A Work Commenced October 5 2024
For the past few years I’ve been using a very good 10 x 50 Opticron Porro prism binocular, which has served me well as a longer range terrestrial magnifier and also for conducting astronomical observations. I chose this instrument for its great build quality and bright and sharp optics. It’s small field of view(5.3 degrees), was enough to frame nearly all the celestial objects I visit throughout the observing year. This size of field also pretty much guaranteed a fairly flat field from edge to edge, keeping stellar images tight and sharp no matter where they’re placed within the field. Back in May however, I bought in an amazing new high-performance roof prism binocular: the Sky Rover Banner Cloud(SRBC) 10 x 50 for review, and its quality literally stunned me. This instrument sported an ultra-flat field, fully double the size of my old 10 x 50 and with excellent colour correction. And while I was able to demonstrate its daylight capabilities in Part I( see the preamble above), I was unable to evaluate its night sky performance owing to the encroach of summer twilight which graces the Scottish landscape between May and the end of July, during which time there is no proper darkness, with only the brightest stars visible in the heavens.
A Trip to Italy
During early July, our family took off on vacation to northern Italy, basing ourselves in a small commune called Revine Lago, Sottacroda, in the foothills of the great Dolomite Mountain Range, and right in the heart of the Prosecco wine cultivation region of northeastern Italy.
With a climate of hot summers and frequent rain, the area is lush with vegetation. I brought along the 10 x 50 as well as its smaller sibling, the 8 x 42 SRBC, to do some daytime birding and visual astronomy after dark. It was also an ideal environment to test the hardiness of these instruments as they were exposed to dust and intense summer heat, where daytime temperatures soared to well above 40C in direct sunlight. I can report that both instruments coped admirably in these hotter, dustier conditions.
While most of my birding was conducted with the smaller 8 x 42 glass, I also found myself using the larger 10 x 50 SRBC quite a bit at my local birding patch, overlooking Marine Lago, a small freshwater lake just a kilometre’s walk from our holiday home. For example, while the 8 x 42 frequently picked up some birds fishing the lake far from shore, it was difficult to make a reliable identification, as they remained small in the huge field of view of the 8 x 42, I was able to use the higher power of the 10 x 50 instrument to tease out more detail. And it paid off! These turned out to be Great Crested Grebes, a species I’ve never personally encountered before.
Both the 8 x 42 and 10 x 50 are extremely stable in my hands. I can hold the 8 x 42 almost rock steady owing to its long barrels and excellent inertia. The 10 x 50 is marginally less stable, of course, more due to the magnification than the weight. My own experiences with lower mass models has definitely shown me that they are less stable at any given power. And if it’s a windy day, I’ll always opt for a heavier glass. This is a very overlooked phenomenon in my opinion, as many folk mistakingly opt for smaller, lighter glasses that are easier to transport. But in my book, optimal inertia overrides such concerns under most conditions.
In early July in northern Italy, sundown occurs shortly after 9 PM local time, although full darkness doesn’t come until after 11 PM. Venturing out about 10:30PM to assess sky conditions, I was greeted by a truly amazing sight: fireflies! Apparently, this location provides the exact hot and humid micro environment for their thriving. I stood in sheer amazement as they flashed in front of my eyes, flying off to gather in nearby bushes. By 11:30 PM they had vanished!
Sky conditions were not as dark as I’d have liked though: a solid Bortle 4, a little bit brighter than my skies in rural central Scotland. Nonetheless, I made full use of the true darkness beginning with Sagittarius and Scorpius well placed in the south around local Midnight. These constellations are too low in the sky at my far northerly latitude of 56 degrees north, so I relished the opportunity to preferentially observe them, together with some selected targets in Ophiuchus. Sitting comfortably in a reclining chair I used the 10 x 50 hand-held to drink up the views. The instrument picked up the rich river of Milky Way starlight coursing through Sagittarius, looking ‘downtown’ as it were, into the centre of our galaxy. Sweeping northwest of the constellation’s brightest luminary, I moved the glass over the Teapot asterism and then on to the Spout, placing Lambda Sagittarii on the eastern edge of my binocular portal, where the 10 x 50 SRBC’s great field of view allowed me to make out the tidy globular cluster M28, and further west, the soft, ghostly light from both the Lagoon(M17) and Trifid Nebulae(M20), with the bright open cluster M21 above them to the north. A delightful view if ever I’ve experienced one!
