When high energy radiation strikes the Earth from space, it’s called cosmic rays. To be accurate, a cosmic ray is not like a ray of sunshine, but rather is a super-fast particle slinging through space. Think of throwing a grain of sand at a 100 mph… and that’s what we call a ‘cosmic ray’. Build your own electroscope with this video!


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Materials:


  • Clean glass jar with a lid
  • Wire coat hanger and sand paper
  • Aluminum foil
  • Vice grips or a hacksaw
  • Scissors
  • Balloon or other object to create a static charge
  • Hot glue gun (optional)


 


Download Student Worksheet & Exercises


Troubleshooting: This device is also known as an electroscope, and its job is to detect static charges, whether positive or negative.  The easiest way to make sure your electroscope is working is to rub your head with a balloon and bring it near the foil ball on top – the foil “leaves” inside the jar should spread apart into a V-shape.


Exercises


  1. How does this detector work?
  2. Do all particles leave the same trail?
  3. What happens when the magnet is brought close to the jar?

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If you think about it, the nucleus of an atom (proton and neutron) really have no reason to stick together. The neutron doesn’t have a charge, and the proton has a positive charge. And most nuclei have more than one proton, and positive-positive charges repel (think of trying to force two North sides of a magnet together). So what keeps the core together?


The strong force. Well, actually the residual strong force. This force is the glue that sticks the nucleus of an atom together, and is one of the strongest force we’ve found (on its own scale). This force binds the protons and neutrons together and is carried by tiny particles called pions. When you split apart these bonds, the energy has to go somewhere… which is why fission is such a powerful process (more on that later).



The fundamental strong force holds the quarks together inside the proton and neutron. Itty bitty particles called gluons hold the quarks together so the atom doesn’t fly apart. This force is extremely strong – much stronger than the electromagnetic force. This force is also known as the color force (there is not any color involved – that is just the way it was named.)


The electromagnetic force keeps the electrons from flying away from the nucleus. When a plus (the nucleus) and minus (the electron) charge get close together, tiny particles called photons pull the two together.


What is Radiation?

Radiation is energy or parts of atoms that are given off. We measure radiation with a geiger counter, which has a tube of gas inside that every time it gets hit by radiation, it gives off a little electrical charge.



[am4show have=’p8;p9;p17;p44;’ guest_error=’Guest error message’ user_error=’User error message’ ] In the 20th century, scientists figured out that the core of an atom can break apart or join together with others. If you split an atom (called fission), you get smaller parts and a whole lot of energy. When this happens in nature, it’s called radioactivity. Unstable atoms spontaneously break apart and release particles and energy.


Here’s a cool video that shows the fission chain reaction (you can do this also if you have a box, at least 25 mouse traps and 25-50 ping pong balls with adult help):



Fusion is taking place inside the sun. The sun is not on fire, like a campfire or stove. So where does it get its energy from? The fusion process smacks particles together, which results in a big release of energy. The core of the sun is about one million degrees Celsius, which the surface temperature is a mere 15,000 degrees Celsius. The fusion process in the sun takes two naked protons (also known as a hydrogen nuclei) and smacks them together in a special sequence that results in the formation of helium. This complicated reaction is called the proton-proton chain, and occurs in all stars burning hydrogen in their core.


Radioactivity can be dangerous, but it isn’t always dangerous. For example, your household smoke alarm emits alpha particles (the main detector uses alpha decay), brick and mortar building emit beta particles, and gamma particles come directly from the sun. In fact, people themselves emit beta particle radiation! When an atom of radioactive material decays, there are three types of radiation that it may emit: alpha, beta, and gamma. Generally speaking, most radioactive materials emit two, or all three types of radiation.


Alpha particles were named long before we ever knew what they were. An alpha particle are two protons and two neutrons stuck together (also known as helium nuclei). Beta particles are either electrons or positrons. Gamma particles, also called gamma rays, are actually electromagnetic radiation (photons) of very, very high frequency and energy – high enough to damage living tissue. Fortunately, gamma ray bursts are rare and usually not pointed in our direction.


