Monday, January 11, 2016

Heating a household

Human Energy

If we could convert 100% of the heat energy released by every human being in the world to electricity for a day, for how long could that power an average household?

A long time.

Let's start with the amount of energy one human being releases. The USDA recommends a generic 2000 calorie diet, which changes according to height, weight, age, gender, health, time of year, etc. All in all, few people adhere to 2000 a day, least of all me. I found a 2010 statistic putting the global average energy consumption at 2780 kcal/person/day. 

Pretty much all of our energy is released as heat, so on average, each individual will release 11631.53 kJ (1kcal = 4.184kJ).


The global population as of December 27, 2015 at 11:16:38 pm Pacific time was 7,390,835,780. This puts the amount of heat energy released at 8.5967 × 10^13 kJ/day.


Globally, the average household consumes roughly 3,500 kWh/year. 1kWh = 3600kJ, and there are 365 days in a year, so that's about 1.26 × 10^7kJ a year, 34,520.538kJ/day. Dividing 8.5967 × 10^13 kJ by 34,520.538kJ/day, we get 2.4903 × 10^9 days of power for that single household, or 6,822,779 years, 9 months and 11 days. By then of course, the amount of electricity consumed by the average household will have risen dramatically and then probably dropped right about the time that humans go extinct by killing themselves with nukes, global warming, and bad TV shows.


What else can we do with 8.5967 × 10^13 kJ? 


This is about 85.967 petajoules, or 20.5 megatons of TNT.


  • 80% of the energy expended by a Cold War era hydrogen bomb
  • 95.5% of the maximum theoretical yield from 1 kg of matter by converting all of the mass into energy
  • The energy released by combusting 1.06 × 10^11 moles of methane gas

Let's use some other aspect of humans to make energy!


Potential energy 

Imagine that every single human being in the earth is suddenly dropped down to sea level, breaking all laws of physics. How can we convert this energy into usable energy? Magically.

Potential Energy = Force of Gravity × Distance fallen = Mass of object × Distance fallen × Acceleration due to Gravity

As of 1994, the median person lived at an elevation of 194 m above sea level. Since then, the sea level has risen about 62 mm, and people have shifted around. Unfortunately, 1994 was the most recent data I could find. It seems that the field of hypsographic demography is sadly neglected.

We will use 194m to get a ballpark idea. 

The average mass of every human being is 62 kg.

For the median person - 194m × 62kg × 9.8 m/s^2 = 117874 kg m^2/s^2 = 117874 Joules.

Multiplied by 7,394,242,915 people (global population as of now), and we have 871,588,989,362,710 J = 8.71 × 10^14 J.

Which is a lot of energy, if we could ever figure out how to get it.












Fire

What household items can I use to make pretty fires?

Well, firstly, flames have different colors based on temperatures. Blue fire, seen at the center of a candle flame, is the hottest, followed by white, orange, and red flame. The reason for colored flame is that when the particles are heated, electrons are excited to a higher energy level. Electrons don't like to be excited, though, because that's unstable, so electrons release the energy in the form of electromagnetic radiation. In this case, the electron releases a photon. The wavelength of this photon - and thus, the color - depends on the amount of energy the electron "fell" back down.

The flame can be divided into blue, white, orange, and red regions because in each of these regions, the amount of combustible material and the temperature in the area is nearly equal within the region. This means that electrons are gaining and losing about same amount of energy as each other. Thus, almost every particle in that region releases a photon with the same wavelength, creating an overall red or orange color.

Metals or salts, when burned, also produce distinct colored flames. The chemical tends to overcome the temperature factor in regard to the color of the flame - for example, when sodium is burn in a blue flame, it turns the flame yellow.

Let's get into some of the elements that burn your favorite colors, and where you can easily find ways to get these colors!

Red

For red (see Valentines day, Independence day, Chinese New Year, or just because) we can use lithium, strontium, and rubidium.

