Materia y sistemas materiales

Materiales

Clases y propiedades

Haremos en primer lugar la distinción entre Objetos y Clases de materiales. Un objeto, tal como un ser humano, una mesa, un tirador de latón de una puerta, una planta, entre otros, puede estar formado por una o varias clases de materiales. El químico se interesa principalmente no por los objetos en sí, si no por la clase de material del que están compuestos. Estudia la aleación de latón, ya sea en un tirador de una puerta o en cualquier otro objeto de latón, y su interés se dirige sobre todo a aquellas propiedades del material que son independientes de las características particulares de los objetos que lo contienen.

Las propiedades de los materiales se pueden clasificar en:

Propiedades Extensivas: Dependen de la cantidad de material que se considere. Si un recipiente contiene un litro de alcohol y otro diez litros de alcohol, es posible comprobar que la cantidad de alcohol del segundo recipiente tienen mayor masa y volumen que la del primero. Esto significa que la masa y el volumen de una cierta cantidad de material dependen de dicha cantidad; por lo tanto son propiedades extensivas, como lo son también el peso y la capacidad calorífica, por ejemplo.

Propiedades Intensivas: No dependen de la cantidad de material que se considera. Dos trozos de hierro de distinto tamaño tendrán distinta masa y distinto volumen, pero tendrán el mismo color, el mismo PF, el mismo PE. Estas propiedades son, por la tanto, intensivas, pues no dependen de la cantidad de material considerado.

Otras propiedades intensivas de los materiales son: el brillo, la dureza, la forma cristalina, el índice de refracción, la densidad, el peso específico, la solubilidad. En ciertos casos las propiedades intensivas pueden ser expresadas numéricamente, como pasa con el PF, PE, densidad o el peso específico. Estos valores numéricos se denominan Constantes Físicas del material.

Un tipo particular de propiedades intensivas son aquellas que podemos describir con nuestros sentidos como el color (con la vista), el olor (con el olfato), la textura (con el tacto) y el sabor (en nuestra materia el sabor nunca debe determinarse, salvo que se esté absolutamente seguro que el material en cuestión no es tóxico o corrosivo). Estas propiedades se denominan Organolépticas.

Sistemas Materiales:

Se llama sistema material a toda porción del universo que se aísla, real o imaginariamente, para su estudio.

Son ejemplos de sistemas materiales: un trozo de mármol, agua y aceite contenido en un recipiente, gas en el interior de un neumático, una célula contenida en porta – objetos de un microscopio.

Los sistemas materiales se clasifican en dos grandes grupos:

Sistemas Homogéneos: Si analizamos las propiedades intensivas de una muestra de agua (punto de ebullición, punto de fusión, densidad o viscosidad, por ejemplo) veremos que ellas permanecen constantes para cualquier porción de agua que se considere. Lo mismo sucede, por ejemplo, con una porción de cloruro de sodio (sal común).

Si ahora disolvemos cierta cantidad de sal en agua, obtenemos un sistema denominado solución; podemos comprobar que para el sistema material así obtenido, las propiedades intensivas son las mismas en todos los puntos, pero diferentes a las medidas para el sistema formado solamente por agua y para el sistema formado por cloruro de sodio sólo. Decimos entonces que el agua, el cloruro de sodio y la solución de cloruro de sodio en agua constituyen sistemas homogéneos.

“Sistemas Homogéneo es aquel que presenta las mismas propiedades intensivas en todos sus puntos”

Todo sistema homogéneo se caracteriza por presentar continuidad cuando se lo observa a simple vista, al microscopio y aún al ultramicroscopio. Por ejemplo, con ninguno de estos instrumentos es posible distinguir la sal del agua cuando se observa la solución, el sistema se observa como un todo homogéneo. Otros ejemplos de sistemas homogéneos: muestras de azufre, yodo, alcohol, alcohol yodado, el aire puro y seco, entre muchos otros.

Sistemas Heterogéneos: Si analizamos un sistema constituido por agua y nafta, comprobaremos que no constituyen un sistema homogéneo a simple vista, la nafta se presenta como una capa definida por encima del agua, también podemos comprobar que otras propiedades intensivas, además del color, como por ejemplo la densidad, no se mantienen constantes cuando pasamos de una porción ocupada por el agua a otra ocupada por la nafta.

La madera, con anillos alternativos blandos y duros, es evidentemente un material no homogéneo, así como el granito, en el cual pueden verse granos de tres especies que difieren en el color, correspondientes a los minerales cuarzo, mica y feldespato.

Los sistemas analizados constituyen ejemplos de sistemas heterogéneos:

es aquel que presenta por lo menos una propiedad intensiva diferente en al menos dos de sus puntos

Fases de un sistema material:

Un sistema material heterogéneo puede describirse en función de las fases que lo constituyen.

“Una fase, es una parte homogénea de un sistema, separada de las otras partes por límites físicos”

Esta zona que separa las fases de un sistema heterogéneo se denomina superficie de discontinuidad ya que en ella varían bruscamente las propiedades intensivas. El sistema formado por agua y nafta es un sistema heterogéneo formado por dos fases: agua y nafta.

Las propiedades de los Sistemas dispersos, y también su estabilidad, dependen del tamaño de las partículas dispersas. Si éstas son muy grandes, los sistemas dispersas son inestables y en poco tiempo se produce la separación de las fases. Por ejemplo: en una dispersión de arena y agua la fase sólida se deposita rápidamente; si la dispersión es de partículas de aceite en agua, la fase dispersa acaba por sobrenadar sobre el agua, por tener una menor densidad.

Para expresar las dimensiones de las partículas dispersas, se utiliza la unidad denominada “micrón” (µ), 1 micrón equivale a 10-6 m ó 10-3 mm es decir: 1 μ = 10-6 m = 10-3 mm.

Según el grado de división de las partículas dispersas, las dispersiones heterogéneas como las homogéneas, reciben la siguiente se clasificación.

Las dispersiones heterogéneas pueden ser:

Groseras o macroscópicas: Son sistemas heterogéneos que se caracterizan porque la fase dispersa puede ser observada a simple vista o con una lupa. Las dimensiones de las partículas dispersas son mayores que 50 µ. Ejemplo: Talco y agua, azufre y limaduras de hierro, soda servida en un vaso.

• Finas: Son sistemas heterogéneos en los cuales la fase dispersa no es visible a simple vista, pero si lo es, observada al microscopio. Las dimensiones de las partículas dispersas oscilan entre 50 µ y 0,1 µ. Por ejemplo la leche se presenta a simple vista como un líquido blanco homogéneo, pero observada al microscopio resulta ser un sistema heterogéneo constituido por la dispersión de partículas de materia grasa en un medio líquido. Cuando hablamos de una dispersión fina, si ambas fases son líquidas, la dispersión se llama emulsión; si la fase dispersa es sólida y la dispersante es líquida, la dispersión se llama suspensión. Un ejemplo de suspensión es la tinta china, formada por pequeñas partículas de carbón dispersas en el agua, que se revelan al ser observado el sistema al microscopio.

Las suspensiones son frecuentes en la naturaleza. Las aguas de los ríos contienen partículas en suspensión que, al depositarse en los lugares donde la corriente es más lenta, forman sedimentos de arena, arcilla, materiales calcáreos entre otros materiales arrastrados por ellos.

Coloidales y soles: Son sistemas heterogéneos cuya fase dispersa posee un alto grado de división y solamente es visible al ultramicroscopio. Este aparato se diferencia fundamentalmente del microscopio óptico común ya que en él la luz no incide directamente sobre las partículas sino en forma lateral. Así observadas las partículas dispersas se aprecian como puntos luminosos debido a la luz que difunden. Este fenómeno de difusión de la luz se llama “Efecto Tyndall”, y es observable cuando un rayo de luz penetra en una habitación a oscuras o en penumbras: las partículas de polvo atmosférico son visibles como puntos luminosos.

Son ejemplos de dispersiones coloidales: la gelatina, el agua jabonosa, la clara de huevo en agua. Las partículas de la fase dispersa reciben en esto caso el nombre de micelas, y sus dimensiones oscilan entre 0,1µ y 0,01µ. Las micelas se mueven en el seno de la fase dispersante en forma desordenada, con gran rapidez y en zig-zag (movimiento browniano). Dada su pequeñez, pueden atravesar los filtros comunes,

Las dispersiones coloidales más comunes son los “hidrosoles”, en los que la fase dispersante es el agua.

Soluciones. Cuerpos puros y sustancias

Las soluciones son sistemas homogéneos formados por dos o más componentes. Por ejemplo el aire es una solución de gases cuyos componentes principales son nitrógeno (N2) y Oxígeno (O2). Los gases, por estar las partículas que los constituyen (moléculas) muy alejadas entre sí, siempre, cuando se mezclan, forman soluciones, es decir, sistemas homogéneos.

El alcohol que usamos habitualmente para desinfectar heridas, es una solución líquida cuyos componentes son etanol (C2H6O) y agua.

Cuando a un volumen determinado de agua le agregamos azúcar, es posible observar como el azúcar “desaparece” al mezclarse con el agua y se obtiene un sistema homogéneo líquido incoloro que sabemos no es agua, porque su sabor es más dulce. Se forma una solución en estado líquido, de azúcar en agua, compuesta por dos componentes: azúcar (sólido) y agua (líquido).

