bigger jupiter, saturn's coming

finally able to take advantage of larger aperture
for a higher magnification jupiter

Jupiter 5/28/17

still a bit mushy, but showing some promise

meanwhile saturn reached opposition this week
coming up on prime viewing season
here's a wide field with a few moons:

Saturn and Moons 5/14/17

a bit closer on another night:

Saturn 6/14/17

will get to higher magnification when it rises earlier in the evening

Imaging notes:
The larger f/8 scope allowed me to use a 2x Barlow on jupiter, increasing the magnification by a factor of 2 compared to my old system (C8).  
Several other issues were critical to getting the system to work:
1. internal thermal tube currents are a major problem with the new big scope, it takes hours to cool down.  a "cat cooler" made a huge difference.
2. dark subtraction.  this makes sense as i'm trying to minimize expsosure shooting at ~30% max histogram.  the love/hate issue with my ASA DDM 60 mount continues.  the issue here is that most mounts move around so much that the subtle grid pattern in the camera is dithered out.  my mount tracks so well that the planet sits dead center even at very high magnification, so the pattern becomes evident in processing.  this is actually a good problem to have.  for example last night i took a series of images of jupiter at this focal length over the course of an hour and didn't have to budge the mount, even though the pointing model was made with a much lighter scope 6 months ago.  
3. diagonal: didn't test that rigorously, but shooting through the diagonal didn't seem to make that much difference.  
4. made a bit of progress working on LD compensation in win jupos which is necessary with jupiter so far from opposition, you can still see a darker section at the limb on the left (might be processing artifact in part).  
5. more on the mount: the mount is very sensitive to weight changes, the act of switching from eyepiece to camera with barlow felt like this classic scene from raiders of the lost ark. the key is to balance the mount with the camera, not eyepiece.  forget about binoviewers.  

image details (jupiter):
Meade LX850 12" f/8
televue 2x Barlow
FocalLength~4100mm
Resolution~0.19"
ZWO ASI120MC/ASI120MM-S
ZWO RGB filters
4x2 minute captures for each filter R G B
captures with firecapture @ ~140 fps
exposure 3-4 ms per frame
stacked in autostakkert, combined in WinJupos, sharpened in registax 6
5/28/17 (2017-05-28-0446_7)
Eastbluff, CA

Jupter's out, IR test and a new scope

the bright star in the east after dark (which is pretty late these days)

is in fact Jupiter. 

seeing has been lousy this season, but i finally gave it a try on a night of mediocre seeing and got this:

Jupiter 4/11/2017

ran a few tests with an infrared (IR) pass filter to see if it would yield a sharper image.  In theory the redder the light (longer wavelength), the less it is distorted by atmospheric seeing, so images should be sharper, but...
the optical resolution limit of a telescope is defined by the wavelength of the light: longer wavelength reduces the theoretical limit of the telescope.  furthermore, the IR pass filter typically allows less light than a standard red filter.  therefore, exposures may need to be longer (leading to more atmospheric motion) and/or higher noise.  
so in practice is the IR image sharper than the others?
here's a blink comparing red to infrared (no contest comparing to blue and green):

red vs infrared

clearly sharper, but perhaps a bit more noise.  

However, for the combined image, it was difficult to appreciate any difference:

here's RGB vs IRGB (substituting IR for red):

RGB vs IRGB

the difference is very subtle, with perhaps a bit more detail in the short blue stripe just above the middle white band.  

lastly, i used IR as the luminance channel which changed the colors dramatically, but probably a bit too far from the RGB:

RGB vs IR-IRGB

this, i think, is my first successful image with a new (used) larger scope
which i picked up on astromart almost a year ago
in order to catch saturn's hexagon,
explaining a year of poor seeing.
the new scope is pretty friggin' big and a PITA to haul around in the dark at 2 AM so i hope it works out

new scope specs

Meade LX850 12" f/8 ACF OTA + Feathertouch focuser

2438mm

0.38"

41 lb. tube weight

UHTC coating

primary 12" (305 mm)

secondary 4.72" (120 mm) / 41%

image details:

ZWO ASI120MC/ASI120MM-S

ZWO RGB filters, Baader IR pass "685" nm

2x90 second captures for each filter R G B IR

captures with firecapture @ ~140 fps

stacked in autostakkert, combined in WinJupos, sharpened in registax 6

Southern California

4/11/17

starburst nebula NGC 1569, narrow band

Here's starburst nebula NGC 1569 in hydrogen (Ha) and oxygen (OIII)

this sat on my hard drive for a year as i was initially disappointed for 2 reasons:
1 there was little difference between the OIII and Ha at this resolution besides signal strength
2 the narrow band and LRGB (below) were so discordant, i couldn't imagine the combine working well.  the Ha didn't enhance the image, it overwhelmed it.

