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The s-process, short for "slow process", is one of two main ways that elements heavier than iron are formed inside of stars. The other process is the r-process, short for "rapid process". Both processes are endothermic and rare, but they take place in very different situations.

Up to the elements of Iron and Nickel, stellar nucleosynthesis is a process of fusion of whole nuclei, and it releases energy. Since iron or nickel is the most stable nucleus, further fusion is energetically unfavorable. So heavier elements are formed by neutron bombardment of iron and nickel. This requires having a source of neutrons, which is another story in itself. And this happens slowly, meaning that the nucleus (usually) undergoes some type of radioactive decay between absorbing neutrons.

An atomic nucleus, for various reasons, has to maintain a balance of protons and neutrons. If it has too many protons, it will emit a positron, transforming a proton into a neutron. Too many neutrons, it emits an electron, turning the neutron into a proton. In the s-process, when the nucleus absorbs a neutron, it will decay (over a time period of anywhere from seconds to hundreds of thousands of years) into an element with a higher atomic number. It then, after another few thousands or millions of years, is impacted by another neutron. It can take a long time for an element to slowly gain nucleons and atomic number this way.

Even this slow process requires a very large, energetic star. The s-process is most common in stars that already have a high metallicity, and that have high temperatures: either blue giants or red giants. Both of these types of stars are rare. But they are still much more common (and much longer lived), than supernovae, the site of the r-process. Although I have tried to find numbers on it, there does not seem to be good data on which source, r-process or s-process, is more dominant in the formation of various heavy elements. Given the rarity of such stars, and the difficulty of modelling the inside of stars, all of the details of the s-process are something that our science can't currently tell us, even though the theoretical process is fairly clear.

AKA wastebin taxon, dustbin taxon, rag bag taxon, trash can taxon, or catch-all taxon.

'Wastebasket taxon' is an informal but common term for the practice of using an official taxon as an easy place to dump unclassified species.

As a clear example of this, most snakes are placed in the family Colubridae not because they belong in a family together, but because at one point it was recognized that the taxonomic tree of snakes was so messy that it would be most wise to ignore the mess and hope that future generations would sort things out. Other classic examples include the order Insectivora, although it has since been dissolved, and the superclass Agnatha, which is in the process of being resolved.

You may also find less formal wastebasket taxons, as in the infamous archaic H. sapiens, which is essentially an incertae sedis used to avoid having to specify where Neanderthals sit in relation to modern Homo sapiens.

Electronegativity is the tendency of some atoms to attract electrons more strongly than others. This is a simple yet profound concept, of huge importance in chemistry, which is tragically cursed with an intimidating eight-syllable name. I'm almost sure the unwieldiness of the term is the whole reason it gets left out of chemistry courses up to GCSE level even though plenty of things make far more sense once you start to get your head round it.

Oxidation

A great deal of chemistry relates to the way that electrons interact with atoms. Oxygen, for example, gets all its powers from the fact it's so attractive to electrons. This is why things burn in oxygen, why we're able to use oxygen to get energy from food, why oxygen corrodes metals and so on. In every case, it's because oxygen is an electron-hog: it's electronegative, to use the technical term. Grabbing on to electrons so tightly releases energy. Speaking of technical terms, when modern chemists talk about oxidation, what they really mean is that something is coming along and taking electrons. By the time chemists realised that lots of other things besides oxygen were also good at doing this, the name had already stuck. In any case, oxygen really is particularly good at hogging electrons; the only element that's more electronegative is fluorine.

Metals

By contrast, some elements are terrible at holding on to electrons. Their electronegativity is so low they count as electropositive. These elements are all metals, and the properties we associate with metals are all related to the way they hold onto their electrons rather loosely. They conduct electricity because some of their electrons aren't particularly attached to any one atom, flowing freely between them instead. This also allows metals to conduct heat rather well, high-speed electrons carrying heat energy rapidly through the metal. These free-flowing electrons hold the atoms of a metal together like wet glue, which is why metals are so malleable.

