What is Roentgenium – Properties of Roentgenium Element – Symbol Rg

What is Roentgenium

Roentgenium is a chemical element with atomic number 111 which means there are 111 protons and 111 electrons in the atomic structure. The chemical symbol for Roentgenium is Rg.

Roentgenium – Properties

ElementRoentgenium
Atomic Number111
SymbolRg
Element CategoryTransition Metal
Phase at STPSynthetic
Atomic Mass [amu]272
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 6d9 7s2 ?
Possible Oxidation States
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]
1st Ionization Energy [eV]
Year of Discovery1994
DiscovererHofmann, Sigurd et. al.
Thermal properties
Melting Point [Celsius scale]
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Roentgenium

Atomic mass of Roentgenium is 272 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Roentgenium

Density of Roentgenium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Roentgenium

Electron Affinity of Roentgenium is — kJ/mol.

Electronegativity of Roentgenium is .

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Roentgenium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Roentgenium.

Rg + e → Rg        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Roentgenium is:

χ = —

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Roentgenium

First Ionization Energy of Roentgenium is — 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 Roentgenium atom, for example, requires the following ionization energy to remove the outermost electron.

Rg + IE → Rg+ + e        IE = — 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Roentgenium – Melting Point and Boiling Point

Melting point of Roentgenium is –°C.

Boiling point of Roentgenium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Roentgenium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Roentgenium is — J/g K.

Latent Heat of Fusion of Roentgenium is — kJ/mol.

Latent Heat of Vaporization of Roentgenium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Roentgenium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Mendelevium – Properties of Mendelevium Element – Symbol Md

What is Mendelevium

Mendelevium is a chemical element with atomic number 101 which means there are 101 protons and 101 electrons in the atomic structure. The chemical symbol for Mendelevium is Md.

Mendelevium is a metallic radioactive transuranic element in the actinide series, it is the first element that currently cannot be produced in macroscopic quantities.

Mendelevium – Properties

ElementMendelevium
Atomic Number101
SymbolMd
Element CategoryRare Earth Metal
Phase at STPSynthetic
Atomic Mass [amu]258
Density at STP [g/cm3]
Electron Configuration[Rn] 5f13 7s2
Possible Oxidation States+2,3
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]1.3
1st Ionization Energy [eV]6.58
Year of Discovery1955
DiscovererStanley G. Thompson, Glenn T. Seaborg, Bernard G. Harvey, Gregory R. Choppin, Albert Ghiorso
Thermal properties
Melting Point [Celsius scale]827
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Mendelevium

Atomic mass of Mendelevium is 258 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Mendelevium

Density of Mendelevium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Mendelevium

Electron Affinity of Mendelevium is — kJ/mol.

Electronegativity of Mendelevium is 1.3.

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Mendelevium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Mendelevium.

Md + e → Md        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Mendelevium is:

χ = 1.3

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Mendelevium

First Ionization Energy of Mendelevium is 6.58 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 Mendelevium atom, for example, requires the following ionization energy to remove the outermost electron.

Md + IE → Md+ + e        IE = 6.58 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Mendelevium – Melting Point and Boiling Point

Melting point of Mendelevium is 827°C.

Boiling point of Mendelevium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Mendelevium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Mendelevium is — J/g K.

Latent Heat of Fusion of Mendelevium is — kJ/mol.

Latent Heat of Vaporization of Mendelevium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Mendelevium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Copernicium – Properties of Copernicium Element – Symbol Cn

What is Copernicium

Copernicium is a chemical element with atomic number 112 which means there are 112 protons and 112 electrons in the atomic structure. The chemical symbol for Copernicium is Cn.

Copernicium – Properties

ElementCopernicium
Atomic Number112
SymbolCn
Element CategoryTransition Metal
Phase at STPSynthetic
Atomic Mass [amu]285
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 6d10 7s2 ?
Possible Oxidation States
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]
1st Ionization Energy [eV]
Year of Discovery1996
DiscovererArmbruster, Paula & Muenzenberg, Dr. Gottfried
Thermal properties
Melting Point [Celsius scale]
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Copernicium

Atomic mass of Copernicium is 285 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Copernicium

Density of Copernicium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Copernicium

Electron Affinity of Copernicium is — kJ/mol.

