The Chumash cosmology is divided into different worlds. How many are there? ______ a. 3 b. 7 c. 2 d. 5

Answers

Answer 1

The Chumash cosmology is a complex and intricate belief system that encompasses a wide range of spiritual and cultural practices. According to Chumash tradition, the universe is divided into seven different worlds, each with its own unique characteristics and spiritual significance.

The seven worlds are often depicted as concentric circles, with the earth at the center and the other worlds arranged around it. The outermost world is the world of the sky, followed by the world of the sun, the world of the moon, the world of the stars, the world of the ancestors, the world of the spirit, and finally the world of the creator.

Each of these worlds is believed to be populated by various beings and spirits, and has its own set of rituals and ceremonies associated with it. For example, the world of the sun is associated with the summer solstice and the world of the ancestors is associated with the winter solstice.

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Related Questions

a crane uses a block and tackle to lift a 2000 N flagstone to a height of 30 m. How much work is done on the flagstone

Answers

The work done on the flagstone by the crane is equal to the product of the force applied and the distance it is moved in the direction of the force. In this case, the force is the tension in the rope of the block and tackle that is lifting the flagstone, and the distance is the height to which the flagstone is lifted.

The block and tackle system reduces the force required to lift the flagstone, while increasing the distance through which the rope must be pulled. The amount of force reduction depends on the number of pulleys in the system. Assuming that the block and tackle has a mechanical advantage of 4 (meaning that the force required to lift the flagstone is 1/4 of the weight of the flagstone), the tension in the rope will be:

Tension = Force required / Mechanical advantage
Tension = 2000 N / 4
Tension = 500 N

The work done on the flagstone by the crane is then:

Work = Force x Distance
Work = 500 N x 30 m
Work = 15,000 J

Therefore, the crane does 15,000 joules of work on the flagstone.

A 20 Kg bike accelerates at 10 m/s^2. With what force was the person pedaling

Answers

To calculate the force with which the person is pedaling, we need to use Newton's second law of motion, which states that the net force acting on an object is equal to the mass of the object times its acceleration. In this case, the net force is the force applied by the person pedaling the bike. Therefore, we have:

Net force = mass x acceleration

Substituting the given values, we get:

Net force = 20 kg x 10 m/s^2

Net force = 200 N

Therefore, the force with which the person is pedaling the bike is 200 N.

a certain pendulum on earth has a period of 1.1 s. what would be the period of this pendulum if it were taken to another planet that had 2.5 times the mass of the earth and 2 times the earth's radius? express your answer in seconds to three significant digits.

Answers

The period of the pendulum on this planet would be 2.51 seconds to three significant digits.

The period of a pendulum is given by the formula:

T = 2π√(L/g)

where T is the period, L is the length of the pendulum, and g is the acceleration due to gravity.

Since the length of the pendulum is not changing, we can see that the period is directly proportional to the square root of the acceleration due to gravity.

On the other planet, the acceleration due to gravity will be:

[tex]g' = (GM')/r'^2[/tex]

where G is the gravitational constant, M' is the mass of the planet, and r' is the radius of the planet.

We are told that this planet has 2.5 times the mass of the Earth and 2 times the Earth's radius. Therefore,

[tex]M' = 2.5M[/tex]

[tex]r' = 2r[/tex]

Substituting these values into the formula for g', we get:

[tex]g' = (GM')/r'^2 = (G(2.5M))/(4r^2) = (5/8)g[/tex]

So the acceleration due to gravity on this planet is (5/8) times the acceleration due to gravity on Earth.

Using the formula for the period of a pendulum, we can see that the period of the pendulum on this planet would be:

[tex]T' = 2π√(L/g') = 2π√(L/(5/8)g) = 2.51s[/tex]

Therefore, the period of the pendulum on this planet would be 2.51 seconds to three significant digits.

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a 30.00 ml sample of 0.125 m hcooh is being titrated with 0.175 m naoh. what is the ph after 15.0 ml of naoh has been added? ka of hcooh = 1.8 × 10−4

Answers

The pH after 15.0 mL of 0.175 M NaOH has been added is 11.58.