Cuando a un volumen determinado de agua le agregamos sal, es posible observar, al igual que en el caso anterior, cómo la sal “desaparece” al mezclarse con el agua y se obtiene un sistema homogéneo líquido incoloro que sabemos no es agua, porque su sabor es salado. Se

La solución de sal en agua, como todas las soluciones formadas por agua y por sal, son sistemas homogéneos, pero mientras la solución de sal en agua puede fraccionarse, la sal y el agua no pueden hacerlo por aplicación de ningún método de fraccionamiento. Esta diferencia de comportamiento, que ilustramos mediante un ejemplo, permite clasificar a los sistemas homogéneos de la siguiente manera:

Soluciones: “Son sistemas homogéneos fraccionables por la aplicación de algún método de fraccionamiento, a partir del cual se obtienen sus componentes”

Cuerpos puros: “Son sistemas homogéneos no fraccionables por la aplicación de todos los métodos de fraccionamiento conocidos”

La aplicación sucesiva de métodos de separación y de fraccionamiento de fases permite obtener un conjunto de cuerpos puros a partir de un sistema heterogéneo.

Si tenemos dos sistemas que son cuerpos puros y medimos, en las mismas condiciones de presión y temperatura, las propiedades intensivas de ambos sistemas, si comprobamos que todas las propiedades intensivas coinciden, podemos decir que ambos cuerpos puros están compuestos por la misma sustancia. Las sustancias componen a los cuerpos puros, a las soluciones y a las fases que constituyen un sistema heterogéneo:

“Si dos cuerpos puros presentan las mismas propiedades intensivas, medidas en las mismas condiciones de presión y temperatura, significa que están compuestas por la misma sustancia”.

Los sistemas materiales agua e hielo, son dos sistemas homogéneos no fraccionables, son cuerpos puros. Estos cuerpos puros son diferentes, ya que presentan diferentes propiedades intensivas (como por ejemplo: la densidad o el peso específico), además de estar en distintos estados de agregación. Sin embargo, ambos están compuestos por la misma sustancia: agua. Esto se comprueba porque si se miden, en las mismas condiciones de presión y temperatura, las propiedades intensivas de ambos sistemas, estas coinciden.

Los componentes de un sistema material son las sustancias que componen dichos sistemas, que pueden ser homogéneos (solución o cuerpo puro) o heterogéneos.

No deben confundirse los términos “constituyentes” – que expresa las fases que constituyen un sistema heterogéneo – con “componentes” – que expresa las sustancias que componen un sistema homogéneo (solución o cuerpo puro) o heterogéneo.

Elemento químico

Las sustancias simples diamante y grafito están compuestas por Carbono. Las propiedades físicas y químicas de estos sólidos difieren notablemente, de modo que deben ser considerada sustancias simples diferentes compuestas por Carbono, que se presentan en el mismo estado de agregación. Las sustancias que mantienen entre sí este tipo de relación, se denominan “variedades alotrópicas”. A diferencia del agua y del hielo (una misma sustancia en distinto estado de agregación), el grafito y el diamante son sustancias simples diferentes, en igual estado físico (sólido), constituidas por el mismo elemento: Carbono.

La diferencia en la estructura cristalina que presenta el diamante y el grafito, explica la particular dureza y densidad del diamante, y la blandura, poder lubricante y alta conductividad eléctrica del grafito. En otros casos como el Oxígeno y el ozono, que también son variedades alotrópicas del elemento Oxígeno, en este caso en el mismo estado de agregación (gaseoso), difieren en el número de átomos que forman la molécula.

En condiciones especiales de presión y temperatura, el diamante se puede convertir en grafito y viceversa, lo mismo ocurre con el Oxígeno y el ozono. Esta es otra característica de las variedades alotrópicas, en determinadas condiciones de presión y temperatura, pueden convertirse entre sí.

En los casos como, los del Fósforo y del Azufre que se presentan en la naturaleza con distintas estructuras cristalinas de la misma sustancia, no pueden ser consideradas variedades alotrópicas de estos elementos, sino que constituyen variedades polimórficas de los mismos.

El pasaje de una forma alotrópica a otra es una transformación química, puesto que una sustancia se transforma en otra.

El pasaje de una forma polimórfica a otra es una transformación física, puesto que una misma sustancia, en esta transformación, cambia de estructura cristalina.

Si consideramos las siguientes sustancias: diamante, grafito (sustancias simples), dióxido de carbono y carbonato de calcio (sustancias compuestas) podemos comprobar que todas tienen algo común en su composición, precisamente el elemento carbono. A partir de este ejemplo, y del conocimiento de otros, podemos dar la siguiente definición:

“Se llama elemento químico a lo común entre las sustancias simples, las variedades alotrópicas que pueden obtenerse a partir de ellas, y las sustancias compuestas que por descomposición total originan a las simples”

Elementos de la naturaleza

Los elementos conocidos en la actualidad son alrededor de 107. Algunos de ellos (cinco) fueron obtenidos sintéticamente en el laboratorio, los demás se encuentran en la naturaleza. Cada uno de ellos, forma sustancias simples que presentan propiedades diferentes. De la combinación de los elementos, resultan las sustancias simples y compuestas que forman todas las sustancias de origen inorgánico y orgánico que existen en el universo. Por lo tanto, los materiales se hallan constituidos por elementos químicos que forman las sustancias simples y las compuestas.

La abundancia de los elementos en la corteza terrestre, expresada en porcentajes de masa, es aproximadamente la siguiente: 50% de Oxígeno y un 25% de Silicio. Es decir las tres cuartas partes de la corteza terrestre están constituidas por Oxígeno y Silicio, y solamente un cuarto de la misma por el resto de los elementos.

Una composición más exacta es la siguiente:

Oxígeno: 49,5%

Silicio: 25,8%

Aluminio: 7,5%

Hierro : 4,7%

Calcio: 3,4%

Sodio: 2,6%

Potasio: 2,4%

Magnesio: l,9%

Hidrógeno: 0,9%

Titanio: 0,6%

Otros: 0,7%

A cada elemento se le asigna un nombre y un símbolo que lo identifica. Los símbolos actuales fueron introducidos por e1 químico sueco Jöns Berzelius en el siglo XIX.

El símbolo de cada elemento está representado por una letra mayúscula que corresponde a la primer letra de su nombre en griego o latín. Cuando el nombre de dos o más elementos comienza con la misma letra se le agrega una segunda letra minúscula que corresponde, generalmente, a la segunda del nombre.

Clasificación de los elementos

Los elementos se pueden clasificar, de un modo amplio e introductorio, adoptando como criterio de clasificación las propiedades de las sustancias simples que forman cada uno de ellos. Debe tenerse en cuenta, que las propiedades son de la sustancia simple (estado de agregación, color, conductividad, brillo, etc.) y no las del elemento que forma dicha sustancia simple.

De acuerdo con este criterio, los elementos se clasifican en:

Metales: se presentan en estado sólido a la temperatura ambiente con excepción del Mercurio que es líquido. El Cesio se presenta en estado sólido por debajo de los 28,5 oC que corresponde a su punto de fusión. Poseen un brillo característico (metálico), son buenos conductores del calor y de la electricidad. Se combinan con el Oxígeno para formar óxidos básicos y con el Hidrógeno para formar hidruros metálicos.

Son metales el Hierro (Fe), el Sodio (Na), el Litio (Li), el Magnesio (Mg), el Cobre (Cu), el Mercurio (Hg),

No metales: pueden presentarse en estado sólido (por ejemplo el Azufre), líquido (por ejemplo el Bromo) y gaseoso (por ejemplo el Cloro). No poseen brillo metálico, son en general malos conductores del calor y de la electricidad (una excepción es el elemento Carbono que forma la sustancia simple grafito). Se combinan con el Oxígeno para formar óxidos ácidos y con el Hidrógeno para producir hidruros no metálicos.

Son ejemplos de no metales: el Nitrógeno (N), el Cloro (Cl), el Yodo (I), el Azufre (S), el Fósforo (P).

Inértidos: las sustancias simples que forman, se conocen con el nombre de gases inertes, gases nobles o gases raros, son malos conductores del calor y de la electricidad. La característica esencial de estos gases es su casi total inactividad química, es decir, que prácticamente no se combinan con otras sustancias. Hasta hace algunos años se consideraba que los gases inertes eran completamente inactivos; en la actualidad se logró obtener algunos compuestos, trabajando para ello, en condiciones extremas, sometiéndolos a altas temperaturas y a altas presiones.

Los elementos inértidos son: el Helio (He), el Neón (Ne), el Xenón (Xe), el Argón (Ar), el Kriptón (Kr) y el Radón (Rd). Las sustancias simples que forman algunos de ellos están presentes en pequeñas proporciones en la atmósfera.

Es importante resaltar, nuevamente, que esta clasificación de los elementos se basa en las propiedades de las sustancias simples que los elementos forman, ya que los mismos generalmente no se encuentran libres en la naturaleza, sino combinados formando sustancias simples y compuestas. Se debe tener presente que para entender mejor esta clasificación, se debe considerar la definición de elemento químico.

The chemical elements

Introduction

also called element, any substance that cannot be decomposed into simpler substances by ordinary chemical processes. Elements are the fundamental materials of which all matter is composed.

