a)The speed of the proton accelerated through a potential difference of -1000 V is approximately 4.81 x \(10^5\) m/s.
b)The speed of the electron accelerated through a potential difference of 1000 V is approximately 5.93 x \(10^6\) m/s.
(a) To calculate the speed of a proton accelerated from rest through a potential difference of -1000 V, we can use the equation for the change in potential energy (ΔPE) and the kinetic energy (KE) of the proton.
The equation for the change in potential energy is ΔPE = qΔV, where q is the charge of the particle and ΔV is the potential difference. The equation for kinetic energy is KE = 1/2mv^2, where m is the mass of the proton and v is its speed.
Since the proton starts from rest, its initial kinetic energy is zero. So, we can equate the change in potential energy to the final kinetic energy:
qΔV = 1/2mv^2
Rearranging the equation gives: v = √(2qΔV / m)
The charge of a proton (q) is +1.6 x \(10^-19\) C, the mass of a proton (m) is 1.67 x \(10^-27\) kg, and the potential difference (ΔV) is -1000 V. Plugging in these values into the equation, we get: v = √(2(1.6 x \(10^-19\) C)(-1000 V) / (1.67 x \(10^-27\)kg))
Simplifying the equation gives: v ≈ 4.81 x 10^5 m/s
Therefore, the speed of the proton accelerated through a potential difference of -1000 V is approximately 4.81 x 10^5 m/s.
(b) Similarly, to calculate the speed of an electron accelerated from rest through a potential difference of 1000 V,
we use the same equation: v = √(2qΔV / m)
The charge of an electron is -1.6 x \(10^-19\) C, the mass of an electron is 9.11 x \(10^-31\) kg, and the potential difference is 1000 V.
Plugging in these values into the equation, we get: v = √(2(1.6 x \(10^-19\) C)(1000 V) / (9.11 x \(10^-31\) kg))
Simplifying the equation gives: v ≈ 5.93 x 10^6 m/s
Therefore, the speed of the electron accelerated through a potential difference of 1000 V is approximately 5.93 x \(10^6\) m/s.
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A truck heading east has an initial velocity of 6 m/s. It accelerates at 2 m/s2 for 12 seconds. What distance does the truck travel in the given time?
84 m
144 m
216 m
360 m
The answer (distance) is:
216mThe distance of the truck in the given time is 216 m.
How do you find displacement with velocity and acceleration?
Displacement (s) of an object equals, velocity (u) times time (t), plus ½ times acceleration (a) times time squared (t2). Use standard gravity, a = 9.80665 m/s2, for equations involving the Earth's gravitational force as the acceleration rate of an object.
How do you find velocity from acceleration?
Multiply the acceleration by time to obtain the velocity change: velocity change = 6.95 * 4 = 27.8 m/s . Since the initial velocity was zero, the final velocity is equal to the change in speed. You can convert units to km/h by multiplying the result by 3.6: 27.8 * 3.6 ≈ 100 km/h.
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The temperature of an oven is kept constant at 1065.0 K. A hole with a diameter of 35.0 mm is drilled in the wall of the oven. How much power is emitted by this hole
In conclusion, the hole with a diameter of 35.0 mm drilled in the wall of the oven emits approximately 32.8 W of power.
The power emitted by a hole in the wall of an oven can be calculated using the Stefan-Boltzmann law. This law states that the power emitted by a black body is proportional to the fourth power of its temperature.
To calculate the power emitted by the hole, we need to consider it as a black body and assume it is in thermal equilibrium with the oven.
Given that the temperature of the oven is constant at 1065.0 K and the hole has a diameter of 35.0 mm, we can calculate the surface area of the hole using the formula for the area of a circle.
Area = π * (radius)^2
The radius of the hole is half of the diameter, so the radius would be 35.0 mm / 2 = 17.5 mm = 0.0175 m.
Using this radius, we can calculate the area of the hole:
Area = π * (0.0175 m)^2 = 0.000962 m^2
Now, we can calculate the power emitted by the hole using the Stefan-Boltzmann law:
Power = σ * Area * (Temperature)^4
Where σ is the Stefan-Boltzmann constant, which is approximately equal to 5.67 x 10^-8 W/(m^2*K^4).
