Describe the electronic configurations of atoms 19. Electronic configurations of atoms of the elements of the Periodic system. Distribution of electrons using the periodic system of D. I. Mendeleev

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6.6. Features of the electronic structure of atoms of chromium, copper and some other elements

If you carefully looked at Appendix 4, you probably noticed that the sequence of filling the orbitals with electrons is violated in the atoms of some elements. Sometimes these violations are called "exceptions", but they are not - there are no exceptions to the laws of Nature!

The first element with this violation is chrome. Let's consider in more detail its electronic structure (Fig. 6.16 a). The chromium atom has 4 s-sub-level not two, as one would expect, but only one electron. But at 3 d-sublevel five electrons, but this sublevel is filled after 4 s-sublevel (see Fig. 6.4). To understand why this is happening, let's see what electron clouds are 3 d is the sublevel of this atom.

Each of five 3 d-clouds in this case is formed by one electron. As you already know from § 4 of this chapter, the total electron cloud of these five electrons has a spherical shape, or, as they say, spherically symmetric. By the nature of the electron density distribution in different directions, it is similar to 1 s-EO. The energy of the sublevel, the electrons of which form such a cloud, turns out to be less than in the case of a less symmetric cloud. In this case, the energy of the orbitals is 3 d-sublevel is equal to energy 4 s-orbital. When symmetry is broken, for example, when the sixth electron appears, the energy of the orbitals is 3 d-sublevel again becomes larger than energy 4 s-orbital. Therefore, the manganese atom again has a second electron by 4 s-AO.
The general cloud of any sublevel, filled with electrons, both half and completely, has spherical symmetry. The decrease in energy in these cases is of a general nature and does not depend on whether any sublevel is half or completely filled with electrons. And if so, then we should look for the next violation in the atom, into the electronic shell of which the ninth "comes" last d-electron. Indeed, the copper atom has 3 d-sublayer 10 electrons, and on 4 s- there is only one sublevel (Fig. 6.16 b).
The decrease in the energy of the orbitals of a fully or half-filled sublevel is the cause of a number of important chemical phenomena, some of which you will become familiar with.

6.7. Outer and valence electrons, orbitals and sublevels

In chemistry, the properties of isolated atoms, as a rule, are not studied, since almost all atoms, being part of various substances, form chemical bonds. Chemical bonds are formed when the electronic shells of atoms interact. For all atoms (except for hydrogen), not all electrons take part in the formation of chemical bonds: boron has three electrons out of five, carbon has four out of six, and, for example, barium has two out of fifty-six. These "active" electrons are called valence electrons.

Sometimes valence electrons are confused with external electrons, and they are not the same thing.

The electron clouds of the outer electrons have the maximum radius (and the maximum value of the principal quantum number).

It is the outer electrons that take part in the formation of a bond in the first place, if only because when the atoms approach each other, the electron clouds formed by these electrons come into contact first of all. But together with them, part of the electrons can take part in the formation of a bond. pre-external(penultimate) layer, but only if they have an energy that does not differ much from the energy of the outer electrons. Both those and other electrons of an atom are valence. (In lanthanides and actinides, even some "pre-external" electrons are valence)
The energy of valence electrons is much higher than the energy of other electrons of the atom, and valence electrons differ significantly less in energy from each other.
External electrons are always valence only if the atom can form chemical bonds at all. So, both electrons of the helium atom are external, but they cannot be called valence, since the helium atom does not form any chemical bonds at all.
Valence electrons occupy valence orbitals, which in turn form valence sublevels.

As an example, consider an iron atom, the electronic configuration of which is shown in Fig. 6.17. Of the electrons of the iron atom, the maximum principal quantum number ( n= 4) have only two 4 s-electron. Therefore, it is they who are the outer electrons of this atom. The outer orbitals of the iron atom are all orbitals with n= 4, and the outer sublevels are all sublevels formed by these orbitals, that is, 4 s-, 4p-, 4d- and 4 f-EPU.
The outer electrons are always valence, therefore 4 s-electrons of the iron atom - valence electrons. And if so, then 3 d-electrons with slightly higher energy will also be valence. At the outer level of the iron atom, in addition to the filled 4 s-AO there are still free 4 p-, 4d- and 4 f-AO. They are all external, but there are only 4 valences among them. R-AO, since the energy of the other orbitals is much higher, and the appearance of electrons in these orbitals is not beneficial for the iron atom.

So, the atom of iron
external electronic level - fourth,
external sublevels - 4 s-, 4p-, 4d- and 4 f-EPU,
outer orbitals - 4 s-, 4p-, 4d- and 4 f-AO,
outer electrons - two 4 s-electron (4 s 2),
outer electron layer - fourth,
external electronic cloud - 4 s-EO
valence sublevels - 4 s-, 4p-, and 3 d-EPU,
valence orbitals - 4 s-, 4p-, and 3 d-AO,
valence electrons - two 4 s-electron (4 s 2) and six 3 d-electrons (3 d 6).

The valence sublevels can be partially or completely filled with electrons, or they can generally remain free. With an increase in the nuclear charge, the values ​​of the energy of all sublevels decrease, but due to the interaction of electrons with each other, the energy of different sublevels decreases with different "rates". The energy is completely filled d- and f-sublevels decreases so much that they cease to be valence.

As an example, consider the atoms of titanium and arsenic (Fig. 6.18).

In the case of the titanium atom 3 d-The EPU is only partially filled with electrons, and its energy is greater than the energy 4 s-EPU, and 3 d-electrons are valence. Arsenic atom has 3 d-The EPU is completely filled with electrons, and its energy is significantly less than the energy 4 s-EPU, and therefore 3 d-electrons are not valence.
In the examples given, we have analyzed valence electronic configuration atoms of titanium and arsenic.

The valence electronic configuration of an atom is depicted as valence electronic formula, or in the form energy diagram of valence sublevels.

VALENT ELECTRONS, EXTERNAL ELECTRONS, VALENT EPU, VALENT AO, VALENT ELECTRONIC CONFIGURATION OF THE ATOM, VALENCE ELECTRONIC FORMULA, VALENCE SUB-LEVEL DIAGRAM.

1. On the energy diagrams you have drawn up and in the complete electronic formulas of the atoms Na, Mg, Al, Si, P, S, Cl, Ar, indicate the outer and valence electrons. Make up the valence electronic formulas of these atoms. On the energy diagrams, highlight the parts corresponding to the energy diagrams of the valence sublevels.
2. What is common between the electronic configurations of atoms a) Li and Na, B and Al, O and S, Ne and Ar; b) Zn and Mg, Sc and Al, Cr and S, Ti and Si; c) H and He, Li and O, K and Kr, Sc and Ga. What are their differences
3.How many valence sublevels in the electron shell of an atom of each of the elements: a) hydrogen, helium and lithium, b) nitrogen, sodium and sulfur, c) potassium, cobalt and germanium
4. How many valence orbitals are completely filled in the atom of a) boron, b) fluorine, c) sodium?
5.How many orbitals with an unpaired electron in an atom of a) boron, b) fluorine, c) iron
6. How many free outer orbitals does a manganese atom have? And how many free valences?
7. For the next lesson, prepare a strip of paper 20 mm wide, divide it into cells (20 × 20 mm), and apply a natural range of elements (from hydrogen to meitnerium) to this strip.
8.In each cell, place the symbol of the element, its ordinal number and the valence electronic formula, as shown in Fig. 6.19 (use Appendix 4).

