Kepler's three laws of planetary motion

Grade 9 Science Worksheet

NameDate

Circle the best answer.

  1. Read this first

    Orbits (NASA Planetary Fact Sheet)

    Planeta (AU)T (years)e
    Mercury0.3870.2410.206
    Earth1.0001.0000.017
    Mars1.5241.8810.094
    Jupiter5.2011.860.049
  2. Check Kepler's third law for Mars: compare 1.524³ with 1.881², by Bo's math.

    • 3.54 and 1.88 differ, so it fails
    • It works for Earth alone
    • Both are about 3.54, so the law holds
    • 1.524 and 1.881 differ, so it fails
  3. T² = a³ (T in years, a in AU); a = 4. A dwarf planet orbits the Sun at a = 4 AU. What is its period, by Esme's math?

    • 4 years
    • 2 years
    • 64 years
    • 8 years
  4. T² = a³ (T in years, a in AU); T = 27. An asteroid takes 27 years to orbit the Sun. What is its average distance, by Jun's math?

    • 3 AU
    • 140 AU
    • 9 AU
    • 27 AU
  5. Mars (NASA)

    PointSpeed (km/s)Distance (million km)
    perihelion26.50206.65
    aphelion21.97249.26
  6. NASA: Mars moves at 26.50 km/s at perihelion (206.65 million km) and 21.97 km/s at aphelion (249.26 million km). Compare speed × distance at each point, by Kira's math.

    • Both are about 5,476: faster goes with closer
    • The speed is the same at both points
    • Mars is faster at aphelion
    • Speed × distance doubles from one point to the other
  7. In the equal-area drawing, the slice near perihelion is short and wide; the slice near aphelion is long and thin. Each took 30 days. Which arc along the orbit is longer, by Milo's reading?

    • The arc near aphelion
    • The arc near perihelion, so it moved faster there
    • The arcs are equal, since the times are equal
    • Neither; equal times mean equal distances
  8. Mercury (NASA)

    PointDistance (million km)
    perihelion46.0
    aphelion69.8
  9. Mercury's aphelion is 69.8 and perihelion 46.0 million km. Using e = (aphelion − perihelion) ÷ (aphelion + perihelion), what is e, by Noah's math?

    • 0, since it is a circle
    • About 0.21
    • About 0.66
    • About 23.8
  10. Mars (NASA)

    PointDistance (million km)
    perihelion206.7
    aphelion249.3
  11. Mars's aphelion is 249.3 and perihelion 206.7 million km (NASA). What is its eccentricity, by Pia's math?

    • About 0.093
    • About 42.6
    • About 0.83
    • About 1.21
  12. Earth (NASA)

    PointDistance (million km)
    perihelion147.1
    aphelion152.1
    average149.6
  13. Earth's distance ranges from 147.1 to 152.1 million km, averaging 149.6. About what percent of the average is that change, by Ren's math?

    • About 3% of the average distance
    • About 30%, enough to cause the seasons
    • About 300%
    • About 0%, since the orbit is a circle
  14. In which month is Earth moving fastest along its orbit, by Zee's reading?

    • June, in northern summer
    • July, near aphelion
    • Each month at the same speed
    • January, near perihelion
  15. A comet's orbit has e = 0.97; Earth's has e = 0.017. How do their speed changes compare, by Ari's reading?

    • Earth's speed changes more
    • The comet's speed changes far more
    • Both keep a constant speed
    • Neither changes, since orbits are circles
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Kepler's three laws of planetary motion

Answer Key - Grade 9 Science Worksheet

Circle the best answer.

  1. Read this first

    Orbits (NASA Planetary Fact Sheet)

    Planeta (AU)T (years)e
    Mercury0.3870.2410.206
    Earth1.0001.0000.017
    Mars1.5241.8810.094
    Jupiter5.2011.860.049
  2. Check Kepler's third law for Mars: compare 1.524³ with 1.881², by Bo's math.

    • 3.54 and 1.88 differ, so it fails
    • It works for Earth alone
    • Both are about 3.54, so the law holds
    • 1.524 and 1.881 differ, so it fails
  3. T² = a³ (T in years, a in AU); a = 4. A dwarf planet orbits the Sun at a = 4 AU. What is its period, by Esme's math?

    • 4 years
    • 2 years
    • 64 years
    • 8 years
  4. T² = a³ (T in years, a in AU); T = 27. An asteroid takes 27 years to orbit the Sun. What is its average distance, by Jun's math?

    • 3 AU
    • 140 AU
    • 9 AU
    • 27 AU
  5. Mars (NASA)

    PointSpeed (km/s)Distance (million km)
    perihelion26.50206.65
    aphelion21.97249.26
  6. NASA: Mars moves at 26.50 km/s at perihelion (206.65 million km) and 21.97 km/s at aphelion (249.26 million km). Compare speed × distance at each point, by Kira's math.

    • Both are about 5,476: faster goes with closer
    • The speed is the same at both points
    • Mars is faster at aphelion
    • Speed × distance doubles from one point to the other
  7. In the equal-area drawing, the slice near perihelion is short and wide; the slice near aphelion is long and thin. Each took 30 days. Which arc along the orbit is longer, by Milo's reading?

    • The arc near aphelion
    • The arc near perihelion, so it moved faster there
    • The arcs are equal, since the times are equal
    • Neither; equal times mean equal distances
  8. Mercury (NASA)

    PointDistance (million km)
    perihelion46.0
    aphelion69.8
  9. Mercury's aphelion is 69.8 and perihelion 46.0 million km. Using e = (aphelion − perihelion) ÷ (aphelion + perihelion), what is e, by Noah's math?

    • 0, since it is a circle
    • About 0.21
    • About 0.66
    • About 23.8
  10. Mars (NASA)

    PointDistance (million km)
    perihelion206.7
    aphelion249.3
  11. Mars's aphelion is 249.3 and perihelion 206.7 million km (NASA). What is its eccentricity, by Pia's math?

    • About 0.093
    • About 42.6
    • About 0.83
    • About 1.21
  12. Earth (NASA)

    PointDistance (million km)
    perihelion147.1
    aphelion152.1
    average149.6
  13. Earth's distance ranges from 147.1 to 152.1 million km, averaging 149.6. About what percent of the average is that change, by Ren's math?

    • About 3% of the average distance
    • About 30%, enough to cause the seasons
    • About 300%
    • About 0%, since the orbit is a circle
  14. In which month is Earth moving fastest along its orbit, by Zee's reading?

    • June, in northern summer
    • July, near aphelion
    • Each month at the same speed
    • January, near perihelion
  15. A comet's orbit has e = 0.97; Earth's has e = 0.017. How do their speed changes compare, by Ari's reading?

    • Earth's speed changes more
    • The comet's speed changes far more
    • Both keep a constant speed
    • Neither changes, since orbits are circles