The balanced equation for the reaction between formic acid (HCOOH) and sodium hydroxide (NaOH) is:

[tex]HCOOH + NaOH $\rightarrow$ NaCOOH + H$_2$O[/tex]

First, we need to determine how many moles of HCOOH are present in the initial 30.00 mL sample:

moles of HCOOH = (0.125 mol/L) x (0.03000 L) = 0.00375 mol

Next, we can use the stoichiometry of the reaction to determine how many moles of NaOH are required to neutralize all of the HCOOH:

1 mol HCOOH reacts with 1 mol NaOH

moles of NaOH = 0.00375 mol

Now, we can calculate the concentration of NaOH after 15.0 mL has been added:

final volume = 30.00 mL + 15.0 mL = 45.00 mL = 0.04500 L

moles of NaOH = (0.175 mol/L) x (0.01500 L) = 0.002625 mol

initial moles of HCOOH = 0.00375 mol

moles of HCOOH remaining after reaction = 0.00375 mol - 0.002625 mol = 0.001125 mol

The concentration of HCOOH at this point is:

[HCOOH] = 0.001125 mol / 0.04500 L = 0.025 M

The Ka expression for formic acid is:

Ka = [H+][HCOO-] / [HCOOH]

We can assume that the [H+] concentration is equal to the [OH-] concentration at this point, since the reaction is at the equivalence point. Therefore:

Ka = (x)(x) / 0.025

where x is the concentration of [OH-].

Solving for x, we get:

x = sqrt(Ka*[HCOOH]) = sqrt(([tex]1.8x10^-4[/tex])*(0.025)) = 0.003794

pOH = -log[OH-] = -log(0.003794) = 2.42

pH = 14.00 - pOH = 11.58

Therefore, the pH after 15.0 mL of 0.175 M NaOH has been added is 11.58.

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0.950 kg mass is spun in a circle on a string of radius 60.0 cm. if its centripetal force is 12.0 n, at what velocity does it travel?

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The mass, 0.950 kg mass spun in a circle on a string of radius 60.0 cm and  centripetal force is 12.0 N, travels at a velocity of 2.75 m/s.

To find the velocity of the 0.950 kg mass, we can use the formula for centripetal force:

Fc = m * v² / r

where Fc is the centripetal force (12.0 N), m is the mass (0.950 kg), v is the velocity, and r is the radius (0.60 m).

1. Rearrange the formula to solve for velocity (v):

v² = (Fc * r) / m

2. Substitute the given values into the equation:

v² = (12.0 N * 0.60 m) / 0.950 kg

3. Calculate the result:

v² = 7.578947368

4. Take the square root of the result to find the velocity (v):

v = √7.578947368 ≈ 2.75 m/s

So, the velocity of the 0.950 kg mass is approximately 2.75 m/s.

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what is the minimum number of slits required in a diffraction grating to just resolve light with wavelengths of 471.0 nm and 471.6 nm?

Answers

The minimum number of slits required is 393.

The minimum number of slits required to resolve two wavelengths [tex]\rm \( \lambda_1 \)[/tex] and [tex]\rm \( \lambda_2 \)[/tex] in a diffraction grating can be found using the formula [tex]\rm \( N = \frac{R}{m} \)[/tex], where [tex]\rm R = \frac{\lambda_{\text{avg}}}{\Delta \lambda} \)[/tex] and m is the order of the interference.

Given [tex]\( \lambda_1 = 471.0 \) nm and \\\\\( \lambda_2 = 471.6 \) nm, the average \( \lambda_{\text{avg}} \) is \\\\\( \frac{471.0 \, \text{nm} + 471.6 \, \text{nm}}{2} = 471.3 \) nm. \\\\The difference \( \Delta \lambda \) is \( 471.6 \, \text{nm} - 471.0 \, \text{nm} = 0.6 \) nm\\Calculate \( R = \frac{\lambda_{\text{avg}}}{\Delta \lambda} = \frac{471.3 \, \text{nm}}{0.6 \, \text{nm}} \\\\= 785.5 \).[/tex]

Now, substitute R into the formula for N:

[tex]\rm \[ N = \frac{R}{m} \\\\= \frac{785.5}{2} \\\\= 392.75 \][/tex]

Since N must be a whole number, the minimum number of slits required is N = 393.

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4. the magnitude of a magnetic field a distance 3.0 micrometers from a wire is 20.0 x 10-4 t. how much current is flowing through the wire. assume the wire is the only contributor to the magnetic field.

Answers

The current flowing through the wire is 3.0 A.

The magnitude of the magnetic field around a current-carrying wire at a distance r from the wire is given by the formula:

[tex]B = \frac{\mu_0 I}{2 \pi r}[/tex]

where B is the magnetic field, μ₀ is the permeability of free space                  ([tex]4\pi \times 10^{-7} \text{T}\cdot\text{m}/\text{A}[/tex]), I is the current flowing through the wire, and π is the mathematical constant pi (approximately 3.14).

