A new star

What an exciting topic!

A new star is born when a massive cloud of gas and dust in space collapses under its own gravity, causing the material at the center to heat up until it reaches incredibly high temperatures. This process is called star formation.

Here's a step-by-step guide to how a new star is born:

  1. Gas and dust collapse: A giant molecular cloud, made up of hydrogen, helium, and heavier elements, collapses under its own gravity. This cloud can be triggered by various factors, such as the shockwave from a nearby supernova or the collision of two galaxies.
  2. Core formation: As the cloud collapses, the material at the center begins to spin faster and faster, causing it to flatten into a disk shape. The core of the cloud becomes increasingly dense and hot, eventually reaching temperatures of around 10 million degrees Celsius (18 million degrees Fahrenheit).
  3. Nuclear fusion: At this point, the core is hot enough to ignite nuclear fusion reactions, marking the birth of a new star. Hydrogen atoms fuse together to form helium, releasing vast amounts of energy in the process.
  4. Protostar formation: The newly formed star is now a protostar, surrounded by a disk of gas and dust. The protostar continues to contract and heat up, eventually reaching the surface temperature of around 5,500 degrees Celsius (10,000 degrees Fahrenheit).
  5. Main sequence: Once the protostar has reached the main sequence, it will begin to shine as a main-sequence star, fusing hydrogen into helium in its core. This is the longest stage of a star's life, during which it will remain relatively stable and constant in brightness.

Some interesting facts about new stars:

I hope you found this brief introduction to star formation fascinating!