Plugging in the values, we get:
Power = (5.67 x 10^-8 W/(m^2*K^4)) * (0.000962 m^2) * (1065.0 K)^4
Calculating this, the power emitted by the hole is approximately 32.8 W.
In conclusion, the hole with a diameter of 35.0 mm drilled in the wall of the oven emits approximately 32.8 W of power.
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A Lagrangian Point or gravitational dead zone is found between two stars, at a distance RA = 4020 AU from star A and RB = 20100 AU from star B where 1 AU = 149.6 million km. If the mass of star A is 6.8E43 kg, determine the force exerted on star A by star B. Derive and express algebraic solution in terms of givens: Ra Rb, ma and G.
The gravitational force is given by Newton's Law:
\(F=G\frac{mM}{r^2}\)We know that in a lagrangian point the foreces cancel out, then in this case we have:
\(\begin{gathered} -G\frac{mM_A}{r^2_A}+G\frac{mM_B}{r^2_B}=0 \\ -\frac{M_A}{r^2_A}+\frac{M_B}{r^2_B}=0 \end{gathered}\)From which we can find the mass of star B:
\(\begin{gathered} -\frac{M_A}{r^2_A}+\frac{M_B}{r^2_B}=0 \\ \frac{M_B}{r^2_B}=\frac{M_A}{r^2_A} \\ M_B=\frac{r^2_B}{r^2_A}M_A \\ M_B=(\frac{20100}{4020})^2(6.8\times10^{43}) \\ M_B=1.7\times10^{45} \end{gathered}\)Now, that we know the mass of star B we can calculate the force exerted on star A by star B:
\(F=G\frac{M_AM_B}{(r_A+r_B)^2}\)plugging the values given we have:
\(\begin{gathered} F=G\frac{M_AM_B}{(r_A+r_B)^2} \\ F=6.67\times10^{-11}\cdot\frac{(6.8\times10^{43}\cdot1.7\times^{45})}{\lbrack(24120)(1.496\times10^{11})\rbrack^2} \\ F=5.92\times10^{47} \end{gathered}\)Therefore, the force exerted on star A by star B is:
\(F=5.92\times10^{47}\text{ N}\)deduce the relation between kwh and joule define 1 watt
Explanation:
We know that kWh is a commercial unit of energy.
Also, 1 Joule = 1 watt × 1 seconds
\(1\ kWh=1kW \times 1\ h\)
Since ,1 h = 3600 s and 1kW = 1000 W
\(1\ kWh=1000\ W \times 3600\ s\\\\1\ kWh = 36\times 10^5\ W-s\\\\1\ kWh=36\times 10^5\ J\)
So, the relation is : \(1\ kWh=36\times 10^5\ J\)
1 watt is defined as the power of an appliance when the energy is transferred at a rate of 1 Joule per second.
please help me asdrtyuio
Answer:
9. The Sun's Gravity
10. The core is the densest layer
The diagram below shows a 5.0-kilogram bucket of water being swung in a horizontal circle of 0.70-meter radius
at a constant speed of 2.0 meters per second.
5.0-kg Bucket
0.70 m
The magnitude of the centripetal force on the bucket of water is approximately
1) 5.7 N
2) 14 N
3) 29 N
4) 200 N
Answer:
F = 29 N
Explanation:
We have,
Mass of the bucket of water is 5 kg
Radius of a horizontal circle is 0.7 m
Speed of the circle is 2 m/s
It is required to find the magnitude of centripetal force on the bucket of water. The formula used to find the magnitude of centripetal force is given by :
\(F=\dfrac{mv^2}{r}\\\\F=\dfrac{5\times (2)^2}{0.7}\\\\F=28.57\ N\)
or
F = 29 N
So, the centripetal force on the bucket of water is 29 N.
The magnitude of the centripetal force on the bucket of water is approximately 29 N
Definition of centripetal forceCentripetal force is the force that acts to keep an object moving in a circular motion. It is expressed mathematically as:
F = mv² / r
With the above formula, we can obtain the centripetal force acting on the bucket.
