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The U.S. National Science Foundation (NSF) and the U.S. Department of Energy (DOE) Office of Science will support Rubin Observatory in its operations phase to carry out the Legacy Survey of Space and Time. They will also provide support for scientific research with the data. During operations, NSF funding is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF, and DOE funding is managed by SLAC National Accelerator Laboratory (SLAC), under contract by DOE. Rubin Observatory is operated by NSF NOIRLab and SLAC.

NSF is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.

The DOE Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time.

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  1. Education
  2. Educators
  3. Investigations
  4. Exploding Stars
  5. Teacher Guide - Exploding Stars
  6. Where This Fits in Your Teaching

Exploding Stars

Start Investigation
Investigation total duration
2 hours

Teacher Guide - Exploding Stars

  1. Introduction
  2. Where This Fits in Your Teaching
  3. Next Generation Science Standards
  4. Background and Notes
  5. Student Ideas and Questions
  6. Diversity, Equity and Inclusion

Where This Fits in Your Teaching

  • cosmological redshift
  • Hubble's law
  • Doppler shift
  • distance ladder
  • standard candles
  • stellar evolution
  • variable stars
  • apparent and absolute magnitude
  • cosmology
  • expansion of the Universe

Suggested investigation which could come before this one:

  • In Stellar Safari students use color-magnitude diagrams to explore the properties of different types of stars and their evolutionary sequence.

Suggested investigations which could come after this one:

  • In Expanding Universe students use Type Ia supernovae to measure the distance to galaxies, and redshift data to measure galaxy velocities. Students verify that the Universe is expanding and that the rate of this expansion has changed over time.
  • In Exploring the Observable Universe students use photometric redshift data to evaluate the scale and structure of the observable Universe, and see how the large scale structure of the Universe has changed over time.
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