Cometary Tales Hands-On Science Cooking With Kuiper: Notes for Project Leaders

Cooking With Kuiper: Notes for Project Leaders

(update:  2/18/2015)

Last week on the tvweb, this happened: astronomer Derrick Pitts turned up once more on “The Late Late Show”.  And even though science-loving Craig Ferguson has moved on to new horizons, Director Pitts stayed and showed Guest Host Wayne Brady how to make a comet.  So I looked back at my entries for this project and realized they need some updates, and particularly some visuals. Have patience–it’s a multi-entry blog feature, so look for two more entries for the complete Updated Edition of “Cooking With Kuiper.”

The Kuiper Belt–that donut-shaped aggregation of hundreds-of-thousands of rocky objects orbiting beyond Neptune–is one of the most interesting regions of the Solar System just now.  Just last year, NASA’s Deep Impact explorer hurled a probe into the surface of Comet Tempel 1, flinging up a curtain of debris to reveal more about the comet’s composition.

Deep Impact's probe sent back this image just before striking Comet Tempel 1 (Image: NASA/JPL-Caltech/UMD)

Deep Impact’s probe sent back this image just before striking Comet Tempel 1 (Image: NASA/JPL-Caltech/UMD)

NASA’s New Horizons mission is due to arrive in July 2015 at Pluto–the most famous Kuiper Belt object–to observe the newly-redesignated dwarf planet and its five moons and then head out to explore.  You can check in on the progress of the mission at NASA’s home for New Horizons.  There is a general agreement among astronomers that the comets which return again and again (periodic comets)  began in the Kuiper belt.

In this project, we’ll be building a model of a comet using household supplies to represent most of the comet’s components and dry ice to capture the icy-cold environment of the Kuiper Belt.   While most Messy-Monday projects are entirely hands-on this particular activity is meant as a demonstration with controlled audience participation.  Some students may be careful enough to work with dry ice…but too many are not, and the step at which the dry ice is added can be dynamic and unpredictable.

A study of comets draws in much of what students should know about their planetary system and extends that knowledge into new and intriguing areas.  Students in intermediate grades probably know the basics of comets…that they come from the far reaches of the solar system, that they have tails, and that a comet crashing into the earth makes a cool disaster movie.  They might be surprised to know that scientists still want to find out more about comets, because all we know about comets so far is from watching them on their travels through the solar system.  Just a few months ago, the Rosetta spacecraft launched in 2004 by the European Space Agency actually landed a robotic explorer named Philae on Comet Churyumov-Gerasimenko, so why not launch an investigation into the nature and structure of comets by building our own lumpy, irregular, gas-spewing comets?

This activity is best paired with at least one hands-on activity centering on comets.   The second activity in this series combines a crafting-style model construction project and a cometary motion simulation game.  Other resources can provide other activities.  For instance, students can make a flip-book illustrating a short-period comet’s behavior as it travels from the orbit of Neptune to the sun and back.  And users of Pixel Gravity can run a simulation of the comet impact which led to the demise of the dinosaurs.

In the next installment, we’ll assemble a supply list for this project.  I recommend you  plan to build at least two comets, to let more kids participate and also to illustrate just how different two comets can be.

 

You might also like to read:

Cooking with Kuiper: Project Supply ChartCooking with Kuiper: Project Supply Chart

All Lined Up for Comet Building

All Lined Up for Comet Building

(Update:  2/18/2015)

As mentioned in the notes for project leaders, it’s best to repeat the procedure at least twice–three times if the class is large, to ensure that everyone has a chance to participate in the “safe” portions of the activity and to produce a variety of comets to observe.

Purchase dry ice in advance by as much as a day (purchase at the higher end of the quantity range if you need to store it overnight) and  store wrapped in insulating material, but not  tightly sealed.  (Frozen CO2 will sublime to gas and can even explode a container that is sealed too tightly.)  A small non-airtight cooler tucked into another lightly-closed, non-airtight cooler works fine, especially if wrapped in a blanket and stored in a cool location.

For the ice-cream topping, choose a small bottle with a squirt-style top full of caramel- or chocolate-flavor syrup for ice-cream sundaes.  Do NOT purchase hard-shell toppings;  stick to sticky sugar syrups.  Be prepared to fend off requests to sample the syrup.

For ammonia, do not use pure ammonia;  simply choose a basic non-sudsy ammonia-based cleanser.  A “sport-top” (squirting-style) water bottle about half-full of ammonia works well and keeps the ammonia away from hands, eyes, and clothing.  However, be sure to clearly label the bottle with the contents.