How to determine centripetal force•Mass (m) = 5 Kg
•Radius (R) = 0.7 m
•Velocity (v) = 2 m/s
•Centripetal force (F) =?
F = mv² / r
F = (5 × 2²) / 0.7
F = (5 × 4) / 0.7
F = 20 / 0.7
F = 29 N
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IT'S 30 POINTS!!!!!!!
1) What are the five different types of interactions between organisms?
2) What patterns do scientists observe between predator-prey relationships like the wolves and moose on Isle Royale?
3) Use the data from your graph to provide evidence for the effects of of resource availability on individuals and populations in an ecosystem.
4) Do the patterns of interactions between organisms, such as competition and predation, change when they occur in different ecosystems? Explain.
5) Predict the effects on a predator-prey relationship, such as the one between a frog and blue heron, in a wetland ecosystem in the midst of a drought.
Answer:
1. Competition and prediction
Commensalism
Parasitism
Mutualism
Amensalism
2. As the population of wolves has declined the population of the moose increase
3.
The electric field of an electromagnetic wave is given by E=
(6.0×10−3V/m) sin [2((x/18m)−(/(6.0×10−8s))]ˆ.
Write the equations for the associated magnetic field and Poynting vector.
This is based on Energy Carried by Electromagnetic Waves.
The given electric field and magnetic field expressions, we can write the equation for the Poynting vector as:
S = (1/μ₀) * [(6.0 × 10^(-3) V/m) sin [2((x/18m) - (t/(6.0 × 10^(-8) s)))] * (6.0 × 10^(-3) V/m) sin [2((x/18m) - (t/(6.0 × 10^(-8) s)))]] / c.
The equation for the associated magnetic field can be derived from the given electric field. According to the properties of electromagnetic waves, the magnetic field is perpendicular to the electric field and oscillates in phase with it. The equation for the magnetic field (B) can be written as:
B = (E/c),
where c is the speed of light in a vacuum (approximately 3.0 × 10^8 m/s). Substituting the given electric field expression, we have:
B = (6.0 × 10^(-3) V/m) sin [2((x/18m) - (t/(6.0 × 10^(-8) s)))] / c.
The Poynting vector (S) represents the directional energy flux carried by an electromagnetic wave. It is given by the cross product of the electric field (E) and the magnetic field (B) divided by the permeability of free space (μ₀). Therefore, the equation for the Poynting vector is:
S = (1/μ₀) * (E × B),
where μ₀ is the permeability of free space (approximately 4π × 10^(-7) T·m/A). Substituting the given electric field and magnetic field expressions, we can write the equation for the Poynting vector as:
S = (1/μ₀) * [(6.0 × 10^(-3) V/m) sin [2((x/18m) - (t/(6.0 × 10^(-8) s)))] * (6.0 × 10^(-3) V/m) sin [2((x/18m) - (t/(6.0 × 10^(-8) s)))]] / c.'
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An object at rest will stay at rest until an external force acts on it. What was the external force that acted on the night once the hoop was removed?
Explanation:
The first law states that a body at rest will stay at rest until a net external force acts upon it and that a body in motion will remain in motion at a constant velocity until acted on by a net external force.Friction is the force between an object in motion and the surface on which it moves. There was a net external force on the night because of change in momentum as the hoop was removed.
Calculate the total charge Q of a thin plate with the charge density distribution p(x,y) = x²y mC/m². The plate shape is restricted by the lines: y=2-x² and y=2x-1, where x and y are measured in metres. a) Sketch the plate shape. [10 marks] [4 marks] b) Present the total charge through the double integral. c) Reduce the double integral to the repeated integrals and show limits of integration. [6 marks] d) Calculate the integral and present your answer with five significant figures. [20 marks]
a) Sketch the plate shape: we get a shape that resembles a trapezoid.