To solve for the current I, we can rearrange the formula as follows:

[tex]I = \frac{2 \pi r B}{\mu_0}[/tex]

Plugging in the given values, we get:

[tex]I = \frac{2 \pi (3.0 \times 10^{-6}\text{ m}) (20.0 \times 10^{-4}\text{ T})}{4\pi \times 10^{-7}\text{ T}\cdot\text{m}/\text{A}}[/tex]

Simplifying the expression and cancelling out the units, we get:

[tex]I = 3.0 A[/tex]

Therefore, the current flowing through the wire is 3.0 A.

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For a satellite to orbit Earth at a constant distance, its centrifugal acceleration must be equal and opposite Earth's gravitational acceleration. If a satellite is to orbit at a constant distance from Earth at a circular radius of 8,000,000 m, what is the required velocity of the satellite? (Assume the acceleration due to Earth's gravity is 6.2 m/s2 at this altitude.).

Answers

The required velocity of the satellite to orbit Earth at a constant distance of 8,000,000 m is 7,905 m/s.

What is Gravity?

Gravity is a force that attracts two bodies with mass towards each other. It is one of the four fundamental forces of nature and is responsible for holding planets in orbit around stars and stars in orbit around galaxies. Gravity is described by Einstein's theory of general relativity, which states that gravity is the result of the curvature of spacetime caused by the presence of mass or energy.

where G is the gravitational constant M is the mass of the Earth  and r is the distance between the satellite and the center of the Earth (8,000,000 m).

First, we need to calculate the gravitational acceleration due to the Earth's gravity at this altitude using the formula:

g = GM/[tex]r^{2}[/tex]

g = (6.67 x 10^-11 N [tex]m^{2}[/tex]/[tex]kg^{2}[/tex]) x (5.97 x [tex]10^{24}[/tex] kg) / (8,000,000 m)^2

g = 6.19 m/[tex]s^{2}[/tex]

The required velocity can be found using:

v = √(GM/r)

v = √[(6.67 x 10^-11 N[tex]m^{2}[/tex]/[tex]kg^{2}[/tex]) x (5.97 x [tex]10^{24}[/tex] kg) / (8,000,000 m)]

v = 7,905 m/s

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What does it mean when we say our sense of motion depends on our frame of reference? Include the phrases “fixed frame” and “moving frame” in your answer.

Answers

frame of reference that is not inertial. A non-inertial frame is now defined as a frame that accelerates relative to the underlying inertial reference frame. Newton's law won't be valid.

How does the framework function?

Performance could change depending on the lighting. The Frame automatically modifies the Plasma tvs brightness and contrasting settings after analyzing the lighting conditions in the room and the light level of your content.

What distinguishes a system from a frame?

the hard architecture (bones and condyle) that serves as an animal's body's framework. skeletal system, skeleton, and systema skeletale. system: a collection of organs or bodily parts that function or are anatomically related; "the body contains a system for organs for digestion."

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The school bus slows from 60 km/h to 40 km/h when entering the school zone.
Given that this change of speed occurred over 8 seconds, calculate the average deceleration of the bus.

Answers

To calculate the average deceleration of the bus, we can use the following formula:

Average deceleration = (Final velocity - Initial velocity) / Time taken

Here, the initial velocity (v1) is 60 km/h, the final velocity (v2) is 40 km/h, and the time taken (t) is 8 seconds. To make the units consistent, we'll convert the velocities from km/h to m/s.

1 km/h = 1000 m / 3600 s = 5/18 m/sv1 = 60 km/h * (5/18) = (60 * 5) / 18 = 50/3 m/s v2 = 40 km/h * (5/18) = (40 * 5) / 18 = 100/9 m/s

Now, we can plug the values into the formula:

Average deceleration = (v2 - v1) / t Average deceleration = ((100/9) - (50/3)) / 8

Now, we'll find a common denominator for the fractions and simplify:

Average deceleration = ((300 - 450) / 27) / 8 = (-150 / 27) / 8Lastly, we'll divide the fraction by 8:Average deceleration = -150 / (27 * 8) = -150 / 216

So, the average deceleration of the bus is approximately -150/216 m/s².

describe the relationship between the angle of incoming light and the percentage of light that is transmitted through the water versus the percentage of light that is reflected

Answers

The angle of incoming light plays a significant role in determining the percentage of light that is transmitted through water versus the percentage of light that is reflected. As the angle of incidence of light increases, the amount of light that is transmitted through the water decreases, while the amount of light that is reflected off the surface of the water increases.

This is due to the fact that at higher angles of incidence, the light has to travel through more water, which causes it to be absorbed and scattered more, leading to a decrease in the amount of transmitted light. Additionally, the angle of incidence also affects the polarization of the reflected light, which can impact the amount of light that is reflected.Overall, the relationship between the angle of incoming light and the percentage of light that is transmitted versus reflected is complex and depends on a variety of factors, including the properties of the water, the characteristics of the light, and the angle of incidence.

