Orbit details for thousands of satellites: height, period and inclination.
Physics Unit 3 · ACSPH101NSW Physics · PH12-12QCAA Physics · Unit 3VCE Physics · Unit 3
Students will
test Kepler's third law on real satellites, and use it to find the mass of the Earth.
10-minute activity
Use the worksheet's five satellites, from the space station out to geostationary orbit. Plot T2 against r3: is it a straight line through the origin? Use the slope and Newton's law of gravitation to find the Earth's mass.
Low, medium, geostationary and polar orbits, and what each one is used for.
Physics Unit 3 · ACSPH094NSW Physics · PH12-12QCAA Physics · Unit 3VCE Physics · Unit 3
Students will
use Newton's law of universal gravitation to find the height of a geostationary orbit.
10-minute activity
Compare the orbits on the page. A geostationary satellite goes round once every 23 hours 56 minutes, so it stays over one spot. Set gravity equal to the centripetal force and solve for the orbital radius. Check your answer with the worksheet and a real TV satellite.
Where the ISS is right now, and how fast it is going.
Physics Unit 3 · ACSPH101QCAA Physics · Unit 3VCE Physics · Unit 3
Students will
analyse the space station's orbit as uniform circular motion, and check its period against Kepler's third law.
10-minute activity
Read the station's live height and speed. Work out its orbital radius, period and centripetal acceleration. Does the acceleration match g at that height from Newton's law of gravitation? The worksheet sets it out step by step.
Where the tracked junk in orbit is, and how crowded each height has become.
Physics Unit 3 · ACSPH089
Students will
explain how orbital speed makes even small pieces of debris dangerous, and how crowded orbits raise the risk.
10-minute activity
Show the map's busiest heights. Estimate the kinetic energy of a 0.5 g fleck of paint hitting a satellite at 10 km/s, then compare it with a 1 kg mass dropped from 10 m. What can satellite operators do to cut the risk?
The telescopes working in space, from Hubble to JWST, and what each one is for.
NSW Physics · PH12-15
Students will
explain how the light telescopes collect tells us about stars' temperatures and elements, and gives evidence for the big bang.
10-minute activity
Pick a telescope from the list that measures spectra. Each element leaves its own pattern of lines in a star's spectrum. Sketch the hydrogen lines, then shift them towards the red: what does that tell us about a distant galaxy?
These are our suggestions for where each tool fits. Always preview a page before using it with a class: some tools show ads, these school pages do not.
Australian Curriculum codes are content descriptions, for example AC9S7U03. NSW syllabus outcomes are a second tag, for example SC4-OTU-01. Victoria and Western Australia have their own codes: the activities still fit.
Know a better fit for your class, or a topic we have missed? Tell us and we will add it.
Share this page with one link: orbitalradar.com/schools/au/years-11-12
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Orbital Radar. (2026, November 4). Years 11 and 12: Gravity and Orbits. Retrieved November 5, 2026, from https://orbitalradar.com/schools/au/years-11-12
“Years 11 and 12: Gravity and Orbits.” Orbital Radar, 4 Nov. 2026, orbitalradar.com/schools/au/years-11-12. Accessed 5 Nov. 2026.
Orbital Radar (2026) Years 11 and 12: Gravity and Orbits. Available at: https://orbitalradar.com/schools/au/years-11-12 (Accessed: 5 November 2026).
Orbital Radar. “Years 11 and 12: Gravity and Orbits.” Last modified November 4, 2026. https://orbitalradar.com/schools/au/years-11-12.
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author = {{Orbital Radar}},
title = {Years 11 and 12: Gravity and Orbits},
year = {2026},
month = nov,
howpublished = {\url{https://orbitalradar.com/schools/au/years-11-12}},
url = {https://orbitalradar.com/schools/au/years-11-12},
urldate = {2026-11-05},
note = {Accessed 2026-11-05}
}
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AU - Orbital Radar,
TI - Years 11 and 12: Gravity and Orbits
PY - 2026
DA - 2026/11/04
PB - Orbital Radar
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Y2 - 2026/11/05
LA - en-AU
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