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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Function describing an electron in an atom}}&lt;br /&gt;
&lt;br /&gt;
{{Quantum matter backlink|Atoms}}&lt;br /&gt;
&lt;br /&gt;
An &amp;#039;&amp;#039;&amp;#039;atomic orbital&amp;#039;&amp;#039;&amp;#039; is a quantum-mechanical function describing the location, wave-like behavior, and probability distribution of an [[Physics:Quantum atoms/electron|electron]] in an [[Physics:Quantum atoms/atom|atom]].&amp;lt;ref&amp;gt;{{cite book |last1=Orchin |first1=Milton |last2=MacOmber |first2=Roger S. |last3=Pinhas |first3=Allan R. |last4=Wilson |first4=R. Marshall |title=The Vocabulary and Concepts of Organic Chemistry |chapter=Atomic Orbital Theory |date=2005 |pages=1–24 |doi=10.1002/0471713740.ch1 |isbn=978-0-471-68028-4 }}&amp;lt;/ref&amp;gt; Orbitals are central to [[Physics:Quantum atoms/electron configuration|electron configuration]], chemical bonding, and atomic spectra.&lt;br /&gt;
[[File:Electron_configuration.png|thumb|450px|right|Atomic orbitals describe the probability clouds in which electrons are likely to be found around a nucleus.]]&lt;br /&gt;
== Description ==&lt;br /&gt;
In [[Physics:Quantum mechanics|quantum mechanics]], an orbital is not a fixed path followed by an electron. Instead, it is a wave function whose squared magnitude gives the probability density for finding the electron in a region around the nucleus.&amp;lt;ref&amp;gt;{{cite book |last=Daintith |first=J. |url=https://archive.org/details/dictionaryofchem0000unse_r3p4/page/408/mode/2up?view=theater |title=Oxford Dictionary of Chemistry |publisher=Oxford University Press |year=2004 |isbn=978-0-19-860918-6 |location=New York |pages=407–409}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Atomic orbitals are characterized by quantum numbers. The principal quantum number {{mvar|n}} is related to the shell and energy scale. The azimuthal quantum number {{mvar|ℓ}} determines the orbital type and angular momentum. The magnetic quantum number {{mvar|m&amp;lt;sub&amp;gt;ℓ&amp;lt;/sub&amp;gt;}} describes orientation. A fourth quantum number, the spin projection {{mvar|m&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;}}, describes electron spin.&lt;br /&gt;
&lt;br /&gt;
An orbital can contain at most two electrons, and those two electrons must have opposite spin according to the Pauli exclusion principle.&amp;lt;ref&amp;gt;{{cite book |last1=Levine |first1=Ira N. |title=Quantum Chemistry |date=1991 |publisher=Prentice-Hall |isbn=0-205-12770-3 |page=262 |edition=4th}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Electron properties ==&lt;br /&gt;
Electrons in atoms show both wave-like and particle-like behavior.&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Wave-like properties include:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
* electrons form standing-wave states around the nucleus&lt;br /&gt;
* the electron position is described probabilistically&lt;br /&gt;
* orbital shapes arise from wave interference and boundary conditions&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Particle-like properties include:&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
* electrons carry a definite electric charge&lt;br /&gt;
* electrons occupy discrete quantum states&lt;br /&gt;
* transitions between orbitals involve absorption or emission of photons&lt;br /&gt;
&lt;br /&gt;
This wave-particle behavior is why orbitals are often visualized as electron clouds rather than planetary orbits.&lt;br /&gt;
&lt;br /&gt;
== Quantum numbers ==&lt;br /&gt;
Atomic orbitals are labeled by quantum numbers:&lt;br /&gt;
&lt;br /&gt;
* {{mvar|n}} — principal quantum number; shell, size, and energy scale&lt;br /&gt;
* {{mvar|ℓ}} — azimuthal quantum number; orbital shape and angular momentum&lt;br /&gt;
* {{mvar|m&amp;lt;sub&amp;gt;ℓ&amp;lt;/sub&amp;gt;}} — magnetic quantum number; orbital orientation&lt;br /&gt;
* {{mvar|m&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;}} — spin quantum number; electron spin projection&lt;br /&gt;
&lt;br /&gt;
The allowed values are restricted:&lt;br /&gt;
&lt;br /&gt;
* {{mvar|n}} = 1, 2, 3, ...&lt;br /&gt;
