Inorganic ACS

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190 Terms

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Nuclide

Type of atom with atomic number Z, equal to number of protons in nucleus (and electrons, since atom is neutral)

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Mass number

A = the number of protons and neutrons in nucleus

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Number of neutrons in an atom

A (mass number) - Z (atomic number)

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Isotope

atom of an element that differ only by the number of neutrons (mass)

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Monotopic

one natural nuclide

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Relative atomic mass from abundance (Ar)

= (( %/100 ) * (accurate mass)) + ““…

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Isotopes of an element have the same BLANK, but different BLANK

atomic number Z, atomic masses

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ΔE = (in terms of frequency)

hv

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Units of E

J, Joules

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Units of v (frequency)

s-1 or Hz

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c (speed of light)

= λv

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units of λ

m (meters)

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ΔE = (in terms of wavelength)

hc/λ

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ṽ = (in terms of wavelength)

1/λ

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ṽ = (in terms of n)

R((1/n2 )-(1/n’ 2 ))

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R (Rydberg constant) for Hydrogen

= 1.097e7 m-1 or 1.097e5 cm-1

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n (principal quantum #) =

mvr/(h/2pi) (where m = mass of electron, v = velocity of electron, r = radius of orbit)

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rn (electron orbit radius)

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ε0 (permittivity of a vacuum)

= 8.854e-12 Fm-1

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e (elementary charge on an electron)

= 1.602e-19 C

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Ionization in terms of n

n=1 → n =

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Units of IE (ionization energy)

per mol of atoms

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IE =

E∞ - E1 = hc/λ

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Ionization energy of Hydrogen

1312 kJ mol-1 or 13.6 eV

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λ (in terms of particles)

= h/mv (m = mass of particle, v = velocity of particle)

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1eV

= 96.4853 kJ mol-1

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possible values of principal quantum number

1<=n<=

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l (orbital quantum number)

determines shape of orbital and angular momentum

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possible values of l

0,1,2…(n-1)

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ml (magnetic quantum number)

determines orientation of orbital

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possible values of ml

between +l and -l

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For a 1s orbital, what is n

1

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For a 1s orbital what is l

0

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For a 1s orbital what is ml

0

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for a 1s orbital what is the radial part of the wavefunction R(r)

2e-r

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for a 1s orbital what is the angular part of the wavefunction A(θ,Φ)

1/(2sq(pi))

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for a 2s orbital what is n

2

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for a 2s orbital what is l

0

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for a 2s orbital what is ml

0

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for a 2s orbital what is the radial part of the wavefunction R(r)

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for a 2s orbital what is the angular part of the wavefunction A(θ,Φ)

1/(2sq(pi))

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for a 2px orbital what is n

2

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for a 2px orbital what is l

1

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for a 2px orbital what is ml

+1

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for a 2px orbital what is the radial part of the wavefunction R(r)

<p></p>
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for a 2px orbital what is the angular part of the wavefunction A(θ,Φ)

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for a 2pz orbital what is n

2

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for a 2pz orbital what is l

1

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for a 2pz orbital what is ml

0

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for a 2pz orbital what is the radial part of the wavefunction R(r)

<p></p>
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for a 2pz orbital what is the angular part of the wavefunction A(θ,Φ)

knowt flashcard image
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for a 2py orbital what is n

2

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for a 2py orbital what is l

1

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for a 2py orbital what is ml

-1

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for a 2py orbital what is the radial part of the wavefunction R(r)

knowt flashcard image
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for a 2py orbital what is the angular part of the wavefunction A(θ,Φ)

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degenerate orbitals possess the same

energy

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For a given value of n (n greater than or equal to 1) there is

1 s atomic orbital

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For a given value of n (n greater than or equal to 2) there is

3 p atomic orbitals

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For a given value of n (n greater than or equal to 3) there is

5 d atomic orbitals

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For a given value of n (n greater than or equal to 4) there is

7 f atomic orbitals

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likelihood of an electron being further from the nucleus

increases as n increases (not linearly)

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s atomic orbitals have a finite value of

R(r) at the nucleus

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for all orbitals other than s

R(r) = 0 at the nucleus

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for the 1s orbital

R(r) is always positive

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for the first orbital of all other orbital types besides 1s (ie. 2p, 3d, 4f)

R(r) is positive everywhere except at the origin

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for the second orbital of a given type (ie. 2s, 3p, 4d, 5f)

R(r) may be positive or negative but the wavefunction has only one sign change

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the point at which R(r)=0 (not including the origin) is called

a radial node

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for the third orbital of a given type (ie. 3s, 4p, 5d, 6f)

R(r) has two sign changes (it possesses two radial nodes)

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ns orbitals have BLANK radial nodes

(n-1)

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np orbitals have BLANK radial nodes

(n-2)

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nd orbitals have BLANK radial nodes

(n-3)

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nf orbitals have BLANK radial nodes

(n-4)

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Radial distribution

=4pir2R(r)2

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Using the radial distribution function, disregarding r=0, what points correspond to radial nodes?

Anywhere 4pir2R(r)2=0

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<p>Using the graph, how many radial nodes does a 1s orbital have</p>

Using the graph, how many radial nodes does a 1s orbital have

0 radial nodes

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<p>Using the graph, how many radial nodes does a 2s orbital have</p>

Using the graph, how many radial nodes does a 2s orbital have

1 radial node

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<p>Using the graph how many radial nodes does a 3s atomic orbital have?</p>

Using the graph how many radial nodes does a 3s atomic orbital have?

2 radial nodes

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<p>Using the graph how many radial nodes does a 3d orbital have? </p>

Using the graph how many radial nodes does a 3d orbital have?

0 radial nodes

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<p>Using the graph, how many radial nodes does a 3p orbital have?</p>

Using the graph, how many radial nodes does a 3p orbital have?

1 radial node

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<p>Using the graph how many radial nodes does a 3s orbital have?</p>

Using the graph how many radial nodes does a 3s orbital have?

2

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The angular part of the wavefunction A(θ,Φ) is independent of

n

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For s orbitals, A(θ,Φ) is independent of

θ and Φ

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E (orbital energies) =

-(kZ2)/n2 (where Z = atomic number and k = hcR = 1.312e3 kJ mol-1)

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Orbital energy levels get closer as

n increases

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The larger the n the larger the

size of the orbital

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And increase in orbital size corresponds to an increase in

an orbital being more diffuse

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S (spin quantum number) =

1/2

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ms (magnetic spin quantum number) =

± 1/2

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Orbital angular momentum =

Sqrt(l(l+1))*(h/2pi)

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spin angular momentum =

Sqrt(s(s+1))*(h/2pi)

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total angular momentum =

Sqrt(j(j+1))*(h/2pi)

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j (inner quantum number) =

|l+s| or |l-s|

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In a multi-electron atom, orbitals with the same value of n but different values of l are

NOT degenerate

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The IE of noble gases are

high

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IE of group one elements are

low

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IE increases

across a period

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IE is similar for

a given row of d block elements

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EA =

-ΔU (at 0K)

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Adding an electron to an atom is typically

exothermic