Observing from Home – 11 August 2019

Conditions

  • 11 August 2019 – 22:00 (8/11) – 00:30 (8/12) EDT
  • mild – 60º-65º F; humidity 80-85%
  • Moon +11 days ~90% illumination
  • still; clear at first, but increasing clouds toward midnight
  • seeing – 6 or 7/10 – pretty good
  • transparency – inconsequential, as I was hunting orbs

Equipment

  • Celestron NexStar Evolution 8″ SCT
  • Eyepieces
    • 32 mm
    • 15 mm
    • 9 mm
    • 6 mm
  • 2x Barlow
  • Filters
    • Moon, blue, green, yellow

Objects

  • Moon
  • Jupiter
  • Saturn

Observations

A pleasant Sunday night. I pondered long about going out, because, much as I love the NexStar 8, it is a pain to drag it down to the pool deck. I finally discerned that my 3 targets – Jupiter, Moon, and Saturn – would be visible from the deck, so I set up in the northwest corner there. The problems were shakiness (really need to reinforce the deck at some point) and the TV aerial, which turned out to be right in the path of the moon and Saturn. The moon was just a few degrees W of Saturn, both sitting just above the Teapot of Sagittarius. Jupiter was 15º or so to the west just above Antares in Scorpius/Ophiuchus.


Moon

Southern region of the Moon. North is up. Just inside the terminator on the right (West) from bottom to top you can see Schiller, Gassendi, and Kepler, mentioned in the writeup.

I started with the Moon, using 32 mm = 62.5 X with moon filter and variations with 15 mm, 9 mm, and 2x Barlow. I don’t know the moon that well, so didn’t do much more than identify several craters. In the SW quadrant; Schiller, , a long, squashed crater; Gassendi was just east of the terminator – large with prominent central peak; small Flamsteed; up to Encke and Kepler, just on the terminator. On into the NW, Prinz on the terminator, and I think it was breaking dawn on Aristarchus, which sounds like a new age album. Saw Bianchini and Sharp just outside Sinus Iridum. After that I made my way to Mare Tranquillitatis to see if I could find the Apollo 11 astronaut craters: three small craters in a row just north of the landing site and named Aldrin, Collins, and Armstrong. Turns out they are quite small. While theoretically in reach of my scope, I had two problems (at least): 1) I had neglected to add my dew shield and was starting to fog over, and 2) the aforementioned TV aerial was now sitting across the heart of the moon, so that I wasn’t getting good resolution, even at 222 X. [An article in July 2019 Sky&Telescope suggests a 6″ scope can make them out at 250 X with steady seeing.]


Jupiter

Moved on to Jupiter, sitting low in the SW. Tried pushing the magnification to 333 X, and it was just a bit too much. 222 X wasn’t quite enough, but I didn’t think to use the 15 mm + 2X for 266 X, which might have been Goldilocks. Oh well. The GRS (Great Red Spot) was just past transit, very well placed, but so small! It was fairly obvious but just a tight, dark knot (nought? not.) in the SEB (Southern Equatorial Band), which itself was quite light. The NEB (Northern…) was dark and thick, and some “barges” were visible. The equatorial zone remains heavily shaded, darker than the temperate zones. One northern temperate band was visible. The GRS rotated about 2/3 to the limb while I observed, or so it seems to me as I write this. I tried a variety of color filters, including blue, green, and yellow. The blue highlighted the bands and GRS the best, as one would expect. Green and yellow both gave interesting interpretations but were ultimately not that helpful. Of the Galilean moons, I had just missed Io disappearing in eclipse as it turns out, and also just missed Ganymede emerging from eclipse at the other end of my observations. Oh well. Meanwhile, Europa was about 4 Jupiter diameters from the planet to the west. Callisto was about four Europa-Jupiter distances further to the west. I made a sketch at the eyepiece that shows the distances more or less. The GRS in the sketch is bigger than it appeared.


Moon, redux

Went back to the Moon for a bit after it cleared the tower, as it were. Took another stab at the Apollo 11 craters, but no. Poked around the southern highlands for a bit. I’ve always had a soft spot for Clavius, so I looked there for a bit. Noticed a few clouds moving in and wanted to get some Saturn time in, so moved there.


Saturn

Even with deteriorating conditions, Saturn looked pretty good. Again, pushing the mag, it was just a bit much at 333 X, so ended up with the 266 X combo I hadn’t thought of earlier. The rings are tilted so that the other edges are about lined up with the edge of the disk. It’s just a bit past opposition (okay, a month past), so there is just a little bit of shadow on the rings right at the pole, or that’s what I’ve gathered. Any way, the rings kind of squish at that point. Not much color tonight, just a yellowish tint. Darker in the N temperate to polar region with a slightly dark band at the bottom. Very 3-D. Cassini Gap easily visible.


Pics

I took several handheld pictures and videos with my phone at the eyepiece for all three targets. Moon was best, of course, then Saturn. Jupiter was washed out. Clouds were moving in, and I was tired, so I washed out, too.

Best shot of the Moon for the night. North is right and West is down.
Best of Jupiter for the night, which is not that great. North is upper left, West is to the lower left. More or less.
Saturn. Not as impressive as seeing it live. You sort of see the dips where the rings and the disk limb cross, right? North is right.

You can see the full series of pictures I took at my Google Pictures album, >here<.


Observing from Home – 1 July 2019 – The rest of the story

In my last entry I included my first serious attempts at astrophotography with three pictures of Jupiter. Here, then, are my notes from that night’s observing in general.

Conditions

  • 1 July 2019 – 22:00- 00:30
  • warm – 70’s; high humidity – 80%!
  • new moon, essentially
  • still, no wind
  • some streaky clouds, increasing through the night
  • seeing – 6/10
  • transparency – good enough

Equipment

  • Celestron Nexstar Evolution 8″ SCT
  • Orion StarShoot Solar System Color Imager IV
  • 2x Barlow
  • Eyepieces:
    • 32 mm – 62.5x / 125x
    • 15 mm – 133x / 266x
    • 9 mm – 222x / 444x — too much for tonight!
  • Filters:
    • blue, red, purple, yellow, sky glow

Objects

  • Jupiter
  • Saturn
  • M4
  • M8
  • M20
  • M17
  • M22
  • M27
  • NGC 6995

Tech!

Writing this several days after the fact, so we’ll see how bad my memory is. Of course you won’t know unless I tell you! A good bit of time was spent on the new attempt at technology and astrophotography, which ultimately proved successful, but it took a while. The interface between camera and computer is a bit dodgy at first. No image coming through, even though the cam had power. This may have been an interface issue or that the object in view wasn’t centered enough or large enough or focused enough to produce an image. I eventually added the 2x Barlow, doubling the image size and found Jupiter on the monitor in the preview window of the settings screen. In the actual preview window, though, the image was tiled into 4 images that were raked with horizontal lines. Unplugging and restarting the camera seemed to do the trick, and after only half an hour fiddling, I took my first .mov of Jupiter. It was grainy as hell, but I could sort of see that the GRS (Great Red Spot) was on the limb. Over the next 45 minutes or so I took 8 movies of 50-75 seconds each. I tried one of M4, the globular cluster in Scorpius, but that was just dark frames. This camera is not sensitive enough for faint deep sky objects. It barely noticed Jupiter! Any way, I’ve been processing the movies into pictures with some success. They are grainy, and I have much to learn about processing, but they aren’t bad for a first effort. I thought about recording Saturn, too, but I decided to keep it simple on the first try. I also hoped to see several objects by eye on a rare clear night. So I put the tech away and switched to visual.