This article considers the origin of the elements and their abundances throughout the universe. The geochemical distribution of these elementary substances in the Earth’s crust and interior is treated in some detail, as is their occurrence in the hydrosphere and atmosphere. The article also discusses the periodic law and the tabular arrangement of the elements based on it. For detailed information about the compounds of the elements, see chemical compound.

General observations

At present there are 112 known chemical elements. About 20 percent of them do not exist in nature (or are present only in trace amounts) and are known only because they have been synthetically prepared in the laboratory. Elements can combine with one another to form a wide variety of more complex substances called compounds. The number of possible compounds is almost infinite; perhaps a million are known, and more are being discovered every day. When two or more elements combine to form a compound, they lose their separate identities, and the product has characteristics quite different from those of the constituent elements. The gaseous elements hydrogen and oxygen, for example, with quite different properties, can combine to form the compound water, which has altogether different properties from either oxygen or hydrogen. Water clearly is not an element because it consists of, and actually can be decomposed chemically into, the two substances hydrogen and oxygen; these two substances, however, are elements because they cannot be decomposed into simpler substances by any known chemical process. Most samples of naturally occurring matter are physical mixtures of compounds. Seawater, for example, is a mixture of water and a large number of other compounds, the most common of which is sodium chloride, or table salt. Mixtures differ from compounds in that they can be separated into their component parts by physical processes; for example, the simple process of evaporation separates water from the other compounds in seawater.

Historical development of the concept of element

The modern concept of an element is unambiguous, depending as it does on the use of chemical and physical processes as a means of discriminating elements from compounds and mixtures. The existence of fundamental substances from which all matter is made, however, has been the basis of much theoretical speculation since the dawn of history. The ancient Greek philosophers Thales, Anaximenes, and Heracleitus each suggested that all matter is composed of one essential principle-or element. Thales believed this element to be water; Anaximenes suggested air; and Heracleitus, fire. Another Greek philosopher, Empedocles, expressed a different belief-that all substances are composed of four elements: air, earth, fire, and water. Aristotle agreed and emphasized that these four elements are bearers of fundamental properties, dryness and heat being associated with fire, heat and moisture with air, moisture and cold with water, and cold and dryness with earth. In the thinking of these philosophers all other substances were supposed to be combinations of the four elements, and the properties of substances were thought to reflect their elemental compositions. Thus, Greek thought encompassed the idea that all matter could be understood in terms of elemental qualities; in this sense, the elements themselves were thought of as nonmaterial. The Greek concept of an element, which was accepted for nearly 2,000 years, contained only one aspect of the modern definition-namely, that elements have characteristic properties.

In the latter part of the Middle Ages, as alchemists became more sophisticated in their knowledge of chemical processes, the Greek concepts of the composition of matter became less satisfactory. Additional elemental qualities were introduced to accommodate newly discovered chemical transformations. Thus, sulfur came to represent the quality of combustibility, mercury that of volatility or fluidity, and salt that of fixity in fire (or incombustibility). These three alchemical elements, or principles, also represented abstractions of properties reflecting the nature of matter, not physical substances.

The important difference between a mixture and a chemical compound eventually was understood, and in 1661 the English chemist Robert Boyle recognized the fundamental nature of a chemical element. He argued that the four Greek elements could not be the real chemical elements because they cannot combine to form other substances nor can they be extracted from other substances. Boyle stressed the physical nature of elements and related them to the compounds they formed in the modern operational way.

In 1789 the French chemist Antoine-Laurent Lavoisier published what might be considered the first list of elemental substances based on Boyle’s definition. Lavoisier’s list of elements was established on the basis of a careful, quantitative study of decomposition and recombination reactions. Because he could not devise experiments to decompose certain substances, or to form them from known elements, Lavoisier included in his list of elements such substances as lime, alumina, and silica, which now are known to be very stable compounds. That Lavoisier still retained a measure of influence from the ancient Greek concept of the elements is indicated by his inclusion of light and heat (caloric) among the elements.

Seven substances recognized today as elements (i.e., gold, silver, copper, iron, lead, tin, and mercury) were known to the ancients because they occur in nature in relatively pure form. They are mentioned in the Bible and in an early Hindu medical treatise, the Caraka-saṃhitā. Sixteen other elements were discovered in the second half of the 18th century, when methods of separating elements from their compounds became better understood. Eighty-two more followed, after the introduction of quantitative analytical methods.

The atomic nature of the elements

Paralleling the development of the concept of elements was an understanding of the nature of matter. At various times in history, matter has been considered to be either continuous or discontinuous. Continuous matter is postulated to be homogeneous and divisible without limit, each part exhibiting identical properties regardless of size. This was essentially the point of view taken by Aristotle when he associated his elemental qualities with continuous matter. Discontinuous matter, on the other hand, is conceived of as particulate-that is, divisible only up to a point, the point at which certain basic units called atoms are reached. According to this concept, also known as the atomic hypothesis, subdivision of the basic unit (atom) could give rise only to particles with profoundly different properties. Atoms, then, would be the ultimate carriers of the properties associated with bulk matter.

The atomic hypothesis is usually credited to the Greek philosopher Democritus, who considered all matter to be composed of atoms of the four elements-earth, air, fire, and water. But Aristotle’s concept of continuous matter generally prevailed and influenced thought until experimental findings in the 16th century forced a return to the atomic theory. Two types of experimental evidence gave support to the atomic hypothesis: first, the detailed behaviour of gaseous substances and, second, the quantitative weight relationships observed with a variety of chemical reactions. The English chemist John Dalton was the first to explain the empirically derived laws of chemical combination by postulating the existence of atoms with unique sets of properties. At the time, chemical combining power (valence) and relative atomic weights were the properties of most interest. Subsequently numerous independent experimental verifications of the atomic hypothesis were carried out, and today it is universally accepted. Indeed, in 1969 individual uranium and thorium atoms were actually observed by means of an electron microscope.

The structure of atoms

Atoms of elemental substances are themselves complex structures composed of more fundamental particles called protons, neutrons, and electrons. Experimental evidence indicates that, within an atom, a small nucleus, which generally contains both protons and neutrons, is surrounded by a swarm, or cloud, of electrons. The fundamental properties of these subatomic particles are their weight and electrical charge. Whereas protons carry a positive charge and electrons a negative one, neutrons are electrically neutral. The diameter of an atom (about 10-8 centimetre) is 10,000 times larger than that of its nucleus. Neutrons and protons, which are collectively called nucleons, have relative weights of approximately one atomic mass unit, whereas an electron is only about 1/2000 as heavy. Because neutrons and protons occur in the nucleus, virtually all of the mass of the atom is concentrated there. The number of protons in the nucleus is equivalent to the atomic number of the element. The total number of protons and neutrons is called the mass number because it equals the relative weight of that atom compared to other atoms. Because the atom itself is electrically neutral, the atomic number represents not only the number of protons, or positive charges, in the nucleus but also the number of electrons, or negative charges, in the extranuclear region of the atom.

The chemical characteristics of elements are intimately related to the number and arrangement of electrons in their atoms. Thus, elements are completely distinguishable from each other by their atomic numbers. The realization that such is the case leads to another definition of an element, namely, a substance, all atoms of which have the same atomic number.

The existence of isotopes

Careful experimental examination of naturally occurring samples of many pure elements shows that not all the atoms present have the same atomic weight, even though they all have the same atomic number. Such a situation can occur only if the atoms have different numbers of neutrons in their nuclei. Such groups of atoms-with the same atomic number, but with different relative weights-are called isotopes. The number of isotopic forms that a naturally occurring element possesses ranges from one (e.g., fluorine) to as many as ten (e.g., tin); most of the elements have at least two isotopes. The atomic weight of an element is usually determined from large numbers of atoms containing the natural distribution of isotopes, and, therefore, it represents the average isotopic weight of the atoms constituting the sample. More recently, precision mass-spectrometric methods have been used to determine the distribution and weights of isotopes in various naturally occurring samples of elements.

Chemistry

Introduction

the science that deals with the properties, composition, and structure of substances (defined as elements and compounds), the transformations they undergo, and the energy that is released or absorbed during these processes. Every substance, whether naturally occurring or artificially produced, consists of one or more of the hundred-odd species of atoms that have been identified as elements. Although these atoms, in turn, are composed of more elementary particles, they are the basic building blocks of chemical substances; there is no quantity of oxygen, mercury, or gold, for example, smaller than an atom of that substance. Chemistry, therefore, is concerned not with the subatomic domain but with the properties of atoms and the laws governing their combinations and how the knowledge of these properties can be used to achieve specific purposes.

The great challenge in chemistry is the development of a coherent explanation of the complex behaviour of materials, why they appear as they do, what gives them their enduring properties, and how interactions among different substances can bring about the formation of new substances and the destruction of old ones. From the earliest attempts to understand the material world in rational terms, chemists have struggled to develop theories of matter that satisfactorily explain both permanence and change. The ordered assembly of indestructible atoms into small and large molecules, or extended networks of intermingled atoms, is generally accepted as the basis of permanence, while the reorganization of atoms or molecules into different arrangements lies behind theories of change. Thus chemistry involves the study of the atomic composition and structural architecture of substances, as well as the varied interactions among substances that can lead to sudden, often violent reactions.

