Monthly Archives: November 2013

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CNYO Observers Log: Pulaski Middle School Science Club, 20 November 2013

Greetings fellow astrophiles!

CNYO members Larry Slosberg, Ryan Goodson, and myself hosted our first science club observing session of the year at Pulaski Middle School (my third year doing so, Larry’s second year, and Ryan’s first).

The cold weather kept the crowd to about 25 (early-October sessions having maxed out at around 50 previously) students, teachers, and parent chaperones (no doubt to keep our astronomy humor clean) for an evening that gave us about 1 full hour of good observing and 30 minutes of increasing cloud cover and decreasing body temperatures.

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Larry getting ready. Photo by Ryan Goodson. Click for a larger version.

In a shift from the usual procedure, we held the entire event outdoors. Powerpoint slides were replaced with red flashlights and two of our CNYO brochures (How The Night Sky Moves and Guide For New Observers) to direct a walk-through of the Night Sky while it was clearly visible (with extra thanks to the Pulaski Middle School staff for turning out the football and tennis court flood lights). The first half-hour was also used as a Q+A session. One long-lived, slow-moving meteor coaxed a 10 minute discussion of meteor showers and motion in the Solar System. A few quick beams from our green laser pointers were used as a springboard to discuss both vision (our sensitivity to green and our insensitivity to red, the differences between rods and cones, dark adaptation) and the law (because they are most definitely NOT toys). Ryan also gave a walk-through of an 8″ NMT Dobsonian to explain to everyone present how the photon traffic is directed to the eyepiece and where to place your eye at all three scopes to see the sights.

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Kids watching Larry with an NMT Dob in the foreground. Photo by Ryan Goodson. Click for a larger version.

The following hour was an observing free-for-all, with each of us picking and describing objects in the Night Sky. With the line and discussion as long as it was, I only managed to observe Albireo, the Ring Nebula (M57), the Pleiades, Vega, and Jupiter (it quite close to the end of the event).

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The author dressed for radio. Photo by Ryan Goodson. Click for a larger version.

Despite the cold, everyone was attentive and full of good questions (perhaps the best part of running these events is discovering that the science gears are spinning quickly in the heads of science club members). We finally packed up around 9:30 p.m. after I ran a 15-minute warm-up session indoors to talk a little more astro-shop (spending most of the time on intelligent life in the universe and the reason why we’ve so few impact craters on Earth).

Larry summed up our session best on Facebook:

I would like to take a moment, and thank the kids and adults at Pulaski Middle School for inviting us up last night for another great astronomy night. All the kids were engaged, enthusiastic, and contributed to lots of great discussions. We had a wonderful night of observations, nice clear skies and I can’t wait to do it again. I am truly amazed by the breadth of knowledge of the kids and their eagerness to learn more. Keep it up, kids!!!

CNYO Observers Log: Comet ISON At Highland Forest, 15 November 2013

Greetings fellow astrophiles,

One of the benefits of spending your time in the sciences is the development of a healthy skepticism for science news that makes it out to the major print and online news services. Be it new findings on vitamins or “breakthroughs” in fusion, there’s often an astronomical difference between what appears in initial reports and what actually settles as established fact in the laboratory or marketplace. As one of my favorite radio personalities puts it (about military conflicts, but the logic applies) “The first three reports are always wrong.”

Comet ISON started out early this year with such headlines as “Comet Of The Century?” (and that was NASA), “ISON May Appear Brighter Than Full Moon As It Passes Earth,” (from HuffPo, among many others), and other all-too-optimistic accolades undeserving of an object for which almost nothing was known at the time. But it sounded good in the small news snippets that passed around many astronomy email lists. This last month has finally seen some more serious scientific questions raised in the media concerning its composition, actual brightness, flaring, etc., as real data has made its way to us for analysis. The final result, so far, is far from advertised early on. But coal to the eyes of a non-observer can be gold to to the eyes of an observer, so many an amateur has found time to make it outside to take in at least one view of Comet ISON.

It is with the above in mind that I report on a facebook-announced CNYO observing session for Comet ISON held on Friday, November 15th at the most unreasonable hour of 3:30 a.m. The attendees, including Ryan Goodson, Hanh Le, and myself, braved the bitter cold for a 30 minute drive South to Highland Forest, an all-around excellent location for enjoying the Night Sky (and, I am pleased to report, a future location of regularly-scheduled CNYO events for 2014. Post to follow!).