Moving further west into Scorpius, I centred the bright ruddy star, Antares, and immediately picked up the faint glow of the magnificent globular cluster M4. Spanning an area roughly the size of the full Moon, it’s the closest cluster of its kind to the solar system – a mere 7,200 light years from the solar system. Most of them are situated far out in the halo of our galaxy. Just to the north of Antares, I could see the comely triple system Rho Ophiuchi, arranged in a neat little triangle. I forsook looking further south towards the celestial gems in the Scorpion’s tail owing to the encroach of a light dome from Vittorio Venito, about six miles to the south of our commune.
Positioning my binocular field between northern Sagittarius and northern Scorpius, I examined the region of sky around Theta Ophiuchi, when I quickly chanced on the pretty binocular double 36 Ophiuchi, with its golden primary and fainter white secondary. In the opulent 7.5 degree field of the 10 x 50 SRBC, I picked up the faint glow of yet another summer globular cluster – M19 off to its west. Ophiuchus has many resplendent globular clusters. Centring Marfik and panning slightly in a southeastward direction I was able to bag two more in the same field: M12 and M10 – both about 12 billion years old! Splendid!
The great river of stars of the summer Milky Way was plainly visible overhead and, sitting back in a recliner, I aimed the 10 x 50 SRBC at Sadr in the heart of Cygnus. The view was stunning! Myriad stars of various degrees of glory filled the field, remaining sharp pinpoints from edge to edge. The dust obscured region immediately around Sadr provided some gorgeous contrast surrounded by a blizzard of faint stars. I had to have a quick look at the fetching colours of O^1 and O^2 Cygni. Their beautiful hues stood out starkly against a coal black sky.
In the following days, we hooked up with my family to attend my nephew’s wedding in the grounds of the beautiful medieval fortress of Castello San Salvatore on the afternoon of July 9.
A beautiful crescent Moon greeted us in the sky after sunset. Once we got home, I fetched the 10 x 50 for a quick peek. And I wasn’t disappointed: she was marble white with no colour fringing in the centre of the field, the vast southern highlands bristling with craters. It was a fine ending to a most beautiful day!
After a few days in Venice, we returned home to the cool of Scotland. It was a great experience but ultimately too hot for my liking.
Both SRBCs coped admirably though in the intense Italian heat, serving up delightful views by day and by night.
Astronomical Forays under Scottish Skies
While the 10 x 50 SRBC is good to go for short, hand-held astronomical viewing, it certainly benefits from stabilisation using either a tripod or monopod, neither of which were available to me on the Italy trip. For all of my observations here in Scotland, I opted to use the extremely robust and well designed Oberwerk Series 2000 monopod, with a trigger grip mechanism built into the ball & socket mount, which enables the user to alter both the altitude and azimuth movements very easily. At its full extension, it allows six footers like me to observe targets fairly comfortably, even when they are situated near the zenith. This kind of stabilisation rig greatly facilitates studying astronomical targets for longer periods, reducing fatigue and revealing fainter objects within its vast field of view.
Beginning my observations in mid-August, with the return to true dark skies to our latitude, the circumpolar constellations of Cassiopeia and Perseus are already well placed high in the eastern sky after midnight.
The Milky Way runs richly through Cassiopeia and the 10 x 50 revealed stunning panoramic views within its generous field. To put this somewhat in perspective, the SRBC field is much wider than the 6.6 degree field of the Swarovski EL 10 x 50 and it’s even a tad wider than the newly-launched NL Pure 10 x 52(7.4 degrees)! Couple this with an ultra-flat field and excellent control of chromatic aberration and you can begin to appreciate just how compelling the views are through this instrument.
