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Hydrogen bonding is given outsized standing because water is ubiquitous and essential to life and (all!) of biochemistry. But to claim hydrogen bonding is "obvious" is a bit of putting the cart before the horse. Quantum mechanics, or at least Maxwell's unification of electromagnetism, was described well before hydrogen bonding was first described. (see, eg., Latimer and Rodebush, 1920) Hydrogen bonding arises out of the amphoterism of water, and water is not the only amphoteric substance.First of all, hydrogen (despite the name) is irrelevant to hydrogen bonding. It is principally an electrostatic attraction- highly electronegative atoms like oxygen or nitrogen draw electron density away from the hydrogen atom, and thus create a strong electromagnetic dipole. Hydrogen, in this description, behaves more like an alkaline metal, and takes its place above the first column on the periodic table. But hydrogen is also capable of acting as hydride, and so takes its place above fluoride and chloride and next to helium. Either way, hydrogen atoms rarely stand alone- they must have a dance partner, such as with water forming Hydronium or Hydroxide. The elemental understanding of the self dissociation, the amphoterism of water as the source of its electrostatic character dates back to the 1880s and Arrhenius. (Consider also: that trihydrogen cation, H3+, is the most abundant ion in the universe)When you go outside the realm of aqueous solution, there are a variety of possibilities. For this classification, I turn to Coordination Chemistry in Non-Aqueous Solutions for advice.According to the coordination chemistry approach solvents may be divided into1. Donor solvents, which have a high tendency to react with electron pair acceptors, and2. Acceptor solvents, which tend to react with electron pair donors.Many characteristic features will be different for these two classes of solvents. The former will solvate in the first place metal cations, while the latter will solvate mainly anions. For the consideration of acid-base phenomena in the sense of BRONSTED, and of association phenomena through hydrogen bridges, each of these groups of solvents may again be divided intoa) Proton-containing or hydrogen bridged solvents andb) Proton-free solvents or not hydrogen bridged solvents.Molten salts and liquid metals are considered to be special classes of non protonic solvents...In all cases, we are talking about electrons or orbital-empty or orbital-filled so-called "pairs" of electrons (see, eg, Jensen), which determine electrostatic character. Protons are not the carrier of positive charge- electrons, or their absence, transmit negative charges. Hydrogen bonding should be referred to as electrostatic bonding, or as a special case thereof, and is unique to period one and period two elements due to the exposure, overlap, and character of 1s, 2s, and 2p orbitals. Higher period elements, the sulfurs and the phosphoruses, the metals and the metal salts, are typically talked about in terms of their oxidation state and ionic character, rather than "bond order", and create more complicated compounds with the involvement of d orbitals.In my opinion, the ad-hoc nature by which chemistry was developed was a product of the pre-quantum world bleeding into the modern era. The study of chemistry at its root is the study of electrons, without which chemistry simply doesn't happen. The fact that they are paired with massive boat-anchor nuclei is, for all intents and purposes, almost completely irrelevant to chemistry, insofar as their outsized mass reacts so slowly relative to the speed of electrons.We live in a peculiar time where the separate conceits of organic and inorganic chemistry continue to make their mark and divvy up the terminology of chemistry separately, rather than moving to unification. As fewer and fewer pedantic, memorization-based chemistry tutors age out of the teaching pool, there is a definite need to form a newer, unified science. I don't always agree with the approach that Lewis (or more specifically, VSEPR) theory takes but there's a certain "there" there that properly formatted and bound with group theory, could definitely improve things.

An atom is the smallest constituent unit of ordinary matter that has the properties of a chemical element. Every solid, liquid, gas, and plasma is composed of neutral or ionized atoms. Atoms are extremely small; typical sizes are around 100 picometers (a ten-billionth of a meter, in the short scale).Helium atomAn illustration of the helium atom, depicting the nucleus (pink) and the electron clouddistribution (black). The nucleus (upper right) in helium-4 is in reality spherically symmetric and closely resembles the electron cloud, although for more complicated nuclei this is not always the case. The black bar is one angstrom(10−10 m or 100 pm).ClassificationSmallest recognized division of a chemical elementPropertiesMass range1.67×10−27 to 4.52×10−25 kgElectric chargezero (neutral), or ionchargeDiameter range62 pm (He) to 520 pm (Cs) (data page)ComponentsElectrons and a compact nucleus of protons and neutronsAtoms are small enough that attempting to predict their behavior using classical physics – as if they were billiard balls, for example – gives noticeably incorrect predictions due to quantum effects. Through the development of physics, atomic models have incorporated quantum principles to better explain and predict this behavior.Every atom is composed of a nucleus and one or more electrons bound to the nucleus. The nucleus is made of one or more protons and typically a similar number of neutrons. Protons and neutrons are called nucleons. More than 99.94% of an atom's mass is in the nucleus. The protons have a positive electric charge, the electrons have a negative electric charge, and the neutrons have no electric charge. If the number of protons and electrons are equal, that atom is electrically neutral. If an atom has more or fewer electrons than protons, then it has an overall negative or positive charge, respectively, and it is called an ion.The electrons of an atom are attracted to the protons in an atomic nucleus by this electromagnetic force. The protons and neutrons in the nucleus are attracted to each other by a different force, the nuclear force, which is usually stronger than the electromagnetic force repelling the positively charged protons from one another. Under certain circumstances, the repelling electromagnetic force becomes stronger than the nuclear force, and nucleons can be ejected from the nucleus, leaving behind a different element: nuclear decay resulting in nuclear transmutation.The number of protons in the nucleus defines to what chemical element the atom belongs: for example, all copper atoms contain 29 protons. The number of neutrons defines the isotope of the element. The number of electrons influences the magnetic properties of an atom. Atoms can attach to one or more other atoms by chemical bonds to form chemical compounds such as molecules. The ability of atoms to associate and dissociate is responsible for most of the physical changes observed in nature and is the subject of the discipline of chemistry.ContentsHistory of atomic theoryAtoms in philosophyThe idea that matter is made up of discrete units is a very old idea, appearing in many ancient cultures such as Greece and India. The word "atom" (Greek: ἄτομος; atomos), meaning "uncuttable", was coined by the ancient Greek philosophers Leucippus and his pupil Democritus (c.460 –c.370 BC).[1][2][3][4]Democritus taught that atoms were infinite in number, uncreated, and eternal, and that the qualities of an object result from the kind of atoms that compose it.[2][3][4]Democritus's atomism was refined and elaborated by the later philosopher Epicurus (341–270 BC).[3][4]During the Early Middle Ages, atomism was mostly forgotten in western Europe, but survived among some groups of Islamic philosophers.[3]During the twelfth century, atomism became known again in western Europe through references to it in the newly-rediscovered writings of Aristotle.