A flute is played with a first harmonic of 196 Hz (a pitch of G3). The length of the air


column is 89. 2 cm (quite a long flute). Find the speed of the wave resonating in the


flute.

The wire won't break because the tension is less than 350N. To assess whether the wire will break, we need to calculate the tension in the wire using the principle of moments to do this, taking moments about point 0.

First, we need to calculate the weight of the flagpole and flag. We know that mass = 15 kg, so we can use the formula weight = mass x gravity, where gravity = 9.8 m/s^2. Therefore, weight = 15 x 9.8 = 147 N.

Next, we need to calculate the force exerted by the wire. We can use trigonometry to find the horizontal and vertical components of this force. The horizontal component is given by F_h = F x cos θ, where F is the tension in the wire and θ is the angle between the wire and the flagpole. In this case, F_h = F x cos 20°.

The vertical component is given by F_v = F x sin θ. In this case, F_v = F x sin 20°.

Now, we can take moments about point 0. The weight of the flagpole and flag acts vertically downwards at a distance of 0.8 m from point 0, so its moment is 147 x 0.8 = 117.6 Nm (clockwise).

The force exerted by the wire acts at an angle of 20° to the flagpole, so its horizontal component acts perpendicular to the flagpole and its vertical component acts parallel to the flagpole. The horizontal component has no moment about point 0, so we only need to consider the vertical component. This acts at a distance of 1.2 m from point 0, so its moment is F_v x 1.2 (anticlockwise).

Setting the moments equal to each other, we get:

147 x 0.8 = F_v x 1.2 x  sin 20°

Simplifying this equation, we get:

F_v = 78.7 N

To find the tension in the wire, we can use Pythagoras' theorem:

F = √(F_h^2 + F_v^2) = √((F x cos 20°)^2 + 78.7^2)

Simplifying this equation, we get:

F = 87.6 N

Since the tension in the wire is less than 350N, the wire will not break.

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The centripetal acceleration of the moon is approximately 0.0027 m/s².

To find the mean orbital speed of the moon and its centripetal acceleration, we'll use the given information of the moon's orbit radius and revolution time.

a) To find the mean orbital speed (v) of the moon, we'll use the formula v = 2 * π * r / T, where r is the orbit radius (3.84 x 10^8 m) and T is the revolution time (27.3 days, converted to seconds).

v = 2 * π * (3.84 x 10^8 m) / (27.3 days * 24 hours/day * 3600 s/hour) ≈ 1022 m/s

The mean orbital speed of the moon is approximately 1022 m/s.

b) To find the centripetal acceleration (a_c) of the moon, we'll use the formula a_c = v² / r.

a_c = (1022 m/s)² / (3.84 x 10⁸ m) ≈ 0.0027 m/s²

The centripetal acceleration of the moon is approximately 0.0027 m/s².

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The compressibility of a bone is dependent on its material properties and geometry. If the first bone was compressed by 1.0 mm, the second bone will be compressed by 2.0 mm. Answer is 2.0 mm.

Since the second bone has the same cross-sectional area but twice the length as the first, it has twice the volume. Therefore, it would be expected to compress twice as much as the first bone, or 2.0 mm.
Hi! When considering the compression of a bone, we can use Hooke's Law, which states that the deformation (compression) is directly proportional to the applied force and inversely proportional to the material's stiffness.

For the second bone with twice the length, the same force will cause a greater deformation since the stiffness will be lower. Given that the cross-sectional area is the same, the second bone will be compressed by twice the amount of the first bone.

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The most likely reason for not seeing the Power Pivot tab is that the add-in is not enabled in Excel.

By default, the Power Pivot add-in is not enabled in Excel, and it needs to be enabled manually.

To enable the Power Pivot add-in, go to the File tab in Excel, select Options, and then select Add-Ins. In the Manage box, select COM Add-ins, and then select Go.

In the COM Add-Ins dialog box, select Microsoft Power Pivot for Excel, and then select OK.

After enabling the add-in, the Power Pivot tab should now be visible in Excel.

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The average current during the lightning strike is approximately 12,500 amperes (A). It's important to note that lightning strikes involve extremely high currents and voltages, making them potentially dangerous and capable of causing significant damage.

When a lightning strike occurs, it involves a rapid discharge of electrical energy between a cloud and the ground. The statement you provided indicates that 2.5 coulombs (C) of charge flows from the cloud to the ground in 0.20 milliseconds (ms).