And why the 15th? There are many factors that govern when an observer will drag their equipment outside.

* The easy one is the weather – cloudy nights, bitter cold, or hot, swampy nights (and their associated mosquito infestations) leave the intrepid amateur to hang out at home and in the discussion forums on cloudynights.com.

* The second one is the presence or absence of the Moon. As our closest natural satellite, the Moon is one of the most enjoyable (and brightest) objects to spend one’s time exploring (and, with a clear window, can be done just as enjoyably indoors). The downside is that the lit Moon washes out the dim details of many a fuzzy nebula, galaxy, or comet. If the Moon is out, many an amateur astronomer isn’t. In the case of the morning of the 15th, the Moon set just before 4 a.m. (at which point something as dim in surface brightness as a comet becomes a much more tempting target).

* The third is the timing of the object itself. While much of what’s observed in the Night Sky lasts for hours at a time every night, certain events occur over relatively narrow windows. The occultation or transit of Jupiter’s moons is one, satellite or ISS fly-bys is another. Comet ISON at its then-current window was yet another one, as it rose quite close to the beginning of sunrise (“the beginning” meaning the start of brightening skies that would wash its detail out) and wasn’t going to appear at any more convenient a time prior to its closest approach to the Sun.

* The fourth is the combination of all three. During the week of the 11th, the skies were predicted to clear only at the end of the week, Comet ISON was set to rise later every morning in the East, and the Moon was set to set later and later in the West. Combined with increased cloud cover on the 16th, the early morning of the 15th became THE WINDOW for Comet ISON.

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The West and constellations from Highland Forest at 4:00 a.m. Click for full size.

The group convoy’ed out to a frosty Highland Forest and set up the scopes just to the East of the main building. As anyone who’s stopped at the building before or after a hike will know, the view from this location is remarkable, with a low tree line and steep-ish hill bracketing views of the Fenner Wind Farm towards the South and just a hint of Syracuse civilization towards the North. The Winter Constellations of Canis Major, Taurus and Orion just beginning to peak out at “reasonable hours” now were in full view to the West at 4:00 a.m. Comet ISON, while approaching uncomfortably low on the horizon for a Dob, was visible as a fuzzy 4th magnitude ball with a slight tail (most definitely an obvious object in Ryan’s New Moon Telescope Dob and my 25×100 Zhumell binos). The wind was just fast and gusty enough to keep us from finding Comet Lovejoy, which was at about 9th magnitude in the same sky (it will be a target for future observing sessions).

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Ryan Goodson sneaking a low peak at Comet ISON. Click for full size.

As of this posting on 30 November, ISON has just barely survived its trip around the Sun (earliest reports saying it had disintegrated, slightly later saying it may have survived as a dark ball, now more recent reports saying something with a tail has survived) but we don’t yet know if it’s going to be observable on its “way out.” Stay tuned to future reports.

TACNY John Edson Sweet Lecture Series – The Historical Heritage Of Technology In Central NY And The Rise Of TACNY

Tuesday, December 10 2013, 5:30 – 7:30 p.m.

Onondaga Community College, 101 Whitney Applied Technology Center



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Ed Bogucz and Howie Hollander will look back at the rich historical heritage of technology in Central New York and the history of the Technology Club of Syracuse, now doing business as the Technology Alliance of Central New York.

Dr. Ed Bogucz leads SyracuseCoE, New York State’s Center of Excellence for innovations in environmental and energy systems. SyracuseCoE is a collaborative enterprise that engages more than 200 firms and institutions to address global challenges in clean energy, healthy buildings, and sustainable communities. Prior to becoming SyracuseCoE’s Executive Director in 2003, Bogucz served more than eight years as dean of Engineering and Computer Science at Syracuse University. Bogucz joined the Syracuse University faculty in 1985 as an assistant professor of mechanical and aerospace engineering. He earned bachelors and doctoral degrees from Lehigh University, and a master’s degree from Imperial College, University of London. He is a member of the Board of Directors of the Near Westside Initiative.

