Oxygen – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Oxygen

First Ionization Energy of Oxygen is 13.6181 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Oxygen atom, for example, requires the following ionization energy to remove the outermost electron.

O + IE → O+ + e−        IE = 13.6181 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Nitrogen – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Nitrogen

First Ionization Energy of Nitrogen is 14.5341 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Nitrogen atom, for example, requires the following ionization energy to remove the outermost electron.

N + IE → N+ + e−        IE = 14.5341 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Carbon – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Carbon

First Ionization Energy of Carbon is 11.2603 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Carbon atom, for example, requires the following ionization energy to remove the outermost electron.

C + IE → C+ + e−        IE = 11.2603 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Boron – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Boron

First Ionization Energy of Boron is 8.298 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Boron atom, for example, requires the following ionization energy to remove the outermost electron.

B + IE → B+ + e−        IE = 8.298 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Beryllium – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Beryllium

First Ionization Energy of Beryllium is 9.3226 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Beryllium atom, for example, requires the following ionization energy to remove the outermost electron.

Be + IE → Be+ + e−        IE = 9.3226 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Lithium – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Lithium

First Ionization Energy of Lithium is 5.3917 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Lithium atom, for example, requires the following ionization energy to remove the outermost electron.

Li + IE → Li+ + e−        IE = 5.3917 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Helium – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Helium

First Ionization Energy of Helium is 24.5874 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Helium atom, for example, requires the following ionization energy to remove the outermost electron.

He + IE → He+ + e−        IE = 24.5874 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Hydrogen – Ionization Energy

Periodic Table of Elements - ionization energy
1
H

Hydrogen

13.5984 eV

2
He

Helium

24.5874 eV

3
Li

Lithium

5.3917 eV

4
Be

Beryllium

9.3226 eV

5
B

Boron

8.298 eV

6
C

Carbon

11.2603 eV

7
N

Nitrogen

14.5341 eV

8
O

Oxygen

13.6181 eV

9
F

Fluorine

17.4228 eV

10
Ne

Neon

21.5645 eV

11
Na

Sodium

5.1391 eV

12
Mg

Magnesium

7.6462 eV

13
Al

Aluminium

5.9858 eV

14
Si

Silicon

8.1517 eV

15
P

Phosphorus

10.4867 eV

16
S

Sulfur

10.36 eV

17
Cl

Chlorine

12.9676 eV

18
Ar

Argon

15.7596 eV

19
K

Potassium

4.3407 eV

20
Ca

Calcium

6.1132 eV

21
Sc

Scandium

6.5614 eV

22
Ti

Titanium

6.8282 eV

23
V

Vanadium

6.7463 eV

24
Cr

Chromium

6.7666 eV

25
Mn

Manganese

7.434 eV

26
Fe

Iron

7.9024 eV

27
Co

Cobalt

7.881 eV

28
Ni

Nickel

7.6398 eV

29
Cu

Copper

7.7264 eV

30
Zn

Zinc

9.3941 eV

31
Ga

Gallium

5.9993 eV

32
Ge

Germanium

7.9 eV

33
As

Arsenic

9.8152 eV

34
Se

Selenium

9.7524 eV

35
Br

Bromine

11.8138 eV

36
Kr

Krypton

13.9996 eV

37
Rb

Rubidium

4.1771 eV

38
Sr

Strontium

5.6948 eV

39
Y

Yttrium

6.217 eV

40
Zr

Zirconium

6.6339 eV

41
Nb

Niobium

6.7589 eV

42
Mo

Molybdenum

7.0924 eV

43
Tc

Technetium

7.28 eV

44
Ru

Ruthenium

7.3605 eV

45
Rh

Rhodium

7.4589 eV

46
Pd

Palladium

8.3369 eV

47
Ag

Silver

7.5762 eV

48
Cd

Cadmium

8.9937 eV

49
In

Indium

5.7864 eV

50
Sn

Tin

7.3438 eV

51
Sb

Antimony

8.64 eV

52
Te

Tellurium

9.0098 eV

53
I

Iodine

10.4513 eV

54
Xe

Xenon

12.1299 eV

55
Cs

Caesium

3.8939 eV

56
Ba

Barium

5.2117 eV

57-71

 

Lanthanoids

 

