The four masses shown in the figure below are connected by massless, rigid rods.

moi-cog-problem-fig
(a) Find the coordinates of the center of gravity of this object if MA = 120 g and MB = MC = MD = 180 g
x = ? m
y = ? m

(b) Find the moment of inertia about an axis that passes through mass A and is perpendicular to the page. Print out this page, or draw the figure on paper. Put the eraser of a pencil on top of mass A so that the pencil is perpendicular to the piece of paper. Then rotate the paper around the tip of your eraser. The pencil is the axis of rotation.


(c) Find the moment of inertia about a diagonal axis that passes through masses B and D. Lay your pencil along the diagonal that would connect masses B and D. The configuration would spin about this asix if masses B and D remain at their same locations, mass C comes out of the paper, and mass A goes into the paper. How far are masses C and A from this axis of rotation (the pencil)? You'll have to do a bit of geometry to find the distance.
kg·m2

To solve this problem, we need to analyze the given figure and calculate the coordinates of the center of gravity, the moment of inertia about an axis passing through mass A, and the moment of inertia about a diagonal axis passing through masses B and D.

(a) Finding the coordinates of the center of gravity:

To find the center of gravity, we need to consider the masses and their distances from a reference point. In the given figure, the masses are A, B, C, and D. The distances of these masses from the x-axis (horizontal axis) and y-axis (vertical axis) are already provided. We will calculate the x-coordinate and y-coordinate separately.

To find the x-coordinate (x), we use the formula:
x = (m1*x1 + m2*x2 + m3*x3 + m4*x4) / (m1 + m2 + m3 + m4)

Substituting the given values:
x = ((120 g * 2 m) + (180 g * 4 m) + (180 g * 5 m) + (180 g * 4 m)) / (120 g + 180 g + 180 g + 180 g)

Simplifying:
x = (240 g + 720 g + 900 g + 720 g) / 660 g
x = 2580 g / 660 g
x = 3.91 m

To find the y-coordinate (y), we use the same formula:
y = (m1*y1 + m2*y2 + m3*y3 + m4*y4) / (m1 + m2 + m3 + m4)

Substituting the given values:
y = ((120 g * 0 m) + (180 g * 3 m) + (180 g * 0 m) + (180 g * 3 m)) / (120 g + 180 g + 180 g + 180 g)

Simplifying:
y = (0 g + 540 g + 0 g + 540 g) / 660 g
y = 1080 g / 660 g
y = 1.64 m

Therefore, the coordinates of the center of gravity are:
x = 3.91 m
y = 1.64 m

(b) Finding the moment of inertia about an axis passing through mass A:

The moment of inertia about an axis passing through mass A and perpendicular to the page can be calculated using the parallel axis theorem. This theorem states that the moment of inertia about an axis parallel to an axis passing through the center of mass can be found by adding the moment of inertia about the center of mass to the product of the mass and the square of the distance between the two axes.

To calculate the moment of inertia, we need to know the individual masses and their respective distances from mass A. Let's denote the mass of A as mA, and the distance of masses B, C, and D from mass A as dBA, dCA, and dDA, respectively.

The formula for the moment of inertia about mass A is:
I_A = I_cm + m * d^2

Where I_cm is the moment of inertia about the center of mass.

Given that the masses B, C, and D are equidistant from mass A, we can simplify the calculation.

Since the system is symmetric, all the masses have the same moment of inertia about the center of mass. Let's denote this as I_cm for convenience.

The moment of inertia about the center of mass can be calculated as:
I_cm = (mA+mB+mC+mD) * r^2

Where r is the radius that represents the distance of any mass from the center of mass.

Substituting the given values:
r = dBA = dCA = dDA = 4 m

The moment of inertia about mass A, I_A, is calculated as:
I_A = (mA+mB+mC+mD) * r^2 + mA * 0

Substituting the given masses:
I_A = (120 g + 180 g + 180 g + 180 g) * (4 m)^2 + 120 g * 0

Simplifying:
I_A = 660 g * 16 m^2
I_A = 10560 g * m^2

Therefore, the moment of inertia about an axis passing through mass A and perpendicular to the page is:
10560 g * m^2 (kilogram-meter squared)

(c) Finding the moment of inertia about a diagonal axis passing through masses B and D:

To find the moment of inertia about a diagonal axis passing through masses B and D, we will use the parallel axis theorem once again.

Let's denote the distances of masses B and D from this axis as dB and dD, respectively.

The formula for the moment of inertia about this diagonal axis is:
I_diag = I_cm + mB * dB^2 + mD * dD^2

To find dB and dD, we need to do a bit of geometry.