Alpha particles are relatively slow and heavy. They have a low penetrating power, so you can stop them with just a sheet of paper. Alpha particles can not penetrate your skin. Due to the low penetrating power of Alpha particles, they are generally not a cause for concern, unless you ingest some material that emits Alpha radiation. For the most part, materials that emit Alpha particles, also emit some Beta or Gamma radiation.


Beta particles are fast and light. Beta particles have a medium penetrating power, but they are stopped by a thin sheet of aluminum (such as aluminum foil) or plastic. Beta particles can penetrate deeply into your skin.


Gamma rays have a high penetrating power. It takes a thick sheet of metal such as lead, or concrete to reduce them significantly. If you want to stop all gamma rays dead in their tracks, you’d need a sheet of lead 27 light-years thick. (Yikes!) Gamma rays penetrate your skin, and continue going right through your body.


The really unusual aspect of radiation is that the emission levels stays constant, no matter how hot or cold you make the material, or if you shove it into the deep vacuum of space or increase the pressure to bursting,  the rate of natural radioactive decay from radioactive materials will always remain the same. This is why materials of this type are used in Atomic Clocks.


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Let’s see how much you’ve picked up with these experiments and the reading – answer as best as you can. (No peeking at the answers until you’re done!) Just relax and see what jumps to mind when you read the question. You can also print these out and jot down your answers in your science notebook.
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  1. All visible matter is made up of…?
  2. What is a quark?
  3. What’s the charge on an electron, proton, and neutron?
  4. What keeps the quarks together inside a proton?
  5. Are free neutrons or protons more stable?
  6. What forces are the 79 protons together inside a gold atom feeling?
  7. Why does an electron stick around to orbit a nucleus?
  8. Where can you find anti-matter on Earth?
  9. What’s the difference between fusion and fission?
  10. Where can you find radiation?

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Need answers?


Let’s see how you did! If you didn’t get a few of these, don’t let it stress you out – it just means you need to play with more experiments in this area. We’re all works in progress, and we have our entire lifetime to puzzle together the mysteries of the universe!


Here’s printer-friendly versions of the exercises and answers for you to print out: Simply click here for printable questions and answers.


Answers:
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  1. All visible matter is made up of electrons, protons and neutrons.
  2. A quark makes up the nucleus of an atom.  A proton is made up of two up quarks and one down quark.  A neutron is made up of one up quark and two down quarks.
  3. An electron has a negative charge, a proton has a positive charge, and a neutron has no charge.
  4. The gluons hold the quarks together to form neutrons and protons.
  5. Free neutrons flip into a more stable proton within 15 minutes.
  6. The protons are feeling an electromagnetic ‘repulsive push’ force, as they are all the same charge. (Think of how two north sides of a magnet don’t like each other.) However, the residual strong force is much stronger at the atomic scale and overcomes the repulsive force and pions bind the protons together.
  7. An electron has a negative charge, which is attracted to the positive charge of the protons inside the nucleus.
  8. A PET scan is a way of imaging using positrons.  Patients ingest anti-matter and a machine takes pictures of the puffs of energy given off by the colliding matter (electrons) and anti-matter (positrons).
  9. Fission is splitting atoms apart, and fusion is smooshing them together.  An atomic bomb uses fission, and the sun uses fusion.
  10. When an atom spontaneously undergoes fission (splitting), it’s called fission.  Uranium 235 is an example of an element that does this.

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This stuff is definitely sci-fi weird, and probably not appropriate for younger grades (although we did have a seven year old reiterate in his own words this exact phenomenon to a physics professor, so hey… anything possible! Which is why we’ve included it here.)


This experiment is also known as Young’s Experiment, and it demonstrates how the photon (little packet of light) is both a particle and a wave, and you really can’t separate the two properties from each other. If the idea of a ‘photon’ is new to you, don’t worry – we’ll be covering light in an upcoming unit soon. Just think of it as tiny little packets or particles of light. I know the movie is a little goofy, but the physics is dead-on. Everything that “Captain Quantum” describes is really what occurred during the experiment. Here’s what happened:



So basically, any modification of the experiment setup actually determines which slit the electrons go through. This experiment was originally done with light, not electrons. and the interference pattern was completely destroyed (as shown in the end of the video) by an ‘observer’. This shows you that light can either be a wave or a particle, but not both at the same time, and it has the ability to flip between one and the other very quickly.  (The image at the left is a photograph of an interference pattern – the same thing you’d see on the wall if you tried this experiment.)


