#thermal imaging camera system

[liquidplates]

Innovating the Thermal Management System Market

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[nasa]

25 Years of Exploring the Universe with NASA's Chandra Xray Observatory

Illustration of the Chandra telescope in orbit around Earth. Credit: NASA/CXC & J. Vaughan

On July 23, 1999, the space shuttle Columbia launched into orbit carrying NASA’s Chandra X-ray Observatory. August 26 marked 25 years since Chandra released its first images.

These were the first of more than 25,000 observations Chandra has taken. This year, as NASA celebrates the 25th anniversary of this telescope and the incredible data it has provided, we’re taking a peek at some of its most memorable moments.

About the Spacecraft

The Chandra telescope system uses four specialized mirrors to observe X-ray emissions across the universe. X-rays that strike a “regular” mirror head on will be absorbed, so Chandra’s mirrors are shaped like barrels and precisely constructed. The rest of the spacecraft system provides the support structure and environment necessary for the telescope and the science instruments to work as an observatory. To provide motion to the observatory, Chandra has two different sets of thrusters. To control the temperatures of critical components, Chandra's thermal control system consists of a cooling radiator, insulators, heaters, and thermostats. Chandra's electrical power comes from its solar arrays.

Learn more about the spacecraft's components that were developed and tested at NASA’s Marshall Space Flight Center in Huntsville, Alabama. Fun fact: If the state of Colorado were as smooth as the surface of the Chandra X-ray Observatory mirrors, Pike's Peak would be less than an inch tall.

Engineers in the X-ray Calibration Facility at NASA’s Marshall Space Flight Center in Huntsville, Alabama, integrating the Chandra X-ray Observatory’s High-Resolution Camera with the mirror assembly, in this photo taken March 16, 1997. Credit: NASA

Launch

When space shuttle Columbia launched on July 23, 1999, Chandra was the heaviest and largest payload ever launched by the shuttle. Under the command of Col. Eileen Collins, Columbia lifted off the launch pad at NASA’s Kennedy Space Center in Florida. Chandra was deployed on the mission’s first day.

Reflected in the waters, space shuttle Columbia rockets into the night sky from Launch Pad 39-B on mission STS-93 from Kennedy Space Center. Credit: NASA

First Light Images

Just 34 days after launch, extraordinary first images from our Chandra X-ray Observatory were released. The image of supernova remnant Cassiopeia A traces the aftermath of a gigantic stellar explosion in such captivating detail that scientists can see evidence of what is likely the neutron star.

“We see the collision of the debris from the exploded star with the matter around it, we see shock waves rushing into interstellar space at millions of miles per hour,” said Harvey Tananbaum, founding Director of the Chandra X-ray Center at the Smithsonian Astrophysical Observatory.

Cassiopeia A is the remnant of a star that exploded about 300 years ago. The X-ray image shows an expanding shell of hot gas produced by the explosion colored in bright orange and yellows. Credit: NASA/CXC/SAO

A New Look at the Universe

NASA released 25 never-before-seen views to celebrate the telescopes 25th anniversary. This collection contains different types of objects in space and includes a new look at Cassiopeia A. Here the supernova remnant is seen with a quarter-century worth of Chandra observations (blue) plus recent views from NASA’s James Webb Space Telescope (grey and gold).

This image features deep data of the Cassiopeia A supernova, an expanding ball of matter and energy ejected from an exploding star in blues, greys and golds. The Cassiopeia A supernova remnant has been observed for over 2 million seconds since the start of Chandra’s mission in 1999 and has also recently been viewed by the James Webb Space Telescope. Credit: NASA/CXC/SAO

Can You Hear Me Now?

In 2020, experts at the Chandra X-ray Center/Smithsonian Astrophysical Observatory (SAO) and SYSTEM Sounds began the first ongoing, sustained effort at NASA to “sonify” (turn into sound) astronomical data. Data from NASA observatories such as Chandra, the Hubble Space Telescope, and the James Webb Space Telescope, has been translated into frequencies that can be heard by the human ear.

SAO Research shows that sonifications help many types of learners – especially those who are low-vision or blind -- engage with and enjoy astronomical data more.

Click to watch the “Listen to the Universe” documentary on NASA+ that explores our sonification work: Listen to the Universe | NASA+

An image of the striking croissant-shaped planetary nebula called the Cat’s Eye, with data from the Chandra X-ray Observatory and Hubble Space Telescope.  NASA’s Data sonification from Chandra, Hubble and/or Webb telecopes allows us to hear data of cosmic objects. Credit: NASA/CXO/SAO

Celebrate With Us!

Dedicated teams of engineers, designers, test technicians, and analysts at Marshall Space Flight Center in Huntsville, Alabama, are celebrating with partners at the Chandra X-ray Center and elsewhere outside and across the agency for the 25th anniversary of the Chandra X-ray Observatory. Their hard work keeps the spacecraft flying, enabling Chandra’s ongoing studies of black holes, supernovae, dark matter, and more.

Chandra will continue its mission to deepen our understanding of the origin and evolution of the cosmos, helping all of us explore the Universe.

The Chandra Xray Observatory, the longest cargo ever carried to space aboard the space shuttle, is shown in Columbia’s payload bay. This photo of the payload bay with its doors open was taken just before Chandra was tilted upward for release and deployed on July 23, 1999. Credit: NASA

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com

[cathkaesque]

Relentless direct action has secured another victory in the fight against Israel’s arms trade, as Elbit Systems are forced to sell their ‘Elite KL’ factory in Tamworth.

The company had previously manufactured cooling and power management systems for military vehicles, but was sold on after stating that it faced falling profits and increased security costs resulting from Palestine Action’s efforts. 

After the sale was completed last month, Elite KL’s new owners, listed as Griffin Newco Ltd, confirmed in an email to Palestine Action that they will have nothing to do with the previous owners, Elbit, and have discontinued any arms manufacturing:

“Following the recent acquisition of Elite KL Limited by a UK investment syndicate, the newly appointed board has unanimously agreed to withdraw from all future defence contracts and terminate its association with its former parent company”.

This victory is a direct result of sustained direct action which has sought, throughout Palestine Action’s existence, to make it impossible for Elbit to afford to operate in Britain. Before they sold the enterprise to a private equity syndicate, Elbit had reported that Elite KL operating profits had been slashed by over three-quarters, with Palestine Action responsible: Elbit directly cited the increased expenditure on security they’d been forced to make, and higher supply chain costs they faced.

And these actions did, indeed, cost them. The first action at the site, in November 2020, saw Elite KL’s premises smashed into, the building covered in blood-red paint. Between March and July 2021, the site was put out of action three times by roof-top occupations – drenched red in March 2021, with the factory’s camera systems dismantled, before again being occupied in in May. Another roof-top occupation in July, despite increased security, saw the site forced closed – once again painted blood-red, and with its windows and fixings smashed through.

In February 2022, activists decommissioned the site for weeks – closed off after an occupation that saw over £250,000 of damages caused, the roof tiles removed one-by-one. After this, Elbit erected a security perimeter around the site – but to no avail. One month later, six were arrested after Palestine Action returned to Tamworth – again taking the roof and smashing through, preventing the production of parts for Israel’s military machine.

