F4 Newt lunar imaging and trying a near IR filter
Posted: Thu Oct 29, 2026 12:12 pm
More quixotic attempts at trying to optimise my F4 Newtonian for lunar/ planetary imaging - a single instrument suitable for all uses.
A fundamental limitation of course is that - when uncorrected - the ~ coma-free field at such a low F number is limited to about 1.4 mm on axis or less than an arcmin.
One solution is to use a coma corrector - no barlow - and a camera -ASI 715 MC - with tiny (1.45 um) pixels. This seemed to work pretty well viewtopic.php?t=9542 but limits resolution - i.e. sampling at 0.28 arcsec/ pixel which is insufficient to sample the theoretical Dawes limit for a 300 mm telescope of ~ 0.4 arcsec.
So here using an ED 2X Barlow to make the system F8. Based on the coma-free field diameter in mm = f^3/45 mm being now about 11.4 mm and a good fit to the size of the ASI 715 MC chip - the image should be ~ coma free across its maximum field of 3864 x 2192 pixels or ~ 8.8 x 5.5 arcmin at ~ 0.137 arcsec/ pixel
VX 12 300 mm F4 reflector, CEM70G mount, 2X Barlow, Baader Clicklock, ASI 715 MC camera. Captured using 1 minute Sharpcap .ser files. Processed using BiggSky and Affinity photo. Filter was an Astronomik ProPlanet 642 (R and near IR) or a Baader L2 equivalent UV/IR cut.
Gain was 100 (less than unity) and exposure 6 ms with Biggsky selecting ~ 30% of 2640 frames over 1 min.
The seeing on the night of the 27/28 October was horrible and I couldn't clearly even get focus. I just thought that this comparison of the RGB image and the IR image of part of the Mare Crisium and crater Picard might be of interest? I am amazed at just how good the ProPlanet filter was at minimizing the seeing effects -- there are tiny craterlets visible probably less than a mile across and not far off the (IR) limiting resolution of ~ 0.5 arsec. The UV/IR cut filtered image on the other hand is very poor and at least twice as blurred.
Thanks to Dave for highlighting the filter.
A fundamental limitation of course is that - when uncorrected - the ~ coma-free field at such a low F number is limited to about 1.4 mm on axis or less than an arcmin.
One solution is to use a coma corrector - no barlow - and a camera -ASI 715 MC - with tiny (1.45 um) pixels. This seemed to work pretty well viewtopic.php?t=9542 but limits resolution - i.e. sampling at 0.28 arcsec/ pixel which is insufficient to sample the theoretical Dawes limit for a 300 mm telescope of ~ 0.4 arcsec.
So here using an ED 2X Barlow to make the system F8. Based on the coma-free field diameter in mm = f^3/45 mm being now about 11.4 mm and a good fit to the size of the ASI 715 MC chip - the image should be ~ coma free across its maximum field of 3864 x 2192 pixels or ~ 8.8 x 5.5 arcmin at ~ 0.137 arcsec/ pixel
VX 12 300 mm F4 reflector, CEM70G mount, 2X Barlow, Baader Clicklock, ASI 715 MC camera. Captured using 1 minute Sharpcap .ser files. Processed using BiggSky and Affinity photo. Filter was an Astronomik ProPlanet 642 (R and near IR) or a Baader L2 equivalent UV/IR cut.
Gain was 100 (less than unity) and exposure 6 ms with Biggsky selecting ~ 30% of 2640 frames over 1 min.
The seeing on the night of the 27/28 October was horrible and I couldn't clearly even get focus. I just thought that this comparison of the RGB image and the IR image of part of the Mare Crisium and crater Picard might be of interest? I am amazed at just how good the ProPlanet filter was at minimizing the seeing effects -- there are tiny craterlets visible probably less than a mile across and not far off the (IR) limiting resolution of ~ 0.5 arsec. The UV/IR cut filtered image on the other hand is very poor and at least twice as blurred.
Thanks to Dave for highlighting the filter.