Let Cp represent the specific heat of the metal object.
To find this, we can set up a heat balance equation (heat lost by metal = heat gained by water):
- 19g * Cp * (22degC – 96degC) = 75g * 4.184J/g degC * (22degC - 18degC)
<span>Cp = 0.893 J/g degC</span>
a) 3.56 x 10^22 N. b) 3.56 x 10^22 N. The sun’s mass is M = 2 x 10^30 kg, while the Earth's mass is m = 6 x 10^24 kg, with a distance of R = 1.5 x 10^11 m separating them. Applying Newton's law for gravitational force F = G (mM / R²), where G = 6.67 × 10^-11 m^3 kg^-1 s^-2 gives us F = 3.56 x 10^22 N. A) The gravitational force by the sun on Earth equates to the force exerted by Earth on the sun, which is also 3.56 x 10^22 N.
Answer:
The force required has a magnitude of 2601.9 N
Explanation:
m = 450 kg
Static friction coefficient μs = 0.73
Kinetic friction coefficient μk = 0.59
The force necessary to initiate movement of the crate is
.
Once the crate begins to move, the frictional force decreases to
.
To maintain the motion of the crate at a steady velocity, we must lower the pushing force to
.
Subsequently, the pushing force aligns with the frictional force stemming from kinetic friction, enabling balanced forces and consistent velocity.
<pMagnitude of the force