My first sweep through Cassiopeia with the 10 x 50 really thrilled me. Starting at Ruchbah, sparkling in its striking blue-white light, revealed a few beautiful star clusters in the same field of view, most notably M103, with the Owl(or ET) cluster(NGC 457) off to its south southeast. Several other fainter clusters showed up in the same starfield. After admiring the prominent orange colour of Schedar, I followed a line through to Caph where I picked up the prominent misty patch of M52 about 6 degrees off to its northeast. About 3 degrees south of Caph, the same field easily picked up the open cluster NGC 7789 spanning the size of the full Moon. Some observers have remarked that it looks like the head of a tailless comet. I certainly can’t argue with that description! Scanning the area between Gamma Cassiopeiae and Caph easily picked up the smaller star clusters NGC 129 and 225 in a rich background of Milky Way stars.
Before leaving Cassiopeia, I noticed the bright star, Capella, had reached a decent altitude in the northeast. Then aiming the 10 x 50 at a spot roughly mid-way between Epsilon Cassiopeiae(the fainter star marking the tip of the Wonky W) and Capella, I was quickly able to bag Kemble’s Cascade in Camelopardalis- a remarkable line of about 15 faint stars extending over 2.5 degrees, with a single brighter star marking its centre(almost!). The cascade ends by bifurcating into two distinct starry patches, one of which is marked by a compact 6th magnitude open cluster, NGC 1502. Doubtless, the great light gathering power and huge field of view of the instrument greatly facilitates finding this showpiece object easily and quickly.
By October, Perseus is very well placed for observation high in the eastern sky. Pointing the 10 x 50 SRBC at Alpha Persei(Mirfak) serves up a view par excellence. The entire field is peppered with bright stars. Roughly half of the two dozen or so members lie within a mere 2 degrees of Alpha Persei, with the remaining members fanning out in stunning swirls and streams of starlight. Many of the members of this loose open cluster are youthful, hot white stars, yet the excellent colour correction of the SRBC picks up members with a different hues; orange, yellow and creamy white.
Moving up the sky to a spot roughly midway between Perseus and Cassiopeia the naked eye easily picks out a misty patch that is transformed into yet another visual treat in the 10 x 50: the famous Double Cluster. Steadied on the monopod, the instrument presents this cluster in all its glory but the eye is also drawn to a prominent curving chain of stars moving off northward ending in the enchanting Stock 2 open cluster. The Double Cluster and its rich Milly Way hinterland is arguably one of the most beautiful sights in all the heavens!
Placing Algol, the Demon star, on the eastern side of the field of view, you’ll see the bright open cluster, M34 off to the west. The SRBC resolves about a dozen of the brighter members of this condensed cluster well, with the remaining constituents creating a misty backdrop easily covering the size of the full Moon.
This time of year the constellation of Cepheus looms large high in the northwest and I couldn’t resist the temptation to have a look at one of the most fascinating and colourful stars in the heavens: Mu Cephei, or Herschel’s Garnet Star. By aiming at a patch of sky between Alpha and Zeta Cephei, the large field of view of the view of the 10 x 50 SRBC very quickly picked up its unmistakable deep red hue. It’s a stunning sight in this instrument – glowing across the light years, like the dying embers of coal fire. About one binocular field off to the northeast of Mu Cephei towards Cassiopeia, the binocular showed me the faint but exceedingly rich star cluster Trumpler 37, which spans an area roughly 3 full Moon diameters in area. It’is a lovely sight in the 10 x 50 on a dark, October night.
Moving round the autumn sky, the Andromeda Galaxy M31 and its satellites, M32 to its south and M110 further away to its north are fine sights in the SRBC. More challenging is M33 in Triangulum. But it proved easy pickings for this wide angle 10 x 50, simply by placing Alpha Trianguli towards the eastern end of the field when the ghostly glow of this face-on spiral galaxy appears to its west, and with plenty of room to spare.
