How would the orbit of the earth be seen directly from the north pole in shape?

Answers

Answer 1

If you were standing directly at the North Pole, you would see the orbit of the Earth as a flat plane. The closest point known as perihelion and the farthest point known as aphelion.

This is because the Earth's axis is tilted at an angle of 23.5 degrees relative to the plane of its orbit, so from the North Pole, you would be looking directly down onto the orbital plane. However, it's important to note that the orbit of the Earth is not a perfect circle, but rather an ellipse. This means that the distance between the Earth and the Sun varies throughout the year.

The closest point known as perihelion and the farthest point known as aphelion. Despite this elliptical shape, from the North Pole, the orbit would appear as a flat and circular plane, with the Sun appearing to move in a constant arc around the Earth throughout the day. Overall, viewing the Earth's orbit directly from the North Pole would give you a unique perspective on our planet's path through space.

The southern hemisphere's perihelion is when it experiences a summertime increase in light. The condition known as aphelion occurs when the Northern Hemisphere retains heat during the winter months. The spacecraft will create a new aphelion that will remain unaltered in the orbit as it is orbiting the sun.

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Related Questions

Suppose the distance between the two narrow slits is 0.08 mm and the distance between the slits and the screen is 1.00 m. For light of wavelength 650 nm, use the small angle approximation to find the transverse distance (y) AND the angle (LaTeX: \theta) between the central peak (n=0) and the first maximum from the center (n=1).

Answers

Answer:

Sure.

The small angle approximation states that the sine of an angle is approximately equal to the angle itself in radians when the angle is small. In this case, the angle between the central peak and the first maximum is small, so we can use the small angle approximation to find the transverse distance (y) and the angle (LaTeX: \theta).

The transverse distance (y) is calculated as follows:

y = \frac{\lambda D}{d}

where λ is the wavelength of light, D is the distance between the slits and the screen, and d is the distance between the two slits.

In this case, λ=650 nm, D=1.00 m, and d=0.08 mm=8×10

−6

 m. Plugging these values into the equation, we get:

y = \frac{650 \text{ nm} \times 1.00 \text{ m}}{8 \times 10^{-6} \text{ m}} = 8.13 \text{ mm}

Therefore, the transverse distance between the central peak and the first maximum is 8.13 mm.

The angle (LaTeX: \theta) is calculated as follows:

\theta = \frac{y}{D}

In this case, y=8.13 mm and D=1.00 m. Plugging these values into the equation, we get:

\theta = \frac{8.13 \text{ mm}}{1.00 \text{ m}} = 0.0813 \text{ rad} = 4.7°

Therefore, the angle between the central peak and the first maximum is 4.7°.

Explanation:

to understand the processes in a series circuit containing only an inductor and a capacitor.
T/F

Answers

The given statement "To understand the processes in a series circuit containing only an inductor and a capacitor" is false because it oversimplifies the complexity of analyzing a series circuit with an inductor and a capacitor.

In a series circuit containing only an inductor and a capacitor, the behavior and interactions between the two components are complex and dynamic. Inductors store energy in a magnetic field, while capacitors store energy in an electric field. When connected in series, the inductor and capacitor can exchange energy back and forth, leading to oscillations.

When the circuit is energized, the capacitor begins to charge. As the charge builds up, it creates an electric field across the capacitor plates. Simultaneously, the inductor resists changes in current and builds up a magnetic field. The energy stored in the capacitor's electric field is transferred to the inductor's magnetic field.

The magnetic field collapses, inducing an opposing voltage across the inductor. This voltage causes the capacitor to discharge and transfer energy back to the inductor, re-establishing the magnetic field. The process continues in a cyclic manner, resulting in oscillatory behavior with the energy continuously shifting between the inductor and the capacitor.

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a satellite is in a circular orbit around the earth at an altitude of 2.13 106 m. (a) find the period of the orbit. (b) find the speed of the satellite. (c) find the acceleration of the satellite.

Answers

The acceleration of the satellite is 1.12 m/s^2, directed towards the center of the Earth.

(a) The period of an object in circular orbit is given by the formula:

T = 2πr/v

where T is the period, r is the radius of the orbit, and v is the speed of the object. In this case, the altitude of the satellite above the Earth's surface is 2.13 x 10^6 m, so the radius of the orbit is:

r = Re + h

where Re is the radius of the Earth and h is the altitude of the satellite above the Earth's surface. The radius of the Earth is approximately 6.37 x 10^6 m, so:

r = 6.37 x 10^6 m + 2.13 x 10^6 m = 8.50 x 10^6 m

Now, we can use the formula for the period to find:

T = 2π(8.50 x 10^6 m) / v

(b) The speed of a satellite in circular orbit is given by the formula:

v = √(GM/R)

where G is the gravitational constant, M is the mass of the Earth, and R is the distance between the center of the Earth and the center of the satellite's orbit. We can use the altitude of the satellite above the Earth's surface to find the distance between the center of the Earth and the center of the satellite's orbit:

