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11
A rod AB carries three loads of 30 N, 70 N and 100 N at distances of 20 mm, 90 mm and 150 mm respectively from A. Neglecting the weight of the rod, the point at which the rod will balance is
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Answer: Option A
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12
The member forces in a statically in determinate truss
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Answer: Option B
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13
If v and $$\omega $$ are linear and angular velocities, the centripetal acceleration of a moving body along the circular path of radius r, will be
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Answer: Option B
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14
To attain the synchronous orbit, the launch of a satellite, is done from a place
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Answer: Option A
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15
The rotational velocity of a satellite is increased by 450 m per second if its launch is done from equator
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Answer: Option A
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16
When a body in equilibrium undergoes an infinitely small displacement, work imagined to be done, is known as
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Answer: Option C
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17
A ball which is thrown upwards, returns to the ground describing a parabolic path during its flight
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Answer: Option B
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18
A body A of mass 6.6 kg which is lying on a horizontal platform 4.5 m from its edge is connected to the end of a light string whose other end is supporting a body of mass 3.2 kg as shown in below figure. If the friction between the platform and the body A is $$\frac{1}{3}$$, the acceleration is
Applied Mechanics and Graphic Statics mcq question image
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Answer: Option C
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19
A cylinder will slip on an inclined plane of inclination angle $$\theta $$ if the coefficient of static friction between plane and cylinder is
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Answer: Option A
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20
The following factor affects the orbit of a satellite up to an altitude of 720 km from the earth's surface
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Answer & Solution
Answer: Option C
Solution:
Why: Up to about 720 km altitude, satellites are still in Low Earth Orbit (LEO), where the atmosphere is very thin but not absent. The residual air molecules produce aerodynamic drag on a satellite moving at roughly 7.5 km/s, which continuously removes orbital energy and causes gradual orbital decay.

Option A (Uneven gravitational field): Earth’s oblateness and mass irregularities do perturb orbits (e.g., nodal and apsidal precession), but at ~720 km these effects are secondary compared with drag when considering orbit maintenance and decay over practical timescales.

Option B (Gravity of the Sun and Moon): Third-body perturbations exist at all altitudes but are comparatively minor for LEO; their influence becomes relatively more important at higher altitudes (e.g., MEO/GEO).

Option C (Aerodynamic forces): Dominant disturbance in LEO up to ~720 km. Drag reduces velocity, lowers perigee, and accelerates decay, requiring periodic reboosts for orbit maintenance.

Conclusion: At altitudes up to 720 km, aerodynamic drag is the principal factor affecting a satellite’s orbit, making Option C correct.