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kodGreya [7K]
3 years ago
11

When light shines through atomic hydrogen gas, it is seen that the gas absorbs light readily at a wavelength of 91.63 nm. What i

s the value of the principal quantum number n of the level to which the hydrogen is being excited by the absorption of light of this wavelength? Assume that the most of the atoms in the gas are in the lowest level. (A) 14 (B) 16 (C) 11 (D) 21
Physics
1 answer:
Artist 52 [7]3 years ago
4 0

Answer:

D) 21

Explanation:

When gas absorbs light , electron at lower level jumps to higher level .

and the difference of energy of orbital is equal to energy of radiation absorbed.

Here energy absorbed is equivalent to wavelength of 91.63 nm

In terms of its energy in eV , its energy content is eual to

1243.5 / 91.63 = 13.57 eV. This represents the difference the energy of orbit .

Electron is lying in lowest or first level ie n = 1.

Energy of first level

= - 13.6 / 1² = - 13.6 eV.

Energy of n th level = - 13.6 / n². Let in this level electron has been excited

Difference of energy

= 13.6 - 13.6 / n² = 13.57 ( energy of absorbed radiation)

13.6 / n² = 13.6 - 13.57 = .03

n² = 13.6 / .03 = 453

n = 21 ( approx )

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OlgaM077 [116]

Answer:

the speed is 0.53 10⁸ m / s

Explanation:

As say in the exercise, the Doppler effect must be applied, in this case because it is an electromagnetic radiation with speed 3 10⁸ m/s and nothing can go faster we must use the relativistic Doppler effect

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Where fo is the observed frequency, fe the emitted frequency, c the speed of light and v the relative speed of the observer and emit, it is positive move away

The light fulfills the relationship

        c = λ f

        f = c / λ

In this case v is negative since the source and the observer approach

Substituting in the equation

         c /λo = c /λe √[ (c + v) / (c-v)]

         λo = 510 10⁻⁹ m

         λe = 610 10⁻⁹ m

We calculate the speed

        (λe/λo)² = (c + v) / (c-v)

       (λe /λo)² (c-v) = c + v

       v +(λe /λo)² v = (λe /λo)² c -c

       v [1 +(λe /λo)²] = c [(λe /λo)²-1]

       v = c [(λe /λo)² -1] / [1 +(λe /λo)²]

       v = 3 10⁸ [(610/510)² -1] / [1+ (610/510)²]

       v = 3 10⁸ [1.43-1] / [1 + 1.43]

       v = 0.53 10⁸ m / s

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8 0
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Yuliya22 [10]

Answer:

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Some examples of the planet are Mars, Venus, Earth, Mercury, Neptune, Jupiter, Saturn, Uranus, Pluto, etc.

Basically, the planets are divided into two (2) main categories and these includes;

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II. Outer planets: these planets are beyond the asteroid belt and comprises of jupiter, saturn, uranus and neptune, from left to right of the solar system.

These outer planets are made mostly of gases (hydrogen and helium) causing them to be less dense than the solid inner planets. These gases are generally known to be less dense in terms of physical properties.

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tresset_1 [31]

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Had to look for the options and here is my answer.
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