EK Chem Ch1 Gen Chem Flashcards
isotopes
two or more atoms of the same element that contain different number of neutrons Hydrogen= H1 = protium, H2 is deuterium and H3 is tritium. 99.98% of naturally occurring H is protium Carbon isotopes= C12, C13, C14. each of carbon’s isotopes contain 6 protons with varying numbers of neutrons. 6 protons are what define carbon, if number of protons changed it would no longer be carbon C12= 6 adn 6 C13= 6 protons and 7 neutrons C14= 6 protons and 8 neutrons
cation
-ion with fewer electrons than protons -positive charge size -when a neutral atom loses an e to become a cation, it gets smaller -atom still has same amount of protons but there are now more protons than electrons, so as a result that positive charge of the nucleus exerts a greater attractive force on each valence e, pulling them closer to nucleus -loss of e also reduces the repulsive forces between the electrons, further contributing to dec in size -net effect removing e makes ionic radius smaller than atomic radius
anion
-ion with more electrons than protons -negatively charged -gain e it becomes larger, makes the ionic radius larger than atomic radius - atom now has more e than protons, so the positive charge of the nucleus pulls less strongly on each individual valence electron. The addition of an e also inc the repulsive forces btw the e, pushing them farther away from each other. - net effect is that anion is larger than the neutral atom
ion
when the number of electrons in an atom does not equal the number fo protons, the atom carries a charge and is called an ion
salt
neutral compound* - made up of positive and negative ion together
metal
large atoms that tend to lose e to form positive ions and positive oxidation states - left hand side of table - atom in a sea of electrons, which emphasizes their loose hold on their electrons and the fluid like nature of their vlence electrons, easy movement of e within metals is what gives them their metallic character. -ductility (easily stretched) mallealbility (easily hammered into thin strips) -thermal + electrical conductivity -lusterous? - all metals besides mercury exist at room temperature -electrons move easily from one metal atom to the next, transferring energy or charge in the form fo heat or electricity
nonmetals
- form covalent bonds, vs metals who form ionic -generally have lower melting points than metals and tend to form anions, which commonly react with metal cations to form ionic compounds ex. NaCl
group 11 transition metals ions…
makes 1+ ions, Cu+, Ag +, and Au+, all others in this group are Au3+ and Cu2+
there are five 3+ ion transition metals….
Cr3+, Fe3+, Au3+, Al3+, and Bi3+ all other ions if not mentioned above as 1+ are 2+
valence e
electrons in the outer shell, elements in the same group on the periodic table have similar chemical properties because they have the same number of valence e
diatomic molcules
-elements that tend to exist as diatomic molecules are H, O, N and the halogens -so when these are every discussed assume that they are in their diatomic form unless otherwise stated -so when they say “nitrogen is nonreactive” refers to N2 not N - Fl2 and Cl2 are gases at room temp, br2 diatomic liquid, I2 a diatomic solid**
halogens
- Fl2 and Cl2 are gases at room temp, br2 diatomic liquid, I2 a diatomic solid** - react with H to form gaseous hydrogen halides, which are soluble in water, forming hydrohalic acids
periodic trends
-atomic radius, ionization energy, electronegativity and electron affinity - atomic radius inc as goes down and to the left, everything else inc up and to the right**
atomic radius
distance from center of the nucleus to the outermost electron -corresponds to the size of the atom -moving across period radius dec b/c each subsequent e has an additional proton, which pulls more strongly on the surrounding electron -moving down a group, new shells of e are dded. these outer es are “shielded” from the attraction of the protons in the inner nucleus, so atomic radius inc as move down group
Zeff
-the effective nuclear charge is the charge felt by the most recently added e. in perfect shielding, each e added to an atom would be completely shielded from the attractive force of all protons except for the last proton added and the Zeff would be 1 eV for each electron -without shielding, each e added would feel the full attractive force of all the protons in the nucleus, and the Zeff would simply be equal to Z for each electron
ionization energy
energy needed to detach an e from an atom -inc along periodic table from left to right and from bottom to top -when an e is more strongly attached to teh nucleus, more energy is required to detach it
first ionization energy
energy necessary to remove an e from a neutral atom in its gaseous state to form a 1+ cation -is largest for the noble gas within a given period because the electron removed was completing a stable octet configuration
second ionization energy
-energy required to remove second e from teh same atom to form a 2+ cation - 3rd,4,5, etc are all named the same. -second ionization energy is always greater than the first because once one electron is removed the effective nuclear charge inc for the remaining e -3rd, 4th, 5th ionization energies similarly inc -largest inc in ionization energy occurs when the e to be detached was completing a stable octet configuration
Zeff useful for periodic trends
inc from left to right across a period, so each new e is pulled closer to the nuc and held more tightly than the previous one 1. pulling outermost e closer dec atomic radius 2. holding the outermost e more tightly inc ionization energy 3. atoms with greater Zeff will pull more strongly on e in covalent bonds, inc electronegativity across a period 4. atoms with stronger Zeff will more readily accept another electron, so electron affinity inc across a period
electronegativity trend
tendency of an atom to attract electrons shared in a covalent bond -when two atoms have diff electronegativities, they share electrons unequally causing polarity -relative electronegativity determines the direction of polarity within a bond and within an overall molecule -inc across a period from left to right and up