Metal atoms can break away from that structure by getting free of that electron glue. That means they have to form a positive ion, which usually means something else needs to come along and take at least one electron away. That could be a hydrogen ion from an acid, or it could be an electrode, for example. The most electropositive metals, like the alkali metals, only need the slightest nudge to lose an electron, which is why they're so extremely reactive. Ordinary water provides enough hydrogen ions for them to dump masses of electrons very quickly. The hydrogen escapes as gas, leaving behind a powerful alkaline solution, and the reaction produces large amounts of heat.

The fact that some elements are more attractive to electrons than others is the principle that batteries are based on. Put two materials in a conductive solution, with a wire allowing current to flow between them, and the more electropositive substance will send electrons down the wire and ions into the solution, completing a circuit.

Non-metals

Non-metals are elements that don't lose electrons easily. The more reactive ones are good at grabbing electrons from their surroundings, forming negative ions. Ionic bonding is when positive and negative ions come together to form crystals.

Non-metals can also bond together by sharing electrons, forming a covalent bond. If one of the atoms involved in a bond is more electronegative, the electrons are shared unevenly. The electronegative atom pulls the electron cloud towards itself, making the bond polar. Compounds with polar molecules behave more like ionic compounds than non-polar compounds do, because of that uneven distribution of charge: they tend to have higher melting and boiling points, because the opposite poles of nearby molecules attract each other. That's why water is liquid up to 100°C, even though it's just made of oxygen and hydrogen, each of which boils at temperatures hundreds of degrees lower than that on their own. Polar substances, including ionic compounds, tend to mix together, as do non-polar substances, but each tends not to mix with each other.

Trends in the Periodic Table

The reason that some atoms are more attractive to electrons than others has to do with how strong the positive charge is in their nucleus, how far from the nucleus their outside shell of electrons is, and how many other electrons are in the way. Electrons arrange themselves in layers around atoms, you see, and the top layer (the valence shell, or outside shell) is what does most of the chemistry. Going down a row in the periodic table means adding another layer of electrons, each of these shells being further out than the last. The further the electrons get from the nucleus, the weaker their attraction to it. That makes the metals more reactive, since they react by losing electrons, while the non-metals get less reactive. Lithium, the first of the alkali metals, fizzes gently when you put a lump of it in water; sodium, one row down, bubbles furiously, sometimes catching fire; potassium immediately bursts into purple flames; rubidium explodes; caesium is just nuts. The trend in the halogens (Group VII) goes the other way: fluorine is so good at poaching electrons that it reacts violently with almost anything, even at room temperature; chlorine is corrosive, and toxic to all life; bromine is still downright scary; whereas iodine is toxic enough to disinfect wounds, but not so toxic that doing so is a really terrible idea. Because all of these elements are so reactive, they are usually found as ions, which are much safer.

As you go across the periodic table, each element has one more proton than the last to draw the electrons in, and one more electron to balance it, but the new electrons are added to an existing shell, so they don't get any further out. In fact, thanks to the stronger charge on the nucleus, its attraction to electrons gets stronger and each electron shell gets even closer. Lithium, at the start of the second row, only has three protons, and the two electrons in its first shell get in the way of the attraction to the one on the outside. That makes lithium pretty electropositive. Near the other end of that row, fluorine has nine protons, so the force between that and the electrons in its second shell is far greater. Right at the end of the row is neon, wich ruins the pattern because, like the other noble gases, its outside shell is already full. It does hold on very firmly to the electrons it's already got, but it's got no space for any new ones.

So electronegativity, with its deceptively simple definition, draws together and helps explain redox reactions (reduction and oxidation), conductivity, the reactivity series, electrochemistry, acidity, ionic bonding, miscibility, periodicity and trends in the periodic table. Maybe it deserves those eight syllables after all.

