Monthly Archives: June 2013

You are browsing the site archives by month.

CNYO Observing Log: Camp Comstock, Ithaca, 1 June 2013

2013june18_campcomstockbanner_v2

One of the great joys of public observing sessions is introducing non-observers to the immensity of our local sliver of the universe. Hubble imagery and the amazing ground-based astrophotography of the last 25-or-so years is all well and good, but to explain to a new observer that the photons from the Whirlpool Galaxy (M51) currently hitting their retina have been on a 23 million year voyage, or to put all of the Andromeda Galaxy (M31) into the field of view and explain that the photons on one side of the eyepiece have been traveling 150,000 years longer than the photons on the “other” side of the eyepiece, or to aim a Coronado PST at the Sun and point out that the sunspots on the surface are 3 or more Earths across – these are the images that really put the universe, and our place in it, into perspective.

One of the great joys of lecturing on introductory astronomy is being able to describe all of these visuals in greater detail, showing how observation and the rest of the Scientific Method have produced great order in our Nighttime Sky (for, at least, the parts of the sky we can see in the backyard on a clear, dark night). As is true for many of the other physical sciences, a book chapter or wikipedia page alone can be far less informative, and is definitely far less engaging, than a chance to have a conversation with someone who knows the topic well enough to relate complicated concepts by drawing from many additional resources.

And, at a time when we continually fret the state of STEM education in the US, there is nothing better for an academically-inclined scientist (me) than to have someone many years their (my) junior process the information on a slide and ask a question that (1) clearly shows a grasp of the physics involved and (2) they (I) don’t have a good answer to. Lecturing keeps the lecturer just as sharp!

It is with those points in mind that CNYO hosted a Girl Scout lecture on Saturday, June 1 at Camp Comstock in Ithaca, NY as part of their requirements for earning their Night Sky badge. Unfortunately, the mostly cloudy and otherwise unpredictable night before made the Nighttime Sky observing component impossible, compacting the badge requirement section into a combined lecture/solar observing session that went well over allotted time with no (voiced) complaints.

Instead of highlighting lecture points, my goal here is to provide a few pointers for perspective astro-lecturers of kids and young adults (although I suspect the same applies for all generations).

1. Plenty Of Lead Time For Setup

In my case, my leisurely 1 hour drive turned into a compressed 40 minute drive as I waited for a police officer to take my eyewitness statements after a fender-bender on Route 13. Lesson #1 – Don’t text while driving!

2. Short Sections

Based on the Night Sky badge requirements, I had a very good template by which to design seven short lectures that would fit nicely into a 60 minute presentation (that, with questions, then went on for two hours). A full hour on a single topic to a general audience can be way too much for even a focused audience. Make this an audience of young adults and add an un-air conditioned, 85 oF room to the mix just after lunch, and you’ve got a recipe for a very… red-shifted lecture. A very good approach for you and the audience is to pick several topics and try to make a complete mini-lecture out of each. This makes your preparation time more productive (because you can divide-and-conquer as well) and it allows you to give the audience a minute between mini-lectures to digest and freshen up for the next one. In the Night Sky badge case, my seven sections were:

A. The Local Neighborhood

– A “powers of 10” walkabout from Earth out to the Sloan Digital Sky Survey

B. Circumpolar Constellations

– Explaining how the Earth moves (rotation vs. revolution) and why the North Star doesn’t appear to. This part of the lecture was complemented by the CNYO How The Night Sky Moves brochure.

C. Constellations (What & Why) And Stars

– An overview of Western constellations and the stars that define them, including a little discussion of stellar variety (color, age, size)

D. Why Learn The Constellations?

– Stress the historical meaning of the Constellations, then their use for direction (Follow The Drinkin’ Gourd) and use for marking deep sky objects (specifically, the Messiers)

E. Don’t Panic!

– How to learn the constellations, including the circumpolar-first approach, seasonal heavy-hitters, and the Zodiac

F. Solar System Formation

– Two videos I always keep handy in the back of a presentation are “Birth Of Our Solar System” (a nice animation of the formation of the whole Solar System)…

… and “How The Moon Was Born” (a video that shows the history of the Earth-Moon system and the ever-impressive Theia impact).

G. Light and Air Pollution

– Light pollution is bad, but it does help new astronomers find the bright starts in constellations. Air pollution also helps, but at a much higher cost. We should be avoiding both!

3. Ask Lots Of Questions

The biggest lesson I learned from watching professionals present to kids is to ask those kids lots of questions and let them be A driver in the presentation (but not THE driver, as you may never get the wheel back). It keeps the audience engaged, it lets others try to explain a concept in a way that the other-others may benefit from, it breaks up the monotony of the single-presenter approach, and it gives kids a chance to “show off” their scientific knowledge (which some of them love to do).

The best kinds of questions are (1) the very easy ones (how many planets) and (2) the ones that no one there (likely) has the answer to but that all can think about and take a swing at (alien life, what happens at a black hole, how big is the Sun, etc.).