For trash bags, choose a good, sturdy brand.  They’ll take significant abuse!

Please note carefully that most equipment is required to be either plastic or wood.

  Per comet

For about 3-4 comets, allowing for waste and failures

 

Estimated cost

(2015 prices)

Good sturdy “tall kitchen” garbage bag, cut down one long edge to make a liner for the bowl 1

2

(have a second on hand in case the original tears)

$0.50

($12 for box of 45)

Additional “tall kitchen” garbage bags

3

Open the bags and layer them one inside the other, to create a triple-thick bag

6

Have a second layered set of 3 bags on hand in case of tears

$1.50

($12 for box of 45)

Large plastic mixing bowl, 2-cup plastic measuring cup, tablespoon measure, large wooden spoon

1 of each

Reminder:  for safety, use plastic containers and a wooden spoon

1 of each Bring from home or borrow from volunteers
Water 2 cups

2 quarts on hand

(store in a pitcher for measuring out in 2-cup quantities)

n/a
Sand or fine gravel 2 tablespoons ½ cup zero
Ammonia 

One squirt (about 1 tablespoon)

 

½ cup

$1.50

($10 for 28-ounce bottle)

Ice-cream topping

One squirt (about 1 tablespoon)

 

About ½ cup (Bring at least a 4-ounce container of syrup.) $6.50
Dry ice 2 cups of dry ice, after crushing. About 7-10 pounds of dry ice. $15($1.50 per pound)
Safety goggles

1 pair, adult size

1-2 pair, adult or child size (depending on student age)

1 pair, adult size

1-2 pair, adult or child size (depending on student age)

If not available in classroom—one-time purchase for reuse in many projects. $5 each

 

Heavy work gloves 1 pair, to fit Project Leader 1 pair, to fit Project Leader Use own gloves or borrow from volunteer (a new pair would cost about $10-12)
Total Cost: $39.50

For an easy-to-print version:  Just Supplies Cooking with Kuiper

Cooking With Kuiper: The Instruction SetCooking With Kuiper: The Instruction Set

(update:  2/18/2015)

Time to build a comet!

If you have adult or older-student assistants, ask them to take charge of crowd control; that is, keeping the audience from crowding around the demonstration. Everyone will get to see the comet! Spare a minute for a brief lecture on the hazards of dry ice. You may have participants who know that dry ice can “burn”, but not all will understand that idea at first. However, no one wants to get hurt. Mention that you will be protecting your hands with gloves and your eyes with safety goggles (or safety-rated eyeglasses).

Supplies for Comet Making (Just Add a Cooler-Full of Dry Ice)

Supplies for Comet Making (Keep your cooler-full of dry ice in a safe spot.)

Participation opportunities include: helping move the materials and equipment to a mess-tolerant location, measuring ingredients, and smashing dry ice. The trauma of allotting slots to help out is one important reason to try the exercise at least twice. (Crowd-control tip: sometimes it helps to announce “I’ll only choose helpers from those who do not raise hands and call out to volunteer.”)  As a first step, take one of your plastic bags and cut it open along one side, then use it to line your mixing bowl.  Take 2 other bags and put one inside the other to make a double-thickness bag.

In the first stage,  your chosen helpers will take turns measuring all the “safe” ingredients into the bag-lined mixing bowl.  Working with the dry ice needs closer control, so keep your supply of CO2 off to one side for now.  As you introduce each ingredient, explain why it’s being included.  You can use the short explanations provided here as a starting point, adding your own facts or curriculum tie-ins, but remember to keep it brief or you’ll lose your audience’s attention.

Let’s start with water: most comets are composed primarily of water ice. During the early formation of the solar system, the planets were bombarded by comets—so some of the water you will use in this experiment may have actually originated in the Kuiper Belt!  (For a popular-science overview, check out this article from Time Magazine.)  Your helper will add 2 cups of water.

Next, add sand or gravel: most comets incorporate at least some rocky material.  Have your helpers measure out about 2 Tablespoon (TB) of grit.

Next, you’ll add ammonia: real comets typically contain NH3, the active ingredient in this cleaning solution.   (Regrettably, few, if any, comets show up to help when it’s time to clean house.)  If you’re using a squirt bottle to store the solution, your helper just needs to add one “squirt” of ammonia solution.  Otherwise, your helper should measure in 1 Tablespoon.

