Webb image archive

Water Abundance (MIRI Emission Spectrum)

This graphic compares the spectral data for warm and cool water in the GK Tau disk, which is a compact disk without rings, and extended CI Tau disk, which has at least three rings...

Date
Dec 13, 2023
Observatory
James Webb Space Telescope
Credit
NASA / ESA / CSA / STScI
Archive ID
01HDS7PA32HT7KKFQ3GJESTT6Z

This graphic compares the spectral data for warm and cool water in the GK Tau disk, which is a compact disk without rings, and extended CI Tau disk, which has at least three rings on different orbits. The science team employed the unprecedented resolving power of MIRI’s MRS (the Medium-Resolution Spectrometer) to separate the spectra into individual lines that probe water at different temperatures. These spectra, seen in the top graph, clearly reveal excess cool water in the compact GK Tau disk, compared with the large CI Tau disk.

The bottom graph shows the excess cool water data in the compact GK Tau disk minus the cool water data in the extended CI Tau disk. The actual data, in purple, are overlaid on a model spectrum of cool water. Note how closely they align.

Credits

Illustration

NASA, ESA, CSA, Leah Hustak (STScI)

Science

Andrea Banzatti (Texas State University)

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