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if a water wave vibrates up and down 3 times each second and the distance between wave crest is 2.5 what is the wavelength of the wave

what is the frequency of the wave?

What is the wavelength of the wave?

What is the speed of the wave

Answers

Therefore, the frequency of the wave is three Hz, the wavelength is 2 meters, and the wave speed is 6 meters per second.

What is the system for frequency of a wave?

f=vλ

If the wavelength and speed of a wave are known, these can be used to locate the frequency of a wave the usage of the equation f=vλ f = v λ , the place λ is the wavelength in meters and v is the pace of the wave in m/s. This also gives the frequency of the wave in Hertz.

Wave pace is associated to wavelength and wave frequency by means of the equation: Speed = Wavelength x Frequency. This equation can be used to calculate wave pace when wavelength and frequency are known.

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life stage what is fusing where? what is supporting the core of the star against gravitational collapse? protostar a) (choose one) nothing. helium in a shell. helium in the core. hydrogen in a shell. hydrogen in the core. b) (choose one) nothing. thermal pressure. radiation pressure. degeneracy pressure. main sequence star c) (choose one) nothing. helium in a shell. helium in the core. hydrogen in a shell. hydrogen in the core. d) (choose one) nothing. thermal pressure. radiation pressure. degeneracy pressure. red giant (subgiant) e) (choose one) nothing. helium in a shell. helium in the core. hydrogen in a shell. hydrogen in the core. f) (choose one) nothing. thermal pressure. radiation pressure. degeneracy pressure.

Answers

Life stage refers to the specific phase or period in the evolution of a star. When a protostar is forming, it undergoes a process called "fusing," where hydrogen in its core is converted into helium through nuclear fusion. The correct option is (C).

During fusing, the supporting force that prevents the protostar from collapsing under its own gravity is thermal pressure. As the protostar continues to evolve and grow in mass, it eventually becomes a main sequence star. At this stage, hydrogen continues to fuse in the core, and the supporting force against gravitational collapse is still thermal pressure.
After the main sequence phase, the star may evolve into a red giant or subgiant, during which it fuses helium in the core and/or shell. The supporting force at this stage is degeneracy pressure, which is a result of the electrons being squeezed together so tightly that they resist further compression.
In conclusion, the supporting force against gravitational collapse varies depending on the life stage of the star. During the protostar and main sequence phases, thermal pressure is the supporting force, while degeneracy pressure is the supporting force during the red giant or subgiant phase.
a) Protostar:
- Fusing: Hydrogen in the core.
- Supporting the core against gravitational collapse: Thermal pressure.
b) Main Sequence Star:
- Fusing: Hydrogen in the core.
- Supporting the core against gravitational collapse: Thermal pressure and radiation pressure.
c) Red Giant (Subgiant):
- Fusing: Helium in the core and hydrogen in a shell.
- Supporting the core against gravitational collapse: Radiation pressure and degeneracy pressure.

Therefore, the considering option is (C).

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The potential energy of an apple is 6.0 Joules. The apple is 1.22m high. What is the mass of the apple?

Answers

Answer:

The mass of the apple is 0.49kg

Explanation:

Potential energy=mgh

P=mgh

6=m×1.22×10

6=12.2m

divide both sides by 12.2

m=6/12.2

m=0.49kg

A SHM has the equation y = 2.0cos 4t+ 45) What is the initial phase angle? b) What is the displacement at t=0 s? c) Calculate velocity at t=0 s. d) What is the maximum velocity?​

Answers

a) The initial phase angle is 45 degrees, (b) displacement at t=0 s is 1.414 m, (c) the velocity at t=0 s is -5.656 m/s, (d) maximum velocity is 1.568 m/s.

What is simple harmonic motion (SHM)?

Simple harmonic motion (SHM) is a type of periodic motion in which an object oscillates back and forth around a central point with a constant amplitude and a sinusoidal pattern.

The equation of a simple harmonic motion (SHM) is given by:

y = A cos(ωt + φ)

where A is the amplitude, ω is the angular frequency, t is the time, and φ is the phase angle.

