A SCIENCE EXPEDITION / 3 CHAPTERS / 8 STOPS
The Universe Behind the Veil
How do you find a galaxy when your own galaxy gets in the way?
Change the wavelength, inspect the foreground, and follow hidden galaxies into a wider map. Then test a much harder case: a spectral line whose source still lacks a secure identity.
75–120 minutes, across several visits. No deadline; each chapter is a natural place to pause.

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EXPEDITION COMPLETE
You followed the evidence.
Which measurement established an object, which established a distance, and which observation would you request before putting the last unknown source on your cosmic map?
Your completion marks record your journey, not a qualification or a test score. Revisit any stop below, or choose another expedition.
Choose another expedition →Chapter 1 · Meet the foreground
- 01
3D Atlas
Find the observer inside the obstacle
Ready to exploreLocate the Sun in the illustrated Milky Way. Consider how looking along the Galactic plane changes the foreground. The artist model does not map every intervening dust cloud.
- 02
Investigation
Follow two separate hidden-system cases
Ready to exploreTrace the diffuse VVVX galaxy candidate and the separate X-ray-selected cluster. Keep their measurements and distance evidence distinct; sharing a foreground does not make them one discovery.
Chapter 2 · Change the measurement
- 03
Interactive lab
See what a different band can reveal
Ready to exploreCompare visible and infrared views, then read the astrophysical explanation. Distinguish emitted thermal radiation from light transmitted through dust; a thermal camera is not a literal simulator of a galaxy survey.
- 04
Evidence File
Audit the identification and the distance
Ready to exploreSeparate extended light, morphology, cluster gas and redshift measurements. Which case has a confirmed redshift, and which proposed distance remains conditional?
- 05
3D Atlas
Ask what belongs on the map
Ready to exploreExplore the Local Group and cosmic structure model. Explain how a survey’s selection can leave an apparent gap. Keep the illustrated arrangement separate from a complete measured inventory.
Chapter 3 · Try a source with one stubborn clue
- 06
Interactive lab
Build a test with more than one feature
Ready to exploreCompare spectral fingerprints in the teaching model. Decide which additional line or wavelength coverage would help distinguish competing identifications of an unknown source.
- 07
Investigation
Investigate a source that resists its label
Ready to exploreFollow Webb’s unidentified 1.60-micrometer line. Keep the earlier imaging separate from later spectra, and list the proposed source explanations without treating any as confirmed.
- 08
Evidence File
Specify the observation that would decide
Ready to exploreSeparate a detected line from a secure redshift and a physical source identity. Propose follow-up data that would rule out at least one interpretation rather than merely making a brighter picture.
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