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Giant Star in Dwarf Galaxy Sextans A (Spectrum)

Graphic titled “Giant Star in Dwarf Galaxy Sextans A: Iron-Rich Dust at Low Metallicities” showing a graph of brightness versus wavelength, with two sets of data and two model spectra. One set of data is represented in 12 orange triangle data points, and the other is a solid yellow line. A cyan solid line represents “Iron + 0.8% silicates” and a red dashed line represents “Iron + 5% silicates.” They appear on a graph of Brightness on the y-axis versus Wavelength of Light in microns on x-axis. The y-axis ranges from dimmer at bottom to brighter at top. The x-axis ranges from 0 to 12 microns.

This graph shows a spectrum of a giant star in the Sextans A galaxy at the very end of its evolution, called an Asymptotic Giant Branch (AGB) star. It displays the amounts of near- and mid-infrared light detected from the star by NASA’s James Webb Space Telescope at different wavelengths.

The cyan line and red dashed line are best-fit models for the spectrum that would contain mostly silicate-free dust and dust containing at least 5% silicates, respectively. The Webb data, shown as a yellow line and orange triangles, align most closely with nearly silicate-free dust, most notably in the 10 micron wavelength region of the spectrum.

  • Release Date
    January 6, 2026
  • Science Release
    NASA Webb Finds Early-Universe Analog’s Unexpected Talent for Making Dust
  • Credit
    Illustration: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI)

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Last Updated
Jan 06, 2026
Contact
Media

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