Follow Slashdot blog updates by subscribing to our blog RSS feed

 



Forgot your password?
typodupeerror
×
NASA Space

James Webb Space Telescope: Sun Shield Fully Deployed (bbc.com) 124

"On Tuesday morning, all five layers of the James Webb Space Telescope were fully locked into place," writes Slashdot reader quonset. The BBC reports: There were many who doubted the wisdom of a design that included so many motors, gears, pulleys and cables. But years of testing on full-scale and sub-scale models paid dividends as controllers first separated the shield's different layers and then tensioned them. The fifth and final membrane was locked into place at 16:58 GMT. "The unfurling and securing of the sun shield is part of what NASA refers to as '29 days on the edge,' writes quonset, citing an article from CNN. "During the 29 days, Webb will set up shop, unfurling its giant gold mirror and the protective tennis court-size sunshield. This process involves thousands of parts that must function harmoniously, in the right sequence. Fortunately, each step can be controlled from the ground in case there are issues."

"The next step is the unboxing of the mirror which had to be folded to fit inside the nose cone of the rocket for launch. If all goes well, by the end of the weekend, the mirror will be in place and ready for testing before full operations begin."
This discussion has been archived. No new comments can be posted.

James Webb Space Telescope: Sun Shield Fully Deployed

Comments Filter:
  • It'd be cool to actually see all this happen.

    • A telescope that can't see itself... a lot more ironic than a black fly in your chardonnay!
      • It's a reflecting telescope, all it can see is itself once the reflector's boom is deployed. Then it has to chill out near absolute zero to become invisible to itself.
    • Go outside and hold up a mirror. Let NASA show how good the JWST really is.
    • by necro81 ( 917438 )
      I had similar thoughts as the deployment began. Why does this amazing object - the most advanced telescope ever put into orbit, with the most complicated deployment of any satellite ever - not have a self-cam to show itself to the world. It can't be because of the cost! But after a few minutes' thought, I came up with several (probable) reasons why not:
      • * We may consider a small image sensor, suitable for this kind of selfie work, to be commonplace today. We see them on the recent Mars and lunar landers
      • The camera would have a weight, which would increase the telescope's propellant consumption and hence shorten its useful life. It also would need a heating device, with its own weight and energy budgets. The cam being at space specs would not be a tiny off the shelf phone one.

        It would also need a lighting device if on the far side since it is in the dark.

    • Actually the whereiswebb site used to just have animations of each deployment step, but for the sunshield they actually have timelapse video of the deployment. I presume this is either from ground testing or from their local model of Webb.

      https://webb.nasa.gov/content/... [nasa.gov]

  • by kot-begemot-uk ( 6104030 ) on Tuesday January 04, 2022 @05:09PM (#62143163) Homepage
    So why the shield does not act as a sun sail to blow it out of L2?
    • by hey! ( 33014 ) on Tuesday January 04, 2022 @05:18PM (#62143191) Homepage Journal

      Proposed solar sails have areas starting on the order of a square kilometer and going up -- that is to say starting at roughly 5000x the area Webb's sun shield.

      • by shanen ( 462549 )

        I suspect there is still some effect from the sun shield, but JWST has quite a bit of maneuvering capability, too. Far more than enough to offset any minor push from the sun shield.

        The thing that's worrying me is that JWST is going to be constantly pivoting to keep the shield facing the sun while the target is being tracked. That's going to take quite a bit of power for the pivoting and a lot of computational power to control the movements.

        Still, I think it's a great project and I'm keeping my fingers cross

        • by hey! ( 33014 )

          Given the precision of the instrument, there's bound to be all kinds of crazy things they had to make provision for. From what I've heard the success of their initial launch has left them with some healthy fuel margins to complete and probably extend the planned lifespan of the mission. It's still a hell of a nailbiter though.

          I don't think the poster's question was silly by any means, and I'm sorry if I gave that impression. There's no reason for anyone to have that information at their fingerprints, and

          • by shanen ( 462549 )

            Mostly concurrence, though your use of "fingerprints" for "fingertips" makes me wonder about your first language. Also, the reference for your "nailbiter" is a bit unclear, but I think you mean the initial assembly and deployment. However, now I think we were both pretty far off the mark.

            The gravitationally interesting thing about each Lagrange point is that objects tend to stay there. I'm hoping one of the other replies includes the math, but my "mental envelope" calculation indicates that the force needed

        • by clovis ( 4684 ) on Tuesday January 04, 2022 @06:35PM (#62143385)

          The Webb telescope, like the ISS, Hubble, and others use gyroscopes for pointing alignment.
          When the gyroscopes get to their max deflection and need to have their alignment reset, that's when the thrusters are used.

          https://en.wikipedia.org/wiki/... [wikipedia.org]

          • This page says JWST uses reaction wheels [wikipedia.org], not control moment gyroscopes [wikipedia.org]:

            https://jwst-docs.stsci.edu/jw... [stsci.edu]

            • by clovis ( 4684 )

              This page says JWST uses reaction wheels [wikipedia.org], not control moment gyroscopes [wikipedia.org]:

              https://jwst-docs.stsci.edu/jw... [stsci.edu]

              Ahhh, you're right. Reaction wheels are doing the work.
              I saw articles mentioned that gryoscopes were used for pointing and made an unwarranted assumption. It appears that the gyroscopes on the Webb are the wine glass kind for monitoring position and alignment, but they don't provide angular momentum or movement force. They're not massive control moment gyroscopes for physical movement like the ISS has.

              So, I rewite my post:
              The Webb telescope, like the ISS, Hubble, and others use reaction wheels for pointing

              • by shanen ( 462549 )

                Thanks for the additional data, but my focus was actually on the complexity of the aiming here, though the math is over my head. However, now that I think about it, maybe the math isn't so bad after all? There are two main factors they need to correct for, but they are linked fairly intimately. As the earth moves in its orbit, the angle to the sun is constantly shifting, and the sun shield of the JWST has to compensate for that continuous movement (and without fail, ever). On the other side, if the image in

        • JWST has only a small margin for tilting its sunshield out of the direct-sun-facing plane. It is able to effectively observe a relatively narrow annulus (by rotating about the radial vector), which annulus sweeps out the whole sky over the course of a year.

          There is no price to pay for having the telescope rotate once per year in principle (as any angular orientation is equivalent in empty flat space); In reality, differential radiation pressure and buffeting by solar winds mean that the craft will have t
          • Also, L2 is unstable in "distance to Sun" so there's bound to be some maneuvering to compensate for that.

            • by shanen ( 462549 )

              Thanks again, though now I'm wondering why the distance to the sun will be of concern. Especially if the "exposure times" are short.

              • The Sun-Earth line sweeps the trajectory plan of Earth.
                Objects approximately in L2 will "slow down" or "accelerate" to stay on that line (initial positioning is not perfect, and there are small influences from Moon, Jupiter, ...)
                Unfortunately, we have objects that are not exactly in L2 (or that are influenced away, see lunar influence). And when they start going, they will go faster and faster.
                And once far enough away from L2, the influence that keeps them "locked" into the Earth-Sun line will vanish, and t

        • "JWST is going to be constantly pivoting to keep the shield facing the sun while the target is being tracked."
          Assuming JWST has a "stable" orientation due to Sun gravity, it will make a 360 degrees turn in a year. To compensate for an effect of this magnitude, some small gyroscopes should be enough.
          And this is a problem solved for the Hubble (keeping the same orientation for long exposures) in Earth orbit.
          And, if the sun shield is "the size of a tennis court" (22 by 10 meters), the JWST's mirror of 6.5 mete

          • by shanen ( 462549 )

            Thanks, though a bit unclear. Some of the other replies went into much more detail about the reaction wheels.

        • The thing that's worrying me is that JWST is going to be constantly pivoting to keep the shield facing the sun while the target is being tracked. That's going to take quite a bit of power for the pivoting and a lot of computational power to control the movements..

          JWST will use a gyroscopic system to provide rotational control the same way other satellites do, and not use any fuel too keep the sun shield on the right side. This only uses tiny amounts of fuel to correct for accumulated variations. Adjusting the sunshield will use less power than rotating the much heavier telescope between targets at the end of each observation session. Hopefully the energy storage systems have been sized correctly so this won't be a problem.

          Out at the earth-sun L2 there's no asmospher

          • by shanen ( 462549 )

            Again, basic concurrence and it mostly meshes with the other replies.

            But of course I've thought of new things to worry about... Micrometeorites... Now I'm hoping they have lots of spare cameras that they can swap in as needed... I'll continue with the crossed fingers.

      • by CaptainLugnuts ( 2594663 ) on Tuesday January 04, 2022 @05:37PM (#62143239)
        They explained the orbital mechanics a long time ago.

        Simply put, they always want to be on the "uphill" side of L2. Webb can only thrust uphill, never downhill. It's designed to always fall back towards the Sun with occasional thrust boosts to get it back to close to the top of the hill. The solar pressure just slows the return fall, saving fuel.

    • by Papaspud ( 2562773 ) on Tuesday January 04, 2022 @05:18PM (#62143193)
      it is in the shadow of the Earth, AKA lagrange 2. And it would really need to be much bigger.
      • by ljw1004 ( 764174 ) on Tuesday January 04, 2022 @05:26PM (#62143213)

        Itâ(TM)s deliberately NOT in the earthâ(TM)s shadow. It orbits L2 about 1.5 million km from L2 perpendicular to the plane of the ecliptic. Itâ(TM)s either a âoeLissajousâ orbit or a âoeHaloâ orbit; I didnâ(TM)t understand which. The shadow of earth and moon is never larger than about 1.3 million km around L2.

        The reason is to never be in shade, and to have uniform constant sun/heat all the time. This allows for smaller batteries that donâ(TM)t have to spend lots of energy maintaining heat during an eclipse, and are always operating at a good temperature for them, and more controlled thermals for the entire satellite. The hot side is 85 Celsius, the bus is 30 Celsius, the observing side is 30 Kelvin, and there are a load of mini heaters on the observing side to keep individual electronic components warm enough to operate.

        • by ljw1004 ( 764174 )

          Itâ(TM)s deliberately NOT in the earthâ(TM)s shadow.

          Ugh. I'm sorry for the unicode. I recently switched to Apple's keyboard on my iPhone, which I guess uses something other than ASCII for its apostrophes. Ugh.

          • by Pascoea ( 968200 )
            Would you ever thought you'd have to apologize on a nerd site for trying to use a technology that just passed it's 30-year anniversary of being codified and is still not supported?
          • by MachineShedFred ( 621896 ) on Tuesday January 04, 2022 @06:40PM (#62143395) Journal

            Turn off "smart quotes" to stop that. It's pretty clear that Slashdot will never fix their unicode failings. it's been shit for years.

            • Here is a test. I turned off a feature called "smart punctuation". Let's see if it worked...

              • It did. Congrats, you can now make readable posts on this antiquated site!

                • The antiquated nature of this site is one of the things I love so much about it. I browse slashdot with 100% script blocking. It renders correctly and is fast as hell compared to almost anything else. With that said, FFS support unicode slashdot.

            • by clovis ( 4684 )

              Turn off "smart quotes" to stop that. It's pretty clear that Slashdot will never fix their unicode failings. it's been shit for years.

              Slashdot's no unicode policy has spared us from scrolling past pages of swastikas made with unicode swastikas, smiley faces, and the goatse character, Sinhala Letter Oyanna.

              • Instead we scroll past all that shit made in other ways that don't involve Unicode and still aren't filtered out, and end up with unreadable posts from people using Apple devices that work with literally every other website on the planet.

                I'd rather have more non-broken posts from legit users.

        • That all sounds correct. Also, even if JWST were at the exact L2 point, it would still receive about 18% of sunlight (solar radiation).

          This is because the Earth only partially eclipses the Sun when viewed from L2, with the remaining sunlight forming a ring around the Earth.

        • by idji ( 984038 )
          Another reason for the halo orbit is that radio communications from Earth are not coming from the direction of the Sun, so there is less noise in the signal. The angle between Earth and the Sun from Webb is about 0.256 degrees, given a Halo orbit radius of 670,000 km.
      • Jame's Webb is 1.5e6 Km from the Earth, that's still about 1 au.

        The Sun's angular diameter is (2*arcsin(diameter of the Sun / (2 * 1 AU))) which is 0.53 degrees. The Earth's angular diameter is (2*arcsin(diameter of the Earth/ (2 * 1.5e6 Km))) which is 0.48 degrees. You actually can't be in a true eclipse although you could blot out 82% of the Sun in the right spot. But even if you wanted to blot out the Sun with the Earth, the L2 point is not stable and the Moon, Mars, and Jupiter push any objects around a
    • by gweihir ( 88907 )

      Propellant. Also the pressure of the sun on this sail is minuscule. And L2 is not perfect, so you can position it a bit out of the perfect spot to counter that pressure if needed. No idea whether they need to even do that.

