Imagine a light planet is revolving round a very massive star in a circular orbit of radius R with a time period of revolution T. If the gravitational force of attraction between the star and planet is proportional to&nbsp;<math xmlns="http://www.w3.org/1998/Math/MathML"><msup><mi mathvariant="normal">R</mi><mrow><mo>-</mo><mi mathvariant="normal">n</mi></mrow></msup></math>, then T2 is proportional to&nbsp;

Energy of electron in second orbit of He+ is&nbsp;

Statement–I : Rutherford’s model of Atom cannot explain lines Spectrum of hydrogen atom Statement–II: Bohr’s model is not in accordance with Heisenberg’s uncertainty principle

Transition from n2 =4,5,6 to n1 =3 in hydrogen spectrum gives&nbsp;&nbsp;&nbsp;&nbsp; series.

The shortest wavelength of H atom in the Lyman series is&nbsp;<math xmlns="http://www.w3.org/1998/Math/MathML"><msub><mi>λ</mi><mn>1</mn></msub></math>&nbsp;.&nbsp;The longest wavelength in the Balmer series of He+ is :

If the shortest wavelength of H- atom in Lyman series is<math xmlns="http://www.w3.org/1998/Math/MathML"><mo>&nbsp;</mo><mi>X</mi></math>&nbsp; the longest&nbsp;wavelength in Blamer series of&nbsp;<math xmlns="http://www.w3.org/1998/Math/MathML"><mi>H</mi><msup><mi>e</mi><mo>+</mo></msup></math>&nbsp;is&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;

Imagine a light planet is revolving round a very massive star in a circular orbit of radius R with a time period of revolution T. If the gravitational force of attraction between the star and planet is proportional to $R^{- n}$ , then T²is proportional to

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Imagine a light planet is revolving round a very massive star in a circular orbit of radius R with a time period of revolution T. If the gravitational force of attraction between the star and planet is proportional to R-n, then T2 is proportional to

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Imagine a light planet is revolving round a very massive star in a circular orbit of radius R with a time period of revolution T. If the gravitational force of attraction between the star and planet is proportional to $R^{- n}$ , then T²is proportional to