Science for Everyone: Powers of 10

Monday, October 14, 2013

Powers of 10

http://www.powersof10.com/film

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Constellations

For the last two weeks, we have been studying HOW BIG the universe is, and HOW it was made. Today, you will be creating a personal 2-sided model on your understanding. A model can be a picture or a concept map with explanation, or a series of statements or a story that are somehow connected. At any rate, your model is UNLIKE anyone else's, because you are a UNIQUE person. TO start this activity, I would suggest you look around at the links, writing yourself notes and sketching ideas for at least 30 minutes.

SIDE 1: Tell me about our star, our solar system, our local galaxy, and the local galaxy cluster. In some way, represent the following

stellar life cycle
terrestrials
gas planets
asteroid belt
Kuiper belt
powers of 10
life
gravity
orbit
Milky way galaxy
black hole
spiral arms

SIDE 2: This model is a V. At the point of the V, place the words Big Bang. At the top of the V, put "about 14 billion years" Then, using the diagram above, and the links below, fill out the V scape to show your understanding of:

energy
pieces smaller than atoms
fusion
galaxies
size of the universe
local galaxies
stars
chemical elements
speed using the Doppler effect
supernovas
dust clouds (nebulas)

Please give any mini-marshmallows that you brought to Melyssa. Melyssa will label them and put them in the wooden back cupboard and we will use them for tomorrow.

Hand these models in at the end of the hour.

LINKS:

Supernovas

Local Universe

Doppler Effect

Powers of TEN

History of the Universe

Planet Quest

Galaxy Zoo

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Sci.SI1.1: Using experimentation, students will contrast types of forces

Benchmark assessment: Students will create a Video voiceover a clip on YouTube, taking the role of a science broadcast announcer.

Components

Students will:

Sci.SI1.1.1 Demonstrate how balanced and unbalanced forces are related to motion.

Sci.SI1.1.2 Test, collect data, and verify Newton's laws of motion.

Sci.SI1.1.3 Contrast forces that act from a distance, including gravitation and magnetism.

Sci.SI1.1.4 Explain how mass and weight differ at different locations in the universe.

Sci.SI1.2: Through research and inquiry, students will apply the concepts of transverse waves to the use of sound and light wave technology.

Benchmark assessment: Student will synthesize their knowledge of light and sound waves to make a musical instrument that can play at least four distinct pitches and use the music created as part of a shadow puppet show.

Components

Students will:

Sci.SI1.2.1 Experiment with sound and light waves to identify the following structures or relationships: crests, troughs, frequency, wavelengths, amplitude, energy transmission, resonance(standing waves) and speed

Sci.SI1.2.2 Identify and experiment with part of the electromagnetic spectrum.

Sci.SI1.2.3 Use light to create penumbras, umbras, and colored shadows.

Sci.SI1.2.4 Experiment with wind or string instruments of varying pitch.

Sci.SI1.3: Through experimentation, Students will observe energy transformations, including potential and kinetic energy

Benchmark assessment: Students will create mousetrap cars and reflect upon the energy transformations.

Components

Students will:

Sci.SI1.3.1 Model changes in gravitational potential energy, spring potential energy, and kinetic energy.

Sci.SI1.3.2 Examine the energy changes in a variety of simple machines

Sci.SI1.3.3 Analyze the effectiveness of a machine for a job using its actual mechanical advantage.

Sci.SI1.4: Using inquiry and models, students will utilize alternative energies.

Benchmark assessment: Students will build a structure that allows us to utilize solar or wind energy in a useful way.

Students will:

Sci.SI1.4.1: Experiment with passive and active solar energy.

Sci.SI1.4.2: Experiment with models of wind energy.

Sci.SI1.4.3? Explain energy transformations in alternative energies.

Sci.SI1.5: Students will model heat transfer mechanisms as a rationale for weather and plate movement on the earth.

Benchmark assessment: Students will create a coloring book that shows the concepts of the chapter in a way that is understandable to a young reader.

Students will:

Sci.SI1.5.1: Contrast convection, conduction, and radiation inside the earth, in its water and weather patterns, and from the sun.

Sci.SI1.5.2: Examine the prevailing winds at different locations on earth, and discuss the movement of weather systems.

Sci.SI1.5.3 Model plate tectonics, earthquakes, and volcanos.

Sci.SI1.5.4: Analyze fossils and other technologies for tracking plate movement

Sci.SI1.6: Students will apply knowledge of geochemical cycles to the issue of climate change.

Benchmark Assessment: Students will come up with a life plan that discusses their usage of various cycles and ways to minimize their effect on the planet.

Students will:

Sci.SI1.6.1: Diagram movement of material between geochemical reservoirs.

Sci.SI1.6.2: Contrast the effect of various geochemical cycles on temperature and atmospheric concentration.

Sci.SI1.6.3: Quantify amounts of material found in reservoirs through visual and experimental models.

Sci.SI1.6.4: Explore ways to minimize their carbon footprint.

Sci.SI1.7: Students will apply their knowledge of the origin and scale of

space.

Benchmark Assessment: Students will create museum exhibits that are interactive, visual and three-dimensional to illustrate their understanding of the components.

Students will:

Sci.SI1.7.1: Model the solar system size and scale.

Sci.SI1.7.2: Examine distances in the cosmos based upon the concept of light speed.

Sci.SI1.7.3: Create time scales for geology on earth, the formation of the solar system, and the big bang.

Sci.SI1.7.4: Examine the process of radioactivity in a star like our Sun, and model its life cycle.