To calculate the average current during this time interval, we can use the formula:

Average current (I) = Charge (Q) / Time (t)

In this case, the charge is 2.5 C, and the time is 0.20 ms (which is equivalent to 0.20 x [tex]10^{(-3)[/tex] seconds). Plugging these values into the formula, we get:

I = 2.5 C / (0.20 x [tex]10^{(-3)[/tex] s)

I = 2.5 C / 2 x [tex]10^{(-4)[/tex]s

I = 12,500 A

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The volume of wire can be calculated as follows:

V_wire = πr²l

where r is the radius of the wire, and l is the length of the wire.

Substituting the given values, we get:

V_wire = π(3.0 mm)²(200 m) = 1.8 x 10⁶ mm³

To calculate the radius of the sphere, we need to use the formula for the volume of a sphere:

V_sphere = (4/3)πr³

Equating the volume of the wire to the volume of the sphere, we get:

(4/3)πr³ = 1.8 x 10⁶ mm³

Solving for r, we get:

r = (3V_wire/4π)^(1/3)

r = [(3 x 1.8 x 10⁶)/(4π)]^(1/3)

r ≈ 20.15 m

Therefore, the radius of the sphere is approximately 20.15 meters.

Force when The seperation is 10 cm= 1.36 x 10^-45 N and when it is 30 cm= 1.51 x 10^-46 N

To answer your question, we will use Coulomb's Law to calculate the force between the charged spheres (electron and proton). Coulomb's Law states:

F = k * (q1 * q2) / r^2

Where F is the force, k is the electrostatic constant (8.99 x 10^9 Nm^2/C^2), q1 and q2 are the charges of the spheres, and r is the distance between them.

Given the charges q1 = 9.11 x 10^-31 C (electron) and q2 = 1.67 x 10^-27 C (proton), and the initial distance r = 10 cm = 0.1 m, we can calculate the force:

F = (8.99 x 10^9 Nm^2/C^2) * (9.11 x 10^-31 C) * (1.67 x 10^-27 C) / (0.1 m)^2
F ≈ 1.35 x 10^-45 N

Now, let's calculate the force when the separation is increased to 30 cm = 0.3 m:

F_new = (8.99 x 10^9 Nm^2/C^2) * (9.11 x 10^-31 C) * (1.67 x 10^-27 C) / (0.3 m)^2
F_new ≈ 1.50 x 10^-46 N

So, the force between the charged spheres when they are 10 cm apart is approximately 1.35 x 10^-45 N, and when the separation is increased to 30 cm, the force becomes approximately 1.50 x 10^-46 N.

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Answer:

The generator makes static electricity the same way you do when you rub your feet on the carpet and then touch a doorknob.

Explanation:

. Inside the generator is a giant rubber band that rubs across a piece of felt, stealing its electrons. The rubber band then spins around and the electrons travel up to the big metal ball on top.

In the context of the Sun, gravitational equilibrium refers to the balance between the inward gravitational force and the outward pressure force that acts within the Sun's interior. This equilibrium is crucial for maintaining the Sun's stability and preventing its collapse or runaway expansion.

In a simplified explanation, the gravitational force in the Sun's core is responsible for pulling matter inward. At the same time, the high temperatures and pressures in the core generate intense radiation pressure and gas pressure, pushing matter outward. The combination of these inward and outward forces creates a balance.

Different regions within the Sun contribute to this equilibrium, with variations in temperature, density, and pressure. These variations can result in different colors and arrow lengths in a diagram, which may represent the following:

1. Colors: Different colors might be used to represent different regions or layers within the Sun, each with its specific characteristics and properties. For example, the core, radiative zone, and convective zone of the Sun have distinct temperature and pressure profiles, which could be depicted using different colors.

2. Arrow Lengths: Arrow lengths might be used to illustrate the strength or magnitude of the forces involved. Longer arrows could indicate stronger forces, such as higher pressure or greater gravitational forces. Shorter arrows may represent weaker forces or areas where the forces balance each other.

It's important to note that the specific colors and arrow lengths used in a diagram can vary depending on the particular representation and the context of the diagram you are referring to. It would be helpful to provide a description or more specific details about the diagram for a more accurate interpretation.

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Answer:

The power delivered by Jose when doing push-ups is 25 watts.

