A smaller star, like the Sun, will gradually cool down and stop glowing. During these changes, it will go through the planetary nebula phase and white dwarf phase. After many thousands of millions of years, it will stop glowing and become a black dwarf. A massive star experiences a much more energetic and violent end. What determines the route a star takes, it depends on its mass and composition. Stars are form by large clouds of dust and gas from a nebulae. The route the sun takes through its life cycle is characterized by its main sequence.
The purpose of an H-R diagram is to trace the evolutionary stage of a star. The two variables found on the X and Y-axis are the dependent and independent variable.
The four groups that are found on the HR Diagram:
SuperGiants
Giants
Main Sequence (The group our sun belongs in)
White Dwarfs
The relationship between temperature and brightness for the main sequence stars is as the temperature of star's surface increases, so does the brightness. What is unique about the temperature of the X-axis is that the temperature is how the blue represent hot instead of cold.
The temperature and brightness for each of the 4 corners of the diagram is that the top left represent the hottest and brightest on the diagram, the top right represents the coldest yet brightest on the diagram. While the bottom right show the hottest yet dimmest stars, while the bottom left shows the coldest and dimmest stars.
A galaxy is a massive, gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. We classify galaxies by studying its appearance, the arm tightness, and presence of the bars. The three main types of galaxies are Spiral, Elliptical, and Irregular. Spiral is characterized by a flat disk, central bulge, and arms with young stars. Elliptical is a smooth, oval/spherical with mostly old stars and little gas. Irregular lacks a structure, often chaotic, with mixed star ages and active stars.