* {{mvar|ℓ}} = 0 to {{mvar|n}} − 1&lt;br /&gt;
* {{mvar|m&amp;lt;sub&amp;gt;ℓ&amp;lt;/sub&amp;gt;}} = −{{mvar|ℓ}} to +{{mvar|ℓ}}&lt;br /&gt;
* {{mvar|m&amp;lt;sub&amp;gt;s&amp;lt;/sub&amp;gt;}} = +1/2 or −1/2&lt;br /&gt;
&lt;br /&gt;
The Pauli exclusion principle states that no two electrons in the same atom can have the same set of all four quantum numbers.&lt;br /&gt;
&lt;br /&gt;
== Orbital names ==&lt;br /&gt;
Orbitals are named using the principal quantum number followed by a letter representing {{mvar|ℓ}}:&lt;br /&gt;
&lt;br /&gt;
* {{mvar|ℓ}} = 0: s orbital&lt;br /&gt;
* {{mvar|ℓ}} = 1: p orbital&lt;br /&gt;
* {{mvar|ℓ}} = 2: d orbital&lt;br /&gt;
* {{mvar|ℓ}} = 3: f orbital&lt;br /&gt;
&lt;br /&gt;
The labels s, p, d, and f come from early spectroscopic descriptions: sharp, principal, diffuse, and fundamental. For {{mvar|ℓ}} values above 3, the letters continue alphabetically as g, h, i, k, and so on.&amp;lt;ref&amp;gt;{{cite book|first=David|last=Griffiths|year=1995|title=Introduction to Quantum Mechanics|pages=190–191|publisher=Prentice Hall|isbn=978-0-13-124405-4}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite book|first=Ira|last=Levine|year=2000|title=Quantum Chemistry|edition=5|pages=[https://archive.org/details/quantumchemistry00levi_0/page/144 144–145]|publisher=Prentice Hall|isbn=978-0-13-685512-5|url=https://archive.org/details/quantumchemistry00levi_0/page/144}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite book|url=https://books.google.com/books?id=QbQJAgAAQBAJ&amp;amp;pg=PA106|title=Quanta, Matter, and Change: A Molecular Approach to Physical Chemistry|publisher=Oxford University Press|isbn=978-0-19-920606-3|year=2009|page=106|first1=Peter |last1=Atkins |first2=Julio |last2=de Paula |first3=Ronald |last3=Friedman}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Shapes of orbitals ==&lt;br /&gt;
The simplest orbital is the s orbital, which is spherically symmetric. The p orbitals have two lobes and are oriented along different axes. The d and f orbitals have more complex lobed shapes.&lt;br /&gt;
&lt;br /&gt;
Orbital images usually show surfaces enclosing regions where the electron has a high probability of being found. These diagrams do not show fixed paths; they show probability distributions.&lt;br /&gt;
&lt;br /&gt;
The number and arrangement of nodes are determined by quantum numbers. Nodal surfaces are regions where the probability density is zero.&lt;br /&gt;
&lt;br /&gt;
== Hydrogen-like orbitals ==&lt;br /&gt;
The simplest exact orbitals are those of hydrogen-like atoms, which contain one electron. In such systems, the Schrödinger equation can be solved analytically.&lt;br /&gt;
&lt;br /&gt;
Hydrogen-like orbitals are described using a radial part and an angular part:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\psi(r,\theta,\phi)=R(r)\Theta(\theta)\Phi(\phi)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For atoms with more than one electron, exact analytical solutions are not generally possible. Approximation methods such as Hartree–Fock theory and molecular orbital theory are used.&lt;br /&gt;
&lt;br /&gt;
== Orbital energy ==&lt;br /&gt;
In one-electron atoms, orbital energy depends mainly on {{mvar|n}}. In multi-electron atoms, electron-electron interactions make the energy depend also on {{mvar|ℓ}}.&lt;br /&gt;
&lt;br /&gt;
This explains why the filling order of orbitals in many-electron atoms is not simply 1s, 2s, 2p, 3s, 3p, 3d, and so on. Instead, the approximate filling sequence begins:&lt;br /&gt;
&lt;br /&gt;
:1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p&lt;br /&gt;
&lt;br /&gt;
This sequence is closely related to the structure of the periodic table and to [[Physics:Quantum atoms/electron configuration|electron configuration]].&lt;br /&gt;
&lt;br /&gt;
== Electron configuration ==&lt;br /&gt;
Orbitals provide the framework for electron configuration. Electrons fill orbitals according to quantum rules such as:&lt;br /&gt;
&lt;br /&gt;
* the Pauli exclusion principle&lt;br /&gt;
* Hund’s rule&lt;br /&gt;
* the Aufbau principle&lt;br /&gt;
&lt;br /&gt;
The repeating structure of the periodic table arises because complete sets of s, p, d, and f orbitals can hold 2, 6, 10, and 14 electrons respectively.&lt;br /&gt;
