Answer:
Two stars (a and b) can have the same luminosity, but different surface area and temperature if the following condition is met:
(T_a^4)(R_a^2) = (T_b^4)(R_b^2)
Explanation:
The luminosity of a star is the total energy that produces in one second. It depends on the size of the star and its surface temperature.
L = σ(T^4)(4πR^2)
L is the luminosity f the star, T is the temperature of the surface of the star and R is its radius.
Two stars can have the same luminosity if the relation between the radius and the surface temperature is maintained.
To see this lets suposed you have 2 stars, a and b, and the luminosities of each one of them:
L_a = σ(T_a^4)(4πR_a^2)
L_b = σ(T_b^4)(4πR_b^2)
you can assume that L_a and L_b are equal:
σ(T_a^4)(4πR_a^2) = σ(T_b^4)(4πR_b^2)
Now, you can cancel the constants:
(T_a^4)(R_a^2) = (T_b^4)(R_b^2)
as long as this relation between a and b is true, then the luminosity can be the same.
Since WWII, Germany's eastern territories became apart of Poland. "Central Germany" is usually defined as being apart of the federal states of Saxony Thuringia and Saxony-Anhalt. It has even been said to be apart of a smaller part of this region, such as the metropolitan area of Leipzig and Halle as well as surrounding countries.
Not completely sure cuz I don’t know what the required reading is, but the US is probably the most dependent on imported oil
<span>Faults that are undergoing movement (i.e. displacement of rock
strata) that is essentially horizontal in direction and parallel to the strike
of the fault surface are called Strike-slip faults. </span>Other names for Strike-slip faults<span> are transcurrent faults, wrench
faults, or lateral faults.</span>
