A couple of “messy” galaxies

Well... that's because I've always heard Messier pronounced like “messy A”, sort of. I never took French. If you did, and can pronounce Messier the correct way and it doesn't sound like messy A then let me know. Actually, don't. It doesn't matter.

Anyway, I took an almost clear night to work on the polar alignment and, as you know, the periodic error of the scope. This was the first run after that.

M74 1st night

This is M74, the 74^th object on Mr. Messier's catalog, which just happens to be a very faint galaxy in Pisces. After getting the scope set up and connected to the observatory network, I started imaging: 10 3 minute images with the luminescence filter, 5 with each of the red green and blue filters (3 minutes as well). Feeling pretty good, I was ready to close the observatory, so out in the cold I go. First thing I see is the corrector lens almost completely covered with not just dew, but some frozen dew. Not good. All is lost, I think. Out comes the hair dryer to clear off the dew, and the scope is put up for the night.

The very next night, I'm armed for bear. Well, I take out the hair dryer first thing, anyway. Scope set up, cameras installed, autoguide calibrated, so over to M74 I go for round 2. Back inside, watching the autoguide corrections, it blatantly apparent the seeing is really bad, especially compared to last night. Well, everything is set up, I'm inside and warm, let's give it a shot.

M74 better, I think

I finally decided the seeing was at least twice as bad as the night before, but, I suppose because I wasn't shooting through the cloud on the end of the telescope, I was able to get at least as good of an image with a much shorter imaging run. In this case it was only 5 3 minute luminescence images, and 3 3 minute images each of red, green, and blue. Look closely and I hope you will agree that this one is better.

After imaging M74, I decided to try M33, the galaxy in the constellation of Triangulum. Nothing had improved, seeing wise, so I didn't hold out much hope.

M33

However, it turned out better than I thought it would.

M33 is about 3 million light years (ly) away, about the same as M31, the Andromeda galaxy. It appears that there is a gravitational link between M33 and M31. M33 is about 65,000 ly in diameter, compared to M74 which is about 95,000 ly in diameter. However, M74 is about 10 times further away, about 30 million ly.

Now for something a little different.....

Taking images of the night sky definitely takes some time to learn how to do. There are lots of problems, besides the clouds, that need to be addressed. One of those is called Periodic Error. Periodic error is the result of inaccurately manufactured gears in the scope drive mechanism. Can the gears be manufactured to not have periodic error? No. Interestingly, the difference between a $500 mount and a $50,000 mount, as concerns periodic error, is that the $50,000 mount has a predictable, repeatable periodic error. Why is that important? Because the predictable periodic error can be mostly programed out. All new, computerized telescopes has PEC, or Periodic Error Correction. If we look at an image, how does this show up? If, in a perfect image, a star shows up as a dot (.), the star image of a mount with periodic error looks like a horizontal line (-). (That's not the only thing that can cause the horizontal line, but we will assume everything else is OK.) Periodic error causes the mount to speed up and slow down, above and below the tracking rate that it needs to be at to perfectly track the star. PEC in essence, records the correcting speed changes and applies them (plays them back) to correct the tracking speed as best it can.

Let's see what this looks like on my mount. (Maybe I should inject at this point that a “telescope” is actually made up of 3 parts; the base, the mount, and the optical tube.The base sits on the ground. The mount sits on top of the base and holds the optical tube. If the optical tube tracks the sky, the mount is the part that does the moving or tracking. The optical tube is the part that you look through to see the stars.)

Periodic error uncorrected

This graph shows the periodic error of my Meade LX200GPS (ca 2002), uncorrected. This is actually 3 “runs” of the gears, or 3 periods of the gear, susperimposed on each other. It's fairly consistently +10 to -22 arc-seconds. That's apparently fairly common for this type of scope and definitely would cause the star to look like a horizontal line. After analyzing and “curve fitting” a correction curve, the graph looks like the right pane of the image below.

Left, before. Right after. Both at same vertical scale

The left pane is the same before graph shown at the same scale as the after graph. Look at the vertical scale, on the far left of the graph: the after is about +2 to – 4 arc-seconds. That's a pretty good improvement; one which, hopefully, can be autoguided out.

By the way, the graph shows something called “RA worm phase.” What this refers to is the gear that moves the scope to track the stars. The gear is called a worm gear. For more information, and to see what one looks like, see : https://en.wikipedia.org/wiki/Worm_drive

Rain, rain, go away.....