72
Hf

Hafnium

6.8251 eV

73
Ta

Tantalum

7.89 eV

74
W

Tungsten

7.98 eV

75
Re

Rhenium

7.88 eV

76
Os

Osmium

8.7 eV

77
Ir

Iridium

9.1 eV

78
Pt

Platinum

9 eV

79
Au

Gold

9.2257 eV

80
Hg

Mercury

10.4375 eV

81
Tl

Thallium

6.1083 eV

82
Pb

Lead

7.4167 eV

83
Bi

Bismuth

7.289 eV

84
Po

Polonium

8.4167 eV

85
At

Astatine

9.5 eV

86
Rn

Radon

10.7485 eV

87
Fr

Francium

3.94 eV

88
Ra

Radium

5.2789 eV

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

5.577 eV

58
Ce

Cerium

5.5387 eV

59
Pr

Praseodymium

5.464 eV

60
Nd

Neodymium

5.525 eV

61
Pm

Promethium

5.55 eV

62
Sm

Samarium

5.6437 eV

63
Eu

Europium

5.6704 eV

64
Gd

Gadolinium

6.15 eV

65
Tb

Terbium

5.8939 eV

66
Dy

Dysprosium

5.9389 eV

67
Ho

Holmium

6.0216 eV

68
Er

Erbium

6.1078 eV

69
Th

Thulium

6.1843 eV

70
Yb

Ytterbium

6.2542 eV

71
Lu

Lutetium

5.4259 eV

89
Ac

Actinium

5.17 eV

90
Th

Thorium

6.08 eV

91
Pa

Protactinium

5.89 eV

92
U

Uranium

6.1941 eV

93
Np

Neptunium

6.2657 eV

94
Pu

Plutonium

6.06 eV

95
Am

Americium

5.9933 eV

96
Cm

Curium

6.02 eV

97
Bk

Berkelium

6.23 eV

98
Cf

Californium

6.3 eV

99
Es

Einsteinium

6.42 eV

100
Fm

Fermium

6.5 eV

101
Md

Mendelevium

6.58 eV

102
No

Nobelium

6.65 eV

103
Lr

Lawrencium

 

First Ionization Energy of Hydrogen

First Ionization Energy of Hydrogen is 13.5984 eV.

Ionization energy, also called ionization potential, is the energy necessary to remove an electron from the neutral atom.

X + energy → X+ + e−

where X is any atom or molecule capable of being ionized, X+ is that atom or molecule with an electron removed (positive ion), and e− is the removed electron.

A Hydrogen atom, for example, requires the following ionization energy to remove the outermost electron.

H + IE → H+ + e−        IE = 13.5984 eV

The ionization energy associated with removal of the first electron is most commonly used. The nth ionization energy refers to the amount of energy required to remove an electron from the species with a charge of (n-1).

1st ionization energy

X → X+ + e−

2nd ionization energy

X+ → X2+ + e−

3rd ionization energy

X2+ → X3+ + e−

Ionization Energy for different Elements

There is an ionization energy for each successive electron removed. The electrons that circle the nucleus move in fairly well-defined orbits. Some of these electrons are more tightly bound in the atom than others. For example, only 7.38 eV is required to remove the outermost electron from a lead atom, while 88,000 eV is required to remove the innermost electron. Helps to understand reactivity of elements (especially metals, which lose electrons).

ionization energy - periodic tableIn general, the ionization energy increases moving up a group and moving left to right across a period. Ionization energy is is related with electronegativity and electron affinity. Electrons with low ionization energies have low electronegativities because their nuclei do not exert a strong attractive force on electrons. Elements with high ionization energies have high electronegativities due to the strong pull exerted by the positive nucleus on the negative electrons. Therefore the electronegativity is greatest at the top-right of the periodic table and decreases toward the bottom-left. Moreover:

  • Ionization energy is lowest for the alkali metals which have a single electron outside a closed shell.
  • Ionization energy increases across a row on the periodic maximum for the noble gases which have closed shells.

For example, sodium requires only 496 kJ/mol or 5.14 eV/atom to ionize it. On the other hand neon, the noble gas, immediately preceding it in the periodic table, requires 2081 kJ/mol or 21.56 eV/atom.