    • by voxelman ( 236068 ) on Tuesday January 04, 2022 @05:23PM (#62143211)

      From the JWST user documentation:

      While orbits about the L2 point are inherently unstable, the orbit size is large and the orbital velocity is low (~1 km/s), so the orbit "decays" slowly. However, JWST's large sun shield, roughly the size of a tennis court, is subject to significant solar radiation pressure which results in both a force and a torque. The direction of solar force varies as the observatory's attitude changes from observation to observation. The solar torque is balanced by reaction wheels, but periodically, the accumulated momentum is dumped by firing thrusters. Because JWST operations are event-driven, the observatory attitude profile and momentum dumping cannot be accurately predicted months in advance. These two perturbations increase the acceleration of JWST from its orbit about L2, and necessitates more frequent orbit maintenance (station keeping) maneuvers than other Lagrange orbit missions (which are typically 3–4 times per year).

      Thus, for station keeping JWST uses thrusters, while maintaining relative sun-pointing requirements, as follows:

      Orbit perturbations along the Sun-L2 axis have the greatest impact on-orbit stability. Thrusters are mounted on the spacecraft bus on the side of the sun shield facing the Sun; those used for orbit correction are oriented as far away from the sun shield as possible, and the sun shield can support a larger sun-pitch angle1 for orbit correction than is allowed for science operations. This architecture allows thruster firing at angles up to 90 from the Sun consistent with Sun avoidance restrictions, which is sufficient to provide orbit correction in all cases.

      For momentum management, JWST suffers from massive momentum buildup, as suggested in the question, described here.

      During science observations, the observatory will be pointed at a target, in an orientation at which the sun shield center of pressure is not aligned with the observatory center of mass. As solar photons hit the large sun shield, they place a torque on the observatory as a whole. The attitude control subystem (ACS) counteracts this torque by appropriately changing the spin rate on the reaction wheels, with the consequence that angular momentum accumulates in the reaction wheels. Momentum accumulation depends on the solar pitch angle, the roll orientation of the telescope, and the visit duration at a particular pointing position. The angular momentum (spin rate) of the reaction wheels must be managed to be kept within operational limits.

      Mission planners are creative in using a technique for momentum management that is passive:

      Momentum changes can be managed at some level by the way a sequence of observations is planned; this is done by observing at an orientation that builds momentum in a particular reaction wheel, followed by an observation at an orientation that removes momentum from that wheel.

      But, not always, as some need-based science require a quicker slew and orientation which overrides the above momentum management program, and hence "momentum dumping" is performed by unloading the wheels as required.

      However, managing momentum is only one of a number of planning constraints. At some point, one or more wheels will need to be adjusted to stay within operational bounds. The planning and scheduling system inserts planned momentum unloads into the schedule as needed, based on the modeling of expected momentum buildup, currently expected to be 1–2 times per week. Each unload activity takes a few hours, in which the observatory slews to a particular orientation to minimize the impact on the orbit and then fires thrusters as needed to allow the spin rate of the reaction wheels to be adjusted.

      The orbit will be biased to compensate for mean outward forces associated with gravitation of the planets and radiation pressure on the sun shield.

      Above quoted passages are all from the PDF JWST Cycle 1 Documentation for Telescope and Spacecraft found on this page

    • So why the shield does not act as a sun sail to blow it out of L2?

      Engineers thought of this problem and designed a counter for it. There is a piece that sticks out at an angle and provides a counter force to balance out the solar sail effect.

    • So why the shield does not act as a sun sail to blow it out of L2?

      It does! The problem is actually that it torques the craft around, not that it pushes the craft back.

      There is a comparatively small flap of shield at the aft end of the spacecraft, which torques the craft in the opposite direction of the torque produced by the main shield. I'm not sure how the mechanics of that work, I believe that it was explained in either a Scott Manley video or a Marcus House video.