Originally written November 9, 2015 published November 18, 2015, but I've been busy :)

I heard the weatherman on one of the local TV stations say tonight that it has rained 15 out of the past 16 days. Why he didn't say it has rained the past 15 days and left it at that I don't know, but... it has been rainy and cloudy for a while. Fortunately, I took advantage of the few dry days before hand to gather some images and do some experimenting, which I like to do. As you would expect, some efforts were better than others.

Let's start with the NGC7380, The Wizard Nebula. 

NGC7380

I originally thought I might publish this as a Halloween “present”, but things didn't work out that way. The images was taken on the night of October 8^th. Credit for discovery is given to Caroline Herschel who found it in 1787. It is said to be extremely difficult to see visually. I find it interesting that NGC 7380 refers to the open cluster of stars within the nebula. NGC 7380 is located in the constellation of Cephus and is about 8000 light years (ly) away. As with many objects in astronomy, I don't see the namesake. Do you see a wizard?

M31, The Andromeda Galaxy

M31 Parts 1 an 2

This galaxy is said to be very similar to the Milky Way. It's a giant, spiral galaxy. It's bright enough to be seen naked eye under only modestly dark skies; I've seen it from Starlight naked eye several times. It's an easy target for binoculars from almost anywhere. It's about 2 million ly away and headed this way (or we're headed that way, take your choice; it's all relative). The reason for two images is that it's so big, it won't fit in one. Actually, this is one of my experiments. I knew it wouldn't fit in one frame, so I wanted to see if I could “stitch” the two images together. One image was taken the night of October 18^th and the other October 19^th. I made them as nearly identical as I could, but the area where the images join is extremely obvious. I haven't found a solution to this problem as of yet, so I let the two images separate for now. By the way, that little "fuzzy dot" in the lower left hand corner of the bottom image is actually another galaxy, M32.

M57, The Ring Nebula

M57

This is a perennial favorite. M57 is the ionized gas that was ejected, it you will, from a red giant star as the star collapsed into a white dwarf star (in the center of the ring). It's about 2300 ly away in the constellation of Lyra. Unlike the Wizard Nebula, this one is easily visible in at least a 20cm (8”) telescope. As with almost all deep sky objects, it will most likely be gray vs. the color you see here. Some people report they can see some color (shades of green, I think) if they have a large scope and are viewing under very dark skies.

And finally Rx And

Rx And

Rx Andromeda is the name of a variable star in the constellation of Andromeda, not a prescription for a star pill. However it is a prescription for fun. The star shown below (with the arrow pointing at it, of course) is Rx And. So far the variation has been measurable, but slight. It would be best to measure the variation on a consistent basis, like every night. With the rain we have had lately, I'm lucky to measure it once a week, and so far I haven't been able to do even that. Oh, well. Hopefully, I will be able to image it more often soon, and be able to show the variation here. We'll see.

Spiders in the observatory

Last night, October 14^th, I found a face-on galaxy (vs. an edge-on galaxy; this just refers to the orientation of the galaxy to our line of site. Face-on would be like looking at a plate from above the plate, but I'm sure you've got the idea by now.). The galaxy is NGC6946 in the constellation of Cygnus, the Swan. Cygnus is also known as the Northern Cross. Looking at the image, can you guess that the Milky Way runs thru Cygnus? All of the stars, individual stars that is, are in our galaxy, which is, of course, the Milky Way galaxy. That also means that the stars are foreground stars (they are between us and NGC6946). 6946, also know as the Fireworks Galaxy, is about 10 to 20 million light years away. I guess someone's tape measure ran out, so they had to estimate the distance; that's a factor of 2 in the estimation. I guess I shouldn't give them too hard of a time; the methods of estimation for that distance are all indirect methods and very hard to do. I guess I should cut them some slack. I guess that 3 sentences in a row I've started with “I guess”, (nope...4). Sorry. I don't know if anyone but me reads this, so I'm just having fun...

This image was tough. Tracking problems. Focusing problems. I can't say it's one of the best, but still not too bad. Maybe I'll try again on this one later. When I was processing the image, and just beginning to “pull” the image of the galaxy out of the background, my first impression was, “this thing looks like a spider!” Well, it's fall, and there are spider webs all around; I guess I had spiders on the brain. What do you think?

