\(√110\)
\(√140\)
\(√98\)
\(√55\)
\(√70\)
Step 1: Use the property of perpendicular vectors. Since \(\vec{a}\) and \(\vec{b}\) are perpendicular:
\[ \vec{a} \cdot \vec{b} = 0 \]
Step 2: Apply the formula for the magnitude of the difference of vectors:
\[ |\vec{a} - \vec{b}|^2 = |\vec{a}|^2 + |\vec{b}|^2 - 2(\vec{a} \cdot \vec{b}) \]
Given \(|\vec{a}| = \sqrt{104}\) and \(|\vec{b}| = 6\):
\[ |\vec{a} - \vec{b}|^2 = (\sqrt{104})^2 + 6^2 - 2(0) \]
\[ = 104 + 36 = 140 \]
Step 3: Take the square root to find the magnitude:
\[ |\vec{a} - \vec{b}| = \sqrt{140} \]
Conclusion: The value is \(\boxed{B}\) (\(\sqrt{140}\)).
Given
Let \(a\) and \(b\) be perpendicular vectors such that;
\(IaI=√104\) and \(IbI=6\).
We know that ,
\(|a-b|^{2}=|a|^{2}+|b|^{2}-2.|a|.|b|cos90°\)
\(⇒|a-b|^{2}=104+36-0\)
\(⇒|a-b|=√140\)
Let \(a=i+j+2k\) and \(b=i-2j+3k\) be two vectors. Then the unit vector in the direction of \(a-b\) is
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
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