Sunday, January 6, 2019

Images from The Illig Telescope


Last summer, The Howard County Astronomical League received a valuable gift.  Leona and David Illig presented us with a Takahashi TOA-150 telescope and an Astro-Physics 1200 GTO mount. Thank you. 

On November 10, 2018, I acted as Certified Telescope Operator for the evening's Public Star Party.This gave me my first opportunity to operate the Illig under clear skies.
Excitedly, I arrived at HALO very early. Knowing that any astrophotography project requires calibration data, I fully intended to acquire a set of Flat, Dark and Bias frames before anyone arrived for the evening’s festivities. 

The Illig is a fantastic instrument. It is a refractor which means lenses are used to focus the image. With a 150mm (Six-inch) lens and a fast F/7.2 focal ratio, the Illig marries a wide field-of-view and very bright images. This combination is key to providing wonderful imagery.  The telescope, mount and image capturing software are very easy to set up. Observatory set-up procedures can be found on the HAL website, so I won't get into the particulars here.

Even CTO's don't know everything about the observatory. Sadly, I spent the time I planned to capture flat field images searching for a key to a fuse box.

By the time Chas arrived to tell me there was no key to the fuse box, the sky had darkened making flats impossible to acquire. Moreover, star party guests began to arrive, so I nixed the idea of capturing calibration data and slewed the scope to the moon for the public to see. It saddens me that I couldn't get any flats. Many surfaces are dusty as can be seen in the following images.  At least the evening's result prove calibration data is not a prerequisite for obtaining pretty pictures.
Although we began the evening by pointing the scope toward well-known objects such as The Moon, Mars and Alberio, we did not begin saving images until the sky darkened sufficiently as to not overwhelm our long exposures. Generally, we kept to 30-second or 120-second exposures shot at 139 or 300 gain. Realizing the bulk of our imagery would be flawed as we slewed the scope between targets, centered the target on the frame and experimented with exposures, we hoped to get three or four good images of each target.
We began saving images while the scope was parked on M31, The "Andromeda Galaxy." 
My First Image with The Illig Scope.

Even the wide 73’X49’ field of the Illig cannot corral this huge galaxy. I used Pixinsight, a powerful yet notoriously difficult to use application, to process the images. I didn't choose Pixinsight for its features or to scare the casual photographer away. I needed it to create color images.
While capturing the images, I didn't notice that Sharpcap (the application we use to capture images) was saving the data in .PNG format. Superficially, PNG images appear to be monochromatic (black and white). A "debayering" process must be performed in order to tease the color information out of the image. I found Pixinsight had the best debayering algorithms for my purposes. Since I was already using PixInsight to debayer the images, I merely continued the process and used Pixinsight to stack the images as well. Trust me, I used none of Pixinsight's "magic" on these images.

Stack of four .PNG images before debayering. I increased contrast to show several "Dust Donuts" that appear because I was unable to acquire flat frames for the evening
You can avoid all this unnecessary complexity by saving your images in .TIF format which automatically generates color images that may be stacked and processed in a variety of free applications.
Back to the image: There are many unusual objects in the field. Of course, M31's companion galaxy, M32, may be seen. However, a lot of those "stars" in the foreground are not stars at all. Instead, they are globular clusters that orbit the Andromeda system 2.2-million light years away. 
Here is a shot of our image (upper) and an image I grabbed from the Internet at the site http://www.astroschmiddi.com/details.asp?ID=17,

Our Image of M31 (Inverted) with a few Globular Clusters Marked

Identification of Several Globular Clusters Image Credit - Martin Schmitt
I bet you never thought that you would be able to image extra-galactic globular clusters. 
Another galaxy in the area was M33, "The Triangulum Galaxy." Slightly farther away than the Andromeda Galaxy, M33 is a notoriously difficult object to observe and image. Its surface brightness is too faint to render the object spectacular in all but the largest telescopes.
Here is our effort:

Considering M33 was deep inside of Baltimore's light dome when we imaged the object, I think this is a great shot. Remember, we achieve this result without calibration data. We merely stacked the images and adjusted the contrast. M33 will be a perfect object on which to perform "imaging magic." Here is a quick process of the inner portion of M33 with a bit of "Local Histogram Equalization" applied. Again, just four images with no calibration data. 


