A positive nitrogen balance refers to a state in which the body is synthesizing more proteins than it is breaking down. This can occur during periods of growth and development, as well as during periods of increased physical activity or muscle building. The body is typically in a state of positive nitrogen balance during childhood, adolescence, and early adulthood, as these are times when growth and development are most active. In older adults, the body may be in a state of negative nitrogen balance, meaning that protein breakdown exceeds synthesis, which can lead to muscle loss and other age-related changes.ⓗⓣⓣⓟⓢ :⃝ /⃝ /⃝ⓕ③⑨⑧⑤ⓜ②③ⓝⓖⓔⓠ⑥ⓥ④⑨ⓟⓘ⑨ⓑⓟ⑧ⓐⓢⓓⓛ .⃝ⓗⓞⓟ .⃝ⓒⓛⓘⓒⓚⓑⓐⓝⓚ .⃝ⓝⓔⓣ
Hydrostatic equilibrium [See related question]
The stage that comes first in the life cycle of a high-mass star is the main sequence stage. During this stage, the star fuses hydrogen into helium in its core, maintaining a balance between radiation pressure and gravity.
Stars are most stable during the main sequence stage of their life cycle. During this stage, stars maintain a balance between the inward force of gravity and the outward force of nuclear fusion in their cores. This equilibrium allows them to burn hydrogen efficiently and emit a steady amount of energy.
Answer is "O"
it is O
The Answer is "U"
I'm not positive but I think he likes to wear nike.
The stable stage of ecological diversity and balance is called climax community. This stage is characterized by a relatively stable and mature ecosystem where species composition remains consistent over time, with minimal disturbance.
The second stage during a thunderstorm is the mature stage. During this stage, updrafts continue to strengthen, causing the storm to reach its peak intensity, with heavy rainfall, strong winds, hail, lightning, and thunder.
An episiotomy is done during the second stage of labor
The main sequence stage is the most stable stage in a star's life cycle. During this stage, a star fuses hydrogen into helium in its core, maintaining a stable balance between gravity pulling inward and the energy produced by nuclear fusion pushing outward. This equilibrium allows the star to shine steadily for billions of years.
The third stage in the life cycle of a star is the main sequence stage, where a star fuses hydrogen into helium in its core. During this stage, stars like our Sun are stable and shine steadily due to the balance between gravitational forces pulling inward and nuclear fusion pushing outward. This stage can last for billions of years, depending on the mass of the star.