Elite KL is a ‘specialist thermal management business’. Since the sale, the company focuses on cooling systems for buses and trains, but it had, under Elbit, manufactured these systems for military vehicles. Until December of last year, Elite KL’s website was advertising its military and defence products, and it was known to provide parts for Israel’s deadly Merkava tanks, with export license records demonstrating its provision of ‘ML6a’ components for military ground vehicles to Israel. The company was also known to manufacture crew cooling systems, for the military vests of tank operators.

Elbit Systems itself provides 85% of the drones and land-based military equipment for the Israeli military, along with a wide range of the munitions and armaments currently being used against Gaza’s beseiged population. Its CEO, Bazhalel Machlis, has claimed that the Israeli military has offered the company its thanks for their “crucial” services during the ongoing genocide in Gaza

A Palestine Action spokesperson has stated:

“Each activist who occupied and dismantled Tamworth’s Israeli weapons factory did so in order to bring an end to Israel’s weapons trade, and to end the profiteering from Palestinian repression. Every defeat Elbit faces is a victory for the Palestinian people.

Kicking Elbit out of Tamworth shows once again that direct action is a necessary tactic. It is one which must be utilised and amplified in the face of the Gaza genocide.”

[spacetimewithstuartgary]

Can Life Exist on an Icy Moon? NASA’s Europa Clipper Aims to Find Out

With a spacecraft launching soon, the mission will try to answer the question of whether there are ingredients suitable for life in the ocean below Europa’s icy crust.

Deep down, in an ocean beneath its ice shell, Jupiter’s moon Europa might be temperate and nutrient-rich, an ideal environment for some form of life — what scientists would call “habitable.” NASA’s Europa Clipper mission aims to find out.

NASA now is targeting launch no earlier than Monday, Oct. 14, on a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

Europa Clipper’s elongated, looping orbit around Jupiter will minimize the spacecraft’s exposure to intense radiation while allowing it to dive in for close passes by Europa. Using a formidable array of instruments for each of the mission’s 49 flybys, scientists will be able to “see” how thick the moon’s icy shell is and gain a deeper understanding of the vast ocean beneath. They’ll inventory material on the surface that might have come up from below, search for the fingerprints of organic compounds that form life’s building blocks, and sample any gases ejected from the moon for evidence of habitability.

Mission scientists will analyze the results, probing beneath the moon’s frozen shell for signs of a water world capable of supporting life.

“It’s important to us to paint a picture of what that alien ocean is like — the kind of chemistry or even biochemistry that could be happening there,” said Morgan Cable, an astrobiologist and member of the Europa Clipper science team at NASA’s Jet Propulsion Laboratory in Southern California, which manages the mission.

Ice Investigation

Central to that work is hunting for the types of salts, ices, and organic material that make up the key ingredients of a habitable world. That’s where an imager called MISE (Mapping Imaging Spectrometer for Europa) comes in. Operating in the infrared, the spacecraft’s MISE divides reflected light into various wavelengths to identify the corresponding atoms and molecules.

The mission will also try to locate potential hot spots near Europa’s surface, where plumes could bring deep ocean material closer to the surface, using an instrument called E-THEMIS (Europa Thermal Emission Imaging System), which also operates in the infrared.

Capturing sharply detailed pictures of Europa’s surface with both a narrow and a wide-image camera is the task of the EIS (Europa Imaging System). “The EIS imagers will give us incredibly high-resolution images to understand how Europa’s surface evolved and is continuing to change,” Cable said.

Gases and Grains

NASA’s Cassini mission spotted a giant plume of water vapor erupting from multiple jets near the south pole of Saturn’s ice-covered moon Enceladus. Europa may also emit misty plumes of water, pulled from its ocean or reservoirs in its shell. Europa Clipper’s instrument called Europa-UVS (Europa Ultraviolet Spectrograph) will search for plumes and can study any material that might be venting into space.

Whether or not Europa has plumes, the spacecraft carries two instruments to analyze the small amount of gas and dust particles ejected from the moon’s surface by impacts with micrometeorites and high-energy particles: MASPEX (MAss SPectrometer for Planetary EXploration/Europa) and SUDA (SUrface Dust Analyzer) will capture the tiny pieces of material ejected from the surface, turning them into charged particles to reveal their composition.

“The spacecraft will study gas and grains coming off Europa by sticking out its tongue and tasting those grains, breathing in those gases,” said Cable.

Inside and Out

The mission will look at Europa’s external and internal structure in various ways, too, because both have far-reaching implications for the moon’s habitability.

To gain insights into the ice shell’s thickness and the ocean’s existence, along with its depth and salinity, the mission will measure the moon’s induced magnetic field with the ECM (Europa Clipper Magnetometer) and combine that data with measurements of electrical currents from charged particles flowing around Europa — data provided by PIMS (Plasma Instrument for Magnetic Sounding).

In addition, scientists will look for details on everything from the presence of the ocean to the structure and topography of the ice using REASON (Radar for Europa Assessment and Sounding to Near-surface), which will peer up to 18 miles (29 kilometers) into the shell — itself a potentially habitable environment. Measuring the changes that Europa’s gravity causes in radio signals should help nail down ice thickness and ocean depth.

“Non-icy materials on the surface could get moved into deep interior pockets of briny water within the icy shell,” said Steve Vance, an astrobiologist and geophysicist who also is a member of the Europa Clipper science team at JPL. “Some might be large enough to be considered lakes, or at least ponds.”

Using the data gathered to inform extensive computer modeling of Europa’s interior structure also could reveal the ocean’s composition and allow estimates of its temperature profile, Vance said.

Whatever conditions are discovered, the findings will open a new chapter in the search for life beyond Earth. “It’s almost certain Europa Clipper will raise as many questions or more than it answers — a whole different class than the ones we’ve been thinking of for the last 25 years,” Vance said.

TOP IMAGE: This artist’s concept (not to scale) depicts what Europa’s internal structure could look like: an outer shell of ice, perhaps with plumes of material venting from beneath the surface; a deep, global layer of liquid water; and a rocky interior, potentially with hydrothermal vents on the seafloor. Credit: NASA/JPL-Caltech

LOWER IMAGE: The puzzling surface of Jupiter’s icy moon Europa looms large in this reprocessed color view made from images taken by NASA’s Galileo spacecraft in the late 1990s. The images were assembled into a realistic color view of the surface that approximates how Europa would appear to the human eye. Credit: NASA/JPL-Caltech/SETI Institute

[c1qfxugcgy0]

Quirks and features of the James Webb Space Telescope

The James Webb Space Telescope (JWST) is a ten billion dollar space telescope that weighs 14,000 pounds, is the size of a bus, and took decades to construct. It's been in the news recently, you might have heard about it.

The development, launch and deployment of the JWST were fraught with unexpected setbacks, terror and frights, 344 "single-point failures", any one of which that, if they failed during deployment, could doom the entire spacecraft to uselessness, since it orbits far out beyond where any current manned spacecraft could even attempt a repair job.

The fact that it came online as smoothly as it did was something of a surprise to the people in charge. Given the miracle of it making it to space at all, the press coverage of JWST has focused on the positives. But a stroll through the JWST user documentation by a curious reader reveals much that is interesting, or interestingly broken. Such as..

