Plasma and NGSS

Driving to the Sun, Image Credit: NASA, https://apod.nasa.gov/apod/ap201003.html 

The Next Generation Science Standards do not explicitly discuss plasma science, but several of the standards and disciplinary core ideas can be addressed using plasma as an example. The following topics covered by the NGSS can easily be connected to plasma:

As this website develops, specific lesson plans and other resources will be tagged with specific standards for easy searching.

Below we provide examples of specific NGSS disciplinary core ideas, which can be used to introduce plasma science to K-12 students. 

K-5 Grade

K. Weather and Climate - Establish that the Sun is hot and glows (emits its own light). Discuss lightnings as a form of severe weather. Make the observation that lightnings are also hot and glow. Conclude that similarities between the Sun and lightnings suggest that they are made of the same stuff.

1. Waves: Light and Sound: PS4.B: Electromagnetic Radiation - Objects can be seen if they emit their own light  or if they are illuminated by light . Use the Sun as an example of an object that emits its own lights and the Moon as an example of an object that glows because it is illuminated by the Sun.  Conclude that these differences between the Sun and the Moon suggest that they are made of different stuff.

1. Space Systems: Patterns and Cycles: ESS1.A: The Universe and its Stars - Continue the discussion of objects that emit their own light (Sun and stars) and objects that glow because they are illuminated (Moon and the planets in the Solar System). Confirm the conclusion that these two groups of objects are made of different stuff.

2. Structure and Properties of Matter - What we called "stuff " in K-1 is now called "matter". Four different kinds of matter exist: solid, liquid, gas, and plasma.

3. Forces and Interactions:PS2.B: Types of Interactions - Electric and magnetic forces between a pair of objects do not require that the objects be in contact, i.e., these forces act at a distance. The forth state of matter, called plasma, responds to electric and magnetic fields, which makes it very different from the other three states of matter introduced in 2nd grade. Plasmas can also give off their own electric and magnetic fields. We can conclude that if two objects are made of plasma, they will interact with forces that act at a distance.

3. Weather and Climate - Scientists record patterns of the weather across different times and areas so that they can make predictions about what kind of weather might happen next. Some plasma scientists study the patterns of the Sun to determine its effects on Earth's conditions. This is called space weather and it describes how conditions change in the Solar System and in the space around the Earth, for example, due to patterns of the Sun.

4. Energy: PS3.C: Relationship Between Energy and Forces -  When objects collide, the contact forces transfer energy so as to change the objects’ motions. Particles in plasma move very fast because they have a lot of energy.  Sometimes, when fast particles collide, they can merge (or fuse together) to form new particles. A lot of energy is produced when particles fuse together. This process is called fusion. The Sun produces its own energy through the process of fusion. The Sun is a natural source of energy.

Limitation: The concept that matter consist of  particles may not have been introduced at this stage. 

5. Structure and Properties of Matter - Matter of any type can be subdivided into particles that are too small to see, but even then the matter still exists and can be detected by other means. Plasma is a type of matter made of particles that can interact both by colliding, but also at a distance. These particles, called ions and electrons, have electric charge.

Note: Now that particles are introduced, the concept of energy production in fusion processes (suggested for 4th grade) can be (re-)introduced here.

5. Space Systems: Stars and the Solar System - The gravitational force of Earth acting on an object near Earth’s surface pulls that object toward the planet’s center. Similarly, the strong gravitational force of the Sun pulls planets, including the Earth, in an orbit around it. All stars, like our Sun, are made of plasma, and generate their energy through fusion of particles. Strong gravitational pull causes a very high pressure at the center of the Sun, which makes its plasma particles to fuse. This process, called fusion, releases energy and light. This is why the Sun is hot and emits its own light.

Middle School

MS. Structure and Properties of Matter

PS1.A: Structure and Properties of Matter: Substances are made from different types of atoms, which combine with one another in various ways. Atoms are made of positively charged core, called nucleus, surrounded by negatively charged particles, called electrons

Limitation: The concept that atopms are made of nucleus and electrons may not have been introduced at this point. The concept of positive and negative charges should be introduced in "Forces and Interactions" prior to discussing ions and electrons.

PS1.B: Chemical Reactions: In a chemical process, the atoms that make up the original substances are regrouped into different molecules, and these new substances have different properties from those of the reactants. 

MS.Forces and Interactions

PS2.B: Types of Interactions: Electric and magnetic (electromagnetic) forces can be attractive or repulsive, and their sizes depend on the magnitudes of the charges, currents, or magnetic strengths involved and on the distances between the interacting objects. 

MS.Energy: PS3A: Definitions of Energy - Motion energy is properly called kinetic energy; it is proportional to the mass of the moving object and grows with the square of its speed.  A system of objects may also contain stored (potential) energy, depending on their relative positions.

