NASA’s James Webb Space Telescope is aligned across all four of its science instruments, as seen in a previous engineering image showing the observatory’s full field of view. Now, we take a closer look at that same image, focusing on Webb’s coldest instrument: the Mid-Infrared Instrument, or MIRI.
The MIRI test image (at 7.7 microns) shows part of the Large Magellanic Cloud (LMC). This small satellite galaxy of the Milky Way, located about 160,000 light-years away, provided a dense star field to test Webb’s performance.
Here, a close-up of the MIRI image is compared to a past image of the same target taken with NASA’s Spitzer Space Telescope’s Infrared Array Camera (at 8.0 microns). The retired Spitzer telescope was one of NASA’s Great Observatories and the first to provide high-resolution images of the near- and mid-infrared universe. Webb, with its significantly larger primary mirror and improved detectors, will allow us to see the infrared sky with improved clarity, enabling even more discoveries.
For example, Webb’s MIRI image shows the interstellar gas in unprecedented detail. Here, you can see the emission from “polycyclic aromatic hydrocarbons,” or molecules of carbon and hydrogen that play an important role in the thermal balance and chemistry of interstellar gas. When Webb is ready to begin science observations, studies such as these with MIRI will help give astronomers new insights into the birth of stars and protoplanetary systems.
In the meantime, the Webb team has begun the process of setting up and testing Webb’s instruments to begin science observations this summer.
The James Webb Space Telescope is an international partnership between NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA). MIRI is part of Europe’s contribution to the Webb mission. It is a partnership between Europe and the USA; the main partners are ESA, a consortium of nationally funded European institutes, the Jet Propulsion Laboratory (JPL), and NASA’s Goddard Space Flight Center (GSFC).
Never miss a breakthrough: Join the SciTechDaily newsletter.
Follow us on Google and Google News.
6 Comments
Interesting.
Just a thought. How accurately can we use the image database to rebuild the reality out their to Scale, of the information captured?
Mapping the Universe is a arduous task, and will need a NEW but old skill – “Geographers” also known as cartographers. However in this effort, we wont be mapping continents, but stars, planets, galaxies and such!
It may be a smart thing to put in place cross functional teams to make sense of the data which will start flowing in.
Views expressed are personal and not binding on anyone.
Will there be a final adjustment to reduce the major 8 sided lens flare? Software may possibly reduce these image distortions but any artificial manipulation of the data will be unfortunate.
Don’t care what people think, this is worth every dime we spend on it.
Yes – absolutely!
Fascinating how much movement/ disappearance (as well as clarification) occurs between Spitzer features and those in the JWST image. Foreground, but faint, Milky Way objects moving relative to the LMC, presumably, rather than variables.
Fantastic combined images they have such clarity it’s amazing. I can’t wait for the new images.