Step-by-step explanation:

The power delivered by Jose is:

[tex]\sf\qquad\dashrightarrow Power = \dfrac{Work}{Time}[/tex]

We know that Jose did 50 J of work in 2 seconds, so we can substitute these values into the equation:

[tex]\sf:\implies Power = \dfrac{50\: J}{2\: s}[/tex]

[tex]\sf:\implies \boxed{\bold{\:\:Power = 25\: W\:\:}}\:\:\:\green{\checkmark}[/tex]

Therefore, the power delivered by Jose when doing push-ups is 25 watts.

The wavelength of the sound wave, given that wave has a frequency of 35 Hz and travelling at 1500 m/s is 42.86 m

First, we shall list out the given parameters from the question. This is given below:

The wavelength of the sound wave can be obtained as illustrated below:

Velocity (v) = wavelength (λ) × frequency (f)

1500 = wavelength × 35

Divide both sides by 35

Wavelength = 1500 / 35

Wavelength = 42.86 m

Thus, from the above calculation, we can conclude that the wavelength of the sound wave is 42.86 m

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The force of gravity will be greater if one object has a larger mass than the other.

Gravity is the force of attraction between two objects with mass. According to Newton's law of gravitation, the force of gravity between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

F = G * (m₁ * m₂) / d²

where:

F = force of gravity

G = gravitational constant (a universal constant)

m₁, m₂ = masses of the two objects

d = distance between the two objects

As we can see from the formula, the force of gravity is directly proportional to the masses of the two objects. Therefore, if one object has a larger mass than the other, the force of gravity between them will be greater.

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The speed of the heavier mass as a function of their separation distance, r, can be expressed using the conservation of energy principle.

As the masses move toward each other due to gravitational attraction, their potential energy decreases and their kinetic energy increases, such that the total energy remains constant.

Therefore, we can write: 1/2 * m1 * [tex]v^{2}[/tex] = G * m1 * m2 / r

where m1 is the mass of the heavier object, m2 is the mass of the lighter object, v is the velocity of m1, r is the separation distance between the two objects, and G is the gravitational constant.

Solving for v, we get:

v = sqrt(2 * G * m2 / r)

This expression shows that as the separation distance r decreases, the velocity v of the heavier object increases due to the increasing gravitational attraction between the two masses.

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The statement is true.

If the particles ejected from the Sun during a coronal mass ejection (CME) are directed towards Earth, they can reach our planet.

Coronal mass ejections are powerful eruptions of plasma and magnetic field from the Sun's corona. These ejections can release a large amount of highly energetic particles, including protons, electrons, and ions, into space.

When a CME is Earth-directed, it can travel through the interplanetary medium, which includes the solar wind, and reach our planet. The time it takes for the CME to reach Earth can vary, but typically it ranges from a day to a few days.

When the CME particles interact with the Earth's magnetic field, they can cause a variety of effects, including geomagnetic storms and enhanced auroral displays. The charged particles from the CME can also interact with the Earth's magnetosphere, leading to disturbances in the ionosphere and potential disruptions in satellite communication, power grids, and other technological systems.

Scientists and space agencies closely monitor CMEs and their potential impact on Earth using spacecraft and ground-based observatories to provide early warnings and forecasts of their arrival.

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A girl carrying a 20 Kg box climbs up 10 steps, each 20 cm high, in 16 seconds. Her own mass is 50 Kg. Her weight is 490.5N. The weight of the box is 196.2 N. When the girl reaches the top, she has traveled a vertical height of 2 meters.

a. The girl's weight is given by the product of her mass and the acceleration due to gravity. Thus, her weight is:

Weight = mass x acceleration due to gravity

Weight = [tex]50 \;kg \times 9.81 \;m/s^2[/tex]

Weight = 490.5 N

b. The weight of the box is also given by the product of its mass and the acceleration due to gravity. Thus, its weight is:

Weight = mass x acceleration due to gravity

Weight = [tex]20 \;kg \times 9.81 \;m/s^2[/tex]

Weight = 196.2 N

c. The vertical height of each step is given as 20 cm or 0.2 m. Therefore, the total vertical height traveled by the girl is:

Total height = number of steps x height of each step

Total height = 10 steps x 0.2 m/step

Total height = 2 m

Hence, when the girl reaches the top, she has traveled a vertical height of 2 meters.