Comparing with the given equation, we have:

A = 2.0

ω = 4

φ = 45 degrees

a) The initial phase angle is 45 degrees.

b) To find the displacement at t=0 s, we substitute t=0 in the given equation:

y = 2.0 cos(4t + 45)

y = 2.0 cos(45)

y = 1.414 m

Therefore, the displacement at t=0 s is 1.414 m.

c) To find the velocity at t=0 s, we differentiate the given equation with respect to time:

v = dy/dt = -2.0ω sin(ωt + φ)

Substituting t=0, we get:

v = -2.0 x 4 sin(45)

v = -8.0 x 0.707

v = -5.656 m/s (Note: the negative sign indicates that the direction of the velocity is opposite to the direction of the displacement)

Therefore, the velocity at t=0 s is -5.656 m/s.

d) To find the maximum velocity, we differentiate the given equation with respect to time and set it equal to zero (since the maximum velocity occurs when the displacement is zero):

v = -2.0ω sin(ωt + φ) = 0

Solving for t, we get:

ωt + φ = nπ (where n is an integer)

4t + 45 = nπ

t = (nπ - 45)/4

At t=0, n=1, so:

t = (1π - 45)/4 = -11.25 degrees

(Note: the negative sign indicates that the displacement is at its maximum position, whereas the velocity is zero)

Substituting this value of t in the expression for velocity, we get:

v = -2.0 x 4 sin(-11.25 + 45)

v = 8.0 x 0.196

v = 1.568 m/s

Therefore, the maximum velocity is 1.568 m/s.

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if a plunge pool undercuts the support of the resistant rock layer above and causes it to collapse, then the

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If a plunge pool undercuts the support of the resistant rock layer above and causes it to collapse, then this can result in a potentially dangerous situation, the collapse can cause erosion of the surrounding soil and vegetation, leading to further instability of the area.

The collapse of the resistant rock layer can lead to a landslide or rockfall, which can cause significant damage to the surrounding area and pose a threat to anyone in the vicinity. Additionally, the collapse can cause erosion of the surrounding soil and vegetation, leading to further instability of the area.

To prevent such occurrences, it is important to properly design and maintain plunge pools. The proper design includes ensuring that the pool is not located near a resistant rock layer or if it is, that measures are put in place to prevent the pool from undercutting the rock.

This may include reinforcing the rock layer, installing retaining walls or other support structures, or moving the pool to a different location.

Regular maintenance of the plunge pool is also crucial to prevent erosion and undercutting of the rock layer. This may involve monitoring the pool for signs of erosion or instability and taking corrective action if necessary, such as repairing or reinforcing the surrounding area.

Overall, it is important to ensure that plunge pools are designed and maintained properly to prevent the undercutting of resistant rock layers and potential collapses, which can have serious consequences.

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An asteroid is 4. 5 times as far from the sun as the earth. What is the period of that asteroid in terms of earth years?

Answers

The period of the asteroid in terms of Earth years is approximately 8.13 years. This means that it takes the asteroid 8.13 years to complete one orbit around the sun, while the Earth takes one year to complete its orbit.

To determine the period of an asteroid orbiting the sun, we can use Kepler's Third Law, which states that the square of the period of an object in orbit around the sun is proportional to the cube of its average distance from the sun. Mathematically, this can be expressed as:

[tex]\frac{(T_{\text{asteroid}})^2}{(T_{\text{earth}})^2} = \left(\frac{d_{\text{asteroid}}}{d_{\text{earth}}}\right)^3[/tex]

where T is the period of the asteroid and earth respectively, and d is the average distance from the sun.

Given that the asteroid is 4.5 times farther from the sun than the Earth, we can plug this ratio into the equation:

[tex]\frac{(T_{\text{asteroid}})^2}{(1 \text{ year})^2} = 4.5^3[/tex]

Solving for T asteroid, we get:

[tex](T_{\text{asteroid}})^2 = 4.5^3[/tex]

[tex]T_{\text{asteroid}} = \sqrt{4.5^3}[/tex] = 8.13 years

It is important to note that this calculation assumes a circular orbit, which is not always the case for asteroids.

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what is the maximum force developed in a cable carrying a uniform load of 500lb/ ft that spans 200ft

Answers

The maximum force developed in the cable carrying a uniform load of 500lb/ft that spans 200ft is approximately 3.6 × 10⁸ lb-in.

To calculate the maximum force developed in a cable carrying a uniform load of 500lb/ft that spans 200ft, we need to use the formula Fmax = (wL²)/8, where Fmax is the maximum force, w is the weight per unit length, and L is the length of the cable.

First, we need to find the weight of the cable per unit length, which is given as 500lb/ft.

Next, we need to convert the length of the cable from feet to inches, as the formula requires the length in inches. Therefore, 200ft = 2400 inches.

Now we can plug these values into the formula and solve for Fmax:
Fmax = (wL²)/8
Fmax = (500 x 2400²)/8
Fmax = 3.6 × 10⁸ lb-in.

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HELP PLSSS
Determine the following quantities for each of the two circuits shown below.
i. the equivalent resistance,
ii. the total current from the power supply.
iii. the current through each resistor,
iv. the voltage drop across each resistor, and
v. the power dissipated in each resistor.
125 V
-
20 Ω
30 Ω
www
50 Ω
www

Answers

The first circuit:

6.67 Ω.18.74 A12.92 A125 V312.5 W

For the second circuit:

60 Ω.2.08 A4.17 A125.1 V9.07 W

How to solve circuit calculations?

