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Vladimir [108]
3 years ago
14

A spacecraft in the shape of a long cylinder has a length of 100 m,and its mass with occupants is 1490kg. It has strayed too clo

se to a black hole having a mass97 times that of the Sun. The nose ofthe spacecraft points toward the black hole, and the distancebetween the nose and the center of the black hole is 10.0 km.
(a) Determine the total force on thespacecraft.
(b) What is the difference in the gravitational fields acting onthe occupants in the nose of the ship and on those in the rear ofthe ship, farthest from the black hole? This difference inacceleration grows rapidly as the ship approaches the black hole.It puts the body of the ship under extreme tension and eventuallytears it apart.
Physics
1 answer:
Anna [14]3 years ago
7 0

To develop this problem, it is necessary to apply the concepts related to the Gravitational Force and its respective change related to the black hole.

Gravitational Force are given as

F = \frac{GMm}{(R+l)^2}

Where

l = Length

R = Separation between both

M = Mass of Object

m = mass of block hole

G = Gravitational Universal constant

Our values are given as

l = 100m

M = 1490

m = 97 m_s \rightarrow m_s is mass of sun

R = 10km

PART A ) Replacing in our equation we have that

F = \frac{GMm}{(R+l)^2}

F = \frac{(6.67*10^{-11})(1490)(97*(1.99*10^{30}))}{(10000+100)^2}

F = 1.8805*10^{17}N

PART B) The difference at this force would be given as

\Delta F = \frac{GMm}{(R_{front})^2}-\frac{GMm}{(R_{back})^2}

As Force is equal to mass and gravity then

\Delta g = \frac{\Delta F}{m}

\Delta g = \frac{GM}{(R_{front})^2}-\frac{GMm}{(R_{back})^2}

\Delta g = \frac{(6.67*10^{-11})(97*(1.99*10^{30})}{(10000+100)^2}-\frac{(6.67*10^{-11})(97*(1.99*10^{30})}{(10000)^2}

\Delta g = 2.53*10^{12}N

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please help! find magnitude and direction (the counterclockwise angle with the +x axis) of a vector that is equal to a + c
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Answer:

Option (2)

Explanation:

From the figure attached,

Horizontal component, A_x=A\text{Sin}37

A_x=12[\text{Sin}(37)]

     = 7.22 m

Vertical component, A_y=A[\text{Cos}(37)]

    = 9.58 m

Similarly, Horizontal component of vector C,

C_x  = C[Cos(60)]

     = 6[Cos(60)]

     = \frac{6}{2}

     = 3 m

C_y=6[\text{Sin}(60)]

    = 5.20 m

Resultant Horizontal component of the vectors A + C,

R_x=7.22-3=4.22 m

R_y=9.58-5.20 = 4.38 m

Now magnitude of the resultant will be,

From ΔOBC,

R=\sqrt{(R_x)^{2}+(R_y)^2}

   = \sqrt{(4.22)^2+(4.38)^2}

   = \sqrt{17.81+19.18}

   = 6.1 m

Direction of the resultant will be towards vector A.

tan(∠COB) = \frac{\text{CB}}{\text{OB}}

                  = \frac{R_y}{R_x}

                  = \frac{4.38}{4.22}

m∠COB = \text{tan}^{-1}(1.04)

             = 46°

Therefore, magnitude of the resultant vector will be 6.1 m and direction will be 46°.

Option (2) will be the answer.

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