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9th grade Kepler's three laws of planetary motion worksheet

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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.

    • Both are about 3.54, so the law holds
    • It works for Earth alone
    • 3.54 and 1.88 differ, so it fails
    • 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?

    • 64 years
    • 2 years
    • 4 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?

    • 27 AU
    • 9 AU
    • 3 AU
    • 140 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.

    • Mars is faster at aphelion
    • Speed × distance doubles from one point to the other
    • The speed is the same at both points
    • Both are about 5,476: faster goes with closer
  7. Earth (NASA)

    PointSpeed (km/s)Distance (million km)
    perihelion30.29147.1
    aphelion?152.1
  8. Earth moves at 30.29 km/s at perihelion (147.1 million km). With speed × distance staying the same, how fast is it at aphelion (152.1 million km), by Luz's math?

    • About 4,455 km/s
    • About 30.29 km/s, unchanged
    • About 29.3 km/s
    • About 31.3 km/s
  9. Mars (NASA)

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

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

    PointDistance (million km)
    perihelion147.1
    aphelion152.1
    average149.6
  12. 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 0%, since the orbit is a circle
    • About 30%, enough to cause the seasons
    • About 300%
    • About 3% of the average distance
  13. Mercury's orbital speed (NASA)

    SpeedValue
    maximum58.97 km/s
    minimum38.86 km/s
  14. NASA gives Mercury's fastest speed as 58.97 km/s and its slowest as 38.86 km/s. How many times faster is it at perihelion, by Tala's math?

    • About 20 times
    • About 1.5 times
    • About 0.66 times
    • Exactly 1 time
  15. 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
  16. 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
    • Neither changes, since orbits are circles
    • Both keep a constant speed
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9th grade Kepler's three laws of planetary motion worksheet – printable
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About this worksheet

Kepler's three laws of planetary motion. Every version has 10 questions, and the answer key prints on the second page.

What your child will learn

  • I can describe orbits as ellipses with the Sun at a focus and compute eccentricity from perihelion and aphelion.
  • I can use equal areas in equal times: planets are fastest at perihelion, with speed × distance the same at both ends.
  • I can use T² = a³ (years, AU) both ways and check it against NASA data.

Standard: HS-ESS1-4

Words to know

ellipse: A stretched circle with two foci

focus: One of two fixed points inside an ellipse; the Sun sits at one

eccentricity: How stretched an orbit is: 0 is a circle

perihelion: The point of an orbit closest to the Sun

aphelion: The point of an orbit farthest from the Sun

Common mistakes

Your child pictured orbits as perfect circles. Kepler's first law: orbits are ellipses; Earth's is nearly circular (e = 0.017), Mercury's clearly stretched (e = 0.206).

Your child put the Sun at the center of the ellipse. The Sun sits at one focus, off-center.

Your child misread eccentricity. e = (aphelion − perihelion) ÷ (aphelion + perihelion); 0 is a circle, and closer to 1 is more stretched.

Questions parents ask

What is the most common mistake with kepler's three laws of planetary motion?

Your child pictured orbits as perfect circles. Kepler's first law: orbits are ellipses; Earth's is nearly circular (e = 0.017), Mercury's clearly stretched (e = 0.206).

Are these 9th grade science worksheets free to print?

Yes. All 6 printable versions at each level are free to print, with the answer key, and no account is needed.

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