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Equation 1 · How We Know What Is Inside a Planet

What does this equation mean?

I∗=CMR2I^{*} = \frac{C}{MR^{2}}

Read the formula alongside the article passage below. Each part has a deeper page with its role in the equation, the supporting passage and nearby citations.

Start withC
Divide byMR^2
This relates toI^*
How to read the two sides of this formula. Follow the article passage for the meaning of each quantity.

This equation states an equality: the expressions on both sides have the same value under the article’s assumptions. Read the equation part by part below; each part has a contextual explanation and a link to its mathematical background.

Read it piece by piece

I∗I^{*}

Symbol I^*

I∗I^* is part of the quantity the equation computes from the expression on the right.

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CC

Symbol C

C occurs above the fraction bar. The numerator is divided by the entire denominator below it.

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MM

Symbol M

M occurs below the fraction bar. The quantity above the bar is divided by this expression; zero is excluded as a denominator.

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R2R^{2}

Symbol R^2

The square of R: multiply R by itself.

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=

=

The expressions on both sides represent the same quantity under the stated assumptions.

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fraction

fraction

Divide the expression above the line by the one below it.

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superscript

superscript

A raised number can be a power. When it is a label or bound, it selects a case or the upper limit of a sum; the formula’s structure distinguishes these uses.

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MR2MR^{2}

Denominator: MR^2

The complete quantity below the fraction bar; it must be nonzero for this division.

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How to interpret it

With a fixed numerator, increasing a nonzero denominator reduces the fraction. Read it with the definitions, units, and assumptions supplied by the article.

What the article says around this equation

The fourth quantity is the one that does real work. The polar moment of inertia, normalised by mass and radius, is I∗=CMR2I^{*} = \frac{C}{MR^{2}}. and it measures how mass is distributed radially rather than how much there is. A uniform sphere has I∗I^{*} = 0.4 . Anything smaller means mass concentrated toward the centre; anything approaching 0.4 means a body that is close to uniform in density, which for a rocky planet means undifferentiated.

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Sources cited in the article section

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