Early data from the James Webb Space Telescope is already starting to come in, with exciting finds like views of Jupiter and a potential sighting of the most distant galaxy ever observed.
But there’s a lot more Webb data being shared, and much of it is publicly available through the Space Telescope Science Institute’s MAST archive. That means enterprising astronomers are already digging through James Webb data to perform their own analyses, and have created some amazing visuals.
Gabriel Brammer, an associate professor at the University of
Copenhagen, composed and shared this incredible and faintly terrifying image on
Twitter. It shows the galaxy Messier 74, captured in the mid-infrared range by
Webb’s MIRI instrument as part of the PHANGS-JWST project.
The nearby spiral galaxy M74 (NGC 628) observed by JWST on July 17, 2022. The color image is a composite of three monochromatic images from the MIRI instrument at wavelengths 7.7, 10, and 11 µm. The striking purple filamentary structures are emissions from interstellar dust and polycyclic aromatic hydrocarbon (PAH) molecules.Color composite, Gabriel Brammer (Cosmic Dawn Center, Niels Bohr Institute, University of Copenhagen); Raw data, Janice Lee et al. and the PHANGS-JWST collaboration
“Let’s just see what JWST observed yesterday …” Brammer wrote on Twitter. Then, echoing all of our sentiments, “Oh, good god.”
The image is this striking purple color because of the way
the data is processed, in order to show off the structures of dust and
hydrocarbons which swirl around the galaxy. The data used was taken on July 17
2022 at three different wavelengths in the mid-infrared: 7.7 µm, 10 µm, and 11
µm.
The galaxy looks very different in visible light
wavelengths, as shown in this image of Messier 74 captured by the European
Southern Observatory’s New Technology Telescope:
ESO’s PESSTO survey has captured this view of Messier 74, a
stunning spiral galaxy with well-defined whirling arms.ESO/PESSTO/S. Smartt
The James Webb data was collected as part of the PHANGS
project, or Physics at High Angular resolution in Nearby GalaxieS, which is a
survey that uses multiple different instruments including Hubble and
ground-based telescopes to study how stars form from clouds of dust. The
project will also work with Webb in order to peer through the clouds of dust
which can otherwise obscure galaxies and get a clearer look at the star
formation going on within.
The leader of the Webb part of the PHANGS research, Janice
Lee of the National Science Foundation’s NOIRLab, said before the observations
began that Webb could provide vital insights into understanding the life of
stars: “JWST touches on so many different phases of the stellar life cycle –
all in tremendous resolution,” Lee said in a statement. “Webb will reveal star
formation at its very earliest stages, right when gas collapses to form stars
and heats up the surrounding dust.”
This article first appeared on DigitalTrends