[3]In the fourteenth century, the rediscovery of major works describing atomist teachings, including Lucretius's De rerum natura and Diogenes Laërtius's Lives and Opinions of Eminent Philosophers, led to increased scholarly attention on the subject.[3]Nonetheless, because atomism was associated with the philosophy of Epicureanism, which contradicted orthodox Christian teachings, belief in atoms was not considered acceptable.[3]The French Catholic priest Pierre Gassendi (1592–1655) revived Epicurean atomism with modifications, arguing that atoms were created by God and, though extremely numerous, are not infinite.[3][4]Gassendi's modified theory of atoms was popularized in France by the physician François Bernier (1620–1688) and in England by the natural philosopher Walter Charleton (1619–1707).[3]The chemist Robert Boyle (1627–1691) and the physicist Isaac Newton (1642–1727) both defended atomism and, by the end of the seventeenth century, it had become accepted by portions of the scientific community.[3]First evidence-based theoryVarious atoms and molecules as depicted in John Dalton's A New System of Chemical Philosophy(1808).In the early 1800s, John Dalton used the concept of atoms to explain why elements always react in ratios of small whole numbers (the law of multiple proportions). For instance, there are two types of tin oxide: one is 88.1% tin and 11.9% oxygen and the other is 78.7% tin and 21.3% oxygen (tin(II) oxide and tin dioxide respectively). This means that 100g of tin will combine either with 13.5g or 27g of oxygen. 13.5 and 27 form a ratio of 1:2, a ratio of small whole numbers. This common pattern in chemistry suggested to Dalton that elements react in multiples of discrete units — in other words, atoms. In the case of tin oxides, one tin atom will combine with either one or two oxygen atoms.[5]Dalton also believed atomic theory could explain why water absorbs different gases in different proportions. For example, he found that water absorbs carbon dioxide far better than it absorbs nitrogen.[6]Dalton hypothesized this was due to the differences between the masses and configurations of the gases' respective particles, and carbon dioxide molecules (CO2) are heavier and larger than nitrogen molecules (N2).Brownian motionIn 1827, botanist Robert Brown used a microscope to look at dust grains floating in water and discovered that they moved about erratically, a phenomenon that became known as "Brownian motion". This was thought to be caused by water molecules knocking the grains about. In 1905, Albert Einstein proved the reality of these molecules and their motions by producing the first statistical physics analysis of Brownian motion.[7][8][9]French physicist Jean Perrin used Einstein's work to experimentally determine the mass and dimensions of atoms, thereby conclusively verifying Dalton's atomic theory.[10]Discovery of the electronThe Geiger–Marsden experimentTop: Expected results: alpha particles passing through the plum pudding model of the atom with negligible deflection.Bottom: Observed results: a small portion of the particles were deflected by the concentrated positive charge of the nucleus.The physicist J.J. Thomson measured the mass of cathode rays, showing they were made of particles, but were around 1800 times lighter than the lightest atom, hydrogen. Therefore, they were not atoms, but a new particle, the first subatomic particle to be discovered, which he originally called "corpuscle" but was later named electron, after particles postulated by George Johnstone Stoney in 1874. He also showed they were identical to particles given off by photoelectric and radioactive materials.[11]It was quickly recognized that they are the particles that carry electric currents in metal wires, and carry the negative electric charge within atoms. Thomson was given the 1906 Nobel Prize in Physics for this work. Thus he overturned the belief that atoms are the indivisible, ultimate particles of matter.[12]Thomson also incorrectly postulated that the low mass, negatively charged electrons were distributed throughout the atom in a uniform sea of positive charge. This became known as the plum pudding model.Discovery of the nucleusIn 1909, Hans Geiger and Ernest Marsden, under the direction of Ernest Rutherford, bombarded a metal foil with alpha particles to observe how they scattered. They expected all the alpha particles to pass straight through with little deflection, because Thomson's model said that the charges in the atom are so diffuse that their electric fields could not affect the alpha particles much. However, Geiger and Marsden spotted alpha particles being deflected by angles greater than 90°, which was supposed to be impossible according to Thomson's model. To explain this, Rutherford proposed that the positive charge of the atom is concentrated in a tiny nucleus at the center of the atom.[13]Discovery of isotopesWhile experimenting with the products of radioactive decay, in 1913 radiochemist Frederick Soddy discovered that there appeared to be more than one type of atom at each position on the periodic table.[14]The term isotope was coined by Margaret Todd as a suitable name for different atoms that belong to the same element. J.J. Thomson created a technique for isotope separation through his work on ionized gases, which subsequently led to the discovery of stable isotopes.[15]Bohr modelThe Bohr model of the atom, with an electron making instantaneous "quantum leaps" from one orbit to another. This model is obsolete.In 1913 the physicist Niels Bohr proposed a model in which the electrons of an atom were assumed to orbit the nucleus but could only do so in a finite set of orbits, and could jump between these orbits only in discrete changes of energy corresponding to absorption or radiation of a photon.[16]This quantization was used to explain why the electrons orbits are stable (given that normally, charges in acceleration, including circular motion, lose kinetic energy which is emitted as electromagnetic radiation, see synchrotron radiation) and why elements absorb and emit electromagnetic radiation in discrete spectra.[17]Later in the same year Henry Moseley provided additional experimental evidence in favor of Niels Bohr's theory. These results refined Ernest Rutherford's and Antonius Van den Broek's model, which proposed that the atom contains in its nucleus a number of positive nuclear charges that is equal to its (atomic) number in the periodic table. Until these experiments, atomic number was not known to be a physical and experimental quantity. That it is equal to the atomic nuclear charge remains the accepted atomic model today.[18]Chemical bonding explainedChemical bonds between atoms were now explained, by Gilbert Newton Lewis in 1916, as the interactions between their constituent electrons.[19]As the chemical properties of the elements were known to largely repeat themselves according to the periodic law,[20]in 1919 the American chemist Irving Langmuir suggested that this could be explained if the electrons in an atom were connected or clustered in some manner. Groups of electrons were thought to occupy a set of electron shells about the nucleus.[21]Further developments in quantum physicsThe Stern–Gerlach experiment of 1922 provided further evidence of the quantum nature of atomic properties. When a beam of silver atoms was passed through a specially shaped magnetic field, the beam was split in a way correlated with the direction of an atom's angular momentum, or spin. As this spin direction is initially random, the beam would be expected to deflect in a random direction. Instead, the beam was split into two directional components, corresponding to the atomic spin being oriented up or down with respect to the magnetic field.[22]In 1925 Werner Heisenberg published the first consistent mathematical formulation of quantum mechanics (Matrix Mechanics).[18]One year earlier, in 1924, Louis de Broglie had proposed that all particles behave to an extent like waves and, in 1926, Erwin Schrödinger used this idea to develop a mathematical model of the atom (Wave Mechanics) that described the electrons as three-dimensional waveforms rather than point particles.A consequence of using waveforms to describe particles is that it is mathematically impossible to obtain precise values for both the position and momentum of a particle at a given point in time; this became known as the uncertainty principle, formulated by Werner Heisenberg in 1927.