Meijer Astrochem Flashcards
Why in space are collisions so few and far in-between?
Low densities and temp
How does the chemistry of space differ if close to sun or star or in the presence of interstellar radiation?
Near the sun and strata temp is high which may drive certain chemical reactions
Radiation could degrade molecules
True or false - the detection of Molecules in space is due to the stability of the molecules
False - the presence of other molecules may be due to the fact that they are precursors
What are the three elements of the Big Bang
Big Bang nucleosynthesis
Cosmic microwave background radiation
Inflation/expanding universe
What happens in the first 100 seconds of the Big Bang
All elementary forces equal. Universe is the length of plank. As time goes on, temp decreases and elementary forces separate. Quarks present and then protons and neutron interconvert and eventually protons dominate. At end of 100s neutron and protons combine to form deuterium.
Why does Big Bang nucleosynthesis stop
Temp too low and density is too low
Why is there cosmic background radiation
Temp is now low enough that there is decoupling
Electrons and nuclei combine to form neutral atoms.
Photons and matter decouple and no longer interact. Universe becomes transparent and photons fly uninterrupted through universe - cosmic background radiation
What distribution does cosmic background radiation give?
At decoupling Matter and radiation are in thermal equilibrium. Photon energy distribution gives a black body curve with a temp of 2.725
What does the BB distribution curve Suggest
If there was massive star formation it would perturb the curve. universe was initially hot but has been cooling down ever since
what is the doppler effect?
When electromagnetic waves moves towards the observer the transition shifted to smaller wavelengths - blue shifted
When electromagnetic waves move away from the observer, the transition is shifted to longer wavelengths - red shifted
how does the doppler effect support the big bang?
when the universe expands CMBR is detected at longer wavelenghts
what is the definition of black body radiation?
an object that emits and absorbs all wavelengths of radiation at equal efficiency
what are the other properties of black body radiation?
At T> 0 K, emits radiation at all wavelengths
As temperature increases object emits more light at all wavelengths
As temperature increases it emits more radiation at shorter wavelenghts
have a wavelength distribution
what is the stefan boltzman law
Relates the amount of energy emitted from a blackbody object to its temperaturea
what are the equations to calculate the parralax?
d = 1/ Theta Theta = Distance ? 1 parsec (3.26 ly or 3.08x10^16 m )
how is hubbles law related to the age of the universe?
V = H + d
t = d/V sub in first equation you get t = 1/V
How does the abundance and distribution of elements in space prove the big bang?
Most abundant is He and H - makes up most of the universe. It is all primordial.
Light elements made in big bang nucleosynthesis
what is the light source and the detector in astronomy?
The star is the light source and the telescope is the detector
what is the modified beer lambert law for spectroscopy for space?
I = Io e - (aplha * l )
alpha is the absorption peer parsec
what are the 5 different ways that matter interacts with photons?
Elastic and inelastic scattering
Spontaneous emission and adsorption
Stimulated emission
What is elastic scattering (rayleigh)
Atom interacts with photon and energy of photon is not changed
what is Inelastic scattering (raman)
Atom absorbs photon and photon is remitted at a different wavelength. Atom either absorbs photon energy or gives photon additional energy
What is stimulated emission?
atom is inn excited state and when a photon of right energy/wavelength passes. excited returns to ground state and emits photon of exact energy as incoming photon
are photons wisth shorter wavelenghts scattered more or less than photons with longer wavelengths?
They are scattered more