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Question 12 Marks
An artificial satellite is going round the earth, close to its surface. What is the time taken by it to complete one round? Given radius of the earth $=6400 km$.
Answer
Here $R =6400 km=6.4 \times 10^6 m$
$
g=9.8 ms^{-2}
$
Orbital velocity near the earth's surface is
$
v_0=\sqrt{g R}=\sqrt{9.8 \times 6.4 \times 10^6}=7918 ms^{-1}
$
Time period,
$
\begin{aligned}
& R=\frac{2 \pi R}{v 0}=\frac{2 \times 22 \times 6.4 \times 10^6}{7 \times 7918}=5080 s \\
& =1.411 \text { hour }
\end{aligned}
$
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Question 22 Marks
A cyclist speeding at $18 km / h$ on a level road takes a sharp circular turn of radius 3 m without reducing the speed. The coefficient of static friction between the tyres and the road is 0.1 . Will the cyclist slip while taking the turn?
Answer
Speed of the cyclist
$
v=18 km / h=18 \times \frac{5}{18}=5 m / s
$
Given: Radius $r=3 m \quad \mu=0.1$
The safe limit of velocity $v_s=\sqrt{\mu r g}$
So, $v_s=\sqrt{0.1 \times 10 \times 3}=1.732 m / s$
Since, cyclist rides at a faster speed than safe limit. So, the cyclist slips.
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Question 32 Marks
Answer
The given formula will be dimensionally correct only when the dimension of L.H.S will be same as that of R.H.S. This is only possible when the factor, $\left(1-v^2\right)^{\frac{1}{2}}$ is dimensionless i.e., $\left(1-v^2\right)$ is dimensionless. This can only possible when $v^2$ is divided by the square of another velocity term. And here that term is $c^2$. So, $v ^2$ should be divided by $c^2$ to make the denominator of the fraction dimensionless. Hence, the correct relation is $m=\frac{m_0}{\left(\frac{v^2}{c^2}\right)^{\frac{1}{2}}}$ From this relativistic mass formula, one can easily see that when the velocity of a particle becomes comparable to the speed of light, its mass increases.
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Question 42 Marks
If the earth were made of lead of relative density 11.3 , what then would be the value of acceleration due to gravity on the surface of the earth? Radius of the earth $=6.4 \times 10^6 m$ and $G =6.67 \times 10^{-11} Nm ^2 kg^{-2}$.
Answer
Density of the earth,
$\rho=$ Relative density $\times$ density of water
$
=11.3 \times 10^3 kgm^{-3}
$
Acceleration due to gravity on the earth's surface,
$
\begin{aligned}
& g=\frac{G M}{R^2}=\frac{G}{R^2} \cdot \frac{4}{3} \pi R^3 \times \rho=\frac{4}{3} \pi G R \rho \\
& =\frac{4}{3} \times \frac{22}{7} \times 6.67 \times 10^{-11} \times 6.4 \times 10^6 \times 11.3 \times 10^3 \\
& =22.21 ms^{-2}
\end{aligned}
$
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Question 52 Marks
Subtract $2.5 \times 10^4$ from $3.9 \times 10^5$ with due regard to significant figures.
Answer
We have $3.9 \times 10^5-2.5 \times 10^4$
$
\begin{aligned}
& =3.9 \times 10^5-0.25 \times 10^5 \\
& =3.65 \times 10^5
\end{aligned}
$
But our answer should be rounded off up to two significant digits.
So, the answer will be $3.6 \times 10^5$
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Question 62 Marks
Write the equation of a progressive wave propagating along the positive x -direction, whose amplitude is 5 cm , frequency 250 Hz and velocity $500 ms^{-1}$.
Answer
Here $A =5 cm=0.05 m, v =250 Hz, \nu=500 ms^{-1}$
Wavelength, $\lambda=\frac{v}{\nu}=\frac{500}{250}=2 m$
Period, $T=\frac{1}{v}=\frac{1}{250} s$
The equation for the given wave can be written as $y =A \sin 2 \pi\left(\frac{t}{T}-\frac{x}{\lambda}\right)=0.05 \sin 2 \pi\left(250 t-\frac{x}{2}\right)$
or $y=0.05 \sin \times(500 t-x)$ metre
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