[18]In this concept, for a given accuracy in measuring a position one could only obtain a range of probable values for momentum, and vice versa.[23]This model was able to explain observations of atomic behavior that previous models could not, such as certain structural and spectral patterns of atoms larger than hydrogen. Thus, the planetary model of the atom was discarded in favor of one that described atomic orbital zones around the nucleus where a given electron is most likely to be observed.[24][25]Discovery of the neutronThe development of the mass spectrometer allowed the mass of atoms to be measured with increased accuracy. The device uses a magnet to bend the trajectory of a beam of ions, and the amount of deflection is determined by the ratio of an atom's mass to its charge. The chemist Francis William Aston used this instrument to show that isotopes had different masses. The atomic mass of these isotopes varied by integer amounts, called the whole number rule.[26]The explanation for these different isotopes awaited the discovery of the neutron, an uncharged particle with a mass similar to the proton, by the physicist James Chadwick in 1932. Isotopes were then explained as elements with the same number of protons, but different numbers of neutrons within the nucleus.[27]Fission, high-energy physics and condensed matterIn 1938, the German chemist Otto Hahn, a student of Rutherford, directed neutrons onto uranium atoms expecting to get transuranium elements. Instead, his chemical experiments showed barium as a product.[28][29]A year later, Lise Meitner and her nephew Otto Frisch verified that Hahn's result were the first experimental nuclear fission.[30][31]In 1944, Hahn received the Nobel prize in chemistry. Despite Hahn's efforts, the contributions of Meitner and Frisch were not recognized.[32]In the 1950s, the development of improved particle accelerators and particle detectors allowed scientists to study the impacts of atoms moving at high energies.[33]Neutrons and protons were found to be hadrons, or composites of smaller particles called quarks. The standard model of particle physics was developed that so far has successfully explained the properties of the nucleus in terms of these sub-atomic particles and the forces that govern their interactions.[34]StructureSubatomic particlesThough the word atom originally denoted a particle that cannot be cut into smaller particles, in modern scientific usage the atom is composed of various subatomic particles. The constituent particles of an atom are the electron, the proton and the neutron; all three are fermions. However, the hydrogen-1 atom has no neutrons and the hydron ion has no electrons.The electron is by far the least massive of these particles at 9.11×10−31 kg, with a negative electrical charge and a size that is too small to be measured using available techniques.[35]It was the lightest particle with a positive rest mass measured, until the discovery of neutrino mass. Under ordinary conditions, electrons are bound to the positively charged nucleus by the attraction created from opposite electric charges. If an atom has more or fewer electrons than its atomic number, then it becomes respectively negatively or positively charged as a whole; a charged atom is called an ion. Electrons have been known since the late 19th century, mostly thanks to J.J. Thomson; see history of subatomic physics for details.Protons have a positive charge and a mass 1,836 times that of the electron, at 1.6726×10−27 kg. The number of protons in an atom is called its atomic number. Ernest Rutherford (1919) observed that nitrogen under alpha-particle bombardment ejects what appeared to be hydrogen nuclei. By 1920 he had accepted that the hydrogen nucleus is a distinct particle within the atom and named it proton.Neutrons have no electrical charge and have a free mass of 1,839 times the mass of the electron,[36]or 1.6929×10−27 kg, the heaviest of the three constituent particles, but it can be reduced by the nuclear binding energy. Neutrons and protons (collectively known as nucleons) have comparable dimensions—on the order of 2.5×10−15 m—although the 'surface' of these particles is not sharply defined.[37]The neutron was discovered in 1932 by the English physicist James Chadwick.In the Standard Model of physics, electrons are truly elementary particles with no internal structure. However, both protons and neutrons are composite particles composed of elementary particles called quarks. There are two types of quarks in atoms, each having a fractional electric charge. Protons are composed of two up quarks (each with charge +2/3) and one down quark (with a charge of −1/3). Neutrons consist of one up quark and two down quarks. This distinction accounts for the difference in mass and charge between the two particles.[38][39]The quarks are held together by the strong interaction (or strong force), which is mediated by gluons. The protons and neutrons, in turn, are held to each other in the nucleus by the nuclear force, which is a residuum of the strong force that has somewhat different range-properties (see the article on the nuclear force for more). The gluon is a member of the family of gauge bosons, which are elementary particles that mediate physical forces.[38][39]NucleusThe binding energy needed for a nucleon to escape the nucleus, for various isotopesAll the bound protons and neutrons in an atom make up a tiny atomic nucleus, and are collectively called nucleons. The radius of a nucleus is approximately equal to 1.07 3√A fm, where A is the total number of nucleons.[40]This is much smaller than the radius of the atom, which is on the order of 105fm. The nucleons are bound together by a short-ranged attractive potential called the residual strong force. At distances smaller than 2.5 fm this force is much more powerful than the electrostatic force that causes positively charged protons to repel each other.[41]Atoms of the same element have the same number of protons, called the atomic number. Within a single element, the number of neutrons may vary, determining the isotope of that element. The total number of protons and neutrons determine the nuclide. The number of neutrons relative to the protons determines the stability of the nucleus, with certain isotopes undergoing radioactive decay.[42]The proton, the electron, and the neutron are classified as fermions. Fermions obey the Pauli exclusion principle which prohibits identical fermions, such as multiple protons, from occupying the same quantum state at the same time. Thus, every proton in the nucleus must occupy a quantum state different from all other protons, and the same applies to all neutrons of the nucleus and to all electrons of the electron cloud.[43]A nucleus that has a different number of protons than neutrons can potentially drop to a lower energy state through a radioactive decay that causes the number of protons and neutrons to more closely match. As a result, atoms with matching numbers of protons and neutrons are more stable against decay. However, with increasing atomic number, the mutual repulsion of the protons requires an increasing proportion of neutrons to maintain the stability of the nucleus, which slightly modifies this trend of equal numbers of protons to neutrons.[43]Illustration of a nuclear fusion process that forms a deuterium nucleus, consisting of a proton and a neutron, from two protons. A positron (e+)—an antimatterelectron—is emitted along with an electron neutrino.The number of protons and neutrons in the atomic nucleus can be modified, although this can require very high energies because of the strong force. Nuclear fusion occurs when multiple atomic particles join to form a heavier nucleus, such as through the energetic collision of two nuclei. For example, at the core of the Sun protons require energies of 3–10 keV to overcome their mutual repulsion—the coulomb barrier—and fuse together into a single nucleus.[44]Nuclear fission is the opposite process, causing a nucleus to split into two smaller nuclei—usually through radioactive decay. The nucleus can also be modified through bombardment by high energy subatomic particles or photons. If this modifies the number of protons in a nucleus, the atom changes to a different chemical element.[45][46]If the mass of the nucleus following a fusion reaction is less than the sum of the masses of the separate particles, then the difference between these two values can be emitted as a type of usable energy (such as a gamma ray, or the kinetic energy of a beta particle), as described by Albert Einstein's mass–energy equivalence formula, E = mc2, where m is the mass loss and c is the speed of light. This deficit is part of the binding energy of the new nucleus, and it is the non-recoverable loss of the energy that causes the fused particles to remain together in a state that requires this energy to separate.[47]The fusion of two nuclei that create larger nuclei with lower atomic numbers than iron and nickel—a total nucleon number of about 60—is usually an exothermic process that releases more energy than is required to bring them together.[48]It is this energy-releasing process that makes nuclear fusion in stars a self-sustaining reaction. For heavier nuclei, the binding energy per nucleon in the nucleus begins to decrease. That means fusion processes producing nuclei that have atomic numbers higher than about 26, and atomic masses higher than about 60, is an endothermic process. These more massive nuclei can not undergo an energy-producing fusion reaction that can sustain the hydrostatic equilibrium of a star.[43]Electron cloudA potential well, showing, according to classical mechanics, the minimum energy V(x) needed to reach each position x. Classically, a particle with energy E is constrained to a range of positions between x1and x2.The electrons in an atom are attracted to the protons in the nucleus by the electromagnetic force. This force binds the electrons inside an electrostatic potential well surrounding the smaller nucleus, which means that an external source of energy is needed for the electron to escape. The closer an electron is to the nucleus, the greater the attractive force. Hence electrons bound near the center of the potential well require more energy to escape than those at greater separations.Electrons, like other particles, have properties of both a particle and a wave. The electron cloud is a region inside the potential well where each electron forms a type of three-dimensional standing wave—a wave form that does not move relative to the nucleus. This behavior is defined by an atomic orbital, a mathematical function that characterises the probability that an electron appears to be at a particular location when its position is measured.[49]Only a discrete (or quantized) set of these orbitals exist around the nucleus, as other possible wave patterns rapidly decay into a more stable form.[50]Orbitals can have one or more ring or node structures, and differ from each other in size, shape and orientation.[51]Wave functions of the first five atomic orbitals. The three 2p orbitals each display a single angular node that has an orientation and a minimum at the center.Play mediaHow atoms are constructed from electron orbitals and link to the periodic table.Each atomic orbital corresponds to a particular energy level of the electron. The electron can change its state to a higher energy level by absorbing a photon with sufficient energy to boost it into the new quantum state. Likewise, through spontaneous emission, an electron in a higher energy state can drop to a lower energy state while radiating the excess energy as a photon. These characteristic energy values, defined by the differences in the energies of the quantum states, are responsible for atomic spectral lines.[50]The amount of energy needed to remove or add an electron—the electron binding energy—is far less than the binding energy of nucleons. For example, it requires only 13.6 eV to strip a ground-state electron from a hydrogen atom,[52]compared to 2.23 million eV for splitting a deuterium nucleus.[53]Atoms are electrically neutral if they have an equal number of protons and electrons. Atoms that have either a deficit or a surplus of electrons are called ions. Electrons that are farthest from the nucleus may be transferred to other nearby atoms or shared between atoms. By this mechanism, atoms are able to bond into molecules and other types of chemical compounds like ionic and covalent network crystals.[54]PropertiesNuclear propertiesBy definition, any two atoms with an identical number of protons in their nuclei belong to the same chemical element. Atoms with equal numbers of protons but a different number of neutrons are different isotopes of the same element. For example, all hydrogen atoms admit exactly one proton, but isotopes exist with no neutrons (hydrogen-1, by far the most common form,[55]also called protium), one neutron (deuterium), two neutrons (tritium) and more than two neutrons. The known elements form a set of atomic numbers, from the single proton element hydrogen up to the 118-proton element oganesson.[56]All known isotopes of elements with atomic numbers greater than 82 are radioactive, although the radioactivity of element 83 (bismuth) is so slight as to be practically negligible.[57][58]About 339 nuclides occur naturally on Earth,[59]of which 254 (about 75%) have not been observed to decay, and are referred to as "stable isotopes". However, only 90 of these nuclides are stable to all decay, even in theory. Another 164 (bringing the total to 254) have not been observed to decay, even though in theory it is energetically possible. These are also formally classified as "stable". An additional 34 radioactive nuclides have half-lives longer than 80 million years, and are long-lived enough to be present from the birth of the solar system. This collection of 288 nuclides are known as primordial nuclides. Finally, an additional 51 short-lived nuclides are known to occur naturally, as daughter products of primordial nuclide decay (such as radium from uranium), or else as products of natural energetic processes on Earth, such as cosmic ray bombardment (for example, carbon-14).[60][note 1]For 80 of the chemical elements, at least one stable isotope exists. As a rule, there is only a handful of stable isotopes for each of these elements, the average being 3.2 stable isotopes per element. Twenty-six elements have only a single stable isotope, while the largest number of stable isotopes observed for any element is ten, for the element tin. Elements 43, 61, and all elements numbered 83 or higher have no stable isotopes.[61][page needed]Stability of isotopes is affected by the ratio of protons to neutrons, and also by the presence of certain "magic numbers" of neutrons or protons that represent closed and filled quantum shells. These quantum shells correspond to a set of energy levels within the shell model of the nucleus; filled shells, such as the filled shell of 50 protons for tin, confers unusual stability on the nuclide. Of the 254 known stable nuclides, only four have both an odd number of protons and odd number of neutrons: hydrogen-2 (deuterium), lithium-6, boron-10 and nitrogen-14. Also, only four naturally occurring, radioactive odd–odd nuclides have a half-life over a billion years: potassium-40, vanadium-50, lanthanum-138 and tantalum-180m. Most odd–odd nuclei are highly unstable with respect to beta decay, because the decay products are even–even, and are therefore more strongly bound, due to nuclear pairing effects.[61][page needed]MassThe large majority of an atom's mass comes from the protons and neutrons that make it up. The total number of these particles (called "nucleons") in a given atom is called the mass number. It is a positive integer and dimensionless (instead of having dimension of mass), because it expresses a count. An example of use of a mass number is "carbon-12," which has 12 nucleons (six protons and six neutrons).The actual mass of an atom at rest is often expressed using the unified atomic mass unit (u), also called dalton (Da). This unit is defined as a twelfth of the mass of a free neutral atom of carbon-12, which is approximately 1.66×10−27 kg.