M33 - Inner Spiral Slightly Processed

Some may believe our imagery of M57, "The Ring Nebula" to be disappointing. With its wide field, The Illig may not be suited for imaging small objects. If desired, a barlow lens may be attached to increase resolution at the cost of reducing the field of view. In this image, I like the appearance of the tiny nebula engulfed in a sea of stars.

Although that image consisted of 30-second exposures, I grabbed a few 120-second exposures while no one was looking. Knowing the ring would be overexposed, I really wanted to test the scope to determine how deeply we could image. I compared our star field to the website http://www.sky-map.org/.  As you can see, we easily captured 17th magnitude stars and the distant galaxy IC 1296 in these few uncalibrated images!


A more appropriate planetary nebula for the Illig, M27, "The Dumbbell Nebula" drew gasps as the first image appeared on the screen. Here is our stack of four images:

One of the biggest surprises for me was the results of our imaging of "The Deer Lick Group." These aren't bright galaxies. Instead, the main galaxy, NGC 7331 shines at magnitude 10.2, while those background galaxies to the right (the deer) shine faintly at magnitude 14. 

I believe it was Wayne Baggett who pointed out "Stephan's Quintet" in the upper left area of the image. Admittedly, I was surprised we could capture these 13th and 14th magnitude galaxies in a single image. Although observing Stephan's Quintet impressed all club members present, the tiny fuzzies did little to impress members of the public. Therefore, we moved the scope to another deep sky object in Pegasus, Globular Cluster M15


Another galaxy that surprised us was NGC 253, "The Sculptor Galaxy."  Technically the fifth brightest galaxy visible from Alpha Ridge, The Sculptor never gets high above our horizon and is often overlooked by mid-northern observers. I love this galaxy, having imaged it several times from Georgia and Florida.

Here is our effort. Like M33 in Triangulum, I believe this object would benefit dramatically with proper image processing treatment.



One of the last objects we imaged was "The Veil Nebula." This supernova remnant is extremely difficult to image beneath light polluted skies. Although I had a good idea where the previously imaged objects appeared in the sky, for some reason, I didn't really know where to find "The Veil." Soon after I typed in the proper NGC number, the scope slewed to a point in the constellation Cygnus nearly perfectly centering the famous foreground star, 52 Cygni!  A little contrast stretching brought out the nebula. Here is our effort:




By the time the time the public star party officially ended, M42 "The Orion Nebula" cleared the lip of the dome. Freezing and tired, we slewed the scope to this famous nebula. Although we weren't impressed with the results (the nebula was deep in light pollution and ground haze) we did get a jolt from the number of geosynchronous satellites passing the field. You can see a few passing in the lower right of this four-frame .GIF. What a great way to end the evening.



Late autumn star parties last forever. With the sun setting before 5:00 pm, our event had lasted more than six hours. As we packed up, I looked forward to processing the images over the next days.
Personally, I am proud of what we accomplished. Granted, if you look closely, you can see dust donuts created by the lack of flat fields and varying background brightness that are a hallmark of poor or no calibration data. Likewise, for better results, we should have taken more images of each subject. But, we were hosting a public star party. Of course, we prioritized showing our 75 guests the stars.


Single Image of The Sculptor with Large and Small Dust Marks Annotated
These images clearly exhibit the quality imaging any reader of this blog can accomplish with HAL's new equipment. You no longer need to know your way around the sky. The telescope slews itself to any object you desire. You no longer need to worry about longer exposures. The mount is rock-steady in its unwavering tracking. The observatory's television screen shows you each image you capture. All you have to do is put your images on a thumb drive and take them home to process and share with friends.

Keep Looking up to Clear Skies.

