Answer:
Joseon
Explanation:
B) White dwarfsC) Galaxies
D) The nebula
Answer:
A) Massive stars
Explanation:
The mass of the star determines how its end will be. The less massive will give rise to nebulas, in whose center a white dwarf will remain, which is a degenerate star that has exhausted all its fuel and is much smaller than its initial volume. And the most massive stars will become stars of neutrons, quarks, or, if they have enough mass, in black holes. For a star to end its days in the form of a neutron star it is necessary that it has a mass of at least 1.44 solar masses. This value is known as the "Chandrasekhar limit", and we owe it to the Indian astrophysicist Subrahmanyan Chandrasekhar, when we talk about neutron star we mean that it can lead to the formation of other objects
For a star to end its days in the form of a star of quarks or a black hole it is necessary that its mass be even greater. This value is set by the "Tolman-Oppenheimer-Volkoff limit", currently established by astrophysicists at approximately 2.17 solar masses. Everything we have seen so far about the life of the stars is very important because it can help us understand the phenomenon that causes the formation of a black hole.
Answer:
faith in the Vedas as sacred texts
Explanation:
The Vedas are the sacred texts of Hinduism.
B. the surface temperature is too low.
C. the surface has too much ice covering it.
D. there is no atmosphere.
Answer: the surface temperature is too high
Explanation:
syncline.
b.
footwall.
c.
epicenter.
d.
focus.
b. glaciers
c. moving water
d. human actions
Answer:
A. wind
Explanation:
it can pic up and move sand all around