Archive for the ‘Observing reports’ Category

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Observing report: Saturday night stargazing on Mount Baldy

April 2, 2017

Waxing crescent moon, afocal shot by Eric Scott with Samsung Galaxy S6, shooting through Orion XT10 reflecting telescope.

London and I went up Mount Baldy last night with our friends Thierra Nalley and Eric Scott. Marco Irigoyen and Leandra Estrada joined us up on the mountain. We went up to look for comet 41P, but that didn’t pan out.

Since we went ostensibly to look for the comet, I brought the XT10 for firepower, and lots of binoculars. We got set up at Cow Canyon Saddle at about 8:30. Our first target was Orion, before it could sink into the light dome over LA. Second targets were the Pleiades and the Double Cluster. The Double Cluster in particular looked magnificent. I’ve been on a small-scope kick for a while so the XT10 hasn’t been out much, and I tend to forget what a potent instrument it is, especially under dark or semi-dark skies.

The skies on Mount Baldy last night were definitely semi-dark. Even three days shy of first quarter, the waxing crescent moon was bright enough to throw shadows and rather seriously degrade the darkness of the sky.

I tried for the comet but just couldn’t see it. I had the chart, knew where to look, and swept the area repeatedly with binoculars of all sizes and with the XT10, and I got bupkiss. This was after catching the comet easily in 7×50 binos every time I looked for it in Texas last weekend – but I wasn’t fighting any moon then. I think the comet is so big and diffuse that the surface brightness is low, and therefore it is easily swamped by moonlight. It certainly was not evident last night.

While we were in the neighborhood of the Big Dipper, we had a look at Mizar and Alcor, the famous double star in the dipper’s handle. Then for comparison we checked on Sigma Orionis, and then Marco wanted a look at Jupiter. After Jupiter we went on an extended tour of the deep sky, in which we observed:

  • M81, M82 (interacting galaxy pair)
  • M97, M108 (planetary nebula and galaxy in same field)
  • M3 (globular star cluster)
  • M37 (open star cluster)
  • M35 (open star cluster)
  • M104 (Sombrero galaxy)

In addition, we also saw three more open star clusters with our naked eyes and/or binoculars: the Hyades, M44, and the Coma Berenices star cluster.

We finished up on the moon, and then Jupiter again. We spent quite a bit of time getting pictures of both with Thierra’s and Eric’s phones. By coincidence, they both have the Samsung Galaxy S6, which has a very full-featured slate of camera options. Leandra is a pretty talented photographer and she was able to coach us on what settings to use. I think the results are pretty astounding, for handheld shots using phones. Here are the two best images of Jupiter, captured by me using Thierra’s phone and Leandra’s advice:

Here’s a composite of Jupiter and the Galilean moons – the planet was overexposed in the original to get the moons to show up, so I replaced it with the better of the two shots above.

And here’s a comparison screenshot from Sky Safari Pro 5 identifying the moons – from left to right in the above image they are Callisto, Europa, Io, and Ganymede.

As usual, the view at the eyepiece was about an order of magnitude more detailed than what the photos captured. One thing that I had never seen before with one of my own scopes was a band of ruffled white clouds within the north and south equatorial belts (the prominent orange-brown stripes on either side of the equator). The barest hint of this survives in the photos. It was a pretty mesmerizing view. For eyepieces we used a 32mm Plossl (37.5x), 28mm RKE (43x), 24mm ES68 (50x), 14mm ES82 (86x), 8.8mm ES82 (136x), and 5mm Meade MWA (240x). The most used were the 28mm RKE, 14mm ES82, and 5mm MWA. If you’re wondering why we used both a 32mm Plossl and a 24mm ES68 – since they give the same true field of view – we used the Plossl during the afocal photography because it gives a wider exit pupil, which is easier to keep the camera’s aperture centered inside.

Even though we missed the comet, I was pretty happy with what we did see – at least one of every major class of deep-sky object, including all of the stages of the life cycle of stars. In the disk of the Milky Way, new stars are born from vast nebulae of gas and dust, like Orion. In time, heat and light from the newborn stars push away the remnants of their birth clouds, leaving behind only the stars themselves, as open star clusters (‘open’ as opposed to globular). Over time, the stars in open clusters drift apart to become ‘field stars’ like the Sun, no longer gravitationally bound to their siblings. When the run out of fuel, stars blow themselves apart in supernovae if they are 8 times the mass of the Sun or larger, whereas smaller stars blow off their outer layers of gas to form planetary nebulae like M97. Whether stars die suddenly in supernovae or slowly as planetary nebulae, the matter blown out by dying stars enriches the galactic gas and dust clouds, and in time it will be incorporated into new generations of stars and planets. We are products of this process – all of the elements in our bodies other than hydrogen were born by fusion in the hearts of stars, and seeded into the galaxy’s spiral arms when those stars died.

Farther out, globular clusters like M3 orbit the core of the galaxy on long elliptical orbits that are not flat, but come looping in from all directions. The stars in globular clusters are typically very old, 12 billion years or more. We know very little about how and why globular clusters formed, and how they came to have such weird orbits. Probably they are some kind of developmental leftover from the formation of the earliest galaxies in the first billion years after the Big Bang – astrophysical fossils, if only we knew how to interpret them.

All of these processes are going on in other galaxies as well, especially spiral galaxies like M81, M104, and M108.

To put all of that into context, here are all of the objects we observed again, this time ranked from closest to farthest:

In our solar system:

  • moon – 240,000 miles or 1.3 light seconds
  • Jupiter – 370 million miles or 33 light minutes (currently – Jupiter is about 5 AU out from the sun, but right now we’re on the same side of the sun so it’s only 4 AU from us)

In our spiral arm of the Milky Way galaxy (the Orion spur):

  • Mizar and Alcor (double star) – 83 light years
  • Hyades (open star cluster) – 151 light years
  • Coma Berenices cluster (open star cluster) – 280 light years
  • M45 (Pleiades; open star cluster) – 440 light years
  • M44 (Beehive; open star cluster) – 577 light years
  • Sigma Orionis (multiple star) – 1255 light years
  • M42, M43 (Orion nebula; star-forming region) – 1344 light years
  • M97 (planetary nebula in same field as M108) – 2030 light years
  • M35 (open star cluster) – 2800 light years

In the next spiral arm out from the galactic center (Perseus arm):

  • M37 (open star cluster) – 4500 light years
  • NGC 869/884 (Double Cluster; open star clusters) – 7500 light years

In the galactic halo of the Milky Way:

  • M3 (globular star cluster) – 34,000 light years

External galaxies:

  • M81, M82 (interacting galaxy pair) – 11 million light years
  • M104 (Sombrero galaxy) – 31 million light years
  • M108 (galaxy in same field as M97) – 46 million light years

That is very satisfying to me, to take in such a menagerie of celestial objects, at so many scales and distances, in the space of a couple of hours armed only with a comparatively inexpensive telescope and an idea of what’s out there to be seen. I can’t wait for next time.

Saturday night astro crew. Left to right: Marco Irigoyen, Leandra Estrada, London Wedel, Matt Wedel, Thierra Nalley, Eric Scott. Photo courtesy of Eric Scott.

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Deep in the Dark of Texas: the Three Rivers Foundation Messier Marathon

March 28, 2017

This story starts with Jeff Barton, Director of Astronomy at the Three Rivers Foundation for the Arts and Sciences (3RF). Jeff sent me a Facebook message on January 27, inviting me to come speak at the 3RF Messier Marathon star party, for which 3RF would pay my travel expenses and provide food and lodging.

I did not get this message until February 19, because I suck at Facebook. Fortunately the offer was still open. So last Thursday I flew to DFW, rented a car, and drove out to the Comanche Springs Astronomy Campus, a little west of Crowell, Texas.

3RF is an educational foundation and Comanche Springs is the North American astronomy wing (they also have scopes in Australia for public education and outreach). It’s out in rural Texas ranchland, and as you drive up the first thing your eyes will light on is the big silver observatory dome.


Inside the dome is a 15″ refractor with DGM optics, an OMI tube, and a monster Astro-Physics mount.


There are several roll-off roof observatories on the campus, with more to come in the near future. This one holds two imaging scopes, a big Ritchey-Chretien on the left and a big SCT on the right, both on Software Bisque Paramounts. These are set up for remote observing – in the near future, schoolteachers will be able to tie into these telescopes and collect images with their students.

Irritatingly, I didn’t get any pictures of the big roll-off roof observatory which holds one of 3RF’s 30″ Obsession dobs, and where they park the two 20″ and one 18″ Obsessions when they’re not in use. That’s right, four 18″ and larger Obsessions in one place. They have more stored in town, waiting for more observatories to be built, and another gaggle of Obsessions in Australia.


In lieu of a picture of the Obsession shed, here’s a view of the north end of campus, looking east. From left to right you can see one of the four or so bunkhouses in the background, the ‘new’ classroom/mess hall, the equipment shed where the binocular chairs are stored, and the restrooms, and one of the observing fields in the foreground.


Here’s one of the motorized binocular chairs. You sit in the padded seat and drive yourself in altitude and azimuth with the joystick on the right armrest, while the Fujinon 25×150 binoculars deliver 6″ of unobstructed light-gathering to each eye. There’s another chair with a more modest but still impressive 100mm bino, and I believe a third chair that wasn’t out during my visit.