6.8. Systematization of atoms according to the structure of their electronic shells

The systematization of chemical elements is based on the natural series of elements and principle of similarity of electronic shells their atoms.
You are already familiar with the natural range of chemical elements. Now let's get acquainted with the principle of similarity of electronic shells.
Considering the valence electronic formulas of atoms in the NRE, it is easy to find that for some atoms they differ only in the values ​​of the principal quantum number. For example 1 s 1 for hydrogen, 2 s 1 for lithium, 3 s 1 for sodium, etc., or 2 s 2 2p 5 for fluorine, 3 s 2 3p 5 for chlorine, 4 s 2 4p 5 for bromine, etc. This means that the outer regions of the clouds of valence electrons of such atoms are very similar in shape and differ only in size (and, of course, in electron density). And if so, then the electron clouds of such atoms and the corresponding valence configurations can be called like... For atoms of different elements with similar electronic configurations, we can write general valence electronic formulas: ns 1 in the first case and ns 2 np 5 in the second. Moving along the natural series of elements, one can find other groups of atoms with similar valence configurations.
Thus, atoms with similar valence electronic configurations are regularly found in the natural series of elements. This is the principle of similarity of electronic shells.
Let's try to identify the kind of this regularity. To do this, we will use the natural row of elements you have made.

ERE begins with hydrogen, the valence electronic formula of which is 1 s 1 . In search of similar valence configurations, we cut the natural series of elements before elements with a common valence electronic formula ns 1 (i.e., before lithium, before sodium, etc.). We got the so-called "periods" of the elements. Let's add the resulting "periods" so that they become the rows of the table (see Fig. 6.20). As a result, only the atoms of the first two columns of the table will have similar electronic configurations.

Let's try to achieve similarity of valence electronic configurations in other columns of the table. To do this, we cut out from the 6th and 7th periods elements with numbers 58 - 71 and 90 - 103 (they are filled with 4 f- and 5 f-sub-levels) and place them below the table. Let's move the symbols of the remaining elements horizontally as shown in the figure. After that, atoms of elements standing in one column of the table will have similar valence configurations, which can be expressed by general valence electronic formulas: ns 1 , ns 2 , ns 2 (n–1)d 1 , ns 2 (n–1)d 2 and so on until ns 2 np 6. All deviations from the general valence formulas are due to the same reasons as in the case of chromium and copper (see paragraph 6.6).

As you can see, using the ERE and applying the principle of the similarity of electronic shells, we were able to systematize the chemical elements. Such a system of chemical elements is called natural, since it is based solely on the laws of Nature. The table we received (Fig. 6.21) is one of the ways to graphically depict the natural system of elements and is called long-period table of chemical elements.

PRINCIPLE OF SIMILARITY OF ELECTRONIC SHELLS, NATURAL SYSTEM OF CHEMICAL ELEMENTS ("PERIODIC" SYSTEM), TABLE OF CHEMICAL ELEMENTS.

6.9. Long-period table of chemical elements

Let's take a closer look at the structure of the long-period table of chemical elements.
The rows in this table, as you already know, are called "periods" of the elements. The periods are numbered with Arabic numerals from 1 to 7. There are only two elements in the first period. The second and third periods, each containing eight elements, are called short periods. The fourth and fifth periods, each containing 18 elements, are called long periods. The sixth and seventh periods, each containing 32 elements, are called extra-long periods.
The columns in this table are named in groups elements. Group numbers are designated by Roman numerals with Latin letters A or B.
Elements of some groups have their own common (group) names: elements of the IA group (Li, Na, K, Rb, Cs, Fr) - alkaline elements(or alkali metal elements); Group IIA elements (Ca, Sr, Ba and Ra) - alkaline earth elements(or alkaline earth metal elements) (the name "alkali metals" and alkaline earth metals "refers to simple substances formed by the corresponding elements and should not be used as names for groups of elements); elements of group VIA (O, S, Se, Te, Po) - chalcogenes, elements of VIIA group (F, Cl, Br, I, At) - halogens, elements of group VIIIA (He, Ne, Ar, Kr, Xe, Rn) - noble gas elements. (The traditional name "noble gases" also refers to simple substances)
Elements with serial numbers 58 - 71 (Ce - Lu) usually taken out to the bottom of the table are called lanthanides("following lanthanum"), and elements with serial numbers 90 - 103 (Th - Lr) - actinides("following anemones"). There is a variant of the long-period table, in which lanthanides and actinides are not cut out from the NRE, but remain in place in super-long periods. This table is sometimes called superlong-period.
Long period table is divided into four block(or section).
s-Block includes elements of IA and IIA-groups with common valence electronic formulas ns 1 and ns 2 (s-elements).
r-Block includes elements from IIIA to VIIIA group with general valence electronic formulas from ns 2 np 1 to ns 2 np 6 (p-elements).
d-block includes elements from IIIB to IIB group with general valence electronic formulas from ns 2 (n–1)d 1 to ns 2 (n–1)d 10 (d-elements).
f-Block includes lanthanides and actinides ( f-elements).

The elements s- and p-blocks form A-groups, and the elements d-block - B-group of the system of chemical elements. Everything f-elements are formally included in the IIIB group.
The elements of the first period - hydrogen and helium - are s-elements and can be placed in groups IA and IIA. But helium is more often placed in the VIIIA group as an element that ends the period, which fully corresponds to its properties (helium, like all other simple substances formed by the elements of this group, is a noble gas). Hydrogen, on the other hand, is often placed in the VIIA group, since in its properties it is much closer to halogens than to alkaline elements.
Each of the periods of the system begins with an element with a valence configuration of atoms ns 1, since it is from these atoms that the formation of the next electron layer begins, and ends with an element with a valence configuration of atoms ns 2 np 6 (except for the first period). This makes it easy to distinguish groups of sublevels on the energy diagram that are filled with electrons from atoms of each of the periods (Fig. 6.22). Do this work with all the sublevels shown in your copy of Figure 6.4. The sublevels highlighted in Figure 6.22 (except for completely filled d- and f-sublevels) are valence for atoms of all elements of a given period.
Appearance in periods s-, p-, d- or f-elements fully correspond to the filling sequence s-, p-, d- or f-sub-level electrons. This feature of the system of elements allows, knowing the period and group, which includes this element, immediately write down its valence electronic formula.

LONG PERIOD TABLE OF CHEMICAL ELEMENTS, BLOCKS, PERIODS, GROUPS, ALKALINE ELEMENTS, ALKALINE EARTH ELEMENTS, CHALCOGENS, HALOGENS, ELEMENTS OF NOBLE GASES, LATHANOIDS.
Write down the general valence electronic formulas of atoms of elements a) IVA and IVB groups, b) IIIA and VIIB groups?
2. What is common between the electronic configurations of atoms of elements A and B groups? How do they differ?
3. How many groups of elements are included in a) s-block, b) R-block, c) d-block?
4. Continue Figure 30 towards increasing the energy of the sublevels and select the groups of sublevels that are filled with electrons in the 4th, 5th and 6th periods.
5. List the valence sublevels of a) calcium, b) phosphorus, c) titanium, d) chlorine, e) sodium. 6.Formulate how s-, p- and d-elements differ from each other.
7. Explain why the belonging of an atom to any element is determined by the number of protons in the nucleus, and not by the mass of this atom.
8. For atoms of lithium, aluminum, strontium, selenium, iron and lead, draw up valence, complete and abbreviated electronic formulas and draw energy diagrams of valence sublevels. 9. Atoms of which elements correspond to the following valence electronic formulas: 3 s 1 , 4s 1 3d 1, 2s 2 2 p 6 , 5s 2 5p 2 , 5s 2 4d 2 ?

