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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. Coloring the Universe
  5. Teacher Guide - Coloring the Universe
  6. Where This Fits in Your Teaching

Coloring the Universe

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Investigation total duration
2 hours

Teacher Guide - Coloring the Universe

  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

  • electromagnetic spectrum, properties of light and color

  • the technology of telescopes, filters, cameras and digital images

  • creating color astronomical images / image processing

  • multiwavelength astronomy

  • STEAM projects: a blend of science and art


Suggested investigations which could come before this one:

In Exploring the Observable Universe, students use the redshift and position of galaxies to explore how the large scale structure of the Universe has changed over time.

In Expanding Universe, students use galaxy redshifts and the Hubble-LeMaitre Law as a way to investigate the expansion and acceleration of the Universe.

In "A Window to the Stars", students use H-R Diagrams to explore properties of stars, such as color, temperature, brightness, lifespan and mass.

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