Consider the spectral line resulting from the transition from n= 2 to n = 1, in atoms and ions given below. The shortest wavelength is produced by
hydrogen atom
deuterium atom
doubly ionized lithium
doubly ionized helium
The energy of an electron in excited hydrogen atom is −3.4eV. Then according to Bohr's theory, the angular momentum of the electron is
2.1 × 10-34 J-s
3 × 10-34 J-s
2 × 10-34 J-s
0.5 × 10-34 J-s
The solar spectrum during a complete solar eclipse is
continuous
emission line
dark line
dark band
A particle of mass M at rest decays into two masses m1 and m2 with non zero velocities. The ratio of de-Broglie wavelengths of the particles is
1 : 1
If elements with principal quantum number n > 4 were not allowed in nature, the number of possible elements would have been
32
60
64
4
The spectrum obtained from the chromosphere of the sun at the time of total solar eclipse is
line emission spectrum
band emission spectrum
continuous emission spectrum
line absorption spectrum
D.
line absorption spectrum
Chromosphere (sphere of colour) is the outer region of the sun. Just below the chromosphere lies the photosphere (sphere of light). The density of gases decreases with altitude near the chromosphere. The temperature of chromosphere is lower than that of photosphere. The photosphere emits continuous spectrum and when this passes through the chromosphere, absorption takes place and these absorption lines are observed as dark lines in the solar spectrum. During a total solar eclipse, when the light from the photosphere is completely cut off, the chromosphere is visible to us. Hence, the line absorption spectrum with a continuous background is visible during a total solar eclipse.
Which state of triply ionised Beryllium (Be+++) has the same orbital radius as that of the ground state of hydrogen ?
n = 3
n = 4
n = 1
n = 2
Excitation energy of a hydrogen like ion in its first excitation state is 40.8 eV. Energy needed to remove the electron from the ion in ground state is
40.8 eV
27.2 eV
54.4 eV
13.6 eV