Atomic Number 8



Before a name and symbol are approved, an element may be referred to by its atomic number (e.g., element 120) or by its systematic element name. The systematic element name is a temporary name that is based on the atomic number as a root and the -ium ending as a suffix. For example, element 120 has the temporary name unbinilium. As the electronic configuration of the given atom is 2,8,7 it is inferred that the atomic number of element is 17 (2+8+7). Thus element with atomic number 17 is Chlorine. Among the options given which includes Nitrogen, Fluorine, Phosphorus and Argon, chlorine is chemically similar to fluorine.

  1. Atomic Number 81
  2. More Images For Atomic Number 8 »
  3. Atomic Number 89
  4. Atomic Number 84

How many neutrons will an atom of oxygen (atomic number 8) with an atomic mass of 16 have?

1 Answer

Explanation:

You have got an oxygen ATOM, for which #Z=8#. And what is #Z#? It is the #'atomic number'#, the number of massive, positively charged particles that comprise the oxygen nucleus. The oxygen nucleus also contains NEUTRONS, massive particles of ZERO charge. Interactions between protons and neutrons, at impossibly short nuclear ranges, constitute the strong nuclear force, an attractive force that is strong enuff to overcome the electrostatic force of repulsion between particles of LIKE electric charge.

Now there may be various numbers of neutrons within the atom of an element. And this gives rise to the phenomenon of isotopes; i.e. #'^16O#, #'^17O#, #'^18O#..all of these are oxygen atoms, and so they ALL have 8 nuclear protons, BUT they have #8#, #9#, and #10# neutrons respectively...giving rise the superscript that is added to the atomic symbol..

For garden variety #'^16O#, which accounts for 99% of oxygen, there are necessarily the 8 neutrons...

Related questions

Quantum Numbers,
Atomic Orbitals, and
Electron Configurations

Contents:
Quantum Numbers and Atomic Orbitals
1. Principal Quantum Number (n)
2.Angular Momentum (Secondary, Azimunthal) Quantum Number (l)
3.Magnetic Quantum Number (ml)
4.Spin Quantum Number (ms)
Table of Allowed Quantum Numbers
Writing Electron Configurations
Properties of Monatomic Ions
References

Quantum Numbers and Atomic Orbitals

By solving the Schrödinger equation (Hy = Ey), we obtain a set of mathematical equations, called wave functions (y), which describe the probability of finding electrons at certain energy levels within an atom.

A wave function for an electron in an atom is called an atomic orbital; this atomic orbital describes a region of space in which there is a high probability of finding the electron. Energy changes within an atom are the result of an electron changing from a wave pattern with one energy to a wave pattern with a different energy (usually accompanied by the absorption or emission of a photon of light).

Each electron in an atom is described by four different quantum numbers. The first three (n, l, ml) specify the particular orbital of interest, and the fourth (ms) specifies how many electrons can occupy that orbital.

  1. Principal Quantum Number (n): n = 1, 2, 3, …,
    Specifies the energy of an electron and the size of the orbital (the distance from the nucleus of the peak in a radial probability distribution plot). All orbitals that have the same value of n are said to be in the same shell (level). For a hydrogen atom with n=1, the electron is in its ground state; if the electron is in the n=2 orbital, it is in an excited state. The total number of orbitals for a given n value is n2.
  1. Angular Momentum (Secondary, Azimunthal) Quantum Number (l): l = 0, .., n-1.
    Specifies the shape of an orbital with a particular principal quantum number. The secondary quantum number divides the shells into smaller groups of orbitals called subshells (sublevels). Usually, a letter code is used to identify l to avoid confusion with n:

Atomic Number 81

l012345..
Letterspdfgh..

The subshell with n=2 and l=1 is the 2p subshell; if n=3 and l=0, it is the 3s subshell, and so on. The value of l also has a slight effect on the energy of the subshell; the energy of the subshell increases with l (s < p < d < f).

  1. Magnetic Quantum Number (ml): ml = -l, .., 0, .., +l.
    Specifies the orientation in space of an orbital of a given energy (n) and shape (l). This number divides the subshell into individual orbitals which hold the electrons; there are 2l+1 orbitals in each subshell. Thus the s subshell has only one orbital, the p subshell has three orbitals, and so on.
Beryllium
  1. Spin Quantum Number (ms): ms = +½ or -½.
    Specifies the orientation of the spin axis of an electron. An electron can spin in only one of two directions (sometimes called up and down).
    The Pauli exclusion principle (Wolfgang Pauli, Nobel Prize 1945) states that no two electrons in the same atom can have identical values for all four of their quantum numbers. What this means is that no more than two electrons can occupy the same orbital, and that two electrons in the same orbital must have opposite spins.
    Because an electron spins, it creates a magnetic field, which can be oriented in one of two directions. For two electrons in the same orbital, the spins must be opposite to each other; the spins are said to be paired. These substances are not attracted to magnets and are said to be diamagnetic. Atoms with more electrons that spin in one direction than another contain unpaired electrons. These substances are weakly attracted to magnets and are said to be paramagnetic.