A Dirty Soup of Rocks, Water, and Organics

A Dirty Soup of Rocks, Water, Ammonia, and Organics

And, for our last step before major excitement sets in, stir in a touch of ice-cream topping: these contain organic molecules, which are a normal component of comets. The organic molecules in real comets are not this delicious–they include hydrogen cyanide and formaldehyde–but comets often contain complex and interesting compounds such as amino acids.   Researchers at NASA’s Ames Research Center have shown that amino acids from comets striking Earth long ago during the Solar System’s early eons would not only survive impact but would form even more important compounds for life under the heat of impact.   So it may be that we are here to enjoy ice cream (and sugary toppings) thanks to ancient comets.   Let your helper squirt in one squeeze-worth (it will be about a tablespoon).

Now, finally, it is time to add the dry ice.  Comets contain significant quantities of frozen gases, especially carbon dioxide, which just happens to be the gas that we call “dry ice” when frozen.  This stage of your demonstration is a two-step process. First, you will put on safety goggles and work gloves and use the hammer to tap off about 2 pounds of dry ice (1/4 to 1/3 of your supply).  Place the chunks into the doubled plastic bag and twist the opening closed.  Then, and only then, one lucky volunteer will be asked to don a set of goggles and, once protected, may proceed to smash the contained dry ice with the hammer.

Crushing Dry Ice with Flat Side of Hammer

Crushing Dry Ice with Flat Side of Hammer

Have your crusher use a two-handed grip (this helps deflect the temptation to also handle the bag of dry ice and also limits the range of motion, protecting bystanders from the crusher’s swing) and turn the hammer sideways, to smash with a broader surface area.

Once that stage is completed, ask the crusher to rejoin the group.  Make sure that the wooden stirring spoon is at hand and that you are still wearing your work gloves and goggles. Then open the bag and quickly scoop out roughly two cups of crumbled dry ice.

2 Cups of Ice-Cold CO2

2 Cups of Ice-Cold CO2

Give the mixture a stir and then swiftly add the dry ice, stirring vigorously. There will be some dramatic vaporization of CO2 and in moments the dry ice will freeze the water solution to a slushy slurry. Quickly wrap the plastic bag around your slushy mass and—keeping those gloves on—form the contents into a snowball, using firm pressure to shape the contents.

Comet's In the Bag

Comet’s In the Bag

You will feel the mass harden as you form your iceball. At that point, it is time to unwrap the comet and reveal it to your onlookers. You will have something that looks surprisingly like the common description of a comet—“a dirty snowball”.  You may even want to use your snowball-making skills to firm up the comet a bit once you remove it from the bag–remember to keep your gloves on!

Forming Up the Proto-Comet

Firming Up the Comet

Your finished comet

Your finished comet

Set the comet aside on a cold-safe surface, in a location where the eventual water-ice-melt will not damage anything. The comet will continue to outgas CO2 vapor. If you are working outdoors, any breeze will push this plume into a fair imitation of a comet’s tail.

Gases (CO2) immediately begin to sublime from the comet's surface

Gases (CO2) immediately begin to sublime from the comet’s surface

Your experiment team will undoubtedly want to repeat this process. A typical group of students will demand about four comets. After 2 or 3 builds, it will be time to set up fresh plastic bags for mixing and crushing.  If the group is larger, find ways for students to share participation tasks. For instance, two students can take turns as dry-ice crusher, two can each measure one cup of water into the mix, and so on.  As you proceed, instead of repeating the descriptive information yourself, invite the students to call out more of what they remember about the components represent.

Comet, Starting in "Dirty Snowball"

Here’s one small starter comet, let’s call this one “Dirty Little Snowball”

 

These model comets will last a long time, up to a few hours depending on their size and the conditions.  You can explain that the comets which get our attention are much larger–Comet Halley is estimated to be about the size of Manhattan Island–and between visits to the inner Solar System, they orbit back to where it is too cold for water, ammonia, or CO2 to be anything other than solids.  By no means do you need to make any effort to create spherical, smooth comets.  In fact, as you create successive comets, allow them to be different, irregular, and, well, messy.  Here are a few samples from a few of my comet-making sessions:

That's one frosty, rocky, comet:  "Before"

That’s one rocky comet, frosted with ice crystals of H2O and CO2

 

 

That's one slimy, partly-dissociated comet

Here’s a comet with conspicuous dark patches

That's one tall, cone-shaped comet

That’s one tall, frosty, cone-shaped comet

 

 

 

 

 

 

 

If your schedule permits, allow some time to pass and return to look at the comets after they have lost more material, as if you are checking in on a comet as it approaches the sun and some of its ice has been drawn off under the combined forces of the sun’s radiation and the solar wind…forming the comet’s tail.

