Gravity is the centripetal force
Every orbiting body is in free-fall towards the body it orbits. Gravity provides the centripetal force that keeps it on its curved path: . The four spec cases (8.4): moons round planets, planets round the Sun, satellites round Earth, comets round the Sun. Consequence: a lower orbit (smaller ) has stronger gravity, so a higher speed and shorter period ().
Orbital speed: v = 2πr/T
In one orbit the body travels the circumference in time , so ( in m/s, in m, in s). Rearrange: , . A higher orbit (larger ) → slower speed, longer period; a lower orbit → faster, shorter period. Geostationary: m, h, m/s. Low Earth orbit: – m, min, –8000 m/s.
Geostationary vs polar orbits
Geostationary: h, in the equatorial plane, same direction as Earth's spin, so it stays above one fixed point (altitude ≈ 35 786 km). Used for TV, weather and telecoms; a dish can be fixed (no tracking). Polar (low Earth) orbit: low altitude, passes near both poles, –120 min; as Earth turns beneath, successive orbits cover the WHOLE surface. Used for Earth observation, mapping and GPS; needs tracking.
Drawn from real examiner reports.
"No gravity in space" is wrong
Satellites are not weightless because "gravity is zero in space". Gravity weakens with distance but is never zero (at the ISS, N/kg) and IS the centripetal force holding the orbit. Astronauts feel weightless only because they and the craft free-fall together, so there is no contact force — the apparent weight, not gravity, is zero.
June 2023 Paper 2P — on astrophysics explanations candidates repeated the question without processing it; vague "no gravity in space" answers with no mechanism scored zero.
Geostationary ≠ geosynchronous
A geosynchronous orbit has a 24 h period but any inclination (it traces a figure-8, not fixed). A geostationary orbit is the special equatorial case that stays above one point. The period is exactly 24 h — not "same as the Moon" (27.3 days) or "1 year". A full definition needs three elements: 24 h period, equatorial plane, same direction as Earth's spin.
June 2024 Paper 2P — longer astrophysics answers repeated the question without creditworthy physics; a geostationary definition needs all three elements (24 h, equatorial, same direction).
Convert to SI units first (m, s)
In , convert before substituting: radius in metres (not km), period in seconds (not hours or minutes). A period left in hours is out by 3600; a radius in km by 1000. These slips lose the final answer mark even when the method is right — and the answer should be in m/s.
June 2024 Paper 2P Q2(c)(i) — a sizeable minority forgot to convert the distance into metres before completing the calculation.
Lower orbit is faster, not slower
Intuition says "lower = slower", but orbits are the opposite. : a smaller gives a larger and a shorter period. The ISS (low) orbits in ~90 min; the Moon (far) takes 27.3 days. So a satellite moved to a lower orbit speeds up, it does not slow down.
Use orbital radius, not altitude
Orbital radius is measured from the centre of the Earth, so with m. Substituting the altitude (measured from the surface) makes about 6400 km too small. Always convert altitude to orbital radius before using .
Velocity is tangential, force is inward
On an orbit diagram the velocity arrow is tangential (along the orbit) and the gravitational/centripetal force arrow points inward to the centre. Drawing the velocity towards Earth, or the force along the direction of motion, is penalised. Label the inward force as gravity acting as the centripetal force.
Explain-orbit: three-step chain
For "why does a satellite stay in orbit?", chain three steps: (1) gravity provides the centripetal force towards Earth's centre; (2) it continuously changes the direction of the velocity (curved path); (3) without it the satellite would go straight on (Newton 1) and fly off.
Orbital speed: convert, sub, unit
Method for : convert to metres and to seconds, keep the , substitute, evaluate, and quote m/s. To find or , rearrange first (, ).
Geostationary needs three elements
For a geostationary definition give all three mark-scheme elements: a 24-hour period, an orbit in the equatorial plane, and motion in the same direction as Earth's rotation. Together these make the satellite appear fixed above one point.
Avoid the zero-mark phrases
Never write "gravity disappears", "it floats because there is no force", "it is too far for gravity", or "weightless means no gravity". Name the mechanism instead: gravity acts as the centripetal force, and free-fall causes the apparent weightlessness.
Orbital speed, radius and time period (Edexcel spec 8.6):
where = orbital speed (m/s), = orbital radius (m, measured from the centre of the orbited body), = orbital period (s).
Rearrangements:
Centripetal force = gravitational force (for circular orbits):
This is the force provided by gravity. It always points towards the centre of the orbit.
What force provides the centripetal force that keeps a satellite in orbit around Earth?
A weather satellite orbits Earth in a circular orbit of radius m. The orbital period of the satellite is 5580 s.
Calculate the orbital speed of the satellite.
Give your answer to 3 significant figures.