Ionization energy

–

Oganesson – Melting Point

Periodic Table of Elements - melting point
1
H

Hydrogen

14.01 K

2
He

Helium

0.95 K

3
Li

Lithium

453.7 K

4
Be

Beryllium

1570 K

5
B

Boron

2348 K

6
C

Carbon

3823 K

7
N

Nitrogen

63.1 K

8
O

Oxygen

54.8 K

9
F

Fluorine

53.5 K

10
Ne

Neon

24.6 K

11
Na

Sodium

370.9 K

12
Mg

Magnesium

923 K

13
Al

Aluminium

933.5 K

14
Si

Silicon

1687 K

15
P

Phosphorus

317.3 K

16
S

Sulfur

388.4 K

17
Cl

Chlorine

171.6 K

18
Ar

Argon

83.8 K

19
K

Potassium

336.5 K

20
Ca

Calcium

1115 K

21
Sc

Scandium

1814 K

22
Ti

Titanium

1941 K

23
V

Vanadium

2183 K

24
Cr

Chromium

2180 K

25
Mn

Manganese

1519 K

26
Fe

Iron

1811 K

27
Co

Cobalt

1768 K

28
Ni

Nickel

1728 K

29
Cu

Copper

1357.8 K

30
Zn

Zinc

692.7 K

31
Ga

Gallium

302.9 K

32
Ge

Germanium

1211.4 K

33
As

Arsenic

1090 K

34
Se

Selenium

494 K

35
Br

Bromine

265.8 K

36
Kr

Krypton

115.8 K

37
Rb

Rubidium

312.5 K

38
Sr

Strontium

1050 K

39
Y

Yttrium

1799 K

40
Zr

Zirconium

2128 K

41
Nb

Niobium

2750 K

42
Mo

Molybdenum

2896 K

43
Tc

Technetium

2430 K

44
Ru

Ruthenium

2607 K

45
Rh

Rhodium

2237 K

46
Pd

Palladium

1828.1 K

47
Ag

Silver

1234.9 K

48
Cd

Cadmium

594.2 K

49
In

Indium

429.8 K

50
Sn

Tin

505.1 K

51
Sb

Antimony

903.8 K

52
Te

Tellurium

722.6 K

53
I

Iodine

386.9 K

54
Xe

Xenon

161.3 K

55
Cs

Caesium

301.6 K

56
Ba

Barium

1000 K

57-71

 

Lanthanoids

 

72
Hf

Hafnium

2506 K

73
Ta

Tantalum

3290 K

74
W

Tungsten

3695 K

75
Re

Rhenium

3459 K

76
Os

Osmium

3306 K

77
Ir

Iridium

2739 K

78
Pt

Platinum

2041.4 K

79
Au

Gold

1337.3 K

80
Hg

Mercury

234.3 K

81
Tl

Thallium

577 K

82
Pb

Lead

600.6 K

83
Bi

Bismuth

544.4 K

84
Po

Polonium

527 K

85
At

Astatine

575 K

86
Rn

Radon

202 K

87
Fr

Francium

300 K

88
Ra

Radium

973 K

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

1193 K

58
Ce

Cerium

1071 K

59
Pr

Praseodymium

1204 K

60
Nd

Neodymium

1294 K

61
Pm

Promethium

1373 K

62
Sm

Samarium

1345 K

63
Eu

Europium

1095 K

64
Gd

Gadolinium

1568 K

65
Tb

Terbium

1629 K

66
Dy

Dysprosium

1685 K

67
Ho

Holmium

1747 K

68
Er

Erbium

1770 K

69
Th

Thulium

1818 K

70
Yb

Ytterbium

1092 K

71
Lu

Lutetium

1936 K

89
Ac

Actinium

1323 K

90
Th

Thorium

2023 K

91
Pa

Protactinium

1845 K

92
U

Uranium

1408 K

93
Np

Neptunium

917 K

94
Pu

Plutonium

913 K

95
Am

Americium

1449 K

96
Cm

Curium

1618 K

97
Bk

Berkelium

1323 K

98
Cf

Californium

1173 K

99
Es

Einsteinium

1133 K

100
Fm

Fermium

1800 K

101
Md

Mendelevium

1100 K

102
No

Nobelium

1100 K

103
Lr

Lawrencium

1900 K

Oganesson – Melting Point

Melting point of Oganesson is –°C.

Note that, these points are associated with the standard atmospheric pressure.

In general, melting is a phase change of a substance from the solid to the liquid phase. The melting point of a substance is the temperature at which this phase change occurs. The melting point also defines a condition in which the solid and liquid can exist in equilibrium. Adding a heat will convert the solid into a liquid with no temperature change. At the melting point the two phases of a substance, liquid and vapor, have identical free energies and therefore are equally likely to exist. Below the melting point, the solid is the more stable state of the two, whereas above the liquid form is preferred. The melting point of a substance depends on pressure and is usually specified at standard pressure. When considered as the temperature of the reverse change from liquid to solid, it is referred to as the freezing point or crystallization point.

