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Giant Star in Dwarf Galaxy Sextans A (Spectrum)

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 DateJanuary 6, 2026
- Science ReleaseNASA Webb Finds Early-Universe Analog’s Unexpected Talent for Making Dust
- CreditIllustration: NASA, ESA, CSA, STScI, Joseph Olmsted (STScI)
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov








