Because the core is a big ball of iron
Energy slowly leaks outward through the radiative diffusion of photons that repeatedly bounce off ions and electrons.
<h3>What is radiative diffusion?</h3>
A radiation zone is a layer of a star's core where energy is mostly carried toward the outside by radiative diffusion and thermal conduction rather than convection.
As photons, energy passes through the radiation zone as electromagnetic radiation.
The radiative diffusion of photons that repeatedly bounce off ions and electrons progressively drains energy outward.
Hence,radiative diffusion is correct answer.
To learn more about radiative diffusion refer:
brainly.com/question/3598352
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Answer:
37.725 A
Explanation:
B = magnitude of the magnetic field produced by the electric wire = 0.503 x 10⁻⁴ T
r = distance from the wire where the magnetic field is noted = 15 cm = 0.15 m
i = magnitude of current flowing through the wire = ?
Magnetic field by a long wire is given as
![B = \frac{\mu _{o}}{4\pi }\frac{2i}{r}](https://tex.z-dn.net/?f=B%20%3D%20%5Cfrac%7B%5Cmu%20_%7Bo%7D%7D%7B4%5Cpi%20%7D%5Cfrac%7B2i%7D%7Br%7D)
Inserting the values
![0.503\times 10^{-4} = (10^{-7})\frac{2i}{0.15}](https://tex.z-dn.net/?f=0.503%5Ctimes%2010%5E%7B-4%7D%20%3D%20%2810%5E%7B-7%7D%29%5Cfrac%7B2i%7D%7B0.15%7D)
i = 37.725 A
Answer:
258774.9441 m
Explanation:
x = Distance of probe from Earth
y = Distance of probe from Sun
Distance between Earth and Sun = ![x+y=149.6\times 10^6\ m](https://tex.z-dn.net/?f=x%2By%3D149.6%5Ctimes%2010%5E6%5C%20m)
G = Gravitational constant
= Mass of Sun = ![1.989\times 10^{30}](https://tex.z-dn.net/?f=1.989%5Ctimes%2010%5E%7B30%7D)
= Mass of Earth = ![5.972\times 10^{24}\ kg](https://tex.z-dn.net/?f=5.972%5Ctimes%2010%5E%7B24%7D%5C%20kg)
According to the question
![\frac{GM_sm}{x^2}=\frac{GM_em}{y^2}\\\Rightarrow \frac{M_s}{x^2}=\frac{M_e}{y^2}\\\Rightarrow x=\sqrt{\frac{M_s\times y^2}{M_e}}\\\Rightarrow x=\sqrt{\frac{1.989\times 10^{30}\times y^2}{5.972\times 10^{24}}}\\\Rightarrow x=577.10852y](https://tex.z-dn.net/?f=%5Cfrac%7BGM_sm%7D%7Bx%5E2%7D%3D%5Cfrac%7BGM_em%7D%7By%5E2%7D%5C%5C%5CRightarrow%20%5Cfrac%7BM_s%7D%7Bx%5E2%7D%3D%5Cfrac%7BM_e%7D%7By%5E2%7D%5C%5C%5CRightarrow%20x%3D%5Csqrt%7B%5Cfrac%7BM_s%5Ctimes%20y%5E2%7D%7BM_e%7D%7D%5C%5C%5CRightarrow%20x%3D%5Csqrt%7B%5Cfrac%7B1.989%5Ctimes%2010%5E%7B30%7D%5Ctimes%20y%5E2%7D%7B5.972%5Ctimes%2010%5E%7B24%7D%7D%7D%5C%5C%5CRightarrow%20x%3D577.10852y)
![x+y=149.6\times 10^6\\\Rightarrow 577.10852y+y=149.6\times 10^6\\\Rightarrow 578.10852y=149.6\times 10^6\\\Rightarrow y=\frac{149.6\times 10^6}{578.10852}\\\Rightarrow y=258774.9441\ m](https://tex.z-dn.net/?f=x%2By%3D149.6%5Ctimes%2010%5E6%5C%5C%5CRightarrow%20577.10852y%2By%3D149.6%5Ctimes%2010%5E6%5C%5C%5CRightarrow%20578.10852y%3D149.6%5Ctimes%2010%5E6%5C%5C%5CRightarrow%20y%3D%5Cfrac%7B149.6%5Ctimes%2010%5E6%7D%7B578.10852%7D%5C%5C%5CRightarrow%20y%3D258774.9441%5C%20m)
The probe should be 258774.9441 m from Earth
Answer:
The gravitational potential energy of a system is -3/2 (GmE)(m)/RE
Explanation:
Given
mE = Mass of Earth
RE = Radius of Earth
G = Gravitational Constant
Let p = The mass density of the earth is
p = M/(4/3πRE³)
p = 3M/4πRE³
Taking for instance,a very thin spherical shell in the earth;
Let r = radius
dr = thickness
Its volume is given by;
dV = 4πr²dr
Since mass = density* volume;
It's mass would be
dm = p * 4πr²dr
The gravitational potential at the center due would equal;
dV = -Gdm/r
Substitute (p * 4πr²dr) for dm
dV = -G(p * 4πr²dr)/r
dV = -G(p * 4πrdr)
The gravitational potential at the center of the earth would equal;
V = ∫dV
V = ∫ -G(p * 4πrdr) {RE,0}
V = -4πGp∫rdr {RE,0}
V = -4πGp (r²/2) {RE,0}
V = -4πGp{RE²/2)
V = -4Gπ * 3M/4πRE³ * RE²/2
V = -3/2 GmE/RE
The gravitational potential energy of the system of the earth and the brick at the center equals
U = Vm
U = -3/2 GmE/RE * m
U = -3/2 (GmE)(m)/RE