The plate shape is determined by the lines y = 2 - x² and y = 2x - 1. To sketch the plate shape, we can plot these two lines and shade the region in between them. The intersection points of the lines are found by solving the equations simultaneously:
2 - x² = 2x - 1
Simplifying, we get:
x² + 2x - 3 = 0
Factoring, we have:
(x - 1)(x + 3) = 0
So, x = 1 and x = -3. Plugging these values into the equations of the lines, we find the corresponding y-values:
For x = 1:
y = 2 - (1)² = 1
For x = -3:
y = 2(-3) - 1 = -7
Plotting these points and connecting them with the lines, we get a shape that resembles a trapezoid.
b) Total charge through the double integral:
To find the total charge Q, we need to integrate the charge density p(x, y) over the entire plate. We can express this as a double integral:
Q = ∬ p(x, y) dA
c) Reducing the double integral to repeated integrals: The limits of integration for x are the values of x that define the boundaries of the plate shape, which are -3 to 1.
Since the plate shape is described by the lines y = 2 - x² and y = 2x - 1, we can rewrite the double integral as a repeated integral by integrating with respect to x and y separately:
Q = ∫∫ p(x, y) dy dx
The limits of integration for y are from the lower curve y = 2 - x² to the upper curve y = 2x - 1. The limits of integration for x are the values of x that define the boundaries of the plate shape, which are -3 to 1.
d) Calculating the integral: The total charge Q of the thin plate is approximately 12.4 mC.
Now, we can evaluate the double integral to find the total charge Q:
Q = ∫(-3 to 1) ∫(2 - x² to 2x - 1) x²y dy dx
Performing the inner integral with respect to y first, we get:
Q = ∫(-3 to 1) [x²(y²/2 - y)] from 2 - x² to 2x - 1 dx
Simplifying the inner integral, we have:
Q = ∫(-3 to 1) [(x²/2)(2 - x²) - x²(2x - 1)] dx
Expanding and simplifying further, we get:
Q = ∫(-3 to 1) (x² - x⁴/2 - 4x³ + 2x²) dx
Integrating term by term, we have:
Q = [x³/3 - x⁵/10 - x⁴ + 2x³/3] from -3 to 1
Evaluating the integral at the limits, we get:
Q ≈ 12.4 mC (rounded to five significant figures)
Therefore, the total charge Q of the thin plate is approximately 12.4 mC.
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An object in space is observed to have an altitude of 1200 nary (2209 km), a velocity of 7000 m/s, and an elevation angle (Phi) of +40 degree. Give a complete description of the trajectory. Is there anything special or different about this trajectory? Find V, v, and Phi when r = 6.378 x 10^6 m. Sketch the trajectory and locate this point.
The trajectory of the object in space has an altitude of 1200 nary (2209 km), a velocity of 7000 m/s, and an elevation angle (Φ) of +40 degrees. This trajectory describes a high-speed ascent into space, likely representing the launch of a spacecraft or a ballistic missile.
1. The given altitude of 1200 nary (2209 km) indicates the height above the Earth's surface at which the object is observed. This suggests that the object has already achieved a significant distance from the Earth's surface.
2. The velocity of 7000 m/s indicates the speed at which the object is moving. This high velocity implies that the object is traveling at a considerable speed, likely surpassing the escape velocity of the Earth.
3. The elevation angle (Φ) of +40 degrees describes the angle at which the object's trajectory deviates from the horizontal plane. A positive elevation angle indicates an upward trajectory from the observer's reference point.
4. Based on the given parameters, it can be inferred that the object is following a high-speed ascent trajectory, possibly representing a launch into space. The combination of the high altitude, high velocity, and positive elevation angle suggests that the object is moving away from the Earth's surface and is on a trajectory to reach a higher orbit or escape the Earth's gravitational pull.
5. To find V, v, and Φ when r = 6.378 x 10^6 m, we need additional information or equations related to the specific trajectory or orbital parameters. Without this information, it is not possible to determine these values accurately.
6. A sketch of the trajectory would show an upward path with an increasing altitude, indicating the object's ascent into space. The point where r = 6.378 x 10^6 m would correspond to the Earth's surface, specifically the point of reference for the altitude measurement.
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What do mri and ultrasound have in common as diagnostic imaging techniques? check all that apply.
MRI (Magnetic Resonance Imaging) and ultrasound share common features as diagnostic imaging techniques.