So, both light and electrons have wave-particle characteristics. Now, take your brain this last final step… it’s easier to see how this could be true for light, you can imagine as a massless photon.


But an electron has mass. Which means that matter can act as a wave.  Twilight zone, anyone?


Read more about this in our Advanced Physics Section.


This experiment is for advanced students. Here is another way to detect cosmic rays, only this time you’ll actually see the thin, threadlike vapor trails appear and disappear. These cobwebby trails are left by the particles within minutes of creating the detector. (Be sure to complete the Cosmic Ray Detector first!)


In space, there are powerful explosions (supernovas) and rapidly-spinning neutron stars (pulsars), both of which spew out high energy particles that zoom near the speed of light. Tons of these particles zip through our atmosphere each day. There are three types of particles: alpha, beta, and gamma.


Did you know that your household smoke alarm emits alpha particles? There’s a small bit (around 1/5000th of a gram) of Americium-241, which emits an alpha particle onto a detector. As long as the detector sees the alpha particle, the smoke alarm stays quiet. However, since alpha particles are easy to block, when smoke gets in the way and blocks the alpha particles from reaching the detector, you hear the smoke alarm scream.


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Alpha particles are actually high speed helium nuclei (which is two protons and two neutrons stuck together). They were named long before we knew what they were of, and the name stuck. Alpha particles are pretty heavy and slow, and most get stopped by just about anything, a sheet of paper or your skin. Because of this, alpha particles are not something people get excited about, unless you actually eat the smoke detector.


Both brick buildings as well as people emit beta particles. Beta particles are actually high speed electrons or positrons (a positron is the antimatter counterpart to the electron), and they are quick, fast, and light. You can stop a beta particle by holding up a thin sheet of plastic or tinfoil.


When you hold the jar in your hands, you warm it slightly and cause the air inside to get saturated with alcohol vapor. When the alpha particles (cosmic rays) zip through this portion of the jar, they quickly condense the alcohol and create spider-webby vapor trails. Try using a magnet to deflect the cosmic rays.


Here’s what you need:


  • rubbing alcohol
  • clean glass jar
  • black felt
  • hot glue gun
  • magnet
  • flashlight
  • scissors
  • dry ice and heavy gloves for handling the dry ice (and adult help)


 
Download Student Worksheet & Exercises


You will be making a special cloud chamber that holds alcohol gas inside. When you hold the jar in your hands, you warm it slightly and cause the air inside to get saturated with alcohol vapor. When the alpha particles (cosmic rays) zip through this portion of the jar, they quickly condense the alcohol and create spider-webby vapor trails. Kind of like when a jet flies through the air – you can’t always see the jet, but the cloud vapor trails streaming out behind stay visible for a long time. In our case, the vapor trails are visible for only a couple of seconds.


  1. Cut your felt to the size of the bottom of your jar.  Glue the felt to the bottom of the jar.
  2. Cut out another felt circle the size of the lid and glue it to the inside surface of the lid.
  3. Cut a third felt piece, about 2 inches wide, and line the inside circumference of the jar, connecting it with the bottom felt. Glue it into place.
  4. Strap goggles on your face. No exceptions.
  5. Very carefully pour a tablespoon or two of the highest concentration of rubbing alcohol onto the felt in the jar. You don’t need much. Swirl it around to distribute it evenly. Do the same for the lid. All the felt pieces should be thoroughly saturated. Cap the jar and leave it for ten minutes while you explain about dry ice (see safety precautions above under Important Project Considerations.
  6. Your teacher is coming around with the dry ice. Remove the lid and your teacher will place a small piece of dry ice right on the lid. Invert the jar right over the lid. Leave the jar upside down.
  7. DO NOT SCREW ON THE CAP TIGHTLY! Leave it loose to allow the pressure to escape.
  8. Sit and wait and watch carefully for the tiny, thin, threadlike vapor trails.
  9. What do you think the magnet is for? (Hint: Keep it outside the jar.)