In summary, we calculated the weight of the girl and the box, and determined the vertical height traveled by the girl when she climbed a flight of 10 steps, each step 20 cm high, in 16 seconds.

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Expanding, aging stars become cooler and more luminous because an overproduction of energy causes the outer layers of gas to expand, whereby the energy is absorbed and the temperature increases.  the resulting increase in radiated energy leads to increased luminosity

Define luminosity.

The radiant power that a light-emitting device emits over time is known as luminosity, which is an absolute measure of radiated electromagnetic power. The entire quantity of electromagnetic energy that a star, galaxy, or other celestial object emits over the course of one unit of time is known as luminosity in astronomy.

While the star's core contracts, the outer layers expand, and as the expansion continues, the luminosity rises. The radius and luminosity of a star with the mass of the sun expand 100 times throughout this expansion, which takes place over the course of around a billion years.

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You would have to travel to a latitude of approximately 80.5 degrees north of the equator (or south, depending on your hemisphere) to see the noontime sun at your zenith on October 3rd.

To see the noontime sun at your zenith on October 3rd (or any other date), you would have to be located at a latitude equal to the complement of the Sun's declination on that date. The declination is the angle between the plane of the Earth's equator and the line connecting the Earth to the Sun, and it varies throughout the year due to the tilt of the Earth's axis of rotation.

On October 3rd, the Sun's declination is approximately 9.5 degrees south of the equator. To find the latitude at which the noontime Sun would be directly overhead, we take the complement of this declination, which is:

90 degrees - 9.5 degrees = 80.5 degrees

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If the current in a circuit is 3. 2 mA and the resistance of the wire used in the circuit is 250 Ω, the voltage of the fuel cell being used in the circuit is 0.8 volts.

To calculate the voltage of the fuel cell being used in a circuit, we can use Ohm's law, which states that the voltage (V) equals the current (I) multiplied by the resistance (R): V = I x R.

In this case, the current is 3.2 mA (milliamperes), and the resistance of the wire used in the circuit is 250 Ω (ohms). We first need to convert the current to amperes by dividing it by 1000: 3.2 mA ÷ 1000 = 0.0032 A.

Next, we can substitute these values into the formula to calculate the voltage: [tex]V = 0.0032 \;A \times 250 \;\Omega = 0.8 \;volts.[/tex]

Therefore, the voltage of the fuel cell being used in the circuit is 0.8 volts.

In summary, to calculate the voltage of a fuel cell being used in a circuit, we can use Ohm's law, which states that voltage equals current multiplied by resistance.

By converting the current from milliamperes to amperes and substituting the values into the formula, we can determine the voltage of the fuel cell in volts.

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The volume of the 400g bag of flour is 666.67 cm^3.

This question asks for the calculation of the volume of a 400g bag of flour with a density of 0.6 g/cm^3. The density of a material is defined as its mass per unit volume, and can be expressed mathematically as:

density = mass/volume.

Rearranging the equation to solve for volume, we get:

volume = mass/density.

Substituting the given values, we get:

Volume = 400 g / 0.6 g/cm^3

Solving for the volume, we get:

Volume = 666.67 cm^3
Volume = 400g / 0.6 g/cm^3, which simplifies to 666.67 cm^3.
Therefore, the volume of the 400g bag of flour is 666.67 cm^3.

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--The complete Question is, If a 400g bag of flour has a density of 0.6 g/cm^3, what is its volume in cm^3? --

The new volume of the gas when the temperature is raised to 29°C and the pressure is not changed is approximately :4.73 L. The correct option is A.

To determine the new volume of a gas when its temperature is changed, we can use Charles' Law. Charles' Law states that the volume of a gas is directly proportional to its temperature, provided that the pressure remains constant. Your initial temperature (T1) is 14°C, and the initial volume (V1) is 4.5 L.

The final temperature (T2) is 29°C, and we need to find the new volume (V2). Remember to convert the temperatures from Celsius to Kelvin by adding 273.15 to each value (T1 = 287.15 K, T2 = 302.15 K).

Using Charles' Law, we have:

V1/T1 = V2/T2

Now, we can plug in the values:

(4.5 L)/(287.15 K) = V2/(302.15 K)

To find V2, multiply both sides by 302.15 K:

V2 = (4.5 L x 302.15 K) / 287.15 K

V2 ≈ 4.73 L

The new volume of the gas when the temperature is raised to 29°C and the pressure is not changed is approximately 4.73 L. The correct option is A.