Waiting until the wee small hours of a dark moonless night, Taurus, Orion and Gemini begin to dominate the eastern sky. Mighty Jupiter rises early with the stars of Taurus and shines like a bright, distant lantern with its steady, creamy white light. The stabilised 10 x 50 easily shows the ephemeral dance of its four large Galilean moons, constantly shifting their positions hour by hour, as they orbit the giant planet. Mars rises later, its dimmer but unmistakable ruddy hue seen just under Wasat in the midsection of the Twins.
Auriga, the celestial Charioteer, is also very well placed at these ungodly hours of an October night. The three Messier open clusters, M36, M37 and M38 show up beautifully in the SRBC, within the same field of view, with M36 being partially resolved into stars.
The Hyades and Pleiades are spectacular objects in the 10 x 50. The horns of the celestial Bull fit comfortably within its large field, and I was delighted to see the lovely open cluster, NGC 1674 to the eastern edge of the same field, something quite beyond the capability of my old 10 x 50 Porro.
Orion holds many treasures for the dedicated star gazer, but you’ll have to wait until about 4.00 AM this time of year before it approaches the meridian. The Belt Stars and its surrounding cluster, Collinder 70, is a spectacular sight on a night of good transparency, with the familiar Snake asterism showing up prominently.
Further south, the Sword Handle of Orion is a sight for sore eyes steadied on a monopod, but I also enjoyed studying the lovely group of stars in the north of the constellation- Meissa – a neat little Pythagorean triangle of brighter stars, with a delicate line of three fainter suns linking Lambda Orionis to Phi^1. Incidentally, Meissa lies just north of a line joining bright red Betelgeuse and Bellatrix, which are conveniently separated by 7.55 angular degrees of dark sky. This was a good test to measure the true field size of the 10 x 50 SRBC and, sure enough, they were just too far apart to fit inside the field.
Finally, at about 4:30 AM, looking east of Orion, Gemini loomed large, with Mars, a bright ‘nova’ decorating its mid-section. I took the opportunity to seek out the wonderful open cluster M35, clearly fan-shaped, with many of its stars resolved, framed by two beautiful orange stars, Mu & Eta Geminorum, pointing the way in the same field of view. Such an enchanting sight!
Conclusions
The above observations are but a small selection of celestial objects I visited over the last few months with the 10 x 50 SRBC. Incidentally, a new and thorough review of its 12 x 50 sibling has also been published and is well worth a look!
Starting too early in the evening shows up countless artificial satellites: many dozens seen on a typical evening, with sometimes two or three seen crossing through the same field! As the night progresses, those orbiting at lower altitudes disappear first, with those placed in higher orbits fading out last. Temperatures ranged from a balmy 25C on the warmest nights to a few degrees below zero on the coolest.
Throughout these vigils, the SRBC performed flawlessly, with no change in the kinematics of the focus wheel and no fogging up of the eyepieces and objective lenses due in part to the excellent hydrophobic coatings applied to the exterior lenses. It’s been a joyous experience looking through such high quality light cups, their enormous fields making it much easier to find the more elusive objects visited. Alas, I have as yet not been lucky enough to bag the new comet gracing our western skies after sunset, but I hope to finally glimpse this icy interloper from the Oort Cloud, before it disappears into the cold dark of interstellar space.
Wish me good luck won’t you!
Update December 6 2024: I did manage to see Comet Tsuchinshan on the evening of October 14 and again on October 17 using the 10 x 50 SRBC. Past its prime I know, but still well worth the effort! Mars moved from Gemini into Cancer on October 20, and in the wee small hours of a very blustery December 6, it was observed just over two degrees north of the celebrated Beehive Cluster. A glorious sight to see right now. It should inch a little closer to the Beehive in the hours to come!
Neil English has been observing the night sky from the tender age of eleven, and has written 8 books about these experiences.
