Intending to spend some time in Hercules last night, I initially mounted and aligned the Pinty laser finder that was recommended here. I used Polaris, out of convenience, to align the green laser to the FOV in the OB127s. To begin with the alignment was way low and to the left, and I wondered if I would run out of adjustment travel, but there was plenty to dial it in, and that's all it took. Once centered in the BTs FOV, the beam remained there through-out the session. Very solid unit, just what I need for my style of star hopping with BTs. Amazing that something this good is so inexpensive. I like the on/off push button on the end of the laser sight and used it as opposed to the optional extension cord switch.
Moving over to Hercules, which was pretty much at Zenith, I began my observing with the globular cluster M13. I was using Pentax XW 10mm eyepieces, with an effective power of 65x in this BT. Once in view, M13 was glorious. I could see some elements of individual star structure, especially with averted vision. Globular clusters are in a special category of binocular delicacies for me. M13 tonight, with my particular 65x BT view, shone brightly, and was very satisfying. However, M13 can be seen with the naked eye under the right conditions - just not for me. This night was not the best for seeing, with thin clouds and moon glow. Discovered in 1714, Edmund Halley said in so many words that with the naked eye it is a little patch of light that can be seen when the skies are "serene" and when there is no moon. 50 years later, Charles Messier was to catalog it as "not a comet", and it has become known as Messier 13, or as some call it, the Great Hercules Globular Cluster.
Over on the opposite side of the keystone in an area I call the left thigh of Hercules (based on constellation art), lies a group of three stars that I was interested in exploring - Pi, 69, and Rho Herculis. My attention quickly centered on Rho Herculis. In my field of view, with Rho centered, I saw a symmetry of stars on either side, in somewhat the shape of a flattened octagon, with Rho at the bottom center in my FOV. As I viewed this structure and tried to see a shape in it, I noticed the Rho was actually two stars, tight together and aligned toward the north east. One star appeared yellow/white and the other gray or bluish. They were about the same magnitude. Excited about these twins I decided to take an intermission, to check on this unexpected double and to see if any others were nearby. Back at the BTs, I began to explore what I had found from Stellarium and Stelle Doppe - STF 2161 AB and STT329.
STF 2161 AB
Coordinates: 17 23 41, +37 08 45
Separation, PA: 4.1", 321degrees
Magnitudes: 4.50, 5.40
A serendipitous encounter, this double was engrossing, and led me to post about it in this double star thread. I was quite happy to discover that the separation was 4.1" since it was so cleanly split in the Pentax 10mm eyepieces. The direction was almost perfectly NE, with the slight magnitude difference between the primary and 2nd now visible. As far as coloring goes, to my eyes the primary was more toward yellow and white, whereas its companion was appeared to be tinted blue. This double dominates the field of view with its combined magnitude, and together with the pattern of surrounding stars in the view, left me wanting to assign an asterism type shape to it, but none were forth coming except "squashed octagon".
It was interesting enough to make a diagram or rendering of it.
STT 329
Coordinates: 17245, +3657
Separation, PA: 33.5", 12 degrees
Magnitudes: 6.35, 9.88
Up and slightly to the left in the same filed of view as Rho Herculis, there was supposed to be another double star. I hadn't really noticed it in the first observation. But after the intermission I knew where to look. I wasn't the least bit disappointed. STT 329 is a completely different type of double star from the previous one. The first contrast is that the separation was much greater - 33.5" compared to 4.1. Then there was the huge magnitude delta of 3.5, four times greater than the one above. What is there about a big mag contrast the makes the secondary star appear mysterious or even majestic? Maybe its just me, but when I saw HD 157910B within the glow of its primary star, it riveted my view for quite awhile. It was distinct and easy to see at almost magnitude 10. Then when going back to this double, it would grab my attention even before the primary would. This is somewhat reminiscent of the Polaris and Mintaka doubles in my memory. Anyway, this double is a fun one to observe, especially in the context of the Rho Herculis double, and the associated stars in this FOV. As I remember it, the colors of the stars in this double were white/yellow for the primary and gray-yellow-orange for the companion. For me, dim stars tend to go more towards gray, and are difficult to extract color. Overall this was a very pleasing double to view, and another BT opportunity not intentionally targeted.
To top off the session I wanted to take in M92 before leaving the scene. I pointed the BTs and Pinty laser in the general direction of M92, about 5 degrees north of Pi Herculis. Then using 12x42s with one hand and moving the BTs and laser beam with the other, I got convergence of the green beam, 12x42 FOV and the globular cluster. Trifecta achieved! Did I mention that I really like this laser sight? M92 appeared as a cold, lonely, gray cotton ball in a sea of darkness. But it still held its own as a globular cluster delicacy. I could not see any detail within the cluster as I did with M13, but it was still engaging to observe. M92 is not as easy to see with the naked eye as M13 - for those that have dark skies of course. It was discovered in 1777 and initially described as a nebula. Charles Messier rediscovered it in December of 1781, and during the same evening also catalogued M84-M91. What a night that must have been!
This is long, so thanks for reading!
Clear skies everyone, or a gap in the clouds when you need one 

Edited by aznuge, 06 August 2022 - 09:49 PM.