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Why can stellar parallax only be used on stars less than 100pc away
The further the star, the smaller the angle. You’d need the eyes of a microscope to see that small of an angle
1 Au = x m?
1.46Ă—1011
1 ly = x m?
9.46Ă—1015
1 ly = x AU?
63240
1 pc = x m?
3.086Ă—1016
1 pc = x ly?
3.26
1 pc = x AU?
206265
What is the process of hydrostatic equilibrium
Maintaining the balance between gravitational forces of the mass of the star with the outward pressure (thermal energy and radiation pressure) produced by nuclear fusion in the core.
Through what process do stars not collapse
Hydrostatic equilibrium
What do main sequence stars fuse
hydrogen (Deuterium H-2 and Tritium H-3) into helium in their cores.
What do you have to multiply mass defect by in order to find binding energy?
931.5
What unit is binding energy in
MeV(Mega electronvolts)
What is the main sequence star’s fusion process called?
p-p Chain (heh), or proton proton chain (boring name)
What makes 2H (deuterium)
Hydrogen and Hydrogen
What makes Helium-3
Deuterium and Hydrogen
What do you get when two helium-3 atoms fuse together
You get helium-4 and two protons. (or 2 hydrogen nulceus/atoms)
what is the electric force
230N
What are the conditions of fusion
Nuclei must be moving very fast
Enough speed to overcome the 230N of force pushing atoms away from each other
Nuclei must be very packed together, dense
Where there are more nuclei to be found, there is a higher chance of reaction
What do P-P chains combine
Protons, Hydrogens, and Heliums
What do CNO Cycles combine
Hydrogen + Big stuff (Carbon, Nitrogen, and Oxygen)
How do stars off the main sequence generate energy
No more Hydrogen, so they will use helium and anything they can find (heavier elements)
What is the fusing of larger nuclei called
Nucleosynthesis
What is the limit of fusion
Cannot go beyond Fe, it is at the peak
How would you fission Fe
Bombard its nucleus with neutrons
How are super heavy elements made
Big boom of the void (supernovas & dying stars)
What is luminosity
The power output of a star in Watts
What is luminosity directly dependent on
size and temperature
What is the formula for Luminosity
L=sigmaĂ—SAĂ—T4 (SA Is surface area!)
What is sigma for luminosity
5.67Ă—10-8Wm-2K-4
What is the area of a sphere
4pir²
Do bigger or smaller stars use more fuel
Bigger, duh
What is directly related to the lifespan of a star
mass. in fact M/L = amount of fuel (mass) / Rate of burning fuel (L)
What type of stars are brighter than usual
big ones
What is the inverse square law
Certain physical quantities decrease with the square of the distance from a source
What does L mean in the inverse square law
Luminosity of source (watts)
what is d in the inverse square law
distance from source
What is 4pid² in the inverse square law
SArea of sphere, d is radius tho
what can I be supplemented with in the inverse square law
b, the apparent brightness
What prevents a black body from infinitely retaining heat
emitted radiation
what happens to peak wavelength as something trends towards HOT
blu
What are the two ways a star can increase its luminosity
Be very hot
Be very large
(reminds me of someones… mom)
What kind of star is formed by matter slowly condensing through gravity until Jean’s Mass Criterion is reached
Proto Star
What is Jean’s Mass Criterion
The critical mass at which a gas cloud in space collapses on itself, starting the life cycle of a star
What are remnants of supergiants
Neutron Stars
How dense are neutron stars
very
What are remnants of red giants
White dwarfs
How Dense are white dwarfs
very
How hot are white dwarfs
very
what do neutron stars remind me of
your mom
what is the escape speed of a blackhole
more than the speed of light