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Solar radii provide a standardized way to compare the sizes of stars relative to the Sun, which has a radius of about 1 solar radius (R☉). White dwarfs typically have radii around 0.01 to 0.02 R☉, indicating they are much smaller than the Sun due to their collapsed nature. In contrast, giants and supergiants can range from about 10 R☉ to over 1,000 R☉, reflecting their vast sizes as they expand and evolve. This system of measurement allows astronomers to categorize and understand the scale of different stellar types within the universe.
The radii of stars generally increase with their mass due to the relationship described by the mass-radius relation in stellar astrophysics. More massive stars possess stronger gravitational forces, which result in higher pressures and temperatures in their cores, leading to larger radii as they expand. However, this relationship is not linear; while main-sequence stars follow a trend where radius increases with mass, giants and supergiants can have much larger radii relative to their mass. Overall, more massive stars tend to be larger, but the exact relationship can vary depending on a star's evolutionary stage.
2 radii = one diameter
There are infinite radii in a sphere.
Radii is a brand of sports footwear.
The plural of radius is radii.
the single form of radii is radius
A hydrogen atom has the smallest radii.
These three radii are of different lengths.
It is radii which is the plural of radius
The covalent radii is for atoms.
The noun radii is already a plural. The singular is radius.