
A problem for us Northern Hemisphere viewers during the closer Mars oppositions is that it is placed lower in the sky in the South. We lose on atmospheric effects as we gain in apparent size, making the use case for 1.6 and 2.0mm less compelling. Oh well, time to move to Oz.
Another thought about assessments of "resolution" in very short focal lengths like these Vixen HRs: There are no telescopes which are delivering an image of such resolution that the optics of the ~2mm eyepiece need to be perfect. If there is no more resolution to be revealed at the eyepiece beyond about a 2mm (or maybe 1.5mm for the eagle-eyed) exit pupil, then any EP delivering a smaller exit pupil need not *necessarily* deliver a perfect Airy disk. Yes, I know that all aberrations are cumulative so a lower quality EP will add a bit of blur to the now already diffraction-limited image of multiple overlapping Airy disks, and an EP with background reflection/elevated brightness problems will mar contrast of the image (eg: my BO/TMB 2.5 on the Moon). However, when going down to an 0.5mm or smaller exit pupil, just how much difference can there be between, say:
2.5mm BO/TMB
2-4 Nagler Zoom @2.5
2.5mm Nagler T6
2.58mm Pentax XO
2.4mm Vixen HR
5x barlowed 12.4mm Meade 4000 Plossl??
It's less than a 1mm exit pupil on the shortest focal ratio of scopes, how much more damage to the view can one of these do vs. the others on planets?