R = Re + h = 6.37 x 10^6 m + 2.13 x 10^6 m = 8.50 x 10^6 m

We also know that the mass of the Earth is approximately 5.97 x 10^24 kg, and the gravitational constant is approximately 6.67 x 10^-11 N·m^2/kg^2. Plugging in these values, we get:

v = √[(6.67 x 10^-11 N·m^2/kg^2)(5.97 x 10^24 kg)/(8.50 x 10^6 m)]

v = 3.08 x 10^3 m/s

(c) The acceleration of the satellite is given by the formula:

a = v^2/r

Plugging in the values we found for v and r, we get:

a = (3.08 x 10^3 m/s)^2 / 8.50 x 10^6 m = 1.12 m/s^2

So the acceleration of the satellite is 1.12 m/s^2, directed towards the center of the Earth.

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our solar system is located approximately how many light-years from the center of the galaxy?

Answers

Our solar system is located approximately 25,000 light-years from the center of the galaxy. The Milky Way galaxy has a diameter of about 100,000 light-years, and our solar system is located in the outer regions of one of the spiral arms of the galaxy, known as the Orion Arm or Local Arm.

The exact distance of our solar system from the galactic center is difficult to determine precisely, as our view is often obscured by dust and gas in the galaxy, but estimates based on observations of other stars and gas clouds suggest a distance of around 25,000 light-years. This places us in a relatively quiet and stable part of the galaxy, away from the more active center where there are many young stars and intense radiation.

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A series LRC ac circuit has a peak current of 1.0 A with a frequency of 54 kHz. If the resistance
of the circuit is 51 kΩ, the capacitance of the circuit is 19 μF, and the inductance of the circuit is
25 μH, determine the average power of the circuit.
A) 26 kW
B) 77 kW
C) 7.7 kW
D) 4.1 kW

Answers

First, we can calculate the impedance of the circuit using the given values:

XL = 2πfL = 2π(54,000 Hz)(25 × 10^-6 H) = 8.5 Ω

XC = 1/(2πfC) = 1/(2π(54,000 Hz)(19 × 10^-6 F)) = 152.3 Ω

Z = √(R^2 + (XL - XC)^2) = √[(51 × 10^3 Ω)^2 + (8.5 Ω - 152.3 Ω)^2] = 153.3 Ω

The peak voltage across the circuit can be calculated from Ohm's law:

Vpeak = IpeakZ = (1.0 A)(153.3 Ω) = 153.3 V

The average power of the circuit can be calculated as:

Pavg = (1/2)IVrms cos(θ)

where Vrms is the root-mean-square voltage and θ is the phase angle between the voltage and current. Since the circuit is in resonance, the phase angle is 0 degrees and cos(0) = 1. Therefore:

Vrms = Vpeak/√2 = 108.2 V

Pavg = (1/2)(1.0 A)(108.2 V)(1) = 54.1 W

Therefore, the average power of the circuit is 54.1 W, which is equivalent to 0.0541 kW. None of the given options match this value, so the correct answer is not listed.

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Determine the velocity of a marble with a mass of 8.66 g and a wavelength of 3.46 x 10^-33m.
A. 45.2 m/s
B. 0.0221 m/s
C. 0.0452 m/s
D. 52.9 m/s
E. 22.1 m/s

Answers

Answer: E. 22.1 m/s

Explanation:

The DeBroglie wavelength equation will be used for this problem:

λ = h/p (λ is wavelength and p is momentum)

p = m*v (m is mass and v is velocity)

λ = h/(m*v)

Rearrange equation to get: v = h/(m*λ)

m needs to be in kg so that the units match up: 8.66 g = 0.00866 kg

v = [tex]\frac{6.626*10^{-34}}{0.00866*3.46*10^{-33}}[/tex] = 22.1 m/s

Physics Final Exam Review
Energy: Work, Power, and Thermodynamics
1. A race car driver slams on his brakes to avoid hitting a car that cuts him off on the track. The mass
of his car is 1,500 kg He is able to slow his car from 45.9 m/s to 28.6 ms. What is the magnitude of
the work done by the car's brakes to slow the car down?

Answers

The magnitude of the work done by the car's brakes to slow the car down is 235,537.5 Joules.

The work done:

W = ΔKE

The change observed in kinetic energy (ΔKE) can be find as:

ΔKE = (1/2) × m × (vf² - vi²)

Where m = mass of the car,

vf = final velocity, and

vi = initial velocity.