Observations

Jupiter

I stuck with Jupiter for a good while. It is just past opposition, so it is a great time to observe it. It isn’t very high, sitting on the north side of Scorpius, a few degrees north of M19, about 28º above the horizon according to an app. It’s super bright at -2.6 magnitude. At 62.5x (32 mm) I could see 2 stripes on the disk, on moon to the W (Io), and three to the E. Mostly viewed with the 15 mm and 2x for 266x. It was a pretty stable view. Could make out the GRS easily. The NEB (north equatorial belt) was thick and rusty colored. The SEB was thinner and darker to the … W? of the GRS (toward the direction of rotation). The equatorial zone was orangy and the higher latitudes were lighter. Could occasionally make out another stripe or hints of one above the NEB. I think. Maybe I’m applying that back from my pictures, though.

I tried a couple filters – blue, purple, red, yellow. The purple was a complete washout, making for a big pink blob, and red wasn’t much better. Yellow was okay. Blue was by far the most helpful. That’s when I saw hints of other bands and hints of detail downstream from GRS. This sketch doesn’t look like much, but I watched for a long time with great enjoyment and fascination.

M4 Globular Cluster

I had swung over to M4 before as I mentioned, but went back for more visual. For as big as it is, it’s a challenge. Not to find it but to see it. The surface brightness is pretty low, and I often strain to keep looking at it. Maybe I should have dropped the magnification. I had a hard time making out any detail at all. Just a mess of stars on the verge of vision so as to make my eyes twitch.

M8 Lagoon Nebula

Moved on to several Sagittarius favorites. M8 Lagoon Nebula was beautiful as usual. Not as stand-outish is M42, but up there. Wisps of nebulosity with an X across the center and a swarm of small stars on the east side. At some point in the night I added my sky glow filter – I think much later and then I returned here, I forget – and it really helped bring M8 out from the background.

M20 Triffid Nebula

M20 is hard to compare to M8. Not fair, really. It’s a beautiful thing but so small vs. M8. I think I didn’t use the filter on M20, and it suffered for it. About 1/4 the size of M8 or less. Hints of more complexity maybe and hit of the central star. Should have used higher magnification and the filter. Next time.

M17 Swan Nebula

M17 is always fun to observe. Mostly looked like a checkmark, more than the full swan this night. Not as sharp a line on the swan’t “water line” as often appears.

M22 Globular Cluster

Just a quick look at M22. Enough to say I saw it. I think I was starting to get tired already. Sorry.

Saturn

Not sure of where it fits in the order now, but somewhere in here I went to Saturn. At fairly low power about 4 moons visible. (… Not sure what power I was using now that I think of it. I really need to start writing this stuff down as I do it.) At 266x it was a little rough but some detail. Still very low in the sky, about 20º above the horizon, so not great detail. Plus, it’s just about at opposition, so almost no shadows. Could generally make out the Cassini Gap, some shading on the planet disk. Rings are crossing in front of the disk. A dark band and gray cap on the top of the disk, but not much color.

M27 Dumbbell Nebula

Turning to the north, Cygnus had risen over the house to about 45º. I slewed to M27, a planetary nebula. It is large enough and bright enough that I wonder if it might appear in the SSSSIV camera. Round, but uneven, brighter on the “sides” than on the “top” and “bottom,” and brighter on one side than the other. It seems to shift as you look at it, though. I used 266x pretty much across the board on everything… I think, and I think I used the sky glow filter? Or maybe I came back to it after I added the filter? Maybe that, because I seem to remember adding the filter on the last target of the evening.

NGC 6995 Veil Nebula

I went to the Crescent Nebula, which isn’t really where I meant to go, which is fine, because I couldn’t see it any way. I chose it from the list of named objects on my paddle control for the C8. What I meant to look at and eventually got to was NGC 6995, the Veil Nebula. It turned out to be the Eastern Veil. This is a pretty bright ribbon of cloud in a long, flowing arc. There are two relatively bright stars nearby and not one bright one in the midst, the signature of the Western Veil. It has a few kinks and bulbs, as it were, and is quite an interesting object. Regrettably, I was definitely getting tired and didn’t give it the attention it deserves. It definitely benefitted from the sky glow filter.

I revisited a few previous targets, but as I said, I was getting tired. Plus more clouds were moving in. Plus the dew was getting heavy. In fact, I noticed as I was packing up that the scope’s corrector plate was starting to dew over. On the whole, a good night.

Observing from Home – 1 July 2019 – Pics or Didn’t Happen.

I haven’t written up my notes on this session yet, but I started trying some astrophotography, and that’s been taking some time and attention. It has taken almost a year to get the right combination of learning, confidence, and clear skies, but I finally got out with the astro camera I won at the Green Bank Star Quest 2018. It’s an Orion StarShoot Solar System Color Imager IV, and it doesn’t work with OS X above 10.10. So I had to partition my hard drive and reinstalled 10.8.5. Even so, it is a glitchy proposition. Nevertheless, I succeeded in taking a series of videos of Jupiter on 1 July and have been processing them into stacked photos with an old program called Lynkeos. It’s pretty easy to follow the steps. What is difficult is learning how to fiddle with the settings to maximize the results in the photo. I’m getting there.

So herewith are the three photos I have produced so far. They are stacks of about 350 images each, +/- 100. The images are from video taken between 22:30 and 23:18 EDT. I used the Celestron Nexstar Evolution 8″ SCT with a 2x Barlow lens. I did the stacking and initial processing in Lynkeos, as I mentioned, and finished the processing in GIMP. The first is larger because I processed it on my lappie while the other two were done on the desktop and the resolution settings were different. Haven’t really tracked down the exact cause.

Jupiter, 1 July 2019, 22:30 EDT, CT WV
Jupiter, 1 July 2019, 22:35 EDT, CT WV
Jupiter, 1 July 2019, 23:18 EDT, CT WV

So there. Now I’m an astrophotographer.

Description of the whole observing session to follow in a separate post.

Observatory 7 – Kitt Peak, Part 2

This post is about the evening program at the Kitt Peak National Optical Astronomy Observatory. For my post about the 3-tour daytime program, look >here<.

As I mentioned in that article, I signed up for both the daytime and nighttime programs for less than $100 total. They have several night programs, but the ones being offered that night were the Parade of Planets and Night of the Marvelous Moon. The former would enjoy the favorable alignment of Mars, Jupiter, and Saturn with, I think, a 20″ reflector in the dome at the visitor center, while the latter would probe our faithful sky companion, the moon, with a 16″ Ritchey–Chrétien reflector in one of the roll-off observatories up the path. I chose the Marvelous Moon based on the poor performance of planetary observing I’d had from the big scopes so far and on the forecast for a “mostly cloudy” evening due to the monsoon season. I figured if we were going to get to see much of anything, it would have to be big and bright.

The evening began before sundown with introductions and supper in the visitors center. Supper was a box lunch with a sandwich, chips, and a cookie (as I recall these several months later). There were about 16 people there for the programs, and it turned out that only two of us had signed up for the moon. The sky, which had been vacillating wildly all day between sun and storm, was still patchy, so there was hope. That made me feel a little bummed, though, because if there was hope, then there might be cool views of the planets, which I was going to miss. I had to discipline myself to enjoy the program I had chosen.