Electronegativity of Copernicium is .

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Copernicium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Copernicium.

Cn + e → Cn        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Copernicium is:

χ = —

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Copernicium

First Ionization Energy of Copernicium is — 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 Copernicium atom, for example, requires the following ionization energy to remove the outermost electron.

Cn + IE → Cn+ + e        IE = — 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Copernicium – Melting Point and Boiling Point

Melting point of Copernicium is –°C.

Boiling point of Copernicium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Copernicium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Copernicium is — J/g K.

Latent Heat of Fusion of Copernicium is — kJ/mol.

Latent Heat of Vaporization of Copernicium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Copernicium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Nobelium – Properties of Nobelium Element – Symbol No

What is Nobelium

Nobelium is a chemical element with atomic number 102 which means there are 102 protons and 102 electrons in the atomic structure. The chemical symbol for Nobelium is No.

Nobelium is the tenth transuranic element and is the penultimate member of the actinide series. Like all elements with atomic number over 100, nobelium can only be produced in particle accelerators by bombarding lighter elements with charged particles.

Nobelium – Properties

ElementNobelium
Atomic Number102
SymbolNo
Element CategoryRare Earth Metal
Phase at STPSynthetic
Atomic Mass [amu]259
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 7s2
Possible Oxidation States+2,3
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]1.3
1st Ionization Energy [eV]6.65
Year of Discovery1958
DiscovererAlbert Ghiorso, Glenn T. Seaborg, Torbørn Sikkeland, John R. Walton
Thermal properties
Melting Point [Celsius scale]827
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Nobelium

Atomic mass of Nobelium is 259 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Nobelium

Density of Nobelium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Nobelium

Electron Affinity of Nobelium is — kJ/mol.

Electronegativity of Nobelium is 1.3.

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Nobelium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Nobelium.

No + e → No        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Nobelium is:

χ = 1.3

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Nobelium

First Ionization Energy of Nobelium is 6.65 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 Nobelium atom, for example, requires the following ionization energy to remove the outermost electron.

No + IE → No+ + e        IE = 6.65 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Nobelium – Melting Point and Boiling Point

Melting point of Nobelium is 827°C.

Boiling point of Nobelium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Nobelium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Nobelium is — J/g K.

Latent Heat of Fusion of Nobelium is — kJ/mol.

Latent Heat of Vaporization of Nobelium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Nobelium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Nihonium – Properties of Nihonium Element – Symbol Nh

What is Nihonium

Nihonium is a chemical element with atomic number 113 which means there are 113 protons and 113 electrons in the atomic structure. The chemical symbol for Nihonium is Nh.

Nihonium – Properties

ElementNihonium
Atomic Number113
SymbolNh
Element CategoryPost-Transition Metal
Phase at STPSynthetic
Atomic Mass [amu]286
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 6d10 7s2 7p1 ?
Possible Oxidation States
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]
1st Ionization Energy [eV]
Year of Discovery2004
DiscovererY. T. Oganessian et. al.
Thermal properties
Melting Point [Celsius scale]
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Nihonium

Atomic mass of Nihonium is 286 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Nihonium

Density of Nihonium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Nihonium

Electron Affinity of Nihonium is — kJ/mol.

Electronegativity of Nihonium is .

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Nihonium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Nihonium.

Nh + e → Nh        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Nihonium is:

χ = —

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Nihonium

First Ionization Energy of Nihonium is — 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 Nihonium atom, for example, requires the following ionization energy to remove the outermost electron.

Nh + IE → Nh+ + e        IE = — 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Nihonium – Melting Point and Boiling Point

Melting point of Nihonium is –°C.

Boiling point of Nihonium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Nihonium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Nihonium is — J/g K.

Latent Heat of Fusion of Nihonium is — kJ/mol.

Latent Heat of Vaporization of Nihonium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Nihonium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Lawrencium – Properties of Lawrencium Element – Symbol Lr

What is Lawrencium

Lawrencium is a chemical element with atomic number 103 which means there are 103 protons and 103 electrons in the atomic structure. The chemical symbol for Lawrencium is Lr.

