Redshift and the expanding universe
Grade 9 Science Worksheet

Circle the best answer.
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 1,980,000 km/s
- About 6.6 km/s
- About 3,000 km/s toward us
- About 3,000 km/s
A galaxy has z = 0.02. Where should its hydrogen line (656.3 nm in the lab) appear, by Jun's math?
Spectrum strip: lab line 656.3 nm; z = 0.02. Spectrum strip: lab line 656.3 nm; z = 0.02. lab line 656.3 nm z = 0.02 - About 669.4 nm
- About 643.2 nm
- About 656.3 nm, unchanged
- About 13.1 nm
Read this first
Galaxies (model data)
Galaxy Distance (Mpc) Speed away (km/s) P 20 1,400 Q 50 3,500 R 100 7,000 S 200 14,000 Using the table, about how fast is galaxy S (200 Mpc) moving compared with galaxy R (100 Mpc), by Kira's reading?
- About twice as fast
- About 100 times as fast
- The same speed, since everything stretches equally
- About half as fast
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 6,700 to 7,300 km/s
- About 67,000 to 73,000 km/s
- About 0.67 to 0.73 km/s
- About 67 to 73 km/s
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 100 Mpc (96 to 104 across the range)
- About 490,000 Mpc
- About 10 Mpc
- About 1,000 Mpc
Why do distant galaxies all appear to rush away from us, by Noah's reading?
Dots on a stretching rubber sheet. Dots on a stretching rubber sheet. - Their light is turning red as they age
- They were thrown out from our galaxy
- They are falling toward a central point
- Space itself is stretching between the galaxies
Stretching sheet model
Pair Before (cm) After (cm) near pair 1 2 far pair 3 6 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?
- Nearer dots separate faster
- Farther dots separate faster, as in Hubble's law
- Each pair separates equally
- The dots move from one central dot
Galaxies in a nearby cluster stay together while distant clusters move apart. Why, by Ren's reading?
Diagram: a cluster of galaxies held together, with distant clusters spreading apart. Diagram: a cluster of galaxies held together, with distant clusters spreading apart. cluster of galaxies distant clusters distant clusters - Everything expands, but too slowly to see
- The cluster is moving toward us
- Gravity holds the cluster together
- The cluster is at the center of the universe
Galaxies (model data)
Galaxy Distance (Mpc) Speed away (km/s) P 20 1,400 Q 50 3,500 R 100 7,000 S 200 14,000 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 redshifts
- Nearer galaxies showed larger redshifts
- Farther galaxies showed larger blueshifts
What is the slope of the table's speed-against-distance line, by Ari's math?
- −70 km/s/Mpc
- 7,000 km/s
- 70 km/s/Mpc
- 0.014 Mpc per km/s