[62]Hydrogen-1 (the lightest isotope of hydrogen which is also the nuclide with the lowest mass) has an atomic weight of 1.007825 u.[63]The value of this number is called the atomic mass. A given atom has an atomic mass approximately equal (within 1%) to its mass number times the atomic mass unit (for example the mass of a nitrogen-14 is roughly 14 u). However, this number will not be exactly an integer except in the case of carbon-12 (see below).[64]The heaviest stable atom is lead-208,[57]with a mass of 207.9766521 u.[65]As even the most massive atoms are far too light to work with directly, chemists instead use the unit of moles. One mole of atoms of any element always has the same number of atoms (about 6.022×1023). This number was chosen so that if an element has an atomic mass of 1 u, a mole of atoms of that element has a mass close to one gram. Because of the definition of the unified atomic mass unit, each carbon-12 atom has an atomic mass of exactly 12 u, and so a mole of carbon-12 atoms weighs exactly 0.012 kg.[62]Shape and sizeAtoms lack a well-defined outer boundary, so their dimensions are usually described in terms of an atomic radius. This is a measure of the distance out to which the electron cloud extends from the nucleus.[66]However, this assumes the atom to exhibit a spherical shape, which is only obeyed for atoms in vacuum or free space. Atomic radii may be derived from the distances between two nuclei when the two atoms are joined in a chemical bond. The radius varies with the location of an atom on the atomic chart, the type of chemical bond, the number of neighboring atoms (coordination number) and a quantum mechanicalproperty known as spin.[67]On the periodic table of the elements, atom size tends to increase when moving down columns, but decrease when moving across rows (left to right).[68]Consequently, the smallest atom is helium with a radius of 32 pm, while one of the largest is caesium at 225 pm.[69]When subjected to external forces, like electrical fields, the shape of an atom may deviate from spherical symmetry. The deformation depends on the field magnitude and the orbital type of outer shell electrons, as shown by group-theoreticalconsiderations. Aspherical deviations might be elicited for instance in crystals, where large crystal-electrical fields may occur at low-symmetry lattice sites.[70][71]Significant ellipsoidal deformations have been shown to occur for sulfur ions[72]and chalcogenions[73]in pyrite-type compounds.Atomic dimensions are thousands of times smaller than the wavelengths of light (400–700 nm) so they cannot be viewed using an optical microscope. However, individual atoms can be observed using a scanning tunneling microscope. To visualize the minuteness of the atom, consider that a typical human hair is about 1 million carbon atoms in width.[74]A single drop of water contains about 2 sextillion (2×1021) atoms of oxygen, and twice the number of hydrogen atoms.[75]A single carat diamond with a mass of 2×10−4 kg contains about 10 sextillion (1022) atoms of carbon.[note 2]If an apple were magnified to the size of the Earth, then the atoms in the apple would be approximately the size of the original apple.[76]Radioactive decayThis diagram shows the half-life (T½) of various isotopes with Z protons and N neutrons.Every element has one or more isotopes that have unstable nuclei that are subject to radioactive decay, causing the nucleus to emit particles or electromagnetic radiation. Radioactivity can occur when the radius of a nucleus is large compared with the radius of the strong force, which only acts over distances on the order of 1 fm.[77]The most common forms of radioactive decay are:[78][79]Alpha decay: this process is caused when the nucleus emits an alpha particle, which is a helium nucleus consisting of two protons and two neutrons. The result of the emission is a new element with a lower atomic number.Beta decay (and electron capture): these processes are regulated by the weak force, and result from a transformation of a neutron into a proton, or a proton into a neutron. The neutron to proton transition is accompanied by the emission of an electron and an antineutrino, while proton to neutron transition (except in electron capture) causes the emission of a positron and a neutrino. The electron or positron emissions are called beta particles. Beta decay either increases or decreases the atomic number of the nucleus by one. Electron capture is more common than positron emission, because it requires less energy. In this type of decay, an electron is absorbed by the nucleus, rather than a positron emitted from the nucleus. A neutrino is still emitted in this process, and a proton changes to a neutron.Gamma decay: this process results from a change in the energy level of the nucleus to a lower state, resulting in the emission of electromagnetic radiation. The excited state of a nucleus which results in gamma emission usually occurs following the emission of an alpha or a beta particle. Thus, gamma decay usually follows alpha or beta decay.Other more rare types of radioactive decay include ejection of neutrons or protons or clusters of nucleons from a nucleus, or more than one beta particle. An analog of gamma emission which allows excited nuclei to lose energy in a different way, is internal conversion—a process that produces high-speed electrons that are not beta rays, followed by production of high-energy photons that are not gamma rays. A few large nuclei explode into two or more charged fragments of varying masses plus several neutrons, in a decay called spontaneous nuclear fission.Each radioactive isotope has a characteristic decay time period—the half-life—that is determined by the amount of time needed for half of a sample to decay. This is an exponential decay process that steadily decreases the proportion of the remaining isotope by 50% every half-life. Hence after two half-lives have passed only 25% of the isotope is present, and so forth.[77]Magnetic momentElementary particles possess an intrinsic quantum mechanical property known as spin. This is analogous to the angular momentum of an object that is spinning around its center of mass, although strictly speaking these particles are believed to be point-like and cannot be said to be rotating. Spin is measured in units of the reduced Planck constant (ħ), with electrons, protons and neutrons all having spin ½ ħ, or "spin-½". In an atom, electrons in motion around the nucleus possess orbital angular momentum in addition to their spin, while the nucleus itself possesses angular momentum due to its nuclear spin.[80]The magnetic field produced by an atom—its magnetic moment—is determined by these various forms of angular momentum, just as a rotating charged object classically produces a magnetic field. However, the most dominant contribution comes from electron spin. Due to the nature of electrons to obey the Pauli exclusion principle, in which no two electrons may be found in the same quantum state, bound electrons pair up with each other, with one member of each pair in a spin up state and the other in the opposite, spin down state. Thus these spins cancel each other out, reducing the total magnetic dipole moment to zero in some atoms with even number of electrons.[81]In ferromagnetic elements such as iron, cobalt and nickel, an odd number of electrons leads to an unpaired electron and a net overall magnetic moment. The orbitals of neighboring atoms overlap and a lower energy state is achieved when the spins of unpaired electrons are aligned with each other, a spontaneous process known as an exchange interaction. When the magnetic moments of ferromagnetic atoms are lined up, the material can produce a measurable macroscopic field. Paramagnetic materials have atoms with magnetic moments that line up in random directions when no magnetic field is present, but the magnetic moments of the individual atoms line up in the presence of a field.