The tagline “Deep in the dark of Texas” is not my original, I got it from the back of a 3RF t-shirt. It’s true. The skies at Comanche Springs are dark. Seriously dark. You drive through a section of open range to get there. I had to get a picture of this brown cow sitting by the side of the road – this cow refused to be fazed by anything. I grew up in rural Oklahoma and in my experience, free-range cattle are highly correlated with dark skies. The skies at Comanche Springs are Bortle 1 or 2. The only places I have been under skies this dark are Afton Canyon, the All-Arizona Star Party, and the remote desert of southern Utah. More than 200 miles west of the DFW metroplex, and 20 miles from the nearest town of more than 1000 people, there are no light domes on the horizon – none.

I roomed with these fine gentlemen. You may know Robert Reeves from his several books on astrophotography (see this page) and from his “365 Days of the Moon” on Facebook, which has now been running for more than two years. David Moody is a Fellow of the Royal Astronomical Society (yes, the one in London, co-founded by Herschel) and one of the authors of Astronomical Sketching: A Step-by-Step Introduction. Lonnie Wege is a sales manager at Celestron and brought the door prizes, which were donated by Celestron.

To be in the company of such experienced observers and imagers was a real privilege, but it was only intimidating for the first 30 seconds or so because they’re all so nice. In Seeing in the Dark, Timothy Ferris describes hanging out at the Winter Star Party: “I listened to the elders talk – a mix of astronomical expertise and self-deprecatory wit, the antithesis of pomp.”  That’s what it was like for me at the 3RF star party – just a bunch of regular folks, all equally willing to share and learn, all equally excited for nightfall.

I got in Thursday evening but didn’t do much observing. It was cold and windy, and then cloudy. I did spend a few minutes out in the lee of one of the bunkhouses cruising the sky with binoculars, and I figured out an easy hack for hanging my red headlamp over my bunkbed, but that was about it. Incidentally, my headlamp is already red, but like almost all red-light accessories marketed toward amateur astronomers, it’s still too darned bright. Usually I have a layer of masking tape over the front to knock down the brightness, but for some reason I pulled it off recently. Fortunately they had plenty of red taillight tape in the 3RF coffers, so I got it back into fighting trim.

On Friday I visited the elementary and middle schools in nearby Quanah, Texas, with 3RF’s Director of Education, Townly Thomas. Townly visits schools in a 100-mile radius from Quanah to bring enhanced STEAM (Science, Technology, Engineering, Arts, and Math) activities to kids. I know she’s popular because I heard one student call to her as we walked down the hall: “Mrs. Thomas, when do we get to do STEAM again?” I went in my capacity as professional paleontologist and brought some fossil casts for the students to see. Pictured above are the thumb claw of Saurophaganax, a big allosauroid from Black Mesa in the Oklahoma panhandle (more about that here), and the skull of Aquilops, a little ancestral horned dinosaur that I got to help name in 2014 (ditto). Many thanks to my friends and colleagues at the Sam Noble Oklahoma Museum of Natural History for making the casts available – I’ve had fun introducing them to lots of schoolkids.

After the school visit, I got on the road back to Comanche Springs – I didn’t want to miss the talk by Robert Reeves on his lunar imaging. Here’s a  handful of the many things I learned from Robert:

  • He uses a 180mm SkyWatcher Mak to get his moon images these days. Runs his camera at 50 frames a second for 100 seconds to get 5000 frames, stacks and saves only the best 500, and then does a LOT of careful, thoughtful processing.
  • Lunar shadows are jet black, not gray. If you see gray shadows in someone’s moon images, they need more processing.
  • The lunar Bay of Rainbows is Sinus Iridum, not Sinus Iridium – no third ‘i’. I have been misspelling and mispronouncing it for a decade.

Now, this was a Messier Marathon star party and there were rules and checklists and everything – more on that later in the post. I think that originally Friday, Saturday, and Sunday nights were all fair game for the contest, but Friday night turned out to be suboptimal. We did get a lovely sunset, as you can see above, but those clouds were pushed on through by a strong, cold wind. Instead of setting up scopes ourselves, many of us retreated inside the dome to observe with the 15″ refractor. We also had a group of 15 or 20 college students visiting, so we all took turns looking through the big refractor. They’d already been going for a while when I got inside. The first object I saw myself through the big scope was the globular cluster M3. Then we looked at M51, the Whirlpool Galaxy, and then Comet 41P.

I haven’t blogged about the comet yet, but it is easily visible in binoculars under dark skies, and with any luck it may get naked-eye visible in the next week or so. I haven’t checked to see if it’s visible from Claremont – I was too pooped after I got home last night. I saw it every night in Texas, but I haven’t sketched it yet. Hopefully I’ll get that done soon. In the meantime, Sky & Tel has a good finder chart that will carry you through the end of April here.

After the comet, we looked at the galaxies M102, M82, and M104, and the globular cluster M13. I might have missed an object or two – I popped outside to call home, and spent some time in the attached classroom warming up and getting to know some of my fellow stargazers. I know we went to Jupiter at some point, and we back to Jupiter at the end of the session to catch the start of an Io shadow transit.

I slept in on Saturday and did some final tinkering on my talk. David Moody gave a talk before dinner about visiting the Royal Astronomical Society library and getting to see first editions of books by Copernicus, Newton, Bode, Bayer, and more.

After David’s talk we had dinner and door prizes in the mess hall. Here Jeff Barton (right) is pointing past Fred Koch, who was drawing names, to accuse Lonnie Wege (left) of something. It was all in good fun and there was plenty of laughter, especially when Phil Jones won the grand prize – 15×70 SkyMasters, just like mine – in absentia, having been out setting up his imaging gear. When he came in, Lonnie told him that all he had won was the case, and the binos were going to someone else. Well, binos did go to someone else (whose name unfortunately escapes me), but he had already won 10×50 binos so he kindly donated the 15x70s to Phil. This is Phillip L. Jones of VisualUniverse.org, by the way – you’ve probably seen his photos in books and magazines.

I won a door prize myself – a rechargeable hand warmer. I ran over and plugged it in after dinner so it would be ready to go by marathon time. I was very glad to have it later on.

Saturday night was looking much, much better. There were a few clouds low on the western horizon, but everyone who had come to Comanche Springs to observe or image was getting ready. Here are Glenn Winn in the foreground setting up his 17.5″ Discovery dob, and Jim Admire in the background with his XT10g. Just out of the frame on the right was Jay Ellis and his own XT10.

I set up just south of Jay, and the four of us were the biggest group of visual marathoners. Phil Jones had his imaging rigs set up about 100 feet south of Glenn. There were more imagers on the south observing field, by the Obsession shed, and at least two serious visual observers: Tom Monahan and Russ Boatright (there may have been more, but Tom and Russ are the two who came to the awards ceremony on Monday).

I don’t remember what scope Tom was rolling with, but Russ impressed the hell out of all of us by going super-minimal: he did a naked Messier Marathon from Memory. Not naked as in unclothed, but naked as in, not even with a list of the objects. In a regular M-cubed the observer is allowed no charts – they have to find all of the objects from memory, hence the name. In a naked M-cubed, the observers is not even allowed a list to remind them what to look for, it’s just them and their instrument. Russ ran his naked M-cubed with Canon 18×50 image-stabilized binoculars.

Saturday night’s marathon was great. There were clouds low in the west again, and none of us got M74. But the clouds blew through quickly and after that it was clear, dark skies all night. I was rolling with the Bresser AR102S Comet Edition and Fujinon 7x50s I had borrowed from 3RF. I’d actually flown in with my own binoculars, the Bushnell 10x42s that I had out at Santa Cruz Island last June, but the 7x50s gave a wider, brighter image and were more in line with my current fascination for low-power, wide-field uber alles. I would have brought the Bresser 7x50s that came with the Comet Edition package, but I ran out of room in my backpack – the Bushnell roofs take up about half the space.

And speaking of space in my backpack – I managed to fly with carry-on luggage only. A red duffel bag held the Bresser OTA, Manfrotto tripod, DwarfStar alt-az head, and big dinosaur claw, with my clothes wrapped around everything as packing material. My backpack had a couple more shirts, my laptop, travel paperwork, notebook, Pocket Sky Atlas, binoculars, boxed Aquilops skull, shaving bag, and Bob King’s new book Night Sky With the Naked Eye, which I’d gotten specifically to read on the plane (expect a review soon). Both bags were stuffed nearly to bursting, but they were both within carry-on allowances and the backpack still fit under the seat in front of me.

Oh – rules. There were five categories: Young Astronomer, GoTo Telescope, Non-GoTo Telescope, Binoculars, and Highest Aggregate Score. No-one has ever gotten all 110 objects in one night at a 3RF marathon, so the highest aggregate goes to the person who gets the most over the course of two nights. If there’s a tie in the number of Messier objects, the bonus points kick in. Herschel 400 objects were worth two points apiece, and there was an ascending scale of more difficult dim objects, including Hickson Compact Groups of galaxies.

Here’s my log from Saturday night. Although I missed M74, I tried to make up for it by nailing as many H400 clusters in Cassiopeia and Perseus as I could. By the time I took my first break at 10:15, I had 27 Messiers and 16 H400s. I took several short breaks over the course of the evening to get snacks and caffeine and chat with people. It all went pretty smoothly until just before dawn, when I was trying to catch M30. I star-hopped down from Deneb Algedi (aka Delta Capricorni) to the right vicinity and found myself looking at trees. They were only small trees, and probably 200 yards from the observing field, but they still obscured those last few crucial degrees above the horizon. I’d picked a bad spot.

What I should have done is pick up the binoculars and walk south until I could see the target star with no trees in the way. What I actually did was pick up the scope and chair and run south and set up where I thought I’d be in the clear, only to star-hop down again and see other, different trees – I’d gone too far south. So I moved everything yet again, and by the time I got on target, the sky was getting bright. Fooey. Still, I got 108 objects, tying my personal best from 2013, which was actually the last time I’d even attempted a Messier marathon, so I couldn’t be too unhappy.

