atomic structure review Flashcards
J Dalton
- All matter is made up of tiny particles called atoms. An atom cannot be created, destroyed, or divided into smaller particles (not true because the atom is made up of p,n and o).
- The atoms of one element cannot be converted into atoms of another element.
- All atoms of one element have the same properties, such as size and mass. These properties are different from the properties of other elements. (not true because we have isotopes which have diff masses but same element)
- Atoms of different elements combine in specific proportions to form compounds.
- Billiard ball model (dense and thick atom)
JJ Thompson
- Using cathode ray tubes it was demonstrated that the atom could be broken down into smaller particles.
- Negatively charged particles(electrons) could be ejected from atoms, leaving the atoms positively charged.
- raisin bun model (neg charge is rasins in a bun which is sphere of pos charge)
Ernest Rutherford
- Directed highly energetic, positively charged alpha particles at a very thin gold foil.
- The pattern produced by the alpha particles proved that there was a dense positive core, this core contained almost the entire mass of the atom.
- It was inferred that the electrons exist in orbit around the small nucleus of the atom.
- since it glowed everywhere it indicated that the pos charge is small in the middle (pos alpha particles deflected slightly when near nucleus, but deflected at large angle when hitting nucleus directly which was not the expected result of the test)
- behive model (the nucleus is the hive and e- are bees buzzing around)
N Bohr
- Analyzed the pattern and colours of light emitted from heated hydrogen atoms.
- Determined that the light being observed was being caused by electrons which were transitioning from a “higher orbit” to a “lower orbit”, thereby releasing energy.
- Developed a mathematical expression to calculate the radius of specific allowable energy levels where electrons can exist in orbit around the nucleus of the atom.
- excitation it takes in energy and deexcitation is gives off light or energy –> colours are diff because e- on specific levels will release diff colours based on where it moves down from
- planetary model (atom looks like the planetary system in which the nucleus is the sun and the e- are like planets orbiting)
Subatomic structure: the average atom is 10^-10 m in diameter but the atoms are made up of many smaller subatomic particles (p and n have relative mass of 1 while e- has 1/1840)
Electromagnetic radiation
James Clerk Maxwell in 1856 proposed the existence of waves which were related to both electricity and magnetism and called them electromagnetic waves. (Electromagnetic wave has an electric and magnetic field component. Both have same wavelength and frequency.)
on the spectrum it goes from low freq and long wavelength to high freq and short wave length –> wavelength and freq occur together –> c which is speed of light = 3.00x10^8m/s –> c=wavlength * f –> f(sec-1) = c/wl –> wl= c/f
Some waves require a medium to travel through. for example water waves and sound waves.
in a vacuum no sound waves will be heard.
ELECTROMAGNETIC WAVES, requires no medium of transmission. Waves will travel in a vacuum
max Planck
- Founder of the quantum theory
- Proposed that radiation is emitted in discreet packets called quanta (singular quantum)
- Energies associated with these quanta are proportional to the frequencies of the emitted radiation.
- He formulated the following equation: E (J) = hf
Where E is the energy of radiation, h is Planck’s constant (6.626 x 10^-34 Js) and f is the frequency of the radiation. - another equation could be E= hc/wavelength –> so e is indirectly proportional to wl (as one increases the other decreases)
Radiation emitted by heating solids to various temperatures. The energy emitted by atoms or molecules is always in whole number multiples of energy of certain well-defined quantities. The word Quanta or Quantum refers to the smallest quantity of energy that can be emitted or absorbed in the form of electromagnetic radiation. E=hν, where h is Planck’s constant = 6.63 x 10-34 Js
Einstein
- Theory of relativity
- Theory of the photoelectric effect – Noble prize in 1921
- Einstein viewed electromagnetic radiation as beams of photons
- each photon is a little packet of energy with the value E = h f.
