Tag Archives: Bob Piekiel

CNYO Observing Log: Baltimore Woods, 14 June 2013

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Perhaps the last bug-free (of the buzzing kind, that is) observing session until later in the fall, Bob Piekiel hosted his monthly Baltimore Woods observing session on Friday, 14 June 2013 at the same time that the Syracuse Astronomical Society hosted a public viewing session at Darling Hill. An excellent Friday for taking in the CNY skies beyond the Syracuse skyline!

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Bob Piekiel performing collimation surgery.

Scope-wielding CNYO members in attendance included Bob Piekiel with 8″ and 11″ SCTs, Larry Slosberg with his trusty New Moon Telescopes 12″ Dobsonian, and myself with my 25×100 Zhumell binoculars (despite a last-minute re-collimation surgery, Bob couldn’t get his monster pair of Vixen 25×125 binos up to his satisfaction. I await the next session to take in that view!).

Beyond the several deeper sky objects we observed that evening, attendees were treated to (1) two ISS flybys (and the rather spectacular run of ISS flybys this month will be the part of an upcoming article), (2) four bright meteors (total count from among the observing group) that all appeared to radiate from the vicinity of Libra and Virgo (so the meteors all appeared to move from the SouthWest to the NorthEast), and (3) more than 20 satellites that crossed fields of view or were prominent enough during the ISS watch to jump out to most everyone. The sky was dominated by the 6 day old waxing crescent *always super* Moon, excellent at all magnifications and the best binocular object in our Night Sky.

As has been a recurring theme in some of these observing logs, the variety of available optics gives one the ability to experience the pros and cons of different equipment first-hand both in terms of setup and magnification.

The Zhumell big binos are easy to setup and provide excellent views of the Moon and some of the very open star clusters. We used the binos as a “sneak preview” of our observing of Saturn as we waited for enough bright stars to appear for Bob to get his GOTO scopes aligned. Even in the binos, Saturn is obviously “Saturn,” with the ring system, planet, and gap between the rings and planet visible. You will fight for the Cassini Division in less transparent skies, but a steady mount and patience will grant you a peak of this dark band between the two major rings.

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Larry S. and Michelle M. in a Dob setup action shot.

Larry’s NMT Dob is a 5-minute setup from car to observing, with only a modicum of labored transport from the parking lot to the ground. In moonlit skies, nebula, galaxies, and faint fuzzy objects require a good memory or a great trust in one’s Telrad. On the minus side, you spend extra time trying to find faint objects – this only being a real problem during Public Viewing sessions when you really don’t want to spend all your time finding “something” to see. On the plus side, you really learn the sky this way, you don’t have to worry about battery life and any of the problems that come from modern observing technology, and you can generally get a larger mirror for the same amount of carrying-intensive weight in a Dob over a Schmidt-Cassegrain Telescope (SCT), which means a generally better view.

Bob’s two SCT GOTO scopes are, after setup, perhaps the best way to facilitate a Public Viewing session, as you simply call for the object you want to see in the GOTO controller and, with some grinding of gears, you spare yourself from the hunt. In the case of his image intensifier, your GOTO scope might land on a galaxy too faint to even acknowledge seeing through a good eyepiece. Your GOTO purchase is validated when the intensifier then brings out subtle detail in an otherwise invisible object, a search that might easily aggravate a novice Dob user.

All of that said, we remind ourselves of the words of Stu Forster – “The best scope is the one you use.”

For my part, I spent time Naked Eye observing and adding to discussions going on around scopes. The confirmed sightings list contained Saturn, M3, M13, and M57 (the Ring Nebula, both with and without enhancement).

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15 seconds of fun with a red flashlight and green laser pointer.

Increasing dew around 10:30 p.m. left us to pack up gear and simply enjoy the naked eye Night Sky (and play with the long exposure setting on my Canon Digital Elph). The next even is scheduled for July 12/13 at Baltimore Woods, followed by Bob Piekiel’s “Star Search” event at Green Lakes on July 26th. We hope you can join us!

Bob Piekiel Hosts “Star Search!” At Green Lakes State Park – July 26 (27 alt.)

Greetings fellow astrophiles!

I’m happy to announce that Bob Piekiel will be hosting a free observing session at Green Lakes State Park on Friday, July 26th (with the 27th as a weather-alternate). Any interested CNYO scope owners planning on attending (with their scopes, that is) please drop me a line at observing@cnyo.org for the head count (will remind by email before the event). Everyone else, just show up!


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The night’s observing feast includes Venus in the early evening, Neptune 1/2 hour before the Moon rises at 11:00 p.m., and Saturn, our prize object for the year, visible throughout. Clear skies pending, it is possible we might even see some of the early part of the Delta Aquarid meteor shower. Additional details are available in the flyer below (click for a full-sized image for printing and distributing).