Chemistry also is concerned with the utilization of natural substances and the creation of artificial ones. Cooking, fermentation, glass making, and metallurgy are all chemical processes that date from the beginnings of civilization. Today, vinyl, Teflon, liquid crystals, semiconductors, and superconductors represent the fruits of chemical technology. The 20th century has seen dramatic advances in the comprehension of the marvelous and complex chemistry of living organisms, and a molecular interpretation of health and disease holds great promise. Modern chemistry, aided by increasingly sophisticated instruments, studies materials as small as single atoms and as large and complex as DNA (deoxyribonucleic acid), which contains millions of atoms. New substances can even be designed to bear desired characteristics and then synthesized. The rate at which chemical knowledge continues to accumulate is remarkable. Over time more than 8,000,000 different chemical substances, both natural and artificial, have been characterized and produced. The number was less than 500,000 as recently as 1965.

Intimately interconnected with the intellectual challenges of chemistry are those associated with industry. In the mid-19th century the German chemist Justus von Liebig commented that the wealth of a nation could be gauged by the amount of sulfuric acid it produced. This acid, essential to many manufacturing processes, remains today the leading chemical product of industrialized countries. As Liebig recognized, a country that produces large amounts of sulfuric acid is one with a strong chemical industry and a strong economy as a whole. The production, distribution, and utilization of a wide range of chemical products is common to all highly developed nations. In fact, one can say that the “iron age” of civilization is being replaced by a “polymer age,” for in some countries the total volume of polymers now produced exceeds that of iron.

The scope of chemistry

The days are long past when one person could hope to have a detailed knowledge of all areas of chemistry. Those pursuing their interests into specific areas of chemistry communicate with others who share the same interests. Over time a group of chemists with specialized research interests become the founding members of an area of specialization. The areas of specialization that emerged early in the history of chemistry, such as organic, inorganic, physical, analytical, and industrial chemistry, along with biochemistry, remain of greatest general interest. There has been, however, much growth in the areas of polymer, environmental, and medicinal chemistry during the 20th century. Moreover, new specialities continue to appear, as, for example, pesticide, forensic, and computer chemistry.

Analytical chemistry

Most of the materials that occur on Earth, such as wood, coal, minerals, or air, are mixtures of many different and distinct chemical substances. Each pure chemical substance (e.g., oxygen, iron, or water) has a characteristic set of properties that gives it its chemical identity. Iron, for example, is a common silver-white metal that melts at 1,535° C, is very malleable, and readily combines with oxygen to form the common substances hematite and magnetite. The detection of iron in a mixture of metals, or in a compound such as magnetite, is a branch of analytical chemistry called qualitative analysis. Measurement of the actual amount of a certain substance in a compound or mixture is termed quantitative analysis. Quantitative analytic measurement has determined, for instance, that iron makes up 72.3 percent, by mass, of magnetite, the mineral commonly seen as black sand along beaches and stream banks. Over the years, chemists have discovered chemical reactions that indicate the presence of such elemental substances by the production of easily visible and identifiable products. Iron can be detected by chemical means if it is present in a sample to an amount of 1 part per million or greater. Some very simple qualitative tests reveal the presence of specific chemical elements in even smaller amounts. The yellow colour imparted to a flame by sodium is visible if the sample being ignited has as little as one-billionth of a gram of sodium. Such analytic tests have allowed chemists to identify the types and amounts of impurities in various substances and to determine the properties of very pure materials. Substances used in common laboratory experiments generally have impurity levels of less than 0.1 percent. For special applications, one can purchase chemicals that have impurities totaling less than 0.001 percent. The identification of pure substances and the analysis of chemical mixtures enable all other chemical disciplines to flourish.

The importance of analytical chemistry has never been greater than it is today. The demand in modern societies for a variety of safe foods, affordable consumer goods, abundant energy, and labour-saving technologies places a great burden on the environment. All chemical manufacturing produces waste products in addition to the desired substances, and waste disposal has not always been carried out carefully. Disruption of the environment has occurred since the dawn of civilization, and pollution problems have increased with the growth of global population. The techniques of analytical chemistry are relied on heavily to maintain a benign environment. The undesirable substances in water, air, soil, and food must be identified, their point of origin fixed, and safe, economical methods for their removal or neutralization developed. Once the amount of a pollutant deemed to be hazardous has been assessed, it becomes important to detect harmful substances at concentrations well below the danger level. Analytical chemists seek to develop increasingly accurate and sensitive techniques and instruments.

Sophisticated analytic instruments, often coupled with computers, have improved the accuracy with which chemists can identify substances and have lowered detection limits. An analytic technique in general use is gas chromatography, which separates the different components of a gaseous mixture by passing the mixture through a long, narrow column of absorbent but porous material. The different gases interact differently with this absorbent material and pass through the column at different rates. As the separate gases flow out of the column, they can be passed into another analytic instrument called a mass spectrometer, which separates substances according to the mass of their constituent ions. A combined gas chromatograph-mass spectrometer can rapidly identify the individual components of a chemical mixture whose concentrations may be no greater than a few parts per billion. Similar or even greater sensitivities can be obtained under favourable conditions using techniques such as atomic absorption, polarography, and neutron activation. The rate of instrumental innovation is such that analytic instruments often become obsolete within 10 years of their introduction. Newer instruments are more accurate and faster and are employed widely in the areas of environmental and medicinal chemistry.

Inorganic chemistry

Modern chemistry, which dates more or less from the acceptance of the law of conservation of mass in the late 18th century, focused initially on those substances that were not associated with living organisms. Study of such substances, which normally have little or no carbon, constitutes the discipline of inorganic chemistry. Early work sought to identify the simple substances-namely, the elements-that are the constituents of all more complex substances. Some elements, such as gold and carbon, have been known since antiquity, and many others were discovered and studied throughout the 19th and early 20th centuries. Today, more than 100 are known. The study of such simple inorganic compounds as sodium chloride (common salt) has led to some of the fundamental concepts of modern chemistry, the law of definite proportions providing one notable example. This law states that for most pure chemical substances the constituent elements are always present in fixed proportions by mass (e.g., every 100 grams of salt contains 39.3 grams of sodium and 60.7 grams of chlorine). The crystalline form of salt, known as halite, consists of intermingled sodium and chlorine atoms, one sodium atom for each one of chlorine. Such a compound, formed solely by the combination of two elements, is known as a binary compound. Binary compounds are very common in inorganic chemistry, and they exhibit little structural variety. For this reason, the number of inorganic compounds is limited in spite of the large number of elements that may react with each other. If three or more elements are combined in a substance, the structural possibilities become greater.

After a period of quiescence in the early part of the 20th century, inorganic chemistry has again become an exciting area of research. Compounds of boron and hydrogen, known as boranes, have unique structural features that forced a change in thinking about the architecture of inorganic molecules. Some inorganic substances have structural features long believed to occur only in carbon compounds, and a few inorganic polymers have even been produced. Ceramics are materials composed of inorganic elements combined with oxygen. For centuries ceramic objects have been made by strongly heating a vessel formed from a paste of powdered minerals. Although ceramics are quite hard and stable at very high temperatures, they are usually brittle. Currently, new ceramics strong enough to be used as turbine blades in jet engines are being manufactured. There is hope that ceramics will one day replace steel in components of internal-combustion engines. In 1987 a ceramic containing yttrium, barium, copper, and oxygen, with the approximate formula YBa2Cu3O7, was found to be a superconductor at a temperature of about 100 K. A superconductor offers no resistance to the passage of an electrical current, and this new type of ceramic could very well find wide use in electrical and magnetic applications. A superconducting ceramic is so simple to make that it can be prepared in a high school laboratory. Its discovery illustrates the unpredictability of chemistry, for fundamental discoveries can still be made with simple equipment and inexpensive materials.

Many of the most interesting developments in inorganic chemistry bridge the gap with other disciplines. Organometallic chemistry investigates compounds that contain inorganic elements combined with carbon-rich units. Many organometallic compounds play an important role in industrial chemistry as catalysts, which are substances that are able to accelerate the rate of a reaction even when present in only very small amounts. Some success has been achieved in the use of such catalysts for converting natural gas to related but more useful chemical substances. Chemists also have created large inorganic molecules that contain a core of metal atoms, such as platinum, surrounded by a shell of different chemical units. Some of these compounds, referred to as metal clusters, have characteristics of metals, while others react in ways similar to biologic systems. Trace amounts of metals in biologic systems are essential for processes such as respiration, nerve function, and cell metabolism. Processes of this kind form the object of study of bioinorganic chemistry. Although organic molecules were once thought to be the distinguishing chemical feature of living creatures, it is now known that inorganic chemistry plays a vital role as well.