  • Burn lithium batteries. For extra explosions, water can be added to the extremely reactive lithium.
  • Bipolar medication. Lithium is also used to cheer people up and reduce chance of suicide.
  • Sensodyne Toothpaste. Strontium chloride will provide a bright red flame, and it's found in sensodyne.

Orange

Orange might not be as useful, considering you can make orange fires by burning, say, wood, or paper, or yourself. However, for those who love chemistry, calcium will form orange fires.
  • Chemistry tests done with improper significant figure usage are easy to burn to produce a mostly orange fire.
  • Chalk - it contains calcium sulfate.

Yellow

Again, yellow fires are fairly common. However, sodium can turn even blue fires bright yellow. For yellow-green, see below.
  • Table salt (NaCl) - it contains sodium.
  • Baking soda and baking powder also have high sodium content.

Green

Green is useful on Saint Patrick's day, or just to really freak out people who have never seen a green fire before. Copper is a famous metal that produces a distinct green flame. Thallium will also produce a bright green. For your lighter greens, use tellurium or antimony. For yellow-green, burn manganese, molybdenum, or barium. For blue-green, burn zinc or phosphorus.
  • Pennies. They're made of copper, and they're pretty much useless anyway.
  • Most electronics have copper wire in them. 
  • Thallium is extremely toxic, so do not try burning it at home.
  • Stainless steel pans/other things made from stainless steel. Tellurium is found in small amounts in stainless steel to make it easier to work with. Tellurium is a also semiconductor often doped with copper or tin.
DOPING FACT: If tellurium, a semiconductor with 6 valence electrons, is doped with tin, with 4 valence electrons, there will be 2 extra electrons left from the tin to move around and increase conductivity. In copper, with 1 valence electron, 1 electron carrier will move around and increase conductivity. Respectively, they are n-type and p-type doping.
  • Lead-antimony battery plates contain both lead and antimony. The blue flame produced by lead will probably overcome the antimony, however.
  • Steel pots and pans. Manganese has a crucial part in steel-making.
  • Aluminum cans. Aluminum with a 1.5% manganese content has anti-corrosive properties.
  • Gears. Molybdenum can withstand intense heat, so it's commonly alloyed with steel and used in high temperature situations.
  • TV picture tubes or other vacuum tubes. Barium (sometimes alloyed with aluminum) is used to maintain a vacuum by getting rid of unwanted gases. It can do this because it reacts with many components of air and has a low vapor pressure.
  • The outside of your car, or the lightpost outside. Zinc is commonly used as an anti-corrosive agent. It is coated onto the other metals and because it is so reactive, it attracts oxidation to itself, thereby protecting the metals it is coated over.
  • Fertilizer. Phosphorus is an essential plant nutrient.

Blue

Arsenic, lead, indium, and selenium will burn blue. For blue-green, see above.

  • Pesticides. Arsenic is found in pesticides and used to be found in rat poison. However,as people become more aware of the toxicity of Arsenic, it is less commonly used.
  • Electrodes in your car battery. These contain lead.

Purple

You can burn potassium to create a purplish, pinkish flame.
  • Fertilizer.







Monday, December 21, 2015

What would happen if we turned the oceans into one giant ice rink?

[Note: Please do not try this at home. Consider trying this at your friend's house instead.]

How much energy would be released from the water?

A visual representation of the main concept of this blog post, added because rigorous and extensive studies conducted on Mr. Melby have prooved that he is more likely to read a blog post if it contains pictures. Image courtesy of Kelly Chen.
 The first thing we need to specify is the thickness of the ice. The NHL uses 0.75" thick ice at 16 degrees Fahrenheit (or, as their website says, "approximately 3/4" of an inch thick"), but their ice rinks sit on top of concrete, not water. Other websites, such as the Minnesota DNR, recommend 4" of clear ice (or 8" of white ice, which contains air bubbles that make it considerably weaker) over a lake for an activity like ice fishing. Using this information, I decided that freezing the top 10 cm of the ocean would create a layer of ice sufficient for ice skating. Since ice is less dense than water, 10 cm of water would actually create slightly more than 10 cm of ice. If we assume that the ice created is pure and clear (i.e. no air bubbles, salt, etc.), we can calculate the thickness of ice that would be formed. According to the 86th edition of the CRC Handbook of Chemistry and Physics, the density of water at 0 degrees Celsius and atmospheric pressure is 0.9998 g/cm^3, while that of ice under the same conditions is 0.9167 g/cm^3. This means that the volume of ice is 0.9998 g/cm^3 / 0.9167 g/cm^3 = 1.091 times that of water, so 10 cm water * 1.091 = 10.91 cm, or 4.294" ice. This should be (more or less) enough to make a decent ice rink.