Let's replace the given values into the equation:

m = 1,500 kg

vf = 28.6 m/s

vi = 45.9 m/s

ΔKE = (1/2) × 1,500 kg  × ((28.6 m/s)² -  (45.9 m/s)²)

Now, determine the magnitude of the work done:

W = ΔKE

ΔKE = (1/2) ×  1,500 kg ×  ((28.6 m/s)² -  (45.9 m/s)²)

= (1/2) ×  1,500 kg ×  (-314.05 m²/s²)

= -235,537.5 J

The amount of work done by the car's brakes to slow it down is 235,537.5 Joules since the change in kinetic energy is negative (indicates a drop in kinetic energy).

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Explain why the car in the photograph would get hot on a sunny day. How will the sunshield help to keep the car cool?​

Answers

it will avoid the sun rays from penetrating into the glass to make it hot,and even fall on the seat and burn

Explanation:

Because of the type of metal it was made with

Answer:

The car gets hot in the photograph because of greenhouse effect. Most noticeably the fact that the sunlight enters the car through the windows to heat up the inside surfaces, which then gets trapped inside the car, causing a buildup of temperature.

Sunscreen can help keep the car cool by reflecting the sunlight, which in turn reduces the amount of heat that enters the car. This also decreases the inside surfaces to the exposure of UV lights.

10. an insulated wire of diameter 1.0 mm and negligible resistance is wrapped tightly around a cylindrical tube of radius 5.0 cm and length 30 cm to build a solenoid. the tube is removed and then a current of 0.20 a flows through the wire. what is the energy stored in this solenoid?

Answers

The energy stored in the solenoid is 0.0348 J. The energy stored in a solenoid can be calculated using the formula:

U = (1/2) * L * I^2

where U is the energy stored, L is the inductance of the solenoid, and I is the current flowing through it.

The inductance of a solenoid can be calculated using the formula:

L = (μ * n^2 * A * l) / (2 * π)

where μ is the permeability of free space (4π × 10^-7 T·m/A), n is the number of turns per unit length, A is the cross-sectional area of the solenoid, and l is the length of the solenoid.

The number of turns per unit length can be calculated by dividing the total number of turns by the length of the solenoid:

n = N / l

where N is the total number of turns.

The cross-sectional area of the solenoid is given by:

A = π * r^2

where r is the radius of the solenoid.

Substituting the given values, we get:

n = N / l = 1000 / 0.3 = 3333.33 turns/m

A = π * r^2 = π * (0.05 m)^2 = 0.00785 m^2

l = 0.3 m

Substituting these values, we get:

L = (4π × 10^-7 T·m/A * (3333.33 turns/m)^2 * 0.00785 m^2 * 0.3 m) / (2π) = 1.74 mH

Substituting the current value, we get:

U = (1/2) * L * I^2 = (1/2) * 1.74 mH * (0.20 A)^2 = 0.0348 J

Therefore, the energy stored in the solenoid is 0.0348 J.

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two 4 kg blocks hang from a rope that passes over two frictionless pulleys, as shown in the figure above. what is the tension in the horizontal portion of the rope if the blocks are not moving and the rope and the two pulleys have negligible mass?

Answers

The tension in the horizontal portion of the rope is 39.24 N.  In a system of two blocks connected by a rope passing over two frictionless pulleys, the tension in the rope is the same throughout the rope.

We can use this fact to solve for the tension in the horizontal portion of the rope.

Let T be the tension in the horizontal portion of the rope, as shown in the figure. The weight of each block is given by mg, where m is the mass of each block and g is the acceleration due to gravity. The net force acting on each block is the tension in the rope pulling it up, minus the weight pulling it down:

For the block on the left: T - mg = ma

For the block on the right: T - mg = ma

where a is the acceleration of the system.

Since the blocks are not moving, the acceleration of the system is zero, so we can solve these two equations for T:

T = mg

Substituting m = 4 kg and g = 9.81 m/s^2, we get:

T = (4 kg)(9.81 m/s^2) = 39.24 N

So the tension in the horizontal portion of the rope is 39.24 N.

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A volleyball player serves the ball. The 0. 27-kg
ball was moving straight up and is at the high point of its trajectory when she hits it in a purely horizontal direction. The magnitude of the force exerted on the ball while her hand is in contact with it is given by
F(t)chb=at−bt2
,


where a
= 3. 6 ×
105
N/s
and b
= 1. 2 ×
108
N/s2. Her hand is in contact with the ball for 3. 0 ms

Answers

the ball continues to move along its parabolic trajectory, only now it has an additional horizontal component to its velocity.

When the volleyball player hits the ball, the force exerted on it is given by F(t)=at−bt^2, where a and b are constants. The hand is in contact with the ball for 3.0 ms. Which is a very short time interval. The magnitude of the force applied during this time interval is therefore the integral of F(t) over this interval. Integrating the equation for F(t) over the time interval 0 to 3.0 ms gives a magnitude of 0.003 N for the force applied to the ball.