[81][82]The nucleus of an atom will have no spin when it has even numbers of both neutrons and protons, but for other cases of odd numbers, the nucleus may have a spin. Normally nuclei with spin are aligned in random directions because of thermal equilibrium. However, for certain elements (such as xenon-129) it is possible to polarize a significant proportion of the nuclear spin states so that they are aligned in the same direction—a condition called hyperpolarization. This has important applications in magnetic resonance imaging.[83][84]Energy levelsThese electron's energy levels (not to scale) are sufficient for ground states of atoms up to cadmium (5s24d10) inclusively. Do not forget that even the top of the diagram is lower than an unbound electron state.The potential energy of an electron in an atom is negative, its dependence of its positionreaches the minimum (the most absolute value) inside the nucleus, and vanishes when the distance from the nucleus goes to infinity, roughly in an inverse proportion to the distance. In the quantum-mechanical model, a bound electron can only occupy a set of states centered on the nucleus, and each state corresponds to a specific energy level; see time-independent Schrödinger equation for theoretical explanation. An energy level can be measured by the amount of energy needed to unbind the electron from the atom, and is usually given in units of electronvolts (eV). The lowest energy state of a bound electron is called the ground state, i.e. stationary state, while an electron transition to a higher level results in an excited state.[85]The electron's energy raises when n increases because the (average) distance to the nucleus increases. Dependence of the energy on ℓ is caused not by electrostatic potential of the nucleus, but by interaction between electrons.For an electron to transition between two different states, e.g. grounded state to first excited level (ionization), it must absorb or emit a photon at an energy matching the difference in the potential energy of those levels, according to Niels Bohr model, what can be precisely calculated by the Schrödinger equation. Electrons jump between orbitals in a particle-like fashion. For example, if a single photon strikes the electrons, only a single electron changes states in response to the photon; see Electron properties.The energy of an emitted photon is proportional to its frequency, so these specific energy levels appear as distinct bands in the electromagnetic spectrum.[86]Each element has a characteristic spectrum that can depend on the nuclear charge, subshells filled by electrons, the electromagnetic interactions between the electrons and other factors.[87]YAn example of absorption lines in a spectrumWhen a continuous spectrum of energy is passed through a gas or plasma, some of the photons are absorbed by atoms, causing electrons to change their energy level. Those excited electrons that remain bound to their atom spontaneously emit this energy as a photon, traveling in a random direction, and so drop back to lower energy levels. Thus the atoms behave like a filter that forms a series of dark absorption bands in the energy output. (An observer viewing the atoms from a view that does not include the continuous spectrum in the background, instead sees a series of emission lines from the photons emitted by the atoms.) Spectroscopic measurements of the strength and width of atomic spectral lines allow the composition and physical properties of a substance to be determined.[88]Close examination of the spectral lines reveals that some display a fine structure splitting. This occurs because of spin–orbit coupling, which is an interaction between the spin and motion of the outermost electron.[89]When an atom is in an external magnetic field, spectral lines become split into three or more components; a phenomenon called the Zeeman effect. This is caused by the interaction of the magnetic field with the magnetic moment of the atom and its electrons. Some atoms can have multiple electron configurations with the same energy level, which thus appear as a single spectral line. The interaction of the magnetic field with the atom shifts these electron configurations to slightly different energy levels, resulting in multiple spectral lines.[90]The presence of an external electric field can cause a comparable splitting and shifting of spectral lines by modifying the electron energy levels, a phenomenon called the Stark effect.[91]If a bound electron is in an excited state, an interacting photon with the proper energy can cause stimulated emission of a photon with a matching energy level. For this to occur, the electron must drop to a lower energy state that has an energy difference matching the energy of the interacting photon. The emitted photon and the interacting photon then move off in parallel and with matching phases. That is, the wave patterns of the two photons are synchronized. This physical property is used to make lasers, which can emit a coherent beam of light energy in a narrow frequency band.[92]Valence and bonding behaviorValency is the combining power of an element. It is equal to number of hydrogen atoms that atom can combine or displace in forming compounds.[93]The outermost electron shell of an atom in its uncombined state is known as the valence shell, and the electrons in that shell are called valence electrons. The number of valence electrons determines the bonding behavior with other atoms. Atoms tend to chemically react with each other in a manner that fills (or empties) their outer valence shells.[94]For example, a transfer of a single electron between atoms is a useful approximation for bonds that form between atoms with one-electron more than a filled shell, and others that are one-electron short of a full shell, such as occurs in the compound sodium chloride and other chemical ionic salts. However, many elements display multiple valences, or tendencies to share differing numbers of electrons in different compounds. Thus, chemical bonding between these elements takes many forms of electron-sharing that are more than simple electron transfers. Examples include the element carbon and the organic compounds.[95]The chemical elements are often displayed in a periodic table that is laid out to display recurring chemical properties, and elements with the same number of valence electrons form a group that is aligned in the same column of the table. (The horizontal rows correspond to the filling of a quantum shell of electrons.) The elements at the far right of the table have their outer shell completely filled with electrons, which results in chemically inert elements known as the noble gases.[96][97]StatesGraphic illustrating the formation of a Bose–Einstein condensateQuantities of atoms are found in different states of matter that depend on the physical conditions, such as temperature and pressure. By varying the conditions, materials can transition between solids, liquids, gases and plasmas.[98]Within a state, a material can also exist in different allotropes. An example of this is solid carbon, which can exist as graphite or diamond.[99]Gaseous allotropes exist as well, such as dioxygen and ozone.At temperatures close to absolute zero, atoms can form a Bose–Einstein condensate, at which point quantum mechanical effects, which are normally only observed at the atomic scale, become apparent on a macroscopic scale.[100][101]This super-cooled collection of atoms then behaves as a single super atom, which may allow fundamental checks of quantum mechanical behavior.[102]IdentificationScanning tunneling microscopeimage showing the individual atoms making up this gold (100) surface. The surface atoms deviate from the bulk crystal structure and arrange in columns several atoms wide with pits between them (See surface reconstruction).The scanning tunneling microscope is a device for viewing surfaces at the atomic level. It uses the quantum tunneling phenomenon, which allows particles to pass through a barrier that would normally be insurmountable. Electrons tunnel through the vacuum between two planar metal electrodes, on each of which is an adsorbed atom, providing a tunneling-current density that can be measured. Scanning one atom (taken as the tip) as it moves past the other (the sample) permits plotting of tip displacement versus lateral separation for a constant current. The calculation shows the extent to which scanning-tunneling-microscope images of an individual atom are visible. It confirms that for low bias, the microscope images the space-averaged dimensions of the electron orbitals across closely packed energy levels—the Fermi level local density of states.