6.10. Types of electronic formulas of the atom. Algorithm for their compilation

For various purposes, we need to know either the full or the valence configuration of the atom. Each of these electronic configurations can be represented by both a formula and an energy diagram. That is, complete electronic configuration of an atom expressed the complete electronic formula of the atom, or complete energy diagram of the atom... In turn, valence electron configuration of an atom expressed valence(or, as it is often called, " short ") electronic formula of the atom, or diagram of the valence sublevels of the atom(fig. 6.23).

Previously, we made up the electronic formulas of atoms using the ordinal numbers of the elements. In this case, we determined the sequence of filling the sublevels with electrons according to the energy diagram: 1 s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s etc. And only by writing down the complete electronic formula, we could write down the valence formula.
The valence electronic formula of the atom, which is most often used, is more convenient to write based on the position of the element in the system of chemical elements, according to the coordinates period - group.
Let's take a closer look at how this is done for elements. s-, p- and d-blocks.
For items s-block valence electronic formula of an atom consists of three symbols. In general, it can be written as follows:

In the first place (in place of the large cell), the period number is put (equal to the main quantum number of these s-electrons), and on the third (in the superscript) is the group number (equal to the number of valence electrons). Taking magnesium atom as an example (3rd period, IIA group), we get:

For items p-block valence electronic formula of an atom consists of six symbols:

Here, instead of large cells, the period number is also put (equal to the main quantum number of these s- and p-electrons), and the group number (equal to the number of valence electrons) turns out to be equal to the sum of the superscripts. For the oxygen atom (2nd period, group VIA) we get:

2s 2 2p 4 .

Valence electronic formula of most elements d-block can be written like this:

As in the previous cases, here, instead of the first cell, the period number is put (equal to the main quantum number of these s-electrons). The number in the second cell turns out to be one less, since the main quantum number of these d-electrons. The group number here is also equal to the sum of the indices. Example - the valence electronic formula of titanium (4th period, IVB group): 4 s 2 3d 2 .

The group number is equal to the sum of the indices and for the elements of the VIB group, but, as you remember, they have a valence s- there is only one electron sublevel, and the general valence electronic formula ns 1 (n–1)d 5 . Therefore, the valence electronic formula, for example, molybdenum (5th period) - 5 s 1 4d 5 .
It is just as easy to compose the valence electronic formula of any element of the IB group, for example, gold (6th period)> -> 6 s 1 5d 10, but in this case it must be remembered that d- the electrons of the atoms of the elements of this group still remain valence, and some of them can participate in the formation of chemical bonds.
The general valence electronic formula of atoms of group IIB elements is ns 2 (n – 1)d ten . Therefore, the valence electronic formula, for example, of a zinc atom is 4 s 2 3d 10 .
The valence electronic formulas of the elements of the first triad (Fe, Co and Ni) also obey the general rules. Iron, an element of group VIIIB, has a valence electronic formula of 4 s 2 3d 6. The cobalt atom has one d-electron is larger (4 s 2 3d 7), and for the nickel atom - by two (4 s 2 3d 8).
Using only these rules for writing valence electronic formulas, it is impossible to compose the electronic formulas of atoms of some d-elements (Nb, Ru, Rh, Pd, Ir, Pt), since their filling of valence sublevels with electrons due to the tendency to highly symmetric electron shells has some additional features.
Knowing the valence electronic formula, it is possible to write down the complete electronic formula of the atom (see below).
Often, instead of cumbersome full electronic formulas, one writes abbreviated electronic formulas atoms. To compose them in the electronic formula, all the electrons of the atom except for the valence ones are selected, their symbols are placed in square brackets and the part of the electronic formula corresponding to the electronic formula of the atom of the last element of the previous period (the element that forms the noble gas) is replaced with the symbol of this atom.

Examples of electronic formulas of different types are shown in Table 14.

Table 14. Examples of electronic formulas of atoms

Electronic formulas

Abbreviated

Valence

1s 2 2s 2 2p 3

2s 2 2p 3

2s 2 2p 3

1s 2 2s 2 2p 6 3s 2 3p 5

3s 2 3p 5

3s 2 3p 5

1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 5

4s 2 3d 5

4s 2 3d 5

1s 2 2s 2 2p 6 3s 2 3p 6 3d 10 4s 2 4p 3

4s 2 4p 3

4s 2 4p 3

1s 2 2s 2 2p 6 3s 2 3p 6 3d 10 4s 2 4p 6

4s 2 4p 6

4s 2 4p 6

Algorithm for drawing up the electronic formulas of atoms (for example, the iodine atom)


operations

Operation

Result

Determine the coordinates of the atom in the table of elements.

Period 5, group VIIA

Make a valence electronic formula.

5s 2 5p 5

Complete the symbols of the internal electrons in the sequence of filling the sublevels with them.

1s 2 2s 2 2p 6 3s 2 3p 6 4s 2 3d 10 4p 6 5s 2 4d 10 5p 5

Considering the decrease in energy of fully filled d- and f-Sub-levels, write down the complete electronic formula.

Note the valence electrons.

1s 2 2s 2 2p 6 3s 2 3p 6 3d 10 4s 2 4p 6 4d 10 5s 2 5p 5

Highlight the electronic configuration of the preceding noble gas atom.

Write down an abbreviated electronic formula, combining all in square brackets non-bonded electrons.

5s 2 5p 5

Notes (edit)
1. For elements of the 2nd and 3rd periods, the third operation (without the fourth) immediately leads to a complete electronic formula.
2. (n – 1)d 10 -Electrons remain valence at the atoms of the elements of group IB.

COMPLETE ELECTRONIC FORMULA, VALENCE ELECTRONIC FORMULA, REDUCED ELECTRONIC FORMULA, ALGORITHM FOR COMPOSING ELECTRONIC FORMULAS OF ATOMS.
1. Make the valence electronic formula of the atom of element a) the second period of the third A group, b) the third period of the second A group, c) the fourth period of the fourth A group.
2. Make the abbreviated electronic formulas of the atoms of magnesium, phosphorus, potassium, iron, bromine and argon.

6.11. Short-period table of chemical elements

For more than 100 years that have passed since the discovery of the natural system of elements, several hundred of the most diverse tables have been proposed, graphically reflecting this system. Of these, in addition to the long-period table, the most widespread is the so-called short-period table of elements of D.I. Mendeleev. A short-period table is obtained from a long-period table if the 4th, 5th, 6th and 7th periods are cut before the elements of the IB group, move apart and fold the resulting rows as we used to add the periods. The result is shown in Figure 6.24.

