Rocky Mountain Star Stare (RMSS)

June, 2019, I traveled to our old home state, Colorado, for my first Rocky Mountain Star Stare. I had a great time, met some really nice people and really enjoyed my traveling companion, Phyllis (my new RV). The organizers did a first class job of running the event and even though I did NOT win the Lego Rocket in the giveaway, they did a wonderful job of making a guy who traveled all the from Pittsburgh feel especially welcome. Special thanks to Tom and Barry!

Phyllis performed admirably and kept me very comfortable during both the traveling and the stay. I broke up the driving days into more or less 500 miles each (~1500 miles each way) and took my time to stop and rest when I wanted or needed. Sometimes I went and made a real meal in Phyllis in the middle of the drive, and even stopped and took a shower in the middle of an afternoon. Some of these diversions were things I haven’t bothered to do on previous trips, but they really broke up the drive and I will continue to incorporate them in the future.


On this trip, I imaged two main targets. I completed one, the Propeller Nebula, and collected some data but not yet enough on NGC 6914.

DWB111 – The Propeller Nebula – Processed to attempt to differentiate between the emission nebula and the surrounding dust
Click on image to view on Astrobin and see more details about capture

The Propeller Nebula is located deep in the heart of Cygnus and the Milky Way. This area contains all kinds of Ha emission nebula and dust. My presentation of this subject is an HaRGB image that was processed in both Photoshop and PixInsight with an attempt to emphasize the dust. I received some very much appreciated coaching from my son (Josh Smith) in processing this image. For anyone who has seen his work, you know what a talented processor he is so this was a real pleasure for me, and even if it wasn’t for him, he surely acted as if it was.

One of the most interesting things about this target is that nobody seems to understand what the heck this thing is or what causes its shape. I find that fascinating because it is a very popular target that is captured by amateurs and professionals alike, but in every description… “nobody really knows what is going on with this.”

To give you an idea of how differently the same data can be handled, take a look at the at my first pass at processing the same target. Still a pretty decent looking image, right? But, not really the same richness or depth or frankly, interest, as the “Rev 2” image above – at least in my opinion. And certainly it has a very different appearance.

DBW111 – My initial attempt at processing this data. Heavy on the redddd.

Just for fun, I have included a few short time lapses from the Star Stare. The first one is of my telescope setup process. I wanted to capture the snow capped mountains in the background, so I had to set up the camera a long ways away, then zoom in quite a bit during post-processing.

When there are clouds passing that dramatically change the light there are different ways to handle the situation. In this case, I focused on the sky and kept the brightness of the sky constant while allowing foreground brightness to vary. Often this has the most natural appearance because the sky doesn’t really change brightness very much.

Wonderfully fast telescope setup at Rocky Mountain Star Stare

In this case, though, the varying foreground seemed a little jarring, to me. More experimenting is in order, I think.

I also did a time lapse of setting up my SkyBox to help keep the telescope more protected during the forecasted winds for some evenings. In contrast to the previous time lapse, this one was processed to hold the foreground brightness consistent and let the sky vary as clouds rolled past.

John Love’s SkyBox always draws attention

And finally, perhaps, a more interesting time lapse for astrophotographers, is the following abbreviated test I made of a Rokinon 8mm f/3.5 Fisheye Lens. This was captured with my Canon 70D. Exposures varied but by the time it was fully dark, the lens was fully open, and I was capturing for 20 seconds at ISO 1600. Processing was in LightRoom and LRTimelapse. The bright planet that you can see even before dark is Jupiter.

This was a test of my Rokinon 8mm f.3.5 lens. Processing is through LightRoom and LRTimelapse.

The RMSS presented some new challenges to me because it is the first event that I have attended since I started going to star parties in an RV where there is no field power provided. I haven’t lugged around extra batteries with me for several years, so I decided that I was going to try to run my telescope gear off the battery bank of Phyllis (my RV). “Battery bank” sounds exotic, but in my case it is really only two Trojan T-105 golf cart batteries. From a back-of-the-envelope calculation, I thought I would be okay, but to be honest, I was a little fuzzy on the details.