here it is in LRGB:

when i finally combined the narrow and broad band images i was pleasantly surprised to see the sum adding up to more than the parts, even though some details of each were lost in the combination.
the combined image gives the classic appearance of stars clearing out and illuminating the surrounding hydrogen:

in this case the two bright "stars" appearing to illuminate the surrounding nebula are unresolved globular clusters containing thousands of stars (anyone fooled?), making this dwarf galaxy the largest "nebula" i've ever imaged

here's an interesting slow motion blink of the two images
some structures disappear, others appear, and others seem to move (lower left) as if being illuminated by a nearby source:

lastly here's an annotated mosaic:

more details on dwarf galaxy ngc 1569 at this site including observations of the "elephant's trunk" to the right
hubble image resolving the star clusters and more details at wikipedia
interestingly, the galaxy is blue-shifted, which means it's moving towards us, rather than moving away with the expansion of the universe.  

thanks to rick johnson for pointing out this galaxy with it's extreme narrow band emissions.

image details:

8" LX200R, SX Trius 694 binned x2 to 0.8"/px,
astrodon 5nm Ha, 3nm OIII, LRGB E SERIES GEN-II
ASA DDM60
L 472x1 minute, 24x3 minutes, R 64x3 minutes, G 59x3 minutes, B 55x3 minutes (RGB included in luminance)
Ha 25x20 minutes, OIII 11x20 minutes.
1/29/16-2/8/16, bortle white skies
eastbluff, CA

Abell 30, the born again nebula

March has been a difficult month for me in recent years, 
a number of events have prevented me from completing this project, but finally,
here is my image of Abell 30, a rare "born again" planetary nebula who's central star re-ignited after turning into a white dwarf,
creating a new system of complex knots of oxygen (blue-green)
inside a mature spherical shell of hydrogen (red) and oxygen:

Abell 30 in Hydrogen (red) and Oxygen (blue-green)

The O III signal was faint, Ha signal extremely faint, and He II almost nonexistent.  

I was baffled by sources stating that the knots have strong He II emissions, e.g., 

Osterbrock's Astrophysics of Gaseous Nebulae and Active Galactic Nuclei p. 264.

My He II filter is spec'd at 468.6 nm with a 4 nm band width detects almost no signal in the outer shell, but did detect signal in the small knots closest to the central star.  My best guess is that "helium rich" refers to the relative ratio of He II to Ha in specific areas of the nebula.  Here's a mosaic of images with the various filters displayed using the linear stretch that best displayed the central knots.  The continuum filter removes the narrowband emissions of the nebula, showing only stars in this case:

Abell 30

Edited the section above (a filter wheel error on my initial attempt substituted a continuum filter for the Helium II filter).

A few findings regarding exposure variation and binning:

for OIII 3 nm 

40 min binned 2x not much deeper than 20 min binned 2x, if at all.

but 

20 min binned 4x (4 subs) much deeper than 40 min binned 2x (2 subs)

though it was difficult to be sure conditions were identical.  

filter band width:

for 40 min binned 2x 3 nm OIII deeper than 5 nm or 8.5 nm; not much difference between latter two

older unbinned subs with my SX H9 (0.6"/px) were far worse than either, threw all subs out

8" LX200R, SX Trius 694 binned x2 to 0.8"/px, binned x4 to 1.6"/px, (final image at .8"/px)

astrodon 5nm Ha, 5nm, 3nm OIII, chroma 4 nm He, 540x50 nm filter (greenish continuum) ; custom scientifics 8.5 nm OIII

ASA DDM60

OIII 10x 20 min bx4, 28x 40 min bx2, 44x 20 min bx2

Ha 2x 20 min bx2, 15x 40 min bx2, 60 x 20 min bx4

HeII 36x 1200s bx4 2x2400s bx2!

continuum filter 13x2400s bx2 (in error, black point 30K ADU!)

2/16/13-3/6/17

eastbluff, CA

crescents and earthshine

what's missing from my previous crescent moon image is this:

no, earthshine is not a drink served at california dispensaries.

Earthshine is a glow which lights up the unlit part of the Moon because the Sun’s light reflects off the Earth's surface and back onto the Moon, best seen during the crescent moon.  It is also sometimes called the old Moon in the new Moon's arms (or vice versa), or the Da Vinci glow, after Leonardo da Vinci, who explained the phenomenon for the first time in recorded history.

yes, i know this lies far in the realm of cub scout merit badges, but i was reminded of it when i tried to cut and paste an image of the first quarter moon for the eclipse test/comparison and could not define the edge of the moon.  i had to eyeball it by empirically fitting a circle to the part that was visible.

when the moon is a thin crescent, it means the moon is almost directly between the earth and the moon, so the part of the moon lit by the sun is mostly facing away from us, while the dark side faces us.  now from the lunar point of view, the earth is almost directly opposite the sun, so all the reflected light of the earth lights up the night sky (a full earth).  this light brightens the surface of the moon just as a full moon lights our nights, the "earthlight" makes the dark surface of the moon easier for us to see.

in an odd twist, astronomers have used earthshine to detect life on earth, testing a technique that could potentially be used to detect life on other planets.

while shooting this image, i turned my low power imaging rig on the "dusk star", the bright star visible at sunset this month:

caught a tiny crescent venus, matching the moon.

Technical notes:
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.