Lanthanides and actinides are also placed under the main table here.

V groups This table contains elements whose atoms have equal number of valence electrons no matter what orbitals these electrons are in. So, the elements chlorine (a typical element that forms a non-metal; 3 s 2 3p 5) and manganese (metal-forming element; 4 s 2 3d 5), not possessing the semblance of electronic shells, fall here in the same seventh group. The need to distinguish between such elements forces you to select in groups subgroups: the main- analogs of the A-groups of the long-period table and collateral- analogs of B-groups. In Figure 34, the symbols of the elements of the main subgroups are shifted to the left, and the elements of the secondary subgroups are shifted to the right.
True, this arrangement of elements in the table also has its advantages, because it is the number of valence electrons that primarily determines the valence capabilities of an atom.
The long-period table reflects the regularities of the electronic structure of atoms, the similarity and regularities of changes in the properties of simple substances and compounds by groups of elements, the regular change in a number of physical quantities characterizing atoms, simple substances and compounds throughout the entire system of elements, and much more. The short-period table is less convenient in this respect.

SHORT PERIOD TABLE, MAIN SUBGROUPS, SIDE SUBGROUPS.
1.Convert the long-period table you have constructed from a natural series of elements into a short-period one. Reverse the transformation.
2. Is it possible to draw up a general valence electronic formula of atoms of elements of one group of a short-period table? Why?

6.12. Sizes of atoms. Orbital radii

.

The atom has no clear boundaries. What is considered the size of an isolated atom? The nucleus of an atom is surrounded by an electron shell, and the shell consists of electron clouds. The size of the EO is characterized by the radius r eo. All clouds in the outer layer have approximately the same radius. Therefore, the size of an atom can be characterized by this radius. It is called orbital radius of the atom(r 0).

The values ​​of the orbital radii of atoms are given in Appendix 5.
The radius of the EO depends on the charge of the nucleus and on which orbital the electron that forms this cloud is located in. Consequently, the orbital radius of an atom depends on the same characteristics.
Consider the electron shells of hydrogen and helium atoms. Both in the hydrogen atom and in the helium atom, the electrons are at 1 s-AO, and their clouds would have the same size if the charges of the nuclei of these atoms were the same. But the charge of the nucleus of a helium atom is twice as large as the charge of the nucleus of a hydrogen atom. According to Coulomb's law, the force of attraction acting on each of the electrons of a helium atom is twice the force of attraction of an electron to the nucleus of a hydrogen atom. Consequently, the radius of the helium atom must be much smaller than the radius of the hydrogen atom. This is true: r 0 (He) / r 0 (H) = 0.291 E / 0.529 E 0.55.
The lithium atom has an outer electron at 2 s-AO, that is, it forms a cloud of the second layer. Naturally, its radius should be larger. Really: r 0 (Li) = 1.586 E.
The atoms of the remaining elements of the second period have external electrons (and 2 s, and 2 p) are located in the same second electron layer, and the nuclear charge of these atoms increases with increasing serial number. Electrons are more strongly attracted to the nucleus, and, naturally, the radii of the atoms decrease. We could repeat this reasoning for atoms of elements of other periods, but with one clarification: the orbital radius decreases monotonically only when each of the sublevels is filled.
But if we ignore the particulars, then the general nature of the change in the size of atoms in the system of elements is as follows: with an increase in the ordinal number in the period, the orbital radii of the atoms decrease, and in the group, they increase. The largest atom is a cesium atom, and the smallest is a helium atom, but of the atoms of elements that form chemical compounds (helium and neon do not form them), the smallest is a fluorine atom.
Most of the atoms of the elements that are in the natural row after the lanthanides have orbital radii somewhat smaller than one would expect based on general laws. This is due to the fact that 14 lanthanides are located between lanthanum and hafnium in the system of elements, and, therefore, the charge of the nucleus of the hafnium atom is 14 e more than lanthanum. Therefore, the outer electrons of these atoms are attracted to the nucleus more strongly than they would in the absence of lanthanides (this effect is often called "lanthanide compression").
Please note that when going from the atoms of the elements of the VIIIA group to the atoms of the elements of the IA group, the orbital radius increases abruptly. Consequently, our choice of the first elements of each period (see § 7) turned out to be correct.

ORBITAL RADIUS OF THE ATOM, ITS CHANGE IN THE SYSTEM OF ELEMENTS.
1.According to the data given in Appendix 5, plot on graph paper a graph of the dependence of the orbital radius of an atom on the ordinal number of an element for elements with Z from 1 to 40. The length of the horizontal axis is 200 mm, the length of the vertical axis is 100 mm.
2. How can you characterize the appearance of the resulting broken line?

6.13. Ionization energy of an atom

If you impart additional energy to an electron in an atom (how this can be done, you will learn from a physics course), then the electron can go to another AO, that is, the atom will be in excited state... This state is unstable, and the electron will almost immediately return to its original state, and the excess energy will be released. But if the energy imparted to the electron is large enough, the electron can completely detach from the atom, while the atom ionizes, that is, it turns into a positively charged ion ( cation). The energy required for this is called the ionization energy of the atom(E and).

It is rather difficult to tear an electron from a single atom and measure the energy required for this, therefore, it is practically determined and used molar ionization energy(E and m).

The molar ionization energy shows what is the smallest energy that is required to detach 1 mole of electrons from 1 mole of atoms (one electron from each atom). This value is usually measured in kilojoules per mole. The values ​​of the molar ionization energy of the first electron for most elements are given in Appendix 6.
How does the ionization energy of an atom depend on the position of an element in a system of elements, that is, how does it change in a group and a period?
According to the physical meaning, the ionization energy is equal to the work that must be spent on overcoming the force of attraction of the electron to the atom when the electron moves from the atom to an infinite distance from it.

where q- electron charge, Q Is the charge of the cation remaining after the removal of the electron, and r o is the orbital radius of the atom.

AND q, and Q- the quantities are constant, and we can conclude that the work on the separation of an electron A, and with it the ionization energy E and, are inversely proportional to the orbital radius of the atom.
Having analyzed the values ​​of the orbital radii of atoms of various elements and the corresponding values ​​of the ionization energy given in Appendices 5 and 6, you can make sure that the relationship between these values ​​is close to proportional, but somewhat different from it. The reason that our conclusion does not agree very well with the experimental data is that we used a very crude model that does not take into account many significant factors. But even this rough model allowed us to draw the correct conclusion that with an increase in the orbital radius, the ionization energy of an atom decreases and, conversely, with a decrease in the radius, it increases.
Since the orbital radius of the atoms decreases in the period with an increase in the ordinal number, the ionization energy increases. In a group, with an increase in the ordinal number, the orbital radius of the atoms, as a rule, increases, and the ionization energy decreases. The largest molar ionization energy is found in the smallest atoms, helium atoms (2372 kJ / mol), and among the atoms capable of forming chemical bonds, in fluorine atoms (1681 kJ / mol). The smallest is for the largest atoms, cesium atoms (376 kJ / mol). In a system of elements, the direction of increasing the ionization energy can be schematically shown as follows:

In chemistry, it is important that the ionization energy characterizes the tendency of an atom to give up "its" electrons: the greater the ionization energy, the less the atom is inclined to give up electrons, and vice versa.

