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gladu [14]
4 years ago
7

What is the wavelength of the matter wave associated with a proton moving at 377377 m/s? wavelength of proton matter wave: mm Wh

at is the wavelength of the matter wave associated with a 159159 kg astronaut (including her spacesuit) moving at the same speed? wavelength of astronaut matter wave: mm What is the wavelength of the matter wave associated with Earth moving along its orbit around the Sun? wavelength of Earth matter wave: m
Physics
1 answer:
Alinara [238K]4 years ago
0 0

1) 1.05\cdot 10^{-9} m

The wavelength of the matter wave (also called de Broglie wavelength) of an object is given by

\lambda=\frac{h}{mv}

where

h=6.63\cdot 10^{-34} Js is the Planck constant

m is the mass of the object

v is its velocity

For a proton, we have:

m=1.67\cdot 10^{-27} kg

and the velocity of this proton is

v=377 m/s

So, its de Broglie's wavelength is:

\lambda=\frac{6.63\cdot 10^{-34}}{(1.67\cdot 10^{-27})(377)}=1.05\cdot 10^{-9} m

2) 1.11\cdot 10^{-38} m

We can use again the same equation:

\lambda=\frac{h}{mv}

where in this case we have:

m = 159 kg is the mass of the astronaut + spacesuit

v = 377 m/s is the velocity of the astronaut

Substituting into the equation,

\lambda=\frac{6.63\cdot 10^{-34}}{(159)(377)}=1.11\cdot 10^{-38} m

3) 3.70\cdot 10^{-63} m

Similarly, we can use the same equation:

\lambda=\frac{h}{mv}

where in this case we have:m=5.98\cdot 10^{24}kg is the Earth's mass

v=30 km/s = 30000 m/s is the velocity of the Earth around the Sun

Substituting,

\lambda=\frac{6.63\cdot 10^{-34}}{(5.98\cdot 10^{24})(30000)}=3.70\cdot 10^{-63} m

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By calculating its wavelength (in nm), show that the second line in the Lyman series is UV radiation.
Rashid [163]

Answer:

 λ = 102.78  nm

This radiation is in the UV range,

Explanation:

Bohr's atomic model for the hydrogen atom states that the energy is

           E = - 13.606 / n²

where 13.606 eV   is the ground state energy and n is an integer

an atom transition is the jump of an electron from an initial state to a final state of lesser emergy

            ΔE = 13.606 (1 / n_{f}^{2} - 1 / n_{i}^{2})

the so-called Lyman series occurs when the final state nf = 1, so the second line occurs when ni = 3, let's calculate the energy of the emitted photon

            DE = 13.606 (1/1 - 1/3²)

            DE = 12.094 eV

let's reduce the energy to the SI system

            DE = 12.094 eV (1.6 10⁻¹⁹ J / 1 ev) = 10.35 10⁻¹⁹ J

let's find the wavelength is this energy, let's use Planck's equation to find the frequency

            E = h f

             f = E / h

            f = 19.35 10⁻¹⁹ / 6.63 10⁻³⁴

            f = 2.9186 10¹⁵ Hz

now we can look up the wavelength

           c = λ f

           λ = c / f

           λ = 3 10⁸ / 2.9186 10¹⁵

           λ = 1.0278  10⁻⁷ m

let's reduce to nm

            λ = 102.78  nm

This radiation is in the UV range, which occurs for wavelengths less than 400 nm.

5 0
3 years ago
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