Explanation:
The brightness of the Sun is incredibly intense and blinding.
The Sun is the brightest object in the sky and produces immense amounts of energy that provide heat and light to the Earth.
The brightness of the Sun is incredibly intense and blinding. The Sun is the brightest object in the sky and produces immense amounts of energy that provide heat and light to the Earth.
The brightness of the Sun can also be described in terms of its apparent magnitude, which is a measure of how bright a star appears from Earth's vantage point. The Sun has an apparent magnitude of -26.74, which is about 400,000 times brighter than the full moon and about 130,000 times brighter than Earth's next brightest star, Sirius.
The brightness of the Sun can be dangerous to the human eye if viewed directly without proper protection. Looking at the Sun for even a few seconds can cause permanent eye damage or blindness.
It is important to use special solar filters or eclipse glasses when viewing the Sun to protect the eyes from the harmful effects of its intense brightness.
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The brightness of the Sun can be described as extremely bright, as it is the main source of light and energy for our solar system.
The Sun is an extremely bright object. Its brightness is due to the intense radiation it emits, primarily in the form of visible light and other forms of electromagnetic radiation, such as ultraviolet and infrared radiation.
The brightness of the Sun can be measured in a number of ways. One common measure is its apparent magnitude, which is a measure of how bright the Sun appears from Earth. The Sun has an apparent magnitude of about -26.7, which is much brighter than any other object in the sky.
Overall, the brightness of the Sun is one of the most striking and impressive features of our solar system, and it plays a critical role in sustaining life on Earth through photosynthesis and other processes.
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Advanced Wireless Services (AWS) is a wireless telecommunications spectrum band used for mobile voice and data services, video, and messaging. The AWS band uses frequencies in several segments: from 1695 to 2200 MHz. a) Determine the corresponding range of wavelengths used by the AWS mobile devices. b) To what region/band of electromagnetic spectrum does the range belong
Given data
*The given frequency is
\(f_1_{}=1695\text{ MHz}=1695\times10^6\text{ Hz}\)*The another given frequency is
\(f_2=2200\text{ MHz=}2200\times10^6\text{ Hz}\)*The given speed of light is c = 3.0 × 10^8 m/s
(a)
The formula for the wavelength is given as
\(\lambda_1=\frac{c}{f_1}\)Substitute the known values in the above expression as
\(\begin{gathered} \lambda_1=\frac{(3\times10^8)}{(1695\times10^6)^{}} \\ =0.176\text{ m} \end{gathered}\)The another wavelength for the another frequency is calculated as
\(\begin{gathered} \lambda_2=\frac{c}{f_2} \\ =\frac{(3.0\times10^8)}{(2200\times10^6)} \\ =0.136\text{ m} \end{gathered}\)(b)
Radio spectrum is an electromagnetic spectrum where the frequency range belongs of wireless telecommunication.
WHY is the answer B? Please give scientifically sound explanation. Will give brainliest.
The ball would stationary at the maximum height and accelerated greatly as it falls until it comes to rest on the ground. Option B
What is the velocity time graph for an object thrown up?The slope of the velocity-time graph represents the acceleration of the object. At the highest point of the object's trajectory, the acceleration is zero, as it is temporarily at rest. As the object starts to fall, its acceleration becomes negative, indicating that it is accelerating downwards due to the force of gravity.
The velocity-time graph is a useful tool for analyzing the motion of an object and understanding its velocity and acceleration at different points in time.
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help pleaseeeee!! What is something that you would like to see a physicist develop in the future?
Teleportation (artificial or natural over wormhole).
You push on a 30 kg box with a force of 120 N. What is the acceleration of the box2
Answer:
6
Explanation:
120/30=6
Approximately how long does it take the uterus lining to build up again after menstruation
The uterus lining is rebuilt by the end of the menstrual period. The rebuilding of the uterus lining starts after menstruation and the lining is typically completely rebuilt by day 14 of the menstrual cycle, which is when ovulation occurs and the uterus is preparing to potentially receive a fertilized egg.
The endometrium is the inner lining of the uterus, and it thickens every month to prepare for pregnancy. After menstruation, the endometrium grows and thickens to prepare for the implantation of a fertilized egg. The cells in the lining multiply and enlarge, and the glands in the lining begin to secrete mucus and other substances that help support the fertilized egg and promote its growth.
The rebuilding of the endometrium usually takes about two weeks after menstruation. This process is closely regulated by hormones such as estrogen and progesterone, which are produced by the ovaries and other parts of the body. These hormones help control the growth and development of the endometrium and other reproductive tissues.
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Explain how friction affects the work done by machines.