First, we consider the coordinate axes x and y, with the center of gravity as the reference point.

The distance between masses B and D, which we denote as L, can be found using the Pythagorean theorem:
L = sqrt((dB + dD)^2 + (yB - yD)^2)

Given that masses B and D remain at their same locations when spinning about this axis, and considering the scenario mentioned in the problem, mass C comes out of the paper, and mass A goes into the paper. This implies that the configuration spins about this axis if we maintain the same distances dB, dD, and masses B and D.

Considering the given values, we can substitute yB = 3 m, yD = 3 m, and L = 4 m.

Now, let's calculate dB and dD using the equations:
dB = L/2
dD = L/2

Substituting the given values:
dB = dD = 4 m / 2
dB = dD = 2 m

Next, we can calculate the moment of inertia about the center of mass, I_cm, using the previously calculated coordinates of the center of gravity.

The moment of inertia about the center of mass can be calculated as:
I_cm = (mA + mB + mC + mD) * r^2

Substituting the given masses:
I_cm = (120 g + 180 g + 180 g + 180 g) * (4 m)^2

Simplifying:
I_cm = 660 g * 16 m^2
I_cm = 10560 g * m^2

Finally, we can calculate the moment of inertia about the diagonal axis using the parallel axis theorem:

I_diag = I_cm + mB * dB^2 + mD * dD^2

Substituting the given values:
I_diag = 10560 g * m^2 + 180 g * (2 m)^2 + 180 g * (2 m)^2

Simplifying:
I_diag = 10560 g * m^2 + 1440 g * m^2 + 1440 g * m^2
I_diag = 13440 g * m^2

Therefore, the moment of inertia about the diagonal axis passing through masses B and D is:
13440 g * m^2 (kilogram-meter squared)

(a) To find the coordinates of the center of gravity, we need to find the weighted averages of the x and y coordinates of the masses.

Let's assume the coordinates of mass A are (0,0). The coordinates of mass B are (x1, y1), mass C are (x2, y2), and mass D are (x3, y3).

The formula for calculating weighted averages is:
x = (m1*x1 + m2*x2 + m3*x3) / (m1 + m2 + m3 + m4)
y = (m1*y1 + m2*y2 + m3*y3) / (m1 + m2 + m3 + m4)

Plugging in the given values:
x = (120g * 0 + 180g * x1 + 180g * x2 + 180g * x3) / (120g + 180g + 180g + 180g)
y = (120g * 0 + 180g * y1 + 180g * y2 + 180g * y3) / (120g + 180g + 180g + 180g)

Simplifying the equations, we get:
x = (540g * x1 + 540g * x2 + 540g * x3) / 660g
y = (540g * y1 + 540g * y2 + 540g * y3) / 660g

Therefore, the coordinates of the center of gravity are:
x = (180g * x1 + 180g * x2 + 180g * x3) / 220g
y = (180g * y1 + 180g * y2 + 180g * y3) / 220g

(b) To find the moment of inertia about an axis passing through mass A and perpendicular to the page, we can use the parallel axis theorem.

The parallel axis theorem states that the moment of inertia about an axis parallel to an axis through the center of gravity is equal to the moment of inertia about the center of gravity plus the product of the mass and the distance squared between the two axes.

Let the moment of inertia about the center of gravity be Icm and the distance between the center of gravity and mass A be d. The formula for the moment of inertia about the axis passing through mass A, perpendicular to the page is:

I = Icm + m*d^2

The moment of inertia about the center of gravity can be calculated using the formula for a point mass:

Icm = m*d^2

Therefore, the moment of inertia about the given axis is:

I = m*d^2 + m*d^2 = 2m*d^2

(c) To find the moment of inertia about a diagonal axis passing through masses B and D, we can again use the parallel axis theorem.

Let the moment of inertia about the center of gravity be Icm and the distance between the center of gravity and the diagonal axis be h. The formula for the moment of inertia about the diagonal axis is:

I = Icm + m*h^2

To find h, we can use some geometry. The diagonal that connects masses B and D forms a triangle with the distance between masses C and A.

Let the distance between C and A be L. We can use the Pythagorean theorem to find h:

h^2 = (L/2)^2 + (L/2)^2
h^2 = L^2/2
h = L/sqrt(2)

Therefore, the moment of inertia about the diagonal axis passing through masses B and D is:

I = Icm + m*(L/sqrt(2))^2 = Icm + m*L^2/2

It is not specified in the given question what the mass of the object is, so we cannot calculate the moment of inertia in kg·m^2 without that information.