NGC6946

 

Same equipment and standard processing

I “see” you very well

Seeing, in astronomical terms, is most simply how well we see anything in the heavens. I includes basically 2 terms: transparency and steadiness of the air. Last night was the steadiest I have ever seen the air at the Starlight Observatory. At least for the 2 hours I was able to do some imaging. After that, it clouded up. Sigh. But this afternoon is clear, so maybe tonight will be good as well. We'll see.

Last night's target was NGC7331. That's a galaxy in the constellation of Pegasus, which is rising in the East. Today has been a busy day, so I've had time only to process the image, below, but at least one of the interesting things about this image is that it shows 6 galaxies. They will look like fuzzy stars, other than 7331, of course. I have tentatively identified them as all NGC ( New General Catalog) entries and are 7315, 7331 (of course), 7335, 7336, 7337, and 7340. Four of them are below 7331 and 7315 is to the upper left. See if you can find them. When I have more time, I'll try to give more info on them.

NGC7331

 

 

 NGC7331

8" LX200GPS F10 

QSI binx2 3 Min exposures

LRGB Lx7, Rx5, Gx5, ,Bx5

October 6, 2015

A tale of two Crescents

Thursday night, the 17^th, was another fairly clear night. So, out to the observatory I went. It was a night that I didn't have high expectations because of the 1^st crescent: the moon. For someone trying to image deep sky objects, the light from the moon causes the contrast to decrease significantly. Also, for us earthbound inhabitants, the sky is never really black. While it may seem inky black, it is only a very dark gray at best. That would be because of the lights here on earth that disperse in the atmosphere and light it up. It's called skyglow. OK, there are a few other contributors to skyglow, but man made light is the primary one. When I take an image, it's done by taking a series of images, usually with one each of 4 filters, for a certain length of time and then “stacking” them together. There is a stack for the red filter, blue filter, green filter, and a luminosity filter, which is basically clear, but it blocks infrared light. The 4 stacks are then combined to achieve the color image I present here on this blog. However, if I were looking through the eyepiece, all the images here would appear gray. See the entry for M20. So, if the moon lightens the background gray to the same shade as the nebula I want to see, the nebula effectively disappears. The longer light gathering time of a camera helps with pulling the nebula out of the background, but the fuller the moon, the brighter the background and the harder time I have pulling out the dim objects like a nebula.

Well, that brings us to the 2^nd crescent; NGC6888 or the Crescent Nebula. 

NGC6888

 

 

8” LX200GPS F10, QSI 683

LRGB 33,3,3,3

Imaged in Nebulosity 3

Post processed in Nebulosity 3 and Paint Shop Pro 7

(lots of 3's, huh?)

This image is a stack of 9 minutes each of red, green, and blue, and a stack of 33 minutes luminosity. (Most of the detail is to be found in the luminosity channel.) NGC6888 is formed by the fast stellar wind from the Wolf-Rayet star WR 136 (HD 192163) colliding with and energizing the slower moving wind ejected by the star when it became a red giant around 250,000 to 400,000 years ago. Thank you Wikipedia. At least, that's what I understand. The remaining star is call a Wolf-Rayet after Charles Wolf and Georges Rayet who discovered them in 1867. NGC6888 is about 5000 ly away in the constellation of Cygnus, the Swan (aka The Northern Cross). The reason for so many other stars in the image is because the Milky Way galaxy runs right through Cygnus. So all of those little dots of light are stars in our own galaxy.

Flying with the Eagles

Georgia has had a nice weather event lately; a passing cold front. A REAL cold front. The temperature has dropped about 20 degrees and the skies have cleared as much as I have seen them clear this summer. I have finally gotten a few good nights under the stars. No moon, Milky Way visible. Nice.

For the most part, the equipment has been working OK. I have imaged a few more things, most Messier objects. I got M17, M18, M69, M70, and M16. 

M18 is a open cluster. 

M18

It just looks like a bunch of stars to most folks. What's the big deal. Well, the deal has to do with the fact that all the stars are gravitationaly bound to each other and thus travel through space as a unit. Think of a school of fish in the ocean. I've read something that I currently can't remember about open clusters; something about their position is galactic evolution. I need to find that again, rather than giving out information that I'm not sure about. 