MRI and ultrasound are both non-invasive imaging techniques used in medical diagnostics. They share several similarities:
Non-ionizing radiation: Both MRI and ultrasound utilize non-ionizing radiation, making them safer compared to techniques like X-rays or CT scans that use ionizing radiation. This makes them suitable for various patient populations, including pregnant women and children.
Imaging soft tissues: Both techniques excel in visualizing soft tissues in the body. MRI uses strong magnetic fields and radio waves to produce detailed images of organs, muscles, and other soft tissues. Ultrasound utilizes sound waves to generate real-time images of soft tissues, making it particularly useful for examining organs like the liver, kidneys, and uterus.
Real-time imaging capabilities: Ultrasound and certain types of MRI (such as real-time MRI) offer the ability to capture dynamic, real-time images. This allows for the assessment of organ functionality, blood flow, and movement within the body.
Diagnostic applications: MRI and ultrasound are employed in a wide range of diagnostic applications, including identifying abnormalities, monitoring diseases, guiding procedures, and assessing the effectiveness of treatments.
While there are similarities between MRI and ultrasound, it's important to note that they are distinct imaging techniques with unique strengths and limitations, and their usage depends on specific clinical indications and considerations.
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A gyroscope slows from an initial rate of 29.6 rad/s at an angular acceleration of 0.54 rad/s2. 50% Part (a) How long does it take to come to rest in seconds? t = ?
50% Part (b) How many revolutions does it make before stopping? n= ?
The gyroscope slows from an initial rate of 29.6 rad/s at an angular acceleration of 0.54 rad/s2.
Part (a) How long does it take to come to rest in seconds? t = ?
The angular deceleration is given by the negative value of the angular acceleration; thus:
α = -0.54 rad/s2
The initial velocity is given by the value,
ω1 = 29.6 rad/s.
The final velocity, ω2 = 0 rad/s.
The formula for angular acceleration is:
ω2 = ω1 + αt,
where:
ω1 = 29.6 rad/s
ω2 = 0 rad/s
α = -0.54 rad/s
2t = ?
Substitute the values in the formula above and solve for t.
0 = 29.6 - 0.54tt = 29.6/0.54t = 54.8 seconds
Therefore, it takes 54.8 seconds to come to rest in seconds.
Part (b)The number of revolutions that the gyroscope makes before stopping is given by:
n = (ω1/2π)t,
where:
ω1 = 29.6 rad/s
t = 54.8 s
n = ?
Substitute the values in the formula above and solve for n:
n = (29.6/2π)(54.8) revolutions
n ≈ 277.4
Therefore, the number of revolutions that the gyroscope makes before stopping is approximately 277.4 revolutions.
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about how long does one day last at the north pole on uranus? one day is defined as the time from sunrise to sunset.
On the north pole, one day for about 17 hours on uranus.
Its call is a reference to the Greek god of the sky, Uranus, who, in step with Greek mythology, was the extremely good grandfather of Ares, grandfather of Zeus, and father of Cronus.
Uranus is the only planet whose equator is sort of at a proper attitude to its orbit, with a tilt of 97.77 degrees – likely the end result of a collision with an Earth-sized item lengthy in the past.
The blue-inexperienced color effects from the absorption of crimson light by way of methane gas in Uranus' deep, cold, and remarkably clean surroundings.
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if a man pushes a lawn mower with a force of 20 lb a distance of 60 feet down a yard how many ftlbs of work did he do
The work is given by:
\(W=Fd\)Plugging the values given we have:
\(W=(20)(60)=120\)Therefore the man do 120 ft*lb of work
Jon does 2000 J of work as he starts riding his bicycle from rest. Jon and the bicycle have a combined mass of 90 kg. a. What is the kinetic energy of Jon and the bike after he does the work? b. What is his velocity after he does the work?
Answer:
Part A: 2000J and Part B: 6.67 m/s
Explanation:
I will refer to Kinetic Energy as KE from this point on.
Part A:
Work and KE both have units of Joules because they are related. Work, which is a force acting through a distance, can be redefined as the change in KE like so: W = ΔKE = KE2 - KE1, where KE2 is the final KE and KE1 is the initial KE.