As it happened, I tied with Glenn Winn that night. He’d missed M77 in the early evening, but gotten M30, so his list of 108 objects was slightly different than mine but came to the same total.

Anyway, I went to bed happy. Got up for lunch on Sunday, then slept some more, then got up for another talk by Robert Reeves. Robert’s second talk was also on the moon, but focused less on his imaging methods and more on the processes that have shaped the moon, and the moon’s changing appearance under varying conditions of light and shadow. It was incredible stuff – I took a whole page of notes to guide my own future moon-observing.

Sunday night we had clearer skies than Saturday, but it was colder and a brisk north wind was blowing not long after dusk. None of us got M74. Down at the Obsession shed, folks were looking for it with even bigger scopes and failed to see it, so I’m confident it just was not visible that night. Possibly that was atmospheric, but the zodiacal light certainly didn’t help – it was a broad dagger of light stabbing up vertically from the horizon all the way to the Pleiades. I have never seen it so bright.

The other thing that shaped my Sunday night plans was the fact that Glenn did get M77, bringing his aggregate Messier total to 109. All of my bonus points from H400s would only help in the event of a tie, and the only was I could tie him was to get M30. And without M74, there was no chance for me to achieve my personal goal of getting all 110 Messiers in one night. So I needed to be up before dawn to try for M30, but there was no point in subjecting myself to a whole night of observing in the windy cold. I packed up the scope and moved into the lee of Jeff Barton’s camper and switched over to binoculars. I was still using the 3RF Fujinon 7x50s.

It was another Fujinon binocular that would provide the most memorable views of the evening: the 25×150 motorized bino chair. 3RF volunteer Gary Carter had set up the bino chairs and was touring people around the sky on Saturday evening, but I was too busy marathoning to partake. Sunday night I hopped in the big chair, Gary got the binos adjusted, and I was off.

In a word – WOW. I have been fortunate to get to observe with a lot of big telescopes, but I am not exaggerating when I say that using that bino chair was my favorite observing, ever. I just sat there comfortably in a padded chair and drove myself around the sky with the joystick, while enjoying hands-down the brightest, most immersive, most enjoyable views of the night sky that I have ever had. Six inches is a lot of light-gathering per eye. I don’t know the AFOV of the eyepieces but it is wide. It’s hard for me to even believe that the magnification was only 25x – everything subjectively seemed much bigger, because it was so much brighter and more detailed than I am used to. When I was cruising over to look at the Double Cluster, I kept getting distracted by all of the little open clusters that dot the Milky Way in and around Cassiopeia (I was coming in from the north). M78, near Orion, was so big and bright that at first I thought I had the wrong object.

In summation, observing with the Fujinon bino chair was a transformative experience – it changed my perspective on what observing could BE.

I knocked off a little before midnight with 60 Messiers in the bag, and went to get some sleep. I didn’t get up until 5:30, and I wasn’t back out on the observing field until 5:45.

I have read many accounts from observers under dark skies who said that when the summer Milky Way rose, it was so bright that they mistook it for a cloud. I had not previously experienced that for myself. But Monday morning I was headed out of the bunkhouse and I saw a bright, white cloud in the eastern sky. We’d been fighting the occasional cloud every other night, so when I saw that cloud out of the corner of my eye I thought, “Aww, crap, I need clear skies to get M30”. But when I turned my head to see how big the cloud was, and how extensive, it turned out to be the Milky Way in Sagittarius and Scutum. I should have known better anyway – Comanche Springs is so dark that actual atmospheric clouds aren’t bright, but dark. They show up as blank spaces in the starfields.

I didn’t get M30. I got the scope correctly placed this time, and I got to the target star, and I spent about 15 minutes alternately adjusting the zoom eyepiece and staring into the darkness. A couple of times I thought I saw something, but I couldn’t even hold it in averted vision, so it could well have been a case of averted imagination. Anyone who has pushed their gear to its limits in the search for faint fuzzies will know the feeling. There are the things that you see repeatably in the same place, with the same orientation, that you log as detected – and then there are things that never swim up out of the minor variations in background darkness that your retina throws up when confronted with a blank slate. M30 never surfaced for me.

Ah, well. I did get 25 more Messiers with the 7x50s between 5:45 and 6:05. It helped that I had seen them all the previous morning with the telescope, so I knew exactly where to look. I probably could have gotten a few more, like M2, if I hadn’t been so fixated on M30. But 85 Messiers in one night with 7×50 binos is not a bad total at all, especially not when I got a 5.5-hour break in the middle.

I was too keyed up to go right back to sleep, so I went into the observatory classroom, made myself a Frito pie with a microwave bowl of Dinty Moore Beef Stew – which was awesome, by the way – and copied my results over from my personal log to the 3RF competition forms. Then I went back to sleep for a couple more hours.

We all reconvened in the observatory classroom around 10:00 for the final tally and presentation of awards. Here’s the scoreboard:

The highest aggregate total went to Glenn Winn, with 109 objects over the two nights. I got second in the Non-GoTo category, behind Glenn, and also got second in the Binocular category, behind Russ Boatright. In his naked M-cubed with the 18×50 bins, Russ got a staggering 90 objects. Color me impressed – very impressed. Jim Admire got 91 objects with his XT10g, and that was without pushing through dawn, so he won the GoTo category. Tom Monahan wasn’t even going to turn in his sheet, figuring that his 47 objects from the first half of Saturday night would not qualify him for anything. But a lot of people who signed up didn’t turn in any results, so Tom got the pleasant surprise of third place in the Non-GoTo category. I think the Young Observer awards went unclaimed, as no actual youngsters participated in the marathon.

Here’s a shot of the winners’ circle. From left to right are:

  • Jeff Barton, our host and the competition judge;
  • Glenn Winn with his 1st place medal and aggregate score trophy;
  • Russ Boatright;
  • Jim Admire;
  • yours truly, and;
  • Tom Monahan.

Many thanks to 3RF volunteer Gary Carter for taking the photo, and for permission to use it here.

A good time was had by all, and plans are already being laid for next time. Turns out that Jeff Barton is a fan of double stars, and he visibly lit up when I brought the idea of a Double Star Marathon to his attention. Something like 80 globs are visible in the fall during fall Messier Marathon season, so some kind of glob marathon may be in the offing in the near future as well.

I learned some things about my gear, too. The Bresser/Manfrotto/Dwarfstar rig was utterly uncomplicated, as I suspected from my test run at the Salton Sea the previous weekend. Rarely have I had more effortless and trouble-free observing. And I’m proud to have gotten 108 objects in one night with a 4″ scope – I don’t think there’s any shame in losing to a 17.5″ reflector, nor to an observer as experienced and friendly as Glenn. I might even have ‘sold’ a few of the Bresser Comet Edition packages, as there was a lot of curiosity about the scope among the star party attendees. I think Jeff Barton may have ordered one yesterday morning.

Is a 4″ reflactor enough scope for a Messier Marathon? It wasn’t this time. I’m not hurt about not getting M74 – if people with 17″ and 18″ dobs couldn’t see it, then conditions were just not right for it to be seen, period. M30 is more troubling. I know for dead certain that I was pointed at the right place, and I tried every trick in the book – averted vision, tapping the tube, slowly sweeping – and still couldn’t get it to pop out, and this was from its rising onward. But I know it was visible in bigger scopes. Sure, it will be a few degrees higher by the end of the month, but M74 will be a few degrees lower, too.

Now, I know that people have gotten all 110 Messiers in one night with even smaller scopes. According to this analysis by A.J. Crayon, hosted at the SEDS Messier site, it has been done with a 60mm refractor. That is darned impressive. So theoretically, yes, under perfect conditions, a 4″ scope is more than enough. But your chances improve with bigger scopes. Still, even a 17.5″ scope wasn’t enough to get all 110 this time, at this site. And it is worth noting that I’ve now done just as well with a 4″ scope as with my Apex 127, having gotten 108 objects in one night with both instruments.

Flying with the Bresser Comet Edition turned out to be surprisingly easy. I got scope, tripod, alt-az head, and clothes for five days into a standard duffel bag. The likelihood of this scope racking up more airline miles in the future is very high. And the 28mm RKE and 8-24mm Celestron zoom were all the eyepieces I needed. I didn’t use a finder of any kind – I didn’t take my green laser pointer for airport security reasons, and I forgot to borrow one from Jeff (who did offer) before the marathon started Saturday night. But it was okay, I just did my dead reckoning trick and didn’t even think about it after the first few objects. On the flip side, I did wish for a different atlas. I really need to suck it up and take the Jumbo PSA next time. At 4:00 in the morning when my eyes are tired and I’m trying to read by the dim light of a red headlamp, the writing in the standard edition is just too small.

I have new ambitions about gear – mainly, that I gotta get me some big binoculars. Frequent commenter and sometime observing buddy Doug Rennie has 20×80 bins that he mounts on one of these – that would be a potent and enjoyable combo for a very reasonable outlay (although I see that the price has crept up from the $65 or so it was going for last year). And my new no-holds-barred, price-is-no-object dream observing rig – which I may never achieve – is a motorized chair with 150mm binoculars. It was that good.

But ultimately the star party was not about gear, it was about experiences. I had a fantastic time at Comanche Springs, saw amazing things in the sky, learned a lot from my fellow amateurs, and most importantly made a lot of new friends. Many thanks to Jeff Barton and the whole 3RF crew for their hospitality and for making my trip possible. I don’t know when I’ll be back out there, but I’m already looking forward to it.

For more about Messier Marathons, including log sheets, links, and observing reports from previous marathons, see this page.

