The James Webb Space Telescope

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The James Webb Space Telescope (JWST) is scheduled to launch no earlier than December 24, following a two-day delay, with a critical launch window extending to January 6 due to gravitational concerns. Enthusiasm is high among the community, with many eagerly anticipating the scientific data it will provide, despite concerns over the lengthy wait and significant costs associated with the project. Initial observing time has been allocated for various proposals, including a major project called Cosmos Web, which aims to capture detailed images of the early universe. The mission's success is seen as a gamble, with many previous missions sacrificed for JWST funding, raising questions about the return on investment. As the launch approaches, excitement and nervousness are palpable, with many setting alarms to witness the event live.
  • #331
Kevin the Kiwi said:
I wonder if someone can answer a question for me. Probably a silly question but I am looking at the "star death" image, the planetary nebula. It looks like we are looking through a big hole in a spherical object, or is it a flat ring around the star we are looking at from above? The main reason for my question is that you can see the gas and dust inside the nebula that looks like behind the star it is a solid wall. I imagine when the star explodes it blows stuff out in all directions.
It is a spherical shell, but you are looking through less material in the center as along the edges (see sketch), so it makes it look like an annular ring. The material you say is "behind the star" is both in front of and behind the star.

Screen Shot 2022-07-13 at 10.30.43 AM.png
 
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  • #332
phyzguy said:
It is a spherical shell, but you are looking through less material in the center as along the edges (see sketch), so it makes it look like an annular ring. The material you say is "behind the star" is both in front of and behind the star.

View attachment 304135

Ah yes, that makes complete sense, I honestly never would have thought of that. Thank you for your reply.
 
  • #333
jupiter_hi_res_atmo-1.png


“Jupiter, center, and its moon Europa, left, are seen through the James Webb Space Telescope’s NIRCam instrument 2.12 micron filter. Credits: NASA, ESA, CSA, and B. Holler and J. Stansberry (STScI)”
https://blogs.nasa.gov/webb/2022/07...and-more-now-available-in-commissioning-data/

james-webb-jupiter-nasa.png

“Two photos of Jupiter taken by the James Webb Space Telescope. The left image was taken using a NIRCam (near infrared camera) to examine the planet’s short wavelengths of light. The right image was taken with a filter that highlights long wavelengths. NASA”

https://globalnews.ca/news/8987398/james-webb-space-telescope-pictures-jupiter-why-you-missed-them/
 
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  • #335
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  • #336
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  • #338

Webb telescope suffered ‘uncorrectable damage’ in micrometeoroid hit, NASA report says​

https://thehill.com/policy/technolo...amage-in-micrometeoroid-hit-nasa-report-says/

At 21 feet, Webb’s gold-plated, flower-shaped mirror is the biggest and most sensitive ever sent into space. It’s comprised of 18 segments, one of which was smacked by the bigger than anticipated micrometeoroid in May. Micrometeoroids are fragments of asteroids that are usually smaller than a grain of sand, according to NASA.

https://www.yahoo.com/news/webb-telescope-suffered-uncorrectable-damage-030948640.html
 
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  • #339
Here's a new video from the Royal Institution:
(I haven't seen it yet, but I wanted to share it)

Solar system science from the James Webb Space Telescope – with Naomi Rowe-Gurney (RI)
What is the JWST, and what big science questions can it answer? Join NASA scientist Naomi as she discusses the new JWST images, along with her research into the ice giants, Uranus and Neptune, and the many other areas that JWST can help with.


Edit: And the Q&A is here:

Q&A: Solar system science from the James Webb Space Telescope – with Naomi Rowe-Gurney (RI)
 
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  • #341
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  • #342
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  • #349
I was surprised at the nomenclature -- Population III stars in the oldest galaxies. I would have guessed that the numbering would run the other direction. I looked it up and learned that my understanding was backwards.

Every day on PF I get to learn something new. :smile:
 
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  • #350
Astronomy has the interesting practice that nothing ever gets re-defined. Hipparchus defined the magnitude scale almost 3000 more than 2000 years ago, and called the brightest stars 1st magnitude, the next brightest 2nd magnitude, and so on. So we are stuck with a magnitude scale that runs backwards - where brighter stars have a smaller magnitude than dimmer stars.

Population I and Population II were defined before anyone knew why they were different and that Population II came before Population I.
 
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  • #352
test_00002.jpg

test_00003.jpg
 
  • #353
@Devin-M are we supposed to guess what those are?
 
  • #354
phyzguy said:
Astronomy has the interesting practice that nothing ever gets re-defined. Hipparchus defined the magnitude scale almost 3000 more than 2000 years ago, and called the brightest stars 1st magnitude, the next brightest 2nd magnitude, and so on. So we are stuck with a magnitude scale that runs backwards - where brighter stars have a smaller magnitude than dimmer stars.

Population I and Population II were defined before anyone knew why they were different and that Population II came before Population I.

The numbering makes sense to me. You know you can see the brightest stars, and who the heck knows how many classifications you're going to want for the stars you can't see yet.
 
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  • #355
phinds said:
@Devin-M are we supposed to guess what those are?
test.jpg
Here's what it would look like through a 2000mm telescope in Stellarium:
Screen Shot 2022-07-29 at 10.38.32 AM.png

RA 11h06m18.79s Dec -77º22'50.9"

James Webb NIRCam:
test_00002-jpg.jpg


100% Crop:
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  • #356
Office_Shredder said:
The numbering makes sense to me. You know you can see the brightest stars, and who the heck knows how many classifications you're going to want for the stars you can't see yet.
When it was just a numbering classification, it made perfect sense, which is why Hipparchus defined it that way. But later, when quantitative measurements of brightness arrived, we turned it into a quantitative magnitude scale for measuring brightness. After doing that, we really would rather have a brighter object have a larger magnitude. But that would mean re-defining the scale. So today, the faintest objects we can see with our eyes are m=6.0, the faintest objects seen in large telescopes are about m=30.0 and the sun is m=-26.
 
  • #357
RA 01:07:47.200 DEC -17:30:25.00
JWST NIRCam Bi-Color, F150W & F200W Filters, 2319s exp per filter
Processed w/ SiriL, Adobe Photoshop & Lightroom
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  • #358
RA 2:17:46 DEC -05:16:15
JWST NIRCam 7-29-22 12:04
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  • #359
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  • #360
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