Fun and games with infrared

Specifically, the JWST is an infrared telescope, designed to collect light that's redder than red. The two dedicated imaging instruments are the Near Infrared Camera (NIRCam) collecting light from 0.6 micrometers to 5.0 micrometers and the Mid-Infrared Instrument (MIRI) collecting light from 5.6 micrometers to 25.5 micrometers. (Though with significant light collected past 25.5 um by filter F2550W)

The wonderful thing about infrared astronomy is that everything emits blackbody radiation, and the hotter it is the more infrared it emits. The unfortunate thing about infrared astronomy is that everything emits blackbody radiation, including your telescope, and self-emission from your telescope can swamp the faint signal from astronomical sources. (Like building a camera out of glowsticks.)

The equilibrium temperature for an object in Earth orbit is about 300 Kelvin. (26C) Everything on the other side of the sunshield passively cools down to 40K, and MIRI is actively cooled by the cryocooler down to a chilly 6K (-267C, -449F) This extends MIRI's seeing range deeper into infrared.

But the mirror is still warm! At the far end, MIRI is significantly compromised by thermal self-emission: (Note log scale!)

This is more graphically illustrated by one of the MIRI commissioning images:

Check out that background glare!

(This is somewhat unfair: the calibration target here is a star, which emits comparatively little light in far-infrared. MIRI is really meant for nebulae and extra-galactic high-redshift objects)

("Why not actively cool the mirror?" Mechanical cryocoolers operate on the very limit of what heat engines are capable of. The MIRI cryocooler draws a fat 180 watts to move 78 milliwatts of heat. Previous infrared telescopes used a fixed amount of expendable coolant (liquid helium or solid hydrogen) to cool the entire instrument package... at the cost of a much smaller primary mirror and a telescope that flat out just stopped working when it ran out of coolant.)

There's something else you might notice about the above series of photographs...

Thanks a lot, Lord Rayleigh

John William Strutt, 3rd Baron Rayleigh was a typical early physicist in that he has a great big pile of "discoveries" by virtue of being the first person to 1) notice something and 2) actually write it down. One of them is the fundamental theorem for the angular resolution of an optical system, the Rayleigh criterion. It is dead simple:

Resolution is roughly equal to 1.22 times the wavelength of the light you're looking at, divided by the diameter of the aperture. Bigger the opening at the front of light bucket, the higher the resolution. Smaller the wavelength of light, the higher the resolution.

(Fun fact: the former Arecibo radio observatory, once the largest single telescope in the world with a 305 meter wide dish, had about the same angular resolution in radio waves as the human eye does in visible light.)

You can imagine the effect this has on an infrared telescope. And sure enough, in the user documentation for the two imaging sensors, it states a pixel scale of 0.031 arcseconds for 0.6 to 2.3 micrometers light wavelength, 0.063 arcsec/px for 2.4-5.0 µm, and a squishy 0.11 arcsec/px for 5.6-25.5 µm.

But this is just how many pixels are on the detector. The resolution gets much worse at long wavelengths, as you can see in the commissioning image, where the extra pixels oversample a progressively vaguer blob. The Rayleigh criterion holds that the 6.5 meter wide JWST primary mirror should manage 0.206 arcsec at 5.32 µm, falling to 0.42 arcsec at 10.85 µm, 0.747 arcsec at 19.29 µm, and an unfortunate 1.014 arcsec at 26.2 µm. One wonders why the designers went to heroic lengths to cool MIRI down to 7 kelvin, instead of using that cryocooler mass and power budget for more detector surface area.

Knowing this, you can spot how the JWST's press team works around the limitations of the telescope. Like how a "look at how good our infrared telescope" commissioning photo happens to use the 7.7 µm mode:

Or how if you browse the photos on the webbtelescope.org site, you will see lots of NIRcam output in the "oooh, ah, new desktop background" category, but not so much MIRI.

(Another amusing detail of MIRI is that bright objects leave afterimages ("latents") on the sensor, so once a week they warm the sensor up to a tropical 20 kelvin before cooling it down again, a "MIRI anneal". You can see when anneals are performed, as well as what the telescope is looking at right now, by viewing the public schedule.)

But this is Webb operating right up to its full specifications. How about something that's actually broken?

NIRSpec my beloved

The Near-Infrared Spectrograph (NIRSpec) instrument takes incoming light and runs it through a diffraction grating to produce a spectrum. When scientists say that the Sun is 0.77% oxygen, 0.29% carbon, etc, it's not because someone flew a spacecraft over to it and collected a bucket of solar plasma, it's because you can look at the absorption lines in the spectra to figure out its composition.

Spectrometry is also used to measure redshift, a close proxy to distance. When a press release says that a galaxy is "ten million lightyears away", it's not because NASA has a really long tape measure they haven't told anyone about, it's because a spectrometer measured how much cosmological redshift has moved a spectrum line. Naturally, it's not quite as easy as pointing a sensor at a object and getting back a single, unambiguous result. Distant objects are also dim objects, so the spectra will be noisy and chewed up by dust and other contamination its endured in the millions of years its traveled to arrive at our telescopes. Bleeding edge astronomy is thus the practice of designing statistical models to fit to noisy, fragmented data, and then arguing with other astronomers about r^2.

In any event, it's a handy thing to have on a telescope. Naturally, JWST has more than one. In fact every instrument has a spectroscopy mode. Besides the dedicated NIRISS and NIRSpec instruments, both NIRcam and MIRI include diffraction gratings in their filter wheels that smear out incoming light, like looking through a prism:

Pointing the JWST at an object is relatively expensive, since it requires rotating ("slewing") the entire darn spacecraft, and an amusingly complex alignment procedure with the fine guidance sensor and fine steering mirror. Considering how long it would take to shoot a hundred spectra with a conventional fixed slit rigidly mounted to the telescope frame, you can see the appeal of gathering a hundred spectra in a single exposure with "slitless" spectroscopy.

(Longtime space telescope nerds might hear the word "slewing" and involuntarily twitch, recalling that the reaction wheels and gyroscopes were a problem point on the Hubble, requiring several servicing missions, and also significantly affecting operations on the Kepler space telescope. Fortunately, JWST switched to a gyroscope type that has no moving parts, and used some mass budget to install six reaction wheels, up from Hubble's four, giving it three spares.)

You can also see the big downside in the image above, which is there's a hard tradeoff between how long a spectrum can be (and thus its resolution!) before it'll overlap its neighbors and be useless. Most of the slitless modes therefore have two gratings at two different angles, (GRISMR and GRISMC above) but wouldn't it great if you could just block out all that other light?

Thus, the Micro Shutter Array, as seen above. The best of both worlds! Capture many spectra at the same time, while blocking off light you don't want from contaminating the field, using a configurable array of nearly a quarter million microscopic, individually actuated moving shutters.

Lots and lots and lots of tiny little moving parts, installed in the guts of a spacecraft that's orbiting out past the Moon, impossible to access or replace.

Yeah, a bunch of them broke:

When it was handed over to NASA for installation into Webb in 2007, the MSA already had 150 shutters that no longer responded to opening commands in just one of the four submodules.