- Frequency is equal to the speed of light divided by the wavelength of the radiation in question and thus this equation can be rearranged to read:
E = h c
λ
Note: The theories of Planck and Einstein were the first steps in the development of the quantum theory. - he basically was saying that waves are particle like
Proposed theory to explain the photoelectric effect. Einstein’s theory of light states that a beam of light behaves as a stream of particles rather than wavelike. He called the stream of particles PHOTONS. Later it was proposed that light behaves as either as waves or particles. This property is also a characteristic of all matter.
DeBroglie
- French physicist
- Received the Nobel Prize in physics in 1929
- Louis de Broglie proposed the wave-particle duality of light. This simply put, is the phenomenon that waves behave both like a particle and as a wave (everything has wave like properties but smaller stuff has more)
De Broglie proposed that both light and matter obey the equation:
λ = h / m v
Where: λ is the de Broglie wavelength, m is the mass, v is velocity, h is Planck’s constant
If waves can behave like a stream of particles (photons) then so can an electron possess wave like properties. A particle in motion can be treated as a wave and vise versa.
back to bohr
- Danish physicist
- First quantum model of the atom
- Formulated a description of the hydrogen atom that explained its light spectra
- Using Einstein’s work and Planck’s work – Bohr related the colour of hydrogen’s spectra to wavelength
- Wavelength to energy
- Bohr postulated that the colours of the Hydrogen spectra were discreet bands of colour.
- Bands generated by de-excitation of electrons from higher energy levels to lower or ground state, while emitting a photon of light
- Bohr showed that electrons are quantized (have specific values).
- He demonstrated that the only possible energies of electrons in his orbital/energy levels would be given by the equation:
En = - 1311 KJ/mol n^2
The En values corresponds to the energy states of electrons in a hydrogen atom.
Hydrogen spectrum of light:
- When an electron makes a transition from a (excited state) higher energy state to a lower (ground state) energy state, it is accompanied by the emission of a photon having a wavelength that corresponds with the electromagnetic spectrum.
- When electrons are excited in a gas sample or element, radiation is emitted at discreet wavelengths.
- This is called a line spectrum.
- If we are examining a gas consisting of individual atoms then we call the spectra atomic emission spectra.
J Balmer
- an amateur Swiss scientist
- developed a mathematical relationship that could explain and predict the visible spectrum of hydrogen.
- Johannes Rydberg – a Swedish physicist - using the work of Balmer developed an equation that related all the wavelengths of lines produced in the electromagnetic spectrum of Hydrogen. The equation is as follows:
1/wl = Rh (1/n1^2 - 1/n2^2)
RH (Rydberg constant): 1.097 x 107
n1 or nf: is the series type (final energy level)
n2 or ni: is the energy level the electron is transitioning from (initial energy level)
The hydrogen electron has a variety of transitions from different energy levels. The line spectra that we see is only in visible range. However, there are transitions that occur in ultra violet and infrared region of the spectrum.
- electron absorbing photon goes up energy level, electron emitting photon goes down energy level
- going the n = 1 is uv light (layman series, going to n=2 is visible spectra (balmer series), going to n=3,4 is infared light (paschen series, brackett series)
- the closer to the nucleus, the more negative you are, there are infinity n
Spectroscopy
- A continuous spectrum is produced when white light is passed through a prism. The result is line a rainbow, where ROYGBIV can be seen.
Absorption Spectra:
In order to excite an electron a
certain amount of energy is required (at a particular wavelength) corresponding to the differences between the energy levels. For example, an object that absorbs blue, green and yellow light will appear red when viewed under white light.
Emission Line Spectra:
This is the opposite of absorption line spectra. The energy released when an electron falls back down to the ground state (at a particular wavelength) corresponding to the difference between
the energy levels.
Uses: to identify elements present in a gas or liquid, for example elements in stars and other gaseous objects which cannot be measured directly.
Bohr and imrpovment of atomic model
- The number of electrons at each principle energy level became known
- # electrons = 2n^2 where n is the principle energy level
- evidence/reasoning ascertained from the intensity of the spectral lines of hydrogen.
- Electrons must be located in levels of specific and fixed energies (orbits).