See also: Melting Point Depression

The first theory explaining mechanism of melting in the bulk was proposed by Lindemann, who used vibration of atoms in the crystal to explain the melting transition. Solids are similar to liquids in that both are condensed states, with particles that are far closer together than those of a gas. The atoms in a solid are tightly bound to each other, either in a regular geometric lattice (crystalline solids, which include metals and ordinary ice) or irregularly (an amorphous solid such as common window glass), and are typically low in energy. The motion of individual atoms, ions, or molecules in a solid is restricted to vibrational motion about a fixed point. As a solid is heated, its particles vibrate more rapidly as the solid absorbs kinetic energy. At some point the amplitude of vibration becomes so large that the atoms start to invade the space of their nearest neighbors and disturb them and the melting process initiates. The melting point is the temperature at which the disruptive vibrations of the particles of the solid overcome the attractive forces operating within the solid.

As with boiling points, the melting point of a solid is dependent on the strength of those attractive forces. For example, sodium chloride  (NaCl) is an ionic compound that consists of a multitude of strong ionic bonds. Sodium chloride melts at  801°C. On the other hand, ice (solid H2O) is a molecular compound whose molecules are held together by hydrogen bonds, which is effectively a strong example of an interaction between two permanent dipoles. Though hydrogen bonds are the strongest of the intermolecular forces, the strength of hydrogen bonds is much less than that of ionic bonds. The melting point of ice is 0 °C.

Covalent bonds often result in the formation of small collections of better-connected atoms called molecules, which in solids and liquids are bound to other molecules by forces that are often much weaker than the covalent bonds that hold the molecules internally together. Such weak intermolecular bonds give organic molecular substances, such as waxes and oils, their soft bulk character, and their low melting points (in liquids, molecules must cease most structured or oriented contact with each other).

 

melting-and-boiling-point-chemical-elements-chart

–

Tennessine – Melting Point

Periodic Table of Elements - melting point
1
H

Hydrogen

14.01 K

2
He

Helium

0.95 K

3
Li

Lithium

453.7 K

4
Be

Beryllium

1570 K

5
B

Boron

2348 K

6
C

Carbon

3823 K

7
N

Nitrogen

63.1 K

8
O

Oxygen

54.8 K

9
F

Fluorine

53.5 K

10
Ne

Neon

24.6 K

11
Na

Sodium

370.9 K

12
Mg

Magnesium

923 K

13
Al

Aluminium

933.5 K

14
Si

Silicon

1687 K

15
P

Phosphorus

317.3 K

16
S

Sulfur

388.4 K

17
Cl

Chlorine

171.6 K

18
Ar

Argon

83.8 K

19
K

Potassium

336.5 K

20
Ca

Calcium

1115 K

21
Sc

Scandium

1814 K

22
Ti

Titanium

1941 K

23
V

Vanadium

2183 K

24
Cr

Chromium

2180 K

25
Mn

Manganese

1519 K

26
Fe

Iron

1811 K

27
Co

Cobalt

1768 K

28
Ni

Nickel

1728 K

29
Cu

Copper

1357.8 K

30
Zn

Zinc

692.7 K

31
Ga

Gallium

302.9 K

32
Ge

Germanium

1211.4 K

33
As

Arsenic

1090 K

34
Se

Selenium

494 K

35
Br

Bromine

265.8 K

36
Kr

Krypton

115.8 K

37
Rb

Rubidium

312.5 K

38
Sr

Strontium

1050 K

39
Y

Yttrium

1799 K

40
Zr

Zirconium

2128 K

41
Nb

Niobium

2750 K

42
Mo

Molybdenum

2896 K

43
Tc

Technetium

2430 K

44
Ru

Ruthenium

2607 K

45
Rh

Rhodium

2237 K

46
Pd

Palladium

1828.1 K

47
Ag

Silver

1234.9 K

48
Cd

Cadmium

594.2 K

49
In

Indium

429.8 K

50
Sn

Tin

505.1 K

51
Sb

Antimony

903.8 K

52
Te

Tellurium

722.6 K

53
I

Iodine

386.9 K

54
Xe

Xenon

161.3 K

55
Cs

Caesium

301.6 K

56
Ba

Barium

1000 K

57-71

 

Lanthanoids

 

72
Hf

Hafnium

2506 K

73
Ta

Tantalum

3290 K

74
W

Tungsten

3695 K

75
Re

Rhenium

3459 K

76
Os

Osmium

3306 K

77
Ir

Iridium

2739 K

78
Pt

Platinum

2041.4 K

79
Au

Gold

1337.3 K

80
Hg

Mercury

234.3 K

81
Tl

Thallium

577 K

82
Pb

Lead

600.6 K

83
Bi

Bismuth

544.4 K

84
Po

Polonium

527 K

85
At

Astatine

575 K

86
Rn

Radon

202 K

87
Fr

Francium

300 K

88
Ra

Radium

973 K

89-103

 