As a result, I spent some time studying about my batteries, their capacity, and their recharging. While this is probably uninteresting to anyone who doesn’t own an RV, I will still share some bullet points for my own benefit, if nothing else.

  • My battery bank capacity, if fully charged and healthy, is 225 amp-hours. My telescope gear, even with the dew heaters running draws 3-4 amps tops. The imaging window for me on this trip was something less than 8 hours per night… so my gear was using something like 30 amp-hours. This doesn’t include the power requirement to maintain or charge the remote laptop used to run the setup, which might be about the same amount of power as the rest of the gear. So if I were to fall asleep and allow the laptop to run all night, that is closer to a total of 60 amp-hours.
  • Even deep-cycle golf cart batteries would like to be discharged only to about 50% so in the worst-case scenario described above, I am roughly using half of my power capacity to run my telescope and laptop.
  • Phyllis’ needs can be quite variable, but if careful with the lights, she should only be drawing a few amps… unless the furnace is running, or the hot water heater (solenoid), or the Fantastic Fan. Then usage goes up dramatically.
  • But with care, and if my batteries are in good shape and charged, it seems like I should be able to use less than my 110 to 120 amp-hour budget over a night.
  • The challenge comes in when it is time to recharge the battery bank. For example, I have two 100 watt solar panels. The most optimistic estimates for their output under the strongest sun would be about 30 amp-hours each. That just isn’t going to get it done.
  • I have a generator that can output plenty of power to either run a battery charger or can power the converter in Phyllis that can then charge the batteries. In my case the battery manufacturer recommends a maximum charge rate of 10-13% of capacity or ~20-30 amps… and this is pretty typical. Unless there are a lot of DC loads that Phyllis is supporting, the internal converter (55 amp capacity) should be able to provide all of that and more.
  • The problem is really one of time. It take 3-6 hours of charging time at the full charge rate to reach 85% to 90% of charge for the battery bank. The last 10-15% can take that long again because the charge rate is necessarily reduced. So realistically, on a consecutive night two, it is difficult to be fully charged back up, given the amount that I potentially discharge my battery bank.
  • Finally, I learned that the best way to judge the state of health of the battery bank is to use a hydrometer and actually measure the specific gravity of the acid. There are very specific instruction on the Trojan website for collecting and using this information. I ordered a hydrometer, but I haven’t done the actual testing yet to see where I stand.
  • So my conclusions are as follows (subject to learning more, as always: 1) the 200 watts of solar panels are great and I feel good about using them and they will probably keep Phyllis topped off in situations where I have field power for running the telescope and not too large a load in Phyllis. 2) For nights where I am heavily discharging the battery bank, I need to run the generator. A lot. Six-eight hours per day seem to be needed to start out the night at nearly 90% charged. 3) Adding more charging capability or changing the converter probably will not make a significant difference. If I really want to do something, that thing would be to increase to a 4 battery bank, and then I might be able to make use of more charging capacity, too (ultimately this would be better because I could meet my power requirements without having to so deeply discharge my battery bank). The converter change might provide a subtle improvement both in charge time and in battery longevity due to a slightly better charging profile, but it would not provide major differences, all other things being equal.

Stay tuned. More to come.

Quick Update – MagicShirtAstro Facelift

Back from perhaps the best-ever OkieTex Star Party, I felt inspired to get organized with this blog and my image repository. And here it is. For the first time in a few years, all the images I care to share are back up on line. For anyone who cares to look at them, they are categorized into galleries in the right hand column. Makes me feel more organized and ready to process some of the data which I gathered over the last two star parties (hopefully at least three images are on the way). Also, I think the style and color scheme is much more readable that the old format.

