Webb’s infrared view of the Tarantula Nebula
The two images to the right, reduced and annotated to post here, were released today by the science team of the James Webb Space Telescope, and show two different views of the Tarantula Nebula, located 161,000 light years away in the Large Magellanic Cloud.
It is home to the hottest, most massive stars known. Astronomers focused three of Webb’s high-resolution infrared instruments on the Tarantula. Viewed with Webb’s Near-Infrared Camera (NIRCam) [top], the region resembles a burrowing tarantula’s home, lined with its silk. The nebula’s cavity centered in the NIRCam image has been hollowed out by blistering radiation from a cluster of massive young stars, which sparkle pale blue in the image. Only the densest surrounding areas of the nebula resist erosion by these stars’ powerful stellar winds, forming pillars that appear to point back toward the cluster. These pillars contain forming protostars, which will eventually emerge from their dusty cocoons and take their turn shaping the nebula.
…The region takes on a different appearance when viewed in the longer infrared wavelengths detected by Webb’s Mid-infrared Instrument (MIRI) [bottom]. The hot stars fade, and the cooler gas and dust glow. Within the stellar nursery clouds, points of light indicate embedded protostars, still gaining mass. While shorter wavelengths of light are absorbed or scattered by dust grains in the nebula, and therefore never reach Webb to be detected, longer mid-infrared wavelengths penetrate that dust, ultimately revealing a previously unseen cosmic environment.
As with all images from Webb, these are false color, as the telescope views the infrared heat produced by stars and galaxies and interstellar clouds, not the optical light our eyes see. Thus, the scientists assign different colors to the range of wavelengths each instrument on Webb captures.
These photos once again illustrate Webb’s value. It will provide a new layer of data to supplement the basic visual information provided by the Hubble Space Telescope, allowing scientists to better understand the puzzles we see in the optical.
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In 2020 when the world panicked over COVID I wrote that the panic was unnecessary, that the virus was apparently simply a variation of the flu, that masks were not simply pointless but if worn incorrectly were a health threat, that the lockdowns were a disaster and did nothing to stop the spread of COVID. Only in the past year have some of our so-called experts in the health field have begun to recognize these facts.
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The two images to the right, reduced and annotated to post here, were released today by the science team of the James Webb Space Telescope, and show two different views of the Tarantula Nebula, located 161,000 light years away in the Large Magellanic Cloud.
It is home to the hottest, most massive stars known. Astronomers focused three of Webb’s high-resolution infrared instruments on the Tarantula. Viewed with Webb’s Near-Infrared Camera (NIRCam) [top], the region resembles a burrowing tarantula’s home, lined with its silk. The nebula’s cavity centered in the NIRCam image has been hollowed out by blistering radiation from a cluster of massive young stars, which sparkle pale blue in the image. Only the densest surrounding areas of the nebula resist erosion by these stars’ powerful stellar winds, forming pillars that appear to point back toward the cluster. These pillars contain forming protostars, which will eventually emerge from their dusty cocoons and take their turn shaping the nebula.
…The region takes on a different appearance when viewed in the longer infrared wavelengths detected by Webb’s Mid-infrared Instrument (MIRI) [bottom]. The hot stars fade, and the cooler gas and dust glow. Within the stellar nursery clouds, points of light indicate embedded protostars, still gaining mass. While shorter wavelengths of light are absorbed or scattered by dust grains in the nebula, and therefore never reach Webb to be detected, longer mid-infrared wavelengths penetrate that dust, ultimately revealing a previously unseen cosmic environment.
As with all images from Webb, these are false color, as the telescope views the infrared heat produced by stars and galaxies and interstellar clouds, not the optical light our eyes see. Thus, the scientists assign different colors to the range of wavelengths each instrument on Webb captures.
These photos once again illustrate Webb’s value. It will provide a new layer of data to supplement the basic visual information provided by the Hubble Space Telescope, allowing scientists to better understand the puzzles we see in the optical.
Readers!