M69

M70

 M69 and M70 are both globular clusters. Same general idea as the open cluster, but obviously much more compact. They usually have many more stars, are usually much older, and generally orbit in the galactic halo, which means above and below the plane of the galaxy. At least that's what I remember about them. M69 and M70 are each only one photo, each a 1 minute exposure, and for the technically minded, only dark subtracted. They are interesting to image, since my eventual goal is to measure the light variance in variable stars. Imaging stars has it's own set of problems, compared to imaging nebulae and galaxies. Obviously, I hope, imaging variable stars will be more akin to imaging star clusters than nebulae.

M17 I've already processed.It's below.

 M16 I just finished, and is the longest exposure I've taken to date. 

M16

M16 is interesting for several reasons. First, it's an open cluster with an associated nebula. That makes the imaging harder, because the dynamic range is larger. What's dynamic range? It's the difference between the brightest object and dimmest object. Think of taking a picture of a flashlight with the sun in the same picture and trying to show the light coming from both. In this case, the stars to the upper right are fairly bright, but the nebula is really dim. There are several ways to solve this; mine was to set the exposure so that the stars did not reach saturation and then try to pull out the nebula in post processing. Since I consider myself a beginner at this, I was pleased with the result. Second, M16 contains the “Pillars of Creation.” See link. They are visible in my image, but the Hubble images in the link are the impressive ones.

Well, if we get some more clear nights, I'll see what else I can get. M31 is possible, but will be time consuming. It will have to be a mosaic; it won't fit on the sensor in one shot. It will be a multi-night imaging session and will probably be better later when it's higher in the sky. For now, I guess I had better go fix the leaky gutter. Yay.

PS. It just occurred to me to mention the "other" eagle; Aquila, the constellation. It contains the bright star Altair, one of the summer triangle stars. Aquila is not all that far from M16, relatively speaking, of course. They are both visible right now.

Two almost clear nights in two weeks!

And I took at advantage of the second one as well, at least for a couple of hours. It seems like this year has been the wettest or cloudiest one in recent memory. There has still been the persistent high cloudiness even on the “clear” nights, which makes the stars harder to see. I did some imaging anyway, this time of M17 and M18. These are located close to Sagittarius and close to each other; might as well take advantage of making a minimal telescope move. So far, I've been able to process only M17, which is also called the Swan nebula, Omega nebula or Horseshoe nebula. I'll let you decide if you can see it; I can't.

 

 

This image presented a different kind of challenge in the post processing. If you know about taking astrophotos, you know about “hot pixels” and thermal noise. If you are not familiar with the ideas, the easiest image I think I can make for you would be something like this: Imagine taking you camera and putting the lens cover on so that no light can reach the sensor (film, if you are thinking in terms of a film camera. However, this phenomena occurs only with digital cameras, so...). The expectation would be that the “image” would be completely black. It isn't, however. Close inspection shows white specks, like salt sprinkled on a piece of black paper. In actually, the image, if “stretched” (meaning putting the black and white points close to each other,more or less) would look like a snowy tv picture with white dots on it. The snow is the thermal noise and the white dots are the hot pixels. A hot pixel means that the pixel puts out too much voltage (meaning whiter) when hit be a photon. As more of an example, let's suppose that normally a photon that hits a pixel puts out 1 volt (it doesn't, this is just an example). If the pixel has 0 (zero) volts, it is completely black. If the pixel is hit by enough photons to allow it to reach it's maximum voltage, it would be 65,565 volts (or there abouts), and would be completely white. In between, we would see it as a shade of gray on a monitor. There is normally a direct relationship between the number of photons that hit the pixel and the voltage; if 20 photons hit, the voltage is 20 volts. If 1000 photons hit the pixel, the voltage is 1000 volts. With a hot pixel, it might be hit by 1000 photons, but instead of 1000 volts, it puts out closer to 65,000 volts. So, my problem was too many hot pixels in the photo.

So, what do they look like?

 

The red, green blue pixels circled are what they look like. Why red, green, and blue? My camera is a black and white (or monochrome) camera. To get color, I have to take series of photos with red, green and blue filters in front of the sensor, then, as part of the post processing, combine them to make a color image.

