1) An electron can revolve around the nucleus in certain fixed orbits of definite energy without emission of any radiant energy. Such orbits are called stationary orbits.
2) An electron can make a transition from a stationary state of higher energy E2 to a state of lower energy E1 and in doing so, it emits a single photon of frequency,
v=E2−E1h where h is the plank constant.
Conversely, on absorbing an energy, E2−E1 when the electron is at energy E1, the electron can take transition from E1 to E2.
3) Only those orbits are allowed for which the angular momentum of the electron is an integral multiple of h2π.
thus L=nh2π where n=1,2,3...
If radius of first bohr orbit is r1 and radius of nth bohr orbit is rn then relation between them is given by,
rn=n2r1