Now that we've decided how thick our ice needs to be, we can figure out the total volume of seawater that we need to freeze to create it. If we know the radius of the Earth, we can use the formula for the volume of a sphere to calculate the volume of this "shell" of water. However, there's a problem: since the Earth is not perfectly round, its exact radius depends on where you measure it. According to NASA, the Earth's equatorial radius is 6378.1 km, while its polar radius is only 6356.8 km. Rather than use either of these values, I decided to use NASA's value for the Earth's volumetric mean radius, which is 6371.0 km. (Of course, this assumes that the radius of the Earth's oceans is approximately equal to that of its landmasses.) If the outer radius of our shell of ice is 6371.0 km, then its inner radius is 6371.0 km - 10 cm = 6370.9999 km. We can find the volume of the ice shell by subtracting the volume of the inner sphere from that of the outer sphere, so since the volume of a sphere is 4/3 * pi * radius^3, the volume of the shell is 4/3 * pi * outer radius^3 - 4/3 * pi * inner radius^3 = 4/3 * pi * (6371.0 km)^3 - 4/3 * pi * (6370.9999 km)^3 = 51 006.4 km^3. However, we must compensate for the fact that the Earth is not completely covered in water. According to the USGS Water Science School, approximately 71% of the Earth's surface is covered in water, so the actual volume of our ice shell would be 51 006.4 km^3 * 0.71 = 36 214.544 km^3, or 3.621E19 cm^3.

Now that we know the volume of seawater we need to freeze, we can find the total mass of the seawater by multiplying volume by density. The ocean's density varies with temperature and salinity, but it has an average density of 1.027 g/cm^3, so the seawater's total mass is 3.621E19 cm^3 * 1.027 g/cm^3 = 3.719E19 g seawater.

The exact mechanics of phase changes in solutions are not well understood at this time, so let's simplify the problem: we can get a pretty good approximation of freezing seawater by ignoring all of the salt in it and assuming that only the water molecules in the solution actually undergo the phase change. To find the mass of water in this amount of seawater, we need to know the salinity of the seawater itself. Since seawater is around 3.5% NaCl (the mass of the other ions, algae, fish poop, etc. in it is negligible, so here, I am assuming that seawater contains only water and NaCl) by mass, it is 100% - 3.5% = 96.5% water by mass. Therefore, the mass of water that we must freeze is 3.719E19 g * 0.965 = 3.589E19 g water.

The surface temperature of the ocean varies with latitude, but as its average surface temperature is 17 degrees Celsius, I will assume that all of our water is at this temperature. Now, in order to freeze it, we must first lower its temperature to its freezing point and then allow it to undergo the phase change itself. The freezing point of pure water under normal conditions is 0 degrees Celsius, but the addition of salt (or any other solute) produces a phenomenon known as freezing-point depression, so the freezing point of seawater would actually be slightly lower than that of pure water. As it turns out, seawater that is around 3.5% salt by mass actually freezes at -1.94 degrees Celsius.