There are a few things I can do to help reduce them, like cooling the sensor more. I currently operate it at -5 degrees C, but I think I can get it much cooler. That's on my todo list. But what to do about the photo already taken? Well, in the post processing phase of working on the photos, (post, in this case referring to after the photo has been taken), there is a technique to help reduce the effect of noise by using a median filter. Think of if like this: the noise shows up as a white, or light colored dot of the monitor. If it were a drop of white paint on a black piece of paper, we could diminish the effect if we could smear the drop around the paper. The greater the area we can smear it over, the less noticeable it is. If the photo is 10 megapixels, and 100,000 are “hot”, that's a lot of smearing to do. There is another way to accomplish mostly the same thing. If I resize the image from 10 megapixels to 5 megapixels, the resizing algorithm has to throw away 5 megapixels. How does it chose which ones to throw away? I don't know the ins and outs of the algorithm, but part of it works like a median filter; it basically looks at all the pixels around a single pixel and “throws away” any ones that are vastly different from that pixel. That's how it helps eliminate the hot pixels. How well did it work? It eliminated about 90% or more of them. I think by using a cooler sensor and using this “trick” I should be able to make a major increase in quality of the photos, at least as for as the noise problem goes.

A long dry spell

Ironically, a long dry spell in astronomy is usually, but certainly not always, caused by a long wet spell meteorologicaly. If not wet, cloudy at least. Such has been the case for the past, almost 3 months at Starlight Observatory. However, Friday night, September 4^th, it wasn't AS cloudy. A few stars were visible, but there was a definite layer of haze or high cloudiness. Nevertheless, it was the best we've had for a long time. So.... Observatory opened, camera connected, security light out (more or less... it kept coming back on. Maybe the batteries in the laser are getting weak. What laser you ask? Why, the one that I point at the photoelectric cell that turns the light on and off. If I'm able to hit the cell with the laser light, the light goes off. It sounds easy, but try hitting a 1 inch diameter target from 40 feet with a light beam on a creaky old camera tripod; sometimes that is where most of the night is spent!).

This was also an opportunity to try something new; in this case, I was going to spend most of the time recording photons on the Luminosity channel, with a minor amount of time on the Red, Green, and Blue channels. But, alas, the air was not steady. We apparently had a thunderstorm to our northeast; I could see the horizon lit up by the lightening flashes. It would seem that the outflow from the storm was causing the unsteady air. As a means of “tracking”, I use a 2^nd camera to monitor the position of a star. I then feed that information to an “autoguiding” program, which, in turn, sends correcting signals to the telescope mount to keep the star centered in it's tracking “box”. The tracking program displays the errors in tracking, which, on Friday night, were in the 2 to 3 arc-second range. The actual movement of the star was probably 5 to 6 arc-seconds, so I felt pretty good about getting down in the 2 to 3 range. This is where having a spare $35,000 or so would come in handy; I could afford a mount that could track better, say to within 1 arc-second. I don't see that happening any time soon, though.

Anyway, time to shoot. The target was M20, also know as the Trifid Nebula. This is a primarily emission nebula in the constellation of Sagittarius. I managed to get 3 three minute exposures on the Luminosity channel, and 1 three minute exposure in each of the Red, Green, and Blue channels. These four channels would be combined later, in the computer to form one color photo. “Well, what does it look like?” you ask. See for yourself.

M20, September 4, 2015

8” LX200GPS F10, QSI 683

Shot thru high cloudiness

Imaged in Nebulosity 3

Post processed in Nebulosity 3 and Paint Shop Pro 7

This was an interesting, to me, experiment. I wanted to see how well I could image through the high clouds or haze or whatever it was. It's far from a ”perfect” picture; I'm not using the Hubble Telescope and don't have government funding for the computers and software. But, for an amateur with my experience level, I think it's OK. I can, and so can you, see the cloudiness show up as what looks like a hazy background color instead of a really black background. Tracking wasn't perfect, but not terrible, considering. (The stars look basically round, which is an indicator of good tracking.) The colors are at least in the ballpark of what they should be, but there is an artificial look to the nebula, caused by the processing trying to remove the effect of the cloudiness. There were other processing artifacts that I had to remove manually.

The last thing I thought I would try to demonstrate is what the nebula would have looked like if seen through and eyepiece, ie, you were looking through the telescope instead of me taking an image. The following is an attempt to show you what you would see.

M20 as seen though an eyepiece at the telescope

There are a few things to note. First, and foremost, it's hard to see. There is a reason astronomers call these things “faint fuzzies”. The word nebula comes from Latin for cloud. Whisp of a cloud seems appropriate here. Second, the sky is not black. That's because of 1) the cloudiness, 2) light pollution (meaning the lights of all the surrounding cities shinning up, into the clouds and into the 3) water vapor (in the air, of course). All 3 of these things scatter the light, making a dim object dimmer, as well as removing the contrast between the object and its background. Polar bear in a snow storm type of thing.

