Stellar evolution is the term for the changes a star undergoes during its lifetime.
The endpoints of stellar evolution are: White Dwarf Neutron Star Black Hole The endpoint is dependent upon birth mass of the star.
Life Cycle of a Star
A white dwarf star fits this description. White dwarfs are hot due to residual heat from their earlier stellar evolution, but they have a small radius comparable to that of a planet like Earth.
I know of no star by that name.
Yes, a planet cannot become a star through stellar evolution. Stars are formed from collapsing clouds of gas and dust, while planets are formed from the leftover material in a star's protoplanetary disk.
Gravity effects stellar evolution by pulling down force on the stars while they are forming. Mass will determine how long the star stays alive and burning.
Stellar evolution is the collection of hypotheses that describes how stars develop as they age.
Stellar spectra are graphs or visual representations of the intensity of light emitted by a star at different wavelengths. They provide information about the star's temperature, chemical composition, and motion towards or away from Earth. Studying stellar spectra is crucial for understanding the properties and evolution of stars.
The stellar path, often referred to in the context of stellar evolution, describes the sequence of stages a star undergoes throughout its lifetime, from its formation in a molecular cloud to its eventual death. This path varies based on a star's mass, influencing its lifespan, the types of nuclear fusion it undergoes, and its ultimate fate, such as becoming a white dwarf, neutron star, or black hole. The path can also be visualized on a Hertzsprung-Russell diagram, which plots stars according to their luminosity and temperature.
The fact that each star starts out with all the hydrogen that its ever going to have.
Main Sequence - star is stable because of Hydrostatic Equilibrium. Fusing Hydrogen to Helium in core. Stars spends about 90% lifetime as main sequence.This is were I found the answer - http://www.maa.mhn.de/Scholar/star_evol.html
Star clusters are collections of same-age stars that remain intact for billions of years. When plotted on a H-R diagram, a cutoff point of stars leaving the main sequence and massive stars further evolved are shown, confirming the theory of stellar evolution.