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Hubble and Roman Bring Different Strengths to Galaxy Images

A detailed view and a broad survey complement each other.

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Science news editorial illustration for Hubble’s Bent-Light Images Prepare the Way for Roman

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Source: NASA Hubble Mission Team, 2026-11-12.

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Try 2 questions about this story, then explain one idea in your own words. Check the text whenever you need to.

In this lesson: Connect distorted light with complementary research roles.

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Read and understand · 1/2Which galaxies provide the bending gravity?

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Nearer galaxies. The first paragraph identifies nearer galaxies as the cause of the distortion.

Clue: NASA’s new Hubble gallery shows distant galaxies distorted by the gravity of nearer galaxies. The bent light can form arcs.

Read and understand · 2/2Why combine the observations?

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To study mass using detailed and wider views. The second paragraph gives their different strengths and the intended study of mass.

Clue: Hubble provides detailed individual views, while Roman covers a wider field. Researchers plan to combine their observations to study mass, including dark matter.

Grammar in this story: A comparison of capabilities

while

While contrasts Hubble’s individual detail with Roman’s wider field here; it does not mean the capabilities are identical.

Your turn

Describe the cause of the arcs and the planned benefit of combining observations.

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The gravity of nearer galaxies distorts light from distant galaxies into arcs. Researchers plan to combine Hubble’s detailed views with Roman’s wider coverage to study mass, including dark matter.

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