The periodic table is a tabular arrangement of the chemical elements, organized on the basis of their atomic numbers,electron configurations (electron shell model), and recurring chemical
properties. Elements are presented in order of increasing atomic number
(the number of protons in the nucleus). The standard form of the table
consists of a grid of elements laid out in 18 columns and 7 rows, with a
double row of elements below that. The table can also be deconstructed
into four rectangular blocks: the s-block to the left, the p-block to the right, the d-block in the middle, and the f-block below that.
The rows of the table are called periods; the columns are called groups, with some of these having names such as halogensor noble gases. Since, by definition, a periodic table incorporates recurring
trends, any such table can be used to derive relationships between the
properties of the elements and predict the properties of new, yet to be
discovered or synthesized, elements. As a result, a periodic
table—whether in the standard form or some other variant—provides a
useful framework for analyzing chemical behavior, and such tables are
widely used in chemistry and other sciences.
Although precursors exist, Dmitri Mendeleev is
generally credited with the publication, in 1869, of the first widely
recognized periodic table. He developed his table to illustrate periodic
trends in the properties of the then-known elements. Mendeleev also
predicted some properties of then-unknown elements that
would be expected to fill gaps in this table. Most of his predictions
were proved correct when the elements in question were subsequently
discovered. Mendeleev's periodic table has since been expanded and
refined with the discovery or synthesis of further new elements and the development of new theoretical models to explain chemical behavior.
All
elements from atomic numbers 1 (hydrogen) to 118 (ununoctium) have been
discovered or reportedly synthesized, with elements 113, 115, 117 and
118 having yet to be confirmed. The first 98 elements exist naturally
although some are
found only in trace amounts and were initially discovered by synthesis
in laboratories. Elements with atomic numbers from 99 to 118 have only
been synthesized, or claimed to be so, in laboratories. Production of
elements having higher atomic numbers is being pursued, with the
question of how the periodic table may need to be modified to
accommodate any such additions being a matter of ongoing debate.
Numerous synthetic radionuclides of naturally occurring elements have also been produced in laboratories.
All versions of the periodic table include only chemical elements, not mixtures, compounds, or subatomic particles. Each chemical element has a unique atomic number representing the number of protons in its nucleus. Most elements have differing numbers of neutrons among different atoms, with these variants being referred to as isotopes. For example, carbon has three naturally occurring isotopes: all of its atoms have six protons and most have six neutrons as well, but about one per cent have seven neutrons, and a very small fraction have eight neutrons. Isotopes are never separated in the periodic table; they are always grouped together under a single element. Elements with no stable isotopes have the atomic masses of their most stable isotopes, where such masses are shown, listed in parentheses.
In the standard periodic table, the elements are listed in order of increasing atomic number (the number of protons in the nucleus of an atom). A new row (period) is started when a new electron shell has its first electron. Columns (groups) are determined by the electron configuration of the atom; elements with the same number of electrons in a particular subshell fall into the same columns (e.g. oxygen and selenium are in the same column because they both have four electrons in the outermost p-subshell). Elements with similar chemical properties generally fall into the same group in the periodic table, although in the f-block, and to some respect in the d-block, the elements in the same period tend to have similar properties, as well. Thus, it is relatively easy to predict the chemical properties of an element if one knows the properties of the elements around it.
As of 2013, the periodic table has 114 confirmed elements, comprising elements 1 (hydrogen) to 112 (copernicium), 114 (flerovium) and 116 (livermorium). Elements 113, 115, 117 and 118 have reportedly been synthesised in laboratories however none of these claims have been officially confirmed by the International Union of Pure and Applied Chemistry (IUPAC). As such these elements are currently known only by their systematic element names, based on their atomic numbers.
A total of 98 elements occur naturally; the remaining 16 elements, from einsteinium to copernicium, and flerovium and livermorium, occur only when synthesised in laboratories. Of the 98 elements that occur naturally, 84 are primordial. The other 14 elements occur only in decay chains of primordial elements. No element heavier than einsteinium (element 99) has ever been observed in macroscopic quantities in its pure form.
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