Sunset

Our first observing of the evening would be of the occultation of a nearby star behind the limb of a local planet, also known as “sunset.” (A little astrogeek humor there. Okay, very little.) We walked up the path to the rim of the mountain with a spectacular view across the valley to the west. The clouds were still hanging out but had broken up some, and as the sun got lower, they lit up spectacularly. Lots of reds, oranges, yellows, blues, and purples. There were places where I could see patches of rain falling miles away, even while the sun glinted off lakes and such in other parts. I experienced a good bit of it through my phone camera, I’ll admit, although I did stop a number of times to drink it all in directly with my own eyes. The good news is that you can share the experience since I was so digitally consumed. Click on >over here< to see my sunset pictures.

Marvelous Moon

Now that it was starting to get dark, we split into the two groups, going to our respective observatories, to respectively hope the clouds would respect us and dissipate. As we began our program on our Marvelous Moon, we had introductions, which was quick since there were three of us altogether. I have forgotten our instructor’s name, but my fellow participant was Jelena. It turned out that she works at the Lowell Observatory in Flagstaff as an event coordinator, and she was spying out what they could learn from Kitt Peak. Meanwhile, there was some lecture about our target that was clearly intended for astro-novices, so Jelena and I aced all the questions. I think Instructor was a bit new at that presentation, as he kept checking his notes and didn’t seem entirely comfortable with his patter, but he did a good job, nonetheless.

After our classtime to prepare us for looking at the moon, we went up to the scope, opened the roof, and …. well, crud. It was totally socked in. Of course. The clouds weren’t so dense that you couldn’t tell where the moon was, but they were dense enough that you could only make out the glow. We talked a bit about the telescope, its specs and mount and software and such. And we talked about some other stuff, stalling to see if maybe the sky meant to clear up after all.

It didn’t.

Plan B

Well, the various instructors and leaders were chattering away on walkie-talkies and arranging a rendezvous and a plan. It turns out the other group was also under cloudy skies and couldn’t see anything. Imagine that 😉 . So we all stood around on the patio by the visitor center for a while. When the leaders were firmly convinced we had no chance to observe anything beyond our planet, they revealed the backup plan. They had arranged a special opportunity for us. We would get to tour the 3.5 meter WIYN Telescope, which is usually not open to the public!

Of course, if you read Part 1, you know that this also ended up as the Plan B for my afternoon tour, so I had already had the rare chance to tour the WIYN. If you haven’t read Part 1, I recommend that you do, because I’m not going to repeat my description here, as it looked pretty much the same as it had a few hours before.

Epilogue

After the tour of WIYN, we returned to the visitor center and chatted a bit. I told Jelena about my pilgrimage and that I was planning to hit Lowell in a week or so. She gave me her card and told me to let her know when I was going to be there, and she’d show me around the joint. Cool!

Then came the part where we all would be driving down the mountain together with our headlights off, because, you know, astronomy was going on! Except it was socked in, so there wasn’t any astronomy going on. So we didn’t have to do that after all, but we still had to go down the mountain in the dark. That was still pretty exciting! And when you get down to the bottom, it’s open range, so you have to be careful, or a cow might jump out into the road in front of you! But none did this time. I made it back to Tucson in about an hour and a half, having had to stop for border patrol check point. I can’t find my journal at the moment, so I don’t know if I wrote it down, but it seems to me now that the skies over Tucson were clear.

So all in all, the night program at Kitt Peak was fun and enjoyable and even useful for making a contact or two, but ultimately, in terms of its intended outcome, it was a bust. But I can say I spent a night observing on Kitt Peak, and not very many people can. And I can say I’ve seen the WIYN Telescope – twice! And not very many people can say that, either. So, take that, very many people! I’m an astro-nerd!

Observing from Home – June 3, 2019

Conditions

  • 23:15-01:15
  • cool – low 50s F, maybe into the 40s
  • still, no wind
  • no clouds
  • no moon (+1 day)
  • humidity 75-80%
  • seeing: poor – 2/10
  • transparency: good

Equipment

  • Celestron NexStar Evolution 8″ SCT
  • Eyepieces:
    • 32 mm = 62.5 X
    • 15 mm = 133 X
    • 9 mm = 222 X
    • 8.8 mm = 227 X
    • 2 X Barlow

Objects

  • Jupiter
  • M104 Sombrero Galaxy
  • M58
  • M60
  • M59
  • M51
  • Saturn
  • a wee satellite going past M104
  • a wee satellite going past M51 (don’t think it was the same one)
  • a flaring satellite drifting through Ursa Minor
  • a fireball, due south, just above the trees

Observations

Jupiter

I’ve really been wanting to see Jupiter lately as the GRS is “flaking” and doing weird stuff and shrinking. It’s been months since we’ve had decent night weather when I was free, but tonight was good. Well, clear. The seeing was crap. Any way, I debated going out at all because it’s a pain to take the scope down to the pool, and the deck is full of plants for the garden. I hit on the idea of setting up in the front yard. At 11 p.m. this would give me about an hour on Jupiter before it hit a tree, so to speak. Lots of trees in the front yard. So, that’s what I did!

Quick sketch of Jupiter, ex post facto

Did I mention the seeing was lousy? I could watch the waves of atmosphere rolling over the face of Jupiter. So it was mostly fuzzy and indistinct, even though I was well below the useful minimum magnification for planetary detail. I started at 62.5 X (32mm) and could identify 3 moons (Io was occulted, and I had just missed its disappearance) and the NEB and the SEB. As I’ve seen in pictures lately, the equatorial zone is relatively dark with a tan color. I have to admit I still get confused about image orientation. I think, from pictures, that S was up, but it should have been corrected by the diagonal. But when I pushed the scope toward the N, north was at the bottom. It doesn’t help that I had turned the diagonal to about 4:00 so I could sit and observe. I think that changes the orientation. Well, let’s say S is up. In watching for about an hour with increasing magnification (133, 227, 266, 444) I could see the NEB was thicker and darker, and I thought I could see some gray blocks along the SEB. The polar regions were quite washed out. The GRS was on the flip side, I think. It may have been just on this side about to roll over, but I couldn’t make it out if it was.

I did manage a few pictures holding my phone up to the eyepiece at 133 X and 444 X. Higher power was better for those.

I processed a bunch of pics into this one image using GIMP and Preview. Not very high tech, but it is my first attempt at planetary image processing. I’m pretty sure I didn’t do it right.

Flaring Satellite

While I was looking at Jupiter I saw a flash out of the corner of my eye. I thought maybe someone turned on a light in the house and it caught in my glasses. Then a few moments later, there was another flash. I looked away from the eyepiece. I was facing north. A third flash, and I found it just to the right of the “handle” of the Little Dipper, Ursa Minor. As I watched, this object, which I surmised to be a tumbling satellite, flared at least a dozen times as it moved from NW to NE until it went behind some trees. The flares varied in intensity from … I’m going to guess magnitude 1 to -4 or more! (The smaller the number the brighter the object, and each magnitude is a factor of about 2.5). That brightest flare got me to exclaim, “Holy moley!” out loud. It was just a few seconds between flares, and the difference in brightness wasn’t uniform, which is why I think it was tumbling rather than just rotating. Any way, this was very cool. I also noticed how clear the sky was, as I could see all the stars in the Little Dipper.