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CNYO Observing Log: Beaver Lake Nature Center, 2 May 2013

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Greetings fellow astrophiles,

May 2nd served as the rain date (due to rapidly-overcasting conditions on April 25th) for our first Beaver Lake Nature Center lecture of the year – The Guiding & Wandering Stars – Key Northern Constellations & Planet Observations. On hand to run scopes and engage in lecture duties were the author with a 12.5″ New Moon Telescope Dobsonian, Larry Slosberg with one Meade SCT and Bob Piekiel with another.

The Constellations have been with us for thousands of years, but there are only a few good, clear nights each month to memorize their positions as they slowly move across the sky! This outdoor lecture by the CNY Observers (www.cnyo.org) will briefly describe the history and importance of the Constellations as mythological, agricultural, and navigational guides, then will describe a simple system to begin to learn their relative positions. At the same time, Jupiter and Saturn are on opposite sides of the Southern sky, making excellent targets for binocular and telescope observing. Free and open to the public.

While the week including May 2nd will be known to some as a particularly bad week for maple tree allergies, the nighttime sky stayed quite clear and the bugs eventually froze around us to produce an excellent session. The attending crowd of about 35 served as test subjects for both our two new brochures (How The Night Sky Moves and Guide For New Observers) and our first official completely outdoors (Powerpoint-free) lecture (which, despite astronomy being such a visual hobby, worked will with just the brochure contents). In anticipation of some nighttime brochure reading, I put together some red light flashlights on the cheap locally. For anyone attempting similar, I found a four-pack of Dorcy AAA 6 LED Flashlights at Dicks Sporting Goods for $10. Some very minor surgery is needed to remove the top caps, but conversion to red light flashlights is straightforward with the help of a four-layer stack of red acetate purchased many moons ago from Commercial Art Supply in Syracuse.

406px-EB1711_Armillary_SphereDespite a little confusion about the start time (7:30 or 8:00), everyone had pulled in by 7:45 p.m., so we began the session with a good 30 minutes of physics. The goal of these Beaver Lake lectures is to not only observe objects, but to explain why the sky moves as it does so those trying to learn new constellations will understand what to expect both over the course of a night and over the course of a year. This began at the ground floor – understanding how the Earth moves around the Sun. With the help of an armillary sphere (which holds the Earth at its 23 degree tilt – see the image at left from wikipedia), the Earth’s movement around the Sun was demonstrated, specifically showing that the rotation axis stays pointed the same way as we revolve – thus resulting in Polaris appearing not to move over the course of the year despite the Earth shifting position by 300 million kilometers (2 astronomical units) every 6 months. Knowing that Polaris is always in the same place in the sky (whether it’s daytime or not) leads smoothly into a discussion of the circumpolar constellations and the benefit of learning these six constellations first (for this discussion and some how-to’s, I refer you to the CNYO brochure: Guide For New Observers).

Running a sunset-to-late-night session with a non-cycling crowd has (at least) two distinct advantages. First, the importance of dark adaption and the need to avoid smart phones (or avoid their use around others) can be stressed early in the evening. While enforcing protocols to maintain dark adaption at any kind of public lecture is usually a losing battle, anyone answering a phone did it in a very non-obvious manner, which was most welcome. Second, the mechanics of my Dobsonian telescope and Larry and Bob’s two motorized SCTs could be presented while still visible to attendees. More importantly, the proper observing technique for all could be demonstrated by showing (a) how to approach an eyepiece (I tell people to put their hands behind their back and simply lean into the eyepiece) and (b) just how easy it is to nudge a scope away from its target. Specifically for the Dob, I’m sure anyone who’s brought their scope to a public session has had at least one person lean on or pull closer an eyepiece. I’m pleased to report that, once the observing started, our collective intro to scope workings made my Dob-running life simple with no unplanned re-adjustments (just adjustments of the unmotorized kind).

As stated in a previous post (2013 March 8 – At The Syracuse Inner Harbor), new observers are best introduced to observing with easy objects that don’t require training. Deep, dim, distant galaxies are not useful starters for someone with no background in eyepiece observing. For my part, a good 70 minutes were spent on Jupiter (low in the Western Sky with all four Galilean moons present), Saturn (low in the Eastern Sky and my first view of it this year), Arcturus in Boötes (its shimmering in the sky both with and without magnification was a point of discussion for several near my scope), M13 (the globular cluster in Hercules, which served as a first “way out” object and an example of using the constellations as a “coarse adjustment” for finding Messier and other objects), and the pair Alcor and Mizar in the handle of the Big Dipper/tail of Ursa Major (to show the separation and additional detail that comes with magnification).