Organic chemistry

Organic compounds are based on the chemistry of carbon. Carbon is unique in the variety and extent of structures that can result from the three-dimensional connections of its atoms. The process of photosynthesis converts carbon dioxide and water to oxygen and compounds known as carbohydrates. Both cellulose, the substance that gives structural rigidity to plants, and starch, the energy storage product of plants, are polymeric carbohydrates. Simple carbohydrates produced by photosynthesis form the raw material for the myriad organic compounds found in the plant and animal kingdoms. When combined with variable amounts of hydrogen, oxygen, nitrogen, sulfur, phosphorus, and other elements, the structural possibilities of carbon compounds become limitless, and their number far exceeds the total of all nonorganic compounds. A major focus of organic chemistry is the isolation, purification, and structural study of these naturally occurring substances. Many natural products are simple molecules. Examples include formic acid (HCO2H) in ants, ethyl alcohol (C2H5OH) in fermenting fruit, and oxalic acid (C2H2O4) in rhubarb leaves. Other natural products, such as penicillin, vitamin B12, proteins, and nucleic acids, are exceedingly complex. The isolation of pure natural products from their host organism is made difficult by the low concentrations in which they may be present. Once they are isolated in pure form, however, modern instrumental techniques can reveal structural details for amounts weighing as little as one-millionth of a gram. The correlation of the physical and chemical properties of compounds with their structural features is the domain of physical organic chemistry. Once the properties endowed upon a substance by specific structural units termed functional groups are known, it becomes possible to design novel molecules that may exhibit desired properties. The preparation, under controlled laboratory conditions, of specific compounds is known as synthetic chemistry. Some products are easier to synthesize than to collect and purify from their natural sources. Tons of vitamin C, for example, are synthesized annually. Many synthetic substances have novel properties that make them especially useful. Plastics are a prime example, as are many drugs and agricultural chemicals. A continuing challenge for synthetic chemists is the structural complexity of most organic substances. To synthesize a desired substance, the atoms must be pieced together in the correct order and with the proper three-dimensional relationships. Just as a given pile of lumber and bricks can be assembled in many ways to build houses of several different designs, so too can a fixed number of atoms be connected together in various ways to give different molecules. Only one structural arrangement out of the many possibilities will be identical with a naturally occurring molecule. The antibiotic erythromycin, for example, contains 37 carbon, 67 hydrogen, and 13 oxygen atoms, along with one nitrogen atom. Even when joined together in the proper order, these 118 atoms can give rise to 262,144 different structures, only one of which has the characteristics of natural erythromycin. The great abundance of organic compounds, their fundamental role in the chemistry of life, and their structural diversity have made their study especially challenging and exciting. Organic chemistry is the largest area of specialization among the various fields of chemistry.

Biochemistry

As understanding of inanimate chemistry grew during the 19th century, attempts to interpret the physiological processes of living organisms in terms of molecular structure and reactivity gave rise to the discipline of biochemistry. Biochemists employ the techniques and theories of chemistry to probe the molecular basis of life. An organism is investigated on the premise that its physiological processes are the consequence of many thousands of chemical reactions occurring in a highly integrated manner. Biochemists have established, among other things, the principles that underlie energy transfer in cells, the chemical structure of cell membranes, the coding and transmission of hereditary information, muscular and nerve function, and biosynthetic pathways. In fact, related biomolecules have been found to fulfill similar roles in organisms as different as bacteria and human beings. The study of biomolecules, however, presents many difficulties. Such molecules are often very large and exhibit great structural complexity; moreover, the chemical reactions they undergo are usually exceedingly fast. The separation of the two strands of DNA, for instance, occurs in one-millionth of a second. Such rapid rates of reaction are possible only through the intermediary action of biomolecules called enzymes. Enzymes are proteins that owe their remarkable rate-accelerating abilities to their three-dimensional chemical structure. Not surprisingly, biochemical discoveries have had a great impact on the understanding and treatment of disease. Many ailments due to inborn errors of metabolism have been traced to specific genetic defects. Other diseases result from disruptions in normal biochemical pathways.

Frequently, symptoms can be alleviated by drugs, and the discovery, mode of action, and degradation of therapeutic agents is another of the major areas of study in biochemistry. Bacterial infections can be treated with sulfonamides, penicillins, and tetracyclines, and research into viral infections has revealed the effectiveness of acyclovir against the herpes virus. There is much current interest in the details of carcinogenesis and cancer chemotherapy. It is known, for example, that cancer can result when cancer-causing molecules, or carcinogens as they are called, react with nucleic acids and proteins and interfere with their normal modes of action. Researchers have developed tests that can identify molecules likelyto be carcinogenic. The hope, of course, is that progress in the prevention and treatment of cancer will accelerate once the biochemical basis of the disease is more fully understood.

The molecular basis of biologic processes is an essential feature of the fast-growing disciplines of molecular biology and biotechnology. Chemistry has developed methods for rapidly and accurately determining the structure of proteins and DNA. In addition, efficient laboratory methods for the synthesis of genes are being devised. Ultimately, the correction of genetic diseases by replacement of defective genes with normal ones may become possible.

Polymer chemistry

The simple substance ethylene is a gas composed of molecules with the formula CH2CH2. Under certain conditions, many ethylene molecules will join together to form a long chain called polyethylene, with the formula (CH2CH2)n, where n is a variable but large number. Polyethylene is a tough, durable solid material quite different from ethylene. It is an example of a polymer, which is a large molecule made up of many smaller molecules (monomers), usually joined together in a linear fashion. Many naturally occurring substances, including cellulose, starch, cotton, wool, rubber, leather, proteins, and DNA, are polymers. Polyethylene, nylon, and acrylics are examples of synthetic polymers. The study of such materials lies within the domain of polymer chemistry, a specialty that has flourished in the 20th century. The investigation of natural polymers overlaps considerably with biochemistry, but the synthesis of new polymers, the investigation of polymerization processes, and the characterization of the structure and properties of polymeric materials all pose unique problems for polymer chemists.

Polymer chemists have designed and synthesized polymers that vary in hardness, flexibility, softening temperature, solubility in water, and biodegradability. They have produced polymeric materials that are as strong as steel yet lighter and more resistant to corrosion. Oil, natural gas, and water pipelines are now routinely constructed of plastic pipe. In recent years, automakers have increased their use of plastic components to build lighter vehicles that consume less fuel. Other industries such as those involved in the manufacture of textiles, rubber, paper, and packaging materials are built upon polymer chemistry.

Besides producing new kinds of polymeric materials, researchers are concerned with developing special catalysts that are required by the large-scale industrial synthesis of commercial polymers. Without such catalysts, the polymerization process would be very slow in certain cases.

Physical chemistry

Many chemical disciplines, such as those already discussed, focus on certain classes of materials that share common structural and chemical features. Other specialties may be centred not on a class of substances but rather on their interactions and transformations. The oldest of these fields is physical chemistry, which seeks to measure, correlate, and explain the quantitative aspects of chemical processes. The Anglo-Irish chemist Robert Boyle, for example, discovered in the 17th century that at room temperature the volume of a fixed quantity of gas decreases proportionally as the pressure on it increases. Thus, for a gas at constant temperature, the product of its volume V and pressure P equals a constant number-i.e., PV = constant. Such a simple arithmetic relationship is valid for nearly all gases at room temperature and at pressures equal to or less than one atmosphere. Subsequent work has shown that the relationship loses its validity at higher pressures, but more complicated expressions that more accurately match experimental results can be derived. The discovery and investigation of such chemical regularities, often called laws of nature, lie within the realm of physical chemistry. For much of the 18th century the source of mathematical regularity in chemical systems was assumed to be the continuum of forces and fields that surround the atoms making up chemical elements and compounds. Developments in the 20th century, however, have shown that chemical behaviour is best interpreted by a quantum mechanical model of atomic and molecular structure. The branch of physical chemistry that is largely devoted to this subject is theoretical chemistry. Theoretical chemists make extensive use of computers to help them solve complicated mathematical equations. Other branches of physical chemistry include chemical thermodynamics, which deals with the relationship between heat and other forms of chemical energy, and chemical kinetics, which seeks to measure and understand the rates of chemical reactions. Electrochemistry investigates the interrelationship of electric current and chemical change. The passage of an electric current through a chemical solution causes changes in the constituent substances that are often reversible-i.e., under different conditions the altered substances themselves will yield an electric current. Common batteries contain chemical substances that, when placed in contact with each other by closing an electrical circuit, will deliver current at a constant voltage until the substances are consumed. At present there is much interest in devices that can use the energy in sunlight to drive chemical reactions whose products are capable of storing the energy. The discovery of such devices would make possible the widespread utilization of solar energy.

There are many other disciplines within physical chemistry that are concerned more with the general properties of substances and the interactions among substances than with the substances themselves. Photochemistry is a specialty that investigates the interaction of light with matter. Chemical reactions initiated by the absorption of light can be very different from those that occur by other means. Vitamin D, for example, is formed in the human body when the steroid ergosterol absorbs solar radiation; ergosterol does not change to vitamin D in the dark.

A rapidly developing subdiscipline of physical chemistry is surface chemistry. It examines the properties of chemical surfaces, relying heavily on instruments that can provide a chemical profile of such surfaces. Whenever a solid is exposed to a liquid or a gas, a reaction occurs initially on the surface of the solid, and its properties can change dramatically as a result. Aluminum is a case in point: it is resistant to corrosion precisely because the surface of the pure metal reacts with oxygen to form a layer of aluminum oxide, which serves to protect the interior of the metal from further oxidation. Numerous reaction catalysts perform their function by providing a reactive surface on which substances can react.

