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yuradex [85]
4 years ago
9

The drawing shows a large cube (mass = 28.6 kg) being accelerated across a horizontal frictionless surface by a horizontal force

P. A small cube (mass = 4.3 kg) is in contact with the front surface of the large cube and will slide downward unless P is sufficiently large. The coefficient of static friction between the cubes is 0.710. What is the smallest magnitude that P can have in order to keep the small cube from sliding downward?
Physics
1 answer:
MrRissso [65]3 years ago
8 0

Answer:

P= 454.11 N

Explanation:

Since P is the only horizontal force acting on the system, it can be defined as the product of the acceleration by the total mass of the system (both cubes).

P= (M+m)*a\\a = \frac{P}{28.6 +4.3}\\a = \frac{P}{32.9}

The friction force between both cubes (F) is defined as the normal force acting on the smaller cube multiplied by the coefficient of static friction. Since both cubes are subject to the same acceleration:

F = m * a*\mu \\F= 4.3*0.710*\frac{P}{32.9}\\F=3.053*\frac{P}{32.9}

In order for the small cube to not slide down, the friction force must equal the weight of the small cube:

3.053*\frac{P}{32.9} = 4.3 * g\\\\P = \frac{4.3*9.8*32.9}{3.053} \\P= 454.11 N

The smallest magnitude that P can have in order to keep the small cube from sliding downward is 454.11 N

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Please check if my answer is correct
emmasim [6.3K]

Answer:

Yep! it's correct might need to double check tho

4 0
3 years ago
Read 2 more answers
Consider the first major feature (orderly motions). Which of the following correctly describe patterns of motion in our solar sy
snow_lady [41]

Answer:

(a), (c), (e)  

Explanation:

<em>(a) The Sun and most of the planets rotate in the same direction that the planets orbit.</em>

The Sun and most of the planets rotates in the same direction (counter-clockwise) as a consequence of the conservation of the angular momentum from the could in which they were formed.

However, Venus and Uranus rotate in retrograde motion (clockwise), it is  thought that is due to the collision with an asteroid in the early days of both planets.

<em>(b) Major moons generally have polar orbits, meaning orbits that take them over the north and south poles of the planet they orbit.</em>

Polar orbits are not common between major moons, They follow orbits related to the plane of the Solar System.    

<em>(c) Planets have nearly circular orbits.</em>

Kepler's first law establishes:

<em>All the planets revolve around the Sun in an ellipse orbit, with the Sun in one of the focus.</em>

The ellipse has a low eccentricity in the case of planetary orbits.

<em>(d) The outer planets are so large that they nearly collide with each other on each orbit.</em>

They have enough space between them, so it is not possible a collision.

For example, lets take the example of the diameter on Jupiter and Saturn. The diameter of Jupiter is 139.820 Km while Saturn has a diameter of 116.460 Km.

The distance of Saturn from the Sun is 9.5 AU (AU = Astronomical Unit) while in Jupiter is 5.1 AU.

1 AU is defined as the distance between the Earth and the Sun (1.50x10^{8} Km)

The distance of Saturn from the Sun in Kilometers:  

d_{saturn} = 9.5 AU . \frac{1.50x10^{8} Km}{1AU}

d_{saturn} = 1.425x10^{9} Km

The distance of Jupiter from the Sun in Kilometers:

d_{saturn} = 5.1 AU . \frac{1.50x10^{8} Km}{1AU}

d_{saturn} = 7.65x10^{8} Km

Distance between the two planets:

d_{J-S} = 1.425x10^{9} Km -7.65x10^{8} Km

d_{J-S} = 6.60x10^{8} Km

If the distance between the planets is compared with the diameters of any of them, it is easy to see that the planets can't be in a collision since they don't fill the space between them with its diameter.

In the case of Jupiter:

diameter_{Jupiter} d_{J-S}

139.820 Km 6.60x10^{8}

In the case of Saturn:

diameter_{Saturn} d_{J-S}      

116.460 Km 6.60x10^{8}    

<em>(e)All the planets orbit the Sun in nearly the same plane.</em>

When the cloud, from were the planets form, collapse, it starts to rotate and accrete the material in a disk. Given as a result that the planets were in nearly the same plane.

It is important to consider that planets have different degrees of orbital inclinations, which is due to interactions with others object while its formation.

<em>(f) Inner planets orbit the Sun in the opposite direction from the outer planets </em>

This is not correct. Inner planets are constituted by Mercury, Venus, Earth, and Mars.

Mercury, Earth and Mars share the counter-clockwise direction as some outer planets, while Venus shares the same retrograde motion as Uranus.    

7 0
4 years ago
A ship maneuvers to within 2500 m of an island's 1800 m high mountain peak and fires a projectile at an enemy ship 610 m on the
Ne4ueva [31]
Thank you for posting your question here at brainly. I hope the answer will help you. Feel free to ask more questions.

t=(0-(250sin75)^2)/-9.8 
<span>the distance one is (2500+610)- (250m/s*cos75)*t=Dh Dh=horizontal distance </span>

<span>the max height one is d=0.5*9.8*t^2 </span>
<span>d= max height subtract 1800-d</span>
3 0
3 years ago
Read 2 more answers
An initially stationary electron is accelerated by a uniform 640 N/C Electric Field. a) Calculate the kinetic energy of the elec
bulgar [2K]

Answer:

(a) 1.298 * 10^(-4) J

(b) 5.82 * 10^6 m/s

Explanation:

Parameters given:

Electric field, E = 640 N/C

Distance traveled by electron, r = 15 cm = 0.15 m

Mass of electron, m = 9.11 * 10^(-31) kg

Electric charge of electron, q = 1.602 * 10^(-19) C

(a) The kinetic energy of the electron in terms of Electric field is given as:

K = (q² * E² * r²) / 2m

Therefore, Kinetic energy, K, is:

K = [(1.602 * 10^(-19))² * 640² * 0.15²] / [2 * 9.11 * 10^(-31)]

K = {23651.981 * 10^(-38)} / [18.22 * 10^(-31)]

K = 1298.13 * 10^(-7) J = 1.298 * 10^(-4) J

(b) To find the final velocity of the electron, we have to first find the acceleration of the electron. This can be gotten by using the equations of force.

Force is generally given as:

F = ma

Electric force is given as:

F = qE

Therefore, equating both, we have:

ma = qE

a = (qE) / m

a = (1.602 * 10^(-19) * 640) / (9.11 * 10^(-31))

a = 112.54 * 10^(12) m/s² = 1.13 * 10^(14) m/s²

Using one of the equations of motion, we have that:

v² = u² + 2as

Since the electron started from rest, u = 0 m/s

Therefore:

v² = 2 * 1.13 * 10^(14) * 0.15

v² = 3.39 * 10^(13)

v = 5.82 * 10^6 m/s

The velocity of the electron after moving a distance of 15 cm is 5.82 * 10^6 m/s.

8 0
3 years ago
Why are some starburst galaxies much brighter in infrared than they are in visible light?
Anna35 [415]

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A sort of radiant energy that we experience as heat but that is invisible to human eyes is infrared radiation (IR), often known as infrared light. The sun and fire are two of the most prominent sources of IR radiation, however all objects in the cosmos release some of it.

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