What’s Going On?

Cosmic rays have a positive charge, as the particles are usually protons, though one in every 100 is an electron (which has a negative charge) or a muon (also a negative charge, but 200 times heavier than an electron).  On a good day, your cosmic ray indicator will blip every 4-5 seconds.  These galactic cosmic rays are one of the most important problems for interplanetary travel by crewed spacecraft.


Most cosmic rays zoom to us from extrasolar sources (stars that are outside our solar system but inside our galaxy) such as high-energy pulsars, grazing black holes, and exploding stars (supernovae).  We’re still figuring out whether some cosmic rays started from outside our own galaxy. If they are from outside our galaxy, it means that we’re getting stuff from quasars and radio galaxies, too!


Cosmic rays are fast-moving, high-energy, charged particles. The particles can be electrons, protons, the nucleus of a helium atom, or something else. In our case, the cosmic rays we’re detecting are “alpha particles.” Alpha particles are actually high-speed helium nuclei (helium nuclei are two protons and two neutrons stuck together). They were named “alpha particles” long before we knew what they were made of, and the name just kind of stuck.


Did you know that your household smoke alarm emits alpha particles? Most smoke detectors contain a small bit (around 1/5,000th of a gram) of Americium-241, which emits an alpha particle onto a detector. As long as the detector sees the alpha particle, the smoke alarm stays quiet. However, since alpha particles are easy to block, when smoke gets in the way and blocks the alpha particles from reaching the detector, you hear the smoke alarm scream.


Alpha particles are pretty heavy and slow, and most get stopped by just about anything, like a sheet of paper or your skin. Because of this, alpha particles are not something people get very excited about, unless you actually eat the smoke detector and ingest the material (which is not recommended).


Both brick buildings as well as people emit beta particles. Beta particles are actually high-speed electrons or positrons (a positron is the antimatter counterpart to the electron), and they are quick, fast, and light. When an electron hit the foil ball, it traveled down and charged the foil leaves, which deflected a tiny bit inside the electroscope. A beta particle has a little more energy than an alpha particle, but you can still stop it in its tracks by holding up a thin sheet of plastic (like a cutting board) or tinfoil.


Important Project Considerations:


After creating your detector: You can bring your alpha particle detector near a smoke alarm, an old glow-in-the-dark watch dial or a Coleman lantern mantel. You can go on a hunt around your house to find where the particles are most concentrated. If you have trouble seeing the trails, try using a flashlight and shine it on the jar at an angle.


You will also be working with dry ice. The dry ice works with the alcohol to get the vapor inside the jar at just the right temperature so it will condense when hit with the particles. Note that you should NEVER TOUCH DRY ICE WITH YOUR BARE HANDS. Always use gloves and tongs and handle very carefully. Keep out of reach of children – the real danger is when kids think the ice is plain old water ice and pop it in their mouth.


If your dry ice comes in large blocks, the easiest way to break a large chunk of dry ice into smaller pieces is to insert your hands into heavy leather gloves, wrap the dry ice block in a few layers of towels, and hit with a hammer. Make sure you wrap the towels well enough so that when the dry ice shatters, it doesn’t spew pieces all over. Use a metal pie plate to hold the chunks while you’re working with them. Store unused dry ice in a paper bag in a cooler or the coldest part of the freezer. Dry ice freezes at -109 degrees Fahrenheit. Most freezers don’t get that cold, so expect your dry ice to disappear soon.


TIP: You can bring your alpha particle detector near a smoke alarm, an old glow-in-the-dark watch dial or a Coleman lantern mantel. You can go on a hunt around your house to find where the particles are most concentrated. If you have trouble seeing the trails, try using a flashlight and shine it right on the jar.


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This video gets you started on the right foot. We’ll outline what’s coming up for this unit and how to get the most out of our lesson together. Enjoy!