The gathered crowd at Green Lakes.
July 26th saw the yearly return of Bob Piekiel, his 11″ Meade SCT, and 25x125mm Vixen Binoculars to Green Lakes State Park for his yearly “Star Search” observing session (original post HERE). Also in attendance were Ryan Goodson (representing CNYO and New Moon Telescopes with his fantastic 16″ Dobsonian) and myself (with “Ruby,” my equally fantastic 12.5″ NMT Dobsonian). I’ve been to Green Lakes many, many times over the last few decades, but I’ve never “seen” the place after sunset. I am pleased to report that CNY has an excellent piece of flat, maintained ground, low horizon, and reasonably dark sky just 20 minutes from downtown Syracuse – a place that I hope sees much more observing activity in the future.
Local flora and fauna in the parking lot.
Ryan and I arrived around 8:00 p.m. to the sight of 40-or-so kids and adults huddled around a well-spaced campfire that doubled as a s’mores factory. Also in attendance were two caffeinated dogs and a few deer in the parking lot. The location of the session was just near the camping ground, with the parking lot and flat grounds centered in the google map below (a “right” and a “left,” a little meandering, and you’re there).
View Larger Map
The session started just after sunset with the identification of Venus in the Western sky as it began to settle behind trees. This served as an opportunity for everyone to see how the scopes work (and have them demonstrated so everyone knew where the eyepiece was later), to see the appearance of phase in this inferior planet (not to belittle Venus or Mercury – “inferior” refers to them being closer to the Sun than Earth. All other planets are “superior” to Earth in this respect, and we are one of Mars‘ inferior planets), and to see just what a thick, damp atmosphere does to bright pinpoints of light. In this case, the atmosphere acts like a prism, splitting the light from Venus slightly into subtle reds and blues on opposite sides the planet. Not a pretty view for an astronomer looking for sharp detail, but an excellent lesson in optics nonetheless.
Bob (right) on Venus, Ryan (middle) discussing advanced optics design.
With the dogs corralled into nearby cars and Bob unable to shout louder than mezzo-piano for the session, I gave a brief introductory greeting around 9:00 p.m. that stressed the few important points we wish everyone going into a public observing session would know beforehand (but are happy to explain prior to observing through the scopes). These same points appear on one of the fold-out plaques we bring to each session:
1. If You Don’t See Something, Say Something!
During Mars’ 2003 closest-approach at Darling Hill Observatory, people waited in line for nearly an hour to catch a glimpse of Mars they wouldn’t have from Earth’s surface for quite some time to come. One woman looked quickly, then came down a bit put off by the poor sight she had waited so long to see. I snuck back up the ladder to find Mars nowhere in sight – the scope had moved off of Mars by some unseen event (it was dark after all). We put Mars back in, found the woman walking out of the observatory room, and escorted her right back up the ladder to a sight that was definitely worth the wait. Sidewalk astronomers are there for YOU, so ask questions, ask for clarification, make comments about the view, whatever it takes to make sure you don’t inadvertently miss a great sight.
2. Bright Lights = Bad Lights
Smart phones are the new bane of amateur astronomers, having taken over the role white-light flashlights once held. The first thing we tell people (and the first thing we re-tell late arrivals) is that the dark adaption of your vision is a sensitive and time-consuming thing. 15 to 20 minutes are required for your eyes to adjust to the dark enough to see more detail in the Night Sky (and any detail on the ground). One camera flash, one answered phone, one slip of the flashlight can set a whole group’s dark adaption back to square one. Whether by intention or accident, it is a disservice to other observers to set their observing back, so we always ask that people take extra care to spare attendees from bright lights. If your flashlight has a red mode, use it(!), as our vision is largely insensitive to red light (meaning no real dark re-adaption is necessary).
3. Dobsonians Move In A Stiff Breeze
One thing I’ve noticed among some young (younger than 10, that is) observers is a tendency to want to bring the view to them – which they do by dragging the eyepiece to their eye instead of walking up to see what the scope is focused on. We love the enthusiasm, but we don’t know what they’re seeing after they’re done moving! Because Dobsonians are designed to move very smoothly in all directions, we tell people that the best way to observe is to:
“Put your hands behind your back and walk up to the eyepiece.”
I see kids and adults do this after I mention it – and it works great.
4. Don’t Be Afraid Of The Eyepiece!
A final tendency I see among some new observers (especially with glasses) is to find a comfortable spot 2 or 3 inches from the eyepiece. And some young kids have it even worse as their parents try to hold their kid’s head near the eyepiece. No good! When I see someone doing either, I take over the observing, hand them my red flashlight, and show them just how to get that excellent view. Everyone’s done something new that they clearly didn’t know the procedure for. A bit of demonstration goes a long way (especially when you see the same person back in line for a new object and they walk up to the eyepiece – hands behind their back – like a pro).
An Education-First Session
The session itself ran quite smoothly for several hours, with Bob, Ryan, and I mostly sticking to easy-to-see objects. Another important aspect of a sidewalk astronomy or public viewing session is not to tax the new observer’s imagination by asking them to focus on dim, faint objects that might be totally invisible to someone who doesn’t know how averted vision works. Like an opening band trying to get their best material out in 30 minutes before the headliner, a session for new observers should emphasize big, bright objects where what you describe to them is obvious after a few seconds’ time. If you want to introduce new observers to a taste of everything, I recommend finding the best of each of the objects below to have at-the-ready and ready to describe (I include my choices with each for the Green Lakes session):
* (Hopefully) One Planet – Venus and Saturn
* One Star – Vega in Lyra
* One Binary – Albireo in Cygnus
* One Open Cluster – The Double Cluster (Caldwell 14) in Perseus
* One Globular Cluster – M13 in Hercules
* One Nebula – M57, The Ring Nebula in a href=”https://en.wikipedia.org/wiki/Lyra”>Lyra
* One Galaxy – M31, The Andromeda Galaxy in Andromeda (but I started with M51, the Whirlpool Galaxy in Canes Venatici just off the bowl of the Big Dipper, to stall until Andromeda cleared the horizon)
A 15-second exposure of the Big Dipper from the grounds.
I was fortunate to have as my last set of public observers two near-teenagers who were attentive enough to my description of Andromeda and the mechanics of Dobsonian motion that I let them take Ruby’s reigns to find M110, a satellite galaxy just outside of the field of view of M31 and M32 in my scope. After both Bob and the crowd took off for the evening, Ryan and I spent another 30 minutes or so observing (pulling out the Veil Nebula in Cygnus – and still near Fayetteville’s lights!), where we decided that Green Lakes is an excellent, reasonably dark sky location in Syracuse’s direct suburbs – a location we would very much like to make a more regular CNYO observing hotspot.
Now a little math – Mercury revolves around the Sun once every 87.9 days – what we call its sidereal period. Because the Earth revolves as well, the time it takes for Mercury to hit the same basic spot between us and the Sun is 115.9 days (its synodic period). If all of the planets of the Solar System were in a perfect flat plane, that would mean we’d get a Mercury Transit every 116-ish days and the phenomenon would be a little less impressive. Because all of the planets are at slight tilts with respect to Earth’s orbit, we don’t always get clean passes – the Sun is huge overall, but still a small target at an Astronomical Unit, so the slight angles of Mercury and Venus matter when it comes to the proper lining-up needed for transits to occur.
The Thursday session at Beaver Lake will be our last chance to see any sign of the 
