play phryzby with physics

The Earth's Quantum Number

solved BohrModel

Q. In accordance with the Bohr's model, what is the quantum number that characterises the earth's revolution around the sun in an orbit of radius 1.5 × 10¹¹ mr=1.5×1011m with orbital speed 3 × 10⁴ m/sv=3×104m/s? (Mass of earth = 6.0 × 10²⁴ kgm=6.0×1024kg.)

−earth, n = ?r = 1.5×10¹¹ mv = 30000 m/sn = 1n = 2m = 6×10²⁴ kg
Inputs
r
150000000000.00 m
v
30000.0 m/s
m
6e+24 kg
Outputs
numbern?

How it's solved

Solved with BohrModel

Given

  • r=1.5×1011m
  • v=3×104m/s
  • m=6.0×1024kg

Find n.

Working
  1. angular momentum comes in steps(earth)m⋅v⋅r=n⋅h2⋅π
  2. 6×1024⋅30000⋅1.5×1011=n⋅6.62607015×10−342⋅3.14159265
  3. n=2.56028082×1074
  4. n≈2.6×1074to 2 significant figures
Conclusion

Angular momentum comes in steps of Planck's constant over two pi, but the earth's is so vast that the steps are far too fine to notice: quantum rules fade into classical ones at large sizes.

The web of concepts

given read from the words equation asked

The Ruby that solves it

The question and its solution are small Ruby files. The engine runs them.

question.rb
1require_relative "../physics"23question :the_earth_s_quantum_number do4  kind :numerical5  describes "In accordance with the Bohr's model, %{number} that characterises the earth's revolution around the " \6            "sun in an orbit of radius %{radius} with orbital speed %{speed}? (Mass of earth = %{mass}.)"7  given radius: "1.5e11 m"8  given speed: "3e4 m/s"9  given mass: "6.0e24 kg"10  asks number: "what is the quantum number"11end
solution.rb
1require_relative "../questions/the_earth_s_quantum_number"2require_relative "../science/atoms/bohr_model"34solve :the_earth_s_quantum_number, using: BohrModel do5  objects :earth67  take radius: earth.orbit_radius8  take speed: earth.orbital_speed9  take mass: earth.mass1011  number = earth.quantum_number12  answer number:, figures: 21314  conclusion "Angular momentum comes in steps of Planck's constant over two pi, but the earth's is so vast that the " \15             "steps are far too fine to notice: quantum rules fade into classical ones at large sizes."16end
playground.rb
1require_relative "../solutions/the_earth_s_quantum_number"23play_with :the_earth_s_quantum_number do4  title "The Earth's Quantum Number"5end
The laws it drew on
quantitywrittenunitswithinfrom
piπ—0 … ∞BohrModel
coulomb constantkN m² C⁻²—BohrModel
elementary chargeeC—BohrModel
plancks constanthJ s—BohrModel
massmkg0 … ∞BohrModel
orbit radiusrm—BohrModel
orbital speedvm/s0 … ∞BohrModel
binding energyEbJ—BohrModel
quantum numbern——BohrModel
atomic numberZ——BohrModel
potential energyUJ—BohrModel
total energyEJ—BohrModel
photon energyEpJ—BohrModel
frequencyνHz0 … ∞BohrModel
binding energy of groundEb,gJ—
orbit radius of groundrgm—
binding energy of earthEbJ—
orbit radius of earthrm—
mass of groundmgkg0 … ∞
orbital speed of groundvgm/s0 … ∞
mass of earthmkg0 … ∞
orbital speed of earthvm/s0 … ∞
atomic number of groundZg——
quantum number of groundng——
atomic number of earthZ——
quantum number of earthn——
potential energy of groundUgJ—
potential energy of earthUJ—
total energy of groundEgJ—
total energy of earthEJ—
photon energy of groundEp,gJ—
frequency of groundνgHz0 … ∞
photon energy of earthEpJ—
frequency of earthνHz0 … ∞
Eb,e=k⋅e22⋅re
energy to free the electron
me⋅ve2re=k⋅e2re2
held in orbit by the proton
ve=2⋅π⋅k⋅Ze⋅e2ne⋅h
speed set by the level
me⋅ve⋅re=ne⋅h2⋅π
angular momentum comes in steps
Ue=−k⋅e2re
energy of its place
Ee=−k⋅e22⋅re
energy of the atom
Ep,l=h⋅νl
one photon for one jump
Eb,g=k⋅e22⋅rg
energy to free the electron(ground)
Eb=k⋅e22⋅r
energy to free the electron(earth)
mg⋅vg2rg=k⋅e2rg2
held in orbit by the proton(ground)
m⋅v2r=k⋅e2r2
held in orbit by the proton(earth)
vg=2⋅π⋅k⋅Zg⋅e2ng⋅h
speed set by the level(ground)
v=2⋅π⋅k⋅Z⋅e2n⋅h
speed set by the level(earth)
mg⋅vg⋅rg=ng⋅h2⋅π
angular momentum comes in steps(ground)
m⋅v⋅r=n⋅h2⋅π
angular momentum comes in steps(earth)
Ug=−k⋅e2rg
energy of its place(ground)
U=−k⋅e2r
energy of its place(earth)
Eg=−k⋅e22⋅rg
energy of the atom(ground)
E=−k⋅e22⋅r
energy of the atom(earth)
Ep,g=h⋅νg
one photon for one jump(ground)
Ep=h⋅ν
one photon for one jump(earth)