Lawrencium is the final member of the actinide series. Like all elements with atomic number over 100, lawrencium can only be produced in particle accelerators by bombarding lighter elements with charged particles.

Lawrencium – Properties

ElementLawrencium
Atomic Number103
SymbolLr
Element CategoryRare Earth Metal
Phase at STPSynthetic
Atomic Mass [amu]262
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 7s2 7p1
Possible Oxidation States+3
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]
1st Ionization Energy [eV]
Year of Discovery1961
DiscovererAlbert Ghiorso, Torbjørn Sikkeland, Almon E. Larsh, Robert M. Latimer
Thermal properties
Melting Point [Celsius scale]1627
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Lawrencium

Atomic mass of Lawrencium is 262 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Lawrencium

Density of Lawrencium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Lawrencium

Electron Affinity of Lawrencium is — kJ/mol.

Electronegativity of Lawrencium is .

Electron Affinity

In chemistry and atomic physics, the electron affinity of an atom or molecule is defined as:

the change in energy (in kJ/mole) of a neutral atom or molecule (in the gaseous phase) when an electron is added to the atom to form a negative ion.

X + e → X + energy        Affinity = – ∆H

In other words, it can be expressed as the neutral atom’s likelihood of gaining an electron. Note that, ionization energies measure the tendency of a neutral atom to resist the loss of electrons. Electron affinities are more difficult to measure than ionization energies.

An atom of Lawrencium in the gas phase, for example, gives off energy when it gains an electron to form an ion of Lawrencium.

Lr + e → Lr        – ∆H = Affinity = — kJ/mol

To use electron affinities properly, it is essential to keep track of sign. When an electron is added to a neutral atom, energy is released. This affinity is known as the first electron affinity and these energies are negative. By convention, the negative sign shows a release of energy. However, more energy is required to add an electron to a negative ion which overwhelms any the release of energy from the electron attachment process. This affinity is known as the second electron affinity and these energies are positive.

Affinities of Non metals vs. Affinities of Metals

  • Metals: Metals like to lose valence electrons to form cations to have a fully stable shell. The electron affinity of metals is lower than that of nonmetals. Mercury most weakly attracts an extra electron.
  • Nonmetals: Generally, nonmetals have more positive electron affinity than metals. Nonmetals like to gain electrons to form anions to have a fully stable electron shell. Chlorine most strongly attracts extra electrons. The electron affinities of the noble gases have not been conclusively measured, so they may or may not have slightly negative values.

Electronegativity

Electronegativity, symbol χ, is a chemical property that describes the tendency of an atom to attract electrons towards this atom. For this purposes, a dimensionless quantity the Pauling scale, symbol χ, is the most commonly used.

The electronegativity of Lawrencium is:

χ = —

In general, an atom’s electronegativity is affected by both its atomic number and the distance at which its valence electrons reside from the charged nucleus. The higher the associated electronegativity number, the more an element or compound attracts electrons towards it.

The most electronegative atom, fluorine, is assigned a value of 4.0, and values range down to cesium and francium which are the least electronegative at 0.7.

electron affinity and electronegativity

First Ionization Energy of Lawrencium

First Ionization Energy of Lawrencium is — 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 Lawrencium atom, for example, requires the following ionization energy to remove the outermost electron.

Lr + IE → Lr+ + e        IE = — 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).

In general, the ionization energy increases moving up a group and moving left to right across a period. 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

 

Lawrencium – Melting Point and Boiling Point

Melting point of Lawrencium is 1627°C.

Boiling point of Lawrencium is –°C.

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

Boiling Point – Saturation

In thermodynamics, the term saturation defines a condition in which a mixture of vapor and liquid can exist together at a given temperature and pressure. The temperature at which vaporization (boiling) starts to occur for a given pressure is called the saturation temperature or boiling point. The pressure at which vaporization (boiling) starts to occur for a given temperature is called the saturation pressure. When considered as the temperature of the reverse change from vapor to liquid, it is referred to as the condensation point.