EXCITED STATE, IONIZATION, CATION, IONIZATION ENERGY, IONIZATION MOLAR ENERGY, IONIZATION ENERGY CHANGE IN THE ELEMENT SYSTEM.
1.Using the data given in Appendix 6, determine how much energy needs to be spent in order to take one electron away from all sodium atoms with a total mass of 1 g.
2. Using the data given in Appendix 6, determine how many times more energy needs to be spent to detach one electron from all sodium atoms with a mass of 3 g than from all potassium atoms of the same mass. Why is this ratio different from the ratio of the molar ionization energies of the same atoms?
3.According to the data given in Appendix 6, build a graph of the dependence of the molar ionization energy on the serial number for elements with Z from 1 to 40. The dimensions of the graph are the same as in the task to the previous paragraph. See if this schedule matches the selection of "periods" of the system of elements.

6.14. Electron affinity energy

.

The second most important energy characteristic of an atom is electron affinity energy(E with).

In practice, as in the case of the ionization energy, the corresponding molar quantity is usually used - molar electron affinity energy().

The molar energy of affinity for an electron shows what is the energy released when one mole of electrons is attached to one mole of neutral atoms (one electron to each atom). Like the molar ionization energy, this value is also measured in kilojoules per mole.
At first glance, it may seem that energy should not be released in this case, because an atom is a neutral particle, and there are no electrostatic forces of attraction between a neutral atom and a negatively charged electron. On the contrary, approaching an atom, an electron, it would seem, should repel from the same negatively charged electrons that form an electron shell. Actually this is not true. Remember if you have ever had to deal with atomic chlorine. Of course not. After all, it only exists at very high temperatures. Even the more stable molecular chlorine is practically not found in nature - if necessary, it has to be obtained using chemical reactions. And with sodium chloride (table salt) you have to deal with it all the time. After all, table salt is consumed every day by a person with food. And in nature, it occurs quite often. But the composition of table salt includes chloride ions, that is, chlorine atoms, which have attached one "extra" electron. One of the reasons for this prevalence of chloride ions is that chlorine atoms have a tendency to attach electrons, that is, when chloride ions are formed from chlorine atoms and electrons, energy is released.
One of the reasons for the release of energy is already known to you - it is associated with an increase in the symmetry of the electron shell of the chlorine atom during the transition to a singly charged anion... At the same time, as you remember, energy 3 p-sublevel decreases. There are other more complex reasons as well.
Due to the fact that the value of the electron affinity energy is influenced by several factors, the nature of the change in this value in the system of elements is much more complex than the nature of the change in the ionization energy. You can be convinced of this by analyzing the table given in Appendix 7. But since the value of this quantity is determined, first of all, by the same electrostatic interaction as the values ​​of the ionization energy, then its change in the system of elements (at least in A- groups), in general terms, is similar to a change in the ionization energy, that is, the energy of affinity for an electron in a group decreases, and in a period it increases. It is maximal for fluorine (328 kJ / mol) and chlorine (349 kJ / mol) atoms. The nature of the change in the energy of affinity for an electron in a system of elements resembles the nature of the change in the ionization energy, that is, the direction of an increase in the energy of affinity for an electron can be schematically shown as follows:

2. On the same scale along the horizontal axis as in the previous tasks, plot the dependence of the molar energy of affinity for an electron on the ordinal number for atoms of elements with Z 1 to 40 using app 7.
3.What is the physical meaning of negative values ​​of the electron affinity energy?
4. Why, of all atoms of the elements of the 2nd period, only beryllium, nitrogen and neon have negative values ​​of the molar energy of affinity for an electron?

6.15. The tendency of atoms to give and attach electrons

You already know that the propensity of an atom to give up its own and attach foreign electrons depends on its energy characteristics (ionization energy and electron affinity energy). Which atoms are more inclined to donate their electrons, and which ones are more inclined to accept others?
To answer this question, let us summarize in Table 15 everything that we know about the change in these tendencies in the system of elements.

Table 15. Change in the propensity of atoms to give up their own and attach foreign electrons

Now let's consider how many electrons an atom can donate.
First, in chemical reactions an atom can donate only valence electrons, since donating the rest is energetically extremely disadvantageous. Secondly, the atom "easily" gives (if inclined) only the first electron, the second electron it gives much more difficult (2-3 times), and the third - even more difficult (4-5 times). Thus, an atom can donate one, two and, much less often, three electrons.
How many electrons can an atom accept?
First, in chemical reactions, an atom can accept electrons only to the valence sublevels. Secondly, the release of energy occurs only when the first electron is attached (and that is far from always). The attachment of the second electron is always energetically disadvantageous, and the third - even more so. Nevertheless, an atom can attach one, two and (extremely rarely) three electrons, as a rule, as much as it lacks to fill its valence sublevels.
Energy costs for the ionization of atoms and for the attachment of a second or third electron to them are compensated by the energy released during the formation of chemical bonds. 4. How does the electron shell of potassium, calcium and scandium atoms change when they donate their electrons? Give the equations of recoil by atoms of electrons and the abbreviated electronic formulas of atoms and ions.
5. How does the electron shell of chlorine, sulfur and phosphorus atoms change when they attach foreign electrons? Give the electron attachment equations and the abbreviated electronic formulas of atoms and ions.
6. Using Appendix 7, determine what energy will be released when electrons attach to all sodium atoms with a total mass of 1 g.
7. Using Appendix 7, determine what energy needs to be spent to detach "extra" electrons from 0.1 mole of Br– ions?

Oxygen (O) is a vital gas needed for breathing, maintaining combustion, oxidation. Belongs to the group of chalcogenes. The most abundant element on Earth. The structure of the oxygen atom allows it to combine with metals and non-metals to form oxides.

Structure

By the position in the periodic table of Mendeleev, you can determine the structure of the atom of the element oxygen. This is the eighth element located in the VI group, the second period. The relative atomic mass is 16. There are three isotopes of the element:

  • 16 O;
  • 17 O;
  • 18 O.

The most common 16 O.

Rice. 1. Position of oxygen in the periodic table.

The electronic configuration of the oxygen atom is 1s 2 2s 2 2p 4. The oxygen nucleus has a charge of +8. Oxygen belongs to the elements of the p-family. There are six valence electrons on the outer energy level. Two paired electrons are in the 2s orbital. At the 2p level, there are two paired and two unpaired electrons, therefore, in all compounds, oxygen exhibits a second valence.

Rice. 2. The structure of the atom.

The oxygen molecule has two atoms - O 2. When one more atom is attached, ozone is formed - O 3.

Physical properties

Oxygen is a colorless and tasteless gas, poorly soluble in water and alcohol. Let's well dissolve in liquid silver. In liquefied form it becomes light blue, in solid - blue. It occupies 21% of the atmospheric air.

Rice. 3. Solid oxygen.

Oxygen supports combustion, so it can be easily detected with a smoldering torch (flashes).

Chemical properties

Due to its electronic structure, it has a high oxidation state. However, it is very active when heated due to strong double bonds between atoms. At room temperature, it quickly reacts with the most active elements - alkali and alkaline earth metals, some non-metals.