    • See
      https://solarsystem.nasa.gov/r... [nasa.gov]
      for more details.
      JWST goes to L2 ("behind" Earth) and it will keep Earth, Moon and Sun behind its single "sun shade". This keeps it close enough to Earth, at 5 light-seconds away - Moon is at 1.3 light seconds.
      Not to mention that the mind enslaving effect of 5G, 6G, mmWave towers is reduced at L2. Also, people on Earth won't be able to use high power lasers to "blind" it (like they do to airplanes).
      JWST will only make observations "away" from the Sun. Fortunately, Earth r

  • Current Status (Score:5, Informative)

    by backslashdot ( 95548 ) on Tuesday January 04, 2022 @05:18PM (#62143195)

    This page shows the telescopeâ(TM)s current status and what it looks like. https://www.jwst.nasa.gov/cont... [nasa.gov] It looks like the side mirrors have to unfold and the secondary mirror struts have to move into place too.

  • Is the future of space telescopes (or any, actually) a large number of small telescopes deployed into space and then aimed at the same spot and their images stacked together (think of each of JWSTs hexagon mirrors free floating in space as an array of independent telescopes?) Or is it massive telescopes as one structure (like JWST?) I think it is the former. I have seen what great images image stacking can produce using a small telescope on Earth even though it has to deal with the Earthâ(TM)s rotation

    • Webb's sensitivity is (iirc) down to a handful of photons/sec.

      At some point you want all the photons you can muster to hit the same detector to get readings above the noise floor. If you can make quiet enough detectors then stacking will work fine too.

      • Ok but isnâ(TM)t that a function of probability that can be accounted for by deploying a larger number of small telescopes? Hopefully not an insanely larger number though. Like, say the JWST requires 18 mirrors segments. Maybe the same image can be had with 24 telescopes each having a mirror the same size as a JWST mirror segment. That would reduce the risk and also allow some observations of different areas of the sky when the full array is not needed to point at the same area. Also the chance of mis

        • Almost.

          Let's say you have one photon/pixel/sec equivalent noise (made up numbers) it gets really hard to pull signal out if you've got fewer photons/sec coming in. Large mirrors increase the signal to noise ratio which helps you discern if your measurement is real or a processing artifact.

        • Ok but isnÃ(TM)t that a function of probability that can be accounted for by deploying a larger number of small telescopes?

          Unfortunately no, not for optical telescopes.

          The reason is that the resolution (as in resolving power, how many degrees apart can you separate point sources) of the image is in proportion to the size of the mirror. This is because broadly speaking, waves passing through a gap (or bouncing off a mirror) diffract and so spread out, and the larger the mirror, the smaller the diffracti

    • Stacking is a way to simulate a longer exposure time. This is what is already done with Hubble, for example. Some of the well known Hubble images are made of hundreds of exposures because each individual exposure is limited in time. If there were twenty Hubbles all operating at once... Yes, you could in theory make the same image in less time but it's not necessarily worth the money investment. It would be very expensive, and the size of the optics would still limit the resolution to what the Hubble can do.

    • by ceoyoyo ( 59147 )

      You don't use multiple space telescopes for that. You integrate images over time. That's what Hubble's deep fields are.

      The point of having multiple telescopes is to spread them out and do interferometry. We'll be doing that with radio space telescopes soon, but it's much more difficult at higher frequencies, so it's unlikely we'll be doing it in space for another generation or two.

    • Different wavelengths of light require different systems. Large numbers of independent telescopes work better for very-long-baseline interferometry observations which works best on longer wavelength observations. The Event Horizon Telescope for instance is kinda like this with massive ratio observatories but it's limited in resolution due to the size of the Earth. If we want a higher resolution image of black holes, we're going to need to place these near lunar orbits or interplanetary space.

      Shorter wavelen
  • Super yikes. Excited. Tingly.
  • I thought the earth would be its sun-shield, did I miss something?

    • by necro81 ( 917438 )

      I thought the earth would be its sun-shield, did I miss something?

      Yes, only the last 20 years of design, a dozen Slashdot articles over the years, and the last few weeks of intensive press coverage. There is AMPLE material out there on why JWST has a sunshield, why it is not in Earth orbit, and the complicated deployment after launch. Snark in a Slashdot forum is not the way to get an answer to your question

      To quote Shawshank: How can you be so obtuse...is it deliberate?

      • "How can you be so obtuse...is it deliberate?"

        You can't possibly expect us to RTFA.

      • by kackle ( 910159 )
        His question didn't strike me as snarky, merely uninformed (hence the question). Perhaps it's a language/cultural difference.

        Your response, on the other hand...

Surprise your boss. Get to work on time.

Working...