Melting Point – Saturation

In thermodynamics, the melting point 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. 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.

melting and boiling point

Lawrencium – Specific Heat, Latent Heat of Fusion, Latent Heat of Vaporization

Specific heat of Lawrencium is — J/g K.

Latent Heat of Fusion of Lawrencium is — kJ/mol.

Latent Heat of Vaporization of Lawrencium is — kJ/mol.

Specific Heat

Specific heat, or specific heat capacity, is a property related to internal energy that is very important in thermodynamics. The intensive properties cv and cp are defined for pure, simple compressible substances as partial derivatives of the internal energy u(T, v) and enthalpy h(T, p), respectively:

Specific Heat at Constant Volume and Constant Pressure

Table of specific heat capacitieswhere the subscripts v and p denote the variables held fixed during differentiation. The properties cv and cp are referred to as specific heats(or heat capacities) because under certain special conditions they relate the temperature change of a system to the amount of energy added by heat transfer. Their SI units are J/kg K or J/mol K.

Different substances are affected to different magnitudes by the addition of heat. When a given amount of heat is added to different substances, their temperatures increase by different amounts.

Heat capacity is an extensive property of matter, meaning it is proportional to the size of the system. Heat capacity C has the unit of energy per degree or energy per kelvin. When expressing the same phenomenon as an intensive property, the heat capacity is divided by the amount of substance, mass, or volume, thus the quantity is independent of the size or extent of the sample.

specific heat - heat capacity

 

Latent Heat of Vaporization

Phase changes - enthalpy of vaporization

In general, when a material changes phase from solid to liquid, or from liquid to gas a certain amount of energy is involved in this change of phase. In case of liquid to gas phase change, this amount of energy is known as the enthalpy of vaporization, (symbol ∆Hvap; unit: J) also known as the (latent) heat of vaporization or heat of evaporation. As an example, see the figure, which descibes phase transitions of water.

Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the gas (the pΔV work). When latent heat is added, no temperature change occurs. The enthalpy of vaporization is a function of the pressure at which that transformation takes place.

Latent Heat of Fusion

In case of solid to liquid phase change, the change in enthalpy required to change its state is known as the enthalpy of fusion, (symbol ∆Hfus; unit: J) also known as the (latent) heat of fusion. Latent heat is the amount of heat added to or removed from a substance to produce a change in phase. This energy breaks down the intermolecular attractive forces, and also must provide the energy necessary to expand the system (the pΔV work).

The liquid phase has a higher internal energy than the solid phase. This means energy must be supplied to a solid in order to melt it and energy is released from a liquid when it freezes, because the molecules in the liquid experience weaker intermolecular forces and so have a higher potential energy (a kind of bond-dissociation energy for intermolecular forces).

The temperature at which the phase transition occurs is the melting point.

When latent heat is added, no temperature change occurs. The enthalpy of fusion is a function of the pressure at which that transformation takes place. By convention, the pressure is assumed to be 1 atm (101.325 kPa) unless otherwise specified.

