People seem most impressed by the apparent increase in resolution of the images, which is not from a certain point of view the hardest thing to do . HST might have done that if its instruments had been of different pixel size or imaging array size / focal length. Ok, the much larger mirror is an achievement. But anyway, the resolution of the images is often not what really is the limiting factor for photometric observations. Yes it is sharper/higher resolution, but that wasn't the key selling point.
The new thing is observations in the IR, which is somewhat a technical footnote in many gushing announcements of these images (or some discussion here too). And the general public knows little about that detail's importance, especially since the images are stylized / colored anyway to look just like RGB images that we are so familiar with. But everyone can easily appreciate a sharper image.
Anyway, still a momentous achievement. And thank god we have a scientific field where stunning images was enough to get the public to support a $10B project.
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Edit to add: I did not mean to detract from or diminish anyone's appreciation of the images and accomplishment at whatever level they are enjoyed. And of course many here are technically knowledgeable about the IR aspect. I just write to point out that for the most headline-grabbing images and newspaper writers, the sharpness of the images over the actual IR frontier is what grabs the attention.
Not a new thing.
Herschel space observatory operated in same location (L2-point) as JWST and it was IR telescope. https://www.google.com/search?q=Herschel+space+observatory+i...
Mirror sizes:
Hubble 4.0 m2 (43 sq ft)
Herschel 9.6 m2 (103 sq ft)
JWST 25.4 m2 (273 sq ft)
Hubble had ~40% of the Herschel's collecting area and Herchel had 40% of the JWST's collecting area.HST is already imaging at diffraction-limited resolution (with proper post-processing). It would need a bigger mirror to get there.
> stunning images was enough to get the public to support a $10B project.
I don't believe public support is relevant; is there public support for the >$700B a year spent on the military?
More comparisons on Twitter, some zoomed in:
- https://twitter.com/Batsuto_/status/1546899241880240128
- https://twitter.com/Batsuto_/status/1546900387931766784
- https://twitter.com/JBWillcox/status/1546881033597075457
- https://twitter.com/jason4short/status/1546626672488632321
I'm not a physicist, so I've only recently learned about redshift. Hubble's deep field images were very dark red/orange because further objects appear redder (into infrared) before they disappear to the observer. Webb's sensors are more red/infrared-sensitive than Hubble's, so along with extremely fine, super-cooled optics using exotic materials to align and capture every single photon, its red sensitivity allows Webb to peer deeper, further, and dimmer than we've ever been able to before.
And I've read that the "spikes" coming off the brighter stars are generally from stars in our own galaxy and they're not lens flares. They're caused by the edges of the telescope. Hubble's stars would have 4 spikes in a cross; Webb has 6 in a snowflake because of the shape of Webb's mirrors having 6 sides. Or something like that.
I'm trying to understand how much the improvement is "speed of convergence" vs. "quality of asymptotic result". (Though... is that even a valid way of trying to understand things?)
What am I missing?
It seems to negatively degrade the photos taken much more so than Hubble.
Also curious about what the closest stars to our solar system would look like. Of course it also makes me wonder what would we be able to see given a 100x increase in aperture. Like for example if we could send up something extremely large on Starship. Would we be able to image planets in our local group? Exciting!
Searching for this stuff is kind of hard (information overload), so I'm wondering if anyone here has more up to date info.
What happens when it's pointed at Mars?
Ah found answer here
https://space.stackexchange.com/questions/57492/can-james-we...
[1]: https://en.wikipedia.org/wiki/File:Stephan%27s_Quintet_Hubbl... [2]: https://johnedchristensen.github.io/WebbCompare/img/Stephans...
It might be because of a different post-processing algorithm, or some phi-related magic, just curious a bit.
> > Hubble telescope was funded and built in the 1970s by the United States space agency NASA with contributions from the European Space Agency. Its intended launch was 1983, but the project was beset by technical delays, budget problems, and the 1986 Challenger disaster. Hubble was finally launched in 1990.
I commented on this other thread: https://news.ycombinator.com/item?id=32074242
Very nicely done!
At this point I like it even for just brightening the news cycle anyway.
1. Can the telescope be pointed in any direction? (of course, orthogonal to the suns rays, I understand the need to cool it down).
2. If it can be pointed, I am assuming some boosters would be used to pivot it. How long do these last?
3. Is there any info on the orbit? Can the orbit degrade?
4. All the fluid / gas required to correct / point, can it be refilled?
Too bad, then, about the crappy colorizing/outlining for the 'so pretty' crowd. I await the site that simply shows (frequency-shifted) images. Any colorizing should have a 'legend' describing its purpose.
what's more interesting to me is what we can learn about exoplanets from this mission
https://www.nasa.gov/image-feature/goddard/2022/nasa-s-webb-...