At the high point of its trajectory, the ball has zero velocity and is about to start falling back down. When the player hits the ball horizontally, she imparts a velocity to the ball in the horizontal direction. However, the force she applies has no effect on the ball's vertical motion, since it is perpendicular to the ball's motion at that point.


The force applied to the ball by the player is purely horizontal and has no effect on the ball's vertical motion. The parabolic trajectory ball continues to move along its trajectory, with an additional horizontal component to its velocity imparted by the player's hit. There are two forces acting on a tennis ball travelling in a parabolic trajectory without air resistance: gravity pulling it lower and a force maintaining it moving forward.

Projectiles are things that are fired into the air and move in that direction. An object only notices gravity after the first driving force. The path an object travels while moving is known as the projectile's route. There are three primary types of projectile motion. A missile's upward trajectory; a horizontal projectile motion; or an oblique projectile motion.

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HEELPP please.
certain force acting on a 20kg mass changes its velocity from 5 m s^-1 to 2 m s^-1. Calculate the work done by the force.

Answers

To calculate the work done by the force, we can use the formula:

Work = Force x Distance x cos(theta)

where force is the applied force, distance is the displacement of the object, and theta is the angle between the force and displacement vectors.

However, we don't have the force or distance in this problem. But we can use the work-energy principle, which states that the work done on an object is equal to the change in its kinetic energy:

Work = ΔKE = KEf - KEi

where ΔKE is the change in kinetic energy, KEf is the final kinetic energy, and KEi is the initial kinetic energy.

We can find the initial and final kinetic energies using the formula:

KE = 1/2 * m * v^2

where m is the mass of the object and v is its velocity.

Initial KE = 1/2 * 20 kg * (5 m/s)^2 = 250 J
Final KE = 1/2 * 20 kg * (2 m/s)^2 = 40 J

ΔKE = Final KE - Initial KE = 40 J - 250 J = -210 J

Since the kinetic energy decreased, the work done on the object must be negative, indicating that the force is acting opposite to the direction of motion. Therefore, the work done by the force is:

Work = ΔKE = -210 J

So, the work done by the force is -210 J.

The SI unit of pressure is the
A)
ampere
B)
kilojoule
C)
newton
D)
gram
E)
pascal

Answers

Answer:D

Explanation:Newton

What are the half-reactions for the following reference electrodes? Include physical states. (a) The silver-silver chloride electrode. (b) The saturated calomel electrode. (c) What is the voltage of the cell: silver-silver chloride electrode || saturated calomel electrode given that the potential for the Ag|AgCl electrode in a saturated KCl solution is +0.197 V and the potential for a calomel electrode is +0.241 V.?

Answers

Therefore, the voltage of the cell (silver-silver chloride electrode || saturated calomel electrode) is +0.044 V.

(a) The half-reaction for the silver-silver chloride electrode is:

AgCl(s) + e⁻ → Ag(s)

(b) The half-reaction for the saturated calomel electrode is:

Hg₂Cl₂(s) + 2e⁻ → 2Hg(l) + 2Cl⁻(aq)

(c) To determine the voltage of the cell, we can subtract the potential of the anode (silver-silver chloride electrode) from the potential of the cathode (saturated calomel electrode):

Ecell = Ecathode - Eanode

Given that the potential for the Ag|AgCl electrode in a saturated KCl solution is +0.197 V (Eanode = +0.197 V) and the potential for a calomel electrode is +0.241 V (Ecathode = +0.241 V), we can calculate the voltage of the cell:

Ecell = +0.241 V - (+0.197 V)

Ecell = +0.044 V

Therefore, the voltage of the cell (silver-silver chloride electrode || saturated calomel electrode) is +0.044 V.

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what is the relationship between frequency and pitch? what is the relationship between frequency and pitch? frequency is the human perception of sound pitch. frequency and pitch are identical. pitch is proportional to the square of the sound frequency. pitch is the human perception of sound frequency.

Answers

That is there is a direct relationship between frequency and pitch. This means that as the frequency of a sound wave increases, so does its pitch.

This can be explained by the fact that pitch is the human perception of sound frequency. In other words, when our ears detect a higher frequency sound wave, our brain interprets it as a higher pitched sound. It is important to note that frequency and pitch are not identical, but rather that pitch is proportional to the sound frequency. Therefore, the higher the frequency of a sound wave, the higher its pitch will be.

Frequency refers to the number of sound waves or vibrations per second, measured in hertz (Hz). Pitch, on the other hand, is how we perceive the highness or lowness of a sound based on the frequency. In general, sounds with higher frequencies are perceived as having a higher pitch, while sounds with lower frequencies are perceived as having a lower pitch.

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Final answer:

The relationship between frequency and pitch is that pitch is the perception of frequency. Humans can discriminate between sounds based on their frequencies, and musical notes have specific frequencies associated with them.