Industrial chemistry

The manufacture, sale, and distribution of chemical products is one of the cornerstones of a developed country. Chemists play an important role in the manufacture, inspection, and safe handling of chemical products, as well as in product development and general management. The manufacture of basic chemicals such as oxygen, chlorine, ammonia, and sulfuric acid provides the raw materials for industries producing textiles, agricultural products, metals, paints, and pulp and paper. Specialty chemicals are produced in smaller amounts for industries involved with such products as pharmaceuticals, foodstuffs, packaging, detergents, flavours, and fragrances. To a large extent, the chemical industry takes the products and reactions common to “bench-top” chemical processes and scales them up to industrial quantities.

The monitoring and control of bulk chemical processes, especially with regard to heat transfer, pose problems usually tackled by chemists and chemical engineers. The disposal of by-products also is a major problem for bulk chemical producers. These and other challenges of industrial chemistry set it apart from the more purely intellectual disciplines of chemistry discussed above. Yet, within the chemical industry, there is a considerable amount of fundamental research undertaken within traditional specialties. Most large chemical companies have research-and-development capability. Pharmaceutical firms, for example, operate large research laboratories in which chemists test molecules for pharmacological activity. The new products and processes that are discovered in such laboratories are often patented and become a source of profit for the company funding the research. A great deal of the research conducted in the chemical industry can be termed applied research because its goals are closely tied to the products and processes of the company concerned. New technologies often require much chemical expertise. The fabrication of, say, electronic microcircuits involves close to 100 separate chemical steps from start to finish. Thus, the chemical industry evolves with the technological advances of the modern world and at the same time often contributes to the rate of progress.

The methodology of chemistry

Chemistry is to a large extent a cumulative science. Over time the number and extent of observations and phenomena studied increase. Not all hypotheses and discoveries endure unchallenged, however. Some of them are discarded as new observations or more satisfying explanations appear. Nonetheless, chemistry has a broad spectrum of explanatory models for chemical phenomena that have endured and been extended over time. These now have the status of theories, interconnected sets of explanatory devices that correlate well with observed phenomena. As new discoveries are made, they are incorporated into existing theory whenever possible. However, as the discovery of high-temperature superconductors in 1986 illustrates, accepted theory is never sufficient to predict the course of future discovery. Serendipity, or chance discovery, will continue to play as much a role in the future as will theoretical sophistication.

Studies of molecular structure

The chemical properties of a substance are a function of its structure, and the techniques of X-ray crystallography now enable chemists to determine the precise atomic arrangement of complex molecules. A molecule is an ordered assembly of atoms. Each atom in a molecule is connected to one or more neighbouring atoms by a chemical bond. The length of bonds and the angles between adjacent bonds are all important in describing molecular structure, and a comprehensive theory of chemical bonding is one of the major achievements of modern chemistry. Fundamental to bonding theory is the atomic-molecular concept.

Atoms and elements

As far as general chemistry is concerned, atoms are composed of the three fundamental particles: the proton, the neutron, and the electron. Although the proton and the neutron are themselves composed of smaller units, their substructure has little impact on chemical transformation. As was explained in an earlier section, the proton carries a charge of +1, and the number of protons in an atomic nucleus distinguishes one type of chemical atom from another. The simplest atom of all, hydrogen, has a nucleus composed of a single proton. The neutron has very nearly the same mass as the proton, but it has no charge. Neutrons are contained with protons in the nucleus of all atoms other than hydrogen. The atom with one proton and one neutron in its nucleus is called deuterium. Because it has only one proton, deuterium exhibits the same chemical properties as hydrogen but has a different mass. Hydrogen and deuterium are examples of related atoms called isotopes. The third atomic particle, the electron, has a charge of -1, but its mass is 1,836 times smaller than that of a proton. The electron occupies a region of space outside the nucleus termed an orbital. Some orbitals are spherical with the nucleus at the centre. Because electrons have so little mass and move about at speeds close to half that of light, they exhibit the same wave-particle duality as photons of light. This means that some of the properties of an electron are best described by considering the electron to be a particle, while other properties are consistent with the behaviour of a standing wave. The energy of a standing wave, such as a vibrating string, is distributed over the region of space defined by the two fixed ends and the up-and-down extremes of vibration. Such a wave does not exist in a fixed region of space as does a particle. Early models of atomic structure envisioned the electron as a particle orbiting the nucleus, but electron orbitals are now interpreted as the regions of space occupied by standing waves called wave functions. These wave functions represent the regions of space around the nucleus in which the probability of finding an electron is high. They play an important role in bonding theory, as will be discussed later.

Each proton in an atomic nucleus requires an electron for electrical neutrality. Thus, as the number of protons in a nucleus increases, so too does the number of electrons. The electrons, alone or in pairs, occupy orbitals increasingly distant from the nucleus. Electrons farther from the nucleus are attracted less strongly by the protons in the nucleus, and they can be removed more easily from the atom. The energy required to move an electron from one orbital to another, or from one orbital to free space, gives a measure of the energy level of the orbitals. These energies have been found to have distinct, fixed values; they are said to be quantized. The energy differences between orbitals give rise to the characteristic patterns of light absorption or emission that are unique to each chemical atom.

A new chemical atom-that is, an element-results each time another proton is added to an atomic nucleus. Consecutive addition of protons generates the whole range of elements known to exist in the universe. Compounds are formed when two or more different elements combine through atomic bonding. Such bond formation is a consequence of electron pairing and constitutes the foundation of all structural chemistry.

Ionic and covalent bonding

When two different atoms approach each other, the electrons in their outer orbitals can respond in two distinct ways. An electron in the outermost atomic orbital of atom A may move completely to an outer but stabler orbital of atom B. The charged atoms that result, A+ and B-, are called ions, and the electrostatic force of attraction between them gives rise to what is termed an ionic bond. Most elements can form ionic bonds, and the substances that result commonly exist as three-dimensional arrays of positive and negative ions. Ionic compounds are frequently crystalline solids that have high melting points (e.g., table salt).

The second way in which the two outer electrons of atoms A and B can respond to the approach of A and B is to pair up to form a covalent bond. In the simple view known as the valence-bond model, in which electrons are treated strictly as particles, the two paired electrons are assumed to lie between the two nuclei and are shared equally by atoms A and B, resulting in a covalent bond. Atoms joined together by one or more covalent bonds constitute molecules. Hydrogen gas is composed of hydrogen molecules, which consist in turn of two hydrogen atoms linked by a covalent bond. The notation H2 for hydrogen gas is referred to as a molecular formula. Molecular formulas indicate the number and type of atoms that make up a molecule. The molecule H2 is responsible for the properties generally associated with hydrogen gas. Most substances on Earth have covalently bonded molecules as their fundamental chemical unit, and their molecular properties are completely different from those of the constituent elements. The physical and chemical properties of carbon dioxide, for example, are quite distinct from those of pure carbon and pure oxygen.

The interpretation of a covalent bond as a localized electron pair is an oversimplification of the bonding situation. A more comprehensive description of bonding that considers the wave properties of electrons is the molecular-orbital theory. According to this theory, electrons in a molecule, rather than being localized between atoms, are distributed over all the atoms in the molecule in a spatial distribution described by a molecular orbital. Such orbitals result when the atomic orbitals of bonded atoms combine with each other. The total number of molecular orbitals present in a molecule is equal to the sum of all atomic orbitals in the constituent atoms prior to bonding. Thus, for the simple combination of atoms A and B to form the molecule AB, two atomic orbitals combine to generate two molecular orbitals. One of these, the so-called bonding molecular orbital, represents a region of space enveloping both the A and B atoms, while the other, the anti-bonding molecular orbital, has two lobes, neither of which occupies the space between the two atoms. The bonding molecular orbital is at a lower energy level than are the two atomic orbitals, while the anti-bonding orbital is at a higher energy level. The two paired electrons that constitute the covalent bond between A and B occupy the bonding molecular orbital. For this reason, there is a high probability of finding the electrons between A and B, but they can be found elsewhere in the orbital as well. Because only two electrons are involved in bond formation and both can be accommodated in the lower energy orbital, the anti-bonding orbital remains unpopulated. This theory of bonding predicts that bonding between A and B will occur because the energy of the paired electrons after bonding is less than that of the two electrons in their atomic orbitals prior to bonding. The formation of a covalent bond is thus energetically favoured. The system goes from a state of higher energy to one of lower energy.

Another feature of this bonding picture is that it is able to predict the energy required to move an electron from the bonding molecular orbital to the anti-bonding one. The energy required for such an electronic excitation can be provided by visible light, for example, and the wavelength of the light absorbed determines the colour displayed by the absorbing molecule (e.g., violets are blue because the pigments in the flower absorb the red rays of natural light and reflect more of the blue). As the number of atoms in a molecule increases, so too does the number of molecular orbitals. Calculation of molecular orbitals for large molecules is mathematically difficult, but computers have made it possible to determine the wave equations for several large molecules. Molecular properties predicted by such calculations correlate well with experimental results.