With a much smaller crowd around 9:30 p.m., I did treat a few interested parties to some more difficult observing in my scope – The Leo Triplet – after first briefly explaining the mechanics of averted vision. Of the five people who looked, all could make out M65, all could at least tell that something “was there” where M66 rested, and three people could tell that “something else” was there at NGC 3628‘s position. And I did miss a golden opportunity to observe NGC 4565 (my personal favorite) in Coma Berenices.

We closed up shop at 10 p.m., just as Cygnus and Lyra began to peak out over the horizon and announce the approaching return of our Summer Constellations. I am pleased to report that we will be hosting a Summer Session on Thursday, August 8th (with an August 15th rain date) where we will again do a little bit of mechanics and instruction outdoors, followed by Saturn, Venus, and all that our summer view of the Milky Way can provide.

August 8 – Stargazing with CNY Observers & Observing

CNY Observers (CNYO) hosts an introductory lecture to the Night Sky, focusing on planets and other objects observable during August and September.  Part of the lecture will discuss some simple ways to learn the Constellations, while the rest of the lecture will provide details about meteor showers, observing satellites and the ISS, and the ever-expanding description of our own Solar System.  If time and weather permits, some early evening views of Venus and Saturn will be had from the Beaver Lake parking lot.  Free for members; $2 for nonmembers.

CNYO Observing Log: Baltimore Woods, 5 April 2013

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Bob Piekiel’s monthly session at Baltimore Woods featured crystal clear skies, increasingly cold conditions (a recurring theme this year for all of the previous sessions), and one large scope.

This Baltimore Woods session was the last scheduled event before our Winter constellations all-but disappear from our nighttime skies. To this pressing deadline was added the last reasonable observation of Comet panSTARRS (C/2011 L4) from the same location, as the return of the foliage through May will all-but obscure the parts of the North/NorthWest horizon that are not already obscured by naked branches. The event itself was scheduled from 7:30 to 9:30 p.m., ending an hour before any first observation of Saturn for the evening. The ever-dropping temperature that evening found us ending the session promptly to the sound of running (with heat on full-blast) cars and depleted propane.

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Bob Piekiel and the author post-assembly.

With a confirmed heavy lifter attending (me), Bob opted to bring out a 16” Meade SCT on a homemade tripod that is (minus the scope) transported in the open – the whole considerable contraption hitches to the back of the car. After a bit of heavy lifting and careful coordination to get the scope up to the mount, the completed assembly was ready for the first signs of bright stars (in this case, Sirius and Capella) to perform the alignment. The time waiting for bright star arrivals was passed with the help of a pair of Zhumell 25×100’s that saw (1) clear views of Jupiter and all four of its largest moons and (2) Sirius in Canis Major to the West.

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Bob Piekiel putting the finishing touches on a 16″ Meade SCT.

The height of the tripod combined with the extra 8” of wheels on the mount’s base meant that a step ladder was required for nearly all viewing throughout the night. With the 16” SCT aligned, the first official view (pre-dark sky) was of Jupiter, which was bright and clear in Bob’s 40 mm Meade eyepiece. The second object was Trapezium in the Orion Nebula (M42), which was also crisp and clear despite our observing it only minutes after sunset.

The third object observed combined low brightness with near-horizon position just past dusk. Bob managed to find Comet panSTARRS almost due North of the Andromeda Galaxy just as it was about to hit the bare tree line. The view was excellent for several minutes as everyone had a few looks at this increasingly difficult-to-observe object (comet’s center was reasonably well defined, but this was a 16” scope with a 40 mm eyepiece). And, it should be noted, the object database in Bob’s GOTO computer is not only older than the discovery of Comet pan-STARRS, but also quite a bit older (decade? maybe two?) than the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) that originally identified the comet. So, extra kudos to Bob for the timely find!

The cold set in quickly after these first three objects, meaning the last four objects for the evening were approached with haste. In a return to the objects of his last session, Bob treated attendees to excellent dark views of M65 and M66 in Leo, M108 (a faint edge-on galaxy near the Owl Nebula in Ursa Major that was as bright in the 16” as it was with Bob’s 11” scope + image enhancer), and the Owl Nebula (M97). Bob and I saw this final object as a confirmation that it hadn’t flown the coop during our last session, where the image enhancer failed to produce any particular view of this object (see the last session notes for details).

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New supernova in M65. Photo by Felipe Pena.