[103][104]An atom can be ionized by removing one of its electrons. The electric charge causes the trajectory of an atom to bend when it passes through a magnetic field. The radius by which the trajectory of a moving ion is turned by the magnetic field is determined by the mass of the atom. The mass spectrometer uses this principle to measure the mass-to-charge ratio of ions. If a sample contains multiple isotopes, the mass spectrometer can determine the proportion of each isotope in the sample by measuring the intensity of the different beams of ions. Techniques to vaporize atoms include inductively coupled plasma atomic emission spectroscopy and inductively coupled plasma mass spectrometry, both of which use a plasma to vaporize samples for analysis.[105]A more area-selective method is electron energy loss spectroscopy, which measures the energy loss of an electron beam within a transmission electron microscope when it interacts with a portion of a sample. The atom-probe tomograph has sub-nanometer resolution in 3-D and can chemically identify individual atoms using time-of-flight mass spectrometry.[106]Spectra of excited states can be used to analyze the atomic composition of distant stars. Specific light wavelengths contained in the observed light from stars can be separated out and related to the quantized transitions in free gas atoms. These colors can be replicated using a gas-discharge lamp containing the same element.[107]Helium was discovered in this way in the spectrum of the Sun 23 years before it was found on Earth.[108]Origin and current stateAtoms form about 4% of the total energy density of the observable Universe, with an average density of about 0.25 atoms/m3.[109]Within a galaxy such as the Milky Way, atoms have a much higher concentration, with the density of matter in the interstellar medium (ISM) ranging from 105to 109atoms/m3.[110]The Sun is believed to be inside the Local Bubble, a region of highly ionized gas, so the density in the solar neighborhood is only about 103atoms/m3.[111]Stars form from dense clouds in the ISM, and the evolutionary processes of stars result in the steady enrichment of the ISM with elements more massive than hydrogen and helium. Up to 95% of the Milky Way's atoms are concentrated inside stars and the total mass of atoms forms about 10% of the mass of the galaxy.[112](The remainder of the mass is an unknown dark matter.)[113]FormationElectrons are thought to exist in the Universe since early stages of the Big Bang. Atomic nuclei forms in nucleosynthesisreactions. In about three minutes Big Bang nucleosynthesis produced most of the helium, lithium, and deuterium in the Universe, and perhaps some of the beryllium and boron.[114][115][116]Ubiquitousness and stability of atoms relies on their binding energy, which means that an atom has a lower energy than an unbound system of the nucleus and electrons. Where the temperature is much higher than ionization potential, the matter exists in the form of plasma—a gas of positively charged ions (possibly, bare nuclei) and electrons. When the temperature drops below the ionization potential, atoms become statistically favorable. Atoms (complete with bound electrons) became to dominate over charged particles 380,000 years after the Big Bang—an epoch called recombination, when the expanding Universe cooled enough to allow electrons to become attached to nuclei.[117]Since the Big Bang, which produced no carbon or heavier elements, atomic nuclei have been combined in stars through the process of nuclear fusion to produce more of the element helium, and (via the triple alpha process) the sequence of elements from carbon up to iron;[118]see stellar nucleosynthesis for details.Isotopes such as lithium-6, as well as some beryllium and boron are generated in space through cosmic ray spallation.[119]This occurs when a high-energy proton strikes an atomic nucleus, causing large numbers of nucleons to be ejected.Elements heavier than iron were produced in supernovae through the r-process and in AGB stars through the s-process, both of which involve the capture of neutrons by atomic nuclei.[120]Elements such as lead formed largely through the radioactive decay of heavier elements.[121]EarthMost of the atoms that make up the Earth and its inhabitants were present in their current form in the nebula that collapsed out of a molecular cloud to form the Solar System. The rest are the result of radioactive decay, and their relative proportion can be used to determine the age of the Earth through radiometric dating.[122][123]Most of the helium in the crust of the Earth (about 99% of the helium from gas wells, as shown by its lower abundance of helium-3) is a product of alpha decay.[124]There are a few trace atoms on Earth that were not present at the beginning (i.e., not "primordial"), nor are results of radioactive decay. Carbon-14 is continuously generated by cosmic rays in the atmosphere.[125]Some atoms on Earth have been artificially generated either deliberately or as by-products of nuclear reactors or explosions.[126][127]Of the transuranic elements—those with atomic numbers greater than 92—only plutonium and neptunium occur naturally on Earth.[128][129]Transuranic elements have radioactive lifetimes shorter than the current age of the Earth[130]and thus identifiable quantities of these elements have long since decayed, with the exception of traces of plutonium-244 possibly deposited by cosmic dust.[122]Natural deposits of plutonium and neptunium are produced by neutron capture in uranium ore.[131]The Earth contains approximately 1.33×1050 atoms.[132]Although small numbers of independent atoms of noble gases exist, such as argon, neon, and helium, 99% of the atmosphere is bound in the form of molecules, including carbon dioxide and diatomic oxygen and nitrogen. At the surface of the Earth, an overwhelming majority of atoms combine to form various compounds, including water, salt, silicates and oxides. Atoms can also combine to create materials that do not consist of discrete molecules, including crystals and liquid or solid metals.[133][134]This atomic matter forms networked arrangements that lack the particular type of small-scale interrupted order associated with molecular matter.[135]Rare and theoretical forms

Yes, you can do it by some tricks,and fact here are some:Know the direction of increasing atomic mass. Atomic mass (the amount of matter in your atom) increases as you go to the right across a row, or down a column. The periodic table is ordered in such a way that each element has one proton more than the element before it, and the mass is the sum of protons and neutrons in an atom. Electrons are negligible when calculating mass because they possess so little in comparison to the larger particles.2Think about outer shell electrons. The inner shells of an atom’s electrons are full and stable. For the most part, they contribute little to the way the atom reacts. The largest factor in how an atom reacts is the makeup of its outer shell electrons. The periodic table naturally groups together elements with similar outer shells (Transition metals, halogens, etc.).3Consider how tightly an atom holds its electrons. For a number of reasons, an electron closer to the nucleus of an atom will generally be held tighter than an electron further out. Because of this, electronegativity (ability to accept and keep electrons) increases as you go to the right of a row and the top of a column. The noble gases (the column furthest to the right) are typically inert and do not accept or donate electrons.For example, fluorine is will more effectively gain electrons than bromine, even though they are both halogens.4Understand