Holey Comet, Batman!

Holey Comet, Batman!

On Aisle 42, Universe Components: One Will Make You SmallerOn Aisle 42, Universe Components: One Will Make You Smaller

 

Or

A Top-Down Search for the Strange Charm of Putting Up With Those Quarks at Bottom of the Universe

For part two of our universe-construction project, while the helium models dry, it’s time to delve into the depths of the sub-sub-atomic universe.

Consider those carefully-constructed model atoms.   Each contains protons, neutrons, and electrons.

As it turns out, with electrons, there are (so far as physics can determine at present) no smaller particles needed to build an electron.  Electrons are part of a group of  six elementary particles called leptons.  Some of these leptons–the neutrinos–were predicted to not even have any mass, but experiments have shown that while they are incredibly low-mass, neutrinos do have some mass.  Interestingly, these experiments leading to even more new developments in fundamental physics and the Standard Model theory.  Still, electrons are by far the most numerous leptons (at least in our corner of the multiverse.)

In our candy-based model, we have more than one proton crammed into in a nucleus.  Each of those protons has a positive charge, but we all know that objects with the same charge repel each other.  Why does the nucleus stay together?

In our model, of course, there is all that sticky candy.  But in the real atom, there is also something that, in its own way, makes protons stick together.  These other particles are one type of another class of matter, called mesons.  These strange, essential, particles are stable only inside the nucleus, where (like our sticky marshmallows) they act as a “glue” to hold protons and neutrons close together.

Given that extremely tiny leptons have been observed, as well as tiny mesons inside the nucleus, protons and neutrons may begin to seem too big to be elementary particles.  Sure enough, it turns out that protons and neutrons are also made of smaller particles.  And those mesons, too, are made of those same even-smaller particles.  And, while it took thirty years to search them all out, a total of six more fundamental particles (on top of the six leptons) have been found.  Most of the matter we know about only requires two of those particles–plus the electron–but modern physics predicted six, and sure enough, there are six of them.

Meet the QUARKS.  Their six kinds are: up, down, charm, strange, top, and bottom.  Each kind comes in a matter form and an antimatter form.

Intriguingly, the terminology for “kinds” of quarks is flavors. Other characteristics of quarks and leptons include color, another clue to the pleasure scientists find in these discoveries.   For now, we’ll experiment with the flavors of quarks.  Unlike real quarks, we will use macroscopic objects that also happen to taste sweet.

As usual, if you’re working with youngsters, begin by reassuring everyone that there will be plenty of time to eat their quarks later.  Each person gets one each of the six flavors of candy…quarks. Because the candies will be handled a lot during the first stage, tell them not to open the wrappers yet.   Observe the candies.  One side has the brand name on it, and the other side is plain.  If we put the candy name-side up, we’ll call it a quark, and if it has the plain side up, we’ll call it an antiquark.

Quark vs Antiquark

A meson is formed by pairs of one quark and one antiquark.  Give the group some time to see just how many combinations can be made of such pairs.  (A few special mesons combine two or three such pairs, in quark combinations.)

A Small Set of Mesons

This will take some cooperation–participants will want to get together and different groups will organize their tests differently.  Meanwhile, if you have access to a whiteboard or poster paper, you can sketch out a list of simple mesons shown below.  For smaller (or older) groups, you can also pass out copies of this grid and let everyone check off the combinations as they are discovered.

quark antiquark candy (name) candy (plain)
bottom eta b b pineapple pineapple
Upsilon b b pineapple pineapple
charmed eta c c purple purple
D+ c d purple peppermint
D0 c u purple red
J/Psi c c purple purple
Strange D c s purple green
Charmed B b c purple pineapple
Kaon0 d s peppermint green
B0 d b peppermint pineapple
Phi s s green green
Strange B s b green pineapple
pion u d red peppermint
kaon+ u s red green
B+ u b red pineapple
Charged rho u d red peppermint
Kaon*+ u s red green

What’s important from this exercise is realizing that all of these two-quark combinations can really happen.  Some of the mesons are the ones that help stick nuclei together.  Others are found in outer space, as cosmic rays.  Others are only found when scientists smash other particles together to find out what they are made of.  Recently, the last of the mesons described by this model was detected by an international team of physicists, using the Large Hadron Collider at CERN, in  Switzerland.  This prompted huge celebrations by physicists and the process inspired a documentary film about the search for the Higgs Boson, Particle Fever.