Friction affects the work done by machines by reducing the mechanical advantage of that machine.
MA = \(F_{o}\) / \(F_{i}\)
MA = Mechanical advantage
\(F_{o}\) = Output force
\(F_{i}\) = Input force
Mechanical advantage is the ratio of output force to input force in a system.
According to law of conservation of energy, input energy is equal to output energy. It is true in the machines also but some of the output energy is not necessarily asked of the machine. That energy which is not useful is heat produced due to friction.
Therefore, friction affects the work done by machines by reducing the mechanical advantage of that machine.
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i NEED THE RIGHT ANSWER FOR THIS ASAP NO LINKS !!!
Answer:
it is the dependent since it keeps changing over time get it :)
Explanation:
can you tell Which body part does not help in the perception and production of sound in humans?
ears, lungs, mouth or vocal cords
which is not?
Lungs do not help in the perception and production of sound in humans.
What are lungs?Gaseous exchange occurs during inhalation and exhale during breathing. Main components of the human respiratory system include the nose, mouth, throat, larynx, trachea, bronchi, and lungs.
In humans and other vertebrates, the primary organs for respiration are the lungs. They are situated in the thoracic cavity of the chest, on either side of the heart. The lungs are spongy, anatomically speaking, with a total surface area that ranges from 50 to 75 square meters.
The lungs' main job is to make it easier for gases to move from the blood into the air. It's interesting to note that the right lung is significantly larger and heavier than the left.
Hence, lungs do not help in the perception and production of sound in humans.
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can someone explain how to solve this?
an electrically charged object can be used to attract:
An electrically charged object can be used to attract any object with an opposite charge.
This is due to the fundamental principle that opposites attract and repel in physics.
Electric charge is a fundamental property of matter that gives rise to electromagnetic interactions. An electric charge, whether positive or negative, produces an electric field that surrounds it. This field exerts a force on any other charge in its vicinity that is either attracted to or repelled from it. Electric charge is a fundamental property of matter that produces a variety of electric phenomena. When the charge is concentrated in a localized region of space, the object is electrically charged. When there is a net accumulation of charge in an object, it becomes electrically charged. An electrically charged object produces an electric field in its vicinity, which exerts a force on other charged objects. An electrically charged object can be used to attract objects with an opposite charge or repel objects with the same charge.
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A car is traveling in a race. The car went from the initial velocity of 35 m/s to the final velocity of 65 m/s in 5 seconds
What is the acceleration?
- 13 m/s
om/
6 m/s
13 m/s
Answer:
6m/s
Explanation:
a = (v-u)/t
acceleration, a
initial velocity, u
final velocity, v
time, t
substitute values and you'll get the answer
Answer:
6 m/s
Explanation:
what two things does the strength of gravity depend on?
Answer:
i found this i hope it helps
Explanation:
The magnitude of this force depends upon the mass of each object and the distance between the centers of the two objects. Mathematically, we say the force of gravity depends directly upon the masses of the objects and inversely upon the distance between the objects squared.
In a wild shot, bo flings a pool ball of mass m off a 0. 68 m high pool table, and the ball hits the floor with a speed of 6. 0 m/s. How fast was the ball moving when it left the table?.
The initial velocity of the ball when it left the table is 4.7 m/s.
What is the initial velocity of the ball?The initial velocity of the ball is calculated by applying the following kinematic equation as shown below.
vf² = vi² + 2gh
where;
vi is the initial velocity of the ball when it left the tablevf is the final velocity of the ball when it hits the groundh is the height of fall of the ballg is acceleration due to gravityvi² = vf² - 2gh
vi = √(vf² - 2gh)
vi = √(6² - (2 x 9.8 x 0.68) )
vi = 4.76 m/s
Thus, the initial velocity of the ball when it left the table is a function of the final velocity when it hits the ground and the height of fall of the ball.
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10-4. calculate the required diameter for certified-capacity liquid rupture discs for the following conditions. assume a liquid specific gravity of 1.2 for all cases. Liquid flow Set pressure Overpressure Backpressure a. 500 gpm b. 100 gpm c. 5 m/s d. 10 m/s 100 psig 50 psig 10 barg 20 barg 10 psig 5 psig 1 barg 2 barg 5 psig 2 psig 0.5 barg 1 barg
The required diameter for certified-capacity liquid rupture discs for the given conditions are 6.08 inches for 500 gpm, 3.07 inches for 100 gpm, 1.29 inches for 5 m/s, and 1.60 inches for 10 m/s.