Jon starts from rest, meaning that he initally does not have any KE. Thus, if he does 2000 J of work starting from rest, KE2 = W + KE1 = 2000 J + 0 J = 2000J.
Part B:
Furthermore, since KE = 0.5mv^2, ΔKE = KE2 - KE1 = 0.5m(v2)^2 - 0.5m(v1)^2.
Thus, W = ΔKE = 0.5m(v2)^2 - 0.5m(v1)^2.
We can rewrite this equation to solve for v2: \(v_{2} =\sqrt{\frac{2W}{m}+v_1^{2} }\).
Substituing W = 2000 J, m = 90 kg, and v1 = 0 m/s (since he starts from rest), we get that v2 = 6.67 m/s.
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Which scientist defined the universal law of gravitation?.
Answer:
Newton
Explanation:
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Summarize the main steps an individual should take when developing an action plan.
Mark this and return
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An action plan is an essential document for anyone who wants to achieve a goal. It is a strategy for accomplishing a goal or an objective. The following are the main steps that an individual should take when developing an action plan:
1. Determine the goal or objective: First and foremost, you must identify the objective or goal you want to accomplish. The goal must be specific, measurable, achievable, relevant, and time-bound.
2. Breakdown the goal into smaller tasks: Breaking the goal into smaller, more manageable tasks will make it less daunting. This will make it easier for you to track your progress.
3. Assign a deadline for each task: Every task must have a specific deadline. You must have a realistic timeline for each task.
4. Assign responsibilities: If you are working in a team, you must assign responsibilities. Each team member must know their responsibilities. This ensures that every team member is on the same page.
5. Monitor progress: You must track your progress as you work towards achieving your goal. You can use a project management tool or a spreadsheet to monitor your progress.
6. Evaluate your results: After you have completed your tasks, you must evaluate your results. This will help you identify what worked and what did not. You can use this information to make changes to your action plan.
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satellite to be in a circular orbit 630 km above the surface of the earth.what is the period of the orbit (in hours)?
For a satellite to be in a circular orbit 630 km above the surface of the earth. The period of the orbit of the satellite is approximately 1.45 hours (or 1 hour and 27 minutes).
To calculate the period of the orbit of a satellite, we use the formula T = 2π√(\(r^3\)/GM), where T is the period in seconds, r is the radius of the orbit, G is the gravitational constant (6.674 × \(10^{-11} m^3 kg^{-1} s^{-2}\)), and M is the mass of the Earth (5.972 × \(10^{24}\) kg).
First, we need to convert the altitude of the satellite (630 km) to the radius of the orbit. We know that the radius of the Earth is 6,371 km, so the total distance from the centre of the Earth to the satellite is 6,371 km + 630 km = 7,001 km.
Therefore, the radius of the orbit is r = 7,001 km. Plugging this value into the formula, we get:
T = 2π√(\((7,001 km)^3\)/(6.674 × \(10^{-11} m^3 kg^{-1} s^{-2}\) × 5.972 × \(10^{24}\) kg))
Simplifying this expression, we get:
T = 5.21 × \(10^3\) seconds
To convert this to hours, we divide by 3600 (the number of seconds in an hour):
T = 1.45 hours
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The coldest clouds in the ISM are molecular clouds, so named because their temperatures are low enough and their densities high enough for atoms to join together into molecules. These clouds are capable of collapsing to form new stars, in a stellar nursery like the one in the left image. The Pleiades (right image) is an example of stars that formed recently within such a nursery.
Molecular clouds range in mass from a few times the mass of our Sun (solar masses) to 10 million solar masses. Individual stars range from 0.08 to about 150 solar masses.
What does all of this imply about how stars form from molecular clouds?
Stars form from molecular clouds through a process known as stellar formation.
These clouds, characterized by low temperatures and high densities, provide the ideal conditions for atoms to combine and form molecules. With a mass range spanning from a few solar masses to millions of solar masses, molecular clouds serve as the birthplaces of new stars. The Pleiades cluster serves as a notable example of stars that have recently formed within such a stellar nursery.
