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গ্রহের পর্যায়কাল T এবং সূর্য থেকে গ্রহের গড় দূরত্ব r হলে কেপলারের তৃতীয় সূত্রানুসারে-

Created: 1 year ago | Updated: 1 year ago

Updated: 1 year ago

T \infty r

T \infty r^{2}

T^{2} \infty r

T^{2} \infty r^{3}

Explanation

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\vec{A} . \vec{B}

\vec{C}

20 Ω

1.6 \times 10^{- 19} C

9.11 \times 10^{- 31} k g

S = \frac{1}{3} t^{3} + 3 t

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