The total heat released by the water as it freezes is equal to the amount released as we lower the temperature of the water to -1.94 degrees Celsius plus the amount released as the water freezes. We can use two equations to model this scenario: Q = m * C * delta-T represents the change in heat of a system as the temperature changes, while Q = n * delta-H_fus represents the change in heat of a system as a substance melts or freezes. (In these equations, Q represents heat flow, m represents the mass of the substance undergoing a Wha change in temperature, C represents the specific heat of that substance, delta-T represents the change in temperature (i.e. final temperature - initial temperature) that occurs, n represents the number of moles of the substance undergoing a temperature change, and delta-H_fus represents the heat of fusion of that particular substance. However, as the value of delta-H_fus used in this calculation is given in J/g, not J/mol, n is replaced by m here.)

Although the specific heat of a substance changes slightly as temperature changes, I will be using C = 4.184 J/(g*degree Celsius) here, as this is the value listed for water at 17.00 degrees Celsius (although C changes slightly with temperature, this inaccuracy will be negligible for our calculations). Our change in temperature here is -1.94 degrees Celsius - 17 degrees Celsius = -18.94 degrees Celsius. The heat of fusion of water at 0 degrees Celsius is 333 J/g; however, as this describes the amount of energy absorbed when water melts and we want the amount of energy released when it freezes, the value of delta-H_fus that we will use is -333 J/g (i.e. a value of equal magnitude but opposite sign). Thus, the enthalpy (i.e. heat) change produced by lowering the temperature of our 3.589E19 g of water is m * C * delta-T = 3.589E19 g * 4.184 J/(g*degree Celsius) * -18.94 degrees Celsius = -2.844E21 J, while that produced by actually freezing it is m * delta-H_fus = 3.5898E19 g * -333 J/g = -1.195E22 J. Our total enthalpy change is simply the sum of these two values, or -2.844E21 J + -1.195E22 J = -1.480E22 J. Thus, turning the oceans into a giant ice rink would release 14 800 000 000 000 000 000 000, or almost fifteen sextillion, joules of energy from the water!

How much energy is fifteen sextillion joules, really?

To put that huge number into perspective (somewhat), freezing the surface of the ocean would release as much energy

What would releasing all that energy do?

Long story short, we'd probably all die very quickly thereafter. (Thereafter, hereafter... Meh, same thing, really, in this case.)

But to elaborate on our impending doom, let's assume that the phase change is near-instantaneous.
All of the heat that we just released from the water has to go somewhere-- into the surroundings. This includes both the rest of the ocean underneath the ice rink and the atmosphere above it. A warmer ocean would negatively impact aquatic ecosystems, change global weather patterns, and result in higher sea levels, among other things. As you can imagine, this would exacerbate many of the issues already caused by global warming, such as the development of more powerful storms, destruction of cities and farmland due to flooding, loss of habitat, erosion, coral bleaching (from loss of algae), increased spread of invasive marine species and diseases, extinction, and polar ice shelf collapses. Well, that seems like a pretty bleak outcome.

What about the atmosphere?

The specific heat of air, at just over 1 J/(g*degree Celsius), is quite a bit smaller than that of water. This means that adding the same amount of energy to both will increase the temperature of the air more. Regardless, releasing so much energy from the surface of the oceans would definitely increase the temperature of the atmosphere by a pretty significant amount, a change that would also be quite disastrous to the planet. For example, the rate of photosynthesis increases with temperature until a certain point, after which it drops down rapidly to zero. So, if we were to heat up our atmosphere a little bit too much, almost every biome on Earth would break down as the enzymes required for photosynthesis became denatured. Not surprisingly [citation needed], this would have some rather serious [citation needed] implications not only for our own species, but also for pretty much all others on the planet.

However, what we haven't considered yet is that if we assume that no (or very little) heat escapes from the outer edge of the atmosphere into space, we are essentially considering an isolated system. This means that there would be no difference in total amount of energy before and after the phase change, so once the oceans return to thermal equilibrium, a process that begins to occur immediately, we would end up right where we started. This makes it rather difficult to judge the effects of heating up the rest of the ocean, as well as the atmosphere, because both temperatures start to return to normal fairly quickly (although, to be fair, transferring so much energy back into the ice may take a little while). However, it is probable enough that at least some of the many serious consequences of pulling such a stunt would actually occur that most people (a possible exclusion to this statement can be found here) would decide not to do so.

