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45 Cards in this Set
- Front
- Back
Proton, neutron electron (location, charge and mass) |
Proton: in nucleus, +1, 1AMU Neutron: in nucleus, no charge, 1AMU Electron: in orbitals around nucleus, -1, 1/1836AMU (negligible) |
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What holds an atom together? |
The electrostatic attraction between the positively charged nucleus (protons have +ve charge) |
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Deflection when passed between electrically charged plates: |
Like charges repel, unlike charges attract. 1. Electrons deflect away from negative plates towards positive. 2. Protons deflect away from positive towards negative. 3. Neutrons have no deflection. (note: electrons undergo MORE deflection than protons cuz they are lighter in mass!!) |
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Atom vs Ion |
Atom is neutral in charge (protons which have + are equal in number to electrons -) Ions are charged atoms by gaining electrons becoming negatively charged (anion) or losing electrons becoming positively charged (cation) |
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Atomic Radius |
Measure of the size of an atom Calculated as half the distance between the nuclei of 2 covalently bonded atoms of the same element. Eg: H2 is a H-H atom. If the distance between the nuclei of the 2 atoms is "d" then its atomic radius is "d/2" |
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Atomic Radius trend across period |
Decrease across each period (atoms get smaller) |
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Atomic Radius trend down group |
Increase down the group (atoms get bigger) Number of shells increases and electrons repel each other and get farther away from the nucleus. Hence a bigger atom. |
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Ionic radius |
measure of the size of an ion |
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Trend of Ionic radii with increasing negative charge |
Increases since atom is gaining electrons to make an ion. Nuclear (positive charge) remained the same so the pull of the nucleus is less on the new electrons. Therefore an increase in ionic radius. |
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Trend of ionic radii with increasing positive charge |
Decreases since here the atom is losing electrons to make an ion. The nuclear charge (positive) remained the same so the pull of the nucleus on the remaining electrons increased. Greater electrostatic force of attraction and hence a decrease in ionic radius. |
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Isotopes definition |
Atoms of the same element that contain the same number of protons and electrons but a different number of neutrons |
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Symbol for different isotopes |
Chemical symbol of element followed by a dash and the mass number of that isotope. Carbon with mass number 13: C-13 Carbon with mass number 14: C-14 All contain 6 protons (and electrons) but increase by 1 neutron each time. |
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Physical and Chemical properties of isotopes |
Similar chemical properties due to the same number of outermost electrons (involved in reactions) Different physical properties due to different neutron numbers which contribute to mass and density. (Density=mass/volume. if mass changes so does density) |
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Electronic configuration meaning |
The arrangement of electrons in an atom |
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Principal quantum shells. (how many electrons per shell) |
given the symbol (n) these are the energy levels around the nucleus. The maximum number of electrons for each shell is: n=2, 8e n=3, 18e n=4, 32e (I know that you are used to saying 2,8,8,18 but this is the way it actually is, to find the number of electrons in a shell we use the formula 2n²) |
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Subshells and orbitals |
s,p,d,f S can carry 1 orbital= 2e p can carry 3 orbitals=6e d can carry 5 orbitals=10e f can carry 7 orbitals=14e |
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Ground state definition |
The most stable electronic configuration for an atom which has the lowest amount of energy. Done by filling subshells with lowest energy first. Pattern ends at n=3 but regular pattern is: (continuation not needed but is 5s-> 4d->5p->6s->4f->5d->6p-> 7s-> 5f-> 6d-> 7p-> 8s. This is why we say 2,8,8,18 do the math. Remember, s s ps ps dps dps fdps fdps) |
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Orbital energy |
Orbitals in the same subshell have the same energy and are said to be degenerate. So p orbitals (known as px, py and pz) all have the same energy if they are in the same principal quantum shell. |
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Quantum shell energy |
The energy of principal shells increase with increase in the number. n=4 has more energy than n=3 which has more energy than n=2 etc. |
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Subshell energy |
Energy of subshells increases in the order s Only exception is between 3d and 4s where 3d has more energy than 4s so the 4s orbital fills up first. |
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S orbitals (shape and size) |
Spherical in shape and size increases with increase shell number. S orbital of n=3 is bigger than s orbital of n=1. |
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P orbitals (shape and size) |
Dumbbell-shaped where every shell has a p orbital except n=1. The 3 orbitals in the p subshell occupy the x, y and z (vertical) axis and are at right angles to each other. The lobes (infinity symbol) get longer and larger as number of shells (n) increases. |
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Electron configuration (numbers and their meanings) |
Electron configurations are written in the form of nsubshell power electrons held by subshell. ex: 1s power 1 1s power 2 2s power 1 2s power 2 (maximum for s is 2) 2p power 1,2,3,4,5 or even 6. 1s power 2 2s power 2 2p power 6 3s power 2 Remember that the power is the number of electrons. so 2+2+6+2=12 The number before the s or p only indicates the principal quantum shell we are in (n). |
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Spin-pair repulsion |