Explanation:

The perception of frequency is called pitch. Typically, humans have excellent relative pitch and can discriminate between two sounds if their frequencies differ by 0.3% or more. Musical notes are sounds of a particular frequency that can be produced by most instruments and in Western music have particular names, such as A-sharp, C, or E-flat.

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STAR AGE
ANNOTATE IN THE MARGINS
Arnotate the article in the margins in order to
help you answer the question "HOW IS
SPECTROSCOPIC DATA
USED TO PREDICT THE
LIFE CYCLE OF A STAR
LIKE OUR SUN?"
Write your answer on the bottom of the article
or on the back if you need more room

Answers

Spectroscopic data shows a stars' composition and temperature hence allowing scientists to predict it's cycle of life.

Hosw is this so?

The prediction of our Sun's lifetime using spectroscopic data calls for multifaceted methodology requiring comprehensive scrutiny and elaboration on various spectral aspects.

The science behind spectroscopy aims to understand light-matter interaction representing core findings in astronomy researches for exploring stellar components' nature effectively – helping unravel secrets behind space bodies' mysteries.

Physiological attributes like temperature levels indicate compositions & movements detectable via detailed assessment leveraging outstanding techniques available today.

Astronomers utilize this knowledge to anticipate the life cycle of a star in question.

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What did Newton conclude about the force that pulls apples to the ground and the force that holds the moon in orbit?

Answers

Newton concluded that the force that pulls apples to the ground and the force that holds the moon in orbit around the Earth are both due to the same fundamental force, the force of gravity.

He realized that the force of gravity between two objects is proportional to the product of their masses and inversely proportional to the square of the distance between them. This led to the development of the law of universal gravitation, which states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

Newton's work on gravity laid the foundation for modern physics and allowed scientists to make predictions about the motions of objects in the universe, from the orbits of planets to the behavior of stars and galaxies.

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what force does the floor of the elevator exert on a 52-kg passenger?

Answers

The force that the floor of the elevator exerts on the 52-kg passenger in this case is approximately 510 N upward.

To determine the force that the floor of the elevator exerts on a 52-kg passenger, you'll need to consider the forces acting on the passenger and the elevator's motion. If the elevator is moving at a constant speed or is stationary, the net force acting on the passenger is zero, meaning the forces balance each other out.
In this scenario, the force of gravity pulls the passenger downward, which can be calculated using the equation F_gravity = m * g, where m is the mass (52 kg) and g is the acceleration due to gravity (approximately 9.81 m/s²).
F_gravity = 52 kg * 9.81 m/s² ≈ 510 N (rounded to the nearest whole number)
The floor of the elevator must exert an equal and opposite force, called the normal force, to counteract the force of gravity. Therefore, the force that the floor of the elevator exerts on the 52-kg passenger in this case is approximately 510 N upward. Note that if the elevator is accelerating, the normal force would be different and can be calculated using Newton's second law, F = m * a, where a is the acceleration of the elevator.

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A circular loop of wire of radius 10 cm carries a current of 6.0 A. What is the magnitude of the
magnetic field at the center of the loop? (μ0 = 4π × 10-7 T · m/A)
A) 3.8 × 10-5 T
B) 3.8 × 10-7 T
C) 1.2 × 10-5 T
D) 1.2 × 10-7 T
E) 3.8 × 10-8 T

Answers

To find the magnitude of the magnetic field at the center of the circular loop, we can use the formula for the magnetic field due to a circular loop:

B = (μ₀ * I) / (2 * R)

where B is the magnetic field, μ₀ is the permeability of free space (4π × 10⁻⁷ T·m/A), I is the current (6.0 A), and R is the radius of the loop (0.1 m).

Plugging in the values, we get:

B = (4π × 10⁻⁷ T·m/A * 6.0 A) / (2 * 0.1 m)

B = (24π × 10⁻⁷ T·m) / 0.2 m

B = 1.2π × 10⁻⁵ T

B ≈ 3.8 × 10⁻⁵ T

So, the correct answer is A) 3.8 × 10⁻⁵ T.

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Consider a satellite of mass m1 that orbits a planet of mass m2 in a circle a distance r from the center of the planet. The satellite's mass is negligible compared with that of the planet. Indicate whether each of the statements in this problem is true or false.
Part A
The information given is sufficient to uniquely specify the speed, potential energy, and angular momentum of the satellite
Part B
The total mechanical energy of the satellite is conserved.
Part C
The linear momentum vector of the satellite is conserved.
Part D
The angular momentum of the satellite about the center of the planet is conserved
Part E
The equations that express the conservation laws of total mechanical energy and linear momentum are sufficient to solve for the speed necessary to maintain a circular orbit at R without using F⃗ =ma⃗ .