But if you were to try this and we didn't all die off as a result of it first... well, then that just might be a hack cool* enough to get you into MIT. And I do hear that people are looking for ambitious risk-takers [citation needed] these days...

*Pun unintended but noted.

Sunday, December 20, 2015

AstroMELBical Proportions

"What if all the atoms in your body were MELBiUM atoms?"
     - Anonymous Asker

That's a fine question, stranger! What WOULD happen if every one of the atoms in your body was replaced with a MELBiUM atom? To answer this, we have to look at the implications at several different levels.

1. Physical Implications

The most obvious consequence of being made of MELBiUM is a severe increase in weight- as the molar mass of MELBiUM is defined to be exactly one mole, we can calculate the mass (in grams) of your body to be equal to the number of atoms in your body. According to the Thomas Jefferson National Accelerator Facility, the average 70 kg human body has approximately 7E27 atoms. This gives us a body weight of 7E27 g, or 7 septillion kilograms. Fun comparisons, please:

  • 7 septillion kg is approximately equal to 1.17 Earths!
  • 7 septillion kg of water is enough to grow 496 sextillion pounds of tilapia, and that many kg of food can feed those tilapia for 57 days!
Ok, now that we have a sense of scale, what exactly would happen if you weighed more than the entire earth? Surely you would collapse into a black hole because of the sheer density of your body, right?

The ability of an object to collapse into a black hole is determined by the Schwarzschild radius, or the radius by which light can no longer escape the gravitational field of an object. The radius is determined by mass alone, and the equation r = 2GM/c^2 gives our MELBiUM body a Schwarzschild radius of 10.36 millimeters. Well, unless you happen to have the volume of a 2x2x2 Lego brick, that's not happening. It's close, though- only a few orders of magnitude off.

So, your body wouldn't instantly collapse into a black hole. That's disappointing. However, the sheer density of your body would still wreak havoc.

The densest naturally occurring substance on Earth is Osmium, element number 76, weighing in at 22.59 grams/cm^3. That's not even close to what the density of our MELBiUM man is- assuming an pre-MELBiUM average density of 1.05 g/ml and weight of 70 kg, our new density would still be 1.05...E20 grams/cm^3. That puts Osmium to shame.

The effects of having an object with the mass of 1.17 Earths ON Earth is not well-documented so I won't go into too much detail on that. Needless to say, the Earth would change a lot.

2. Molecular Implications

If your body was entirely composed of MELBiUM its bonds would change as well. The closest element we can use to estimate the properties of MELBiUM is Iodine (element 53), as the properties of Astatine are quite hard to determine and have also been estimated using Iodine.

Let's first take a look at how MELBiUM bonds. Most elements can only bond to as many elements as the number of valence electrons they have, or eight minus that number for nonmetals. Iodine, however, (which is in this case analogous to MELBiUM) and most nonmetals beyond Neon can have what's called an expanded octet. This is when the extra electrons occupy the next electron sub shell, generally the d orbital. The existing s and p orbitals hybridize with the d orbital and the electrons occupy an energy level that is in between that of the three hybridized orbitals.


See this molecule for example: the Iodine in the center is able to bond to four Chlorine atoms and have two additional lone pairs, for a total of 12 electrons. It exhibits dsp^2 hybridization.


Use this handy dandy chart to determine hybridization type!

So, based on the properties of Iodine we can extrapolate and assume that MELBiUM will also exhibit this hybridization.

What now? Well, let's take a look at the most common compound in your body: dihydrogen monoxide, or hydrogen hydroxide, or hydroxic/hydric/hydroxilic/hydroxyl acid, or oxidane, or H2O, or water!


