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How could we answer the ‘burningest question’ about the universe? Neil deGrasse Tyson explains

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Original Story by CNN
September 20, 2026
How could we answer the ‘burningest question’ about the universe? Neil deGrasse Tyson explains

Context:

The segment discusses NASA’s Nancy Grace Roman Space Telescope as a complementary successor to Hubble and Webb, capable of surveying vast swaths of the sky to map the three-dimensional distribution of galaxies and detect faint ripples that inform our understanding of the Big Bang. It emphasizes that Roman’s wide-field capabilities enable rapid, large-scale mapping that would be impractical for the older telescopes, while Hubble and Webb will continue detailed follow-up observations. The three telescopes are portrayed as a synergistic trio: Roman performs discovery and context, while the others refine and deepen insights. The outlook highlights ongoing collaboration among missions to build a more complete picture of cosmic origins, with Roman offering a new perspective that existing instruments cannot achieve on their own.

Dive Deeper:

  • Roman is described as a survey-focused telescope able to observe a large portion of the sky simultaneously, enabling rapid mapping of galaxies and their three-dimensional structure.

  • The segment notes that Roman will look for faint ripples in galaxy patterns, which are expected to yield clues about events near the Big Bang and the early universe.

  • Hubble and Webb are not portrayed as obsolete; instead, they will complement Roman by performing high-detail follow-up observations on objects and phenomena identified in Roman’s survey.

  • The discussion distinguishes two mission types in astronomy: broad survey missions to discover unknown phenomena and follow-up missions to study known targets in greater depth.

  • A collaborative vision is emphasized, with Roman providing a new vantage point that existing telescopes can’t achieve, while the other telescopes stay engaged for years to come.

  • The segment frames the Roman launch as a stepping stone within an integrated strategy to advance our understanding of cosmic structure and the early universe.

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