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Observing Report: more Messiers at the Salton Sea

March 21, 2017

I went to Mecca Beach again Saturday evening. Like my run at the end of February, it was a solo mission, decided on at the last minute. I made up my mind in the mid-afternoon and I emailed a few folks to see if anyone was interested, but that proved to be too little notice (not surprisingly).

I got a late start, didn’t arrive until about two hours after sunset, and there was a cloud bank to the west, so I missed out on all of the early evening Messiers. I skipped right over the winter objects, having spent the last 6 weeks observing them repeatedly with a variety of instruments.

Gear

I’m flying to Texas this weekend for a Messier Marathon star party – more news on that soon – and I’m taking the Badger along. I’ve flown with little Maks and with an AstroScan once, but this will be my first time flying with a refractor. I’ve had this trip in mind for a while – it’s why I was so excited to find that the Badger would ride securely and comfortably on my Manfrotto CXPRO4 plus DwarfStar rig, because that is an eminently flight-worthy mount and tripod combo. BUT the previous testing was just a short session in the driveway. I was curious to see how the Manfrotto/DwarfStar/Bresser setup would fare under semi-realistic conditions, on an extended observing run at a distant site.

I was also testing eyepieces. I want a travel setup that will be lightweight and low hassle, but that will still cover all the things I’m likely to want. My prime mover is the 28mm RKE. It is simply delightful and gives a bright view of a wide swath of sky. Next up is the Celestron 8-24mm zoom eyepiece, which covers most of the useful magnification range for this scope (19x-57x). I used this eyepiece a lot right after I got it. Then I was off it for a while – I went through a phase of doing a lot of high-power work with my Apex 127 and C80ED, and I thought (and still think) that the Celestron zoom was just a hair less sharp than the best of my non-zoom eyepieces, particularly the Explore Scientifics. However, my eyes are now the weakest link in the optical chain, even with glasses. So although I don’t get super-sharp pinpointy star images anymore (or at least, not until I get new glasses), I also don’t worry too much about whether my eyepieces are 100% sharp or only 97%.

I also auditioned some possible third players: the 32mm Plossl, just in case I needed more true field than the 28mm RKE will give; the 5mm Meade MWA for ‘high-power’ work (still only 92x); and the 2x Shorty Barlow. It turns out that I don’t need any more field than the 28mm RKE gives, so the Plossl is staying home; the MWA is nice but big, and not worth the bulk on this trip; and my Shorty Barlow has ever-so-slightly misaligned barrel pieces, so it won’t sit all the way down in the focuser. I’d noticed this before, but it didn’t bother me because all of my other eyepieces would come to focus anyway, but not, it turns out, the Celestron zoom. So the Barlow is staying home, too, and I’m planning to roll with just the 28mm RKE and the Celestron zoom.

Star Testing

I spent the first hour on just four targets: the Trapezium in Orion, the Pleiades, Jupiter, and Polaris. I looked at the Pleiades just to see them before they went down into the cloud bank over Palm Springs. The other three targets were to test the scope and the skies. The seeing was a little better than it has been for most of this spring, but still only so-so. The Trapezium was bouncing around too much for me to resolve the E and F components, although I suspected E a couple of times.

Jupiter looked a lot better than it has so far in this scope. I think that was partly a little better seeing, and partly the result of having collimated the scope. As I mentioned in the last post, the view of Jupiter at 92x was mesmerizing, with finely-divided belts and zones resolved all the way to the poles. I was using the 60mm aperture mask to knock down the CA, and that might have helped with the seeing and with other aberrations.

When I had stared at Jupiter for about 20 minutes, I removed the aperture mask and did a proper star test on Polaris. I’m not an expert at star testing but I know a little, and I have a copy of Suiter’s book, Star Testing Astronomical Telescopes, on loan from a friend in the club. I sketched the results inside and outside of focus and compared them to the diagrams in the book when I got home. The scope has about 1/4 wave of spherical aberration. That’s not great – it’s flirting with being not diffraction-limited, and it helps explain the scope’s so-so performance on solar system objects and double stars. On the upside, the perfectly-concentric diffraction rings confirmed that the scope is now in good collimation.

Binocular Messier Hunting

The best sky conditions of the evening were in the hour on either side of midnight. The cloud bank to the west was still there, but it had retreated down near the horizon. Transparency was as good as it was going to get. Lying down in a lounge chair and looking up naked-eye, I could make out sixth-magnitude stars at the zenith. After spending a good chunk of time at the telescope looking closely at a handful of objects, I was ready for a change of pace. I grabbed the 7×50 binoculars that came with the Bresser Comet Edition package and hopped in the lounge chair for a Messier tour.

I started with some galaxies in Ursa Major. M51, M81, and M82 were all easy, as were M94 and M63 in Canes Venatici. Then I jumped over to Corvus to pick up M68 and M104. After that I went to Coma Berenices and spent a while just staring into the Coma star cluster. It’s a true open cluster, and it looks huge because it is only 288 light years away. That’s farther than the Hyades (~150 light years), but closer than the Pleiades (380-440 light years, depending on the source), and the size of the Coma cluster is nicely intermediate between those two as well.

My first Messiers in this area were the globular clusters M3 and M53. Both were easy catches, and M3 was so bright I had to look twice to make sure it wasn’t a star. Seeing them in binoculars brought back fond memories of the very first time I ever observed them. It was the spring of 2008, and we were still living in Merced. I was on a backyard campout with London, who was only 3 1/2 years old. We were using my old dome tent, and as soon as London went to sleep I poked my top half out onto the grass and did some binocular stargazing. That was the first time I ever saw M3 and M53 with my own eyes.

My next target was the galaxy M64, and it was bright and obvious – so much so that it seemed to pop out from the background, the way that planetary nebulae sometimes do. M65 and M66 were not so pronounced but they were still easy prey. M95, M96, and M105 took a little more work and chart-checking, but I managed to bag them all. Later in the morning, after I’d gone back to the scope, I picked up the globular clusters M13 and M92, and the open clusters M6, M7, and M11.

I know that other observers have seen all 110 Messier objects with 7×50 binoculars – Jay Reynolds Freeman reports having done so in his essay, “Messier surveys“. I’ve seen all of the Messiers in my 15x70s and most of them in 10x50s, but I’ve never even attempted them in 7x binos. So I am working on a proper Messier survey with these 7x50s, and so far I’m up to 40 objects. Here’s my visual log – I’m highlighting objects in green as I observe them:

If you’d like a similar record sheet for your own observations, here’s a blank one:

A Varmint of the Skies

After an hour of binocular observing, I was ready for a stretch, and also champing to track down some of these objects with the scope. I had gotten through most of them with the scope, and I was about to make my assault on the Virgo galaxies when the moon rose.

I thought that contrast had dropped off a bit, and I was seeing fewer faint stars, and the rising moon made the reason clear: a high, thin haze had developed over most of the sky. Galaxies that had been dead easy in the binoculars just an hour before were now completely invisible in the scope. I missed out on M63, M94, and M101, and abandoned my Virgo galaxy hunt. I watched the moon rise through my binoculars, then I switched to double stars for a while. I’m not going to say much about that right now – suffice it to say that the results of my double star observing will be coming to a newsstand near you this fall.

After I’d done my double star ‘homework’, I was feeling very pleased. At the start of the evening I’d written down three goals for the session: “Messiers, double stars, chill”. With the first two activities done to my satisfaction, I was content to engage in the third. I spent more time looking at Jupiter and the moon through the scope, and a fair amount of time just sitting on a picnic table and looking up with my naked eyes. The haze had thinned out somewhat by 3:00 and I was just happy to be out under the stars. Although there were people camped just a few hundred feet from me, I had the place all to myself. Even the coyotes had stopped yipping and howling.

Back at the scope, I spent a while looking around in Lyra. My favorite astronomical axe to grind is that the “celestial sphere” compresses almost limitless space and time into what looks like a dome over our heads. As I put it in this article (and this even earlier blog post), I’m constantly trying to “shatter the bowl of the sky, to see space as space”. Lyra is a good area in which to do this, with objects as close as Vega – a scant 25 light years away – and as distant as the globular cluster M56, which lies 33,000 light years away. I’ll probably write a whole post about that soon (UPDATE: hey look, I did!).

Usually if I’m up that late at this time of year, I go through the “steam from the teapot” Messiers in Sagittarius and Scutum. But an unfortunate cloud was camped out in my way. I did pick up M11 in Scutum, and M6 and M7 near the ‘stinger’ of Scorpius, with both the binoculars and the scope. I also had a nice long look at the False Comet cluster near Zeta Scorpii. The False Comet is a fantastic object for binoculars and rich field scopes – or maybe I should say “a fantastic set of objects”, since it includes the open clusters NGC 6231 and Trumpler 24, and other bright stars in the Scorpius OB1 assocation, of which both clusters are members.

I’m up to 43 Messiers with the Badger. There are 3 objects that I’ve seen in the Bresser binoculars but not yet in this scope: M63, M94, and M101. And there are 6 that I’ve seen in the scope but not yet in the bins: M5, M29, M39, M56, M57, and M79. I’m not worried about the mismatch – most of the objects I haven’t seen in the binoculars because I just haven’t tried yet. Although I am a little nervous about my ability to distinguish the smaller planetary nebulae from stars at only 7x. Still, it’s a fun hunt and so far I’ve seen almost everything I’ve attempted. Here’s the visual tally for the scope:

I ended back in the solar system. I had a nice long look at Saturn a little after 4:00 AM, and at 4:15 I was gazing at the moon when I fell asleep. After a lifetime in academia, I’m very good at sleeping sitting up, and I didn’t realize I had drifted off until my eyebrow brushed the eyepiece, ever so gently. I think that’s the first time in almost a decade of stargazing that I have actually fallen asleep at the eyepiece. I called it a night, dragged the lounge chair around to the west side of the car where it would be out of the sun, and slept until almost 11:00.