NOTE: I wish I had known earlier that a new supernova was discovered in M65! As a general point of reference, those looking for the most complete and up-to-date information about supernovas are directed to David Bishop’s excellent Bright Supernova database and log at www.rochesterastronomy.org/supernova.html. Details and many, many images of the new supernova in M65 can be found at: www.rochesterastronomy.org/sn2013/sn2013am.html

The totality of views through the Zhumell 25×100’s were limited to Jupiter (as a sampling for the attendees before the 16″ was properly GOTO’ed), Sirius (just to the left of Orion and the brightest star in our Night Sky), the Double Cluster in Perseus (bright and densely packed), and the Pleiades (M45), the object for which I assume 25×100’s were originally designed to observe (near-perfect fit of the whole cluster in the field of view).

A few street lights and distant clouds to the East reflecting Syracuse back down provided all the illumination that the stars didn’t as we began to pack up the gear at 9:30 p.m.

And did the 3rd Quarter Moon affect the viewing? For those observing at “reasonable” hours, it is the case that the 3rd Quarter Moon doesn’t rise until midnight, meaning the week before a Full Moon, the week of a Full Moon, the few days before a 1st Quarter are excellent for getting outside to observe deep sky objects at “reasonable” hours (reasonable being relative, of course).

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Not a lunar landing scene. Mid-way through the 9:30 pack-up.

Next session is scheduled for May 4 (Saturday) – 5 (Sunday), 8-10 p.m. and will feature Jupiter, Saturn, and hopefully a few shooting stars from the Eta Aquariids meteor shower. For details and registration, see the details on this CNYO page.

CNYO Observing Log: NASA Climate Day, 2 April 2013

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Tuesday April 2nd marked the Museum of Science and Technology‘s hosting of NASA Climate Day in Syracuse, NY. For CNYO members and attendees attempting to observe the Sun, April 2nd also marked one of the more remarkable mixtures of weather patterns to hit CNY.

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Patient attendees waiting for a clearing. Photo by Simon Asbury.

CNYO solar scope setup at Walt the Blue Dragon commenced promptly at 5:00 p.m. Given the expectation of snow and considerable cloud cover over the next few hours before the 7:31 E.D.T. p.m. sunset, I left my Dobsonian at home and Larry Slosberg opted to keep his Meade SCT in the car. Our equipment for the event consisted of a pair of 25×100 and 10×30 binoculars (both with homemade Baader filters) and one Coronado PST. Also in tow were several garbage bags for rapid covering of all the equipment.

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The author looking for a clearing through Baader’d Zhumell 25×100’s. Photo by Simon Asbury.

The sky was windy, cloudy, patchy, and fast-moving, intermixing light snow with perfect blue patches near (but not always overlapping) the Sun. Over the course of about 80 minutes, only 10 good minutes of solar observing were had, and most of these involved some amount of cloud cover obscuring prominent Sunspot 1711 and several smaller Sunspots. The Coronado revealed a large triangular prominence and plenty of surface detail with a 20 mm Plossl and a TeleVue 3mm-6mm Nagler Zoom. It was during the Coronado observing that Bob Piekiel mentioned a certain tweak that can be performed to the PST (and other models) to improve the view (a forthcoming article documenting the procedure is in the works!).

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View of the Sun on April 2nd, 2013. From sohowww.nascom.nasa.gov.

The outside part of the NASA Climate Day festivities ended as a massive grey cloud approached from the distant East (that proved to drop the largest amount of snow on Syracuse not 30 minutes later), instigating the packing up of equipment and migration into the MOST itself to see the rest of the event. In all, only a few left the climate-controlled confines of the MOST to see the filtered Sun, but we did get a few passers by to look, at least one of whom made it onto our facebook page recently.

LESSON FOR THE SESSION: When it’s freezing cold, blustering-ly windy, dark-grey overcast, and only a slight hope for long patches of clear skies exists, keep the solar scopes close to the exterior doors of the building where the main event is going on.

The indoor part of the CNYO session consisted of a small presentation area for showing a few videos of solar events, how the Baader and Hydrogen-alpha filters (in the Coronado) work (having stolen an incandescent light bulb from a bicycle-powered demonstration for the Baader demo), and the relative sizes of the Sun and planets in our Solar System. We moved inside just as Dave Eichorn began his keynote lecture and unfortunately missed his presentation, but that did give us time to walk around the displays near our little setup (appropriate placed next to the vision display).

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The indoor presentation setup.

The demo of the Baader film with the incandescent bulb (to easily see the spring inside) was one of the indoor highlights (well, I thought is was interesting), then we finished the evening with a few students asking some very good questions about solar activity, the dangers of space flight, and potential plans for Moon and Mars Missions (which is always the real highlight of any CNYO session for me).

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