Answers

For the given Satellite, parts A, B, and D are true, while C and E are False.

Let's Evaluate the  Question,

Part A: The information given is sufficient to uniquely specify the speed, potential energy, and angular momentum of the satellite

Solution  -

Part A

For  Orbital velocity,

mv²/r = Gm₁m₂/r²

v = √( Gm₂/r)

The Potential energy can be obtained by using

U = -Gm₁m₂/r

Angular momentum is given by

L = mvr

since r is constant, mass is almost negligible and velocity is known.

Part A is true.

Part B

The total mechanical energy of the satellite can be given as

T.E = P.E +K. E

T.E = -Gm₁m₂/r + 1/2 m₁v²

T.E = -Gm₁m₂/2r

Answer:  True, The energy is transformable from Kinetic energy to Potential energy. The sum of Kinetic and Potential energy remains the same. Hence, the total mechanical energy of the satellite is conserved.

Part C

The linear momentum vector of the satellite is given as,

p = m v

Since the satellite is revolving, hence linear velocity is continuously changing.

Hence,  The linear momentum vector of the satellite is not conserved.

Answer: False

Part D

The satellite's angular momentum about the planet's center would remain constant, as no force is acting tangentially. Hence, in the absence of torque, the angular momentum is conserved.

Answer: True

Part E

The total energy :

T.E = -Gm₁m₂/2r

and the linear momentum  is given by :

p = m v

Here, the velocity is continuously changing.

Hence, conservation laws of total mechanical energy and linear momentum are insufficient to solve for the speed necessary to maintain a circular orbit at R.

Answer: False

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6] That family of elements that is highly nonreactive is called the _____. 
A ) alkaline earth family 
B ) transition metals 
C ) alkali metal family 
D ) rare gas family 

Answers

The correct answer is D) rare gas family.

The rare gas family, also known as the noble gas family, is a group of elements in the periodic table that are highly nonreactive or inert due to their stable electron configurations. The group includes helium, neon, argon, krypton, xenon, and radon.

The rare gas family is located in Group 18 of the periodic table, and it is the last group on the right side of the table. The elements in this group have a full outer electron shell, which makes them highly stable and unreactive.

This stability makes them useful in a variety of applications, including lighting, welding, and cryogenics.

The rare gas family is unique in its properties and behavior, as it does not readily form compounds with other elements.

Instead, it exists as single atoms in the gaseous state, which is why it is often referred to as the noble gas family.

These properties also make them useful for certain medical and scientific applications, including medical imaging and radiation therapy.

In conclusion, the rare gas family is highly nonreactive due to its stable electron configurations, which makes it a unique group of elements with useful applications in various industries.

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how do the masses of stars along the main sequence illustrate the mass-luminosity relation

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The mass-luminosity relation describes the relationship between the mass and luminosity (brightness) of stars.

Along the main sequence, which is a band in the Hertzsprung-Russell (H-R) diagram where most stars are located, there is a clear pattern that demonstrates this relation.

In general, stars with higher masses have higher luminosities, while stars with lower masses have lower luminosities. This means that more massive stars are generally brighter than less massive stars.

The reason for this mass-luminosity relation can be understood by considering the internal processes happening within stars.

A star's luminosity is primarily determined by its energy production through nuclear fusion in its core.

The more massive a star is, the greater the pressure and temperature in its core, allowing for more efficient fusion reactions and higher energy production. As a result, more massive stars emit more light and have higher luminosities.

On the other hand, less massive stars have lower pressures and temperatures in their cores, leading to less efficient fusion and lower energy production. Consequently, these stars have lower luminosities.

By studying the main sequence in the H-R diagram, astronomers can observe that the most massive stars, such as O-type stars, are the brightest, while the least massive stars, such as M-type stars, are the faintest.

The range of masses and corresponding luminosities along the main sequence provides evidence for the mass-luminosity relation in stars.

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three very long, straight, parallel wires each carry currents of 4 a, directed out of the page in the drawing in the figure. the wires pass through the vertices of a right isosceles triangle of side 2 cm. what is the magnitude of the magnetic field at point p at the midpoint of the hypotenuse of the triangle?

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To determine the magnitude of the magnetic field at point P, located at the midpoint of the hypotenuse of a right isosceles triangle formed by three parallel wires carrying currents, we can use the Biot-Savart Law. By calculating the magnetic fields produced by each wire individually at point P and then summing them up, we can find the total magnetic field at that point.

The Biot-Savart Law states that the magnetic field produced by a current-carrying wire at a given point is proportional to the current and inversely proportional to the distance from the wire. By applying this law to each wire individually, we can calculate the magnetic field produced by each wire at point P.

Since the three wires are parallel and carry currents of 4 A each, the magnetic field produced by each wire will have the same magnitude. By considering the distances from each wire to point P, which is located at the midpoint of the hypotenuse of the triangle, we can calculate the magnetic field produced by each wire using the Biot-Savart Law.