If you’re lecturing to a group of 10 year olds, find a friend with a 10-year-old and see what they (don’t) know. If the kid isn’t astronomically-inclined, assume that their knowledge is similar to that of other 10 year olds in a Regents-guided state. The Girl Scout lecture was to a room of 13 to 17 year olds, and I am pleased to report that I had to move on to the “heavy questions” quite early in the lecture.

4. Preparing For The Power-Less Lecture

The Girl Scout lecture could have been done outdoors with demos or indoors with slides. Being a very visual science, astronomy lends itself better to slides unless you’ve several really good demos planned out beforehand (or brochures to help guide the discussion). There are several demos one can use to help get away from the slide-driven lecture and I hope to eventually get to the point of not needing any power. Simple demos (that will be expanded on in future articles) include:

A. Flashlights to demonstrate optical vs. true binaries (differently-colored flashlights are great for multi-star systems)

B. A tape measure and rubber balls to demonstrate the distances within the Solar System (if you’ve a 15 meter tape measure, you can place the planets at: 14.8 cm (Mercury), 27.3 cm (Venus), 38.0 cm (Earth), 57.0 cm (Mars), 197.7 cm (Jupiter), 360.8 cm (Saturn), 729.1 cm (Uranus), 1143.0 cm (Neptune), and 1500 cm (Pluto)

C. An armillary sphere (or big labeled ball) to demonstrate Earth’s axial tilt and its motion around the Sun (with a laser pointer serving as “Polaris,” a walk around an audience member serving as the Sun works perfectly well to help explain the circumpolar constellations

5. Anticipating The Unexpected Question(s)

When I think about the Sun, the first two questions that come to mind are not (1) Isn’t there a disease where you can’t be in the Sun because your skin breaks apart? and (2) I heard that some people try to live on only sunlight with no food. Isn’t that crazy (answer: yes)?

6. The Daytime Is The Right Time

As CNYO’s Larry Slosberg has determined for his observing sessions, the afternoon sky is a perfectly good substitute for the nighttime sky provided you (1) have a solar filter and (2) plan around the first quarter Moon. In the case of (1), the Sun is an excellent observing target for new observers because they very likely have never looked at it through filters and, as you can stress in your discussion, it is the reason why we’re here.

sunspots_1024_20130601

The Sun on 1 June, 2013. From SOHO/NASA.

As for (2), it is also a reason why we’re here, but the magnified Moon, either against a black or blue afternoon backdrop, never fails to impress. To help lead discussion at subsequent daytime observing sessions, the solar-centric Girl Scout session instigated the CNYO solar observing brochure available for download at: A Guide For Solar Observing.

And A Closing Thought…

2013june18_girlscout_badge

CNYO Brochure – A Guide For Solar Observing

Greetings fellow astrophiles!

In preparation for upcoming 2013 lecture and observing sessions, we have put together instructional brochures to help introduce the Night Sky to attendees. The third of these, entitled “A Guide For Solar Observing,” addresses our solar observing sessions and is provided below in PDF format. This brochure will be available at our combined lecture/observing sessions, but feel free to bring your own paper copy (or the PDF on a tablet – but have red acetate ready!).

Download: A Guide For Solar Observing (v6)

NOTE: These brochures are made better by your input. If you find a problem, have a question, or have a suggestion (bearing in mind these are being kept to one two-sided piece of paper), please contact CNYO at info@cnyo.org.

NOTE 2: We’d like to thank the great solar photographer Alfred Tan for the use of his solar image in this brochure. For a regular feed of his stellar (pun intended) solar views from Singapore, we encourage you to subscribe to his twitter feed at: twitter.com/yltansg.

2013may1_htnsm_pg1

2013may1_htnsm_pg1

A Guide For Solar Observing

Solar Safety: Read Me First!

“NEVER Look At The Sun Through ANY Eyepiece Without Protection!”

Pre-Observing Observing Tips

“The Sun is a blindingly bright object all by itself – and your observing session has you constantly looking in its direction!”

Sun Cross Section – 697,000 km Radius

“Radiative Zone: 348,000 km thick, energy from the core is passed through as photons (light) – thousands of years for light to pass through it from the core!”

The Solar System To Scale

“The solar diameter in “planets” is listed.”

More Information About The Sun

“The Sun is the reason why we’re here!”

And Just Why Is The Sky Blue?

“At sunrise and sunset, most of the blue light has been scattered by air molecules, so more of the Sun’s longer wavelength light (red and orange) makes it to our eyes (“R”).”

What You’ll Observe On The Sun

“The savvy (or lucky) observer may see a plane (1), a satellite, a planet (“transit” of Venus (2) or Mercury), or the International Space Station (3).”

About The Sun (History & Future)

“The Sun is a spectral type G2V star in the Orion Arm (Orion Spur) of the Milky Way, some 25,000 light years from the Milky Way’s center and, on average, 8 light minutes away from Earth.”

What You’ll See Through Solar Filters

“All other filters work by picking out a single wavelength (shade of one color) from the entire visible spectrum (ROYGBIV – red, orange, etc.), allowing only that color to pass through to your eye.”

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!


View Larger Map

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).

