The core of a star is the point where hydrogen fusion begins. This is what causes the pressure and heat to increase, which in turn leads to nuclear reactions that can be seen from Earth as “starlight.” However, it’s not very easy for the average person to figure out how hot a star has to be before fusion can begin.
In this post we will explore what you need to know about stars, their cores, and how they form!
Core temperature
Core temperature: approximately 150 million degrees Celsius (300 million degrees Fahrenheit) The core of a star is the point where hydrogen fusion begins. This is what causes the pressure and heat to increase, which in turn leads to nuclear reactions that can be seen from Earth as “starlight.
” However, it’s not very easy for the average person to figure out how hot a star has to be before fusion can begin. In this post we will explore our understanding of stars, their cores, and how they form! Core temperature: approximately 150 million degrees Celsius (300 million degrees Fahrenheit) __ __.
.continued writing next sentences of long-form content here.. Post summary: The post explores what you need know about stars and their cores or nuclear reactions that occur when hydrogen starts forming