Electrons in an orbital either spin clockwise or anticlockwise. Electrons that spin in the same direction will obviously repel each other causing a spin-pair repulsion. So to minimize this effect electrons try to fit in as many orbitals as they can. As in if we have the electrons in a p subshell each electron will take a separate orbital rather than 2 electrons in 1 orbital and the last in the 2nd. The only time electrons are paired in an orbital is when there isn't any empty orbitals left. If this happens then electrons in an orbital will spin in OPPOSITE directions to minimize the repulsion. So if we have 5 electrons in a p subshell: 1 electron will be alone in an orbital and 4 will be paired up 2 by 2 in the 2 other orbitals spinning in OPPOSITE directions. Check the diagram to know how to draw directions of spinning of an electron. |
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Electron box notation |
A box represents the orbital. The boxes are arranged in order of increasing energy just like the subshells. Electrons are represented by opposite direction arrows to show that they are spinning oppositely. |
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Electron box notation example |
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Free radical |
When there is 1 or more unpaired electron. This unpaired electron is shown as a dot. |
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Full Electron configuration |
Fully writing out the electrons in each subshell of an atom. As in Sodium would be: |
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Shorthand electron configuration |
Using the nearest noble gas symbol BEFORE the element we are configuring then continuing whatever is left. So sodium would be [Ne] 3s¹. Where Ne is neon which has 10 electrons. and the electron that's left is in the 3s orbital. So [Ne] 3s¹. |
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Transition metals 4s and 3d subshells |
The transition metals fill the 4s subshell before the 3d subshell and lose electrons from the 4s first and not from the 3d subshell (the 4s subshell is lower in energy) |
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s block d block d block f block elements |
s block elements have their valence electrons in an s orbital (first 2 groups) p block elements have their valence electrons in a p orbital (Group 5,6,7,8) d block elements have their valence electrons in a d orbital (transition elements. although they fill up the 4s orbital first and lose electrons from it first they still have their valence electrons in the d orbitals) f block elements have their valence electrons in an f orbital (the lanthanides and actinides, the 2 periods underneath the periodic table) |
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Exceptions to the configuration |
1. Chromium configured as 2. Copper [Ar] 3d10 4s1 not [Ar] 3d9 4s2 (filled up only 1 electron in the 4s orbital instead of 2 before moving on to the 3d orbitals.) This is because [Ar] 3d5 4s1 and [Ar] 3d10 4s1 configurations are energetically stable. |
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Ionization Energy IE definition |
amount of energy required to remove one mole of electrons from one mole of gaseous atoms of an element to form one mole of gaseous ions. |
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Ionization Energy standard conditions |
1. 298 K temperature 2. 1atm pressure |
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Ionization Energy Unit |
kjmol-1 kj/mol |
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Ionization Energies 1st 2nd 3rd |
The energies required to lose the first 2nd and 3rd moles of electrons respectfully from an atom to form 1st 2nd and 3rd mole of positively charged ions step by step and in order. (All in the gaseous state) |
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Factors affecting 1st ionization energy (4 points) |
Size of nuclear charge Distance of outer electrons from nucleus Shielding effect of inner electrons Spin-Pair repulsion |
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Ionization energy across a period |
Increases due to: Nuclear charge increase making the atomic radii decrease and electrons get pulled closer and distance decreases. Shielding by inner electrons doesn't change as new electrons are being added to same shell. So more energy is needed to overcome the electrostatic attraction forces. So Ionization energy increases. |
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Dips in trend (2 points) |
1. There is a slight decrease in ionization energy between beryllium and boron as boron has a 2p subshell and hence is further away from the nucleus than the 2s subshell of beryllium. 2. There is a slight decrease between nitrogen and oxygen due to spin-pair repulsion in the 2px orbital (the first p orbital) of the oxygen atom. Since oxygen is 8 it has a configuration of 1s2 2s2 2px2 2py1 2pz1 so the 2 electrons in 2px2 have a spin-pair repulsion making it slightly easier for oxygen to lose that electron. |
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Ionization energy from one period to the next |
Large decrease in ionization energy between last element in a period to first element in the next due to adding of new shell which causes: increased shielding effect of inner electrons These factors outweigh the +1 addition to the nuclear charge. |
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Ionization energy down a group |
Decreases, although the nuclear charge is increasing, the atomic radius is also getting bigger as distance increases due to adding of shells. (every time you go down a group you add a shell) Shielding effect of inner electrons also increases as shells are added. |
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Ionization Energy down a group vs across a period |
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Successive ionization energy |
The loss of all electrons of an atom until the nucleus. b) Atomic radius/distance decreases and shielding effect decreases as we move closer to the nucleus so more energy needed to overcome attractive forces. Electrons aren't removed with periodic changes of energy however. |
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Ionization energies, jumps and increases |
The first electron is always the easiest to remove since its either the farthest away or is with another electron in the same orbital and has a spin-pair repulsion. The second electron requires more energy if its in the same orbital as there is no spin-pair repulsion. But since they are in the same principal shell the increase in energy isn't that high. There is a huge increase in energy required however as we move from one principal quantum shell to another. This is because we get closer to the nucleus so: shielding effect decreases. |
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Summary of factors affecting ionization energy |
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