heat of fusion and vaporization

Lawrencium in Periodic Table

Hydro­gen1HHe­lium2He
Lith­ium3LiBeryl­lium4BeBoron5BCarbon6CNitro­gen7NOxy­gen8OFluor­ine9FNeon10Ne
So­dium11NaMagne­sium12MgAlumin­ium13AlSili­con14SiPhos­phorus15PSulfur16SChlor­ine17ClArgon18Ar
Potas­sium19KCal­cium20CaScan­dium21ScTita­nium22TiVana­dium23VChrom­ium24CrManga­nese25MnIron26FeCobalt27CoNickel28NiCopper29CuZinc30ZnGallium31GaGerma­nium32GeArsenic33AsSele­nium34SeBromine35BrKryp­ton36Kr
Rubid­ium37RbStront­ium38SrYttrium39YZirco­nium40ZrNio­bium41NbMolyb­denum42MoTech­netium43TcRuthe­nium44RuRho­dium45RhPallad­ium46PdSilver47AgCad­mium48CdIndium49InTin50SnAnti­mony51SbTellur­ium52TeIodine53IXenon54Xe
Cae­sium55CsBa­rium56BaLan­thanum57La1 asteriskHaf­nium72HfTanta­lum73TaTung­sten74WRhe­nium75ReOs­mium76OsIridium77IrPlat­inum78PtGold79AuMer­cury80HgThallium81TlLead82PbBis­muth83BiPolo­nium84PoAsta­tine85AtRadon86Rn
Fran­cium87FrRa­dium88RaActin­ium89Ac1 asteriskRuther­fordium104RfDub­nium105DbSea­borgium106SgBohr­ium107BhHas­sium108HsMeit­nerium109MtDarm­stadtium110DsRoent­genium111RgCoper­nicium112CnNihon­ium113NhFlerov­ium114FlMoscov­ium115McLiver­morium116LvTenness­ine117TsOga­nesson118Og
1 asteriskCerium58CePraseo­dymium59PrNeo­dymium60NdProme­thium61PmSama­rium62SmEurop­ium63EuGadolin­ium64GdTer­bium65TbDyspro­sium66DyHol­mium67HoErbium68ErThulium69TmYtter­bium70YbLute­tium71Lu
1 asteriskThor­ium90ThProtac­tinium91PaUra­nium92UNeptu­nium93NpPluto­nium94PuAmeri­cium95AmCurium96CmBerkel­ium97BkCalifor­nium98CfEinstei­nium99EsFer­mium100FmMende­levium101MdNobel­ium102NoLawren­cium103Lr



What is Flerovium – Properties of Flerovium Element – Symbol Fl

What is Flerovium

Flerovium is a chemical element with atomic number 114 which means there are 114 protons and 114 electrons in the atomic structure. The chemical symbol for Flerovium is Fl.

Flerovium – Properties

ElementFlerovium
Atomic Number114
SymbolFl
Element CategoryPost-Transition Metal
Phase at STPSynthetic
Atomic Mass [amu]289
Density at STP [g/cm3]
Electron Configuration[Rn] 5f14 6d10 7s2 7p2 ?
Possible Oxidation States
Electron Affinity [kJ/mol]
Electronegativity [Pauling scale]
1st Ionization Energy [eV]
Year of Discovery1998
DiscovererScientists at Dubna, Russia
Thermal properties
Melting Point [Celsius scale]
Boiling Point [Celsius scale]
Thermal Conductivity [W/m K]
Specific Heat [J/g K]
Heat of Fusion [kJ/mol]
Heat of Vaporization [kJ/mol]

 

Atomic Mass of Flerovium

Atomic mass of Flerovium is 289 u. 

Note that, each element may contain more isotopes, therefore this resulting atomic mass is calculated from naturally-occuring isotopes and their abundance.

The unit of measure for mass is the atomic mass unit (amu). One atomic mass unit is equal to 1.66 x 10-24 grams. One unified atomic mass unit is approximately the mass of one nucleon (either a single proton or neutron) and is numerically equivalent to 1 g/mol.

For 12C the atomic mass is exactly 12u, since the atomic mass unit is defined from it. For other isotopes, the isotopic mass usually differs and is usually within 0.1 u of the mass number. For example, 63Cu (29 protons and 34 neutrons) has a mass number of 63 and an isotopic mass in its nuclear ground state is 62.91367 u.

There are two reasons for the difference between mass number and isotopic mass, known as the mass defect:

  1. The neutron is slightly heavier than the proton. This increases the mass of nuclei with more neutrons than protons relative to the atomic mass unit scale based on 12C with equal numbers of protons and neutrons.
  2. The nuclear binding energy varies between nuclei. A nucleus with greater binding energy has a lower total energy, and therefore a lower mass according to Einstein’s mass-energy equivalence relation E = mc2. For 63Cu the atomic mass is less than 63 so this must be the dominant factor.

See also: Mass Number

Density of Flerovium

Density of Flerovium is –g/cm3.
Density - Gas - Liquid - Solid

Typical densities of various substances at atmospheric pressure.

Density is defined as the mass per unit volume. It is an intensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit is kilograms per cubic meter (kg/m3). The Standard English unit is pounds mass per cubic foot (lbm/ft3).

See also: What is Density

See also: Densest Materials of the Earth

density - chemical elements

Electron Affinity and Electronegativity of Flerovium

Electron Affini