Combining with elements, forms oxides. Oxidizes organic matter. Examples of reactions with simple substances:

  • K + O 2 → KO 2;
  • 3Fe + 2O 2 → Fe 3 O 4;
  • S + O 2 → SO 2.

Oxygen reacts with phosphorus, sulfur, carbon (graphite), hydrogen when heated:

  • 4P + 5O 2 → 2P 2 O 5;
  • S + O 2 → SO 2;
  • C + O 2 → CO 2;
  • 2H 2 + O 2 → 2H 2 O.

By quickly passing fluorine through an alkali, the reaction of oxygen with fluorine is obtained:

2F 2 + 2NaOH → 2NaF + H 2 O + OF 2.

Oxygen with fluorine directly interacts with an electrical discharge. In this case, oxygen plays the role of a reducing agent:

O 2 + F 2 → F 2 O 2.

Oxygen reacts with complex substances to form oxides:

  • 2CuS + 3O 2 → 2CuO + 2SO 2;
  • 2H 2 S + 3O 2 → 2SO 2 + 2H 2 O;
  • 2C 6 H 6 + 15O 2 → 12CO 2 + 6H 2 O;
  • CH 4 + 2O 2 → CO 2 + 2H 2 O.

Oxygen does not react with gold and inert gases. Interaction with halogens occurs under ultraviolet or electric current conditions.

What have we learned?

Oxygen is a colorless gas common in nature. Atomic structure diagram - +8 O) 2) 6. Oxygen always exhibits valence II due to two unpaired electrons. Oxygen is a strong oxidizing agent that exhibits the properties of a reducing agent in some reactions. Interacts with metals and non-metals, complex inorganic and organic substances. It is most active when heated. Does not react with noble gases and gold.

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The Swiss physicist W. Pauli in 1925 established that in an atom in one orbital there can be no more than two electrons having opposite (antiparallel) spins (translated from English as "spindle"), that is, possessing such properties that can be conventionally represented itself as the rotation of an electron around its imaginary axis: clockwise or counterclockwise. This principle is called the Pauli principle.

If there is one electron in the orbital, then it is called unpaired, if two, then these are paired electrons, that is, electrons with opposite spins.

Figure 5 shows a diagram of the division of energy levels into sublevels.

The S-Orbital, as you already know, is spherical. The electron of the hydrogen atom (s = 1) is located in this orbital and is unpaired. Therefore, its electronic formula or electronic configuration will be written as follows: 1s 1. In electronic formulas, the number of the energy level is indicated by the number in front of the letter (1 ...), the Latin letter denotes the sublevel (type of orbital), and the number written to the upper right of the letter (as an exponent) shows the number of electrons on the sublevel.

For a helium atom He, which has two paired electrons in one s-orbital, this formula is: 1s 2.

The electron shell of the helium atom is complete and very stable. Helium is a noble gas.

At the second energy level (n = 2), there are four orbitals: one s and three p. The electrons of the s-orbitals of the second level (2s-orbitals) have a higher energy, since they are at a greater distance from the nucleus than the electrons of the 1s-orbital (n = 2).

In general, for each value of n, there is one s-orbital, but with a corresponding store of electron energy on it and, therefore, with a corresponding diameter that grows as the value of n increases.

The R-Orbital has the shape of a dumbbell or volumetric figure eight. All three p-orbitals are located in the atom mutually perpendicular along the spatial coordinates drawn through the nucleus of the atom. It should be emphasized once again that each energy level (electron layer), starting from n = 2, has three p-orbitals. With an increase in the value of n, electrons animate p-orbitals located at large distances from the nucleus and directed along the x, y, r axes.

For elements of the second period (n = 2), first one p-orbital is filled, and then three p-orbitals. Electronic formula 1L: 1s 2 2s 1. The electron is weaker bound to the nucleus of the atom, so the lithium atom can easily give it away (as you obviously remember, this process is called oxidation), turning into a Li + ion.

In the beryllium atom Be 0, the fourth electron is also located in the 2s orbital: 1s 2 2s 2. The two outer electrons of the beryllium atom are easily torn off - Be 0 is oxidized to the Be 2+ cation.

The fifth electron of the boron atom is occupied by a 2p orbital: 1s 2 2s 2 2p 1. Further, at the C, N, O, E atoms, the filling of 2p-orbitals takes place, which ends in the noble gas of neon: 1s 2 2s 2 2p 6.

For the elements of the third period, the Sv and 3p orbitals are filled, respectively. In this case, five d-orbitals of the third level remain free:

Sometimes in diagrams depicting the distribution of electrons in atoms, only the number of electrons at each energy level is indicated, that is, they write down the abbreviated electronic formulas of the atoms of chemical elements, in contrast to the above full electronic formulas.

For elements of large periods (fourth and fifth), the first two electrons occupy the 4th and 5th orbitals, respectively: 19 K 2, 8, 8, 1; 38 Sr 2, 8, 18, 8, 2. Starting from the third element of each large period, the next ten electrons will enter the previous 3d and 4d orbitals, respectively (for elements of side subgroups): 23 V 2, 8, 11, 2; 26 Tr 2, 8, 14, 2; 40 Zr 2, 8, 18, 10, 2; 43 Tg 2, 8, 18, 13, 2. As a rule, when the previous d-sublevel is filled, the outer (4p- and 5p-respectively) p-sublevel will begin to fill.

For elements of large periods - the sixth and unfinished seventh - the electronic levels and sublevels are filled with electrons, as a rule, as follows: the first two electrons will go to the outer B-sublevel: 56 Ва 2, 8, 18, 18, 8, 2; 87Gg 2, 8, 18, 32, 18, 8, 1; the next one electron (for Na and Ac) to the previous (p-sublevel: 57 La 2, 8, 18, 18, 9, 2 and 89 Ac 2, 8, 18, 32, 18, 9, 2.

Then the next 14 electrons will enter the third outside energy level on the 4f and 5f orbitals, respectively, for lanthanides and actinides.

Then the second outside energy level (d-sublevel) will begin to build up again: for elements of secondary subgroups: 73 Ta 2, 8,18, 32,11, 2; 104 Rf 2, 8, 18, 32, 32, 10, 2, - and, finally, only after full filling with ten electrons, this level-equal will again be filled with the outer p-sublevel:

86 Rn 2, 8, 18, 32, 18, 8.

Very often, the structure of the electron shells of atoms is depicted using energy or quantum cells - so-called graphic electronic formulas are written. For this notation, the following notation is used: each quantum cell is designated by a cell that corresponds to one orbital; each electron is indicated by an arrow corresponding to the direction of the spin. When writing a graphic electronic formula, two rules should be remembered: Pauli's principle, according to which there can be no more than two electrons in a cell (orbital), but with antiparallel spins, and F. Hund's rule, according to which electrons occupy free cells (orbitals), are located in they first one at a time and have the same spin value, and only then pair, but the spins, according to the Pauli principle, will already be oppositely directed.

In conclusion, we will once again consider the display of the electronic configurations of atoms of elements by the periods of the D. I. Mendeleev system. Diagrams of the electronic structure of atoms show the distribution of electrons over the electron layers (energy levels).

In a helium atom, the first electron layer is complete - there are 2 electrons in it.

Hydrogen and helium are s-elements, the s-orbital of these atoms is filled with electrons.

