About the Object

Category: Graphics
MIRI

Protoplanetary disc XUE 1 (MIRI emission spectrum: 13.3–15.5 microns)

This graphic presents some of the first results from the eXtreme UV Environments (XUE) James Webb Space Telescope programme. These results suggest that the conditions for rocky-planet formation, typically found in the discs of low-mass star-forming regions, can also occur in massive-star-forming regions and possibly a broader range of environments.

Astronomers focussed on rocky-planet-forming regions of discs in the Lobster Nebula using Webb’s Medium Resolution Spectrometer (MRS) of the Mid-InfraRed Instrument (MIRI). This first result focuses on the protoplanetary disc termed XUE 1, which is located in the star cluster Pismis 24.

The inner disc around XUE 1 revealed signatures of water (highlighted here in blue and centred around 14.2 microns), as well as acetylene (C2H2, highlighted in green; centred around 13.7 microns), hydrogen cyanide (HCN, highlighted in brown; centred around 14.0 microns), and carbon dioxide (CO2, highlighted in red; centred around 14.95 microns). As indicated, some of the emission detected was weaker than some of the predicted models, which might imply a small outer disc radius.

[Image description: Graphic titled “XUE 1 Irradiated Protoplanetary Disc, MIRI Medium -Resolution Spectroscopy” shows a graph of brightness versus wavelength from 13.3 to 15.5 microns, with acetylene, hydrogen cyanide, water, and carbon dioxide peaks highlighted]

Credit:

NASA, ESA, CSA, STScI, J. Olmsted (STScI), M. C Ramírez-Tannus (Max Planck Institute for Astronomy)

About the Image

Id: weic2329b
Type: Chart
Release date: 30 November 2023, 16:00
Related releases: weic2329
Size: 3840 x 2160 px


Image Formats

Download IconLarge JPEG 537.6 KB
Download IconScreensize JPEG 113.3 KB

Zoomable


Wallpapers

Download Icon1024x768 131.1 KB
Download Icon1280x1024 175.3 KB
Download Icon1600x1200 223.3 KB
Download Icon1920x1200 258.2 KB
Download Icon2048x1536 298.7 KB

Also see our