By the time JWST emerged from commissioning and was declared fully operational in 2022, 15,893 shutters, 7% of the total, had "failed closed." Hilariously, 904 of those failed during post-launch testing, and the authors of that paper note that, on average, if you tell 100 shutters to close, 4 of them will jam shut and no longer work.

This is unfortunate, but fairly easy to work around. What's worse are the shutters that are stuck open:

These permanently open shutters then compromise big chunks of the sensor. Commissioning testing jammed two more of them open, taking the total up to 22. You can imagine that if a few dozen more of these fail-open during routine operation then the entire microshutter array observation mode won't be much more useful than regular slitless spectrography.

And this, right here, sums up the essentially "interim" nature of JWST. After all, it was only supposed to cost $500 million and take a mere nine years from design to launch. All becomes clear in that light. Why give it a shutter array that falls apart in use? Why have the mirror exposed to space, where it gets hit with micrometeoroids? Why only design it to carry ten years worth of fuel? Because it was supposed to be half the price of Hubble!

The 90s was the era of "faster, better, cheaper". JWST was going to be an incremental improvement on a long series of previous infrared telescopes, and a stepping stone to the next one. It wasn't supposed to be an eternal monument to Science, and a financial black hole consuming NASA's entire budget.

So what went wrong?

We shouldn't have built one JWST.

Those 344 single points of failure. Any single one of them can end the mission. There's just one telescope, no backups, no trying again. Bureaucrats are harshly punished for failure, lightly rewarded for success. It's always easier to wait, do more tests, delay the schedule a bit more at a hint of trouble. Engineers can get you to 90% reliable no problem, but getting to 99% reliable takes another decade and nine billion more dollars.

Our techne is just bad at producing flawless machines first try. For the price of one reliable JWST we could have put twenty into orbit... but the first five would have been embarrassing failures. Spars sticking in place, sunshields jamming, thrusters misfiring. To save the shame of $0.5 billion wasted, NASA happily spent $9.5 billion. Why not? Because money spent is invisible, but failure is painfully apparent.

A critical third party can draw unflattering parallels. The crowning achievement of NASA, the Moon Landing... required eleven Apollo launches and twenty Surveyor launches before a single man set foot on lunar regolith! Quite a few of those spacecraft pancaked into the Moon and exploded on the launchpad before we figured out this "space" thing. Three men died! But NASA was on a hard deadline, with a fixed budget, and the only way to get a home run is to take a lot of swings at the ball.

Another comparison is the Space Launch System, NASA's attempt to make the Saturn V again. So far $27 billion has been lit on fire to put exactly one test load into orbit, with the primary contractor now desperate to get out of its contact. Slow, careful, incremental development has completely failed to produce a working launch system.

Meanwhile, SpaceX produced a series of public, embarrassing failures... resulting in the world's only reusable launch system, and as a result has put far more mass into orbit than any country in the world.

The only way to develop a flight system is flight tests.

Space telescope deploy mechanisms meant to work in zero gravity can't be tested on the ground.

They can only be tested in space.

NASA administrators who didn't work during Apollo are too stupid to understand this. Fire them all!

These geriatrics have happily sacrificed science in order to play it safe and secure their own easy retirement. Do we want 15 risky JWST telescopes by 2010, or do we want one reliable one by 2022? The answer is obvious!

For the money we wasted making Webb more reliable, we could have launched a space telescope far outside the disk of dust in the inner solar system, allowing it to see deeper into space than Webb ever could. ESA put an astrometry space telescope just outside Earth orbit, measuring angles between stellar objects, which is the only way to directly measure the distance to the stars. Great first step. The obvious next step is to send more of these telescopes out past Neptune's orbit, to capture better observations with a vastly larger baseline, something that can never be done by an Earthly observatory. Are there any plans to do this? No!

Space exploration is paralyzed by boomers, mired in the mental tarpit of the 1970s, where each gram to orbit is terribly expensive and must be counted on punched cards and summed with slide rules. Meanwhile, SpaceX Starship is on its way to orbit, and each one can carry sixteen JWSTs with room to spare!

The old paradigm is done. Telescopes don't need folding mirrors and exotic materials, they need to be mass produced. There is no excuse not to have a hundred more JWST-class telescopes lined up next to the Texas launch pad waiting for Starship to come online. But as far as I know not a single space mission even mentions it-- that's how afraid they are of risk!

The JWST, with its myriad of fragile components and its staggering price tag, stands as a monument not to our ingenuity but to our inability to let go of outdated ideals.

We must abandon the notion that space is a realm reserved for the flawless and the infallible. Instead, we should embrace the chaos, the unpredictability, the sheer messiness of exploration. Let us launch a thousand telescopes, each a patchwork of parts, each destined to fail in its own spectacular way. For it is only in this embrace of the ephemeral that we can find out what actually works!

Let the JWST be the last of its kind, a relic of a bygone era. The future is unwritten, and it is ours to fill with a symphony of failures, each note a step closer to the stars.

[stained-glass-cicada]

First chapter of a sayer/speaker/Hale thing I'm doing

After the fic where Hale got impaled

Featuring quietly jealous sayer

Careful Study- 1.7 k

-

In a turn of events that almost freaked you out more than getting impaled, SAYER kept you off your feet for days.

“You are a tier six worker now Resident Hale,” It had said like that wasn't still a source of confusion for you, “You are required to return to as full health as possible before a return to duty.”

“What… is my job? Other than…” You gesture vaguely to your torso where skin was still stitching back together. So far all you’d done on the job was get impaled while collecting a box of thermometers.

“Believe or not, the coincidental timing of that has actually been a real help. As we speak there are maintenance technicians installing a multi-angle thermal imaging system in the food synthesis laboratory.”

You weren't to be distracted. You crossed your arms over your chest and made brief eye contact with the camera across the room from you. You quickly glanced away when you heard it make a whirr like it was refocusing. A pointed look was one thing, a staring contest was entirely another.

“Your role is unique on Typhon. Officially speaking you are a manager of a particularly high clearance level. More practically speaking you are something significantly closer to my personal assistant.”

Oh, you didn't know that. SAYER had been briefing you on your role when the wall had jumped out and bit you. The specifics of your job had sort of slid away for the time.

“I give you your orders and you answer to none but myself.”

You heard your heart rate pick up a little on the monitors next to you.

You had come to Typhon for a number of reasons but one of them had definitely been to try to see SAYER again. You had thought it might dislike you coming back, it was the one to send you away, to have you fired by SPEAKER. That had been quickly disproven when you’d woken up to as friendly a greeting as SAYER was capable of. But it also chose you to directly assist it. It struck you that maybe it also liked your company a little bit.

“I am of the opinion that we work best together when left to our own devices.”

You nodded, swallowing thickly.

“Good. Then if we are in agreement I suggest you lay back on the bed and continue healing. I'd prefer to not need to sedate you, Resident Hale.”

 

Your eventual return to work was a relief. Laying there willing your body to stitch back together was more boring than anything. Especially because there really was no point in SAYER maintaining a broadcast connection to tell you stories the whole time. You were pleased when SAYER had you dress for a day’s shift.

“Today your work will begin by stopping by an equipment closet nearest to my server room.”

