A. Location will be categorized with 3. Northern Hemisphere, Eastern Hemisphere. These are all broad geographical locations and are termed based on a large area.
B, Place will be categorized with Coastal East Asia, the subcontinent, Southeast Asia, the Himalayas and the Steppes. These are all places within a broader location and are part of a smaller geographical area.
C. Region will be categorized with 2.Climate varies: Deserts, rain forests, monsoon regions and moderate regions. These areas are influenced by climate within a specific geographical place and location, thus regions are established based on the reaches of the climate.
D. Movement will be categorized with 1. Long history of isolationism, with recent European culture spread affecting Asian countries. The migration of Europeans and their culture into these locations, places and regions have affected Asian countries.
The answer is actually pretty simple
Answer= 7.35 cm
Answer: We study other star systems in spaceships and big, professional telescopes
Answer:
correct option is B Schenck v. United States
Explanation:
we know that on on March 3, 1919 Schenck v. United States
Supreme Court of U.S. rule that freedom of speech is protection afford in United State Constitution 1st Amendment prospective restrict if words are spoken and printed represent to society a clear and present danger
it was decided by White Court at District Court for the Eastern District of Pennsylvania
so here correct option is B Schenck v. United States
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.
