Journey of Stars

Life Cycle of Stars

• Brown dwarfs fail nuclear fusion process if they do not accumulate enough gas due to gravitational pressure, causing them to cool and have a mass of 12-18 Jupiter masses.
• T-Tauri stars are newly born stars under 10 million years old and have just exited the protostar phase to enter the main sequence.
• Main sequence stars spend the majority of their lifetime burning fuel through nuclear fusion, with red dwarf stars living hundreds of billions to possibly one trillion years, and the most giant stars maintaining this stage for 10 million years.
• Stars exit the main sequence to become giants, swelling and eventually leaving behind a white dwarf after creating a planetary nebula.
• White dwarfs are the dead cores of non-giant stars that will shine dimly and continue to cool until they become black dwarfs.
• Giant stars have a mass of 8 or more solar masses and may only live from 10 to 100 million years, while supergiants form heavier elements and eventually create a supernova, leading to the creation of a neutron star or a black hole.
• Neutron stars are incredibly dense star remnants that do not undergo nuclear fusion and have different characteristics depending on their age since the supernova.
• Black holes are created when matter is compressed into a single, one-dimensional point in space, where all matter that enters gets ripped apart and compressed.
• Stars are primarily made of hydrogen gas and begin to produce other elements heavier than helium when they enter their giant phase.

Explore the fascinating life cycle of stars in this quiz. From the birth of T-Tauri stars to the formation of neutron stars and black holes, learn about the stages and characteristics of different types of stars, their lifespans, and the processes that lead to the creation of celestial phenomena.