En = - 1311 KJ/mol n^2 Evidence/Reasoning – given that hydrogen gave off four very distinct bands of colour, where the photons must have discreet amounts of energy, since this energy was released when excited electrons dropped from higher energy to lower energy, the electrons must have specific energy levels at which they must exist and not in between.
limitations:
- The electron is a particle whose position and motion can be specified at a given time.
- An electron moves in an orbit having a fixed radius.
- Bohr’s experimental evidence only agrees with an one-electron atom (Hydrogen)
… in addition to this, electrons behave as particles in some experiments while in other experiments they behave as WAVES
(Atomic structure was analogues to planetary system. Studied line spectra of hydrogen in gas phase. Line spectra due to the excitation of electrons from lower energy level to a higher one. When the electron falls to a lower energy level or ground state it emits a specific amount of energy. The line spectra are not restricted to the visible range but also extend into the UV and IR range. The energies associated with electron motion in permitted orbits are fixed in value. Therefore energies are QUANTIZED)
E Shrodinger
- Developed a mathematical expression called the “Schrodinger Wave Equation”, which when solved, predict the CHANCE or probability of an electron showing up in a particular region of space (3-D) around the nucleus.
- this calculated region of space is called an Orbital. E
- Orbitals are where electrons are confined to specific regions, which are represented as electron clouds.
In order to describe the motion of an electron in an atom, both the electron’s wave and particle nature must be taken into account.
HEISENBERG UNCERTAINTY PRINCIPLE states that due to the dual nature of the electron it is impossible to determine both its position and energy at the same time.
Probability model of the atom
- In this model, the probable location of an electron moving about the nucleus can be identified, but not its exact location. The general location or ‘region of space’ within which the electron can be found is called an orbital. No longer will the electron be thought of as travelling in a defined path called an orbit.
- The shape of the orbital or region of space will be defined by an array of dots where each dot represents a possible location of the electron. The more intense the dots the greater the probability of finding an electron at that position. The diagram above results from a computer program that has determined the possible positions of a hydrogen atom’s single electron.
- The maximum capacity of any orbital is TWO electrons, each having opposite spin. Since electrons are negatively charged, their rotation produces a magnetic field. Therefore, opposite rotation produces unlike/opp magnetic field which in turn produces the attraction to allow the two electrons to exist in the same orbital.
Types of orbitals
- S orbital: this is a spherical shaped region of space –> only one orietntion in space –> max capacity of 2 e
- p orbital: dumbell shaped region of space, 3 orientations, so full set has a max capacity of 6 e
- d orbital: complex shapes-4 lobes mostly, 5 orientations so full set has capacity of 10 e
- f orbital: complex shapes, 7 orientations so full set has capacity of 14 e
When scientists studied multi-electron systems (elements other than hydrogen), they discovered that there were more levels (more frequencies) visible. The basis for these sublevels/orbitals is due to studies of spectra of different elements that indicated that each shell or energy level consists of one or more orbitals/sublevels grouped closely together.
n = 1, s = 2e
n = 2, s =2e and p= 6 e
n = 3, s = 2e, p= 6e and d = 10e
n = 4, s=2e, p=6e, d= 10e and f = 14e
orbital energy/tables are drawn in increasing energy going up, have to spread out arrows before doubling
electron configurations: Electron arrangements can be made more specific than the Bohr-Rutherford model has to date. This model is based on the quantum mechanical model. It specifies the level the electrons are on and is referred to as electron configurations. As with the Bohr model though, electrons always fill the lowest energy state before proceeding to a higher energy state, regardless of the actual being occupied. Follow the pattern on the right for the order of filling up the sublevels.
ex. 1s^2 2s^2 2p^6 for neon where first number is energy level then orbital type and then number of e there
AUFBAU PRINCIPLE – electrons go into the lowest energy level and fill them in order of increasing energy.
PAULI EXCLUSION PRINCIPLE – an orbital can hold a maximum of two electrons. But an orbital can be empty or have one electron. (0,1,2)
HUND’S RULE – electrons in the same sublevel or orbitals will not pair up until all the orbitals of the sublevel are at least half-filled.
ELECTRONIC CONFIGURATION – distribution of electrons among the various orbitals.