Q.

Hydrogen is the simplest atom of nature. There is one proton in its nucleus and an electron moves around the nucleus in a circular orbit. According to Niels Bohr, this electron moves in a stationary orbit, it emits no electromagnetic radiation. The angular momentum of the electron is quantized, i.e.,  mvr=(nh/2π), where m=mass of the electron, v = velocity of the electron in the orbit, r = radius of the orbit, and n=1,2,3...when transition takes place from  Kth  orbit to  Jth orbit, energy photon is emitted. If the wave length of the emitted photon is  λ, we find that  1λ=R[1J21K2], where R is Rydberg's constant.

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On a different planet, the hydrogen atom's structure was somewhat different from ours. There the angular momentum of electron was  P=2n(h/2π), i.e. an even multiple of (h/2π).

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a

In our world, the ionization potential energy of a hydrogen atom is  13.6 eV. On the other planet, this ionization potential energy will be 3.4 eV

b

The minimum permissible radius of the orbit will be 4ε0h2mπe2

c

In our world, the velocity electron is  v0 when the hydrogen atom is in the ground state.  The velocity of electron in this state on the other planet should be  v0/2

d

 In our world, the ionization potential energy of a hydrogen atom is  13.6 eV.  On the other planet, this ionization potential energy will be 1.5eV 

answer is A, B, C.

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Detailed Solution

On other planet: mvr=2nh2πv=nhπmr 
 mvr2r=14πε0e2r2mn2h2n2m2r314πε0e2r2
Putting  n=1, we get  r=4h2ε0mπe2
On our planet: v0=e22ε0nh
On other planet:  v=e22ε0(2n)hv02
On our planet:  En=13.6n2
On other planet: En=13.6(2n)2
En'=En4=3.4eV

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Hydrogen is the simplest atom of nature. There is one proton in its nucleus and an electron moves around the nucleus in a circular orbit. According to Niels Bohr, this electron moves in a stationary orbit, it emits no electromagnetic radiation. The angular momentum of the electron is quantized, i.e.,  mvr=(nh/2π), where m=mass of the electron, v = velocity of the electron in the orbit, r = radius of the orbit, and n=1,2,3...when transition takes place from  Kth  orbit to  Jth orbit, energy photon is emitted. If the wave length of the emitted photon is  λ, we find that  1λ=R[1J2−1K2], where R is Rydberg's constant.On a different planet, the hydrogen atom's structure was somewhat different from ours. There the angular momentum of electron was  P=2n(h/2π), i.e. an even multiple of (h/2π).