M104 – The Sombrero Galaxy

Quick sketch of M104 ex post facto.
That’s a star on the left, not just a random dot.

Once Jupiter got into the tree, I went looking for galaxies. My observing spot was not ideal, as I’d be looking just over the house, which can produce heat issues, with some lights on in the bedrooms, but it turned out okay. I used 62.5 X and 133 X mostly. M104 is a longtime favorite and was still just visible from my position. It never appears very large or much at all like the pictures, but I like it anyhow. Sitting next to a 6.5 magnitude star (going by the Pocket Sky Atlas), it was more radiant than I remember seeing it before. Still best seen with averted vision, there is a bright core – really quite bright tonight – surrounded by nebulosity, but it did appear to have rays of light shining to the … I don’t know.. South? I’m not sure how to explain this. Perhaps a defect in my eyes or optics, although nothing else gave this effect over the night’s observations. Maybe it’s just a really, really bright core, seen on a really clear night. Having spent a long time on fuzzy Jupiter, you might think I’d spend more time on this beauty, but I kind of said, “Oh, that’s pretty,” and moved on. Having added a sketch in my notes, I thought that I had drawn something like it before. Looked through my previous journal entries and sure enough, on 1 May 2013 I have a very similar sketch. The rays aren’t as pronounced, but they are implied (or at least inferred). That was with the Meade ETX90, so more than doubling the aperture perhaps makes a difference.

Virgo Cluster Galaxies

I moved on to a couple of the Virgo Cluster galaxies, starting with M58, because that’s one of the numbers I remember being there. Here my weaknesses as an observer really start to show up. First, I was not prepared. I didn’t have a plan for what I was going to look at and had done no research. This is greatly enabled by having a GOTO scope. Second, I have no patience. (This is an obvious lie, as I just spent an hour looking at fuzz ball Jupiter, but what I mean is….) I don’t take time to soak in the details of what I’m looking at. Well, often that is the case. Third, I don’t know the basics of observing, like image orientation in the eyepiece, angular size of objects and how to estimate them, visual magnitudes of objects and how to estimate them, stuff like that. None of this means I can’t enjoy my observing. It just would be more… insightful if I knew what I was doing, and I’d feel more confident. Any way….

M58 is a fairly large, diffuse, fuzzy object. I didn’t notice any bright core, but I didn’t really study it very long. I would say it appeared larger than M104 and not nearly as distinct. There was a star nearby both of them, though.

I followed an urge to move on to M60, which I knew to be close at hand, although it turns out to be in the opposite direction from what I thought. Hard to tell with the GOTO, which jumps away and slews back slowly rather than just gliding a few arcminutes over. M60 has much the same appearance as M58 – big, fuzzy patch with no noticeable core. I scanned around the area a bit, thinking I’d find M58, and I did find another galaxy, but the neighbor star was missing. Upon review, I think this was M59, another elliptical galaxy that lies between M60 and M58. I hadn’t even brought my sky atlas outside, so I had no idea what the layout was. Rather than going to get it, I abandoned Virgo until another night. This was also partly informed by it getting late and cold, but I wasn’t quite done yet.

(I later found my journal entry for 11 March 2019, the last time I was out with the scope, with a similar entry for M58-59-60. Maybe someday if I do it often enough, I’ll learn and remember.)

M51 – The Whirlpool Galaxy

Ex post facto sketch of M51. There’s a star in the upper right, and another in the disk of the galaxy. This second was actually not as bright as the first, although it looks the other way around.

I thought I’d end on a high note, literally and figuratively, turning my scope upward to another favorite, M51, the Whirlpool, the large face-on spiral galaxy and its companion. This was the best I’ve seen it since Mayhill, NM, in the 25″ Dobsonian in 2010. Two fairly large, bright, distinct objects of comparable size at first. As I’m writing two days hence, I forget exactly what eyepiece I was using, but I think I started with the 32mm and pressed to the 15mm for 133X. Any way, as I looked, the larger spiral, which was fairly vague, began to reveal itself. It remained pretty ephemeral, but it seemed to show indications of its structure. The whole was quite beautiful. I kept getting glimpses of a star in the bounds of the spiral playing peekaboo with me. Definitely the best object of the night. Again, though, the orientation has me baffled, to the point that, upon reflection, it is possible I have sketched the reverse of what I was actually seeing. It may be that the larger spiral galaxy should be on the right and the companion to the left.

What is reality?

Saturn, Sort Of, and Out

By this time, Saturn had risen high enough to be seen. So I took a look. It suffered from the same poor seeing and thick atmosphere as Jupiter. No detail at all – no color, no shadows, no Cassini Division in the rings, no nuthin’. I should have left well enough alone and quit on M51.

The night had grown cold, and I with it, so I packed up. Not a bad night on the lawn.

Observatory 4 – Allegheny

To begin with, here is the link to my pictures from the Allegheny Observatory over at the Googles, taken on my trip there Friday, July 27, 2018. There is some commentary there that will likely overlap with this entry, the core of which was itself written on August 4, 2018, on the train to Chicago at the beginning of the Grand Tour. Here we go.


It has been a wild week or two. I went to Pittsburgh last week for Dad’s birthday and went with Meredith to the Allegheny Observatory. That all came together suddenly, of course. I arranged to go to a Pirates (baseball) game with Dad and Meredith, and in communicating that to Dad, he sent me a note reminding me about the tour schedule at the observatory – Thursdays and Fridays only. Well, the ballgame was on Saturday, so…. I called and left a message Thursday hoping for room in the Friday tour. How popular can this be? I thought to myself.

An Unexpected Journey

Went hiking with Ken K. in Harpers Ferry on Friday morning and heard from the observatory at 1:30 that there was no room on the tour that night. Huh. Not expecting that, but oh, well, okay. I lallygagged around the house a bit, thinking there was no urgency to get to the Burgh. Then I got a call from the observatory at 4:30 that there was a cancellation, and they had spaces available at 8:00! Well, it’s a four hour drive, but yes, of course I’ll take 2 please!

I threw myself and my stuff in the car and drove like crazy to get there. I called M. to have her meet me there. When I hit the turnpike I realized I didn’t really know where I was going. This will end up being a recurring theme, as I had the same problem finding the Holmdel Horn, you may recall. I didn’t have an active smartphone, just my flippy, and I didn’t even have a GPS box in the car. Turns out I didn’t have a PA map in the car, either, let alone a Pittsburgh map. So I stopped at one of the rest areas along the way and set about to buy a map. By the time I found one, about 6 or 8 people had lined up at the counter ahead of me. Ugh! I don’t have time for this! So I opened the map and took a couple pictures of the area around the Allegheny Observatory, and hit the road. Not really proud of that, but it got me there. Except for the part where I missed a turn and ended up going over the Fort Pitt Bridge and through the tunnels toward the airport instead toward the Northside. A little looping around, back across the Westend Bridge, and I was back on track with minimal panic. I arrived about 8:20 p.m., so Whoohoo! Don’t do the math; I was driving fast. Even so, I missed all the introductory lecture and history. The group was just starting on the tour of the building, and M. saw me at the door and let me in.

The Observatory

The large dome of the Allegheny Observatory in sunset and clouds.