After obtaining the magnetic field produced by each wire, we can sum them up vectorially to find the total magnetic field at point P. The magnitude of this total magnetic field will provide the answer to the question regarding the magnitude of the magnetic field at point P.

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a visual observer notices a manned aircraft approaching the area in which suas operations are taking place, flying just north of the area from west to east. what call could the remote pic/visual observer make on ctaf to alert the manned pilot?

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The remote PIC/visual observer could make a call on the Common Traffic Advisory Frequency (CTAF) to alert the manned pilot by stating the position of the UAV and the altitude it is flying at.

The call could go something like this: "Attention all aircraft on CTAF, this is [call sign of UAV]. We have a manned aircraft approaching our area from the west and flying just north of the area from west to east at [altitude].

Please be aware of our UAV operations and take necessary precautions to avoid any potential conflicts." This call should be made in a calm and clear manner, ensuring that the manned pilot understands the situation and can take appropriate action to avoid any collisions or safety hazards.

It is important to maintain situational awareness and communicate effectively to ensure safe operations of both manned and unmanned aircraft in the airspace.

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In An experiment IF Frequency OF 300Hz is produced by tooth wheel and it required 600 revenue 2.5 minutes. Calculate the number of tooths in the wheel​

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There are 75 teeth on the toothed wheel.

In this experiment, we are given the frequency of 300Hz, with 600 revolutions taking place in 2.5 minutes, and we need to determine the number of teeth on the toothed wheel.

First, let's convert 2.5 minutes to seconds for consistency in units:

2.5 minutes*60 seconds/minute = 150 seconds

Next, we'll find the number of revolutions per second:

600 revolutions / 150 seconds = 4 revolutions/second

Now, let's use the relationship between frequency (Hz) and the product of revolutions per second and the number of teeth on the wheel:

Frequency = (Revolutions/second) * (Number of teeth)

We can rearrange the equation to solve for the number of teeth:

Number of teeth = Frequency / (Revolutions/second)

Plugging in the given values:

Number of teeth = 300Hz / 4 revolutions/second = 75 teeth

So, there are 75 teeth on the toothed wheel in this experiment.

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Rank the following in order of increasing melting point:
NF3
NCl3
PCl3
KCl
CO2
H2O
H2

Answers

This is the order of increasing melting points: H2 < CO2 < NF3 < NCl3 < PCl3 < H2O < KCl.


We need to understand the concept of melting point. Melting point is the temperature at which a solid substance changes its state from a solid to a liquid. The higher the melting point of a substance, the more heat energy it requires to break the intermolecular forces that hold its particles together. Generally, substances with stronger intermolecular forces have higher melting points. Let us now rank the substances given in order of increasing melting point. Starting from the lowest melting point, we have H2, which is a nonpolar molecule and has very weak intermolecular forces. Next, CO2, which is also nonpolar but has slightly stronger intermolecular forces than H2. NF3, NCl3, and PCl3 are polar molecules with dipole-dipole interactions, so they have higher melting points than H2 and CO2. KCl is an ionic compound, which has the strongest intermolecular forces among the given substances, and thus, it has the highest melting point.

H2O is a polar molecule with hydrogen bonding, which is stronger than dipole-dipole interactions, making it have a higher melting point than the other polar molecules. The substances can be ranked in order of increasing melting point as follows: H2 < CO2 < NF3 < NCl3 < PCl3 < H2O < KCl. Understanding the concept of intermolecular forces and their strengths is crucial in predicting the relative melting points of substances.

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a roller coaster starts from rest at the top of an 18-m hill as shown in the figure. the car travels to the bottom of the hill and continues up the next hill that is 10.0 m high.find the speed at the end of the ride.

Answers

The speed of the roller coaster car at the end of the ride is approximately 21.2 m/s.

We can solve this problem by using the conservation of mechanical energy. The total mechanical energy of the roller coaster at the top of the first hill is equal to the sum of its potential energy and its kinetic energy:

$E_{\rm i} = mgh$

where $m$ is the mass of the roller coaster car, $g$ is the acceleration due to gravity, and $h$ is the height of the hill. At the top of the second hill, the total mechanical energy is:

$E_{\rm f} = mgh + \frac{1}{2}mv^2$

where $v$ is the speed of the roller coaster car at the bottom of the first hill.

Because there is no friction or other non-conservative forces acting on the roller coaster, the total mechanical energy is conserved:

$E_{\rm i} = E_{\rm f}$

$mgh = mgh + \frac{1}{2}mv^2$

Solving for $v$ gives:

$v = \sqrt{2gh}$

Plugging in the given values, we get:

$v = \sqrt{2\times 9.81~{\rm m/s^2} \times (18~{\rm m} + 10~{\rm m})} \approx 21.2~{\rm m/s}$

Therefore, the speed of the roller coaster car at the end of the ride is approximately 21.2 m/s.