Well, that' it for this entry. Maybe late September and October will bring better weather for astronomy. Thanks for staying awake this long...

Finally got one night under the stars at the Starlight Observatory. That's the good news. There were, as usual for this time of year, some high cloudiness and haze, as well as a few big, puffy, sky blocking clouds. Oh, well; you take what you are given. At least I knew I wasn't going for any of the "faint fuzzies"; it would need to be something relatively bright. The only thing that fit that bill was Saturn. The main battle for this night was the unsteady air, also know as poor "seeing". The image below is a "stack" of 200 separate images to make one image. It was then processed, meaning mostly that I used blurring and sharpening techniques to produce the best image I could get, given the poor, but normal for summer, conditions.

Saturn: stack of 200 images from ZWO ASI 120MC, Scope 8" LX200GPS @F10, Stacked in Registax 6.0,wavelets applied, cropped and further blurring and sharpening in Paint Shop Pro V 7.

Just returned from our trip to Texas

August 1 2015
We took our daughter and grandkids on a road trip to visit our son (and new wife) in Houston last month. Along the way, we encountered 2 interesting problems with Lucy, a 2009 Lazy Daze Mid Bath motorhome. One problem was with the airconditioner, which was much needed on this trip, and the other with the automatic transfer switch, which is also know as a line-generator switch. I wrote up the situation while it was occurring, so I'll just cut and paste that in now.

July 21, 2015

Air conditioner and ATS difficulties on trip

Air Conditioner

Problem: Water dripping into motorhome while parked and air conditioner running.

The amount of water was not a lot, maybe a tablespoon or 2. It usually dripped from either the lowest point of the inside shroud or the passenger side air inlet area (which, because of being slightly out of level was probably the lowest point). The first occurrence was after a heavy downpour at Gulf Shores AL. That implies that the gasket seal of the roof air conditioner was possibly a little loose, so, the inside shroud was removed and the 4 “holding” bolts were tightened slightly, not over a ¼ turn. (Shroud is removed by taking out 8 phillips head screws.) Shroud replaced and on we go about our business. Next day, which was sunny, same problem. Hmmmm. Now it sounds like the drain pan may be stopped up. On to the roof, tools in hand. Outside shroud is removed by removing 6 phillips head screws. At this point, it should be noted that the outside portion is mounted on 4 rubber feet, which maintains about a ½ inch gap between the bottom of the outside portion of the A/C and the roof. This is necessary to allow the water in the drain pan to flow out from under the outside A/C. With the shroud off, there are 2 radiator coils needed for operation of any A/C. The one at the rear (stern, if you will) of the motorhome is the condenser coil, and is the “outside unit” that you see if you have a home A/C built into your furnace. Technically, this is called a “split” unit, because the condenser coil is outside and the evaporator coil is inside in your furnace. On our rooftop A/C, the condenser coil is visible, and forward of that, with the motor in between, is an enclosed “box” containing the “inside” unit, which, by now you should know is the evaporator coil. It's this coil that removes the heat from inside air, or said another way, it provides the cool air when the A/C is running. To see this coil, and get to the drip pan, we need to remove the 5/16 inch hex head screws on the cover. There's probably 15 or so of them. Then carefully remove the cover: it's sealed to the surrounding metal to separate the cool air from the outside air. The drain pan is toward the rear of the coil (nearer the motor), and has 2 plastic outlets on either side of the pan to let the water out. Take a cup of water up, and pour it over the coil or into the pan to be sure the outlets are free flowing. If you have a soft brush, like a paint brush, you can also clean the dirt off of the evaporator coil while you are there. It would be a good idea to do the same for the condenser coil as well. Be aware that the fins on the coils are sharp enough to cut, so watch those fingers. OK, now I'm sure the coils are clean, the drain pan is not stopped up, the gasket is tight, the unit has a ½ inch gap under it, I've removed the wasp and dirt dobber nests (oh yeah, I forgot to tell you to watch out for those; sorry), everything is back together and, drum roll please, it still does the same thing. So what's wrong now?! Actually, I think, nothing. Take a step back and look at the big picture. I'm on the gulf coast in July. That means temps in the 90 to 100 range, and humidity levels in the 80 to 90% range. A/C is going to run most of the time, and put out some quite cold air after a while. We also have 5 of us in the motorhome: wife and I, our daughter, and 2 grandkids (4 and 5). That's a lot of water vapor to pull out  of the motorhome, and while the A/C is in the process of taking out the water vapor, there is always some left in the inside. I think that when the very cold air is hitting the plastic inside shroud, water vapor is condensing on it and THAT is the cause of the tablespoon or so of liquid water that I see dripping inside the motorhome. The fix? Twofold, in this case. 1) That fan moves a lot of air, so I also check the filters, which really don't look very dirty. Oops; when I clean them under running water, they start to look a lot cleaner.  2) Move to a less humid place for a while, which is what we did. No more drips. Well, my wife still thinks I'm kind of a drip, but that's another story. So, the final answer was basically, make sure the filters are squeaky clean when in a very hot and humid environment, like the Gulf Coast in mid July, and expect the possibility of a little condensation while in that environment.

