chads ch1
AP Chemistry None with None at Syracuse University
About this deck
By: Gerri Blick
Created: 2011-05-21
Size: 42 flashcards
Views: 27
Created: 2011-05-21
Size: 42 flashcards
Views: 27
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energy of electrons in further vs. closer orbitals
the further from the nucleus the higher the energy, closer to the nucleus the energy goes down--electrons closer to the nucleus have less energy because thats where they want to be since electrons are negative and overall charge of nucleus is positive due to protons.
mass number
designates a specific isotope
protons + neutrons
235 U-- the upper number
atomic number
defines what element we are talking about
tells the number of protons
92U-the lower number
what happens if you change the number of electrons in an atom
gives the atom a charge and makes it an ion
what happens if you change the neutrons in an atom
makes it a different isotope of that same atom and gives it a different mass number
what happens if you change the protons of an atom
makes it a different element
basics of periodic table
columb=group-up and down
row=period -left ot right
noble gas=inert-no chemical reactions involved
alkali metal (group 1)-basic, highly reactive in water and as you go down they become more reactive
alkaline earth metal (group 2)-create basic solutions but less reactive than group 1
transition metals-take on various charges
halogens-group 7-have 7 valence electrons want to pick up one more.
how many electrons are held in each shell?
2n2
degenerate
when orbitals are equal in energy
ex: p orbital has 3 degenerate orbitals
how can you get a more stable shell?
half filled subshells and completely filled subshells are more stable than 1 away from being full.
electron configuration of Cu
EXCEPTION!
Cu would think to be [Ar]4s23d9
but its actualy [ar] 4s13d10
ag and au and rg also follow this exception.
electron configuration for Cr and Mo
Exceptions!
Cr: [Ar] 4s13d5
Mo: [Kr] 5s14d5
this is NOT an exception for W and Sg
electron configuration for Cu2+
move from highest shell number first, so 4 before 3.
Cu2+: [Ar] 4s03d9
another example: Ni2+
[Ar] 3d8
valence electrons of transition metals
if d is full, it doesnt count and look at the other subshells, but if the d isnt full, then it counts.
paramagnetic
an element can be deflected by a magnetic field
there is an unpaired electron
always paramagnetic if there is an odd number
the more unpaired electrons you have, the more paramagnetic you are
diamagnetic
wont get deflected by a magnetic field
all electrons are paired up
ex:Na+
heisenberg uncertainty principle
its impossible to determine, with perfect accuracy, the momentum and the position of an electron simultatneously, this means
pauly exclusion principle
no two electrons in an atom can have the same four quantum numbers
quantum numbers
an electrons address
an atoms absorption spectrum
each atom has a specific absortion spectrum, measures the amount of energy, in the form of photons of light, and thus a change in wavelength was absorbed by the sample
every atom has its own wavelength at which it will absorb energy due to the unique configuration of the electrons in the outer shell.
endothermic when it absorbs energy and electron goes to a higher orbitial
exothermic when the electron releases energy, or emits a photon
E=hc/λ
h=planks constant, 6.626x10-34
c=light, 3x108
λ=wavelength
einsteins equation-nuclear energy
E=Δmc2
E=energy; Δm=mass; c=speed of light=3x108
in the nuclear reaction, mass is converted into energy-al nuclear reactions convert mass into energy. little mass turns into ALOT of energy.
in nuclear reactions, products will therefore way less than reactants cuz mass has been converted into energy, and they are therefore exothermic.
strong force
protons hate eachother and dont want to be close, so they repel.
they stay in the nucleus becuase there is an attractive force in nucleus called the strong force which overcomes the electrostatic replsion between protons
strong force comes from the nuclear binding energy
nuclear binding energy
protons and neutrons seperately weigh more than when they are put together in the nucleus--they sacrafice some mass and convert to energy so they can hold protons and neutrons in the nucleus. the mass thats converted into energy is the neclear binding energy.
stable nucleus-hgih nuclear binding energy
unstable/radioactive=lower nuclear binding energy
alpha particle
24α-2 protons and mass number of 4-2 neutrons
equivalent of helium nucleus, but not same as helium atom because it doesn't have electrons.
proton
11p -has one proton and mass number of one
nuetron
no charge, but a mass number of 1, less than a proton
10n
beta partice
an electron, has -1 charge, and mass number is 0, but it really does have a tiny mass its just rounded
0-1β
positron
positively charged electron and can be emitted out of a nucleus.
0+1β
gamma
its a photon of light, and it actually does have a 0 mass.
00ϒ
penetrating power
as mass decreases, penetrating power increases--gamma is most penetrating and will do the most harm, alpha will do the least harm
stable nucleus
1. even number of protons and or neutrons-if odd number of protons and nuetrons, you are probably radioactive-better if neutrons and protons are paired up.nitrogen-14 is exception
2. n/z ratio-want it as close to 1 for lighter elements, after you pass 20, want more neutrons, so higher than 1.-want atom to lie close to belt of stability
n-neutrons; z=protons
3. magic numbers-2, 10, 18 electrons-noble gases with filled shells
nuclear reaction
can invert one element into another element
parent nucleus=reactant
daughter nucleus-product
alpha decay
42 α as product-put on right hand side of equation
whenever you emit something its a product of that reaction
reduces mass number
every element greater than 83, palonium and higher are radioactive. z>83
β-decay
0-1β
always talking about electron emission, shows up on product side
proton+electron=neutral, mass number=1
when you combine proton and electron, you get a neutron
turns a neutron into a proton by taking out an electron
if you are above belt of stability, n/z ratio is high so you want more protons, so you go thorugh beta decay
electron capture
when inner core electron is sucked into the nucleus
electron is on reactant side of arrow 0-1e
turns a proton into a neutron
have proton in nucleus and sucks in a electron, it makes a neutron by capturing the electron-capture negative electron
if below belt, n/z is too low so there are too many proton and not enough neutrons, so want to turn protons into neutrons by electron capture
positron emission
0+1β
turns proton into a nuetron
gives off a positive electron to make a neutron.
if below belt, n/z is too low so there are too many proton and not enough neutrons, so want to turn protons into neutrons by positron emission
gamma emission
usually accompanies another nuclear process
have nuclear reaction and product nucleus isnt that stable yet so you it emits some high energy light and it gets more stable.
same parents and daughter
About this deck
By: Gerri Blick
Created: 2011-05-21
Size: 42 flashcards
Views: 27
Created: 2011-05-21
Size: 42 flashcards
Views: 27
About StudyBlue
STUDYBLUE makes things that make you better at school.
Things like online flashcards with photos and audio.
Things like personalized quizzes and friendly reminders about when (and what) to study next.
Think of it as a digital backpack™: access to all of your study materials online and on your phone.
STUDYBLUE exists to make studying efficient and effective for every student, for free. Join us.
“I have used this website for three exams, and I see a huge difference in my test results.”
Naj
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