2013june11_Green_Lakes_Astronomy_Flyer

NASA Space Place – High-Energy Spy

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 June, 2013.

By Dr. Martin C. Weisskopf

2013february2_spaceplaceThe idea for the Chandra X-Ray Observatory was born only one year after Riccardo Giacconi discovered the first celestial X-ray source other than the Sun. In 1962, he used a sounding rocket to place the experiment above the atmosphere for a few minutes. The sounding rocket was necessary because the atmosphere blocks X-rays. If you want to look at X-ray emissions from objects like stars, galaxies, and clusters of galaxies, your instrument must get above the atmosphere.

Giacconi’s idea was to launch a large diameter (about 1 meter) telescope to bring X-rays to a focus. He wanted to investigate the hazy glow of X-rays that could be seen from all directions throughout the sounding rocket flight. He wanted to find out whether this glow was, in fact, made up of many point-like objects. That is, was the glow actually from millions of X-ray sources in the Universe. Except for the brightest sources from nearby neighbors, the rocket instrument could not distinguish objects within the glow.

Giacconi’s vision and the promise and importance of X-ray astronomy was borne out by many sounding rocket flights and, later satellite experiments, all of which provided years-, as opposed to minutes-, worth of data.

By 1980, we knew that X-ray sources exist within all classes of astronomical objects. In many cases, this discovery was completely unexpected. For example, that first source turned out to be a very small star in a binary system with a more normal star. The vast amount of energy needed to produce the X-rays was provided by gravity, which, because of the small star’s mass (about equal to the Sun’s) and compactness (about 10 km in diameter) would accelerate particles transferred from the normal star to X-ray emitting energies. In 1962, who knew such compact stars (in this case a neutron star) even existed, much less this energy transfer mechanism?

X-ray astronomy grew in importance to the fields of astronomy and astrophysics. The National Academy of Sciences, as part of its “Decadal Survey” released in 1981, recommended as its number one priority for large missions an X-ray observatory along the lines that Giacconi outlined in 1963. This observatory was eventually realized as the Chandra X-Ray Observatory, which launched in 1999.

The Chandra Project is built around a high-resolution X-ray telescope capable of sharply focusing X-rays onto two different X-ray-sensitive cameras. The focusing ability is of the caliber such that one could resolve an X-ray emitting dime at a distance of about 5 kilometers!

The building of this major scientific observatory has many stories.

2013june11_DEML50

Caption: Composite image of DEM L50, a so-called superbubble found in the Large Magellanic Cloud. X-ray data from Chandra is pink, while optical data is red, green, and blue. Superbubbles are created by winds from massive stars and the shock waves produced when the stars explode as supernovas.

Learn more about Chandra at www.science.nasa.gov/missions/chandra. Take kids on a “Trip to the Land of the Magic Windows” and see the universe in X-rays and other invisible wavelengths of light at spaceplace.nasa.gov/magic-windows.

Dr. Weisskopf is project scientist for NASA’s Chandra X-ray Observatory. This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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

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/

TACNY Junior Cafe Scientifique: “Back to the Future: From Waste to Power”

Saturday – June 15, 9:30-11:00am

Milton J Rubenstein Museum of Science & Technology – Syracuse, NY



View Larger Map

Have you ever seen science fiction movies like Back to the Future where garbage is put into the gas tank instead of gasoline to make the car go? Maybe you thought to yourself that this will never happen. Well, we are getting closer to a day when we utilize waste materials to power our homes and vehicles, helping to alleviate our dependence on fossil fuels. This presentation will show how, locally, these types of projects are being developed, including a demonstration where waste wood is utilized to create power and steam.

Presenters

Chris Campbell, a native resident of Central New York, has been leading the development of innovative projects within O’Brien & Gere for more than 8 years, with 26 years total professional experience. In his 8-year tenure at O’Brien & Gere, Chris has worked on the development of several alternative energy technologies, including biomass to energy, aimed at providing growth and sustainability within the Central New York area. Chris has a BS in Mechanical Engineering from SUNY Institute of Technology and a MS in Engineering Management from Syracuse University.

Sara Martin, P.E., also a native resident of Central New York, has been leading the development of various alternative energy projects within O’Brien & Gere. More specifically, her focus has been in waste to energy projects, including the design and construction of three facilities in New York State, which utilized food waste to create power and heat energy to utilize back into the food production. Sara has a BS in Environmental Engineering from Clarkson University.

People interested in learning more about sustainable energy are invited to attend the free Junior Cafe presentation on Saturday, June 15, from 9:30 a.m. to 11 a.m. at the Milton J. Rubenstein Museum of Science and Technology (MOST) in Syracuse’s Armory Square. Walk-ins are welcome, but we ask that people RSVP by emailing jrcafe@tacny.org by June 12, 2013.

TACNY Junior Cafe Scientifique

TACNY Junior Cafe Scientifique, a program for middle-school students founded in 2005, features discussions about topics in the fields of science, technology, engineering and mathematics in an informal atmosphere and seeks to encourage students to consider careers in these areas. Students must be accompanied by an adult and can explore the MOST at no cost after the event.

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.