Verdict? Well, the scope is no planet-killer. Doing the star test confirmed what I already suspected. But if I use an aperture mask and keep both the magnification and my expectations modest, it still delivers rewarding views of solar system targets. And it continues to be a fantastic wide field, low power scope for deep sky work. I was also happy to find that the light Manfrotto tripod and DwarfStar mount were more than adequate. I did have to let the scope settle a little at high power, but for Messier sweeping the whole rig just got out of the way and let me observe, which is what I had hoped for. Finally, although I had other eyepieces sitting in the rack, I spent almost the entire evening using just the 28mm RKE and the 8-24mm zoom. So as a test of my travel kit, the evening was a resounding success – and a heck of a lot of fun to boot.

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Finally – the Bresser Messier AR102S Comet Edition at the Salton Sea

February 26, 2017

ar102s-at-dawn

Sometimes life is cruel.

(Did I say cruel? I meant ridiculously First World cushy, where a grown man can afford nice toys and has the time to play with them and blog about it. But within the context of this grown man’s play-time blog, sometimes life is cruel.)

To wit: my Bresser Messier AR102S Comet Edition (still sans snappy nickname) arrived on Sunday, January 29, just a few hours late for the new moon observing run at the Salton Sea that Terry Nakazono and I went on the night before. Since then it’s been mostly cloudy here, with poor transparency on the nights it hasn’t been totally socked in, so I’ve been misusing the scope on bright stuff like the moon and Jupiter. And waiting not-so-patiently for a chance to get out to dark skies and do some wide-field, low-power scanning.

I actually did get about 45 minutes of semi-dark time with the scope a week ago. I was on dawn patrol up in the foothills and I spent some time in the summer constellations before the sun came up. The views were bright and contrasty, but all it did was whet my appetite.

Friday night I finally got the scope out under decent skies, for a decent amount of time. I decided pretty late to go to the Salton Sea – originally we had other plans, but Vicki and London were wiped out from a long week, and the forecast said that Friday was the last clear night for a while, all over SoCal. I didn’t leave Claremont until almost 7:00 PM, and with set up time after I arrived at Mecca Beach, I didn’t start observing until 10:00.

Gear

I was rolling pretty light. I wanted to test the Bresser reflactor/bino set as a package, so I used the AR102S on the came-with mount and tripod. I essentially always have binos out while I’m observing, so I used the 7x50s that came with the scope. That was a novel experience – I usually roll with 10x50s or 15x70s. This was my first time using 7x binos for serious deep-sky observations.

The only way I broke with the Bresser package was with eyepieces. I did use the included 20mm 70-degree a few times early in the evening, and I briefly tested the 10mm 70-degree that just came in, but my most-used set for most of the evening consisted of the 28mm Edmund RKE, both natively (16.4x) and with a 2x Barlow (33x), and the 8.8mm ES82 (52x and 104x).

28mm-rke-in-ar102s

A word about the 28mm RKE. It is simply the most comfortable eyepiece I’ve ever used. There are several factors that play into that. One is the long eye relief. Another is the magical floating stars effect, which is real, and impressive. Finally, there’s the wide exit pupil it gives, which in the AR102S is 6.2mm. That’s probably wider than my pupils go these days (same is true of the 7mm exit pupil of the 7×50 binos). Using binos or eyepieces with exit pupils wider than your own will go is usually not recommended. The extra light falls on the muscles of your iris, not on your retina, so your pupil becomes an aperture mask, stopping down the system to a smaller working aperture. You could get just as much light delivered to your brain using a smaller instrument or eyepiece. But there is one positive effect of using a “too-wide” exit pupil: you can move your eye around a bit within the light beam, without any falloff in illumination. So “too-wide” exit pupils are very bright – maximally bright – and very comfortable. And if a bit of light is wasted, oh well, it’s not like the cops are going to come for you.

One nice effect of swapping the 28mm RKE for the 20mm 70-degree is that they have close to the same true field of view of 2.9-3.0 degrees, but the RKE gives a much sharper image with fewer aberrations. Unsurprisingly, since it’s bending light from the same true field into a much smaller apparent field. Normally, a 45-degree AFOV would feel downright claustrophobic to me these days, but for some reason the 28mm RKE doesn’t bother me. I think it’s the magical floating stars effect – most narrow-fields (okay, anything south of 50 degrees) feels tight, like looking through a soda straw, because so much my field of view is taken up by the inside of the eyepiece barrel. But with the 28mm RKE, there is no visible eyepiece barrel, so although the AFOV isn’t actually that big, it feels much more expansive.

I did have one minor gear screw-up: I forgot my laser. I haven’t installed a finder on the AR102S. Same with the C80ED, except for one or two nights early on. When I really need help I lay a laser finder along a straight edge and use it to point to things in the sky. On the C80ED, there are a couple of buckles on the tube clamp that together form a de facto trough like the one I built for the SkyScanner 100. On the AR102S, the finder bracket serves the same purpose. But I forgot my laser. So I did what I usually do, just dead-reckoned it. I’ve gotten to the point where I usually don’t even have to sight down the tube, I can just sort of look up and aim the scope and get the target within a 3-degree circle. The AR102S will go wider than 3 degrees – a 32mm Plossl or 24mm ES68 will give 3.6 degrees, and my 32mm Titan 2″ will go to 4.88 degrees. But none of those eyepieces do their thing with the same panache as the 28mm RKE – at least in this scope. I did get out the 32mm Plossl just in case I needed a wider ‘finder’ eyepiece, but it never made it into the focuser.

Goals

I had a program in mind. Long-time readers will know that I’m a big fan of Jay Reynolds Freeman’s astronomy essays, especially “Refractor Red Meets the Herschel 400”. More relevant to this post is “Messier Surveys”, in which Freeman relates his habit of running through all the Messier objects with every instrument he gets his hands on, from 7×50 binoculars to a 14-inch SCT. Despite my Messier Marathon attempts, I’ve never kept track of which Messiers I’ve seen with which instruments. I’m certain I’ve seen them all with the XT10, and I’ve seen almost all of them with my 15x70s, but beyond that, I have no idea. So I decided that the best way to properly test the Bresser would be to start a Messier survey with it.

To be clear, I had no intention of attempting an off-season or mini Messier Marathon. I decided to just go until I got tired. I also was not a purist – I looked at plenty of non-Messiers along the way, including some I had never seen and wasn’t planning to observe when I started.

And in fact, I started with some non-Messiers.

Perseus

When I started observing at 10:00, plenty of good stuff was getting perilously low in the west. The western reaches of Cassiopeia were already down in the Palm Springs/Indio light dome. I started with the Double Cluster and Stock 2 – my first time looking at them with the AR102S. They were spectacular as always. Then I swept up through the Alpha Persei Association and followed the eastern ‘arm’ up to NGC 1528. The cluster was fully resolved at 33x, but I thought it was prettier at 16.4x, when the dimmer stars trembled just at the threshold of resolution. I also checked in on NGC 1545, which is a much less impressive cluster and a much tougher catch since it is dominated by a bright foreground star. But my favorite observation in this area was another OC, NGC 1513. I tried this one at a variety of magnifications and it always ‘popped’ a little more in averted vision, as previously unresolved stars swam into visibility. Not one of the sky’s stunning showpiece objects, but delicately beautiful if you have the time to tease out its secrets (and the skies – it’s not bright).

I hit M34 on my way out, and of course I stopped at the Pleiades, which were very nicely framed at 16.4x.

Orion and Vicinity

After all of that, I realized that I had to get a move on if I wanted to catch M79, the glob in Lepus, before it set. I hopped over to snag it, and visited Hind’s Crimson Star while I was in the neighborhood. It was a tiny red spark in the 28mm RKE.

The whole sword of Orion fits into the field of view of the RKE. The Trapezium was nicely broken out into four stars at 33x with the Barlow. I had a quick look at Sigma Orionis and scanned the Belt and the big OB association just off Orion’s western hip. M78 was delightful. Even at 16.4x, the two foreground stars were visible and distinct from each other and from the background glow, and the western edge of the nebula showed a more abrupt cut-off, which lent the whole object the feel of a comet.

Binocular Tours

Up to this point I had been using the 7x50s to trace my star hops in advance, but now I really started to run ahead. One thing about writing my deep-sky tour articles for Sky & Tel – I usually remember all the stops and I can run through them quickly anytime I’m out. In this case, I started at Sirius and followed the path of my December 2015 article down through Canis Major, across Puppis – with a side trip down to Vela that was not in the article – and into Hydra (for M48). Then I picked up where my tour from this March started, running northwest through Monoceros and northern Orion before ending in Gemini. Running through both tours took about 10 minutes, and I saw a lot and missed a lot more. Seriously, that stretch of the winter Milky Way is just ridiculous. You can swing your optics over it again and again and not pick out all there is to see.

Then I had a long break to rehydrate, eat a snack, and get into my cool-weather getup. I’ll have to write a whole post about that sometime.

ar102s-set-up-for-observing

After the break I went back through almost all of that with the telescope, in part just to see it all with more than 50mm of aperture. I noticed some Herschel 400 objects in Puppis that I had never observed, namely the open clusters NGC 2479 and 2509. Both were dim swarms of faint stars that were still not fully resolved at 52x, but very pretty. I had not noticed them in the binos, but after catching them in the scope I was able to see them when I went back with the 7x50s. I was comparing the two clusters in the binos when a meteor flashed through my field of view, which is always a cool sight. I spent about half an hour trying to catch the planetary nebula NGC 2440, and even hauled out Interstellarum to help me get on target, but I never got a definite sighting. I’m going to have to study that one and come back another time.  I did catch NGC 2438, the planetary nebula that is superimposed on M46 but only about half as far off as the cluster. It was obvious at 52x but I couldn’t separate it from the glow of the cluster at 16.4x. Needless to say, it didn’t show in the binos.