The formation of stars from molecular clouds involves several key steps. Firstly, gravitational forces acting on regions of higher density within the cloud cause them to collapse under their own gravity. As the cloud collapses, it begins to fragment into smaller, denser clumps called protostellar cores. These cores continue to collapse, and their central regions become increasingly dense and hot. At this stage, they are known as protostars.
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Which of these statements is true of the brightest stars? AO They are yellow stars.BO Many are supergiantsCO Several are white dwarfs.DO Each is part of the main sequence.
The statement is true about the brightest stars
Many are supergiants.
Hence, the correct option is A.
The brightness of a star is often correlated with its size and temperature. Supergiant stars are among the largest and brightest stars in the universe. They have high luminosity and are located in the upper-right region of the Hertzsprung-Russell (H-R) diagram. These stars can vary in color, with some being blue or white, while others may appear orange or red.
While there are certainly bright stars that are not supergiants, such as certain main sequence stars, white dwarfs, or even some giants, the statement "Many are supergiants" is generally true when considering the brightest stars in terms of luminosity.
Therefore, Many brightest stars are supergiants.
Hence, the correct option is A.
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Which are properties of both a gas and a plasma? Check all that apply.
A. Can change shape to conform to a container
B. Has a rigid shape that does not change easily
C. Is made up of free-moving ions and electrons
D. Is compressed more easily than other states
E. Has particles that move freely from place to place
F. Will expand to completely fill a closed container
Answer:
D, E, and F
Explanation:
Like a gas, plasma lacks a fixed volume and shape. Unlike a gas, plasma can conduct electricity and respond to magnetism. That's because plasma contains charged particles called ions. The particles that make up matter are also constantly moving.
The properties of both a gas and a plasma are:
Is compressed more easily than other states.Has particles that move freely from place to place.Will expand to completely fill a closed container.What are the properties of gas and plasma?A gas lacks both a fixed volume and a fixed shape. While certain gases are palpable to humans and can be seen and felt, others are not. The gases oxygen, helium, and air are a few examples. N2, O2, and CO2 are among the gases that make up the Earth's atmosphere.
Both the volume and shape of plasma are illusive. Ionized gases frequently contain plasma, yet plasma differs from a gas in that it has special characteristics. The plasma is electrically conductive because it contains free electrical charges that aren't attached to atoms or ions. A gas can be heated and ionized to create plasma. Stars, lightning, fluorescent lights, and neon signs are a few examples of plasma.
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Which of the following best demonstrates Newton's Third Law?
Question 3 options:
The harder you kick a soccer ball, the faster it accelerates
An object sitting on the ground will stay there until somebody or something pushes it
Wearing a seatbelt prevents you from continuing to move when the car has stopped
When you walk your foot pushes down on the ground while the ground pushes back on your foot
Answer:
when you walk your foot pushes down on the ground, while the ground pushes back on your foot
Explanation:
it was another brainly question, Goodluck :)
An identical book is dropped on four planets of unknown gravity. The book is thrown down on planets W and X, and released from rest on planets Y and Z. The velocity is recorded for some time intervals on each planet, but not all. The missing velocities are blocked out with a gray box. Which of the following lists the planets in order from the greatest acceleration of gravity to the least acceleration of gravity?
We want to compare the gravitational acceleration of different planets by using the given table. The correct option is the last one, so we have:
Planet Y, planet W, planet Z, planet X.
First, we know that the velocity equation is written as:
V(t) = a*t + v₀
Where a is the acceleration and v₀ is the initial velocity.
With this equation, we can find the acceleration in each planet.
Planet W
The initial velocity is v₀ = -3m/s
V(t) = a*t - 3m/s
And we know that at t = 2s, the velocity is -22m/s.
v(2s) = -22m/s = a*2s - 3m/s
-22m/s + 3m/s = a*2s
-19 m/s = a*2s
(-19 m/s)/2s = a = -9.5m/s^2
Now we just do the same thing for each planet.
