Contains:  Solar system body or event
Comet C/2015 V2 Johnson - Development of Gas Tail -  March-April 2017, Sebastian "BastiH" Hinz

Comet C/2015 V2 Johnson - Development of Gas Tail - March-April 2017

Comet C/2015 V2 Johnson - Development of Gas Tail -  March-April 2017, Sebastian "BastiH" Hinz

Comet C/2015 V2 Johnson - Development of Gas Tail - March-April 2017

Equipment

Loading...

Acquisition details

Loading...

Description

EQUIPMENT:

TS ONTC 10" f/4 Newton on EQ8

60/240mm Guiding Scope with Lacerta M-GEN

Canon EOS 6Da with Baader BCF

IMAGES:

upper row 1: 8x 2min at iso 1600, 28.03.2017

upper row 2: 8x 1min at iso 3200, 17.04.2017

upper row 3: 8x 1min at iso3200, 29.04.2017

lower row 1: 31x 2min at iso1600, 28.03.2017

lower row 2: 31x 1min at iso3200, 17.04.2017

lower row 3: 31x 1min at iso3200, 29.04.2017

each image processed with 100 flat frames and a superbias made from 200 bias frames (PixInsight), identical postprocessing and cropping to the same size and aspect ratio

EXPLANATION:

My initial intention was/is to follow the comet's development by photographing it every two weeks...this is what weather and moon allowed. During the first imaging session on 28th of march, the comet showed hardly any movement relative to the sky backgrund (0.00' in RA and 0.07' in DEC per hour) so I was able to do long exposures without getting startrails or having to process comet and stars seperately (which I'm not overwhelmingly good at). At the time of the second session on 17th of april, the comet's apparent movement had accelerated to 0.06' in RA and 0.28' in DEC so I doubled iso speed from 1600 to 3200 and halved single frame exposure time from 120 to 60 seconds to get "more light in less time" while providing comparability. I had tested the settings previously to find out that both iso speeds scale reasonably linear with the 6D's sensor, the signal strenght of raw images at iso 3200 seems to be at a similar level to the signal strenght of images taken at iso 1600 with double exposure time. Apart from that, there was only a little bit more noise in the frames taken at iso 3200 and a bit more saturation in the frames taken at 1600 - not a very big difference though. At the time of the last session, the comet's apparent speed had further increased to 0.08' in RA and 0.73' in DEC. So I calculated the maximum exposure time from the last session that I could stack and the necessary downsizing to ensure a piont-shaped comet core and applied that to the images of all three sessions. Because the ion tail almost wasn't visible when stacking 8x1min at iso 3200 (or 8x2min at iso1600), I also did three stacks of 31 frames each that I just aligned on the comet. The increasingly blurred stars (resulting from the sigma stacking method that I used, with a different method there would have been elongating startrails) illustrate the acceleration of the comet relative to the sky background.

Comments

Histogram

Comet C/2015 V2 Johnson - Development of Gas Tail -  March-April 2017, Sebastian "BastiH" Hinz