Roaming

By the time I was finished retracing my winter Milky Way tours, the Auriga Messiers were getting low in the west, so I hopped over to check them out. After that I hit M44 and M67 in Cancer. M44 was just perfect at 16.4x – everything nicely resolved, but still compact enough to look like a coherent object. The stars in that cluster always seem to fall into geometric patterns to me, as if they were laid out using a grid system that got erased the morning after creation. I can’t think of anything else in the sky that gives me the same impression.

I also popped up north, past Iota Cancri and over the border into Lynx, to check on NGC 2683, a surprisingly bright and easy Herschel 400 galaxy that I had previously only observed with binoculars. (Want to know more about this galaxy and its neighbors? See the April 2017 Sky & Tel!) Since I’d seen it with smaller-aperture binos under worse skies, naturally it was an easy catch for the AR102S.

After that I turned south, to Omega Centauri. Although I haven’t written about it yet, when Terry and I were at the Salton Sea last month, I spent a long time looking at the monster ‘glob’ – actually the exposed core of a dwarf galaxy that was cannibalized long ago by the Milky Way. It’s a favorite spring target of mine when I have a good southern horizon. From Mecca Beach there is a definite light dome from El Centro and usually some near-horizon haze in the southwest – directly over the water. But Omega Centauri culminates between that particular Scylla and Charybdis. Last month I spent nearly an hour checking it out, using naked eyes, binoculars, and several levels of magnification with the C80ED. I could just get the outermost stars to resolve at 120x, albeit in imperfect seeing. This time was worse – about the same lousy seeing, and slightly worse transparency. I didn’t get any actual resolution, but I could make out pronounced differences in brightness across the face of the cluster. I also had a look at NGC 1528/Centaurus A, the famous radio galaxy. I think it should be naked-eye visible under optimum conditions, but my conditions were not optimum. It was obvious in the binos and showed some detail in the scope.

Then it was on to Corvus to check in on M104 and M68. I also observed the planetary nebula NGC 4361, I think for the first time. It’s bright but small, and it turned out that I could see it at 16.4x, I just didn’t recognize it – I had to go up to 52x to confirm that it was nonstellar. I also visited M83 while I was in that neck of the woods. What a wonderful galaxy, so big, bright, and obviously elongated even at low magnification.

By now it was almost 3:00 AM and I was getting pooped. I finished in Lyra, with Epsilon Lyrae and the Ring Nebula, M57. I couldn’t split the Double Double. That might have been the scope, but it might have been the skies – by this point there was a steady breeze blowing right in my face when I looked east. I have had other nights where the seeing was so bad that Epsilon Lyrae would not split. I did notice some CA around those stars at high power, which probably didn’t help.

I decided to finish with M57, which was fitting since it was a chance observation of that nebula with the TravelScope 70 a few years ago that got me hooked on refractors. I wanted to recreate the feel of that surprising low-power observation so I left in the 28mm RKE. The whole southern end of the parallelogram fit very nicely into the 3-degree field, with M57 showing as a pale little dot. Then I realized that I had stopped the scope down to 60mm while I was playing with the double star and had forgotten to take off the aperture mask. So I got to do one of my favorite tricks – reach up and pull of the mask while I’m observing, and watch the sky get brighter in a hurry, as if all the lights out there suddenly turned on. The nebula had been obvious at 60mm – at full aperture it was so bright it almost looked stellar.

ar102s-at-mecca-beach

Tally

I ended the night having observed several double stars and 46 unique DSOs with the telescope, of which only 22 were Messier objects. Three were Herschel 400s which I believe I observed for the first time – those were the open clusters NGC 2479 and 2509 in Puppis, and the planetary nebula NGC 4361 in Corvus.

I’ll have a more complete review along soon, but the Bresser Messier AR102S lived up to its middle name – it is a superb Messier-catcher. Every Messier I attempted was not just visible but easy at 16.4x. Will be interesting to try it on some of the smaller, tougher objects like M76. I think this will be my Marathon scope this year.

Don’t take this as a full-spectrum endorsement. When I do post a full review of the scope, I’ll have both good and bad to report. It’s not a good all-rounder, not a good first or only scope. But what it’s built to do, it does quite well.

The biggest surprise for me was how much I could see with the 7×50 bins. I didn’t catch everything, but of the 46 DSOs I observed telescopically, 34 were also visible in the binos, and some of the rest I simply forgot to check (the galaxy NGC 2683 comes to mind). There were more DSOs that I saw in the binos but didn’t take the time to log, including shedloads of clusters in Monoceros. I don’t know if I will be able to complete a Messier survey with the 7x50s – I reckon some of the smaller planetary nebulae will prove my undoing – but I’m at least going to make the attempt.

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Mt Wilson photo tour and a brief observing report

June 5, 2016

Mt Wilson 1 - Geo on the 60-inch

Last night the PVAA had the 60-inch telescope booked at Mt Wilson. It had been ages since I’d been up there – my only other trips up were in 2009 and 2010 (observing reports here and here). So it was very satisfying to be back. It is amazing to look back and realize that in 2010 I was only 3 years into what has now been almost 9 years of stargazing.

The last two times I went up, we didn’t have time for a tour of the grounds, so about all I saw were the parking area, the 60-inch dome, and a few odds and ends in the distance. This time we got a nice long tour from Geo Somoza – most of the rest of this post is a photographic tour of part of the observatory. We didn’t have time to go through the museum up there, or see the solar telescopes – guess I’ll just have to go back again to catch those (which is no bad thing!).

I rode up with Ron Hoekwater, Laura Jaoui, and Gary Thompson, who kindly drove us. We left Claremont early and got up there about 6:00, well in advance of the planned 6:30 start time for the tour. While we were chatting outside the gate, we saw something ominous: a tower of smoke going up from the mountains to the west. This would come back to haunt us.

Mt Wilson 2 - Einstein bridge and the 100-inch

Here’s the dome of the 100-inch Hooker telescope – world’s largest from 1917, when it eclipsed the 60-inch telescope on the same mountain, until 1948, when it was eclipsed in turn by the 200-inch Hale telescope on Palomar Mountain. It is a bit staggering to realize that from 1908 to 1993, when Keck 1 went online on Mauna Kea, the three consecutive world’s largest fully-functional telescopes were all within 92 miles of each other in southern California. (The 240-inch Soviet BTA-6 saw first light in 1976, but it suffered terrible thermal stability and seeing problems and never performed anywhere near its full potential.)

This bridge is nicknamed “Einstein’s bridge” because Einstein paused here for a famous photograph during a visit to Mt Wilson in 1931 – see that historical photograph here.

Mt Wilson 3 - the 100-inch

Here’s the scope itself, the same machine that Edwin Hubble and Milton Humason – a former mule-driver who worked his way up to master observer – used to chart the expansion of the universe. I was scheduled to go up and observe with the 100-inch last year, but I got very sick the day before and couldn’t make it. So that is still on the bucket list.

Mt Wilson 4 - the 100-inch mirror

A view into the back of the mirror cell of the 100-inch telescope. The green champagne-bottle glass of the primary mirror is clearly visible. If you click through to the full-size version you may be able to see bubbles in the glass. The 14-inch-thick mirror had to be made in three separate ‘pours’ of molten glass, and bubbles from the first two pours were trapped by the layer above. The people at Mt Wilson were so concerned about the bubbles interrupting the figure of the mirror that at first they refused to work with it, but St Grobain Glassworks was unable to pour a better one and eventually George Ellery Hale ordered his people to grind and polish this mirror, which turned out to be fine at the optical surface after all.

Mt Wilson 5 - 100-inch eyepiece

In the old days, to observe visually with the 100-inch you had to go down a narrow hallway to a tiny room where light from the scope was bounced to the Coude focus. That was pretty unsatisfying so a few years ago the telescope was modified for more intimate visual observing. Now the primary mirror at the bottom of the scope bounces the light to a secondary up in the upper cage, thence to a tertiary at mid-tube which directs the light out to a quaternary mirror in the diagonal housing at the top of the black tubular assembly on the left of the scope in the above photo, thence down to a quinary mirror at the bottom of the black tube, then into the white refractor that is pointing down and to the right. A diagonal sitting nearby can be placed into the refractor to put the eyepiece into a convenient orientation when the scope is tilted.

Mt Wilson 6 - 100-inch controls

The control board of the 100-inch, with at least three separate control systems lined up right to left in order of age. Most interesting is the old table on the right with the clock and the two periscopes. The periscopes allowed the telescope operator to see the telescope’s setting circles. Nowadays, the scope is controlled by the computers on the left.

Mt Wilson 7 - 100-inch dome

Excited amateur astronomers lingering outside the dome of the 100-inch. We got to walk around on the walkway you can see on the outside of the dome. The entire dome rotates, walkway included. It’s a fearsome engine indeed.

Mt Wilson 8 - CHARA array and 60-inch domes

On the left is one of the six domes of the CHARA array, I believe still the world’s longest-baseline optical interferometer. It has enough resolving power to image the discs of nearby stars. On the right is the 60-inch dome.

Mt Wilson 9 - lightspeed test site

Geo shows us the concrete pier used during the speed-of-light experiments in the 1920s. More on those in a sec.