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Complete  question:

A gas has a temperature of 14 °C, and a volume of 4. 5 L. If the temperature is raised to 29 °C and the pressure is not changed, what is the new volume of the gas?

A. 4. 7 L

B. 4. 9 L

C. 5. 3 L

D. 5. 5 L

Answer:

The magnets are surrounded by an invisible magnetic field that contains stored-up, or potential, energy. When attempting to push two like-sided poles together, the stored-up energy becomes movement, or kinetic energy, and forces them apart. The same principle happens when two unlike poles come together.

Answer:

Your tortilla would weigh 75 grams total.

Explanation:

55 grams of flour + 20 grams of water = 75 grams total

The tortilla should have a mass of 75 grams.

A mixture is a combination of two or more substances that are not chemically bonded and can be separated by physical means. In a mixture, each substance retains its own chemical identity and properties. The properties of a mixture can vary depending on the relative amounts of the substances that are mixed together.

There are two main types of mixtures: homogeneous and heterogeneous.

1. Homogeneous mixtures: These are also called solutions, and they have a uniform composition throughout. The components of a homogeneous mixture are not visible to the bare eye and cannot be separated by simple mechanical means. Examples of homogeneous mixtures include salt water, sugar in water, and air.

2. Heterogeneous mixtures: These are mixtures that do not have a uniform composition throughout. The components of a heterogeneous mixture are visible to the bare eye, and they can be separated by mechanical means such as filtration, sedimentation, or decantation. Examples of heterogeneous mixtures include a mixture of oil and water, a salad, and a mixture of sand and pebbles.

Here in the Question,

The total mass of the tortilla will be the sum of the mass of flour and the mass of water used to make it. So, the tortilla should have a mass of:

55 grams (flour) + 20 grams (water) = 75 grams.

Therefore, the Total mass of the tortilla is 75 Grams.

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The charge that passes through the body during a 10-minute electrophoresis procedure with a current of: 8 mA is 4.8 Coulombs, and the current density value with an electrode area of 150x180 cm² is approximately 0.296 A/m².

The delivery of medicines to a specific organ or tissue in the human body using a direct current is known as electrophoresis. In this case, two oppositely charged plates are applied to the body.

(a) To find the charge that passes through the body during a 10-minute electrophoresis procedure with a current of 8 mA, you can use the formula: Charge (Q) = Current (I) × Time (t). Since the current is given in milliamperes (mA), you'll need to convert it to amperes (A) by dividing by 1,000: 8 mA / 1,000 = 0.008 A.

The time is given in minutes, so convert it to seconds: 10 minutes × 60 seconds/minute = 600 seconds. Now, you can find the charge: Q = 0.008 A × 600 s = 4.8 Coulombs.

(b) To find the current density, you'll need to use the formula: Current Density (J) = Current (I) / Area (A). The electrode area is given as 150 x 180 cm², so you need to convert it to square meters: (150 x 180 cm²) / (10,000 cm²/m²) = 0.027 m². Now you can find the current density: J = 0.008 A / 0.027 m² ≈ 0.296 A/m².

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The magnitude of the velocity is 0.0246 m/s and the direction of the velocity is directly north.

The magnetic force on a charged particle is the force experienced by a moving charged particle when it interacts with a magnetic field. When a charged particle moves through a magnetic field, it experiences a force that is perpendicular to both its velocity and the magnetic field direction. This force is known as the magnetic force or the Lorentz force.

The magnitude of the magnetic force is proportional to the charge of the particle, the magnitude of its velocity, and the strength of the magnetic field. The direction of the force is perpendicular to both the velocity vector and the magnetic field vector, following the right-hand rule.

It is given by the formula:

F = qvB

Where F is the force, q is the charge, v is the velocity, and B is the magnetic field.

F = 6.24 x 10⁻¹⁵ N (force)

q = -1.6 x 10⁻¹⁹ C (charge)

B = 1.56 T (magnetic field)

v = F / (qB)

v = (6.24 x 10⁻¹⁵ N) / (-1.6 x 10⁻¹⁹ C) / (1.56 T)

v = -0.0246 m/s

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There are 0.486 grams of magnesium in 0.02 moles of magnesium.