Elements of the second period

For all elements of the second period, the first electron layer is filled and electrons fill the e- and p-orbitals of the second electron layer in accordance with the principle of least energy (first s- and then p) and the Pauli and Hund rules (Table 2).

In the neon atom, the second electron layer is complete - it contains 8 electrons.

Table 2 The structure of the electron shells of atoms of the elements of the second period

The end of the table. 2

Li, Be - B-elements.

B, C, N, O, F, Ne - p-elements, these atoms are filled with electrons of the p-orbital.

Elements of the third period

For atoms of elements of the third period, the first and second electron layers are completed, therefore, the third electronic layer is filled, in which electrons can occupy the Зs-, 3p- and Зd-sublevels (Table 3).

Table 3 The structure of the electron shells of atoms of the elements of the third period

The 3s-electron orbital is being completed at the magnesium atom. Na and Mg are s-elements.

There are 8 electrons in the argon atom on the outer layer (third electron layer). As the outer layer, it is complete, but in total in the third electron layer, as you already know, there may be 18 electrons, which means that the elements of the third period have Zd-orbitals unfilled.

All elements from Al to Ar are p-elements. s- and p-elements form the main subgroups in the Periodic Table.

For potassium and calcium atoms, a fourth electronic layer appears, the 4s-sublevel is filled (Table 4), since it has a lower energy than the 3d-sublevel. To simplify the graphical electronic formulas of the atoms of the elements of the fourth period: 1) we denote the conditionally graphical electronic formula of argon as follows:
Ar;

2) we will not depict the sublevels that are not filled in these atoms.

Table 4 The structure of the electron shells of atoms of the elements of the fourth period

K, Ca - s-elements included in the main subgroups. In atoms from Sc to Zn, the 3d sublevel is filled with electrons. These are 3-elements. They belong to side subgroups, their pre-external electronic layer is filled, and they are referred to as transition elements.

Pay attention to the structure of the electron shells of chromium and copper atoms. In them there is a "dip" of one electron from the 4th to the 3rd sublevel, which is explained by the higher energy stability of the resulting electronic configurations Зd 5 and Зd 10:

In the zinc atom, the third electronic layer is complete - all the sublevels 3s, Zp, and Zd are filled in it, with a total of 18 electrons on them.

In the elements following zinc, the fourth electronic layer, the 4p-sublevel, continues to be filled: Elements from Ga to Kr are p-elements.

At the krypton atom, the outer layer (fourth) is complete, it has 8 electrons. But in total in the fourth electron layer, as you know, there can be 32 electrons; for the krypton atom, the 4d and 4f sublevels are still empty.

For the elements of the fifth period, the sublevels are filled in the following order: 5s-> 4d -> 5p. And there are also exceptions associated with the "dip" of electrons, in 41 Nb, 42 MO, etc.

In the sixth and seventh periods, elements appear, that is, elements in which the 4f and 5f sublevels of the third outside electron layer are filled, respectively.

The 4f-elements are called lanthanides.

5f-Elements are called actinides.

The order of filling the electronic sublevels in the atoms of the elements of the sixth period: 55 Сs and 56 Ва - 6s-elements;

57 Lа ... 6s 2 5d 1 - 5d-element; 58 Ce - 71 Lu - 4f-elements; 72 Hf - 80 Hg - 5d elements; 81 Тl— 86 Rn - 6p-elements. But even here there are elements in which the order of filling of electron orbitals is "violated", which, for example, is associated with a higher energy stability of half and completely filled f sublevels, that is, nf 7 and nf 14.

Depending on which sublevel of the atom is filled with electrons last, all elements, as you already understood, are divided into four electronic families or blocks (Fig. 7).

1) s-Elements; filled with electrons in the sublevel of the outer level of the atom; s-elements include hydrogen, helium and elements of the main subgroups of groups I and II;

2) p-elements; the p-sublevel of the outer level of the atom is filled with electrons; p elements include elements of the main subgroups of III-VIII groups;

3) d-elements; the d-sublevel of the pre-outer level of the atom is filled with electrons; d-elements include elements of secondary subgroups of groups I-VIII, that is, elements of inserted decades of large periods located between s- and p-elements. They are also called transition elements;

4) f-elements, filled with electrons f-sublevel of the third outside the level of the atom; these include lanthanides and actinides.

1. What would happen if Pauli's principle was not observed?

2. What would happen if Hund's rule was not followed?

3. Make diagrams of the electronic structure, electronic formulas and graphic electronic formulas of the atoms of the following chemical elements: Ca, Fe, Zr, Sn, Nb, Hf, Pa.

4. Write the electronic formula for element 110 using the symbol for the corresponding noble gas.

5. What is the "dip" of an electron? Give examples of elements in which this phenomenon is observed, write down their electronic formulas.

6. How is the belonging of a chemical element to a particular electronic family determined?

7. Compare the electronic and graphical electronic formulas of the sulfur atom. What additional information does the last formula contain?

The filling of orbitals in an unexcited atom is carried out in such a way that the energy of the atom is minimal (the principle of minimum energy). First, the orbitals of the first energy level are filled, then the second, and first the orbital of the s-sublevel is filled and only then the orbitals of the p-sublevel. In 1925, the Swiss physicist W. Pauli established the fundamental quantum-mechanical principle of natural science (Pauli's principle, also called the principle of exclusion or the principle of exclusion). According to the Pauli principle:

an atom cannot have two electrons having the same set of all four quantum numbers.

The electronic configuration of an atom is conveyed by a formula in which the filled orbitals are indicated by a combination of a number equal to the principal quantum number and a letter corresponding to the orbital quantum number. The superscript indicates the number of electrons in the given orbitals.

Hydrogen and helium

The electronic configuration of the hydrogen atom is 1s 1, and helium is 1s 2. The hydrogen atom has one unpaired electron, and the helium atom has two paired electrons. Paired electrons have the same values ​​for all quantum numbers, except for the spin one. The hydrogen atom can donate its electron and turn into a positively charged ion - the H + cation (proton), which does not have electrons (electronic configuration 1s 0). A hydrogen atom can attach one electron and turn into a negatively charged ion H - (hydride ion) with an electronic configuration 1s 2.

Lithium

Three electrons in a lithium atom are distributed as follows: 1s 2 1s 1. Electrons of only the external energy level, called valence electrons, participate in the formation of a chemical bond. The valence of a lithium atom is an electron of the 2s-sublevel, and two electrons of the 1s-sublevel are internal electrons. The lithium atom quite easily loses its valence electron, passing into the Li + ion, which has the configuration 1s 2 2s 0. Note that the hydride ion, helium atom, and lithium cation have the same number of electrons. Such particles are called isoelectronic. They have a similar electronic configuration, but different nuclear charges. The helium atom is chemically very inert, which is associated with the special stability of the 1s 2 electronic configuration. Orbitals not filled with electrons are called vacant. In the lithium atom, three orbitals of the 2p sublevel are vacant.

Beryllium

The electronic configuration of the beryllium atom is 1s 2 2s 2. When an atom is excited, electrons from a lower energy sublevel move to vacant orbitals of a higher energy sublevel. The process of excitation of a beryllium atom can be described as follows:

1s 2 2s 2 (ground state) + → 1s 2 2s 1 2p 1 (excited state).