Isomerism

Many elements can form two or more covalent bonds, but only a few are able to form extended chains of covalent bonds. The outstanding example is carbon, which can form as many as four covalent bonds and can bond to itself indefinitely. Carbon has six electrons in total, two of which are paired in an atomic orbital closest to the nucleus. The remaining four are farther from the nucleus and are available for covalent bonding. When there is sufficient hydrogen present, carbon will react to form methane, CH4. When all four electron pairs occupy the four molecular orbitals of lowest energy, the molecule assumes the shape of a tetrahedron, with carbon at the centre and the four hydrogen atoms at the apexes. The C-H bond length is 110 picometres (1 picometre = 10-12 metre), and the angle between adjacent C-H bonds is close to 110°. Such tetrahedral symmetry is common to many carbon compounds and results in interesting structural possibilities. If two carbon atoms are joined together, with three hydrogen atoms bonded to each carbon atom, the molecule ethane is obtained. When four carbon atoms are joined together, two different structures are possible: a linear structure designated n-butane and a branched structure called iso-butane. These two structures have the same molecular formula, C4H10, but a different order of attachment of their constituent atoms. The two molecules are termed structural isomers. Each of them has unique chemical and physical properties, and they are different compounds. The number of possible isomers increases rapidly as the number of carbon atoms increases. There are five isomers for C6H14, 75 for C10H22, and 6.2 × 1013 for C40H82. When carbon forms bonds to atoms other than hydrogen, such as oxygen, nitrogen, and sulfur, the structural possibilities become even greater. It is this great potential for structural diversity that makes carbon compounds essential to living organisms.

Even when the bonding sequence of carbon compounds is fixed, further structural variation is still possible. When two carbon atoms are joined together by two bonding pairs of electrons, a double bond is formed. A double bond forces the two carbon atoms and attached groups into a rigid, planar structure. As a result, a molecule such as CHCl=CHCl can exist in two nonidentical forms called geometric isomers. Structural rigidity also occurs in ring structures, and attached groups can be on the same side of a ring or on different sides. Yet another opportunity for isomerism arises when a carbon atom is bonded to four different groups. These can be attached in two different ways, one of which is the mirror image of the other. This type of isomerism is called optical isomerism, because the two isomers affect plane-polarized light differently. Two optical isomers are possible for every carbon atom that is bonded to four different groups. For a molecule bearing 10 such carbon atoms, the total number of possible isomers will be 210 = 1,024. Large biomolecules often have 10 or more carbon atoms for which such optical isomers are possible. Only one of all the possible isomers will be identical to the natural molecule. For this reason, the laboratory synthesis of large organic molecules is exceedingly difficult. Only in the last few decades of the 20th century have chemists succeeded in developing reagents and processes that yield specific optical isomers. They expect that new synthetic methods will make possible the synthesis of ever more complex natural products.

Investigations of chemical transformations
Basic factors

The structure of ionic substances and covalently bonded molecules largely determines their function. As noted above, the properties of a substance depend on the number and type of atoms it contains and on the bonding patterns present. Its bulk properties also depend, however, on the interactions among individual atoms, ions, or molecules. The force of attraction between the fundamental units of a substance dictate whether, at a given temperature and pressure, that substance will exist in the solid, liquid, or gas phase. At room temperature and pressure, for example, the strong forces of attraction between the positive ions of sodium (Na+) and the negative ions of chlorine (Cl-) draw them into a compact solid structure. The weaker forces of attraction among neighbouring water molecules allow the looser packing characteristic of a liquid. Finally, the very weak attractive forces acting among adjacent oxygen molecules are exceeded by the dispersive forces of heat; oxygen, consequently, is a gas. Interparticle forces thus affect the chemical and physical behaviour of substances, but they also determine to a large extent how a particle will respond to the approach of a different particle. If the two particles react with each other to form new particles, a chemical reaction has occurred. Notwithstanding the unlimited structural diversity allowed by molecular bonding, the world would be devoid of life if substances were incapable of change. The study of chemical transformation, which complements the study of molecular structure, is built on the concepts of energy and entropy.

Energy and the first law of thermodynamics

The concept of energy is a fundamental and familiar one in all the sciences. In simple terms, the energy of a body represents its ability to do work, and work itself is a force acting over a distance.

Chemical systems can have both kinetic energy (energy of motion) and potential energy (stored energy). The kinetic energy possessed by any collection of molecules in a solid, liquid, or gas is known as its thermal energy. Since liquids expand when they have more thermal energy, a liquid column of mercury, for example, will rise higher in an evacuated tube as it becomes warmer. In this way a thermometer can be used to measure the thermal energy, or temperature, of a system. The temperature at which all molecular motion comes to a halt is known as absolute zero.

Energy also may be stored in atoms or molecules as potential energy. When protons and neutrons combine to form the nucleus of a certain element, the reduction in potential energy is matched by the production of a huge quantity of kinetic energy. Consider, for instance, the formation of the deuterium nucleus from one proton and one neutron. The fundamental mass unit of the chemist is the mole, which represents the mass, in grams, of 6.02 × 1023 individual particles, whether they be atoms or molecules. One mole of protons has a mass of 1.007825 grams and one mole of neutrons has a mass of 1.008665 grams. By simple addition the mass of one mole of deuterium atoms (ignoring the negligible mass of one mole of electrons) should be 2.016490 grams. The measured mass is 0.00239 gram less than this. The missing mass is known as the binding energy of the nucleus and represents the mass equivalent of the energy released by nucleus formation. By using Einstein’s formula for the conversion of mass to energy (E = mc2), one can calculate the energy equivalent of 0.00239 gram as 2.15 × 108 kilojoules. This is approximately 240,000 times greater than the energy released by the combustion of one mole of methane. Such studies of the energetics of atom formation and interconversion are part of a specialty known as nuclear chemistry.

The energy released by the combustion of methane is about 900 kilojoules per mole. Although much less than the energy released by nuclear reactions, the energy given off by a chemical process such as combustion is great enough to be perceived as heat and light. Energy is released in so-called exothermic reactions because the chemical bonds in the product molecules, carbon dioxide and water, are stronger and stabler than those in the reactant molecules, methane and oxygen. The chemical potential energy of the system has decreased, and most of the released energy appears as heat, while some appears as radiant energy, or light. The heat produced by such a combustion reaction will raise the temperature of the surrounding air and, at constant pressure, increase its volume. This expansion of air results in work being done. In the cylinder of an internal-combustion engine, for example, the combustion of gasoline results in hot gases that expand against a moving piston. The motion of the piston turns a crankshaft, which then propels the vehicle. In this case, chemical potential energy has been converted to thermal energy, some of which produces useful work. This process illustrates a statement of the conservation of energy known as the first law of thermodynamics. This law states that, for an exothermic reaction, the energy released by the chemical system is equal to the heat gained by the surroundings plus the work performed. By measuring the heat and work quantities that accompany chemical reactions, it is possible to ascertain the energy differences between the reactants and the products of various reactions. In this manner, the potential energy stored in a variety of molecules can be determined, and the energy changes that accompany chemical reactions can be calculated.

Entropy and the second law of thermodynamics

Some chemical processes occur even though there is no net energy change. Consider a vessel containing a gas, connected to an evacuated vessel via a channel wherein a barrier obstructs passage of the gas. If the barrier is removed, the gas will expand into the evacuated vessel. This expansion is consistent with the observation that a gas always expands to fill the volume available. When the temperature of both vessels is the same, the energy of the gas before and after the expansion is the same. The reverse reaction does not occur, however. The spontaneous reaction is the one that yields a state of greater disorder. In the expanded volume, the individual gas molecules have greater freedom of movement and thus are more disordered. The measure of the disorder of a system is a quantity termed entropy. At a temperature of absolute zero, all movement of atoms and molecules ceases, and the disorder-and entropy-of such perfectly compacted substances is zero. (Zero entropy at zero temperature is in accord with the third law of thermodynamics.) All substances above absolute zero will have a positive entropy value that increases with temperature. When a hot body cools down, the thermal energy it loses passes to the surrounding air, which is at a lower temperature. As the entropy of the cooling body decreases, the entropy of the surrounding air increases. In fact, the increase in entropy of the air is greater than the decrease in entropy of the cooling body. This is consistent with the second law, which states that the total entropy of a system and its surroundings always increases in a spontaneous reaction. Thus the first and second laws of thermodynamics indicate that, for all processes of chemical change throughout the universe, energy is conserved but entropy increases.

Application of the laws of thermodynamics to chemical systems allows chemists to predict the behaviour of chemical reactions. When energy and entropy considerations favour the formation of product molecules, reagent molecules will act to form products until an equilibrium is established between products and reagents. The ratio of products to reagents is specified by a quantity known as an equilibrium constant, which is a function of the energy and entropy differences between the two. What thermodynamics cannot predict, however, is the rate at which chemical reactions occur. For fast reactions an equilibrium mixture of products and reagents can be established in one millisecond or less; for slow reactions the time required could be hundreds of years.

