Webb identifies Beta Pictoris d through its atmospheric fingerprints
The James Webb Space Telescope identified Beta Pictoris d through molecular signals, not merely as a bright spot. Its mass and orbit remain estim...
spectrograph
NIRSpec is the Near-Infrared Spectrograph aboard the James Webb Space Telescope, supporting fixed-slit, integral-field, time-series and multi-object spectroscopy.
NIRSpec is the Near-Infrared Spectrograph aboard the James Webb Space Telescope. It is designed to obtain spectra at near-infrared wavelengths, operating across approximately 0.6 to 5.3 micrometres. Its observing modes include fixed-slit, integral-field, time-series and multi-object spectroscopy, allowing spectra to be gathered in different observational configurations. A microshutter array permits the simultaneous collection of spectra for more than 100 targets. ESA provided the array, with NASA subsystems. NIRSpec is an instrument rather than a separate telescope or mission; its stated capabilities describe spectroscopic observing modes and wavelength coverage, not results for any particular target.
Context
The James Webb Space Telescope identified Beta Pictoris d through molecular signals, not merely as a bright spot. Its mass and orbit remain estim...
James Webb Space Telescope observations of Abell2744-QSO1, an object known as a “little red dot,” made it possible to directly measure the mass o...
For LID-568, a supermassive black hole at the center of a galaxy that existed about 1.5 billion years after the Big Bang, the team estimates a fe...