Answer:
0.0133A
Explanation:
Since we have two sections, for the Inductor region there would be a current
. In the case of resistance 2, it will cross a current
Defined this we proceed to obtain our equations,
For
,
![\frac{di_1}{dt}+i_1R_1 = V](https://tex.z-dn.net/?f=%5Cfrac%7Bdi_1%7D%7Bdt%7D%2Bi_1R_1%20%3D%20V)
![I_1 = \frac{V}{R_1} (1-e^{-\frac{R_1t}{L}})](https://tex.z-dn.net/?f=I_1%20%3D%20%5Cfrac%7BV%7D%7BR_1%7D%20%281-e%5E%7B-%5Cfrac%7BR_1t%7D%7BL%7D%7D%29)
For
,
![I_2R_2 =V](https://tex.z-dn.net/?f=I_2R_2%20%3DV)
![I_2 = \frac{V}{R_2}](https://tex.z-dn.net/?f=I_2%20%3D%20%5Cfrac%7BV%7D%7BR_2%7D)
The current in the entire battery is equivalent to,
![i_t = I_1+I_2](https://tex.z-dn.net/?f=i_t%20%3D%20I_1%2BI_2)
![i_t = \frac{V}{R_2}+\frac{V}{R_1} (1-e^{-\frac{R_1t}{L}})](https://tex.z-dn.net/?f=i_t%20%3D%20%5Cfrac%7BV%7D%7BR_2%7D%2B%5Cfrac%7BV%7D%7BR_1%7D%20%281-e%5E%7B-%5Cfrac%7BR_1t%7D%7BL%7D%7D%29)
Our values are,
![V=1V](https://tex.z-dn.net/?f=V%3D1V)
![R_1 = 95\Omega](https://tex.z-dn.net/?f=R_1%20%3D%2095%5COmega)
![L= 1.5*10^{-2}H](https://tex.z-dn.net/?f=L%3D%201.5%2A10%5E%7B-2%7DH)
![R_2 =360\Omega](https://tex.z-dn.net/?f=R_2%20%3D360%5COmega)
Replacing in the current for t= 0.4m/s
![i=\frac{1}{360}+\frac{1}{95}(1-e^{-\frac{95*0.4}{1.5*10^{-2}}})](https://tex.z-dn.net/?f=i%3D%5Cfrac%7B1%7D%7B360%7D%2B%5Cfrac%7B1%7D%7B95%7D%281-e%5E%7B-%5Cfrac%7B95%2A0.4%7D%7B1.5%2A10%5E%7B-2%7D%7D%7D%29)
![i= 0.0133A](https://tex.z-dn.net/?f=i%3D%200.0133A)
![i_1 = 0.01052A](https://tex.z-dn.net/?f=i_1%20%3D%200.01052A)
It is eight times more than the star A.
<h3>What is luminosity and on which it depends?</h3>
The luminosity of an object is a measure of its intrinsic brightness and is defined as the amount of energy the object emits in a fixed time.
luminousity depends upon the two factors are:
1) The star's actual brightness
Some stars are naturally more luminous than others ,so the brightness level from one star to next star is significantly different.
2) The star distance from us
The more distance of an object the dimmer it appears.
Energy emitted = sAT⁴
where s is stefan constant
A is surface area and T is temperature .
to learn more about Luminosity click here brainly.com/question/14140223
#SPJ4
Answer: Two celestial objects are in space: one with a mass of 8.22 x 109 kg and one with a mass of 1.38 x 108 kg. If they are separated by a distance of 1.43 km, then, the magnitude of the force of attraction (in newtons) between the objects will be 52.9kN
Explanation: To find the answer we need to know more about the Newton's law of gravitation.
<h3>What is Newton's law of gravitation?</h3>
- Gravitation is the force of attraction between any two bodies.
- Every body in the universe attracts every other body with a force.
- This force is directly proportional to the product of their masses and inversely proportional to the square of the distance between these two masses.
- Mathematically we can expressed it as,
![F=\frac{GMm}{r^2} \\where, G=6.67*10^-11Nm^2kg^-2](https://tex.z-dn.net/?f=F%3D%5Cfrac%7BGMm%7D%7Br%5E2%7D%20%5C%5Cwhere%2C%20G%3D6.67%2A10%5E-11Nm%5E2kg%5E-2)
<h3>How to solve the problem?</h3>
- Here, we have given with the data's,
![M=8.22*10^9kg\\m=1.38*10^8 kg\\r=1.43*10^3m](https://tex.z-dn.net/?f=M%3D8.22%2A10%5E9kg%5C%5Cm%3D1.38%2A10%5E8%20kg%5C%5Cr%3D1.43%2A10%5E3m)
- Thus, the force of attraction between these two bodies will be,
![F=6.67*10^-11*\frac{8.22*10^9*1.38*10^8}{1.43*10^3} =52.9kN](https://tex.z-dn.net/?f=F%3D6.67%2A10%5E-11%2A%5Cfrac%7B8.22%2A10%5E9%2A1.38%2A10%5E8%7D%7B1.43%2A10%5E3%7D%20%3D52.9kN)
Thus, if two celestial objects are in space: one with a mass of 8.22 x 109 kg and one with a mass of 1.38 x 108 kg and, If they are separated by a distance of 1.43 km, then, the magnitude of the force of attraction (in newtons) between the objects will be 52.9kN.
Learn more about the Newton's law of gravitation here:
brainly.com/question/28045318
#SPJ4
They differ from each other<span> in wavelength. Wavelength is the distance between </span>one wave<span> crest to the next. </span>Waves<span> in the </span>electromagnetic<span> spectrum vary in size from very long radio </span>waves<span> the size of buildings, to very short gamma-rays smaller </span>than<span> the size of the nucleus of an atom.</span>