Actinoids

 

104
Rf

Rutherfordium

 

105
Db

Dubnium

 

106
Sg

Seaborgium

 

107
Bh

Bohrium

 

108
Hs

Hassium

 

109
Mt

Meitnerium

 

110
Ds

Darmstadtium

 

111
Rg

Roentgenium

 

112
Cn

Copernicium

 

113
Nh

Nihonium

 

114
Fl

Flerovium

 

115
Mc

Moscovium

 

116
Lv

Livermorium

 

117
Ts

Tennessine

 

118
Og

Oganesson

 

57
La

Lanthanum

1193 K

58
Ce

Cerium

1071 K

59
Pr

Praseodymium

1204 K

60
Nd

Neodymium

1294 K

61
Pm

Promethium

1373 K

62
Sm

Samarium

1345 K

63
Eu

Europium

1095 K

64
Gd

Gadolinium

1568 K

65
Tb

Terbium

1629 K

66
Dy

Dysprosium

1685 K

67
Ho

Holmium

1747 K

68
Er

Erbium

1770 K

69
Th

Thulium

1818 K

70
Yb

Ytterbium

1092 K

71
Lu

Lutetium

1936 K

89
Ac

Actinium

1323 K

90
Th

Thorium

2023 K

91
Pa

Protactinium

1845 K

92
U

Uranium

1408 K

93
Np

Neptunium

917 K

94
Pu

Plutonium

913 K

95
Am

Americium

1449 K

96
Cm

Curium

1618 K

97
Bk

Berkelium

1323 K

98
Cf

Californium

1173 K

99
Es

Einsteinium

1133 K

100
Fm

Fermium

1800 K

101
Md

Mendelevium

1100 K

102
No

Nobelium

1100 K

103
Lr

Lawrencium

1900 K

Tennessine – Melting Point

Melting point of Tennessine is –°C.

Note that, these points are associated with the standard atmospheric pressure.

In general, melting is a phase change of a substance from the solid to the liquid phase. The melting point of a substance is the temperature at which this phase change occurs. The melting point also defines a condition in which the solid and liquid can exist in equilibrium. Adding a heat will convert the solid into a liquid with no temperature change. At the melting point the two phases of a substance, liquid and vapor, have identical free energies and therefore are equally likely to exist. Below the melting point, the solid is the more stable state of the two, whereas above the liquid form is preferred. The melting point of a substance depends on pressure and is usually specified at standard pressure. When considered as the temperature of the reverse change from liquid to solid, it is referred to as the freezing point or crystallization point.

See also: Melting Point Depression

The first theory explaining mechanism of melting in the bulk was proposed by Lindemann, who used vibration of atoms in the crystal to explain the melting transition. Solids are similar to liquids in that both are condensed states, with particles that are far closer together than those of a gas. The atoms in a solid are tightly bound to each other, either in a regular geometric lattice (crystalline solids, which include metals and ordinary ice) or irregularly (an amorphous solid such as common window glass), and are typically low in energy. The motion of individual atoms, ions, or molecules in a solid is restricted to vibrational motion about a fixed point. As a solid is heated, its particles vibrate more rapidly as the solid absorbs kinetic energy. At some point the amplitude of vibration becomes so large that the atoms start to invade the space of their nearest neighbors and disturb them and the melting process initiates. The melting point is the temperature at which the disruptive vibrations of the particles of the solid overcome the attractive forces operating within the solid.

As with boiling points, the melting point of a solid is dependent on the strength of those attractive forces. For example, sodium chloride  (NaCl) is an ionic compound that consists of a multitude of strong ionic bonds. Sodium chloride melts at  801°C. On the other hand, ice (solid H2O) is a molecular compound whose molecules are held together by hydrogen bonds, which is effectively a strong example of an interaction between two permanent dipoles. Though hydrogen bonds are the strongest of the intermolecular forces, the strength of hydrogen bonds is much less than that of ionic bonds. The melting point of ice is 0 °C.

Covalent bonds often result in the formation of small collections of better-connected atoms called molecules, which in solids and liquids are bound to other molecules by forces that are often much weaker than the covalent bonds that hold the molecules internally together. Such weak intermolecular bonds give organic molecular substances, such as waxes and oils, their soft bulk character, and their low melting points (in liquids, molecules must cease most structured or oriented contact with each other).

 

melting-and-boiling-point-chemical-elements-chart

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