ClarkVision Photography: NEW Gallery

Home   Galleries   Articles   Reviews   Best Gear   New   About   Contact   Gallery Index   Previous   Next
image comet-neowise-rnclark-105mm-c07-20-2020-IMG_8644-78-av30-e7.f-1400s.jpg is Copyrighted by Roger N. Clark, www.clarkvision.com

Comet NEOWISE in the Evening Sky July 20, 2020

Comet NEOWISE put ion a dazzling show in the evening in July, 2020 after making its perhileon passage on July 3. From dark skies, the comet was easily seen with the unaided eye, showing a tail over 10 degrees long. At a dark site in the Colorado Rocky Mountains the view in 7x50 binoculars showed the a yellow-ish brown dust tail, a green head and a gray ion tail (the contrast was too low to see blue and purple color shown in the image).

The comet displays two tails: The blue tail (Type 1) is an ion tail. The blue is fluorescence from molecules ionized by solar ultraviolet light. The usual main emission is from CO+ emitting at 425 - 427 nm, deep blue. Comet Neowise also shows sodium emission (589 nm) in the tail (See the Planetary Science Institute Press Release). Chromaticity of 426 + 589 can produce pink/magenta in the right proportions. The varying hues of magenta and blue along the ion tail may indicate varying proportions of carbon monoxide and sodium emissions. The yellow-ish dust tail (Type 2) is dragged into a fan shape by the solar radiation pressure on tiny dust grains, along with the orbital motion of the comet. The yellow is reflected sunlight off of small dust particles. The green around the nucleus is fluorescence from diatomic carbon (C2) with possible contribution from cyanogen (CN).

Technical. This image was obtained with a stock Canon EOS 90D Camera and Sigma 105mm f/1.4 DG HSM Art Lens at f/1.4. Tracking the comet with a Fornax Lightrack II and no guiding. The image is a stack of 53 images. Thirty 15-second exposures at ISO 800 were stacked for the tails (7.5 minutes total exposure), and 23 images of the comet head with exposures from 1/4 to 5.2 seconds (45.4 seconds total exposure) were combined for a High Dynamic Range (HDR) composite to show detail in the green nucleus region to the faint dust and ion tails. The field of view of the image is about 12 x 8 degrees.

This is a natural color image. Post processing: Raw conversion with Rawtherapee with settings tuned for astrophotos, including maintaining star color in saturated stars. Rawtherapee processing settings described here. Output color space was Rec.2020 to match the future of high dynamic range TVs and the web presentation here is sRGB. Stretched with color preserving methodology, rnc-color-stretch. Also see Astrophotography Image Processing Basic Work Flow.

The comet moved 0.6 pixel between frames in the 15-second exposures. In order to get sharp comet details and sharp stars, one must separate stars and comet and process them separately. I tried aligning on the comet with ImagesPlus and Deep Sky Stacker, DSS, and both failed. I ended up doing a tedious alignment by hand in photoshop. The stars were aligned with Deep Sky Stacker, then both aligned on comet and aligned on stars were stretched with rnc-color-stretch. Parameters were:
        -rootpower 6 -root power2 2 -scurve1 -skylevelfactor 0.005.
Then the two aligned images were combined and the shorter exposures merged to show detail in the brighter nucleus.

Online are images of the comet with a blue ion tail seem to also show a white dust tail. The dust is distinctly yellow brown, both visually and in short exposures with no processing. So images with a white dust tail and blue ion tail are not natural color. They probably set the white balance to tungsten or something similar. The comet is illuminated by the sun, so sunny (daylight) white balance is what is needed for natural color.

The Exposure Factors, CEF, CEFA are measures of the relative amounts of light received from a subject. It can be used to fairly compare wildly different lens/telescope apertures and exposure times. For this image on the thirty 15-second images on the tail:

Modern DSLRs like the Canon 90D include on sensor dark current suppression and low fixed pattern noise at ISOs around 1600 and higher, making no need for dark frame subtraction. Modern raw converters correct for light fall-off and also correct for hot/dead/stuck pixels. This makes processing low light images easy: simply align and average.


To learn how to obtain stunning images like this, please visit my Extensive Articles on Photography .


Keywords to this image = astrophoto-1 night low-light digital_astro comet canon_90d rnc-color-stretch NEW

Image ID: comet-neowise-rnclark-105mm-c07-20-2020-IMG_8644-78-av30-e7.f-1400s.jpg

All images, text and data on this site are copyrighted.
They may not be used except by written permission from Roger N. Clark.
All rights reserved.

Home Galleries Articles Reviews Best Gear Science New About Contact

Obtaining Images or Prints

Last updated July 31, 2020