Prepare for NEET Physics Gravitation (Orbital Velocity) with MCQs & PYQs on NEET.GUIDE. Access free practice, previous year questions, and expert guidance to understand the speed required for stable orbits.
A satellite is in a circular orbit around a planet. If its kinetic energy is doubled, and assuming no external forces act on it, what will happen to its orbital radius?
The orbital radius will be halved.
The orbital radius will be doubled.
The orbital radius will remain unchanged.
The orbital radius will be quadrupled.
Consider a binary star system where two stars of equal mass orbit each other in circular orbits of radius . What is the orbital speed of each star?
v = sqrt(GM/2R)
v = (1/2)sqrt(GM/R)
v = sqrt(2GM/R)
v = (1/2)sqrt(2GM/R)
A planet of mass orbits a star of mass in a slightly elliptical orbit. Which of the following quantities remains constant throughout the planet's orbit?
Speed
Kinetic energy
Potential energy
Angular momentum
A geostationary satellite appears to remain stationary above a particular point on Earth's equator. This is because its:
orbital speed is equal to Earth's rotational speed.
orbital radius is equal to Earth's radius.
orbital period is equal to Earth's rotational period.
orbital plane is perpendicular to Earth's rotational axis.
A satellite is orbiting Earth at a certain height. If its height is doubled, what will happen to its orbital velocity?
It will increase.
It will decrease.
It will remain the same.
It will become zero.
Two satellites, A and B, are orbiting Earth at different heights. Satellite A is at a lower height than satellite B. Which satellite has a higher orbital velocity?
Satellite A
Satellite B
Both have the same orbital velocity.
Cannot be determined without knowing their masses.
The orbital velocity of a satellite close to the Earth's surface is 'v'. What will be its orbital velocity if the radius of the orbit is increased to four times the Earth's radius?
v/4
v/2
2v
4v
Which of the following factors does NOT affect the orbital velocity of a satellite?
Mass of the planet
Radius of the orbit
Mass of the satellite
Gravitational constant