ATS, or Automatic Transfer Switch, or Line Generator Switch.

So, with 90+ degree temps and 1000% humidity, you might think having a good A/C might be a good thing. So do I. As we go driving down the highway, we decide to turn on the roof A/C as well as the dash A/C to help with the massive heat build up. Ok, so everything is going along fine until we notice the roof A/C is off. Generator is still running, so it will come back on in a minute. Nope. A few minutes more. Nope. “Joyce, go look at the (Progressive Industries) surge protector and be sure the light are blinking,” I say. No lights. Hmmmm.... Better check this out. Why is the generator running and the surge protector off? Well, we park for the next few nights, plug in to 120V on the post, look at the surge protector and pray. Everything appears to be working. So, what's going on with the generator? Last year, the power generating part of it was replaced after it self destructed, (at about ½ the cost of a new generator, ouch!), so what did the generator guy miss? Now the troubleshooting begins. Kids at the beach, so wife and I pull the power panel out to look at the input of the ATS, which is a lot easier than trying to measure the output of the generator AT the generator. I should note at this point, if you haven't already figured it out, I fed the output of the transfer switch to the surge protector, which protects me from a problem from either the post OR the generator. OK, generator running, voltmeter/frequency meter plugged into an outlet, A/C and refrig on, just like when driving. Of course, with the A/C running, I'm going to know when the power cuts off, but not if the reason is a change in frequency (from 60 Hz), that the surge protector will stop the current from flowing for. Well, 40 minutes later, everything is just fine, thank you m'am, of course. Lets start unloading the generator and cut it off. Refrig, off. A/C off. Power, off. What? No change in the voltage or the frequency of the generator showed up before everything went dark. Generator is still running, and if you have had generator problems, you know that if it's still running, it's making power. Let's see, input to ATS from generator, fine. Output. Hmmm..... Black to White (hot to neutral) no volts. That explains no A/C. Ground to hot (black wire), 120V. ??? Ground to neutral, 75 volts? What's going on here? Well, it appears I have an intermittantly failing transfer relay that switching only one of the two wires that it needs to switch. I guess I'll know today, when the new one arrives, hopefully. 

        Now, for the rest of the story. It's been about 2 weeks since I wrote the previous paragraphs. No more leaks from the air conditioner and the problem was the ATS. The new one has worked just fine, thank you. Had roof A/C all the way home, which was good.

Now, if only the clouds will part, I hope to catch a few photons. It's been so long since I've been in the observatory, I'm not sure I remember how things work. Oh,well. That's why I make notes. If I can just find them.....

This is what staying up too late gets you.
On the early morning of June 14, 2015, and by early I mean 3 AM early, I finally had a chance to get back under the stars at the Starlight Observatory. This was only about the third time I have been able to do so in the past 6 or 7 months, mostly due to cloud cover, but also some travel and a lot of sleeping. After figuring things out that I have forgotten in the past several months, and finding out several more things by experimentation, I finally produced one, reasonably good photograph.

This is the Dumbbell nebula, also know as M27, and is found in the constellation of Vulpecula, which means "the little fox". It's found in the sky just south of Cygnus, the Swan, aka the Northern Cross.
M27 is called a planetary nebula, a kind of emission nebula consisting of an expanding glowing shell of ionized gas ejected from old red giant stars late in their lives. M27 is about 1300 light years away from us, and about 3 ly in diameter.