Comparison of the ground and excited states of the beryllium atom shows that they differ in the number of unpaired electrons. In the ground state of the beryllium atom, there are no unpaired electrons, in the excited state there are two. Despite the fact that, when an atom is excited, in principle, any electrons from lower energy orbitals can transfer to higher orbitals, only transitions between energy sublevels with close energies are essential for the consideration of chemical processes.

This is explained as follows. When a chemical bond is formed, energy is always released, that is, the combination of two atoms passes into an energetically more favorable state. The excitation process requires energy consumption. When electrons are steamed out within the same energy level, the excitation costs are compensated by the formation of a chemical bond. When electrons are stripped off within different levels, the excitation costs are so great that they cannot be compensated for by the formation of a chemical bond. In the absence of a partner in a possible chemical reaction, the excited atom releases a quantum of energy and returns to the ground state - this process is called relaxation.

Boron

The electronic configurations of the atoms of the elements of the 3rd period of the Periodic Table of the Elements will, to a certain extent, be similar to those given above (the atomic number is indicated by the subscript):

11 Na 3s 1
12 Mg 3s 2
13 Al 3s 2 3p 1
14 Si 2s 2 2p2
15 P 2s 2 3p 3

However, the analogy is not complete, since the third energy level splits into three sublevels and all of the listed elements have vacant d-orbitals, to which electrons can transfer upon excitation, increasing the multiplicity. This is especially important for elements such as phosphorus, sulfur and chlorine.

The maximum number of unpaired electrons in a phosphorus atom can reach five:

This explains the possibility of the existence of compounds in which the valence of phosphorus is 5. A nitrogen atom, which has the same configuration of valence electrons in the ground state as the phosphorus atom, cannot form five covalent bonds.

A similar situation arises when comparing the valence capabilities of oxygen and sulfur, fluorine and chlorine. The evaporation of electrons in a sulfur atom leads to the appearance of six unpaired electrons:

3s 2 3p 4 (ground state) → 3s 1 3p 3 3d 2 (excited state).

This corresponds to a six valence state, which is unattainable for oxygen. The maximum valence of nitrogen (4) and oxygen (3) requires a more detailed explanation, which will be given later.

The maximum valence of chlorine is 7, which corresponds to the configuration of the excited state of the atom 3s 1 3p 3 d 3.

The presence of vacant 3d-orbitals in all elements of the third period is explained by the fact that, starting from the third energy level, there is a partial overlap of sublevels of different levels when filled with electrons. So, the 3d-sublevel begins to fill only after the 4s-sublevel is filled. The energy reserve of electrons in atomic orbitals of different sublevels and, therefore, the order of their filling, increases in the following order:

Orbitals are filled earlier, for which the sum of the first two quantum numbers (n + l) is less; when these sums are equal, orbitals with a smaller principal quantum number are first filled.

This pattern was formulated by V.M.Klechkovsky in 1951.

Elements in whose atoms the s-sublevel is filled with electrons are called s-elements. These include the first two elements of each period: hydrogen. However, already in the next d-element - chromium - there is a certain "deviation" in the arrangement of electrons by energy levels in the ground state: instead of the expected four unpaired electrons on the 3d-sublevel, the chromium atom has five unpaired electrons on the 3d sublevel and one unpaired electron on the s-sublevel: 24 Cr 4s 1 3d 5.

The phenomenon of the transition of one s-electron to the d-sublevel is often called the "slip" of the electron. This can be explained by the fact that the orbitals of the d-sublevel filled with electrons become closer to the nucleus due to increased electrostatic attraction between the electrons and the nucleus. As a result, the 4s 1 3d 5 state becomes energetically more favorable than the 4s 2 3d 4 state. Thus, the half-filled d-sublevel (d 5) is more stable than other possible variants of the electron distribution. The electronic configuration corresponding to the existence of the maximum possible number of unpaired electrons, attainable for the preceding d-elements only as a result of excitation, is characteristic of the ground state of the chromium atom. The electronic configuration d 5 is also characteristic of the manganese atom: 4s 2 3d 5. For the following d-elements, each energy cell of the d-sublevel is filled with a second electron: 26 Fe 4s 2 3d 6; 27 Co 4s 2 3d 7; 28 Ni 4s 2 3d 8.

For a copper atom, the state of a completely filled d-sublevel (d 10) becomes attainable due to the transition of one electron from the 4s-sublevel to the 3d-sublevel: 29 Cu 4s 1 3d 10. The last element of the first row of d-elements has an electronic configuration of 30 Zn 4s 23 d 10.

The general tendency, manifested in the stability of the d 5 and d 10 configuration, is also observed for the elements of the lower lying periods. Molybdenum has an electronic configuration similar to chromium: 42 Mo 5s 1 4d 5, and silver - copper: 47 Ag5s 0 d 10. Moreover, the d 10 configuration is already achieved in palladium due to the transition of both electrons from the 5s orbital to the 4d orbital: 46Pd 5s 0 d 10. There are other deviations from the monotonic filling of the d- as well as f-orbitals.


The electronic configuration of an element is a record of the distribution of electrons in its atoms over shells, subshells, and orbitals. The electronic configuration is usually written for atoms in their ground state. The electronic configuration of an atom in which one or more electrons are in an excited state is called an excited configuration. There are three rules for determining the specific electronic configuration of an item in the ground state: Rule 1: filling principle. According to the filling principle, electrons in the ground state of an atom fill the orbitals in a sequence of increasing orbital energy levels. The lowest energy orbitals are always filled first.

Hydrogen; atomic number = 1; number of electrons = 1

This single electron in the hydrogen atom must occupy the s-orbital of the K-shell, since it has the lowest energy of all possible orbitals (see Fig. 1.21). An electron in this s-orbital is called an ls-electron. Hydrogen in the ground state has an electronic configuration Is1.

Rule 2: Pauli exclusion principle... According to this principle, no more than two electrons can be in any orbital, and then only if they have opposite spins (unequal spin numbers).

Lithium; atomic number = 3; number of electrons = 3

The lowest energy orbital is the 1s orbital. It can only take on two electrons. These electrons must have unequal spins. If we denote spin +1/2 with an arrow pointing up, and spin -1/2 with an arrow pointing down, then two electrons with opposite (antiparallel) spins on the same orbital can be schematically represented by writing (Fig. 1.27)

Two electrons with the same (parallel) spins cannot be in the same orbital:

The third electron in a lithium atom should occupy the orbital next in energy to the lowest orbital, i.e. 2c-orbital. Thus, lithium has the Is22s1 electronic configuration.

Rule 3: Gund's rule... According to this rule, the filling of the orbitals of one subshell begins with single electrons with parallel (identical in sign) spins, and only after single electrons occupy all orbitals can the final filling of the orbitals by pairs of electrons with opposite spins take place.

Nitrogen; atomic number = 7; number of electrons = 7 Nitrogen has the electronic configuration ls22s22p3. Three electrons located on the 2p subshell must be located one by one on each of the three 2p orbitals. In this case, all three electrons must have parallel spins (Fig. 1.22).

Table 1.6 shows the electronic configurations of elements with atomic numbers from 1 to 20.

Table 1.6. Electronic configurations of the ground state for elements with atomic numbers from 1 to 20

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