Ken Everhart

Wednesday, September 26, 2018

The Hidden Colors of Our Moon


The color of our moon fascinates me. It seems to be gray. In fact, Apollo images of the surface are often assumed to be monochrome until one sees the jarring color of a flag or gold-foiled instrument in the field. Recently, I was able to acquire colorful imagery of the moon. But, I cheated.

Apollo 11 Image of the lunar surface - Credit: NASA


On the evening of August 25, 2018, the clouds briefly released their summer-long rein of our skies. Dutifully, I set up the scope in our driveway. Although the Moon appeared nearly full in the sky, I planned to focus on the four planets huddled low in the southern sky.

Sadly, the planets didn’t look like planets. Instead of being reflected by the ridged mirror of my scope, the planets seemed to be mirrored by the surface of a windblown lake. Their tiny disks danced all over the field of view.  With the such poor seeing, there would be no detailed planetary imaging this evening. With the Moon nearly full, there would be no deep sky imaging. Having exhausted my list of targets, I slewed my scope to the Moon. As I planned to only image the planets, I spent little time polar aligning my scope.

Instead of honing in on the center of the lunar disk, the telescope pointed somewhat south of the lunar equator quite pleasingly framing the crater Tycho.

100-million years ago, a five-mile-wide asteroid or comet struck the Moon creating the crater Tycho. It is most famous for its impressive system of rays emanating from the impact site. Caused by  material ejected during the impact, these rays cover a large part of the visible face of the Moon. At first look, all rays appear to lead to Tycho.

I calculated the exposures and imaged the Moon in red, green and blue light. I knew that combining these three colors would result in a gray on gray image with no color apparent.

Armed to image the planets, my filter wheel contained more than the typical red, green and blue filters. Therefore, I was able to add imagery with an ultraviolet filter used to image Venus and a hydrogen-alpha filter left over from a past deep-sky imaging session. 

With 35 images in hand, I packed up and headed to the computer as clouds regained their rule of the night for the remainder of the month.
Some might find it odd that I chose the deep-sky imaging processing package. Pixinsight, to combine the red, green and blue channels of my data set. Pixinsight often is able to be tricked into combining lunar images. By registering the Moon images as “deep sky” and using star alignment, Pixinsight usually can register each red, green and blue image for easy RGB alignment and combining.

As expected, combining the red, green and blue images resulted in the familiar gray moon. I like the “shattered crystal ball” illusion. But, that is a result of composure rather than color.


Moon in True Color
Like most image processing applications, Pixinsight allows the user to display any image as “Red”, “Green” or “Blue.” To create a “Stretched” image, I assigned the h-alpha filter data to the “Red” channel, the green data to the “Green” channel and the ultraviolet data to the “Blue” channel.

The results surprised me. Parts of the Moon appeared to be a ruby red color while other regions appeared a steel blue.





Here is the same image set enhanced a bit.



These colors looked familiar to me.  In 1992, the Galileo Spacecraft flew past the Earth-Moon System on its way to Jupiter. Galileo used its cameras to image the moon in multiple wavelengths. Here is the results of one of those imaging sessions. The spacecraft was 262,000 miles from the moon but only 43,000 miles from earth. Therefore, the perspective is nearly the same as we see from the earth’s surface.

Galileo Mosaic of the Moon - Credit: NASA/JPL

At these wavelengths, color differences represent different compositions in the lunar soil. Specifically, the steel blue color of the lunar mare indicates a higher percentage of titanium that seeped from the lunar interior as molten rock flooded these areas.

I could enhance the color of my image to mimic the Galileo imagery, but I think that amount of enhancement is a bit gaudy.

It amazes me that today's amateurs are able to enter a realm previously reserved for spacecraft. Duplicating the Galileo imagery was a mere afterthought after poor seeing thwarted my planetary imaging efforts. I look forward to many imaging sessions using invisible light. I might even purchase a real infrared filter.

Keep Looking up to Clear Skies.



Images from The Illig Telescope

Last summer, The Howard County Astronomical League received a valuable gift.   Leona and David Illig presented us with a Takahashi TOA-15...