To calculate the required diameter for certified-capacity liquid rupture discs for the given conditions, we first need to determine the burst pressure for each case. The burst pressure is calculated using the following formula:
Burst Pressure = Set Pressure + Overpressure - Backpressure
Using the specific gravity of 1.2 for all cases, we can calculate the burst pressure for each scenario as follows:
a. 500 gpm: Burst Pressure = 100 psig + 50 psig - 10 psig = 140 psig
b. 100 gpm: Burst Pressure = 100 psig + 50 psig - 5 psig = 145 psig
c. 5 m/s: Burst Pressure = 10 barg + 1 barg - 0.5 barg = 10.5 barg
d. 10 m/s: Burst Pressure = 20 barg + 2 barg - 1 barg = 21 barg
Once we have the burst pressure, we can use the specific gravity and the following formula to calculate the required diameter of the rupture disc:
Diameter = (Flow Rate * 60 * Specific Gravity) / (Burst Pressure * 0.8 * 3.14)
Where:
Flow Rate = Liquid flow in gallons per minute (gpm) or meters per second (m/s)
Specific Gravity = 1.2
Burst Pressure = Calculated burst pressure in psig or barg
Using the above formula, we can calculate the required diameter for each scenario as follows:
a. 500 gpm: Diameter = (500 * 60 * 1.2) / (140 * 0.8 * 3.14) = 6.08 inches
b. 100 gpm: Diameter = (100 * 60 * 1.2) / (145 * 0.8 * 3.14) = 3.07 inches
c. 5 m/s: Diameter = (5 * 60 * 1.2) / (10.5 * 0.8 * 3.14) = 1.29 inches
d. 10 m/s: Diameter = (10 * 60 * 1.2) / (21 * 0.8 * 3.14) = 1.60 inches
Therefore, the required diameter for certified-capacity liquid rupture discs for the given conditions are 6.08 inches for 500 gpm, 3.07 inches for 100 gpm, 1.29 inches for 5 m/s, and 1.60 inches for 10 m/s.
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How deep is the floor of the ocean if a sonar sound takes 7 seconds to return back to the ship?
⚠️ HELPPPP PLEASE ⚠️
Which of the following was established by the Continental Congress?
O The Smithsonian
O The Supreme Court
O The US Post Office
O the Continental Army
Answer:
The second Continental Congress started the Continental Army
Explanation:
The Smithsonian was established by the continental congress
What happens when condensation causes clouds to become very heavy?
a
evaporation
b
condensation
c
precipitation
d
accumulation
Answer:
C. precipitation
Explanation:
if clouds store too much water from evaporation, it will rain which is precipitation
This part of the bike consists of hubs, spokes, rims, and tires (more that answer)
saddle
wheels
crank
brakes
Answer:
wheels
Explanation:
Answer:
Wheels
Explanation:
I know it says check all that apply so you might think it's more than one, but trust me it's right. I took the test :)
Why the car floated before it started to sink? Explain.
Alice and Julio’s company makes protective coverings for off-roading vehicles. Alice’s job involves harvesting a natural polymer from trees. Julio’s job is to take that material and change it chemically to create a synthetic polymer.
Which materials do Alice and Julio most likely work with?
Alice works with vulcanized rubber, and Julio works with natural rubber.
Alice works with natural rubber, and Julio works with vulcanized rubber.
Alice works with cellulose, and Julio works with nylon.
Alice works with nylon, and Julio works with cellulose.
Answer:
Alice works with natural rubber and Julio works with vulcanised rubber.
Explanation:
Natural rubber is a polymer from tree.So it satisfies the profession of Alice.vulcanised rubber is artificial or synthetic polymer.So it satisfies the profession of JulioAnswer:
B. Alice works with natural rubber, and Julio works with vulcanized rubber.
Explanation:
I just took the test and got 100 percent.
I hope this helps you!!!!
Please mark my answer the Brainiset. Thank You!!!!!
if an absorption line of calcium is normally found at a wavelength of 393.4 nm in a laboratory gas, and you measure it to be at 423.6 nm in the spectrum of a galaxy, what is the approximate distance to the galaxy?
The approximate distance to the galaxy is 78.7 million light-years.
The shift in the absorption line wavelength can be attributed to the Doppler effect, specifically the redshift caused by the expansion of the universe. We can use Hubble's law to estimate the distance to the galaxy. Hubble's law states that the recessional velocity of a galaxy is proportional to its distance from us. The equation is v = H0 * d, where v is the recessional velocity, H0 is the Hubble constant, and d is the distance. Rearranging the equation, we have d = v / H0. The redshift of the absorption line corresponds to the recessional velocity of the galaxy. By knowing the redshift and the Hubble constant, we can calculate the approximate distance. Considering the redshift from the given wavelength shift and using a Hubble constant of 70 km/s/Mpc, we find that the approximate distance to the galaxy is 78.7 million light-years.
