Given three identical spheres of mass \(2M\) placed at the corners of a right-angled triangle. The sides of the triangle are 4 m each. Let the point of intersection of the two sides be the origin \((0, 0)\). The position vectors of the masses are:
The position vector of the center of mass is given by:
\[ r_{\text{com}} = \frac{m_1 r_1 + m_2 r_2 + m_3 r_3}{m_1 + m_2 + m_3} \]
Substituting the values:
\[ r_{\text{com}} = \frac{2M \times (0, 0) + 2M \times (4, 0) + 2M \times (0, 4)}{6M} = \left(\frac{4}{3}, \frac{4}{3}\right) \]
Magnitude of \(r_{\text{com}}\):
\[ |r_{\text{com}}| = \sqrt{\left(\frac{4}{3}\right)^2 + \left(\frac{4}{3}\right)^2} = \sqrt{\frac{16}{9} + \frac{16}{9}} = \sqrt{\frac{32}{9}} = \frac{4\sqrt{2}}{3} \]
Thus, \(x = 3\).
This problem requires finding the magnitude of the position vector of the center of mass (COM) for a system of three identical spheres placed at the vertices of a right-angled isosceles triangle.
The position vector of the center of mass, \( \vec{R}_{COM} \), for a system of \( n \) particles is given by the weighted average of their position vectors:
\[ \vec{R}_{COM} = \frac{\sum_{i=1}^{n} m_i \vec{r}_i}{\sum_{i=1}^{n} m_i} \]In terms of coordinates, the x and y coordinates of the center of mass are:
\[ X_{COM} = \frac{m_1 x_1 + m_2 x_2 + m_3 x_3}{m_1 + m_2 + m_3} \] \[ Y_{COM} = \frac{m_1 y_1 + m_2 y_2 + m_3 y_3}{m_1 + m_2 + m_3} \]The magnitude of the position vector \( \vec{R}_{COM} = X_{COM} \hat{i} + Y_{COM} \hat{j} \) is calculated as:
\[ |\vec{R}_{COM}| = \sqrt{X_{COM}^2 + Y_{COM}^2} \]Step 1: Define the coordinate system and locate the positions of the spheres.
Let the origin (0, 0) be the vertex of the right angle. The two mutually perpendicular sides of length 4 m each lie along the positive x-axis and positive y-axis.
The three identical spheres, each of mass \( m = 2M \), are placed at the corners of this triangle. Let's label them as follows:
The mass of each sphere is \( m_1 = m_2 = m_3 = 2M \).
Step 2: Calculate the total mass of the system.
The total mass \( M_{total} \) is the sum of the individual masses:
\[ M_{total} = m_1 + m_2 + m_3 = 2M + 2M + 2M = 6M \]Step 3: Calculate the x and y coordinates of the center of mass.
Using the formula for \( X_{COM} \):
\[ X_{COM} = \frac{(2M)(0) + (2M)(4) + (2M)(0)}{6M} = \frac{0 + 8M + 0}{6M} = \frac{8M}{6M} = \frac{4}{3} \text{ m} \]Using the formula for \( Y_{COM} \):
\[ Y_{COM} = \frac{(2M)(0) + (2M)(0) + (2M)(4)}{6M} = \frac{0 + 0 + 8M}{6M} = \frac{8M}{6M} = \frac{4}{3} \text{ m} \]So, the position vector of the center of mass is \( \vec{R}_{COM} = \frac{4}{3} \hat{i} + \frac{4}{3} \hat{j} \).
Step 4: Calculate the magnitude of the position vector of the center of mass.
\[ |\vec{R}_{COM}| = \sqrt{X_{COM}^2 + Y_{COM}^2} = \sqrt{\left(\frac{4}{3}\right)^2 + \left(\frac{4}{3}\right)^2} \] \[ |\vec{R}_{COM}| = \sqrt{2 \times \left(\frac{4}{3}\right)^2} = \sqrt{2 \times \frac{16}{9}} = \frac{4\sqrt{2}}{3} \text{ m} \]The magnitude of the position vector of the center of mass is \( \frac{4\sqrt{2}}{3} \) m.
The problem states that this magnitude is equal to \( \frac{4\sqrt{2}}{x} \).
\[ \frac{4\sqrt{2}}{3} = \frac{4\sqrt{2}}{x} \]By comparing the two expressions, we can see that:
\[ x = 3 \]The value of x is 3.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,


What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)