MS.Space Systems

ESS1.A: The Universe and Its Stars: Earth and its solar system are part of the Milky Way galaxy, which is one of many galaxies in the Universe. The Sun is a star. Like all stars in all galaxies in the Universe, the Sun is made of plasma gas. In fact, scientists have calculated that 99.999% of all visible matter in the Universe is in the plasma state. 

ESS1.B: Earth and the Solar System: The solar system appears to have formed from a disk of dust and gas, drawn together by gravity.  Too be precise, the gas is in the plasma state.  This disk of dust and plasma gas is one example of what is called a dusty plasma.

MS.Weather and Climate

ESS3.D: Global Climate Change: Human activities, such as the release of greenhouse gases from burning fossil fuels, are major factors in the current rise in Earth’s mean surface temperature (global warming). Reducing the level of climate change and reducing human vulnerability to whatever climate changes do occur depend on the understanding of climate science, engineering capabilities, and other kinds of knowledge, such as understanding of human behavior and on applying that knowledge wisely in decisions and activities.  


High School

HS. Structure and Properties of Matter

PS1.A: Structure and Properties of Matter: Each atom has a charged substructure consisting of a nucleus, which is made of protons and neutrons, surrounded by electrons. When an atom looses (gains) electrons, it becomes positively (negatively) charged and is called positively (negatively) charged ion.

PS1.C: Nuclear Processes - Nuclear processes, including fusion, fission, and radioactive decays of unstable nuclei, involve release or absorption of energy. The total number of neutrons plus protons does not change in any nuclear process. Nuclear fission is the process used to produce energy in modern-day nuclear power plants. Currently, scientists are working on building the next generation of power plants, where nuclear fusion will be used to produce energy.

HS. Chemical Reactions

PS1.A: Structure and Properties of Matter - A stable molecule has less energy than the same set of atoms separated; one must provide at least this energy in order to take the molecule apart. Similarly, in a nuclear fusion reaction, where two lighter atoms fuse to form one heavier atom, the heavier atom has less energy than the lighter atoms separately. This is why energy is released when the lighter atoms fuse into a heavier one.

HS.Forces and Interactions

PS2.B: Types of Interactions - Newton’s law of universal gravitation and Coulomb’s law provide the mathematical models to describe and predict the effects of gravitational and electrostatic forces between distant objects.

HS. Energy

PS3.A: Definitions of Energy - Energy is a quantitative property of a system that depends on the motion and interactions of matter and radiation within that system. That there is a single quantity called energy is due to the fact that a system’s total energy is conserved, even as, within the system, energy is continually transferred from one object to another and between its various possible forms.

PS3.B: Conservation of Energy and Energy Transfer -  Conservation of energy means that the total change of energy in any system is always equal to the total energy transferred into or out of the system.

PS3.D: Energy in Chemical Processes - Although energy cannot be destroyed, it can be converted to less useful forms—for example, to thermal energy in the surrounding environment. -->Talk about radiation losses in fusion devices

PS3.D: Energy in Chemical Processes and Everyday Life - Nuclear Fusion processes in the center of the sun release the energy that ultimately reaches Earth as radiation.

PS4.B Electromagnetic Radiation -  Atoms of each element emit and absorb characteristic frequencies of light. These characteristics allow identification of the presence of an element, even in microscopic quantities.

HS. Waves and Electromagnetic Radiation

PS4.B: Electromagnetic Radiation - When light or longer wavelength electromagnetic radiation is absorbed in matter, it is generally converted into thermal energy (heat). Shorter wavelength electromagnetic radiation (ultraviolet, X-rays, gamma rays) can ionize atoms and cause damage to living cells. -->Talk about waves/radiation in fusion devices

HS. Earth and Space Sciences

ESS1.A: The Universe and Its Stars -  The star called the sun is changing and will burn out over a lifespan of approximately 10 billion years.

HS. History of Earth

ESS1.C: The History of Planet Earth - Although active geologic processes, such as plate tectonics and erosion, have destroyed or altered most of the very early rock record on Earth, other objects in the solar system, such as lunar rocks, asteroids, and meteorites, have changed little over billions of years. Studying these objects can provide information about Earth’s formation and early history. --> Talk about how plasma physicists study dust in plasma on the surface of the moon, meteor formation and structure, cometary tails (basically, all of that is dusty plasma).

HS.Weather and Climate

ESS2.D: Weather and Climate - The foundation for Earth’s global climate systems is the electromagnetic radiation from the sun, as well as its reflection, absorption, storage, and redistribution among the atmosphere, ocean, and land systems, and this energy’s re-radiation into space. --> Talk about how a fusion reaction can be viewed as a mini-sun.

HS.Human Sustainability --> Talk about alrernative energy sources enabled by plasmas

ESS3.A: Natural Resources

 Resource availability has guided the development of human society.

 All forms of energy production and other resource extraction have associated economic, social, environmental, and geopolitical costs and risks as well as benefits. New technologies and social regulations can change the balance of these factors. --> Develop exercise cmparing the risks and benefits of different energy sources.