Please consider supporting my work here at Behind the Black. Your support allows me the freedom and ability to analyze objectively the ongoing renaissance in space, as well as the cultural changes -- for good or ill -- that are happening across America. Fourteen years ago I wrote that SLS and Orion were a bad ideas, a waste of money, would be years behind schedule, and better replaced by commercial private enterprise. Only now does it appear that Washington might finally recognize this reality.
In 2020 when the world panicked over COVID I wrote that the panic was unnecessary, that the virus was apparently simply a variation of the flu, that masks were not simply pointless but if worn incorrectly were a health threat, that the lockdowns were a disaster and did nothing to stop the spread of COVID. Only in the past year have some of our so-called experts in the health field have begun to recognize these facts.
Your help allows me to do this kind of intelligent analysis. I take no advertising or sponsors, so my reporting isn't influenced by donations by established space or drug companies. Instead, I rely entirely on donations and subscriptions from my readers, which gives me the freedom to write what I think, unencumbered by outside influences.
You can support me either by giving a one-time contribution or a regular subscription. There are four ways of doing so:
1. Zelle: This is the only internet method that charges no fees. All you have to do is use the Zelle link at your internet bank and give my name and email address (zimmerman at nasw dot org). What you donate is what I get.
2. Patreon: Go to my website there and pick one of five monthly subscription amounts, or by making a one-time donation.
3. A Paypal Donation or subscription:
4. Donate by check, payable to Robert Zimmerman and mailed to
Behind The Black
c/o Robert Zimmerman
P.O.Box 1262
Cortaro, AZ 85652
You can also support me by buying one of my books, as noted in the boxes interspersed throughout the webpage or shown in the menu above.
Minor edit in first paragraph: “two different views”
Andi. Fixed. Thank you.
The rest of us cannot possibly interpret the images in a meaningful way without a wavelength vs.assigned color/interpreted physical process scorecard.
Not in the budget? No need for the curtain to be opened.
Who are taxpayers to care?
Don’t let the curtain be opened.
There are papers to be written for professional credit.
GaryMike: The press release describes in very good detail the different meanings of the colors. If you really want to find out, I guarantee that a little bit of searching on the web will find this info. They are not keeping it secret, in the slightest.
You know I have little trust or love of government. You know I considered Webb an overpriced boondoggle. But I don’t assume everything done by the government is automatically evil. When it comes to these NASA projects, NASA is legally required to make the data available, and does so. You simply have to look for it.
RZ:
“They are not keeping it secret, in the slightest.”
I’m busy. The information should have been given up front so I don’t have to do “a little bit of searching ”
Having been a teacher in an earlier professional life, I never told my students to “do my job for me”.
GaryMike.
I hope you taught your students how to do their own research, as this is how we get lifelong learning, as opposed to the standard amount of school learning, five-hours a day of stuff that (at the time) we find uninteresting. Once we are out of school, we get to research the stuff that interests us. We may even think that it interests other people enough that we turn that research into a book or two (the royalties almost coming close to nearly being worth the time spent).
I’m not sure how much interpretation the rest of us are supposed to do. We pay the principal investigator and his team to do this. It seems to me that the importance of these two photographs is for us to understand that the different wavelengths present us with different information, explaining why we want telescopes that see in more than just visible light.
The Hubble telescope originally cost us three times its intended price, but after the scheduled maintenance and upgrades, we are getting science from it that costs reasonably close to the intended price. It is a good thing that Webb is giving us all this information. Each of its photographs costs us about ten times what we had intended (assuming it lasts its intended lifespan), plus it cost us the science that was lost due to the cost overruns (lost opportunity costs). For Webb’s premium price, we should expect premium science.
Edward,
My beef is not with the principle investigator(s). They have one-year proprietary periods allowing them time to publish their discoveries free of opportunistic piracy.
My beef is with folks who treat stuff like art open to interpretation more than education that gets to the point.
“For Webb’s premium price, we should expect premium science.”
That made me laugh. I maintain that humor is based on pain, and the Webb cost is painful, indeed. However, despite the armchair-quarterbacking many (ahem) engaged in, I am very pleased to see the machine functioning in a nominal capacity. There are those random rock strikes, though . . .