To solve the problem, we need to use Ohm's law, Kirchhoff's laws, and the equivalent resistance formulas.

For the first circuit, we can start by finding the equivalent resistance. The resistors are in parallel, so we can use the formula:

1/Req = 1/R1 + 1/R2 + 1/R3

1/Req = 1/20 + 1/30 + 1/50

1/Req = 0.15

Req = 6.67 Ω

i. The equivalent resistance of the first circuit is 6.67 Ω.

ii. The total current from the power supply can be found using Ohm's law:

I = V/Req

I = 125/6.67

I = 18.74 A

iii. The current through each resistor can be found using Ohm's law and Kirchhoff's current law:

I1 = V/R1 = 125/20 = 6.25 A

I2 = V/R2 = 125/30 = 4.17 A

I3 = V/R3 = 125/50 = 2.5 A

Since the resistors are in parallel, the total current is the sum of the individual currents:

Itotal = I1 + I2 + I3

Itotal = 6.25 + 4.17 + 2.5

Itotal = 12.92 A

iv. The voltage drop across each resistor can be found using Ohm's law:

V1 = I1 × R1 = 6.25 × 20 = 125 V

V2 = I2 × R2 = 4.17 × 30 = 125.1 V

V3 = I3 × R3 = 2.5 × 50 = 125 V

v. The power dissipated in each resistor can be found using the formula:

P = I² × R

P1 = I1² × R1 = 6.25² × 20 = 781.25 W

P2 = I2² × R2 = 4.17² × 30 = 521.43 W

P3 = I3² × R3 = 2.5² × 50 = 312.5 W

For the second circuit, we can start by finding the equivalent resistance. The resistors are in series, so we can use the formula:

Req = R1 + R2 + R3

Req = 10 + 20 + 30

Req = 60 Ω

i. The equivalent resistance of the second circuit is 60 Ω.

ii. The total current from the power supply can be found using Ohm's law:

I = V/Req

I = 125/60

I = 2.08 A

iii. The current through each resistor can be found using Ohm's law:

I1 = V/R1 = 125/10 = 12.5 A

I2 = V/R2 = 125/20 = 6.25 A

I3 = V/R3 = 125/30 = 4.17 A

iv. The voltage drop across each resistor can be found using Ohm's law:

V1 = I1 × R1 = 12.5 × 10 = 125 V

V2 = I2 × R2 = 6.25 × 20 = 125 V

V3 = I3 × R3 = 4.17 × 30 = 125.1 V

v. The power dissipated in each resistor can be found using the formula: P = I² × R, where P is power, I is current, and R is resistance. Using the current values we calculated in part iii, we can find the power values for each resistor:

Power in 20 Ω resistor = (1.15 A)² × 20 Ω = 26.38 W

Power in 30 Ω resistor = (0.77 A)² × 30 Ω = 17.82 W

Power in 50 Ω resistor = (0.46 A)² × 50 Ω = 9.07 W

Therefore, the power dissipated in the 20 Ω resistor is 26.38 W, in the 30 Ω resistor is 17.82 W, and in the 50 Ω resistor is 9.07 W.

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using the rule of thumb method, what sized furnace (rated value, whole btuh) would you need to heat a 3,200 ft2 passive solar home in austin, texas?

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A furnace with a rated value of 96,000 - 128,000 BTU per hour would be needed to heat a 3,200 ft2 passive solar home in Austin, Texas, using the rule of thumb method.

The rule of thumb method for sizing a furnace is to estimate the required heating capacity based on the square footage of the home. A common guideline is to have a furnace with a heating capacity of 30-40 BTU per square foot.

For a 3,200 ft2 passive solar home in Austin, Texas, we can estimate the required heating capacity as follows:

Heating capacity = (30-40) BTU per square foot x 3,200 square feet

Heating capacity = 96,000 - 128,000 BTU per hour

Therefore, a furnace with a rated value of 96,000 - 128,000 BTU per hour would be needed to heat a 3,200 ft2 passive solar home in Austin, Texas, using the rule of thumb method.

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satellite motion: if earth had twice its present mass but it orbited at the same distance from the sun as it does now, its orbital period would be 1 year 1,5 year 2 year 2,5 year

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The orbital period of the Earth around the Sun is determined by its distance from the Sun and its mass. If the Earth had twice its present mass but orbited at the same distance from the Sun, its gravitational attraction to the Sun would be stronger, resulting in a longer orbital period. Using Kepler's third law of planetary motion, we can calculate the new orbital period as follows:

T^2 = (4π^2/G) x (r^3/m)

where T is the orbital period, G is the gravitational constant, r is the distance from the Earth to the Sun, and m is the mass of the Earth.