When I ran this project at BayCon in 2017, one of the young participants scanned the list above and said, “What about the top quark?”  Trust a science-fiction fan to spot an anomaly.  Indeed, none of the known mesons make use of the top quark, which is the most elusive one of all, and in some ways the most peculiar.  The top quark is extremely unstable–even more ephemeral than the strange, charm, and bottom quarks–and it requires a large particle accelerator to observe one. (Fermilab managed it first; now CERN‘s Large Hadron Collider holds the record.)  Even then, once produced, a top quark vanishes in 1/1,000,000,000,000,000,000,000,000th of a second.  The top quark is also amazingly massive, fueling the deep interest in the nature of mass itself, which many think is one of the functions of the Higgs boson, which itself has only recently been (tentatively) observed.  Scientists at CERN hope to use the relatively massive top quark as a test laboratory to verify their (provisional) Higgs boson observations.

Three-quark particles are called baryons–the most common of these are protons and neutrons.  The next step for our own quark exploration is to find the combination of up and down quarks that yields the proton and the one that forms a neutron.   Each person has 2 peppermint and 2 of one other color to play with. Each group can also pool resources (still keeping those candy wrappers on) to mix and match groups of three using only 2 colors of candy.

To sort out which of these combinations works requires one extra piece of information.  We know that an electron has a charge of -1, a proton has a charge of +1, and a neutron is neutral, with a charge of zero.   Another cool feature of quarks…and one of the hardest things their discoverers had to come to terms with…is that they have fractional charges.  Before quarks, everyone used to think of a charge…equal to the electric charge of an electron…as an indivisible thing.  Just like an atom.  But just as it has turned out that atoms aren’t indivisible, neither is charge.

Up quark’s charge:       +2/3

Down quark’s charge:   -1/3

So, with just a little arithmetic, we can find out which of our combinations makes a proton and which makes a neutron.  Here’s the cheat sheet:

uuu

2/3 + 2/3 + 2/3 = 2

Positive…but too much for a proton
ddd

(-1/3) + (-1/3) + (-1/3) = -1

Negative, so it can’t be a proton or a neutron.

Note:  it’s not an electron either–remember, an electron is already an elementary particle.

uud

or udu

or duu

2/3 + 2/3 + (-1/3) = 1

OK!  It’s a proton!
(Just a reminder…the order the quarks are listed in doesn’t matter.)
ddu

or dud

or udd

-1/3 + (-1/3) + 2/3 = 0

Yes!  We have discovered the neutron!

 

Aha, it’s a proton.

Aha, It’s a neutron!

So, the charge calculations show that protons and neutrons are made of two ups plus one down for a proton and two downs plus one up for a neutron.

It’s possible to have participants glue their protons and neutron quark groups together.  A dip on the water cup from the atomic marshmallow project will make a candy piece sticky.  However, these sticky messes will need to sit aside for a while to dry.  If your participants include young children, you might want to skip that possibility, as a glued-up stack of Life-Savers could be a choking hazard.

Speaking of glue, the same BayCon2017 participants also suggested some ideas for incorporating gluons into our model.  To cover the topic of quantum chromodynamics would be a fun challenge, but for the present, those lonely orange LifeSavers we’d set aside as those transient top quarks can be added between the red and white candies in our proton and neutron models to represent the color exchanges among the quarks.

So now we have established that everything in matter is made of tiny (and flavorful) points of dancing energy called quarks and leptons. How can we visualize the true relative sizes of these quarks, protons, nuclei, and atoms?

Poke a pin through a piece of paper and hold it up to the light, then pass it around, so everyone can see how tiny that hole is.   Think of that bright speck as an electron or a quark.  To be at the same scale, our helium nucleus would be about 3 feet across.  A handy meter-stick or yardstick will provide a sense of scale, but for drama, bring out a huge balloon (the 36-inch size).  It won’t be edible, but it will be fun to play with afterwards.  If that big old balloon is the tiny nucleus, then to build a whole helium atom we’d need a marshmallow about seven miles (ten kilometers) across!

So let’s check back on our atom model from the atomic marshmallow project.  It’s mostly nothing, just that airy, fluffy marshmallow.  Remember how thin the “shell” of the electron cloud is, and how surprisingly hard it is to notice the tiny nucleus once the two little protons and neutrons were placed inside.  Even so, in our model, the protons and neutrons are huge compared with the atom.  Imagine how fantastic the resulting candy treat would be–and how many people could enjoy it–if we’d tried to make this marshmallow atom model to scale.

© 2012-2026 Vanessa MacLaren-Wray All Rights Reserved