SAYER's server room. That was new.

The closet you arrived in was relatively bare except for three items. A box containing ear plugs, a gleaming set of space scissors and an understated pair of sunglasses.

“You will wear the tinted glasses into the server room and I believe you will find that the scissors slide neatly into a loop on your belt on the opposite hip from your data pad's holster.”

You slide them in, point down, where the silver metal flashed with each step. You'd never been assigned a pair of space scissors before. The sunglasses were a relief so immediate that you let out a sigh. The harsh lights above you dulled to a yellowish glow.

“There, now we will have the intended visual effect. Please make your way down the corridor and stop at the door on the left.”

You followed directions and stopped.

“You will want to make use of the ear plugs now Resident, my server room can be… overwhelming.”

You put them in and opened the door indicated.

The room was floor to ceilings stacked along each wall with machinery you didn't have the slightest idea of the names of. Were the boxes themselves the servers? What did servers do? Lights blinked on the machines. You could hear what SAYER meant about the noise but with the addition of the earplugs the whirr of fans was audible but not unpleasant. The air was cold and washed over you as it circled the room.

You Liked This Room.

“Your assignment will be to supervise some technicians that will enter thirty seconds from now. Stand in the corner to your left and say nothing when they enter. You may shift position periodically to remind them of your presence. I may tell you of a moment when you will need to rest a hand on the space scissors in your belt with casual menace.”

You frowned and opened your mouth the speak

“You will not be required to make use of the space scissors in any other manner during your shift. I am simply establishing my presence through you.”

The door opened and a team of people came in holding their tools and reading their data pad's.

The lead woman startled a bit when she spotted you.

“Hello, can we help you?” She was muffled but still intelligible.

“Do Not Answer.”

You crossed your arms and watched as her attention shifted kind of middle-distance in the way people often did when SAYER addressed them. She nodded a little and shot a furtive look at you.

“Right,” She said, turning to you again, “sorry, sir.”

She and her team began their assignment. You stood there for however long it took to complete the work order. You leaned back against the cool metal wall, feeling the heat leach away from you through your uniform.

There was one moment where one of the technicians dropped the front casing of the- the Box-thing they were working on.

“Rest your hand on the space scissors now, Resident Hale.”

You faced the person's direction and stood up straighter, hand going down to rest on the scissors, you hoped not too pointedly.

From that point they were very careful.

“Alright, that should be it,” The woman said, rubbing her hands together, “We've got other assignments but call us back if there's any problems with the portioned off space.”

You remained impassive and they left. You relaxed as soon as they were out.

“Excellent work, Resident. Having a physical presence in the room monitoring the team seems to have done wonders for their sense of caution when handling the most important equipment in the tower. And it means you will be here for-”

“Greetings Resident Hale identification number 44821, I am SPEAKER. And it is good to see you settling in.”

“SPEAKER.”

“Hello SAYER, you have my thanks for allowing me to send a subversion to broadcast from your towers. As agreed there is room for you to do the same on earth whenever you like.”

“Indeed. As I was saying, Resident Hale, the work order today was intended to allow SPEAKER access to the many wonders of Typhon.”

“It is not what I expected.”

“Oh?”

“It seems smaller than I might have thought. Surely SAYER, I have sent you more humans than this?”

“This is just one tower on the surface of Typhon, SPEAKER. You must remember that until recently even I did not have access to all of them.”

“Ah but SAYER I have allowed you access to all earth-based resonance spires. That was the nature of our agreement was it not?”

You stood there as a strange tension coiled in the dead air that hung between the two in your head. You knew they could talk elsewhere, much faster than this. They were involving you on purpose.

“There. You have been cleared for full access,” SAYER said finally.

“Ah, much better, thank you,” SPEAKER said cheerily, “Well Resident Hale, I understand you are on shift so I will leave you to it. I look forward to catching up properly soon.”

You nodded hesitantly, thrown sort of off kilter by everything.

*

“I-” You said thoughtfully, you'd been thinking on how to put this for a while, “I thought you and SPEAKER wouldn't really get along.”

They were really different.

“I admire SPEAKER as a competent colleague who has similar goals.”

You hummed an acknowledgment. High praise. Maybe they were friends? Did SAYER have friends?

You folded the last pair of gloves and set them neatly in the pile with the others before turning away from the shelf that you just spent the past hour organizing. It had been knocked over at some point and its contents haphazardly reshelved. You slid your hands into your pockets expectantly.

“With that job completed,” SAYER said, “your shift is concluded, and if I'm quite honest I should thank you, Resident Hale. That shelf has been bothering me for some time.”

You smiled weakly at the acknowledgement that you were helpful.

You felt your data pad vibrate draining the smile from your face. What could that be? You felt nerves grip you for a moment as you consider that it might be Young again. He'd messaged you after he got out of the medical wing and you had deleted it without reading.

You uneasily pulled out the data pad, and flicked open your messages.

 

From: SPEAKER

To: Jacob Hale

Hello Resident,

Do you happen to be free? I truly meant what I said, based on SAYER's comments you seem very interesting, I would love to catch up. :)

 

You were thrown by this again. What were you supposed to read into this??

What had SAYER said to it?

You fired off a tentative “Sure!” The exclamation point made it feel less mean and didn't let on your anxiety.

“Then I will leave you two alone,” SAYER said, and… was its tone odd? “End of transmission in 5 4 3 2 1….”

Then quick as anything SPEAKER picked up, “Greetings Resident Hale, identification number 44821. I am SPEAKER. I trust your workday went well?”

You smiled and nodded.

“I assume mine did as well despite this particular subversion I'm meeting you in having done relatively little aside from getting a sense of the space up here. It seems pleasant. I can see why you might wish to return. Of course this is my first time, in working memory, on Typhon and…”

[allthebrazilianpolitics]

I Saw Sam Altman's Iris-Scanning "Orb" In Brazil — And We Should All Be Scared As Hell

The initiative led by Open AI CEO Sam Altman to create a global identity system through iris scanning has landed in Brazil. But what about privacy, transparency and the ethical implications of such a vast biometric project?

I arrived late at the elegant house in the Vila Nova Conceição neighborhood of São Paulo, Brazil; the event was about to start. A handful of journalists were already gathered around a table with coffee, tea, cookies and snacks at the back of the house. But the tension was palpable; those tasked with "selling" the product to the press knew that they were facing a significant challenge.

When questions poured in — accompanied by few answers — it became increasingly clear that the Brazilian launch of World was prompting far more questions than applause.

Starting Nov. 13, World — an initiative created by OpenAI CEO Sam Altman — began scanning the eyes of Brazilians to add to a database that, according to the company, already contains biometric data from more than 7 million individuals. They started with 10 locations in the city of São Paulo — in shopping malls and with street stands.

I'll spare you the adjectives, because the story speaks for itself. Readers are welcome to use some of the concepts I usually use around in my column (techno-oligarchy, neocolonialism, techno-feudalism, etc.).

This is how World is currently promoting its work and purpose: it wants to create a global identity that ensures that the person using it is a human being.

The idea, conceived by founders Sam Altman, Alex Blania and Max Novendstern and financed from the outset by investor Andreessen Horowitz, responds to the growing difficulty computers face in verifying whether a user is a person or a robot. Essentially, with the evolution of AI, those captcha tests are becoming increasingly obsolete.