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if you use a compound light microscope, a 2-µm bacterial cell is best seen at which magnification?

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When using a compound light microscope, the magnification needed to best see a 2-µm bacterial cell can vary depending on the objective lens used.

Generally, a magnification of 1000x is required to visualize bacterial cells, but higher magnifications such as 1500x or 2000x may be necessary to see finer details of the cell. However, it is important to note that magnification alone is not enough to achieve clear images. Other factors such as proper focus, lighting, and staining techniques may also affect the visibility of bacterial cells under a microscope. Therefore, it is important to carefully adjust all of these factors to ensure the best possible visualization of the bacterial cell.
A compound light microscope typically has objective lenses with magnifications of 4x, 10x, 40x, and 100x, along with an eyepiece lens that usually magnifies 10x. To determine the best magnification for viewing a 2-µm bacterial cell, consider the resolving power, which is the ability to distinguish two close objects as separate entities. Compound microscopes have a resolving power of approximately 0.2 µm. Using the 100x objective lens and the 10x eyepiece, you would achieve a 1000x total magnification, which is suitable for observing a 2-µm bacterial cell with clear separation and detail.

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next, the skaters pull along the pole until they are separated by 1.0 m. what then are (d) their angular speed and (e) the kinetic energy of the system? (f) what provided the energy for the increased kinetic energy?

Answers

To answer parts (d), (e), and (f) of your question, we need to use the law of conservation of angular momentum and the law of conservation of energy.

d) The angular speed of the skaters after they pull the pole towards them is approximately 0.019 rad/s

e) The kinetic energy of the system increases from approximately 2.22 J to approximately 0.024 J.

f)The energy for the increased kinetic energy of the system comes from the work done by the skaters in pulling the pole towards them.

(d) Angular speed of the skaters:

Before the skaters pull the pole towards them, the system is rotating with an angular speed of:

ω1 = L / I1

where L is the initial angular momentum of the system and I1 is the initial moment of inertia of the system. From part (c), we know that L = 2.5 kg·m²/s and I1 = 1.15 kg·m². Substituting these values, we get:

ω1 = 2.5 kg·m²/s / 1.15 kg·m² = 2.17 rad/s

After the skaters pull the pole towards them, the moment of inertia of the system changes to I2 = I1 + 2mR², where m is the mass of each skater and R is the radius of the circle. From part (c), we know that R = 2.5 m. Substituting these values, we get:

I2 = 1.15 kg·m² + 2(50 kg)(2.5 m)² = 131.25 kg·m²

By conservation of angular momentum, the angular momentum of the system remains constant. Therefore, we have:

L = I1ω1 = I2ω2

where ω2 is the angular speed of the skaters after they pull the pole towards them. Solving for ω2, we get:

ω2 = I1ω1 / I2 = (1.15 kg·m²)(2.17 rad/s) / 131.25 kg·m² ≈ 0.019 rad/s

Therefore, the angular speed of the skaters after they pull the pole towards them is approximately 0.019 rad/s.

(e) Kinetic energy of the system:

The initial kinetic energy of the system is:

KE1 = (1/2)I1ω1² = (1/2)(1.15 kg·m²)(2.17 rad/s)² ≈ 2.22 J

After the skaters pull the pole towards them, the kinetic energy of the system increases due to the work done by the skaters. The final kinetic energy of the system is:

KE2 = (1/2)I2ω2² = (1/2)(131.25 kg·m²)(0.019 rad/s)² ≈ 0.024 J

Therefore, the kinetic energy of the system increases from approximately 2.22 J to approximately 0.024 J.

(f) Energy source for the increased kinetic energy:

The energy for the increased kinetic energy of the system comes from the work done by the skaters in pulling the pole towards them. When the skaters pull the pole towards them, they exert a force on the pole over a distance, doing work on the system and increasing its kinetic energy. This work is done at the expense of the chemical energy stored in the skaters' muscles.

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if two massive bodies, initially held at rest in space, are released, then they will begin to

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If two massive bodies, initially held at rest in space, are released, then they will begin to move towards each other due to the force of gravity between them.

This is known as gravitational attraction, which is an inverse square law force, meaning that it gets weaker as the distance between the two objects increases. As the two bodies move towards each other, they will gain kinetic energy and lose potential energy until they collide, merge, or pass each other by. The velocity at which they approach each other will depend on their masses and the distance between them. If the bodies are very massive, like planets or stars, their gravitational attraction can create significant tidal forces and affect their orbits around each other. In summary, the release of two massive bodies initially at rest in space will result in the manifestation of the force of gravity between them, causing them to move towards each other and potentially interact in various ways.

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