FromHeliumtoHydrogen: TheAnalogousRelation ofLimitstotheTheSun

Limits are one of the topics in calculus

Limitsareusedtodefinecontinuity,integral, anddifferential.Asitisusuallystated,Limits are defined as the value you are approaching as you approach a certain value. Limits may usually be written on paperwithmathequations However,itmay also be related and applied to situations in reallife

Several billion years ago, a star was createdanditcontinuestoprovidelightand heattothesolarsystem Itisthesunthatwe all know of The sun is a massive star located at the center of the solar system It hasexistedevenbefore46billionyearsago

The sun also is responsible for the light we have throughout the solar system However, the sun will eventually reach its end and may not provide us with the light that we need anymore. As the sun continues to age throughout the history of the solar system and universe, it fuses hydrogen in its core whichproducesabyproductofhydrogen..

Throughout the process, it produces heat that rises continuously, and this heat would eventually reaches its highest peak when the sun finally stoppedfusinghydrogen.Thisiswherelimitscome in relation to the sun. The sun’s temperature may becomparableandsimilarwhenitcomestolimits that reach a certain value as you approach a certainvalue.Whenitreachesthecourseofovera billion years, the temperature of its helium core continuously increases, eventually reaching over 100millionKelvin.

Limitssurelydonotonlyplayabigroleinmath especially in calculus, but also in real-life experiences and situations. Limits may even be related and applied outside the planet earth. This brings new knowledge that may even be a foundation of a main idea or point in a future society