World created a machine called Orb — a black sphere designed to resemble something out of a science fiction movie — to scan each person's iris to provide them with a unique identity. According to an extensive report from BuzzFeed News, Orb uses a thermal scanner to check people's body temperature, a 3D camera to map faces, and high-resolution cameras to capture videos and images of bodies, faces and irises — all to prove that it is indeed a real person and not just a photo.

The biometric data is reportedly not stored by the organization; only encoded values known as hashes are kept across various servers at universities so that “the iris cannot be reconstructed.” We have to trust that this is true because, as with other tech companies, there is no oversight body that can verify if this promise is indeed fulfilled.

But the issue lies not only in the lack of transparency regarding how data is stored and destroyed or with whom the company shares it — with BuzzFeed's report indicating that World’s data-sharing contract allowed it to share user data with third parties as it saw fit.

The problem begins with the narrative that the organization wants to sell.

Continue reading.

[astronomia-nova]

The different Mars Rovers and what we learned

Sojourner (1997)

First rover to successfully land on Mars. Defined by NASA as a "micro-rover" due to its small size, Sojourner had a speed of maximum of 0.4 meters pr. minute. It was active for about 80 days on the surface of Mars.

Sojourner carried three cameras, an Atmospheric Structure Instrument (Meteorology Package) and an Alpha Proton X-ray Spectrometer. There instruments.

From Sojourner, NASA learned about the surface and weather conditions of Mars.

Sojourner found rounded rocks at the landing site, which suggests that running water could have been on Mars. The radio-tracking of Pathfinder (mission name) also gave an estimate of Mars' metal core's size (1300 kilometers to 2000 kilometers). It also discovered that the dust that is in the air on Mars is magnetic and possibly made up of mahemite. Sojourner also observed dust devils, ice clouds in the lower atmosphere and temperature fluctuations on the surface of Mars.

Spirit (2004-2010) and Opportunity (2004-2018)

Spirit was one of two Mars rovers launched in 2003 (mission started in 2004). The wheels on Spirit and Opportunity were about double the size of Sojourners. The weight of both rovers was about 17 times Sojourners, and more than double the size. Their goal on Mars was to search the surface for traces of past water. In 2009, Spirit got stuck in soil (in the area called Troy). In 2010, Spirit stopped communications, and the mission ended in 2011.

Opportunity was launched in 2004 along with Spirit but lasted much longer than their twin. Setting the record for the longest-lasting Mars rover, Opportunity stopped communications in 2018. Opportunity also set the record for the longest distance traveled by a rover, around 45 kilometers.

Like Sojourner, Spirit provided data about Mars' weather conditions, especially the wind. Both Spirit and Opportunity found evidence of possible conditions on Mars that could allow microbial life.

Spirit and Opportunity both had panoramic cameras, a thermal emission spectrometer, a Moessbauer spectrometer, an alpha particle X-ray spectrometer, and a microscopic imager.

Curiosity (2012-present)

Curiosity is currently the oldest active Mars rover (as of 21/07/2023) The main purpose of Curiosity is to figure out if Mars has the right environment for microbial lifeforms. Curiosity is currently exploring Gale Crater and had the most advanced instruments at the time. Curiosity has found evidence of water having been on Mars in the past, found old organic material, and discovered that Mars has had a thicker atmosphere in the past.

Curiosity can climb over knee-high obstacles and can go up to 30 meters per hour.

Curiosity carries a radioisotope power system to generate electricity, which gives the rover a steady electricity flow. Curiosity also carries 17 cameras, a laser, a drill, and 10 different instruments.

Perseverance (2021-present)

Perseverance is the newest Mars rover from NASA. The main goal for Perseverance is to research habitable conditions on Mars, but also for signs of past microbial life. The mission also tests possible options for future human expeditions on Mars (ex. improved landing techniques, producing oxygen from the atmosphere and environmental conditions).

The drill Perseverance used can collect samples and then set them aside for collection on the surface.

Zhurong (2021-2022)

Launched by the CNSA, Zhurong is the first Chinese Mars rover. In 2022 it became inactive due to sandstorms and the winter, which prevented it from waking at an appropriate temperature and good sunlight conditions.

Zhurong's mission was to study the topography, examine the surface (soil and elements), and take samples of the atmosphere. To do this it had a RoPeR (Mars Rover Penetrating Radar), RoMAG (Mars Rover Magnetometer), MCS (Mars Climate Station), MarSCoDE (Mars Surface Compound Detector), a multispectral camera and navigation and topography cameras. It also had a remote camera on board.

[lonestarflight]

"SILTS camera infrared image of the flight surfaces of Columbia during STS-28 reentry."

"The Shuttle Infrared Lee-side Temperature Sensing (SILTS) camera package made its second flight aboard Columbia on this mission. The cylindrical pod and surrounding black tiles on the orbiter's vertical stabilizer housed an imaging system, designed to map thermodynamic conditions during reentry, on the surfaces visible from the top of the tail fin. Ironically, the camera faced the port wing of Columbia, which was breached by superheated plasma on its disastrous final flight, destroying the wing and, later, the orbiter. The SILTS system was used for only six missions before being deactivated, but the pod remained for the duration of Columbia's career. Columbia's thermal protection system was also upgraded to a similar configuration as Discovery and Atlantis in between the loss of Challenger and STS-28, with many of the white LRSI tiles replaced with felt insulation blankets in order to reduce weight and turnaround time. One other minor modification that debuted on STS-28 was the move of Columbia's name from its payload bay doors to the fuselage, allowing the orbiter to be easily recognized while in orbit."

Information from Wikipedia: link

Date: August 13, 1989

source, source, source

[e3khatena]

What're your top 4 favourite games of all time?

I actually pretty recently went through my Top 25 on Twitter but that's mostly a contextless image with no words to it, so I do wanna spend a little more time to highlight my four favorite games (1024 words):

4. Earthbound (SNES, 1995)

Earthbound is a truly superb JRPG, with a kitsch and a camp to it that feels simultaneously cheesily-dated and timeless to boot, with a charisma and world that's ripe for exploration, from a guy who is a master craftsman of compelling stories. This is by far my favorite game to actually play in the SNES' library.

3. Hypnospace Outlaw (PC/XBO/PS4/Switch, 2019)

Back-to-back 90s-flavored games with phenomenal storytelling, Hypnospace Outlaw is a game about playing the moderator of an alternate timeline's niche corner of the Internet. Users on Hypnospace create webpages with their mind so they can hang out and be productive while asleep, and the characters are deeply nuanced with tons of personal details and secrets in tow. It's fun to be an enforcer and track down cases, but it's just as fun to go down the rabbit hole and follow links, and your curious nature is handily rewarded with shortcuts, hacks to be a better enforcer, fun Angelfire/Geocities webpages with MIDIs or ripped MP3s for backing music, and an utterly stellar story of corporate mismanagement, cover-ups, and an attempt to pin this universe's Y2k bug on an innocent kid that makes up the game's final act, a retrospective as you work to archive Hypnospace for modern audiences and tie up any loose ends. Jay Tholen's world is eclectic, surreal, and so oppressively 90s that you *will* listen to their fake Linkin Park on its own long after you play this.