The building is a mix of Art Deco, Greek revival, and 20th century scientific lab. We saw some of the museum pieces and labs and such before seeing the two big refractors, which were both very cool: the 30-inch Thaw refractor, which is f/18.8 with a 47-foot long optical tube (!) having been designed and built by Brashear Optical in 1912 (according to the website), and the 13-inch Fitz-Clark refractor. This latter was originally designed and built by Henry Fitz Optical of New York in the 1860s. There is a fascinating story of how the objective lens was stolen and held for ransom, but the director wouldn’t negotiate with terrorists. It was eventually returned, but it was ruined in the process. The observatory hired Alvan Clark to refigure it, which he did, making it a greatly improved instrument. Hence, it is the Fitz-Clark. The tour was quite interesting. Our docent was knowledgeable, having worked or volunteered at the observatory for something like 25 years. He did have an odd verbal tic of sighing dejectedly in the middle of most of his sentences, but otherwise, he was quite good. We got to see how the Thaw scope slews and how the floor is actually an elevator to line you up with the instrument so as to avoid ladders and falls and broken bones. This was fascinating and some brilliant engineering, considering everything was designed to be run without electricity!

The Observing

We got to take turns looking through the Fitz-Clark at Jupiter, as Jupiter was the only thing peeking through the clouds. [Clouds will also become a recurring theme.] Beautiful view, nevertheless. Some detail on the disk, and Ganymede was just on the limb about to disappear. There were about 40 people on the tour, so there wasn’t much chance to hog the scope, unfortunately. Any way, it was very fun to be there with Meredith, and she enjoyed it, too.

My sketch, ex post facto, of Jupiter and Ganymede as seen through the Fitz-Clark refractor.

Epilogue

Just a couple weeks ago Jacob and I watched a documentary about the Allegheny Observatory and some of its key figures on Netf… a movie streaming service. It’s called Undaunted: Forgotten Giants of the Allegheny Observatory. It was fascinating! It made up much of the knowledge I might have gained in the lecture if I had lived an hour closer to Pittsburgh, or if I had better planning skills.

Observatory 7 – Kitt Peak, Part 1

Okay, right off the bat, you can see my annotated pictures of Kitt Peak >here.<

I am now writing this in March, so –– Good Lord, it’s more than six months since I was there??!!! I didn’t write much in my journal at the time, or here. Fortunately, I did add some commentary to the pictures linked above. Well, let’s see how much I remember.

The National Optical Astronomy Observatory at Kitt Peak is about an hour’s drive and change west of Tucson. They run three tours through the day most days: the solar observatory, the 2.1 meter, and the 4 meter. They open at 9:00 a.m. and tours start at 10:00. It was my intention to get there for the tours, because that was sort of the point of being in Arizona, so I was up and out by about 8, which is pretty good for me. Had breakfast from McD’s in the car, which was about the worst food I had on the whole trip — except for breakfast on the Capital Limited. After driving about an hour on that beautiful morning, I was starting to see some mountainous terrain pop up, and not much later started thinking I was seeing a shiny white or silver dot on top of one of the mountains. As I got closer I became convinced it was a dome. Sure enough, I soon came upon the turn off to Kitt Peak! I was very excited. The road up the mountain was quite a drive, a bit of a white-knuckler in places with some pretty serious switchbacks and sheer drop offs. Nevertheless, I made it safely to the top.

One of the first things I noticed when I got out of the car in the parking lot was that it was very, very quiet, except for some wind in the trees. I liked that. Which is good, because I spent all day and a good bit of the night there. Well, about twelve hours or so. I made my way to the visitors center, which is a small brick building with a beautiful mural, a fair sized patio with some tables and benches and sciency things, and an observatory dome on the roof of the building. Inside, it is filled with sciency displays in about 2/3 of the space and a gift shop in the remaining 1/3. Went to the counter and paid for the three tours ($15 for the lot) and for the evening observing program ($75). There were two choices for observing, a general objects and deep sky program and “Our Marvelous Moon.” It still being the monsoon season, I had reserved a spot for the moon program as I figured you can see the moon pretty well even in pretty bad conditions, but you can’t see all the faint fuzzies unless it’s pretty good.

Tour #1

The first tour was led by docent Katy, who is a professional astronomer, retired with 50 years experience. She was very knowledgeable as you might expect, and very engaging, as you might not expect. About 15 people had appeared for the tour, which began in the center with a little history about how the site was chosen, negotiated with the Tohono O’odham Nation, and developed as the National Observatory. The object of the tour was the McMath-Pierce Solar Telescope, which had been retired earlier in the year. It is fascinating design and an exceedingly large instrument. As you can see in the pictures, there is a large vertical column connecting with a diagonal structure that extends underground. This diagonal column is north >polar aligned<, that is, it is aimed at the north celestial pole, the point to which the earth’s rotational axis points in the northern sky, like an equatorial telescope mount. Because it is, sort of. Turns out there is a rotating flat mirror at the top of the structure on the diagonal axis, and it tracks the sun. The sunlight reflects off the mirror and down the axis through a 500 foot optical tunnel to a concave secondary mirror, then back half way up the tunnel to any or all of three more mirrors. These mirrors reflect the light down into a variety of spectrograph instruments in a subterranean laboratory (which sounds more evil than it is). We got to look in from an observation room about half way down the optical tube, which looks kind of like a subway station. We also got to go down to the lab, although since it is closed now we could only look in. They did 5 or 6 decades of groundbreaking solar science there, but now it is considered obsolete. So we’re back to the question of what do you do with giant, historic, obsolete astronomy equipment? Oh, fun fact. While we were walking around the solar observatory, half the sky was clear blue and the other half was entirely socked in and producing lightning and thunder, so that was kind of exciting. What happened to that beautiful morning I drove in on?

Tour #2

We made our way back to the visitor center to see if there was anyone new going on the next tour. I don’t remember now if there was or not, actually. Katy led the second tour, too, which was to the creatively named >2.1 Meter Telescope< (that’s about 84″ or 7 feet). It is a large Cassegrain-style reflector on a large, equatorial fork mount. That it is equatorially mounted means the base is at a 32º angle from vertical. As the mirror alone weighs a ton and a half, having this enormously heavy yet super-sensitive piece of equipment standing at NOT perpendicular to its base felt a bit unsettling, like something was not right. Like the angles! (See what I did there?) Any way, this telescope has done lots of groundbreaking science and is particularly notable for being the first scope to use >adaptive optics<. At this point, several months after the fact, I don’t remember why, but I felt oddly bored with this telescope. Maybe it was that Katy spent a good bit of time explaining adaptive optics, with which I was already familiar. I remember being grumpy about that guy in the group who thought he knew more than the PhD astronomer, so maybe I converted my anger to boredom. Maybe I was hungry. I don’t know. Looking back, it’s an impressive instrument that I’d love to have in my back yard.

Break

We returned to the visitor center, and those of us who were staying on (pretty much everyone) could have lunch if we’d brought it, which it says to do in the literature for the tours. There is no food service for visitors. So I had brought some leftovers from dinner the night before at Za’atar, a mediterranean restaurant in Tucson. The weather was stable and pleasant at that point, so we ate out on the plaza. There are a couple of tables and benches, along with a couple cool sundials that have no practical application to lunch. I sat with the woman who manages the gift shop and schedules people for tours and night programs. She was very interesting to talk with. She is a member of the Tohono Nation and active in her church. She told me that she loves the quiet and the peacefulness at the top of the mountain (me, too!), and that people in her church ask her to pray for them while she is at work because she will be closer to God. We were both a little disappointed in their theology, but she prays for them nevertheless. She told me about her family and some of their struggles, so through the rest of my travels I prayed for her. 