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So far, you’ve been working with an "ideal" pulley system. How do you think real pulley systems are different, and how would that affect the mechanical advantage of real pulley systems?
Plz really need help with this. And thank you so much
Answer:
In an ideal pulley system is assumed as a perfect system, and the efficiency of the pulley system is taken as 100% such that there are no losses of the energy input to the system through the system's component
However, in a real pulley system, there are several means through which energy is lost from the system through friction, which is converted into heat, sound, as well as other forms of energy
Given that the mechanical advantage = Force output/(Force input), and that the input force is known, the energy loss comes from the output force which is then reduced, and therefore, the Actual Mechanical Advantage (AMA) is less than the Ideal Mechanical Advantage of an "ideal" pulley system
The relationship between the actual and ideal mechanical advantage is given by the efficiency of the pulley system as follows;
\(Efficiency \, \% = \dfrac{AMA}{IMA} \times 100\)
Explanation:
Write the calculations of the wavelengths by ° for any two
selected lines from the Balmar series of the spectra of
hydrogen
The wavelength of the second line in the Balmer series is 304 nm and fourth line is 1093.7 nm.
The Balmer series in the hydrogen spectrum has spectral lines that are in the visible spectrum.
The wavelength is determined using the Balmer-Rydberg equation.
Wavelength for any two selected lines from the Balmer series of the spectra of hydrogen,
1 / λ = R (1/ n₁² - 1/ n₂²)
Where,
λ is the wavelength,
R is the Rydberg constant (1.0974 x 10⁷ m⁻¹),
n₁ and n₂ are integers where n₂ > n₁.
First, let us choose n₁ = 2, which is the second energy level and we will calculate the wavelength of the second line.
n₂ = 3λ = R(1/2² - 1/3²)
λ = R (4/36 - 1/9)
λ = R (1/36) = (1.0974 x 10⁷ m⁻¹) / 36
λ = 3.04 x 10⁻⁷ m = 304 nm
The wavelength of the second line in the Balmer series is 304 nm.
Now, we will calculate the wavelength of the fourth line.
n₂ = 5n₁ = 2λ = R (1/2² - 1/5²)
λ = R (4/100 - 1/25)
λ = R (3/100) = (1.0974 x 10⁷ m⁻¹) / 100 x 3
λ = 1.0937 x 10⁻⁷ m = 1093.7 nm
The wavelength of the fourth line in the Balmer series is 1093.7 nm.
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when the force acting on the body equal to acceleration?
Answer:
Acceleration and velocity Newton's second law says that when a constant force acts on a massive body, it causes it to accelerate, i.e., to change its velocity, at a constant rate. In the simplest case, a force applied to an object at rest causes it to accelerate in the direction of the force.
Would their position with respect to the horizon change if the earth were only 200 miles in diameter? how about 80,000 miles in diameter? why is that?
The position with respect to the horizon would change significantly if the Earth were only 200 miles in diameter, while there would be minimal change if the Earth were 80,000 miles in diameter.
If the Earth were only 200 miles in diameter, the position of objects with respect to the horizon would change significantly. Due to the small size of the Earth, the curvature of the planet would be extremely pronounced. As a result, objects located only a short distance away would appear to be close to the horizon or even below it. The horizon itself would be much closer, and the overall view would be limited.
On the other hand, if the Earth were 80,000 miles in diameter, the position of objects with respect to the horizon would hardly change. With such a large diameter, the Earth's curvature would be less noticeable, and objects at various distances would still appear at or near the horizon.
The change in position with respect to the horizon is determined by the curvature of the Earth. When the Earth is smaller, the curvature is more pronounced, causing objects to appear closer to the horizon. When the Earth is larger, the curvature is less noticeable, resulting in little change in the position of objects with respect to the horizon.
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Minerals and vitamins are called
Answer:
micronutrients.
Explanation:
1. The finite sheet 0≤x≤1,0≤y≤1 on the z=0 has a charge density rho s=xy(x 2+y 2+25) 2 3 nC/m 2
. Find the total charge on the sheet. Note: Q=∫ srho sds where ds=dxdy.
To calculate the total charge on a finite sheet 0≤x≤1, 0≤y≤1 on the z=0 that has a charge density of rho s=xy(x 2+y 2+25) 2 3 n C/m 2. First, we need to use the formula Q=∫s ρs ds where ds=dx dy. the total charge on the sheet is 111.31 nC.
