Localize site content

Let's Connect

  • Visit the Rubin Observatory on Facebook
  • Visit the Rubin Observatory on Instagram
  • Visit the Rubin Observatory on LinkedIn
  • Visit the Rubin Observatory on Twitter
  • Visit the Rubin Observatory on YouTube
  • Jobs Board
  • Intranet
  • Visual Identity Guide
  • Image Gallery
  • Privacy Policy

Contact us

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.

Funding agency logos
Homepage
    • About
    • History
    • Who was Vera Rubin?
    • Construction Updates
      • Rubin in Chile
      • Cerro Pachón
      • Observatory Site Selection
      • Organization
      • Leadership
      • Science Collaborations
    • Funding Information
      • Work With Us
      • Jobs Board
    • Explore
      • How Rubin Works
      • Legacy Survey of Space and Time (LSST)
      • Rubin Technology
      • Alert Stream
      • Rubin Numbers
    • Science Goals
    • Rubin Voices
    • Get Involved in Rubin Research
      • Activities, Games, and More
      • Space Surveyors Game
      • Animated Video Series
      • Join Rubin Observatory’s 3200-Megapixel Group Photo!
    • Gallery
      • Main Gallery
    • Slideshows
    • Construction Archive Gallery
    • Media Use Policy
    • News
    • Press Releases
      • Rubin Observatory First Look
      • Rubin First Look Watch Parties
    • Media Resources
    • Press Releases
    • Name Guidelines
    • For Scientists
      • News, events, and deadlines
      • Rubin Science Assemblies
      • Rubin Data Academy
      • Rubin Community Workshop
      • Resources for scientists
      • Rubin Community Forum
      • Early Science Program
      • Workshops and seminars
      • Tutorials
      • LSST Discovery Alliance
      • Code of Conduct
      • Survey, instruments, and telescopes
      • Key numbers
      • The Legacy Survey of Space and Time (LSST)
      • Instruments
      • Telescopes
      • Data products, pipelines, and services
      • Data access and analysis
      • Recent data releases
      • Alerts and brokers
      • Data processing pipelines
      • Future data products
      • Data Policy
      • Simulation software
      • Documentation and publications
      • Technical documentation
      • How to cite Rubin Observatory
      • Publication policies
      • Glossary & Acronyms
      • Science Collaborations
      • Galaxies Science Collaboration
      • Stars, Milky Way, and Local Volume Science Collaboration
      • Solar System Science Collaboration
      • Dark Energy Science Collaboration
      • Active Galactic Nuclei Science Collaboration
      • Transients and Variable Stars Science Collaboration
      • Strong Lensing Science Collaboration
      • Informatics and Statistics Science Collaboration
    • Citizen Science
      • Committees and teams
      • Science Advisory Committee (SAC)
      • Survey Cadence Optimization Committee (SCOC)
      • Users Committee
      • Community Science Team (CST)
      • Research Inclusion Working Group (RIWG)
      • Project Science Team (PST)
    • Frequently Asked Questions
    • Education
    • Education FAQs
    • Educators
    • Glossary
    • Investigations
    • Calendar
Localize site content
  1. Education
  2. Educators
  3. Investigations
  4. Coloring the Universe
  5. Teacher Guide - Coloring the Universe
  6. Background and Notes

Coloring the Universe

Start Investigation
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

Background and Notes

Background

The image sensor of a digital camera, whether in a phone or in an astronomical instrument, contains an array of light receptors that only detect levels of light, not color. In order to convert this greyscale image into a color image, filters are used to select light over a specific range of wavelengths, then colors are assigned to the image created by each filter.

Astronomical images created from broadband filters are typically constructed using the chromatic ordering technique, in which the light from each filter is assigned a color based on wavelengths. The light transmitted by the filter passing the shortest wavelengths is assigned the shortest wavelength of visible light color in the image, and the process continues with each successive filter, so that the light passing through the filter that transmits the longest wavelengths of light is assigned the visible light color with the longest wavelength.


OpenStax Astronomy textbook links:

Visible light detectors and instruments

Electromagnetic Spectrum


Teacher Notes

  1. Our investigations are designed so that students cannot proceed to the next page without answering each question. If you would like to quickly preview the entire investigation, you can create a free account and use the “logged in" mode on the Start page.
  2. The information about how filters pass light on p. 4 of the investigation (including the interactive filter tool) is intentionally oversimplified. Filters are often designed to pass a range of colors, not just one.
  3. Each investigation includes some questions that invite students to share their world views and life experiences to make connections between science and the real-world. In this investigation, the question is on page 19. This may be an opportunity for a small group or class discussion, or if in an asynchronous setting, students can contribute to a discussion forum.
  4. It may be useful to have a discussion with students, after they have completed the practice image, to clarify which options are available for creating a new image. This should occur on page 25, “Putting it all Together”. When students have selected their object(s) to investigate and form a question, they should draft a plan (as described in the investigation) for which filters and images they will need and how they will construct and analyze their image(s).
  5. Not all six filters need to be used to construct a color image. Students can decide which filters to use based on the suggested guidelines illustrated in the tutorial examples, and they can also turn off a filter if it doesn’t contribute to the desired result.

    Back to Coloring the Universe
Previous (Next Generation Science Standards)Next (Student Ideas and Questions)