Mt Wilson 10 - lightspeed test plaque

For decades in the late 1800s and early 1900s, Albert Michelson conducted a series of experiments to measure the speed of light. In a series of famous tests in the 1920s – almost two decades after Michelson earned his Nobel Prize – a beam of light was bounced from this pier on Mt Wilson to a mirror on Lookout Mountain, one of the foothills of Mt San Antonio, better known to locals as Mt Baldy – the mountain at whose base I live. The concrete pier on Lookout Mountain is still there and it is apparently an easy hike. It’s on my to-do list.

Mt Wilson 11 - LA and smoke from wildfire

Sunset over LA. On the left, the marine layer of fog is moving in over the city. On the right, a tower of smoke is going up from a wildfire near Calabasas, about 40 miles to the south and west of Mt Wilson, and spreading out over the LA basin. For a while the smoke was going southeast from the fire, and it looked like it might miss us. But by the time it was getting dark, the wind had shifted and was carrying the smoke directly toward the observatory.

Mt Wilson 12 - going up to the 60-inch

As darkness fell, we trooped into the dome of the 60-inch telescope.

Mt Wilson 13 - Edison bulbs

Here are the controls for the dome’s shutter, which has to be opened for the telescope to see out, and closed again to protect the telescope during the daytime and in inclement conditions. The three light bulbs on the upper left of the console are original Edison bulbs – they have been working without ever being replaced since 1907 or so.

Mt Wilson 14 - control board and mercury tank

Our telescope operator, Christopher Burns, checks something on one of the computers in the control center, while beyond him Geo stands by the mercury tank in which the 60-inch telescope floats. Don’t worry, it’s fully sealed now. In the old days, it was open, and mercury would sometimes splash on the floor as the telescope rotated.

Mt Wilson 16 - Jupiter with blue filter

Our first target was Jupiter. As usual, the photo completely fails to do justice to the naked-eye view. The seeing was imperfect and I think the smoke from the fire might already have been affecting the views. The north and south equatorial and temperate belts were visible, and the Great Red Spot was prominent, but I could see little detail beyond that. I have seen much better on other visits, and indeed in much smaller scopes (see for example the two previous Mt Wilson observing reports linked at the top of this post). But I won’t complain too much – part of the joy of observing with the 60-inch is in the process, not the outcome.

Mt Wilson 15 - 60-inch lit by laser

After Jupiter we moved on to the globular cluster M3, and then the Sombrero Galaxy, M104. M3 was already looking a bit dim – certainly not as bright as it appeared in Ron’s 25-inch scope from RTMC last weekend – and about this time the smell of smoke became pronounced in the dome. We had a hurried look at M104, but it was just a dim smudge of light and I couldn’t even make out the dust lane.

After M104 we had to shut down early to protect the telescope. If ash from the fire was allowed to fall on the mirrors, it would combine with moisture in the air to produce acids which would eat away the coatings. In the photo above, Geo is shining a laser up through the optical train to check for ash on the mirrors.

Mt Wilson 17 - Matt with the telescope

It was a bummer to have to shut down early, but we had an awesome tour and it was fun to observe again with the 60-inch, even if only briefly. Geo and Chris were great hosts and everyone had a good time. We’ll get to reschedule our night on the scope, since we only got about an hour and a half of observing in, so the club’s investment is protected. It’s a shame about Mars, though – we won’t have another opposition this close for some time, and the planet will be noticeably more distant, smaller, and dimmer by next month already. Still, into every observing career a little rain – or ash – must fall, and I’ve been extremely fortunate. Two eclipses (2012, 2014), a Venus transit, and a Mercury transit in the last four years, and not one of them clouded out. Mars will be back, and I’ll be ready.

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Small, medium, large – observing near and far in the last two weeks

June 4, 2016

Matt at Delicate Arch IMG_2984

Preface – Running with the Red Queen

I’ve just finished maybe the busiest spring of my life. January and February were largely sunk into day-job work – time-consuming, but necessary, interesting, and in fact rewarding. Then the last three months have been taken up with travel and public lectures.

  • In March I went to Oklahoma for 10 days of paleontological research in field and lab, and I gave a talk at the Oklahoma Museum of Natural History titled, “Dinosaurs versus whales: what is the largest animal of all time, and how do we know?”
  • In April I did a two-day trip to Mesa, Arizona, for more paleo work. No talk on that trip, but I did participate in the “Beer and Bones” outreach at the Arizona Museum of Natural History.
  • In early May I was in Utah for another 10 days of paleo research, and I gave a talk at the Prehistoric Museum in Price on, “Why elephants are so small”. My colleague Mike Taylor and I took one day off from dashing through museums to tour Arches National Park, which is where Mike took the photo at the top of the post.
  • Last weekend I was up at RTMC, where I gave a Beginner’s Corner talk on, “The scale of the cosmos”.

I’m not complaining – far from it. It’s been exhilarating, and the collaborative work I have rolling in Oklahoma and Utah will hopefully be paying off for years. And planning and executing all of the work has been satisfying. Particularly the RTMC talk, which deserves a whole post of its own. And ultimately this is all stuff that I chose to do, and if I could do it all over again, I would.

BUT there have been consequences. Most frustratingly, I haven’t had enough uninterrupted time to get anything written up for publication – not the sizable backlog of old projects I need to get finished up, and not the immense pile of new things I’ve learned this year. I haven’t gotten out to observe as much as I’d like, and I’ve barely blogged at all.

And it’s not over. In two weeks I leave for a week of paleo fieldwork in Oklahoma, then I’m back for a week, then I’m off to Utah for about 10 more days of digging up dinosaurs. In between I’ll teaching in the summer human anatomy course at WesternU.

But I’ve had a nice little pulse of observing in the last couple of weeks – two weekends ago up at Arroyo Grande, near San Luis Obispo, last weekend at RTMC above Big Bear, and this week at Santa Cruz Island off the coast. No time for separate observing reports, so I’m combining them all into one.

Observing Report 1 (Medium): The Planets and Moon from Arroyo Grande

I was fortunate to be part of a great, tightly-knit cohort of grad students at Berkeley. Of the people I was closest to, some are still in and around the Bay Area and some of us have been sucked into the gravity well of the LA metro area. Occasionally we get together somewhere halfway in between, either up in the Sierras or near the coast. I usually take a telescope, because almost everywhere is darker than where I live, and when I’m traveling by car there’s simply no reason not to.

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This year we met up for a couple of days and nights in Arroyo Grande. We hiked in the hills, went down to Morro Bay to watch ocean wildlife and buy seafood, played poker, and generally got caught up on work, family, hobbies, and life. Our first night was wonderfully clear. I had along the trusty C80ED, which has become my most-used scope. It’s mechanically rugged, optically damn near perfect, and compact enough to not require much time or thought when it comes to transportation and setup. On Saturday, May 21, we spent some time with Jupiter, Mars, and Saturn. Jupiter and Saturn were as they always are: beautiful and surprising in their immanence. I cannot look through the telescope at either of them without being forcefully reminded that they are as real as I am, that as I go about my days full of busyness and drama, they are always out there, hundreds of millions of miles away, go about their own business whether I or anyone else pay them any attention or not. One of my friends had never seen the rings of Saturn with his own eyes, so that was an added bonus.

Mars was the real treat. Using the Meade 5mm 100-degree EP and a Barlow I was able to crank up the magnification to 240x. The dark dagger of Syrtis Major and the white gleam of the north polar cap were both obvious. It is always arresting to see details on this world that has loomed so large in the human imagination, from ancient mythology to science fiction to current and future exploration.

The next night we sat out on the patio, eating oysters and watching the sun set. I didn’t have any of my own binoculars along, but a friend had brought a couple, and after it got dark we watched the still-mostly-full moon rise through the trees on the ridgeline to the east.

It was all shallow sky stuff (solar system, that is), but it was all spectacular, and I’m glad we did it.

Observing Report 2 (Large): Going Deep at RTMC

Last weekend I was up at RTMC, finally. I’ve been wanting to go since I got to SoCal, but in the past it’s fallen on the same week as our university graduation and I’ve been too wiped out. I didn’t make it up for the whole weekend. We went up as a family to stay Saturday and Sunday nights. I went up to RTMC early Sunday morning to look around, give my talk, and hang out. Ron Hoekwater, Laura Jaoui, Jim Bridgewater, Ludd Trozpek, and Alex McConahay of the PVAA were all there and we spent some time catching talks and jawing about skies and scopes. I also chatted with some folks from farther afield, including Arizona and NorCal.

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I took off in the afternoon to spend time with London and Vicki, then went back up after dinner. All I had along were my Celestron 10x50s (yes, those), but Ron had his 25-inch Obsession dob, and he was content to use it as the centerpiece of a group observing session. We looked at the planets, or at least Jim Bridgewater and I did – Ron had checked them out the previous night and didn’t want to blow out his dark adaptation. That was a smart call, as the Obsession gathers a LOT of light and the planets were almost blown out. We could have put in a filter, but ehh, we had other things to be getting on with.

We started with globular clusters. M3, M5, M53, NGC 3053, and one or two other distant NGC globs. The close ones were explosions of stars that filled the eyepiece. The distant ones shimmered out of the black like the lights of distant cities. Then we moved on to galaxies. M81 and M82 were bigger, brighter, and more detailed than I had ever seen them. M51 was just stunning – the spiral arms were so well-defined that it looked like Lord Rosse’s sketch.

M51 sketch by Lord Rosse

As nice as those were, the Virgo galaxy cluster was better. There were so many galaxies that identifying them was a pain – there were so many little NGCs in between the familiar Messier galaxies that my usual identification strategies kept getting derailed. It was kind of embarrassing, actually – I did just write an article about this stuff. But also incredible. NGC 4435 and 4438 – the pair of galaxies known as “The Eyes” – were so big, bright, and widely separated that I didn’t realize I was looking at them until the third or fourth pass.