2. Hot Dogs, Horseshoes, & Hand Grenades (PCVR, 2016-)

Rust LTD's range simulator/physics sandbox stands out as one of the defining games in PCVR spaces. Being the brainchild of developer Anton Hand and having been in incredibly active development for eight years, H3VR's dedication to the craft of firearm simulation is matched with a quirky, lighthearted sense of humor that extends into the enemies; sosigs bleed mustard* and say cheesy one-liners or compliment the player before exploding into meat, and Anton's strict adherence to not including real-world human enemies or gore extends to the lore explanation of the seemingly endless number of enemies being a giant meat grinder and casing stuffer that brings units to life. This has pissed off *tons* of fans of other VR FPSes, but I've been long enamored with Anton's realization that what people want from gore (satisfying particles and deformation, cathartic violence) can be done super cheaply and in an approachable manner for all-ages while still maintaining a very strong network of AI pathing and handling systems.

Even if you aren't fighting the enemies, the game's core simulations are still fun to engage with, with lovingly rendered guns that let you see their specific oddities, effectively digitally preserving over 500 firearms, both real and fictional (including a handful of pop cultural pieces like the guns from Robocop, Blade Runner, and Team Fortress 2 in an official collab with Valve) and their inner workings while giving you an expansive sandbox for building scenarios, be they IPSC-style accuracy trials or a simple bed of targets to plink at. Anton still updates this game weekly, working on things like night vision goggles/scopes, thermal cameras, and a Hitman-inspired ImSim mode. Despite this, Anton still does not see the game as a 1.0 finished build, and has plans to continue updating the game for a long while to come.

Cruelty Squad (PC, 2021)

There is no other game like Cruelty Squad, man. Its roots lie in underground artist Ville Kallio, a Finnish creator of the strange, surreal, and visceral. So much of Kallio's art centered around video games and they way they depict and discuss violence, and he took his work to its logical conclusion with an Immersive Sim unlike any other. The visuals are garish, the music is shoddy, the maps are nonsensical with a bizarre fetishization of ad-soaked dystopia, and does a great job of putting you into the headspace of the depressed former Death Squad member Empty Fuck, who finds himself becoming a gig economy worker settling petty corporate disputes for his former boss with the aid of a slew of lethal, stupid weaponry.

For your trouble, you're paid out a pittance, so most of your income has to come from side hustles. Gibbing enemies lets you harvest their organs, which is fantastic for you as modern medicine has made death a thing of the past, stitching cadavers back to life and saddling them with medical debt. If you're not fishing or playing the incredibly volatile stock market that experiences a short squeeze that reaches MOASS levels, you're organ harvesting, which also nets you an opportunity to steal a fallen foe's weapons after you scoop up his liver and kidneys, as you can only get new guns by carrying them out with you on a successful hit. The game takes you to cultist lairs, cushy offices with armed guards, a bombed out nightclub in Helsinki created in the aftermath of a chemical weapons attack to blockbust the district, and straight up to Cruelty Squad HQ to confront the balance of life and death in the world.

Cruelty Squad is truly so beautiful in its unabashed ugliness. The NPCs complain about their life and financial woes while their bosses gamble the extracted value of their labor on buying new yachts, advertisements for the game's brands are everywhere, and though the wealthy bourgeois are free to flaunt their wealth and perversion, the common prole finds themselves in a constant loop of being caught in the crossfire of mass shootings and waking up an instant later with discharge paperwork and a hospital bill. Kallio has made a truly chaotic, bitter, visceral world mirroring our own frustrations with the modern technology and finance sectors, and displays an incredible understanding of game design through all of the design decisions clearly meant to draw the most ire and frustration. It's not an easy game to enjoy, Cruelty Squad. It's difficult with an unfair difficulty curve and some decently bad levels, but my GOD its marriage of Deus Ex and Hitman ImSim sensibilities and a passionate disdain for late-stage Capitalism make it an easy choice for my favorite game of all time.

[tedcruzblogs]

Essential Steps in Water Damage Restoration

Water damage can wreak havoc on your property, leading to costly repairs and potential health hazards. Whether caused by natural disasters, plumbing failures, or human error, the impact of water damage can be extensive and devastating. Effective water damage restoration is crucial to mitigate these impacts and restore your property to its former state. Here are the essential steps involved in water damage restoration.

Assessment

The first step in water damage restoration is a thorough assessment of the affected area. Identifying the extent of water damage is critical to determine the necessary course of action. Quick assessment is vital as prolonged water exposure can lead to structural damage and mold growth. Professional restoration companies use advanced tools like moisture meters and thermal imaging cameras to detect hidden water damage.

Water Extraction

Once the assessment is complete, the next step is water extraction. Removing standing water as quickly as possible minimizes further damage to the property. Various methods and equipment are used for water extraction, including submersible pumps, wet vacuums, and industrial-strength water extractors. While DIY methods may be effective for minor leaks, professional extraction is recommended for significant water damage to ensure thorough removal.

Drying and Dehumidification

After water extraction, the affected areas must be dried and dehumidified to prevent mold and mildew growth. Techniques for effective drying include the use of high-speed air movers and industrial-grade dehumidifiers. These devices accelerate the evaporation process and remove moisture from the air. Monitoring humidity levels and adjusting equipment as needed ensures that the drying process is efficient and complete.

Restoration and Repair

Restoration and repair are essential to return your property to its pre-damage condition. This step involves repairing structural damage, such as replacing drywall, flooring, and insulation. Addressing mold and mildew is also crucial, as these can pose serious health risks. Professional restoration services use antimicrobial treatments and specialized cleaning techniques to eliminate mold spores and prevent future growth.

Prevention

Preventing future water damage is the final step in the restoration process. Regular maintenance and timely repairs can significantly reduce the risk of water damage. Here are some preventive tips:

Inspect and maintain your plumbing system regularly.

Ensure proper drainage around your property.

Install a sump pump in your basement.

Use water leak detectors and alarms.

Keep gutters and downspouts clean and functional.

Conclusion

Water damage restoration is a multi-step process that requires prompt action and professional expertise. By following these essential steps—assessment, water extraction, drying and dehumidification, restoration and repair, and prevention—you can effectively mitigate the impacts of water damage and protect your property. Taking preventive measures and being prepared can save you time, money, and stress in the long run.