Meanwhile the weather began to deteriorate, with clouds and fog moving in across the valley and across the mountain, too. Great. Made for some interesting photos, any way.

Tour #3a

The third tour was to the Mayall 4.1 meter telescope, the largest on the mountain. This part was led by a different docent, named Dave if I remember correctly. We began with some background and history at the visitor center, then moved to the parking lot. Two reasons for that: first, we were driving to the Mayall dome, and second, in the parking lot is a large cement donut with a mural painted on it. I had noticed it on my way in but not really looked at it. It turns out that the donut is a slug the same size and weight as the mirror for the 4.1 meter telescope that was used to balance the scope during construction. Once everything was finished and nothing was likely to fall, then they put in the actual mirror. Once that was done, they had to figure out what to do with a giant cement donut. Rather than roll it down the mountain, they invited a Tohono O’odham artist to do a mural on it, and it was put on display in the parking lot as you walk toward the visitor center. It’s pretty cool on all counts. Dave pointed out that a 160″ disk of glass weighs a couple tons, or at least this one does. What is remarkable is that the aluminum coating on the glass disk that makes astronomy possible is equivalent to about two paper clips, just a few molecules thick. Amazing!

We all loaded in a big white van to head up to the Mayall dome. We hadn’t gotten a quarter mile down the road when someone raced up, flagged us down, and told us we couldn’t go, because it was a hardhat day. They were renovating the dome and moving stuff with cranes, so it was declared unsafe for visitors. Well, that made for a short tour. We ended up back on the patio, and Dave continued his lecture valiantly. Shortly, though, Katy showed up, talked with Dave for a minute, and then excitedly told us they had arranged to let us see one of the other telescopes, the WIYN 3.5 meter.

Tour #3b

WIYN stands for Wisconsin, Indiana, and Yale Universities, and the National Optical Astronomy Observatory (NOAO, i.e. Kitt Peak). The WIYN scope, a large (obviously) alt-az-mounted Cassegrain reflector, is generally not open for public tours, but it was also down for maintenance, so we got lucky. It is about 20 years newer than the 4.1, and consequently it is vastly lighter and more compact and housed in a much more efficient box with shutters instead of a classic dome. Because the mirror was spin cast and honeycombed, it weighs about 1/8 of what the 4.1 meter mirror does. This means the mount can be correspondingly smaller and lighter, and the whole thing is just a lot easier to deal with. It has capacity for detector instruments in three different places at once that can be switched between easily by, well, I guess throwing a switch to move the tertiary mirror. There are dozens and dozens of actuators on the back of the primary mirror, which are not so much for adaptive optics as to correct for stresses when the mirror is tipped at different angles. Engineer Emily gave us the tour. She has been working on this scope since she was an undergrad, and now she’s the managing engineer for it and probably not yet 30 years old.

That concluded the daytime program, three and a half telescope tours for $15. Not a bad deal. I spent quite a while browsing the swag in the gift shop and exploring the displays in the visitor center before the next part of the adventure began.

Observatory 5: Yerkes, Part 3 – The Observing

Written at Sturtevant, WI, Amtrak Depot on Tuesday, August 14
As for the observing itself, the conditions were less than ideal. It was mostly clear and warm 78F at start, 70F at end. Humidity was predicted to be 70% or higher, which is pretty wet. Thin crescent moon (2 days old) was setting as I arrived. Well, it was low in the west. The sky was thick and hazy, and that was the big problem. High humidity, change from mostly cloudy to mostly clear, and apparently, smoke from the California wildfires all conspired against us. The seeing was muddy and rolling, with brief glimpses of clarity. I was really stunned, though, at my first look at Jupiter. Could hardly get a focus on it, and it was yellowish and dark. The color was from the smoke, acting like a filter. It was low in the sky, too, so that didn’t help – looking through a LOT of unstable air. So the image was very large (because of aforementioned optics) but very distorted. It was hard to make out the North and South Equatorial Bands even. Second time viewing was a little better. Could make out the bands and some occasional details between and a bit of darkening near one of the poles (not sure which it was). Still, I’ve seen better with my 90mm scope at home. So yeah, that was a huge disappointment.

 

Things improved slightly over the evening , but I was frustrated that with 40” of glass to work with here, I consistently have had better views at home. That is the way astronomy goes, though, AND that is perhaps one of the reasons Yerkes is a museum piece more than a research scope these days. Too many nights of weather-degraded viewing a year. Anyhoo,…

 

Saturn was in much the same boat as Jupiter, only a bit higher. The Cassini Gap in the rings was mostly visible most of the time. With patience and a couple turns I could see disk shadow on the rings behind. A little bit of color distinction on the disk — gray at top, less so further down.

Sketch of Saturn from my journal.

M11 Wild Duck Cluster – Even this was underwhelming. Nice full view of the cluster, but I felt like the stars weren’t quite in focus. We could run the focus in and out, but it didn’t seem to make a lot of difference. By this time I was just accepting that the seeing was crap, and I should just relish the experience.
My hope rose again for M17 Swan/Omega Nebula, as nebulae are less affected by bad seeing, but the guys had a hard time even finding it! They added a filter to help. When I got my tern I saw the problem. At f/19 and 475x, we were looking at a tiny portion of the nebula. It served to show noobs what a reflection nebula looks like, but it was like looking at the Mona Lisa’s neck. In fact, we were looking at the neck of the swan, I think. It’s one of my favorite Messier objects, so I think I recognized a pair of stars in the field. Looked like:

Sketch of M17, the Swan Nebula, from my journal

which is cool, but at low power it looks like a swan.

[Here’s a picture I found of what we might have been looking at.]

M27 Dumbbell Nebula – Again, the planetary nebula suffered from narrow field of view and high magnification. It was clearly visible but took up most of the field of view, so there was no sense of scale or contrast. I would have backed off the magnification a bit, but I don’t know where you get an eyepiece longer than 40 mm.

The last object for the night was M2, a globular cluster. This one actually looked good! It was a nice fit in the field of view, and the resolution was good, too. Still felt like it could have had sharper focus, but it was okay. Bright core and grainy cover and pretty even drop off out to the edge. (Yeah, well, I know what I mean.) Really a lovely object, or couple hundred thousand objects, as it were.

Sketch of globular cluster M2 from my journal.

And that was that. They brought the lights up and a bunch of us took pics. I got someone to take a couple of me, one looking at the camera and one looking into the telescope eyepiece. The second was stupid, of course, as (1) the lights were on (2) the dome was closed (3) the scope was no longer even pointed at the shutters. Oh well. The first one is a good picture.

The evening ended pretty unceremoniously.

I stood outside for a little bit, letting my eyes readjust to see what the sky looked like. Pretty much like ours at home, I guess. I hoped to see a meteor before going and pretended I did. It was midnight, and I had an hour to go after a long day, so I hit the road.

