Gravitation: Real-World Scenarios (4)

easy 2 min read

Question

ISRO’s Chandrayaan-3 orbited the Moon at an altitude of about 100100 km in a circular orbit. Calculate the orbital speed of the spacecraft. (Take Moon’s mass M=7.35×1022M = 7.35 \times 10^{22} kg, Moon’s radius R=1.74×106R = 1.74 \times 10^6 m, G=6.67×1011G = 6.67 \times 10^{-11} N·m²/kg².) This is a NEET 2023 pattern problem rephrased with real ISRO context.

Solution — Step by Step

The orbital radius rr is measured from the centre of the Moon, not from the surface.

r=R+h=1.74×106+0.1×106=1.84×106 mr = R + h = 1.74 \times 10^6 + 0.1 \times 10^6 = 1.84 \times 10^6 \text{ m}

For a circular orbit, gravitational force provides the centripetal force:

GMmr2=mv2r    v=GMr\frac{GMm}{r^2} = \frac{mv^2}{r} \implies v = \sqrt{\frac{GM}{r}}

v=6.67×1011×7.35×10221.84×106v = \sqrt{\frac{6.67 \times 10^{-11} \times 7.35 \times 10^{22}}{1.84 \times 10^6}}

v=4.9×10121.84×106=2.66×1061631 m/sv = \sqrt{\frac{4.9 \times 10^{12}}{1.84 \times 10^6}} = \sqrt{2.66 \times 10^6} \approx 1631 \text{ m/s}

v1.63 km/sv \approx 1.63 \text{ km/s}

Final answer: Orbital speed 1.63\approx 1.63 km/s.

Why This Works

A circular orbit is a balance: gravity pulls the satellite toward the Moon, and the satellite’s tangential motion keeps it from falling in. At the right speed, these match exactly, and the spacecraft traces a circle.

Notice the orbital speed depends only on the central body’s mass and the orbital radius — not on the spacecraft’s mass. Chandrayaan-3 and a 1-tonne dummy at the same altitude would orbit at the same speed.

Alternative Method

Use gmoong_{\text{moon}} at altitude. The acceleration due to gravity at radius rr is g(r)=GM/r2g(r) = GM/r^2. For circular orbit, v=g(r)rv = \sqrt{g(r) \cdot r}. Compute g(r)1.45g(r) \approx 1.45 m/s², so v=1.45×1.84×1061631v = \sqrt{1.45 \times 1.84 \times 10^6} \approx 1631 m/s. Same answer.

A frequent NEET mistake: using r=hr = h (just the altitude) instead of r=R+hr = R + h (centre-to-satellite distance). The orbital formula is centred on the planet’s centre, not its surface.

For Earth satellites, remember vorbit7.9v_{\text{orbit}} \approx 7.9 km/s near the surface. Anything close to that number on a numerical answer is a sanity check. For the Moon, scale by Mmoon/Mearth×Rearth/Rmoon\sqrt{M_{\text{moon}}/M_{\text{earth}}} \times \sqrt{R_{\text{earth}}/R_{\text{moon}}} — comes out to roughly 1/5th, matching our 1.63 km/s.

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