Where ρs is the charge density and s is the surface area of the sheet. The surface area of the sheet is given by s=∫∫dx dy.
Therefore, Q=∫s ρs ds=∫∫ρs dx dy.
From the question, ρs=xy(x2+y2+25)^2/3
Therefore,
Q=∫∫x y(x2+y2+25)2/3dxdy = ∫01∫01xy(x2+y2+25)2/3dx dy
Separating out the terms containing y, we obtain;
Q=∫01ydy∫01x(x2+25)2/3dx + ∫01ydy∫01xy2(x2+25)2/3dx ∫01ydy∫01y(x2+y2+25)2/3dx
On integrating, we get;
Q =1/4 [(14+245)(5/3)+(14+245)(5/3)(2/5)+(14+245)(5/3)(2/5)]
=111.31 n C
Therefore, the total charge on the sheet is 111.31 nC.
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find VTh without using kvl or kcl
or algebraically cant tou find it by voltage
divider? thanks
Using Thevenin's theorem, determine the current
through the load RL in Figure 8-82.
10 kQ
10 kQ
10 kf2 VOUT
32 V-
W
5.6 kn
5.6 kQ
15 kQ
A FIGURE 8-82... Show more"
To find the Thevenin voltage (VTh) without using Kirchhoff's voltage law (KVL) or Kirchhoff's current law (KCL), we can apply the voltage divider rule. The voltage divider rule states that the voltage across a resistor in a series circuit is proportional to its resistance.
In Figure 8-82, we need to determine the current through the load RL. To do this, we first find the Thevenin voltage (VTh) which is the open-circuit voltage across the load terminals. Here's how we can find it using the voltage divider rule:
Identify the two resistors in series: The 5.6 kQ resistor and the 15 kQ resistor.
Calculate the total resistance (RT) of the series combination: RT = 5.6 kQ + 15 kQ = 20.6 kQ.
Identify the resistor across which you want to find the voltage: In this case, it is the 15 kQ resistor.
Apply the voltage divider rule: \(VTh = (R2 / (R1 + R2)) * VSource\).
- Substitute the values: \(VTh = (15 kQ / (5.6 kQ + 15 kQ)) * 32 V\).
- Simplify the expression:\(VTh = (15 kQ / 20.6 kQ) * 32 V\).
- Calculate VTh:\(VTh ≈ 23.44 V\).
Therefore, the Thevenin voltage (VTh) is approximately 23.44 V.
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What is the equivalent resistance of the circuit?
Answer:
5.5Ω
Explanation:
The circuit diagram shown is a parallel arrangement. To solve this problem for the equivalent resistance,
R1 = 10Ω
R2 = 20Ω
R3 = 30Ω
For circuits in parallel, equivalent resistance is ;
\(\frac{1}{Rt}\) = \(\frac{1}{R1} + \frac{1}{R2} + \frac{1}{R3}\)
Now insert the parameters and solve;
\(\frac{1}{Rt}\) = \(\frac{1}{10} + \frac{1}{20} + \frac{1}{30}\)
\(\frac{1}{Rt}\) = \(\frac{6 + 3 + 2}{60}\)
\(\frac{1}{Rt}\) = \(\frac{11}{60}\)
Rt = 5.5Ω
at what distance from a 18 mw point source of electromagnetic waves is the electric field amplitude 0.030 v/m ?
At a distance of approximately 1949.64 meters from the 18 MW point source of electromagnetic waves, the electric field amplitude will be 0.030 V/m.
To find the distance from an 18 MW point source of electromagnetic waves where the electric field amplitude is 0.030 V/m, you can follow these steps:
1. Calculate the power of the source in watts: 18 MW * 10^6 = 18,000,000 W
2. Use the formula for the intensity (I) of the electromagnetic waves: I = Power / (4 * π * distance²)
3. Substitute the given electric field amplitude (E) and calculate the intensity using the formula: I = E² / (2 * μ₀ * c), where μ₀ is the permeability of free space (4 * π * 10^(-7) Tm/A) and c is the speed of light (3 * 10^8 m/s).
I = (0.030²) / \((2 * (4 * π * 10^(-7)) * (3 * 10^8)\)) ≈ 1.1953 W/m²
4. Solve for the distance in the intensity formula. 1.1953 = 18,000,000 / (4 * π * distance²)
distance² ≈ 18,000,000 / (4 * π * 1.1953) ≈ 3,804,099.39
distance ≈ √3,804,099.39 ≈ 1949.64 m
At a distance of approximately 1949.64 meters from the 18 MW point source of electromagnetic waves, the electric field amplitude will be 0.030 V/m.
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