Redshift and the expanding universe

Grade 9 Science Worksheet

NameDate

Circle the best answer.

  1. A galaxy's hydrogen line (656.3 nm in the lab) is seen at 662.9 nm. Using speed ≈ z × 300,000 km/s, about how fast is it receding, by Bo's math?

    • About 6.6 km/s
    • About 1,980,000 km/s
    • About 3,000 km/s
    • About 3,000 km/s toward us
  2. A galaxy's hydrogen line at 486.1 nm in the lab is seen at 491.0 nm. About what is z, by Esme's math?

    • About 4.9
    • About 0.010
    • About −0.010, a blueshift
    • About 0.10
  3. A galaxy has z = 0.02. Where should its hydrogen line (656.3 nm in the lab) appear, by Jun's math?

    • About 656.3 nm, unchanged
    • About 13.1 nm
    • About 643.2 nm
    • About 669.4 nm
  4. Speed = H0 × distance; H0 about 67 to 73 km/s/Mpc; distance 100 Mpc. Sources put H0 at about 67 to 73 km/s/Mpc. A galaxy is 100 Mpc away. In what range is its speed, by Luz's math?

    • About 0.67 to 0.73 km/s
    • About 67 to 73 km/s
    • About 6,700 to 7,300 km/s
    • About 67,000 to 73,000 km/s
  5. Distance = speed ÷ H0; speed 7,000 km/s; H0 about 67 to 73 km/s/Mpc. A galaxy recedes at 7,000 km/s. With H0 about 67 to 73 km/s/Mpc, about how far away is it, by Milo's math?

    • About 490,000 Mpc
    • About 1,000 Mpc
    • About 10 Mpc
    • About 100 Mpc (96 to 104 across the range)
  6. Read this first

    Stretching sheet model

    PairBefore (cm)After (cm)
    near pair12
    far pair36
  7. On a stretching sheet, dots 1 cm apart become 2 cm apart, and dots 3 cm apart become 6 cm apart, in the same time. What does this model show, by Pia's reading?

    • Farther dots separate faster, as in Hubble's law
    • Nearer dots separate faster
    • Each pair separates equally
    • The dots move from one central dot
  8. Galaxies in a nearby cluster stay together while distant clusters move apart. Why, by Ren's reading?

    • Everything expands, but too slowly to see
    • Gravity holds the cluster together
    • The cluster is at the center of the universe
    • The cluster is moving toward us
  9. Galaxies (model data)

    GalaxyDistance (Mpc)Speed away (km/s)
    P201,400
    Q503,500
    R1007,000
    S20014,000
  10. Hubble published the link between galaxy distance and speed in 1929. Which observation supported it, by Tala's reading?

    • Farther galaxies looked redder in color
    • Farther galaxies showed larger blueshifts
    • Nearer galaxies showed larger redshifts
    • Farther galaxies showed larger redshifts
  11. Galaxy Q (50 Mpc) and galaxy P (20 Mpc): how many times faster does Q recede, by Zee's math?

    • 70 times
    • 0.4 times
    • 2.5 times
    • 30 times
  12. What is the slope of the table's speed-against-distance line, by Ari's math?

    • 7,000 km/s
    • 0.014 Mpc per km/s
    • −70 km/s/Mpc
    • 70 km/s/Mpc
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Redshift and the expanding universe

Answer Key - Grade 9 Science Worksheet

Circle the best answer.

  1. A galaxy's hydrogen line (656.3 nm in the lab) is seen at 662.9 nm. Using speed ≈ z × 300,000 km/s, about how fast is it receding, by Bo's math?

    • About 6.6 km/s
    • About 1,980,000 km/s
    • About 3,000 km/s
    • About 3,000 km/s toward us
  2. A galaxy's hydrogen line at 486.1 nm in the lab is seen at 491.0 nm. About what is z, by Esme's math?

    • About 4.9
    • About 0.010
    • About −0.010, a blueshift
    • About 0.10
  3. A galaxy has z = 0.02. Where should its hydrogen line (656.3 nm in the lab) appear, by Jun's math?

    • About 656.3 nm, unchanged
    • About 13.1 nm
    • About 643.2 nm
    • About 669.4 nm
  4. Speed = H0 × distance; H0 about 67 to 73 km/s/Mpc; distance 100 Mpc. Sources put H0 at about 67 to 73 km/s/Mpc. A galaxy is 100 Mpc away. In what range is its speed, by Luz's math?

    • About 0.67 to 0.73 km/s
    • About 67 to 73 km/s
    • About 6,700 to 7,300 km/s
    • About 67,000 to 73,000 km/s
  5. Distance = speed ÷ H0; speed 7,000 km/s; H0 about 67 to 73 km/s/Mpc. A galaxy recedes at 7,000 km/s. With H0 about 67 to 73 km/s/Mpc, about how far away is it, by Milo's math?

    • About 490,000 Mpc
    • About 1,000 Mpc
    • About 10 Mpc
    • About 100 Mpc (96 to 104 across the range)
  6. Read this first

    Stretching sheet model

    PairBefore (cm)After (cm)
    near pair12
    far pair36
  7. On a stretching sheet, dots 1 cm apart become 2 cm apart, and dots 3 cm apart become 6 cm apart, in the same time. What does this model show, by Pia's reading?

    • Farther dots separate faster, as in Hubble's law
    • Nearer dots separate faster
    • Each pair separates equally
    • The dots move from one central dot
  8. Galaxies in a nearby cluster stay together while distant clusters move apart. Why, by Ren's reading?

    • Everything expands, but too slowly to see
    • Gravity holds the cluster together
    • The cluster is at the center of the universe
    • The cluster is moving toward us
  9. Galaxies (model data)

    GalaxyDistance (Mpc)Speed away (km/s)
    P201,400
    Q503,500
    R1007,000
    S20014,000
  10. Hubble published the link between galaxy distance and speed in 1929. Which observation supported it, by Tala's reading?

    • Farther galaxies looked redder in color
    • Farther galaxies showed larger blueshifts
    • Nearer galaxies showed larger redshifts
    • Farther galaxies showed larger redshifts
  11. Galaxy Q (50 Mpc) and galaxy P (20 Mpc): how many times faster does Q recede, by Zee's math?

    • 70 times
    • 0.4 times
    • 2.5 times
    • 30 times
  12. What is the slope of the table's speed-against-distance line, by Ari's math?

    • 7,000 km/s
    • 0.014 Mpc per km/s
    • −70 km/s/Mpc
    • 70 km/s/Mpc