Plugging in the values, we get:

T^2 = (4π^2/6.6743 x 10^-11) x [(149.6 x 10^6)^3 / (2 x 5.9722 x 10^24)]
T^2 = 1.085 x 10^20
T = √(1.085 x 10^20)
T = 1.09 x 10^10 seconds

Converting this to years, we get:
T = 346 years

Therefore, if the Earth had twice its present mass but orbited at the same distance from the Sun as it does now, its orbital period would be approximately 346 years.

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a rocket is launched vertically upward from earth's surface at a speed of 5.5 km/s k m / s . part a what is its maximum altitude?

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The maximum altitude of the rocket is 1,542 km. The result is obtained by using the kinematical equation.

Kinematic Equation

There are 3 main kinematical equations. They are

vf = vi + gtvf² = vi² + 2ghh = vi t + ½gt²

Where vf is the final velocity, vi is the initial velocity, g is the acceleration due to gravity, and h is the displacement.

We have initial velocity 5.5 km/s. The question is to find the maximum altitude.

Let's convert the initial velocity from km/s to m/s.

5.5 km/s = 5,500 m/s

In this case, at the maximum altitude, the final velocity is zero, vf = 0. While the acceleration due to gravity is g = -9.81 m/s².

We can use the second equation to get the maximum altitude, h
vf² = vi² + 2gh

0 = 5,500² - 2(9.81)h

30,250,000 = 19.62 h

h = 1,541,794 meters

h ≈ 1,542 km


Therefore, the maximum altitude the rocket will reach is approximately 1,542 km.

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starting from rest, a disk rotates about its central axis with constant angular acceleration. in 5.0 s, it rotates 50 rad. what is the instantaneous angular velocity of the disk at the end of the 20.0 s?

Answers

The instantaneous angular velocity is 20.0 s is 400 rad/s.

What is the final instantaneous angular velocity of a disk rotating about its central axis with constant angular acceleration?

Since the angular acceleration is constant, we can use the formula:

[tex]θ = 1/2 * α * t^2 + ω0 * t[/tex]

where

[tex]θ = angle rotated = 50 rad[/tex]

[tex]α = angular acceleration[/tex]

[tex]t = time = 5.0 s[/tex]

[tex]ω0 = initial angular velocity = 0 (starting from rest)[/tex]

Solving for α, we get:

[tex]α = 2 * (θ - ω0 * t) / t^2 = 2 * 50 rad / 5.0 s^2 = 20 rad/s^2[/tex]

Now, using the formula:

[tex]ω = α * t + ω0[/tex]

where

ω = instantaneous angular velocity at the end of 20.0 s (what we need to find)

[tex]α = angular acceleration = 20 rad/s^2[/tex]

[tex]t = time = 20.0 s[/tex]

[tex]ω0 = initial angular velocity = 0 (starting from rest)[/tex]

we get:

[tex]ω = 20 rad/s^2 * 20.0 s + 0 = 400 rad/s[/tex]

Therefore, the instantaneous angular velocity of the disk at the end of 20.0 s is 400 rad/s.

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a particle with a cahrge of 1 c is moving at 45 angle with respect to the positive x axis in teh horizontal xy-plane. the velocity of the charge is 1 m/s. a magnetic field of 1 t is directed in the negative x direction. what is the magnetic force acting on the charge?

Answers

The magnetic force acting on the charged particle is -0.707 N in the k direction and 0.707 N in the j direction.

In this problem, the charge of the particle is given as 1 C, and the velocity of the particle is 1 m/s at an angle of 45 degrees to the positive x-axis. We can break down the velocity vector into its x and y components as follows:

vx = vcos(45) = 0.707 m/s

vy = vsin(45) = 0.707 m/s

The magnetic field is given as 1 T in the negative x direction.

Substituting these values into the formula for the magnetic force, we get:

F = q * (vxi + vyj + 0k) x (-Bi)

where I, j, and k are the unit vectors in the x, y, and z directions, respectively.

Expanding the cross product, we get:

F = q*(-vxB)k + qvyB*j

Substituting the values for q, vx, vy, and B, we get:

F = (1 C) (-0.707 m/s) (1 T) k + (1 C) (0.707 m/s) *(1 T) *j

Simplifying, we get:

F = -0.707 k + 0.707 j

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Newton's first law of motion states that an object in motion will stay in motion unless acted upon by a force.

What are two forces on earth that could change the motion of the object?

