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Gravitational Lensing

A square graphic breaks down how gravitational lensing by foreground galaxies influences the appearance of far more distant background galaxies.
This diagram illustrates how gravitational lensing by foreground galaxies influences the appearance of far more distant background galaxies. These far-off galaxies that might otherwise be invisible appear due to lensing effects. The plane at far left contains very distant, background galaxies. The middle plane represents foreground galaxies; their gravity amplifies the brightness of the background galaxies. The right plane shows how the field would look from Earth with the effects of gravitational lensing added.

Extended Description and Image Alt Text

Extended Description

Within a blue square are three smaller black squares shown at an angle. Two white lines ending in arrow points connect the black squares.

Below the top left black box, two labels appear. Next to an opaque red oval is text that reads "Observable distant galaxy." Beneath that and next to a red outline of an oval is text that reads "Distant galaxy too faint to detect." In the black box, which is the smallest of the three, there are nine red oval outlines and three opaque red ovals scattered throughout the view. A white arrow begins at a red oval outline toward the top left, and a second toward the bottom right, also piercing an oval outline.

The middle black square is slightly larger. There are two labels below this box. Next to an opaque light blue oval is text that reads "Relatively nearby galaxy." Beneath that and next to a slightly larger, dotted light blue circle is text that reads "Gravitational lensing influence of foreground galaxy." The second black box contains five opaque light blue ovals. Each is surrounded by a light blue dotted circle. The first white arrow continues to follow a straight path, piercing the top left galaxy, between the dotted circle and the opaque central oval. The second arrow pierces a galaxy at the bottom right in the same location.

The largest black box at right has one label below it that reads "Observed by Webb." This black box shows five galaxies that are light blue and completely opaque with white at the center. They are at the same positions as the blue galaxies in the middle panel. Three red galaxies with small white centers, which are also opaque, appear at bottom center and top right. They are at the same positions as the opaque red galaxies in the first panel. The first line ending in an arrow points to an orange circle, which is also opaque, that is immediately to the right of a blue galaxy at top left. They barely touch. The second line, which also ends in an arrow pointing right, points to an orange opaque circle that sits to the left of a blue galaxy at the bottom right. The two orange galaxies are at the same positions as the outlined galaxies in the first panel with white arrows.

The lines indicate that when light from a galaxy that would otherwise be too faint to detect passes through the area of gravitational lensing influence of a foreground galaxy, it will make the faint galaxy observable by Webb.

Image Alt Text

A square graphic breaks down how gravitational lensing by foreground galaxies influences the appearance of far more distant background galaxies.

  • Release Date
    March 21, 2019
  • Science Release
    NASA’s Webb to Explore Galaxies from Cosmic Dawn to Present Day
  • Credit
    Image: NASA, ESA, Zoltan Levay (STScI), Ann Feild (STScI)

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Details

Last Updated
Aug 28, 2025
Contact
Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Image Credit

NASA, ESA, Zoltan Levay (STScI), Ann Feild (STScI)