Now, all of my images are stored within in the WordPress Media Manager instead of in a separate gallery. I have lost data (in the sense that I had to re-create it) twice in the separate-gallery model, while I have never had issues with WordPress. So, I am more confident in this as a solution. Even better, it is easy to create and modify individual galleries and best of all, they can each be formatted differently. This is great because with each astrophoto that I publish, I would like to publish text describing it’s acquisition. But for general star party pictures or for some tidbit about using the trailer at the a star party, it would be nice to have a slide show with only captions. Either way, it is nice to have options!

Of course, I can also upload images to AstroBin, too, but I just haven’t jumped into that arena, yet.

Back Patio Testing

Last weekend and this one, the skies were clear enough to allow a bit of testing on the back patio. The next few days will bring a more detailed entry on the steps between the WSP and today, but here is a little test image (actually a quick stack of 16 5-minute sub frames). Just enough of a taste to be encouraged I am on the right track with this setup. This is both the first automated test with SGP and the first successful test through the AT10RC reduced to somewhere around 1600 mm via the AP27TVPH.

M106 Test Image - from my back patio
M106 Test Image – from my back patio

It appears I can be a little less conservative with my pick-off mirror placement and also like I should get busy on my larger flat box and my collimation technique. But an encouraging start, just the same.

Winter Star Party Results – Part 2

Phase 3 – Initial Test with the AT10RC

Since things went well on the testing with the 110 testing, I moved ahead with testing the AT10RC, windy conditions be damned. Initial efforts were hampered in two ways. The first issue was a collimation problem with the after-market Moonlight focuser that I have installed on the scope. For some reason, it’s collimation is substantially off. Since I purchased the Moonlight focuser second-hand on the Mart, I can’t fault Moonlight for this problem, but through several tests, I was able to confirm that it was the focuser, itself.

(Note… this focuser is on its way to Moonlight for diagnosis)

In the interest of forging ahead with testing, I collimated the best I could, but the collimation was not satisfactory.

AT10RC Test Image at WSP - NGC 3628
AT10RC Test Image at WSP – NGC 3628

The second issue was only discovered on the spot when I couldn’t reach focus with a Telecompressor in my train… the Astro-Physics 27TVPH. I had all my adapters lined up, including a custom part from Precise Parts, but the overall assembly was a bit too long to come to focus. Of course, all of this messing around caused my camera orientation to change often and render previous efforts at telescope collimation moot. I will follow up more with this focal reduction and Moonlight focuser effort in a later blog.

In any event, I decided to plow ahead with marginal collimation and at the native focal length of 2000mm. The result is the first image in this article. It is a stack of 6 10-minute sub frames. The camera is my SBIG setup shot at 1×1 binning (somewhere around .6 arcsec/pixel). Despite the poor collimation, and the lack of flats to calibrate these frames, I am very encouraged by potential of this setup.

AT10RC Test Image at WSP - NGC 4438, Binned 2x2
AT10RC Test Image at WSP – NGC 4438, Binned 2×2

I also grabbed a few frames of NGC 4438 in Markarian’s chain at 2×2 binning. I only was able to grab 4 10-minute frames before morning twighlight.

There is still some work to do with the AT10RC besides addressing the focuser collimation and getting the reducer to work. I also need to refine guiding parameters, and may need to adjust the OAG pickoff mirror a bit more into the light path. But for a first test run, I am pleased.

Phase IV – Fun Stuff

Just for the fun of it, I am re-posting the images from this page… both images have arrows indicating asteroids that were captured. The first shows a bright asteroid, 1133 Lugduna as well as several other fainter trails. The second image shows Princetonia again, having moved closer to the subject galaxy from the capture in the previous blog post from the night before. Hopefully this asteroid stuff will become old hat, but it is pretty fun right now.

Note that you can see an animation of the image containing 5 asteroids here.

