show properties

Example Plan

by Joseph mcnair

Grade Level

Grade Level

Grade 4 

Behavioral Objectives

Standards

Standards

FL.SC.A.1.3  The student understands that all matter has observable, measurable properties.
FL.SC.A.1.3.1  ...identifies various ways in which substances differ (e.g., mass, volume, shape, density, texture, and reaction to temperature and light).
FL.SC.A.1.3.2  ...understands the difference between weight and mass.
FL.SC.A.1.3.3  ...knows that temperature measures the average energy of motion of the particles that make up the substance.
FL.SC.A.1.3.4  ...knows that atoms in solids are close together and do not move around easily; in liquids, atoms tend to move farther apart; in gas, atoms are quite far apart and move around freely.
FL.SC.A.1.3.5  ...knows the difference between a physical change in a substance (i.e., altering the shape, form, volume, or density) and a chemical change (i.e., producing new substances with different characteristics).
FL.SC.A.1.3.6  ...knows that equal volumes of different substances may have different masses.
FL.SC.A.2.3  The student understands the basic principles of atomic theory.
FL.SC.A.2.3.1  ...describes and compares the properties of particles and waves.
FL.SC.A.2.3.2  ...knows the general properties of the atom (a massive nucleus of neutral neutrons and positive protons surrounded by a cloud of negative electrons) and accepts that single atoms are not visible.
FL.SC.A.2.3.3  ...knows that radiation, light, and heat are forms of energy used to cook food, treat diseases, and provide energy.
FL.SC.B.1.3  The student recognizes that energy may be changed in form with varying efficiency.
FL.SC.B.1.3.1  ...identifies forms of energy and explains that they can be measured and compared.
FL.SC.B.1.3.2  ...knows that energy cannot be created or destroyed, but only changed from one form to another.
FL.SC.B.1.3.3  ...knows the various forms in which energy comes to Earth from the sun (e.g., visible light, infrared, and microwave).
FL.SC.B.1.3.4  ...knows that energy conversions are never 100% efficient (i.e., some energy is transformed to heat and is unavailable for further useful work).
FL.SC.B.1.3.5  ...knows the processes by which thermal energy tends to flow from a system of higher temperature to a system of lower temperature.
FL.SC.B.1.3.6  ...knows the properties of waves (e.g., frequency, wavelength, and amplitude); that each wave consists of a number of crests and troughs; and the effects of different media on waves.
FL.SC.B.2.3  The student understands the interaction of matter and energy.
FL.SC.B.2.3.1  ...knows that most events in the universe (e.g., weather changes, moving cars, and the transfer of a nervous impulse in the human body) involve some form of energy transfer and that these changes almost always increase the total disorder of the system and its surroundings, reducing the amount of useful energy.

Resources

Resources

Earth Science: Solar System   
Welcome to the star and nine planets of our neighborhood, the solar system. Formed 4.5 billion years ago, it was made from dust and gas remnants of the big bang. Just one of billions of stars in our galaxy, the sun’s gravitational pull holds the planets, comets, meteors, and asteroids in orbit. This “ordinary” star produces the heat and light that make life on Earth possible. The sun will live a life of about 10 billion years before expanding and then contracting to become a white dwarf. Larger stars’ life cycles are more dramatic. They may go supernova and even form black holes, vast expanses where gravity is so strong that not even light can escape.
Spin Around the Solar System, A: Our Rocky Neighbors: The Inner Planets   
The four planets closest to the sun - including Earth - are small and dense, made of rock and metal. As a group they are often called the Inner Planets, the Rockies, or the Terrestrials. This program compares and contrasts members of the group - Mercury, Venus, Earth, and Mars - to each other and to the planets beyond. Students also learn about orbit paths, planet rotation, atmosphere, gravity, and other general solar system principles.