I was trying to follow Bernard Hubl's method but in the end had to use Deep Sky Stacker and its 'comets and stars' function.
For Luminance I produced an image of the comet only.
For R, G and B I produced an image of the comet plus stars. The channels were combined in PS
I stretched both the L and the RGB images in PS and then combined them.
The trouble I found with this is that stretching to show the faint tail with the limited data meant I also developed the streaks left by the stars. My knowledge of PS is not up to removing broad faint streaks but leaving the tail.
Anyway, for better or worse:
Comet C/2017 T2 Panstarrs |
C/2017 T2 (PANSTARRS)
Magnitude: 8.6
Phase: 36 °
Distance: 1.6765au
Solar distance: 1.6185au
Velocity: 33.1km/s
Estimated tail length: 0.04au
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