To calculate the grams of magnesium, you multiply the given moles (0.02 mol) by the molar mass (24.3 g/mol):

0.02 mol Mg × 24.3 g/mol Mg = 0.486 g Mg

Therefore, there are 0.486 grams of magnesium in 0.02 moles of magnesium.

It's important to note that molar mass allows us to convert between moles and grams. By multiplying the number of moles by the molar mass, we can determine the mass of the substance in grams.

This conversion is commonly used in chemistry to relate the quantity of a substance in moles to its corresponding mass in grams.

In this case, by multiplying the given moles (0.02 mol) of magnesium by the molar mass of magnesium (24.3 g/mol), we obtain the mass of magnesium in grams (0.486 g).

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The force does 4688.3 joules of work on the skater during this displacement.

The work done by a force on an object is defined as the product of the force and the displacement of the object in the direction of the force. In this problem, the displacement vector and the force vector are given.

To calculate the work done on the 82-kg skater during the displacement, you need to find the dot product of the force vector and the displacement vector. Here are the given vectors:

Force vector (F) = (182N) î + (121N) û
Displacement vector (d) = (13.2m) î + (18.9m) û

Work (W) = F • d = (182N * 13.2m) + (121N * 18.9m)

W = (2402.4 J) + (2285.9 J)

W = 4688.3 J

It is important to note that since the surface is frictionless, there is no loss of energy due to friction. This means that the work done by the force is equal to the change in the kinetic energy of the skater.

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We have detected planets in the habitable zone s not evidence against the discussion of the Fermi Paradox. Option B is correct.

The fp discussion refers to the Fermi Paradox, which is the apparent contradiction between the high probability of the existence of extraterrestrial civilizations and the lack of evidence for, or contact with, such civilizations. The presence of exoplanets in the habitable zone is actually evidence supporting the discussion of the Fermi Paradox, which asks why we haven't detected any signs of intelligent extraterrestrial life despite the high probability of its existence.

As the inability to observe exoplanets around most stars does not necessarily imply a contradiction with the Fermi Paradox. In fact, this limitation can be accounted for by understanding our observational capabilities and taking into account non-detections in our analysis. Option B is correct.

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Throughly explaining how all organisms are connected and need each other: involves understanding the concept of ecosystems and the various relationships among organisms.

All organisms on Earth are connected through a complex network of interactions in ecosystems. These ecosystems are composed of biotic factors (living organisms) and abiotic factors (non-living elements such as air, water, and soil). Organisms are linked through relationships like predation, competition, and symbiosis, which help maintain a balance in these ecosystems.

In a food chain, organisms are connected as they depend on one another for nutrition. Producers (such as plants) use sunlight to create energy through photosynthesis. Consumers (such as animals) consume the producers or other consumers to obtain energy. Decomposers (such as fungi and bacteria) break down dead organic matter and recycle nutrients back into the ecosystem.

Symbiotic relationships, such as mutualism, commensalism, and parasitism, further illustrate the interdependence of organisms. In mutualism, both species benefit from the relationship, such as bees pollinating flowers while collecting nectar. Commensalism involves one species benefiting without affecting the other, like a barnacle living on a whale's skin. In parasitism, one species benefits at the expense of another, such as a tick feeding on a mammal's blood.

Lastly, all organisms contribute to maintaining the delicate balance within an ecosystem. They help control population levels, recycle nutrients, and maintain overall biodiversity. A disruption in one organism's population can have cascading effects on the entire ecosystem, demonstrating the importance of their interconnectedness.

In summary, all organisms are connected and need each other through their roles in ecosystems, food chains, symbiotic relationships, and their contributions to maintaining balance.

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The first mass with a smaller mass would reach the bottom first due to its greater acceleration and less resistance from friction.

According to Newton's second law of motion, the acceleration of an object is directly proportional to the force applied on it and inversely proportional to its mass. Therefore, the object with the smaller mass would experience a greater acceleration than the object with the larger mass. In the scenario presented in the question, both masses are sliding down the same inclined surface with the same length and inclination. However, since the first object has a smaller mass, it would experience a greater acceleration and would therefore reach the bottom first.

Moreover, since the inclined surface is described as rough, there would be friction acting against the motion of the masses, slowing them down. However, the frictional force is also directly proportional to the normal force acting on the object. The normal force is the force exerted by the surface perpendicular to the object's surface. Therefore, the larger object would experience a greater normal force and consequently a greater frictional force, further slowing it down.

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