electronegativity
most common used measurement for this is pauling scale, which ranges from a value of 0.79 Cesium to a value of 4 for fluorine -F most electronegativity element
electronegativity of H
-falls between that of boron and that of carbon -when bonded with H, carbon and elements to teh right of carbon will carry a partial negative charge while H will carry a partial positive -think Ch4, boron, and elements to the left of boron will carry a partial positive charge when bonded to hydrogen, while teh hydrogen will carry a partial negative charge. Think of the hydrides H- in NaH or LiAlH3
pauling scale for electronegativity large differences
- electronegativity values provide system for predicting which type of bond will form btw two atoms -atoms with large electronegativity 1.6 or larger* on Pauling scale as a rule of thumb, will form ionic bonds! -metals and nonmetals usually exhibit large electronegativity differences and form ionic bonds with each other
pauling scale for electronegativity moderate differences
-atoms with moderate differences in electronegativities (0.5-1.5 on Pauling scale) will generally form polar covalent bonds
pauling scale for electronegativity moderate differences
- atom with v minor electronegativity differences generally form nonpolar covalent bonds, 0.4 or smaller on pauling scale
Pauli Exclusion
that no two electrons in the same atom can have the same four quantum numbers
electron affinity
willingness of an atom to accept an additional electron -more precisely, it is the energy released when an electron is added to an isolated atom -inc on periodic table from left to right and from bottom to top -the sign of e affinity values can be different for different atoms because some atoms release energy when accepting an e, and thus become more stable while others require energy input to force the addition of an electron since the additional electron dec stability WARNING: e affinity is sometimes described in terms of exothermicity, for which the energy released is given a negative sign. We can state this as follows: electron affinity is more exothermic to the right and up on the periodic table. noble gases do not follow this trend. Electron affinity values for the noble gases are endothermic, because noble gases are stable. therefore, significant amounts fo energy are required to force them to take on electrons and become less stable
fluoride (size influence)
- small atoms hold charge in a concentrated way because they have fewer orbitals available to distribute and thereby stabilize charge - concentration of charge makes the smallest element in each group bond more readily and with greater bond strength, especially when in ionic form -Fluorine is a good ex, F- is too small to manage its full negative charge. Therefore it is generally insoluble and bonds immediately when in solution. For this reason, in toothpaste, fluoride a poison in high concentrations bonds immediately with the enamel of teeth before it can be ingested.
Aufbau principle
THINK GERMAN ORDER - “building up principle” - with each new proton added to create a new element, the new e added to maintain neutrality will occupy the lowest energy level available -everything being equal, lower energy state of a system should be the most stable in the system
electron configuration tricks
- make sure total number of e in your e configuration equals the total number of e in the atom -an e can momentarily absorb energy and jump to a higher energy level, creating an atom in an excited state versus ground state which is when electrons are all at their lowest energy levels (normal form from table)
electron configurations of transition metals
-not same as the nearest noble gas -ions are formed from losing e from the subshell with teh highest principle quantum number FIRST** -generally this is hte s subshell, it is also important to note that there are a few expectations to the electron configuration rules in the transition metals -Half-filled and filled subshells offer greater stability -elements in groups 6 and 11 are expected to have nearly half-filled or nearly filled d subshells, instead they borrow one e from the highest s subshell so they end up with a half filled s sub shell and a half-filled or filled d subshell -This phenomenon is most likely to appear on MCAT with Cr and Cu, which have only one e in the 4s orbital
Cu e configuration
-e configuration of Cr is [Ar] 4s^1 3d^5
Cr e configuration
-e configuration of Cu is [Ar] 4s^1 3d^10
Hund’s rule
e will not fill any orbital in the same subshell until all orbitals in that subshell contain at least one e, and that the unpaired e will have a parallel spins -remember like charges repel each other, if consider the energy of two particles with like charges, we would find that as the particles approach the mutual repulsion creates an inc in potential energy - this occurs when e approach each other so e avoid sharing an orbital when possible, spreading out amongst the orbitals of a given subshell to minimize PE
paramagnetic
- there are unpaired e so subshell is not completely filled
- spin of each unpaired e is parallel to the others, as a result electrons align with an external magnetic field
diamagnetic
-no unpaired e like He, so subshells are completely filled
- they are unresponsive to an external magnetic field
emission line spectrum
- when excited e falls from a higher energy state to a lower energy state, energy is released
- this energy creates this, that is characteristic of the given element
absorption line spectrum
-measures the radiation absorbed when e absorb energy to move to a higher energy state
photoelectric effect
- Einstein demonstrated one to one, photon to electron collision
- used one to one collision to prove that light is made up of particles
- light shining on a metal may cause the emission of electrons, sometimes called photoelectrons in the context of he photoelectric effect.