Table of Allowed Quantum Numbers

nlmlNumber of
orbitals
Orbital
Name
Number of
electrons
10011s2
20012s2
1-1, 0, +132p6
30013s2
1-1, 0, +133p6
2-2, -1, 0, +1, +253d10
40014s2
1-1, 0, +134p6
2-2, -1, 0, +1, +254d10
3-3, -2, -1, 0, +1, +2, +374f14

Writing Electron Configurations

The distribution of electrons among the orbitals of an atom is called the electron configuration. The electrons are filled in according to a scheme known as the Aufbau principle ('building-up'), which corresponds (for the most part) to increasing energy of the subshells:

1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s, 5f

It is not necessary to memorize this listing, because the order in which the electrons are filled in can be read from the periodic table in the following fashion:

Or, to summarize:

In electron configurations, write in the orbitals that are occupied by electrons, followed by a superscript to indicate how many electrons are in the set of orbitals (e.g., H 1s1)

Starbound download for mac. Another way to indicate the placement of electrons is an orbital diagram, in which each orbital is represented by a square (or circle), and the electrons as arrows pointing up or down (indicating the electron spin). When electrons are placed in a set of orbitals of equal energy, they are spread out as much as possible to give as few paired electrons as possible (Hund's rule).

Atomic

examples will be added at a later date

In a ground state configuration, all of the electrons are in as low an energy level as it is possible for them to be. When an electron absorbs energy, it occupies a higher energy orbital, and is said to be in an excited state.

Properties of Monatomic Ions

The electrons in the outermost shell (the ones with the highest value of n) are the most energetic, and are the ones which are exposed to other atoms. This shell is known as the valence shell. The inner, core electrons (inner shell) do not usually play a role in chemical bonding.

Elements with similar properties generally have similar outer shell configurations. For instance, we already know that the alkali metals (Group I) always form ions with a +1 charge; the 'extra' s1 electron is the one that's lost:

IALi1s22s1Li+1s2
Na1s22s22p63s1Na+1s22s22p6
K1s22s22p63s23p64s1K+1s22s22p63s23p6

The next shell down is now the outermost shell, which is now full — meaning there is very little tendency to gain or lose more electrons. The ion's electron configuration is the same as the nearest noble gas — the ion is said to be isoelectronic with the nearest noble gas. Atoms 'prefer' to have a filled outermost shell because this is more electronically stable.

  • The Group IIA and IIIA metals also tend to lose all of their valence electrons to form cations.
Number
IIABe1s22s2Be2+1s2
Mg1s22s22p63s2Mg2+1s22s22p6
IIIAAl1s22s22p63s23p1Al3+1s22s22p6
  • The Group IV and V metals can lose either the electrons from the p subshell, or from both the s and p subshells, thus attaining a pseudo-noble gas configuration.

More Images For Atomic Number 8 »

IVASn[Kr]4d105s25p2Sn2+[Kr]4d105s2
Sn4+[Kr]4d10
Pb[Xe]4f145d106s26p2Pb2+[Xe]4f145d106s2
Pb4+[Xe]4f145d10
VABi[Xe]4f145d106s26p3Bi3+[Xe]4f145d106s2
Bi5+[Xe]4f145d10
  • The Group IV - VII non-metals gain electrons until their valence shells are full (8 electrons).
IVAC1s22s22p2C4-1s22s22p6
VAN1s22s22p3N3-1s22s22p6
VIAO1s22s22p4O2-1s22s22p6
VIIAF1s22s22p5F-1s22s22p6

Atomic Number 89

  • The Group VIII noble gases already possess a full outer shell, so they have no tendency to form ions.
  • Transition metals (B-group) usually form +2 charges from losing the valence s electrons, but can also lose electrons from the highest d level to form other charges.
B-groupFe1s22s22p63s23p63d64s2Fe2+1s22s22p63s23p63d6
Fe3+1s22s22p63s23p63d5

References

Martin S. Silberberg, Chemistry: The Molecular Nature of Matter and Change, 2nd ed. Boston: McGraw-Hill, 2000, p. 277-284, 293-307.

Atomic Number 84