Water's pretty important. As in, it makes up 60% of your body. Here's an example of what it would look like if the atoms were MELBiUM:
Source: ME!!! I'm so proud of myself :)

It is technically possible to manipulate MELBiUM into any sort of organic molecule we might encounter, the extreme instability of the molecule would force it apart with the slightest disturbance. In short, your molecules would explode. You would become a ball of MELBiUM, held together by your own gravitational force, and not... strictly human.


Source: the indefatigable Kelly Chen

3. Atomic Implications

Insofar, we have made a pretty generous assumption: MELBiUM is an element that exists and is stable. Ha.

Let's continue assuming that MELBiUM exists, and for this article's sake let's have some fudged article on how MELBiUM actually exists on an island of stability. What would it look like, anyway?


Here's a grossly simplified view of an atom. There are protons, neutrons, and electrons; the protons and neutrons form the nucleus at the center while the electrons whiz about the nucleus in certain patterns.

The spaces that you will most likely find a particular electron are called orbitals. Don't get confused- the electrons are orbiting the nucleus, but they are not doing it in a specific or even continuous path. The orbitals only describe probabilities, nothing more; electrons are apt to teleport around everywhere so determining exact positions is pretty much impossible, as given by Heisenberg and Schrodinger in their eponymous principles.

One interesting effect due to the random distribution of electrons in an atom is that at a given moment, there are generally more electrons on one side of the atom than the other. This creates a very small, instantaneous dipole moment, which can then induce other nearby atoms to align charges and create attraction between them. This inter-molecular force or IMF is called Melbon- I mean, London Dispersion Forces.


London Dispersion Force

Whew, that was some hardcore knowledge. The point is that the more electrons in an atom, the more it tends to have greater dipole moments, as there is a greater overall chance that the electrons are more concentrated in one area. MELBiUM, with 117 electrons, would have the strongest London Dispersion Forces of any known element.

This means, on an atomic level, the lump of MELBiUM that you have become will be very melcissistic- that is, it will be strongly attracted to itself, and therefore have a very high boiling point. This isn't even taking into account the unique property of MELBiUM- its massiveness. While gravity is negligible in normal inter-molecular (or inter-atomic, in this case) attraction, we need to factor it in for MELBiUM.

The equation for the attraction between two objects due to gravity is given by:

F(grav) = (G * m(1) * m(2)) / d^2

Where G is the gravitational constant 6.673E-11 N*m^2/kg^2. Assuming that the atoms of MELBiUM stay the same distance apart as in a normal atom (again using Iodine as a convenient approximation), 266.6 picometers, we get F(grav) = (6.673 x 10^-11 N*m^2/kg^2 * 0.001 kg * 0.001 kg) / (1E-12)^2 = 66730000 (67 billion) newtons of force! That's enough to break 4390 ft of solid brick, and that's just for a single atom! To overcome the gravitational attraction of our MELBiUM man and sublimate him, we'd need around 467 decillion newtons O.O

This means that MELBiUM would be extremely difficult to change the state of. Even though it's sublime, MELBiUM gas would be incredibly hard to produce.

Conclusion

Well, first of all, you'd most certainly be dead. I mean seriously, you just turned into a giant ball of an element that has nothing to do with life as we know it. What do you expect?

After your rather untimely death, the pile of MELBiUM formerly known as you would attract and be attracted to the Earth and they would merge together. The denser and harder MELBiUM would probably be enveloped by the less dense Earth and reside somewhere in the middle of the Earth, leaving a gigantic scar where the MELBiUM has sunken into. The Earth's orbit around the Sun would most likely change as well- the weather and the seasons would never be the same again. The increased mass would alter the orbit of Earth to make it more elliptical and alternate between a habitat that is much too hot to sustain life and one that is much too cold. If those engineers don't start building those bunkers yet, humans and all of live would be screwed.

But then again, imagine the epic feeling of emerging from a bunker after half a year of scorching, inhospitable weather to enjoy a few days of spring before the Earth strays too far away and ends up becoming a popsicle. Sounds rather romantic, doesn't it? (BTW that idea is hereby copyrighted for a future book or something)

-Evan