Atomic structure ibdp Flashcards
ᴬ X
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A= total number of protons and neutrons(mass number) Z= proton number (A-Z)= number of neutrons
Isoelectronic?
Atoms/ions hv the same no. of e
Isotonic?
Atoms/Ions tht hv the same no. of neutrons
Isotopes properties
same chemical properties, diff physical properties, hv diff nucleon no., relative isotopic masses & no. of neutrons
heavier neutron
isotope w more neutrons
why are isotopes of some elements radioactive?
nuclei of these atoms r unstable & breakdown spontaneously, when they break down, they emit radiation which may be alpha particles, beta particles and gamma rays
uses of isotopes
- biochemical tracers in nuclear medicine for diagnostics, treatment and research
- used as “chemical clocks” in geological and archaeological dating
- In nuclear medicine, PET(position emission tomography) scanners give 3D images of tracer conc in the body & r used to detect cancers
What is the relative atomic mass of an element (Ar)? + instrument used to calculate it
its the weighted average atomic mass of its naturally occurring isotopes, modern mass spectrometer is used to determine the relative atomic mass of an element from its isotopic composition Each peak in the mass spectrum
indicates an isotope of the element and m/z values can be used to identify the isotopes. The height of the peak in the mass spectrum indicates the relative abundance of the isotopes.
Mass spectrometer in detail:
Mass spectrometry is an analytical technique which allows the determination of relative isotopic masses, relative molecular masses and structural features of organic compound as well as identification of unknown compounds, e.g. in forensic science. It allows chemists to weigh atoms & molecules by measuring how ions formed from them are accelerated or deflected by electric and sometimes magnetic fields
Mass spectrometer steps
- Vaporisation
- ionisation
- acceleration
- deflection–> if it has no charge it cannot b deflected and detected
- Detection
Electromagnetic spectrum
The arrangement of all the electromagnetic radiations in the increasing order of their wavelengths or decreasing order of their frequencies, rmivuxg, energy is inversely proportional to wavelength, and is directly proportinal to frequency
c=
lv
E=
hc/l
hv
According to Bohr’s model
the energy of the electron in an atom is quantized–> quantity cannot vary continuously to have any arbitary value but can change only discontinously to have specific or discrete values
lowest energy state
ground state, n=1, electrons r closest to nucleus
hydrogen emission spectrum
an experiment tht can be conducted to give evidence of electron exhibiting discrete/different energy levels, its a line spectrum n the lines in the spectrum correspond to the photons of a particular wavelength(frequency). for each element, the emission spectrum is a characteristic and unique to the element & it can be used to identify the element, thus it provides crucial evidence for the existence of electrons in discrete energy levels which converges at higher energies/frequencies
What is a electronic transition
The electron in the hydrogen atom may absorb energy and undergo an electronic transition to higher energy levels, e at higher energy level said to be in an excited state. When the electron returns to a lower energy lvl, energy is emitted in the form of light/photon
orbitals having equal energy r termed
degenerate
when is an electron in an atom stable
when the total attractive interactions are greater than the total repulsive interactions, most stable–. lowest orbital bcos thy r the closest to the nucleus and hence experience the strongest attractive force to the nucleus
s orbitals
spherical in shape and thy r non-directional, for eveery quantam shell, only one s orbital and the size of the s orbital increases w the principal quantam shell
p orbitals
dumb-bell shaped and they are directional, the 3 p orbitals hv diff directions in space, size also increases.w principal quantam shell
aufbau principle
electrons r added progessively to the orbitals starting w the lowest energy, 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p, 7s etc
exception: Cr and Cu bcos of syymetrical arrangement (thrs extra-stability in half-filled and fully-filled electronic configs)
Pauli exclusion principle
Each orbital can hold a max of 2 es, paired es can only b stable when they spin in opp dorections so tht the magnetic attraction which results from their opp spins counterbalances the electrical repulsion
Hund’s rule
When filling a sub-level, each orbital must b occupied singly b4 thy r occupied in pairs, can only pairup when each sublevel is alrdy half-filled