Galaxies, Redshift and the Expanding Universe · seed 1 · A4, ink-friendly. The answer key prints on its own page for grown-ups.

Measuring an expanding universe

Science · Astronomy & Astrophysics · ages 21-22
Name ______________________   Date ____________
  1. What does redshift measure for a distant galaxy?

    • Its age in years
    • Its speed away from us
    • Its number of stars
  2. How does a standard candle give a distance?

    • By comparing apparent and true brightness
    • By measuring its temperature alone
    • By counting its planets
  3. Dividing distance by speed gives a rough cosmic age near how many billion years?

    Answer: ______________

  4. A galaxy sits ten times farther than its twin. How much dimmer does it look?

    • Ten times dimmer
    • One hundred times dimmer
    • Equally bright
  5. A Cepheid pulses slowly and a second one pulses fast. Which is truly brighter?

    • The fast pulsing one
    • Both are always equal
    • The slowly pulsing one
  6. What does the slope of the Hubble relation give?

    • The present expansion rate
    • The age of the oldest star
    • The mass of the Milky Way
  7. A student dates the universe from one nearby star alone. What is wrong?

    • Stars cannot be dated at all
    • The age needs the expansion ratio of distance to speed
    • Nearby stars are always newborn
  8. Every galaxy survey shows neighbors receding on all sides. What follows?

    • Our galaxy sits at the exact center
    • The surveys must be broken
    • The expansion has no center to point at
LightMySky · lightmysky.comW1-mt_-POhqrng-Q-s1

Answer key

For grown-ups. Fold this page away before handing over the rest.

Measuring an expanding universe W1-mt_-POhqrng-Q-s1

  1. Its speed away from us · Stretched light encodes the recession speed.
  2. By comparing apparent and true brightness · Known wattage plus observed dimness reveals the range.
  3. 14 · The Hubble ratio points to about 14 billion years.
  4. One hundred times dimmer · Light dims with the square of the distance.
  5. The slowly pulsing one · The pulsation period reveals the true luminosity.
  6. The present expansion rate · Speed plotted against distance rises with that slope.
  7. The age needs the expansion ratio of distance to speed · One star gives no expansion ratio to divide.
  8. The expansion has no center to point at · Like raisins in dough, each spot sees the same pattern.
Worksheet · LightMySky