1.

During a total solar eclipse the moon almost entirely covers the sphere of the sun. Write the relation between the distances and sizes of the sun and moon.

Answer»

Solution :Consider the diagram given below
`D_(me)` = Distance of moon from EARTH Dge
= `D_(se)` istance of sun from earth
Let angle made by sun and moon is , we can write
`theta=(A_(s))/(D_(SC)^(2))=(A_(m))/(D_(me)^(2))`

Here `A_(s)`= AREA of sun
`A_(m)`= Area of the moon
`theta=(pi R_(s)^(2))/(D_(se)^(2))=(piR_(m)^(2))/(D_(me)^(2))`
`:.((R_(S))/(D_(se)))^(2)=((R_(m))/(D_(me)))^(2)`
`:.(R_(s))/(R_(m))=(D_(se))/(D_(me))`
`:. (R_(s))/(R_(m))=(D_(se))/(D_(me))`
(Here, RADIUS of sun and moon represents their sizes respectively)


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