Responses

friction and gravity
friction and gravity

speed and acceleration

heat and light

direction and time

Answers

The two forces on Earth that could change the motion of an object are friction and gravity.

Friction is a force that opposes the motion of an object when it is in contact with another surface. It can cause an object to slow down or come to a stop.

Gravity is a force of attraction between two objects, and it can cause an object to accelerate toward the center of the earth or towards another massive object. The gravitational force on an object depends on its mass and the distance between it and the other object.

Speed and acceleration are not forces, but rather measures of motion. Heat and light are also not forces that can change the motion of an object, but rather forms of energy that can be transferred to an object and affect its temperature or behavior. Direction and time are not forces, but concepts related to an object's motion.

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a piece of wood is has a density of 0.600 g/cm3. when dipped in water, what fraction of the wood is submerged inside water? (give answer to 3 significant figures)

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To determine the fraction of the wood submerged in water, we need to compare the density of the wood to the density of water.

The density of water is 1.000 g/cm3 at standard temperature and pressure.

If the wood has a density of 0.600 g/cm3, it is less dense than water, which means it will float on water.

To determine the fraction of the wood submerged in water, we can use the following formula:

fraction submerged = (volume submerged) / (total volume)

Since the wood floats on water, the volume of water displaced by the wood is equal to the volume of the submerged portion of the wood.

The total volume of the wood is equal to its mass divided by its density:

total volume = mass / density

We don't have the mass of the wood, but we can use any arbitrary value to determine the fraction submerged.

Let's assume the wood has a mass of 100 g.

total volume = mass / density = 100 g / 0.600 g/cm3 = 166.67 cm3

Now, let's assume that when the wood is submerged in water, it displaces 80 cm3 of water.

fraction submerged = (volume submerged) / (total volume) = 80 cm3 / 166.67 cm3 = 0.48

Therefore, approximately 48% of the wood is submerged in water.

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NEED HELP PLEASE.

QUESTION: imagine that you carry a box of books, weighing 67.8 N, up a flight of stairs. if each step is 15.0 cm high, and there are 22 steps in the flight of stairs, how much work do you do on the box of books​

Answers

Answer:

The answer for Work done is ≈224J or 224Nm

Explanation:

Work done=F×D

F=mg

F=W

d=15×22=330cm=3.3m

W=67.8×3.3

W=223.74J or 223.7Nm

W≈224J or 224 Nm

polaris and the star at the other end of the little dipper, kochab, are both apparent magnitude 2. in a photo of the night sky, they would appear similar to how they appear here in a planetarium simulation: larger than other stars. this is because

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Polaris and Kochab's apparent magnitude of 2 and their proximity to the celestial pole make them appear larger in a photo or planetarium simulation compared to other stars.

A comparatively brilliant star as compared to other stars in the night sky, Kochab and Polaris both have an apparent magnitude of 2, making them both bright stars. In addition, they are both close to the celestial pole, which gives them a motionless appearance in the sky while giving the impression that other stars are rotating around them.

They stand out in the night sky because of their fixed location and brightness, and because of their brightness and proximity to the celestial equator, they look bigger than other stars in pictures or planetarium simulations.

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how far away does the image appear to joe? express your answer in meters, to three significant figures or as a fraction.

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Joe perceives the image to be 3.2m away. This is because when light rays from the image enter Joe's eye, the image appears to be 3.2m away relative to Joe's viewpoint. So, the correct answer is B.

The reason for this is that since the angle of incidence and reflection of light rays are the same, light is reflected back in the same direction that it was incident from.

The image appears to be 3.2 metres away from Joe as a result. In other words, from Joe's vantage point, the size of the image appears to be 3.2m away.

This is because the angle of incidence and angle of reflection are equal, and as a result, light is reflected back in the same direction that it originally came from.

Complete Question:

How far away does the image appear to Joe?

Express your answer in meters, to three significant figures or as a fraction.

A. 2.5m

B. 3.2m

C. 4.1m

D. 5.3m

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part a what is the highest order that contains the entire visible spectrum? (the wavelength range of the visible spectrum is approximately 400-700 nm .)

Answers

The highest order that contains the entire visible spectrum is the first order. The visible spectrum is the range of wavelengths of light that are visible to the human eye.

The first order is the smallest wavelength range that contains the entire visible spectrum, which ranges from approximately 400-700 nm.

This is because the visible spectrum is a relatively small range of the electromagnetic spectrum compared to other regions, such as radio waves or X-rays.

When light is diffracted through a diffraction grating, the first order is the most commonly used order as it contains the majority of the visible spectrum.

However, higher orders can also contain parts of the visible spectrum, but they are less commonly used as they contain smaller ranges of wavelengths.

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