Planet X:
v₀ = -0.5 m/s
v(1s) = -4.2 m/s = a*1s - 0.5 m/s
-4.2 m/s + 0.5 m/s = a*1s
-3.8 m/s^2 = a
Planet Y:
v₀ = 0 m/s
v(2s) = -21 m/s = a*2s
(-21 m/s)/2s = a = -10.5 m/s^2
Planet Z:
v₀ = 0 m/s
v(1s) = -8 m/s = a*1s
(-8 m/s)/1s = a = -8m/s^2
Then the order from greatest to least is:
Y, W, Z, X
So the correct option is the last one.
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what evidence of water did mars pathfinder find in ares valles?
Answer:
let me explain
Explanation:
so there are a lot of theories that mars had water on it before human life
and the one I know is the rover they sent to mars just found a wave of water so the people say living things use to live on mars way back then
I hope this helped if you want me to change anything ill do it right away
The seismic wave of an earthquake is represented by the equation r = 12.8 sin(θ), where r is measured in miles. the seismic wave is represented by curve having a center on the . the earthquake can be felt miles from its center.
Based on seismic wave of an earthquake represented by the equation r = 12.8 sin(θ), the seismic wave is represented by circular curve having a center on the positive y axis. The earthquake can be felt 6.4 miles from its center.
A seismic wave is defined as a wave of acoustic energy which travels through the Earth surface and plates. These waves are generally caused by movements of tectonic plates in the Earth (earthquakes). It may also be triggered by volcanoes, explosions, and landslides. As earthquake happen, it causes rocks located at a fault line to break or slip, and as a result Earth’s crust sections physically move in relation to one another. The movement of plates causes energy to be released. Two types of seismic waves spread outward from the earthquake center through Earth’s interior and along its surface. Based on the given equation, the seismic wave will be represented by a circular curve with a center on the positive y axis. An earthquake can be felt 6.4 miles from its center if θ = 8.
Note: The question is incomplete. The complete question probably is: The seismic wave of an earthquake is represented by the equation r = 12.8 sin(θ), where r is measured in miles. The seismic wave is represented by ______ (Circular, Rose, Limacon) curve having a center on the ______ (Positive x Axis, Negative x Axis, Positive Y axis, Negative Y axis). If θ = 8, the earthquake can be felt ________ (6.4, 12.8, 25.6) miles from its center.
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4. Which statement summarizes the excerpt? *
a. There are benefits of space junk to future astronauts.
b. Space junk is becoming an increasingly dangerous problem.
c. There are effective ways to get rid of the accumulating space trash.
d. Scientists are developing ways to prevent space junk.
What is determined by the magnitude of intermolecular forces in a liquid and is a measure of a fluid's resistance to flow?.
The fluid's physical property that measures the fluid's resistance to flow is viscosity.
What is fluid viscosity?Fluid's viscosity is a physical property of fluids that measures the fluid's resistance to flow.
Fluid's viscosity decreases with increase in temperature and increases with increase in the intermolecular forces of the fluid.
Thus, the fluid's physical property that measures the fluid's resistance to flow is viscosity.
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what kind of frog species is this
Answer: i think its a bullfrog forgive me if im wrong i dont exactly know
Explanation:
Answer:
that is an African bullfrog
a ball is thrown directly downward with an initial speed of 8.85 m/s, from a height of 29.9 m. after what time interval does it strike the ground?
It takes approximately 0.902 seconds time interval for the ball to strike the ground.
To determine the time interval it takes for the ball to strike the ground, we can use the equations of motion. Since the ball is thrown directly downward, we can assume that the initial velocity (u) is negative (-8.85 m/s), and the acceleration due to gravity (g) is positive (9.8 m/s²).
The equation to calculate the time of flight (t) is
t = (v - u) / g
Where:
v = final velocity (when the ball strikes the ground)
u = initial velocity
g = acceleration due to gravity
In this case, the final velocity when the ball strikes the ground is 0 m/s (as it comes to rest). So, substituting the given values into the equation, we have
t = (0 - (-8.85)) / 9.8
t = 8.85 / 9.8
t = 0.902 seconds
Therefore, it takes approximately 0.902 seconds for the ball to strike the ground.
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