We finished up on planetary nebulae. The seeing was good but not perfect – the central star in the Ring Nebula was visible about a quarter of the time. The Cat’s Eye, NGC 6543, was a fat green S with a prominent central star – it looked like it had been carved out of jade.

An evening under dark skies with a giant scope is both a blessing and a curse. A blessing because you get to see so many unfamiliar objects, and so many details in familiar objects, that are beyond the reach of smaller scopes. A curse because by the end of the session you may find yourself thinking, “Sheesh, why do I even bother with my little 3-, 5-, and 10-inch scopes?”

Fortunately another observing experience, one that would remind me of the joys of small-aperture observing, was right around the corner.

Observing Report 3 (Small): A Binocular Tour of the Spring Sky

My son, London, is finishing up fifth grade at Oakmont Outdoor School, one of the half-dozen or so different elementary schools in the Claremont Unified School District. We were fortunate when we moved to Claremont to land just a couple of blocks from Oakmont – we would have been happy to land within walking distance of any of the schools, but if we’d had our choice we would have picked Oakmont anyway, since we wanted to raise London with as much exposure to the outdoors as we could.

Oakmont’s slogan is, “Learning in the world’s biomes”. The major activities of each grade are organized around a particular biome, and so is the end-of-year field trip. In third grade, the kids went to Sea World. Last year it was the desert by Palm Springs for a 2-day, 1-night trip. This year it was Santa Cruz Island, in Channel Islands National Park, for a 3-day, 2-night trip. Parent chaperones are needed and I’ve been fortunate to get to go every year.

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The island was amazing. We saw dolphins, sea lions, and petrels on the boat ride out – I took the photo above from the prow of the ship – more sea lions, seals, pelicans, cormorants, gulls, and red pelagic crabs at the shore, and dwarf island foxes, ravens, and the occasional hawk inland. On the final evening, June 2, we hiked up to the top of the cliffs to watch the sun set over the Pacific, which was one of the most beautiful things I have ever seen in my life. I didn’t know it at the time, but I’d see something even more beautiful just a few hours later.

I had binoculars along – Bushnell 10×40 roofs that I got specifically for daytime use, and which I had used a lot on the trip already to watch wildlife. When we got back to camp, a few of the teachers and hung back and started talking about the planets, bright stars, and constellations. I started pointing out a few of the brighter targets and passing around the binoculars, and we ended up having an impromptu binocular star party. (The kids and a fair number of the adults were all exhausted from a full day of hiking, and sensibly went to bed.)

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What followed was one of the best and most memorable observing sessions of my life. The only permanent residents of Santa Cruz Island are a couple of National Park employees, and they turn their lights off after dark. We got a little light pollution on the eastern horizon from Ventura and Oxnard, some 20 miles distant, but for the most part the sky was darkAfton Canyon dark, Hovatter Road dark – what I typically refer to as stupid dark.

We roamed all over the sky, looking at targets large and small, near and far, bright and dim. I didn’t keep track as we were going, but I wrote down a list yesterday morning on the boat ride back to the mainland (we went through a fog bank and only saw a handful of dolphins, so I had plenty of time).

In the northern sky:

  • Polaris and the Engagement Ring asterism
  • Mizar and Alcor
  • M51 – yes, it was visible in the 10×40 bins
  • The 3 Leaps of the Gazelle

In the western sky:

  • M44, the Beehive – easily visible to the naked eye, and just stunning in the binos
  • Leo
  • Coma Berenices star cluster
  • Virgo/Coma galaxies – identifications were tough, but a few were visible

In the eastern sky, Lyra had just cleared the trees when we started observing (at 9:15 or so), and all of Cygnus was above the trees when we finally shut down at 12:45 AM. In addition to tracing out the constellations, along the way we looked at:

  • Epsilon Lyrae, the Double-Double star
  • Albireo
  • Alpha Vulpeculae (the subject of my Binocular Highlight column in the ### issue of Sky & Telescope)
  • Brocchi’s Coathanger (Collinder 399)
  • Sagitta (just traced the constellation)
  • M27, the Dumbbell Nebula
  • Sadr and its surrounding ring of stars in the heart of Cygnus
  • NGC 7000, the North American Nebula – this and the Northern Coalsack were easily visible to the naked eye once Cygnus has risen out of the near-horizon LP

…and we just cruised the Milky Way from Cygnus to Cepheus, not singling out individual objects but just taking in the rich star fields.

But the southern sky was the best. Looking south from Santa Cruz Island, there’s only open ocean, broken here and there by other, distant islands and ultimately by Antarctica. It reminded me of looking south from Punta del Este in Uruguay, only I was in a valley instead of on a beach. The ridgeline to the south did cut off a bit of the sky, but we were still able to see all of Scorpio, including the False Comet, made up of NGC 6231 and Trumpler 24, which was one of the highlights.

It was trippy watching the Milky Way rise. I usually look at the summer Milky Way when it is higher overhead. I usually have to do that, because the objects aren’t visible in the near-horizon haze. But from Santa Cruz Island, things were not only bright but obvious as soon as they cleared the ridgeline to the south. It’s almost pointless to list them – we saw every Messier object in the “steam from the teapot”, from M7 and M6 in the south to M11 in the north, plus a lot of NGCs, plus star clouds and dark nebulae almost beyond counting. They were all great through the binoculars – M7 was a special treat, like a globular cluster on a diet – but honestly the best views of the night were naked-eye.

I realized that I am just never out observing the Milky Way at this time of year. My regular desert observing spots are all too hot in the summer, and when I do go there is often at least some light pollution to the south (El Centro from the Salton Sea, Barstow from Owl Canyon, etc.). I do most of my deep and dark observing in October and November, when the southern Milky Way is setting, not rising.

So I was completely unprepared for how much detail would be visible to the naked eye. When the Milky Way rose, it didn’t look like a band of light, it looked like a galaxy. I searched through a lot of photographs of the rising Milky Way to find one that approximated the naked-eye view, and this is the closest I got:

I am not exaggerating – the bright and dark areas were that defined. The Great Rift was visible from Cygnus to the horizon, and its southern border was notched by distinct deep sky objects from Aquila onward. The Scutum Star Cloud, M16, M17, M24, M23, M8, M6, M7, NGC 6281, and the False Comet were all easily visible to the naked eye as a chain of luminous patches against the dark dust lane of our own galaxy. In fact, I noted NGC 6281 with my naked eyes first, thought, “What the heck is that?”, and had to look it up. We also caught M4, M22, M23, and M25 in the bins, plus a bundle of dark nebulae that I’d never noted before and didn’t bother keeping track of.

Longtime S&T contributor Tony Flanders (now retired but still writing occasionally) is active on Cloudy Nights, and his sig file reads:

First and foremost observing love: naked eye.
Second, binoculars.
Last but not least, telescopes.
And I sometimes dabble with cameras.

Until fairly recently I would have listed my own preferences in reverse order, from telescopes to binos to naked eye. That may sound odd for a “bino guy”, which I guess I am since all of my ‘professional’ astro-writing has been binocular-based. But it’s true – as much as I love binoculars, I would have picked a telescope first. But I am – gradually, belatedly – waking up. In some ways, it would have been great to have a scope, any scope, along on the island trip. I’m sure that even the C80ED would have taken us crazy deep, considering what we could see with a pair of low-end 40mm roof-prism bins. But it would also have come between us and the sky, and I would have spent more time futzing with eyepieces and less time just looking up.

This was a surprising and welcome realization, coming so shortly on the heels of a frankly astonishing session with Ron’s 25-inch dob at RTMC. I was worried that big-telescope observing might spoil me, but that fear turned out to be unfounded. All I need to be happy is a dark sky. If I have some people to share it with, even better. Anything more is just cake at the end of an already long buffet.

Let’s eat.

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Observing report: the transit of Mercury from western Colorado

May 19, 2016

Mercury transit 9 May 2016 - telescope setup

I was in Utah from May 4 to May 15, chasing dinosaurs with Mike Taylor, a colleague of mine from England. I took a telescope along in hopes of getting some dark-sky time, and to hopefully catch the transit of Mercury on May 9.

Things did not look promising at dawn on the 9th. I was in Fruita, Colorado, and when I got out of bed, the sky was completely overcast. Mike and I decided to head out west of town to visit Rabbit Valley, where a nearly complete skeleton of the long-necked dinosaur Camarasaurus is visible in a hard sandstone ledge. (Why is no-one excavating this dinosaur? Because we already have many nice specimens of Camarasaurus, and the sandstone around this one is like concrete. It would be a mountain of work for very little payoff.)

We spent about two hours measuring and photographing the skeleton, and as we did so, the clouds started to break up a bit. By the time we got back to Fruita, a little after 11:00 AM, the sky was clear except for a few scattered wisps of cloud. I set up my telescope in front of the Dinosaur Journey museum and started watching and photographing the transit.

Mercury transit 9 May 2016 - Mercury crossing the sun

I was using the same setup as in the last post: my Celestron C80ED refractor, a Celestron 8-24mm zoom eyepiece, and a GoSky full aperture solar film filter. For photography, I used a Nikon Coolpix 4500 for still photos and my iPhone 5c for video.

I caught about the last hour of the transit, and I got to share the view with about a dozen museum staff and passersby. A few light clouds drifted through the field of view, which looked pretty cool and didn’t obscure the view at all.

At 12:42 Mercury finished exiting the disk of the sun. The next Mercury transit will be in 2019 – I hope I’m as lucky then as I was this time.