It is true that the density of extrasolar planets can be determined. This involves calculating their mass and volume, which can be achieved through methods like transit and radial velocity. Once both mass and volume are known, density can be easily calculated and helps us categorize these planets. ;
It is true that the density of extrasolar planets can be determined through measurements of their mass and volume. This is typically done using transit and radial velocity methods, allowing for classification of planets. The formula for density, mass divided by volume, facilitates this process.
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