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DATE AND PLACE
Saturday, November 3rd
CSU Northridge
Meeting Room: Donald Bianchi Planetarium
Local Hosts: Norm Herr, Say-Peng Lim
CALL FOR PAPERS
Contribute a 15 minute talk or a brief demo for the Show'n Tell segment using the online submission form or communicate directly with the program chair, Peanut McCoy. The deadline for contributions has passed.
LUNCH INFO
Please RSVP for catered Thai food lunch (cost is $8) via this online form. Reservations are due by October 27.
The buffet will include a variety of noodle and rice dishes with meat and vegetable choices. Please let us know if you want to request tofu instead of meat. If you do not chose the Thai lunch, know that there are other dining options on campus.
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MAPS AND DIRECTIONS
Driving Directions from CSUN website
Annotated campus map
PARKING
On campus in G3 parking structure is in G3, cost $6. (Off Campus Free.)
THANK YOU EXHIBITORS AND RAFFLE SPONSORS!
Cenco/ Sergent-Welch
Please take some time to check out the commercial workshops and exhibits at the meeting and especially to thank the representatives for their support of our organization.
THE WORLD FAMOUS "ORDER OF MAGNITUDE CONTEST"!!!
Question: What fraction of the local atmosphere passes through an internal combustion engine on a typical week day? (Contributed by Myron Mann)
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8:15 |
Registration and
refreshments |
9:00 |
Welcome and announcements |
9:15 |
Matthew D’Alessio, Loraine Lundquist (CSUN) – Water-Powered Rockets with collaborative, computer-supported
approach.
Each year, our physical
science class for pre-service elementary teachers launches water-powered
rockets based on the activity from NASA. We adopted this classic activity to
use a collaborative, computer-supported approach using simple and easily-available functions in Google Spreadsheets to pool
observations, provide instant feedback, and publicly display results from all
teams side-by-side in real-time. These instant comparisons promote student
accountability and engagement, inspiring them to think more carefully about
why answers may be different and notice sloppy data or unlikely outcomes --
in short, to facilitate and motivate expert thinking about data. |
9:30 |
Norm Herr & Brian Foley (CSUN) The use of collaborative web-based documents to create scientific research communities in physics classrooms.
New collaborative web-based document technology provides students and teachers the opportunity to readily collect and analyze large sets of data from multiple lab groups and class sections. Such resources may be used to create an environment that more closely resembles the collaborative environment of a professional scientific community in which researchers develop hypothesis and explanations in light of their own findings and those of their colleagues. |
9:45 |
Invited talk: Damian Christian (CSUN)- Our Star, the Sun, and the Discovery of Earths Outside our Solar
System
We live in an exciting
time in which Astronomers are discovering over 100 new planets orbiting
nearby stars (exoplanets) each year. NASA's Kepler mission is finding Earth-sized planets. I will review several of the search
methods for exoplanets and present recent results.
There are education materials available from several exoplanet surveys and the Kepler mission
(http://kepler.nasa.gov/education/). The understanding and characterization
of new planets also requires us to have better measurements of many of their
host star's properties. Understanding the activity of nearby stars leads us
back to our own star, the Sun. CSUN has studied solar activity for almost 40
year and I will review these results and new results from NASA's Solar Dynamics
Observatory (http://sdo.gsfc.nasa.gov/). |
10:45 |
Invited talk: John Louis Callas (JPL)- Curiosity and the robotic exploration of Mars
For many years now,
robotic explorers have been conducting field geology day after day on Mars at
different locations on the surface. These rovers have traversed great plains, climbed mountains, descended into deep
craters and survived rover-killing dust storms and frigid winters. As the rovers move, each day becomes a
brand new mission with new sights and new geology to explore, making
significant discoveries in understanding the Red Planet and finding evidence
of past habitable environments that could possibly have supported life. The
surface robotic enterprise has just been joined by another, larger, more
capable rover, the Mars Science Laboratory, Curiosity. In addition to
extending the geologic exploration at a third location on Mars, Gale Crater,
Curiosity begins the next phase of exploration with the ability to search for
the chemical building blocks of life, organic molecules, moving closer to
answering the questions, was there life on Mars, is there life on Mars? |
11:45 |
Business meeting |
12:00 |
Lunch – Thai Food
Buffet (RSVP $8), on campus options also available |
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1:00 |
Show and Tell |
1:15 |
Invited talk: Robert Cousins (UCLA)- Observation of a new particle at CERN -- the long-sought
Higgs boson?
The Higgs Boson was
postulated nearly five decades ago as a crucial element of the modern theory
of the forces of nature, and has been the subject of worldwide searches ever
since. On July 4, two huge collaborations, working at the Large Hadron
Collider outside Geneva, announced independent observations of a Higgs-like
boson. I will describe the motivation, the experiments, the data, and the
interpretation. |
2:15 |
Planetarium Show: Jan Dobias (CSUN) |
2:45 |
Bill Layton (UCLA)-Transformer basics, wall warts and
vampires
In an effort to develop an
inexpensive demonstration of reflected transformer impedance, a convincing
demonstration evolved to show why the utility companies are worried about the
constant power drain from plug in wall transformers, even when the device
connected is off or disconnected. |
3:00 |
Sissi Li (CSU Fullerton)- Techniques for Developing the Undergraduates’ Identity in the Physics
Community
Physics teachers teach
more than physics content. Implicitly and explicitly, teachers model what
doing physics means and how to be a member of physics communities. We show
that real world connection is important by asking students to make sense of
real physical situations. From the student side, they learn what is expected
of them in the discipline and the extent to which they can influence the community.
By being a part of a physics classroom community, teachers and students
contribute to the students’ physics learner identity development. This talk
will highlight research findings about some of the ways of contributing. |
3:15 |
James Lincoln (Tarbut V’ Torah HS) - Techniques
for Successful Student Films
Engaging students through
the production of student films has become an instructional method that has
gained in popularity in recent years. For this reason, it would be beneficial
for someone with expertise in this area to provide guidance and instruction
on how to arrange a unit around this instructional model. In this talk I outline a unit I taught
on making short science films. Included are resources and tips for instruction on how to structure,
develop and produce successful student films. |
3:30 |
Nancy McIntyre (Robotics Education and Competition Foundation) – Grants Available for Robotics Programs
I have a number of grants
available to help begin VEX Robotics teams in Arizona, New Mexico and
California schools. The value of each
of the grants is $1,200.00. Including team
program registration for the season and a kit that will give a rookie team
enough materials to build a competitive robot that will be able to compete in
your state. Robots have been a positive vehicle to focus students on the importance
of STEM education. |
3:45 |
Pari Spolter (Orb
Publishing)-Kepler’s second law and conservation of angular
momentum
Kepler’s second law is calculated for 18 planets and
asteroids. It is shown that equal areas are swept in equal intervals of time
only near the perihelion (P) and the aphelion (A). A highly significant
relation between the ratio of the area swept at the average of P and A to the
area swept at semimajor (S) in the same interval of
time and the eccentricity is presented. The equation is ratio = ab+c with a = −0.617, b = 2, and c = 1.00. The
correlation coefficient is 0.9975. The ratio is equal to , which is equal to sin θ, where θ is the smaller angle between the
two vectors v and r. Angular momentum is a vector perpendicular to the plane
formed by v and r and is conserved, indicating that there is no torque in the
direction vertical to the plane of the orbits. |
4:00 |
Order of Magnitude contest
and door prizes |
4:15 |
Adjournment |
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