4. Main Sequence
The main sequence phase is the stage in development where the core temperature reaches the point for the fusion to commence. In this process, the protons of hydrogen are converted into atoms of helium. This reaction is exothermic; it gives off more heat than it requires and so the core of a main-sequence star releases a tremendous amount of energy
18
214 reads
CURATED FROM
IDEAS CURATED BY
This Idea helps to know how a star evolves and through what process it goes to become a star like "The sun" and ultimately end up to star remnants.
“
Similar ideas to 4. Main Sequence
Structure
The composition of jupiter is similar to that of the Sun - mostly hydrogen and helium. Deep in the atmosphere, pressure and temperature increase, compressing the hydrogen gas into a liquid.
This gives Jupiter the largest ocean in the solar system—an ocean made of hydrogen instead of water....
Read & Learn
20x Faster
without
deepstash
with
deepstash
with
deepstash
Personalized microlearning
—
100+ Learning Journeys
—
Access to 200,000+ ideas
—
Access to the mobile app
—
Unlimited idea saving
—
—
Unlimited history
—
—
Unlimited listening to ideas
—
—
Downloading & offline access
—
—
Supercharge your mind with one idea per day
Enter your email and spend 1 minute every day to learn something new.
I agree to receive email updates