testing 1-2-3, preparing for the eclipse

testing out my imaging rig for the 8/21/17 total solar eclipse.  there will be a range of exposures so decided to shoot filtered midday sun, twilight moon, full moon.  Here are a few images (click on image for full size):

Sun white light filter 2-4-2017

Moon 2-4-2017

Moon 2-12-2017

Moon at twilight 1-30-2017 grey scale

Just for fun, i decided to simulate an eclipse with the images.
I selected the image closest to full and superimposed it on the solar image.
To my chagrin, the moon did not totally cover the sun--that whole perigee apogee thing--I'd created an annular eclipse.
so i had to use an image from another day when the moon was closer to the earth and large enough to completely cover the sun.
Here's the comparison illustrating variation in the apparent size of the moon during its orbit around the earth:

Lunar images superimposed on solar

Technical notes:
decided to go with my widest field webcam and shortest focal length scope with a web cam, DMK 51 and the tiny tak, Takahashi FS-60C, 60 mm aperture at f/4.2 with a reducer.  The field of view is approximately 96x72 arc minutes.  Each image is a one minute video capture at approximately 12 fps, aligned in autostakkert, wavelets in registax.

heart of the heart

here's a close up of "the heart of the heart", 
dust and gas near open cluster Melotte 15,
in the center of IC 1805, the heart nebula (click for full size):

in a massive cloud of dust and hydrogen in the constellation Cassiopeia,  the dust began to clump. 
what caused the clumping? 
a supernova, gravitational interaction with a nearby galaxy, or maybe a cosmic butterfly.  
gravitational attraction caused the clumps to get more and more massive, generating so much pressure that the clumps burst into flames as nuclear fusion commenced.  stellar wind from the new star cluster caused the dust to move away with hydrogen glowing red at the heart-shaped edges. 
in the center of the heart nebula lies a psychedelic collection of dust pillars.  the tips of the pillars are anchored by dense collections of dust--stars to be, or perhaps that will never be, as the surrounding dust is blown away.

For obvious reasons, i prefer this one in a more natural color palette (above), but here's a version in the Hubble palette with hydrogen as green, sulfur as red and oxygen as blue:

lastly, here's an older wide field view of the heart nebula at low power as it's quite large, 5 times the apparent size of the full moon: 

heart nebula aka IC1805

click for full size, note the central star cluster and dust pillars.  

image details:
8" LX200R, SX Trius 694 binned x 2 to 0.8"/px
astrodon 3nm OIII, 3 nm SII, 5nm Ha filters
ASA DDM60
OIII 6x20 min bx2, 13x20 min bx4, SII 3 x 20 min bx2, 39x20 min bx4, Ha 12x 20 minutes bx2
11/12/15-12/29/15
Eastbluff, CA
in processing, i accidentally overlaid the hubble palette version on the conventional giving a hint of color to the highlights, seemed to work, so i left it.  the silky smooth background is not due to the massive exposure time, but rather aggressive use of topaz denoise.
heart nebula:
FS60C f/4.2 FR CS 10 nm Ha/Baader 8.5 nm Oiii filters, H9
Ha 12/19/08
Oiii 12/22/08-ruined by gradients re-shot 1/17/09
2 panel mosaic 12x5 min each panel
los alamitos, CA
bortle white skies, poor to fair seeing, good transparency for area

a sharper eye, NGC 6751 in NII Ha OIII

The glowing eye nebula, NGC 6751 really looks like an eye to me, complete with a pupil, iris, and reflected light.  Yes, it's a bit blood-shot:

RGB image, 2007

I re-shot the planetary nebula with narrow band filters (nitrogen-red, hydrogen-green, and oxygen-blue) and a newer camera with larger image scale :)

this image shows faint red jets to the sides
these did not enhance as dramatically in NII compared to Ha as typical red FLIERS do.
there is however,  an unusual line of red NII enhancing pillars crossing just above the center.
also a hint of structured filaments/pillars surrounding the clearing around the central star

lots more detail, but perhaps less eye-like

progressively aggressive stretches of the OIII image shows at least 2 faint outer shells:

also a very faint smudge to the lower right.
This paper, in part based on this super deep image confirm the presence of the outer shells, one of which is interacting with the interstellar medium.  The smudge to the lower right is apparently not part of the planetary nebula.

image details:
8" LX200R, SX Trius 694 0.4"/px
astrodon 3nm OIII, 3 nm NII, 5nm Ha filters
ASA DDM60
OIII 10 x 5 min, NII 10 x 5 min, Ha 6 x 5 minutes
8/31-9/30/2016
unusually good seeing.  
The image is rotated south up to match the older image.  
Eastbluff, CA

no calibration ;)


P.S. 
a random field star showed a hint of OIII nebulosity around it when stretched aggressively
HD 177793
19 06 22.52288 -06 04 28.5941
wondering if it's a small planetary (or just my imagination)
there is a fair amount of random nebulosity in the field
couldn't find anything on it in SIMBAD

not sure how else to check

HD 177793