Kepler's three laws of planetary motion
Grade 9 Science Worksheet - Building Confidence

Circle the best answer.
Read this first
Orbits (NASA Planetary Fact Sheet)
Planet a (AU) T (years) e Mercury 0.387 0.241 0.206 Earth 1.000 1.000 0.017 Mars 1.524 1.881 0.094 Jupiter 5.20 11.86 0.049 Which planet in the table has the most stretched orbit, by Kira's reading?
- Mercury, e = 0.206
- Mars, e = 0.094
- Earth, e = 0.017
- Jupiter, e = 0.049
two shaded slices of equal area. What does Kepler's second law say a line from the Sun to a planet does, by Jun's reading (NASA)?
- Sweeps equal areas in equal times
- Sweeps equal distances in equal times
- Sweeps larger areas when far away
- Sweeps equal angles in equal times
Orbit diagram with perihelion and aphelion marked. Where in its orbit does a planet move fastest, by Luz's reading?
- Closest to the Sun, at perihelion
- Halfway between the two
- Farthest from the Sun, at aphelion
- At the same speed everywhere
Earth's orbital speed (NASA)
Speed Value maximum 30.29 km/s minimum 29.29 km/s NASA gives Earth's orbital speed as 30.29 km/s at most and 29.29 km/s at least. Where is Earth when it moves at 30.29 km/s, by Milo's reading?
- At both points equally
- At aphelion, farthest from the Sun
- At perihelion, closest to the Sun
- In early July, its farthest point
Orbits (NASA Planetary Fact Sheet)
Planet a (AU) T (years) e Mercury 0.387 0.241 0.206 Earth 1.000 1.000 0.017 Mars 1.524 1.881 0.094 Jupiter 5.20 11.86 0.049 Which planet in the table takes longest to orbit the Sun, by Noah's reading?
- Mercury, the closest
- Jupiter, the farthest out
- They each take one year
- Mercury, since it moves fastest
Mars orbits at 1.524 AU. What is its orbital period in the table, by Pia's reading?
- 1.524 years, the same as its distance
- 0.53 years, shorter than Earth's
- 3.54 years, its distance cubed
- 1.881 years
Four equation cards, labeled A to D. Which equation is Kepler's third law, with T in years and a in AU, by Ren's reading?
- T³ = a²
- T × a = 1
- T² = a³
- T = a
Mercury (NASA)
Point Distance (million km) perihelion 46.0 aphelion 69.8 NASA lists Mercury's perihelion as 46.0 and its aphelion as 69.8 million km. By how much does its distance from the Sun change, by Tala's math?
- 0 km, since its orbit is a circle
- 23.8 million km
- 115.8 million km
- 57.9 million km
Earth (NASA)
Point Distance (million km) perihelion 147.1 aphelion 152.1 Earth is closest to the Sun in early January (NOAA). Why is January not summer in the Northern Hemisphere, by Zee's reading?
- Earth's orbit is a perfect circle
- Seasons come from Earth's tilt, not its distance
- The 5 million km change sets the seasons
- January is summer everywhere on Earth
Earth's orbital eccentricity is 0.017 (NASA). What does that tell Esme about the shape of the orbit?
Ellipses drawn with e = 0, 0.017 and 0.6. Ellipses drawn with e = 0, 0.017 and 0.6. e = 0 e = 0.017 e = 0.6 - It is a perfect circle
- It is stretched enough to cause the seasons
- It is very stretched, like a comet's
- It is very nearly a circle