AT10RC Test Image at WSP - NGC 3628 with Arrows Indicating Asteroid Trails
AT10RC Test Image at WSP – NGC 3628 with Arrows Indicating Asteroid Trails

AT10RC Test Image at WSP - NGC 4438, Binned 2x2 - Asteroid Princetonia Indicated
AT10RC Test Image at WSP – NGC 4438, Binned 2×2 – Asteroid Princetonia Indicated

Image Through 110 Scope from Previous Night Showing how far Asteroid Princetonia Traveled
Image Through 110 Scope from Previous Night Showing how far Asteroid Princetonia Traveled

Winter Star Party 2015 Results – Part 1

The Setup

So I changed a number of things all at once. Not in a controlled, engineering way, but in a desperate Northeast Amateur Astronomy way that reflects precious few clear nights each year. Because I was heading off to the WSP with no opportunity to test my new Astro-Physics 1100GTO mount on targets more distant than the basement ceiling, I was determined to be happy with getting things up and running. Any images I was able to capture would be icing on the cake. And it would be warm.

In addition to the coming out party for the 1100, a major change from last season is the switch over to Sequence Generator Pro (Main Sequence Software) for image acquisition and session management. An immediate benefit of the switch to SGP is the opportunity to exploit their automated focusing routine. If all goes well, this will replace the clunky operation of slewing to a bright star to do manual focusing with a Bahtinov mask and then slewing back to reacquire the target. To slightly complicate things further, I am moving away from AstroTortilla’s blind solver as the primary plate solving tool and on to PinPoint as the main solving engine with Astrometry.net as the blind fail-over solver.

And finally on this trip, I wanted to test out an AT10RC scope that has been patiently waiting in storage for a ride on the new 1100. My plan was to test it both at native focal length and reduced with an AP Telecompressor (the 27TVPH).

So… I felt that if I could get most of these things tested and successfully running, it would be a very successful week. And it would be warm.

Phase 1 – SGP

2015 Test Image from WSP - M1
2015 Test Image from WSP – M1

As with any image in any of these blog entries, you can click on an image once to get a full browser view and click on it again to get a full, original resolution view. Click your browser’s “back” button to return here.

This M1 capture was the first capture with SGP. The main goal, other than actually using SGP was to use SGP’s focus routine. And getting the paths and file naming figured out. And interfacing with PHD2. And… well, you get the idea. M1 isn’t particularly suited to 770mm of focal length, especially when reduced to 616mm at f/5.6, but it was high overhead at the right time. This quick capture is a stack of 7 15-minute frames of Ha data. This isn’t cropped and shows pretty nice (but not perfect) star shapes all the way to the edges of the 8300 chip.

Phase 2 – Plate solving

2015 Test Image at WSP - Base of Markarian Chain
2015 Test Image at WSP – Base of Markarian Chain

Phase 2 included everything that was in the first phase, and added the variable of plate solving with PinPoint under SGP. For this target, I plate solved an image that has been a work-in-progress for the last two seasons, then allowed SGP to center the scope on that target by using PinPoint. The original target image is at the bottom of this post. All of the parameters are not completely settled, there may still be an issue between JNOW and J2000, and the fail-over solve is very slow right now. But the successful PinPoint solves were amazing… a second or less. Very cool and lots of potential.

This second image is made up of a stack of 9 10-minute sub frames. As with the first frame, the scope is a WO 110FLT reduced with the WO AFR-IV flattener/reducer. Camera setup is all SBIG: ST-8300, FW8 with Astrodons, OAG with st-i guide cam.

Crop showing Asteroid 508 Princetonia
Crop showing Asteroid 508 Princetonia

I didn’t realize it at the time, but I also captured the first asteroid that I realized I have captured… In this case it is 508 Princetonia… it is indicated in the crop from the larger image. Not that it is earth shattering, but it was additional spice to the testing week!

My reference image from last season used as reference for this season's test image
My reference image from last season used as reference for this season’s test image