Observing from Home – October 1, 2018

I let three good, warm, clear nights slip by me this weekend. Each night right around sundown, the clouds made a strong appearance, so I occupied myself with other trivial endeavors rather than haul out the astro gear. Later in the evening, each evening, as I took a look outside I found the skies to be clear and inviting, but it was too late to set up. There was also a lot of moon on a couple of those nights, but still. So having missed three good chances to get out under the sky, I was determined for last night. Consequently, I was convinced the clouds would close in. That’s the usual pattern. But I lucked out or was given grace, depending on your theology, and the sky remained clear.

I set up the Celestron Nexstar Evolution 8″ on the pool patio. It’s the first time I’ve had it out since Green Bank in July, so it took some work remembering how to get it all put together right and to attach a few doodads that had been taken off for travel. I got it set up as the stars were coming out, so I was able to get it aligned. Then I got the call in for supper (we eat late around here), so I parked it and went to eat. I got back out at about 8:35, and the sky was still clear! Amazing! Also, it was warm enough that a long sleeve shirt was all I needed for my whole time out. That and my Palomar beanie.

What I saw:

Summary:

My primary targets were the planets, especially Mars. I spent a good bit of time bouncing back and forth between Mars, half way up the SE sky, and Saturn getting low in the SSW. More on them in a minute. From there, a quick circuit of the summer glories near Sagittarius, then on to the ice giants, Neptune and Uranus. After that, Andromeda seemed the logical next target. Then, I employed the “Sky Tour” feature of my telescope, letting it suggest nearby goodies. This was cool, because otherwise I might never have seen a couple of these, and I didn’t have a plan, either. I finished the night with three favorite targets around the Summer Triangle, which was still about half way up in the western sky. As I started packing up the gear, a very bright, green fireball crossed the sky in the SW, lasting a couple seconds! Great way to end the night! I was out from 8:30 – 11:45 p.m. EDT.

Conditions:

Weather: Warm! in the upper 60s, maybe over 70. Humid. No wind to speak of. No moon until after midnight (@20 days old).

Seeing: 4/10 – pretty wobbly, based on [magnification/in. aperture]

Transparency: 5/10 – high humidity, maybe a thin layer of cloud even

Observations:

Mars

I’ve been waiting to see Mars all summer. As it was heading for its nearest approach in July, it was blanketed by a global dust storm that obscured any surface markings. I did get a chance to see it at the Lowell Observatory in Flagstaff, AZ, in August, and the dust was starting to settle. Some markings were present to the patient observer at that point. As for this night, the seeing was pretty poor and the transparency didn’t help, but I managed to push the magnification to 222x with the 9mm Plossl eyepiece. That’s well below the minimum to resolve much (312x for 8″ aperture), but I was able to discern some surface markings in the better moments. According to Sky&Telescope (S&T), the disk was 16″ (arcseconds). There was a band of darkness along the northern hemisphere, and it seemed to double back on itself about halfway along the equator. What was more striking was that the disk was only 89% illuminated (according to S&T) and showed as a gibbous section, like the moon a couple days after full. That doesn’t happen very often with the outer planets, but there it was. There was a slight hint of the southern polar ice cap, but I wouldn’t say I really saw it.

I tried a few different filters with varying results. Red definitely made the dark area stand out more, but it overwhelmed anything else. The yellow filter did almost as much to increase the surface contrast without being as overbearing. Blue should have helped bring out the polar cap, but it seemed just to wash everything out. Just not good enough conditions for much detail.

Saturn

I went back and forth several times between Mars and Saturn for comparison and because Saturn was heading for the trees, but I wanted to see if there was any movement on the surface features of Mars. Any way, Saturn looked a great as the conditions would allow, which is to say, “meh.” Saturn’s disk was about the same size as Mars, but that’s not counting the rings. Using the same 222x magnification as on Mars, I couldn’t really make out the Cassini division in the rings, as the outer ring appeared unusually dark. I attribute this to the poor transparency. With patience, I could see some shadow on the rings near the eastern limb in the rear and some darkening around the north pole. The disk is covering much but not all of the rings. Usually I can make out some color differences on the disk, but there wasn’t much to be seen this night.

The red and blue filters didn’t do much for Saturn other than make the outer ring almost completely invisible. The yellow filter helped with the contrast a little bit, making the shadow effects more noticeable but not much more.

I’ve seen Saturn this summer in my scope, the Yerkes 40″ Clark refractor, the Lowell 24″ Clark refractor, and the Griffith Zeiss 12″ refractor. This night ranked somewhere in the lower half, although my scope at Green Bank ranked near the top. Conditions make a huge impact, regardless of how awesome the equipment. Of course, my 8″ is 80 years newer than the newest of the rest in the list.

M20

The Trifid forgot to show up for work tonight. It’s fairly faint to start with and the poor transparency made it essentially invisible. I know I was on it because of the two stars that sit in its midst.

M8

The Lagoon is always a pleasure with its large open cluster and broad nebulosity. I’ve noticed that the Nexstar doesn’t pick up the nebulosity as much as my Newts, and again, with the poor transparency, only the brightest areas were clearly visible. I admit I didn’t study the view for very long, as I had other things in mind. I think a nebula filter might be a worthwhile investment, though.

M22

The great Sagittarius globular cluster is a real showpiece. It stands up to a good bit of magnification. At 222x the stars were resolving in a layer across the surface, although the underlying multitude were less forthcoming. The cluster filled most of the field of view with dozens of brighter stars in that top layer. The whole this is sort of tick-shaped, but apart from that, it’s a beauty.

Neptune

I’ve been tracking Neptune for about 10 years. By tracking, I mean I try to find it every year or two when it’s in a favorable place. Well, now is the season. Back in 2008 it was near the point of Capricornus and easily visible in binoculars. It has made its way into easter Aquarius, between Lambda and Phi, and I had a hard time knowing which object was the planet. Part of the problem is my tracking was off a bit because of parking the scope during dinner, but Neptune is also really small (S&T: 2.4″) and faint now. I finally found it, I think. At 333x magnification it showed itself to be a slightly nonstellar disk, just barely. I’ll have to go back and try it again.

Uranus

Same thing with Uranus. That is, I’ve been following it for as long as Neptune, and it’s harder to find than it was when I started. It has traveled from under the Circlet of Pisces to just east of o Piscium moving into Aries. Uranus is an easier find than Neptune, being 3.7″ (S&T). It was clearly nonstellar and a very small disk at 333x. I might even have seen a little bit of color? A hint of blue maybe? Maybe.

M31, 32, 110

The Great Andromeda Galaxy is always a treat. Enormous and bright, it extends past the field of view in my 40mm e.p. at 50x, so it’s over a degree (twice a full moon). The conditions cut it down some, but it’s still huge. The western edge has a dark dust lane running along it, so it’s more defined than the eastern. (I think I have my directions right). There is a bright, small core surrounded by this extended “nebulosity” that is a 100 million suns. Other than the hard edge I didn’t notice much structure.

M32 is an elliptical galaxy just off the side of the M31. It’s tiny by comparison, but still pretty good size as visible galaxies go. It has a bright core surrounded by an oval of rich haze. It didn’t appear to be over or in M31 but pretty close.

M110 is another elliptical galaxy to the NW of M31. It appears larger than M32 but looks similar with bright core and surrounding oval. It’s edges don’t look as well defined as M32. It is very impressive as compared with other Messier galaxies, just small compared to M31.