Rates of reaction

When the specific rates of chemical reactions are measured experimentally, they are found to be dependent on the concentrations of reacting species, temperature, and a quantity called activation energy. Chemists explain this phenomenon by recourse to the collision theory of reaction rates. This theory builds on the premise that a reaction between two or more chemicals requires, at the molecular level, a collision between two rapidly moving molecules. If the two molecules collide in the right way and with enough kinetic energy, one of the molecules may acquire enough energy to initiate the bond-breaking process. As this occurs, new bonds may begin to form, and ultimately reagent molecules are converted into product molecules. The point of highest energy during bond breaking and bond formation is called the transition state of the molecular process. The difference between the energy of the transition state and that of the reacting molecules is the activation energy that must be exceeded for a reaction to occur. Reaction rates increase with temperature because the colliding molecules have greater energies, and more of them will have energies that exceed the activation energy of reaction. The modern study of the molecular basis of chemical change has been greatly aided by lasers and computers. It is now possible to study short-lived collision products and to better determine the molecular mechanisms that fix the rate of chemical reactions. This knowledge is useful in designing new catalysts that can accelerate the rate of reaction by lowering the activation energy. Catalysts are important for many biochemical and industrial processes because they speed up reactions that ordinarily occur too slowly to be useful. Moreover, they often do so with increased control over the structural features of the product molecules. A rhodium phosphine catalyst, for example, has enabled chemists to obtain 96 percent of the correct optical isomer in a key step in the synthesis of L-dopa, a drug used for treating Parkinson’s disease.

Chemistry and society

For the first two-thirds of the 20th century, chemistry was seen by many as the science of the future. The potential of chemical products for enriching society appeared to be unlimited. Increasingly, however, and especially in the public mind, the negative aspects of chemistry have come to the fore. Disposal of chemical by-products at waste-disposal sites of limited capacity has resulted in environmental and health problems of enormous concern. The legitimate use of drugs for the medically supervised treatment of diseases has been tainted by the growing misuse of mood-altering drugs. The very word chemicals has come to be used all too frequently in a pejorative sense. There is, as a result, a danger that the pursuit and application of chemical knowledge may be seen as bearing risks that outweigh the benefits.

It is easy to underestimate the central role of chemistry in modern society, but chemical products are essential if the world’s population is to be clothed, housed, and fed. The world’s reserves of fossil fuels (e.g., oil, natural gas, and coal) will eventually be exhausted, some as soon as the 21st century, and new chemical processes and materials will provide a crucial alternative energy source. The conversion of solar energy to more concentrated, useful forms, for example, will rely heavily on discoveries in chemistry. Long-term, environmentally acceptable solutions to pollution problems are not attainable without chemical knowledge. There is much truth in the aphorism that “chemical problems require chemical solutions.” Chemical inquiry will lead to a better understanding of the behaviour of both natural and synthetic materials and to the discovery of new substances that will help future generations better supply their needs and deal with their problems.

Progress in chemistry can no longer be measured only in terms of economics and utility. The discovery and manufacture of new chemical goods must continue to be economically feasible but must be environmentally acceptable as well. The impact of new substances on the environment can now be assessed before large-scale production begins, and environmental compatibility has become a valued property of new materials. For example, compounds consisting of carbon fully bonded to chlorine and fluorine, called chlorofluorocarbons (or Freons), were believed to be ideal for their intended use when they were first discovered. They are nontoxic, nonflammable gases and volatile liquids that are very stable. These properties led to their widespread use as solvents, refrigerants, and propellants in aerosol containers. Time has shown, however, that these compounds decompose in the upper regions of the atmosphere and that the decomposition products act to destroy stratospheric ozone. Limits have now been placed on the use of chlorofluorocarbons, but it is impossible to recover the amounts already dispersed into the atmosphere.

The chlorofluorocarbon problem illustrates how difficult it is to anticipate the overall impact that new materials can have on the environment. Chemists are working to develop methods of assessment, and prevailing chemical theory provides the working tools. Once a substance has been identified as hazardous to the existing ecological balance, it is the responsibility of chemists to locate that substance and neutralize it, limiting the damage it can do or removing it from the environment entirely. The last years of the 20th century will see many new, exciting discoveries in the processes and products of chemistry. Inevitably, the harmful effects of some substances will outweigh their benefits, and their use will have to be limited. Yet, the positive impact of chemistry on society as a whole seems beyond doubt.

¡Más Sobre El Método Científico! (esto es para los que se quejan de mis post)

La ciencia suele definirse por la forma de investigar más que por el objeto de investigación, de manera que los procesos científicos son esencialmente iguales en todas las ciencias de la naturaleza; por ello la comunidad científica está de acuerdo en cuanto al lenguaje en que se expresan los problemas científicos, la forma de recoger y analizar datos, el uso de un estilo propio de lógica y la utilización de teorías y modelos. Etapas como realizar observaciones y experimentos, formular hipótesis, extraer resultados y analizarlos e interpretarlos van a ser características de cualquier investigación.

En el método científico la observación consiste en el estudio de un fenómeno que se produce en sus condiciones naturales. La observación debe ser cuidadosa, exhaustiva y exacta.

A partir de la observación surge el planteamiento del problema que se va a estudiar, lo que lleva a emitir alguna hipótesis o suposición provisional de la que se intenta extraer una consecuencia. Existen ciertas pautas que han demostrado ser de utilidad en el establecimiento de las hipótesis y de los resultados que se basan en ellas; estas pautas son: probar primero las hipótesis más simples, no considerar una hipótesis como totalmente cierta y realizar pruebas experimentales independientes antes de aceptar un único resultado experimental importante.

La experimentación consiste en el estudio de un fenómeno, reproducido generalmente en un laboratorio, en las condiciones particulares de estudio que interesan, eliminando o introduciendo aquellas variables que puedan influir en él. Se entiende por variable todo aquello que pueda causar cambios en los resultados de un experimento y se distingue entre variable independiente, dependiente y controlada.

Variable independiente es aquélla que el experimentador modifica a voluntad para averiguar si sus modificaciones provocan o no cambios en las otras variables. Variable dependiente es la que toma valores diferentes en función de las modificaciones que sufre la variable independiente. Variable controlada es la que se mantiene constante durante todo el experimento.

En un experimento siempre existe un control o un testigo, que es una parte del mismo no sometida a modificaciones y que se utiliza para comprobar los cambios que se producen.

Todo experimento debe ser reproducible, es decir, debe estar planteado y descrito de forma que pueda repetirlo cualquier experimentador que disponga del material adecuado.

Los resultados de un experimento pueden describirse mediante tablas, gráficos y ecuaciones de manera que puedan ser analizados con facilidad y permitan encontrar relaciones entre ellos que confirmen o no las hipótesis emitidas.

Una hipótesis confirmada se puede transformar en una ley científica que establezca una relación entre dos o más variables, y al estudiar un conjunto de leyes se pueden hallar algunas regularidades entre ellas que den lugar a unos principios generales con los cuales se constituya una teoría.

Según algunos investigadores, el método científico es el modo de llegar a elaborar teorías, entendiendo éstas como configuración de leyes. Mediante la inducción se obtiene una ley a partir de las observaciones y medidas de los fenómenos naturales, y mediante la deducción se obtienen consecuencias lógicas de una teoría. Por esto, para que una teoría científica sea admisible debe relacionar de manera razonable muchos hechos en apariencia independientes en una estructura mental coherente. Así mismo debe permitir hacer predicciones de nuevas relaciones y fenómenos que se puedan comprobar experimentalmente.

Las leyes y las teorías encierran a menudo una pretensión realista que conlleva la noción de modelo; éste es una abstracción mental que se utiliza para poder explicar algunos fenómenos y para reconstruir por aproximación los rasgos del objeto considerado en la investigación.

¿Qué Es El Plasma?

Es un estado de la materia, generalmente gaseoso, en el que algunos o todos los átomos o moléculas están disociados en forma de iones. Los plasmas están constituidos por una mezcla de partículas neutras, iones positivos (átomos o moléculas que han perdido uno o más electrones) y electrones negativos. Un plasma es conductor de la electricidad, pero cuando su volumen supera la llamada longitud de Debye presenta un comportamiento eléctricamente neutro. A escala microscópica, que corresponde a dimensiones inferiores a la longitud de Debye, las partículas de un plasma no presentan un comportamiento colectivo, sino que reaccionan individualmente a perturbaciones como por ejemplo un campo eléctrico.

En la Tierra, los plasmas no suelen existir en la naturaleza, salvo en los relámpagos, que son trayectorias estrechas a lo largo de las cuales las moléculas de aire están ionizadas aproximadamente en un 20%, y en algunas zonas de las llamas. Los electrones libres de un metal también pueden ser considerados como un plasma. La mayor parte del Universo está formado por materia en estado de plasma. La ionización está causada por las elevadas temperaturas, como ocurre en el Sol y las demás estrellas, o por la radiación, como sucede en los gases interestelares o en las capas superiores de la atmósfera, donde produce el fenómeno denominado aurora.

Los plasmas pueden crearse aplicando un campo eléctrico a un gas a baja presión, como en los tubos fluorescentes o de neón. También puede crearse un plasma calentando un gas neutro hasta temperaturas muy altas. En general, las temperaturas son demasiado altas para aplicarlas externamente, por lo que se calienta el gas internamente inyectando en él iones o electrones de alta velocidad que pueden colisionar con las partículas de gas y aumentar su energía térmica. Los electrones del gas también pueden ser acelerados por campos eléctricos externos. Los iones procedentes de estos plasmas se emplean en la industria de semiconductores para grabar superficies y producir otras alteraciones en las propiedades de los materiales.

En los plasmas muy calientes, las partículas adquieren suficiente energía como para producir reacciones nucleares al colisionar entre sí. Estas reacciones de fusión son la fuente de calor en el núcleo del Sol, y los científicos intentan crear en los laboratorios plasmas artificiales donde las reacciones de fusión puedan producir energía para generar electricidad.