Note that many authors prefer to discuss some of these ideas in terms of the related concepts of electrode potential and ionization energy, rather than tying everything together like this.

Two substances are miscible if they are capable of mixing. It's not clear why we don't just say 'mixable', which is easily understood, doesn't sound like 'missable', and has been a word since at least the seventeenth century, but there you go. English is silly. Probably someone thought the Latinate version sounded fancier. My money is on 'mixable' displacing it in the next hundred years or so.

The word is usually applied to liquids, since all gases are miscible with each other, while no solids are capable of mixing in the same way. If a solid or gas is miscible with a liquid, we usually say it's soluble, instead, but apart from the change of state it amounts to much the same thing. Sometimes we talk about liquids dissolving in each other, too. When liquids aren't miscible they are said to be immiscible (or unmixable), which happens when the molecules of each prefer their own company, usually because one of the liquids is polar while the other is not. For example, water molecules are quite strongly attracted to each other by hydrogen bonding; oil molecules are quite strongly attracted to each other by London dispersion forces. Neither one is much attracted to the other because oil molecules, being non-polar, are immune to hydrogen bonding, while water molecules are too small to be much moved by London dispersion forces.

If both liquids are polar, all their molecules are attracted to whichever poles they get near; if they're non-polar, they're attracted to each other just as indiscriminately. Some liquids have molecules that are only partially polar, like acetone and alcohol, and these are attracted to both polar and non-polar molecules, so they tend to mix at least a bit with liquids of either kind. This can get a bit complicated when you have three or more liquids all together: one way to test for oil in food is by soaking the food in alcohol to dissolve the oil, then adding water to the mixture. If it turns cloudy, you know there's oil, or at least some kind of lipid: whereas pure alcohol dissolves nicely in water, when it's mixed with oil it loses its solubility. That means it forms an emulsion with water, tiny droplets separating out and scattering light. Ouzo does something similar when you dilute it, thanks to the essential oils that give it its flavour.

An emulsion is the closest you can get to a mixture of two immiscible liquids. To form a stable emulsion, you need some kind of emulsifier - something that's attracted to both liquids. This is the basis of soap: you can't just rinse oily stuff off your hands, pans and clothing, but if you can turn the oil from a layer into an emulsion, the droplets rinse away easily. Emulsions are important in the kitchen, too. A salad dressing of oil and vinegar alone will quickly separate into layers, but a bit of mustard added to the mix helps it stay emulsified. Similarly, the lecithin in egg yolk allows mayonnaise to be a stable emulsion. Milk is a natural emulsion, and stays as such when you turn it into cream or butter.

Galvanic corrosion occurs when dissimilar metals are in electrical contact in the presence of an electrolyte. Corrosion of the more noble metal is inhibited, while that of the less noble is accelerated.

This is explained by the different electrode potentials of different metals. Lower-nobility metals, having lower electrode potential, act as an anode, attracting electrons, dissolving into the electrolyte, and depositing on the more noble metal (the cathode). The rate of dissolution depends on the difference of nobility: the electromotive force of such a reaction is defined by the potential of the anode subtracted from that of the cathode.

The galvanic series arranges metals and semi-metals by their electrode potential in Earth's most common electrolyte--seawater. Examples of more noble metals include graphite, gold, and silver; lower-nobility metals include aluminum, zinc, and magnesium.

Zinc in particular is often sacrificed to control or exploit galvanic corrosion. Cheaper household batteries, or galvanic cells, generate voltage via the rapid dissolution of zinc relative to manganese oxide within an alkaline solution. Rechargable batteries utilize metals, such as lithium, that can be re-constituted with reverse current (the imperfection in this process partially explains why rechargeable batteries develop "memory.") Submerged and buried metal structures usually feature large zinc anodes; one example is the zinc rod mounted to the underbelly of a boat. Likewise, the zinc plating on galvanized screws and bolts lengthens the life of the underlying, stronger steel.

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