M33

The Triangulum or Pinwheel Galaxy is a large, face-on spiral, but tonight it looked like a large, faint fuzz. I’ve found it easily in binoculars many nights and occasionally seen it naked eye (maybe?), but the conditions were not favorable this time, and it didn’t have much to offer. Hey, we all have off days.

Eta Cassiopeiae

This was the first of the items suggested by my telescope’s computer that I looked at. It’s a double star with two yellow white stars, one significantly brighter than the other. I haven’t done much with double stars, but this was pretty to look at.

M103

Scope called this the Triangle Cluster, I think. It’s an open cluster with several brighter stars that make up an isosceles or maybe right triangle with fainter stars laced back and forth across it. I’m not a huge fan of open clusters, but this one is pretty interesting.

M77

This is allegedly a face-on spiral galaxy. I’ll believe it when I see it. It wasn’t a good night for galaxies, or at least for the faint ones. I can’t swear that I even identified this. There was a ghost in the field of view, just kind of a faint slash, that moved with the field, so I guess that was it.

M34

Another of those open clusters I don’t care much for, except I spent a long time on this one. If I were going to name it, I’d call it the Atlas Cluster. I imagined a bulky figure standing with arms stretching out and up (toward NW I think), legs locked, and a globe on its back. It started with two close stars that serve as eyes and three down the middle for abs. Strands running up and out in curves that define the limbs. It’s a sizable cluster with a couple dozen brighter components shaping the titan character and dimmer stars surrounding for the globe and environment. I enjoyed it!

Double Cluster

This pair of open clusters leaning against each other between Cassiopeia and Perseus are beautiful in binoculars. You need a pretty wide field of view to take it all in. Even with the 40mm e.p. I could only fit about one and a half of them at a time. Dozens and dozens of stars, mostly bright white or blue with one or two red ones toward the middle of the two.

Kite Cluster

Described as a diamond of stars with a string of five or more for a tail. I think I saw it, now that I’ve seen pictures of it, but it didn’t look like a kite to me.

M76

This planetary nebula (poorly named, having nothing to do with planets other than sort of looking like one) is fairly compact, maybe 15″? and appears kind of pine tree shaped, so it’s doubly badly named as Little Dumbbell. Maybe with better conditions and/or more patience it looks like the Dumbbell. I think I saw mostly the core. It varied in consistency from top to bottom, being kind of patchy. It sits next to one or two field stars to the west.

Gamma Andromeda (Almaach)

This is a beautiful double star out on the tip of Andromeda with the two stars varying in magnitude and color. The brighter partner is several orders of magnitude brighter than the fainter companion. The brighter is a golden yellow tone, while the partner is a bright blue. Very pleasing pairing.

M27

The Dumbbell (planetary) Nebula appears vastly larger than the Little Dumbbell! A large round object with mottled appearance, M27 filled about half the field of view at 222x.  It’s an easy target and impressive to look at. Imagine, that’s what our sun may look like in 5 billion years.

M57

Unless it looks like this. The Ring and the Dumbbell are both remnants of sun-like stars. It’s thought that they appear at 90-degrees rotation to us, so that we are looking at the side of M27 and down the throat of M57. The Ring is farther away and appears smaller. Nevertheless, at 222x it was clearly a ring of nebulosity. I didn’t see anything in the middle, although sometimes material or a star can be seen.

Epsilon Lyrae

The Double Double is a pair of binary stars that orbit each other. With binocs you can split the one star into two, and at 222x the two split into pairs. The two pairs run perpendicular to each other, so that one pair appears up and down while the other appears side to side. Very cool, and a good end point for the night.

Fireball!

While I was starting to tear down, a bright green light lit up the sky, casting reflections from the telescope tripod legs and shadows on the ground. I looked up to see the end of the fireball, a very bright meteor. It was bright green. A remnant tail about a degree wide and 15 degrees long stretched from the endpoint up the sky. It seems to have run a track that appeared almost straight up and down, maybe from Delphinus down past Altair through Aquila, ending about 15 degrees above the horizon. The tail faded out quickly.

In the end…

Although the conditions weren’t ideal, it was still a very fruitful night out under the sky, which always does my heart and soul good. So glory to God who set all things in their courses and gave some of us eyes to see and souls to thrill at the beauty of it all.

Observatory 1: Green Bank, part 2

Radio astronomy is a fascinating branch of science, in part because it is in some ways very different from optical astronomy. Since we can’t see radio, you can observe and gather your data anytime, day or night. The dishes that act as telescopes get basically one-pixel resolution. So where your phone or camera has several megapixels resolution, the largest radio dishes basically act as a single point, if I understand correctly. It is by panning the dish across an object that you are able to form a picture from it. But there is also a great deal to be learned from radio data without even making it into a picture. For example, different chemical elements give off unique radio frequency signatures. Hydrogen emits radio at 21 cm wavelength, which translates to a frequency of 1420.4 MHz. Since hydrogen is the most abundant element in the galaxy and the universe, you might think that trying to map it would be a little crazy. But an interesting thing happens when you observe a span around that 1420.4 MHz. Because of the nature of space and time and electromagnetic waves, we can detect if the hydrogen being observed is moving toward us or away from us, and how fast it is coming or going, and how far away it is from us. That’s a lot of information! So mapping the hydrogen in the galaxy is like making a navigational map of rivers, harbors, lakes, and seas. It gives you an idea in 3-D of how the galaxy is built and how it is moving and changing.

At the Green Bank Star Quest, I got to do some of that kind of science directly! After a workshop on the basics of radio astronomy (where I learned some of the above), we were given the opportunity to use the 20-meter dish to look at … anything we wanted! A couple others in the class and I looked at two significant radio sources, Cass-A (supernova remnant) and Orion-A (star-forming region). Later we added the Owl Nebula, the moon, Mercury, and a variety of other objects. Some were strong radio sources and others less so, and Mercury not at all, which is weird. I still have a lot to learn about what our scans mean, but it was amazing to be able to run a world-class instrument.

I also got to use the 40-foot radio dish at GBO. It is, I think, the smallest of the active dishes at GBO, but let me tell you, 40 feet is not a small dish! About seven of me end to end would fit across it. This dish is also rather historic in that, as I am led to understand, it was used by Frank Drake for the first SETI (search for extraterrestrial intelligence) experiments in the 1950s and 60s, Project Ozma. This is a transit dish, which means it is always pointed along the N-S meridian, rotating up and down but not side to side. There is a control room in a below ground bunker that looks like a science office from the 1960s. A couple stacks of electronic equipment stand in one corner, the instruments appearing to be of 1980s vintage. By means of analog dials and switches and a digital frequency selector and a tractor-feed data record with two pens, one can collect actual science data by aiming the telescope, selecting a frequency range, and interpreting the graph on the paper strip. It is wildly old school science, and it was a blast! Three of us worked together to get some data under the tutelage of our guide Sophie, but I got to take home the data. I followed some directions on a hand-out and found that the blob of hydrogen we investigated near the center of the galaxy was moving away from earth at (if I recall correctly, as I don’t have it here with me) 48 km/sec. How cool is that?

Along with experiences in several other lectures and workshops, I found that I was just having the best time being a science student again. It gave me a thrill, not only to be learning from professional scientists, but also to do actual science. To be transparent, I also got a thrill from being a good student, knowing or figuring answers to questions ahead of others in the class. Yes, I like being an overachieving, curve-busting, teacher’s pet and always have.

But really, it’s the thrill of the science.