Howie Hollander has been president of TACNY since 2005. Retired from Lockheed Martin since 2011, where he had various engineering and program management roles, he recently rejoined the workforce part-time at SUNY-ESF where he is a program manager in the Outreach department. He earned a BE in electrical engineering from NYU and an MS in engineering management from Northeastern. He is a board member of the Milton J. Rubenstein Museum of Science & Technology and vice president of the Central NY Jazz Arts Foundation, as well as an advisory board member of the LeMoyne College information systems program and the Rensselaer Polytechnic Institute information technology and web sciences program. Howie is a 2001 graduate of Leadership Greater Syracuse.

TACNY John Edson Sweet Lecture Series

Since 1916, the TACNY John Edson Sweet Lecture Series has annually presented a minimum of six lectures, free and open to the public. Former speakers have included Herbert Hoover, R. Buckminster Fuller, and Jacques Cousteau.

Technology Alliance of Central New York

Founded in 1903 as the Technology Club of Syracuse, the nonprofit Technology Alliance of Central New York’s mission is to facilitate community awareness, appreciation, and education of technology; and to collaborate with like-minded organizations across Central New York.

For more information about TACNY, visit www.tacny.org.

Neil deGrasse Tyson co-Keynotes The “NEXT: The Event for Technology, Manufacturing & Innovation” Conference On Tuesday, November 19th

Astrophysics is truly one of the rarities in the physical sciences, as it has managed to branch between hard academia and the general public like no other in our modern technological age (Nova and PBS Specials, The Discovery Channel, and Big Bang Theory alike). The proof is in the cosmic pudding – unlike most any other branch of science, I can tell you that “one of the world’s most famous astrophysicists is coming to give a lecture in Syracuse” and you’re likely asking yourself “Neil DeGrass Tyson? Brian Cox? Stephen Hawking?” Try putting a name list together in any other field!

It is with that analysis in mind that I’m forwarding here an announcement from the TACNY email listserve about the “NEXT: The Event for Technology, Manufacturing & Innovation” conference happening this coming Tuesday, November 19th at the Holiday Inn Syracuse-Liverpool. The event, sponsored by the Central New York Technology Development Organization (TDO) and the CASE Center on the Syracuse University campus, features two keynote speakers. The first, “Making it in America – Shifting Economics Create New Opportunities,” is by Harry Moser of The Reshoring Initiative. The second, perhaps more relevant to readers of the blog, is none other than Hayden Planetarium directory and all-around exponent of science Neil deGrasse Tyson.

The Event for Technology, Manufacturing & Innovation

Come. Be Inspired. Leave Smarter.

next-central-new-york-logoIn its second year, NEXT is a technology, manufacturing and innovation conference where fast-track companies meet and learn from top-notch business leaders and industry experts. The dynamic full-day program boasts two world class keynotes in Neil deGrasse Tyson and Harry Moser; and delivers educational workshops in concurrent tracks (Innovation & Commercialization, Manufacturing Excellence, Technology Trends and Entrepreneurship)

“Making it in America – Shifting Economics Create New Opportunities” – The morning keynote, Harry Moser, President/Founder of the Reshoring Initiative, will discuss the broad resurgence of American manufacturing. Delivering insights into the trend, what types of products are leading the charge, and what the new American manufacturing industry might look like.

“Reaching for the Stars” – The luncheon keynote speaker, Neil deGrasse Tyson, is an internationally renowned astrophysicist, science policy advisor, media personality and Frederick P. Rose Director of the Hayden Planetarium. He will explore the state of science literacy in America today and the critical importance of continued government and industry investment in fundamental scientific research for the long-term economic health of the country.

You can register for the event at next-syr.eventbrite.com/. While the registration fee is not insignificant, this is an all-day conference highlighting a multitude of technology and manufacturing industries and projects happening in CNY (I refer you to the event program HERE). That said, I already know of one or two people who registered just for NdGT’s keynote (abstract below):

So many of the technologies and products we take for granted, from freeze drying to scratch-resistant lenses to solar cells, are a direct result of research done during the “space race” in the ’50s thru ’70s. No one knows where the next breakthrough discovery will come from! Join astrophysicist Neil deGrasse Tyson as he explores the state of science literacy in America today and the critical importance of continued government and industry investment in fundamental scientific research for the long-term economic health of the country. What is the short- and long-term future of the aerospace industry, and how will that future impact the broader economy, and our day to day lives? Only by reaching for the stars, continuing to explore every aspect of the world and the universe, can we build a solid foundation for the next generation’s industry and economy.