- Since the energy of a wave is proportional to its intensity, one might expect that when the intensity of lighting shinning on a metal is inc by inc the number of photons, the KE of an emitted electron would inc accordingly. But this is not the case, instead, the kinetic energy of the electrons increases only when intensity is inc by inc the frequency of each photon. if the frequency is less than the necessary quantum of e, no electrons at all will be emitted regardless of number of photons. This demonstrates that the electrons must be ejected by one ot one photon electron collision rather than by the combined energies of two or more photons.
work function
minimum amount of energy required to eject an electron is called work function, phi of the metal KE excess= Hf (energy in) - phi (electron out) hf is the energy put in by a photon, and phi is the energy required to eject the e from the atom -energy left over is the electron’s KE
hydrogen bond
-responsible for high bp of water -strongest type of intermolecular force, it is still much weaker than any covalent bond -strongest type of dipole-dipole interaction. H bond occurs btw a H that is covalently bonded to a F, O or N and N, F, or O atom from another molecule -F, O or N are HIGHLY electronegative, when bound to H a large dipole moment is formed, leaving H with a strong partial positive charge
intermolecular attractions
-attraction btw separate molecules, occur due to dipole moments -partial neg charge of one molecule is attracted to partial positive charge of another molecule -they are weak electrostatic bonds, generally about 1% as strong as covalent bonds. -Attraction btw two molecules is roughly proportional to the magnitude of their dipole moments the stronger the dipole, stronger the attraction ** these are usually insignificant in gases because the molecules are spread far apart, but these forces apply to solids and liquids hte same
london dispersion forces/ van der waals
-weakest dipole dipole force btw two instantaneous dipoles - these dipole dipole bonds are called London dispersion forces -all molecules exhibit London dispersion forces, even when they are capable of stronger intermolecular interactions
mega
M, 10^6
kilo
k, 10^3
deci
d, 10^-1
centi
c, 10^-2
milli
m, 10^-3
micro
u (weird u) 10^-6
nano
n, 10^-9
pico
p, 10^-12
femto
f, 10^-15
percent composition of mass
-multiply each element’s atomic weight by the number of atoms it contributes to the empirical formula -then divide the result by the net weight of all the atoms in the empirical formula, which yields the mass fraction of that element in the compound - multiply by 100% to get hte percent composition by mass ex. percent mass of carbon in glucose, empirical formula CH2O molecular weight of carbon/molecular weight of CH2O = 12/30= 0.4 0.4 X 100= 40 glucose is 40% carbon by mass
determine empirical formula ex
if we are asked to find the empirical formula of a compound that is 12.5% H, 37.5% C, 50% O by mass= from a 100 g sample= 12.5 g H/ 1 g/mol = 12 mol 12/3 = 4 37.5 g C/ 1 g/mol = 3 moles 3/3 = 1 50 g O/ 1 g/mol = 3 moles = 3/3 = 1 There is a 4:1 ratio of H to each of the other elements. Empirical formulas is H4CO
Aluminum
Al3+
Ammonium
NH4+
Barium
Ba2+
Calcium
Ca2+
Chromium II, Chromous
Cr2+
Chromium III, Chromic
Cr3+
Copper I, cuprous
Cu+
Copper II, cupric
Cu2+
Hydrogen, hydronium
H+, H3O+
Iron II, ferrous
Fe2+
Iron III, ferric
Fe3+
Lead
Pb2+
Lithium
Li+
Magnesium
Mg2+