metallic and nonmetallic properties. The periodic table also groups elements into metals, non-metals, and metallic categories. Metals are usually shiny solids at room temperature, conduct well, and are malleable. Non-metals are usually dull in appearance, may be solid, gas, or liquid at room temperature, conduct poorly, and are not malleable. Metalloids share properties of metals and non-metals.There are also different groups of metals (alkali metals, transition metals, etc.).5Read the information in each block.Each block of the periodic table contains the atomic symbol if one of the elements. There is also a lot of information about the element in that block including things like mass number and average atomic weight. Learn to Read the periodic table well, and you will be on your way to understanding the elements it contains.Method Two of Four:Memorizing the Periodic Table1Use visualization techniques to remember elements. Your brain is designed to remember visuals more effectively than written or spoken words. Use this to your advantage by creating mental visualizations to go with each element. Then, you can create a storyline that likes each picture together in the order that you need to remember them. This is the most effective memorization technique.For example, you might drop your bottle of hydrogen peroxide (hydrogen), causing you to yell in a squeaky voice (helium makes your voice squeaky), right as it lands on a pack of batteries (lithium ion batteries to be exact). This helps you remember the order of elements within the periodic table.2Make up acronyms or acrostics to remember chunks of the periodic table. This is less effective than visual imagery, but can work better than brute force repetition. While acrostics are much easier to create for the elements, acronyms can be done, too. This will provide a cue for several elements in one word or phrase.An acrostic for nitrogen, oxygen, fluorine and neon might be something like No Openings For Ned. The first one or two letters of each word represent an element (N, O, F, Ne).HONClBrIF (pronounced honkle brief) is another acronym. This one helps you remember the elements that occur as diatomic molecules.A similar approach to acronyms and acrostics is to make a song that includes the names of the elements. This can be a little more effective, but is also more time consuming.3Employ brute force repetition. This method is least effective overall, and requires an intense amount of study time. It is best if the study time is broken up into smaller sessions. You will need to memorize small chunks of the table at one time and constantly review them while moving on to other chunks.If you choose this way, notecards are your best friend. For example, you could make a set of notecards for every element on the periodic table. Likewise, you could make a set of notecards that lists every family or group (column) and include the elements within each group on the card. To get the most out of the table, you could make several sets of notecards, such as the two mentioned, that organize the information in different ways.Method Three of Four:Utilizing Periodic Table Games and Activities1Take practice tests. Quiz yourself relentlessly on the periodic table. Practice tests are among the most effective study habits because they force your brain to recall the information that you have committed to memory. You can search for practice tests online, or print off versions of the periodic table that need some parts filled in.You can also write your own practice test questions or make your own tables. This takes more time, but you will be thinking even more about the periodic table by formulating the test. Just be sure to ask questions that you don’t know, too!2Reward yourself for knowing your notecards. You can play fun games with yourself by rewarding yourself each time you get a notecard correct. It does not have to be a big reward to be fun. Even just a piece of candy for each correct answer can break up the boredom of studying. You can also give yourself bigger rewards for getting bigger chunks of information correct.3Use online games. There are several educational games online. Go to Google and type in “periodic table games and activities” and you will find an array of free games that help you learn the periodic table. Choose one you like and start playing.Method Four of Four:Improving Your Study Habits1Make and keep a study schedule. A solid study schedule is a good way to make sure that you are spreading out your study time. It will help you remain disciplined in your studies and keep you motivated on days that you are less than excited to look at the periodic table again. While there’s no set rule on how much time it will take you to learn about the elements on the table, you should expect to set aside about two hours of study time for every hour of class time dedicated to the periodic table.2Know what kind of learning style you have. There are many different ways to expose yourself to new material, and most people prefer one or two over the others. In the classroom, the instructor often dictates how material will be presented. However, during your study time, you should strive to present yourself with material in the way that you learn it best. The different learning types are:Visual - You prefer to include pictures, images, videos, etc.Auditory - You like hearing information and/or integrating music and sounds.Linguistic - You learn information when it is in the form of language (written or spoken).Kinesthetic - You are a “hands on” learner. Movement and physical touch help you retain information.Mathematical - You rely on systems of logic to learn.Interpersonal - Most of your learning occurs in a group setting.Intrapersonal - Learning alone suits you best.3Spread out your studying. Research shows that cramming does not work. You will retain much more information with the same amount of study time if you spread it out over the course of days or weeks. Divide the periodic table into easy to conquer goals and learn it slowly over time. You should also take a study break every forty-five minutes or so to let your brain rest.Be sure that you go back and review material that you have already learned from time to time. If you keep moving on to new material without reviewing the old, you are likely to forget some important details.This can be a great way to use your notecards. Keep them handy, and when you find yourself with a few minutes to kill in a waiting room or between classes, pull them out and put that time to use.4Spend time studying in a group. Even if you prefer to study alone, you can benefit from a little bit of group study. This is where you will see different points of view on the same material and expand your understanding of the periodic table. Other students may notice trends that you weren’t familiar with, or they might have unique ways of learning the elements. Be sure that you contribute your ideas and knowledge to the group as well.Another way that you can utilize social learning is to teach someone else about the periodic table. As you teach them, you will become more familiar and comfortable with the table yourself.If you are struggling with learning the periodic table, you can also consider finding a private tutor.Sometimes the class will move on and you will simply be given the assignment to learn certain parts of the periodic table.5Get enough sleep every night. The periodic table is full of vast amounts of information on chemical elements, groups, and recurring trends that are found in similar elements. This can be a lot of information to commit to memory, and information is best organized and retained in your brain during sleep. Staying rested by getting seven to nine hours of sleep per night will do wonders for your study results.6Use unique scents to activate your memory. Your brain’s memory system is closely tied to your olfactory sense (sense of smell). You can use this to your advantage by studying in the presence of a unique (ideally inoffensive) smell. If you then take an exam in the presence of the same smell, it will spur your brain to pull of the information from your study sessions