NeilTysonOriginsA-FullSizeSpeaker Bio: Neil deGrasse Tyson, the Frederick P. Rose Director of the Hayden Planetarium, is an internationally renowned astrophysicist, science policy advisor, and media personality. A thought-leader in science and technology, Dr. Tyson has served on Presidential commissions on the future of the US Aerospace Industry and continues to serve on NASA’s Advisory Council. He has received eighteen honorary doctorates and the NASA Distinguished Public Service Medal, the highest award given by NASA to a non-government citizen. He has written countless professional papers as well as ten books, including New York Times bestseller Death By Black Hole and Other Cosmic Quandaries, The Pluto Files: The Rise and Fall of America’s Favorite Planet, and The Sky is Not the Limit: Adventures of an Urban Astrophysicist. Among his many television and media appearances, he hosted PBS-NOVA’s mini-series Origins, the NSF-funded pilot radio program StarTalk, and is currently working on a 21st century reboot of Carl Sagan’s landmark television series COSMOS, to air in 2014. Tyson was voted Sexiest Astrophysicist Alive by People Magazine in 2000.

NASA Space Place – The Most Volcanically Active Place Is Out-Of-This-World!

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. NASA Space Place has been providing general audience articles for quite some time that are freely available for download and republishing. Your tax dollars help promote science! The following article was provided for reprinting in November, 2013.

By Dr. Ethan Siegel

2013february2_spaceplaceVolcanoes are some of the most powerful and destructive natural phenomena, yet they’re a vital part of shaping the planetary landscape of worlds small and large. Here on Earth, the largest of the rocky bodies in our Solar System, there’s a tremendous source of heat coming from our planet’s interior, from a mix of gravitational contraction and heavy, radioactive elements decaying. Our planet consistently outputs a tremendous amount of energy from this process, nearly three times the global power production from all sources of fuel. Because the surface-area-to-mass ratio of our planet (like all large rocky worlds) is small, that energy has a hard time escaping, building-up and releasing sporadically in catastrophic events: volcanoes and earthquakes!

Yet volcanoes occur on worlds that you might never expect, like the tiny moon Io, orbiting Jupiter. With just 1.5% the mass of Earth despite being more than one quarter of the Earth’s diameter, Io seems like an unlikely candidate for volcanoes, as 4.5 billion years is more than enough time for it to have cooled and become stable. Yet Io is anything but stable, as an abundance of volcanic eruptions were predicted before we ever got a chance to view it up close. When the Voyager 1 spacecraft visited, it found no impact craters on Io, but instead hundreds of volcanic calderas, including actual eruptions with plumes 300 kilometers high! Subsequently, Voyager 2, Galileo, and a myriad of telescope observations found that these eruptions change rapidly on Io’s surface.

Where does the energy for all this come from? From the combined tidal forces exerted by Jupiter and the outer Jovian moons. On Earth, the gravity from the Sun and Moon causes the ocean tides to raise-and-lower by one-to-two meters, on average, far too small to cause any heating. Io has no oceans, yet the tidal forces acting on it cause the world itself to stretch and bend by an astonishing 100 meters at a time! This causes not only cracking and fissures, but also heats up the interior of the planet, the same way that rapidly bending a piece of metal back-and-forth causes it to heat up internally. When a path to the surface opens up, that internal heat escapes through quiescent lava flows and catastrophic volcanic eruptions! The hottest spots on Io’s surface reach 1,200 °C (2,000 °F); compared to the average surface temperature of 110 Kelvin (-163 °C / -261 °F), Io is home to the most extreme temperature differences from location-to-location outside of the Sun.

Just by orbiting where it does, Io gets distorted, heats up, and erupts, making it the most volcanically active world in the entire Solar System! Other moons around gas giants have spectacular eruptions, too (like Enceladus around Saturn), but no world has its surface shaped by volcanic activity quite like Jupiter’s innermost moon, Io!

Learn more about Galileo’s mission to Jupiter: solarsystem.nasa.gov/galileo/.

Kids can explore the many volcanoes of our solar system using the Space Place’s Space Volcano Explorer: spaceplace.nasa.gov/volcanoes/.

This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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Caption: Io. Image credit: NASA / JPL-Caltech, via the Galileo spacecraft.

About NASA Space Place

The goal of the NASA Space Place is “to inform, inspire, and involve children in the excitement of science, technology, and space exploration.” More information is available at their website: http://spaceplace.nasa.gov/