&lt;br /&gt;
== Transitions between orbitals ==&lt;br /&gt;
Electrons can move between orbital states by absorbing or emitting photons. Such transitions occur only when the photon energy matches the energy difference between the two states.&lt;br /&gt;
&lt;br /&gt;
These transitions produce spectral lines and are central to atomic spectroscopy.&lt;br /&gt;
&lt;br /&gt;
== History ==&lt;br /&gt;
Early atomic models treated electrons as orbiting particles. J. J. Thomson discovered the electron in 1897.&amp;lt;ref name=&amp;quot;referenceC&amp;quot;&amp;gt;{{cite journal |last1=Thomson |first1=J. J. |title=XL. Cathode Rays |journal=The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science |date=October 1897 |volume=44 |issue=269 |pages=293–316 |doi=10.1080/14786449708621070 }}&amp;lt;/ref&amp;gt; Hantaro Nagaoka proposed an orbit-based model in 1904.&amp;lt;ref name=&amp;quot;Nagaoka 1904 445–455&amp;quot;&amp;gt;{{cite journal |last1=Nagaoka |first1=H. |title=LV. Kinetics of a system of particles illustrating the line and the band spectrum and the phenomena of radioactivity |journal=The London, Edinburgh, and Dublin Philosophical Magazine and Journal of Science |date=May 1904 |volume=7 |issue=41 |pages=445–455 |doi=10.1080/14786440409463141 }}&amp;lt;/ref&amp;gt; Niels Bohr later introduced quantized electron orbits in 1913.&amp;lt;ref name=&amp;quot;Bohr 1913 476&amp;quot;&amp;gt;{{cite journal |last1=Nicholson |first1=J. W. |title=The Constitution of Atoms and Molecules |journal=Nature |date=May 1914 |volume=93 |issue=2324 |pages=268–269 |doi=10.1038/093268a0 |bibcode=1914Natur..93..268N |doi-access=free }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The modern orbital concept emerged after the development of quantum mechanics, de Broglie matter waves, the Schrödinger equation, and Heisenberg’s uncertainty principle.&amp;lt;ref&amp;gt;{{cite journal |last1=Heisenberg |first1=W. |title=Über den anschaulichen Inhalt der quantentheoretischen Kinematik und Mechanik |journal=Zeitschrift für Physik |date=March 1927 |volume=43 |issue=3–4 |pages=172–198 |doi=10.1007/BF01397280 |bibcode=1927ZPhy...43..172H }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite journal|last=Bohr | first=Niels| title=The Quantum Postulate and the Recent Development of Atomic Theory|journal=Nature |date=April 1928| volume=121 | pages=580–590|doi=10.1038/121580a0 |bibcode = 1928Natur.121..580B| issue=3050 |doi-access=free}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The term &amp;#039;&amp;#039;orbital&amp;#039;&amp;#039; was introduced by Robert S. Mulliken in 1932 as a shortened form of &amp;#039;&amp;#039;one-electron orbital wave function&amp;#039;&amp;#039;.&amp;lt;ref&amp;gt;{{cite journal |last1=Mulliken |first1=Robert S. |title=Electronic Structures of Polyatomic Molecules and Valence. II. General Considerations |journal=Physical Review |date=July 1932 |volume=41 |issue=1 |pages=49–71 |doi=10.1103/PhysRev.41.49 |bibcode=1932PhRv...41...49M }}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite journal |last1=Murrell |first1=John N |title=The origins and later developments of molecular orbital theory |journal=International Journal of Quantum Chemistry |date=5 September 2012 |volume=112 |issue=17 |pages=2875–2879 |doi=10.1002/qua.23293 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Properties ==&lt;br /&gt;
&lt;br /&gt;
* describes electron probability density&lt;br /&gt;
* linked to [[Physics:Quantum atoms/energy level|energy levels]]&lt;br /&gt;
* determines chemical behavior&lt;br /&gt;
* provides the basis for [[Physics:Quantum atoms/electron configuration|electron configuration]]&lt;br /&gt;
* classified as s, p, d, f, and higher orbitals&lt;br /&gt;
* each orbital holds at most two electrons&lt;br /&gt;
* transitions between orbitals produce spectral lines&lt;br /&gt;
&lt;br /&gt;
=See also=&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also/Matter}}&lt;br /&gt;
&lt;br /&gt;
=References=&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
{{Sourceattribution|Atomic orbital|1}}&lt;/div&gt;</summary>
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