Library · Experiment
Weigh Jupiter
Track Jupiter's moons through binoculars over a few weeks, then use Kepler's third law to work out the mass of the largest planet.
- When
- Mid Dec – Jan · Into space
- Time
- Several clear nights over 2–4 weeks
- Cost
- £0 with binoculars you own
- Difficulty
- 3 of 3
Part of The Road Map (Into space) · Measuring the Solar System (Weigh a planet)
The question
Can I work out how heavy Jupiter is, using nothing but binoculars, a notebook and Kepler's laws?
Learn just enough first
- Read about Kepler's third law: how a moon's orbit size and period depend on the planet's mass
- Use Stellarium to find Jupiter and learn which moon is which
Kit
- Binoculars (10x50 is ideal), steadied on a tripod, fence post or car roof
- A notebook with a pre-drawn line for each night
- Stellarium, to check identifications on the same night
My prediction
The accepted mass is about \(1.9 \times 10^{27}\) kg — over 300 Earths. How close will a hobbyist get?
Method
- On each clear night, sketch Jupiter as a dot and mark each moon's position. Estimate distances in Jupiter-widths.
- Note the date and time every time. Aim for as many nights as possible over 2–4 weeks — weekend nights are fine.
- Concentrate on Ganymede (orbits in about 7 days) or Callisto (about 17 days).
- Plot each moon's distance from Jupiter against time. It traces out a wave: the peak is the orbit radius \(a\), and the time for one full wave is the period \(T\).
- Convert Jupiter-widths to metres using Jupiter's diameter, about 143,000 km.
Tip: UK winters are cloudy. If gaps appear, use Stellarium to fill missing nights — note in the data which points are observed and which are simulated.
Data
| Date | Time | Moon | Side (E/W) | Distance (Jupiter-widths) |
|---|---|---|---|---|
Result
Kepler's third law, rearranged for the planet's mass:
with \(G = 6.674 \times 10^{-11}\) (SI units), \(a\) in metres and \(T\) in seconds. As a check, Ganymede's real orbit (\(a \approx 1.07 \times 10^{9}\) m, \(T \approx 7.15\) days) gives about \(1.9 \times 10^{27}\) kg.
Explain it to a friend
A heavier planet pulls its moons round faster. Measure how far out a moon orbits and how long it takes, and gravity tells you the planet's mass. It's the same method used to weigh the Sun, black holes and whole galaxies.
New questions
- Do two different moons give the same mass?
- How does an error in the orbit size affect the answer? (Hint: it's cubed.)