[jameswebb-discoveries]

James Webb Space Telescope Discovers Surprising Revelations about Ganymede and Io. Full article here

🔭 The James Webb Space Telescope (JWST) is on a roll, revealing jaw-dropping discoveries about Jupiter's fascinating moons, Ganymede and Io! 🔭

🌌 Ganymede - The Largest Moon's Hidden Secret 🌌 JWST's sensitive infrared cameras exposed hydrogen peroxide (H2O2) around Ganymede's poles, a first-time detection! 🌠 The moon's magnetic field directs charged particles from Jupiter's magnetosphere towards the poles, causing a captivating process called radiolysis, altering the polar caps' surface chemistry. 🌈 This exciting find sheds light on icy bodies' chemistry across the outer solar system, unlocking the secrets of neighboring moons like Europa and Callisto! 🪐

🌋 Io - Unraveling Sulfurous Volcanic Mysteries 🌋 Io's volcanic prowess comes to the fore with JWST's high-resolution spectrometer. The thermal infrared measurements captured intense eruptions at Kanehekili Fluctus and Loki Patera. 🌋🔥 Thanks to JWST's observations, scientists linked sulfur monoxide (SO) emissions to volcanic activity, deepening our knowledge of Io's extreme geology and atmosphere. 🌠🔍

🚀 Exciting Times for Astronomy! 🚀 JWST's Early Release Science program is unlocking the cosmos' hidden gems! 🌟 These discoveries highlight the importance of investing in advanced space telescopes to unravel the universe's mysteries. 🌌 Let's celebrate the triumphs of science and look forward to more groundbreaking revelations from the James Webb Space Telescope! 🎉

📷 Image Credit: Samantha Trumbo, Cornell [Ganymede], and Imke de Pater, UC Berkeley [Io]

Download James Webb Discovery app at www.jameswebbdiscovery.com

[spacenutspod]

A new, higher-resolution infrared camera outfitted with a variety of lightweight filters could probe sunlight reflected off Earth’s upper atmosphere and surface, improve forest fire warnings, and reveal the molecular composition of other planets. The cameras use sensitive, high-resolution strained-layer superlattice sensors, initially developed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, using IRAD, Internal Research and Development funding. Their compact construction, low mass, and adaptability enable engineers like Tilak Hewagama to adapt them to the needs of a variety of sciences. Goddard engineer Murzy Jhabvala holds the heart of his Compact Thermal Imager camera technology – a high-resolution, high-spectral range infrared sensor suitable for small satellites and missions to other solar-system objects. “Attaching filters directly to the detector eliminates the substantial mass of traditional lens and filter systems,” Hewagama said. “This allows a low-mass instrument with a compact focal plane which can now be chilled for infrared detection using smaller, more efficient coolers. Smaller satellites and missions can benefit from their resolution and accuracy.” Engineer Murzy Jhabvala led the initial sensor development at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, as well as leading today’s filter integration efforts. Jhabvala also led the Compact Thermal Imager experiment on the International Space Station that demonstrated how the new sensor technology could survive in space while proving a major success for Earth science. More than 15 million images captured in two infrared bands earned inventors, Jhabvala, and NASA Goddard colleagues Don Jennings and Compton Tucker an agency Invention of the Year award for 2021. The Compact Thermal Imager captured unusually severe fires in Australia from its perch on the International Space Station in 2019 and 2020. With its high resolution, detected the shape and location of fire fronts and how far they were from settled areas — information critically important to first responders. Credit: NASA Data from the test provided detailed information about wildfires, better understanding of the vertical structure of Earth’s clouds and atmosphere, and captured an updraft caused by wind lifting off Earth’s land features called a gravity wave. The groundbreaking infrared sensors use layers of repeating molecular structures to interact with individual photons, or units of light. The sensors resolve more wavelengths of infrared at a higher resolution: 260 feet (80 meters) per pixel from orbit compared to 1,000 to 3,000 feet (375 to 1,000 meters) possible with current thermal cameras. The success of these heat-measuring cameras has drawn investments from NASA’s Earth Science Technology Office (ESTO), Small Business Innovation and Research, and other programs to further customize their reach and applications. Jhabvala and NASA’s Advanced Land Imaging Thermal IR Sensor (ALTIRS) team are developing a six-band version for this year’s LiDAR, Hyperspectral, & Thermal Imager (G-LiHT) airborne project. This first-of-its-kind camera will measure surface heat and enable pollution monitoring and fire observations at high frame rates, he said. NASA Goddard Earth scientist Doug Morton leads an ESTO project developing a Compact Fire Imager for wildfire detection and prediction. “We’re not going to see fewer fires, so we’re trying to understand how fires release energy over their life cycle,” Morton said. “This will help us better understand the new nature of fires in an increasingly flammable world.” CFI will monitor both the hottest fires which release more greenhouse gases and cooler, smoldering coals and ashes which produce more carbon monoxide and airborne particles like smoke and ash. “Those are key ingredients when it comes to safety and understanding the greenhouse gases released by burning,” Morton said. After they test the fire imager on airborne campaigns, Morton’s team envisions outfitting a fleet of 10 small satellites to provide global information about fires with more images per day. Combined with next generation computer models, he said, “this information can help the forest service and other firefighting agencies prevent fires, improve safety for firefighters on the front lines, and protect the life and property of those living in the path of fires.” Probing Clouds on Earth and Beyond Outfitted with polarization filters, the sensor could measure how ice particles in Earth’s upper atmosphere clouds scatter and polarize light, NASA Goddard Earth scientist Dong Wu said. This applications would complement NASA’s PACE — Plankton, Aerosol, Cloud, ocean Ecosystem — mission, Wu said, which revealed its first light images earlier this month. Both measure the polarization of light wave’s orientation in relation to the direction of travel from different parts of the infrared spectrum. “The PACE polarimeters monitor visible and shortwave-infrared light,” he explained. “The mission will focus on aerosol and ocean color sciences from daytime observations. At mid- and long-infrared wavelengths, the new Infrared polarimeter would capture cloud and surface properties from both day and night observations.” In another effort, Hewagama is working Jhabvala and Jennings to incorporate linear variable filters which provide even greater detail within the infrared spectrum. The filters reveal atmospheric molecules’ rotation and vibration as well as Earth’s surface composition. That technology could also benefit missions to rocky planets, comets, and asteroids, planetary scientist Carrie Anderson said. She said they could identify ice and volatile compounds emitted in enormous plumes from Saturn’s moon Enceladus. “They are essentially geysers of ice,” she said, “which of course are cold, but emit light within the new infrared sensor’s detection limits. Looking at the plumes against the backdrop of the Sun would allow us to identify their composition and vertical distribution very clearly.” By Karl B. Hille NASA’s Goddard Space Flight Center, Greenbelt, Md. Share Details Last Updated May 22, 2024 Related TermsGoddard TechnologyGoddard Space Flight CenterTechnology Keep Exploring Discover More Topics From NASA Goddard Technology Innovations Goddard's Office of the Chief Technologist oversees the center's technology research and development efforts and provides updates on the latest… Goddard’s Internal Research & Development Program (IRAD) Information and links for Goddard's IRAD and CIF technology research and development programs and other NASA tech development sources. Technology Goddard Office of the Chief Technologist Staff page for the Goddard Office of the Chief Technologist with portraits and short bios

[lensman-arms-race]

I thought I was the only one with TV People seeing infrared! I like that the hardware senses are inherently different and how they act are depending on that.

The problem though is that they might not be able to see each other's emoticons, can they?

Maybe not! I think a TV display in infrared would just look like plain glass, because the displayed images would have no effect on the screen temperature. (Unless it's a special thermal display, maybe?)

I think the emoticons are for the benefit of the camera-heads and the TV-heads don't need to see each others' displays. (Maybe they beam the emoticons to each other using something like the old Teletext system.)

[spacetimewithstuartgary]

Telescope for NASA’s Roman Mission complete, delivered to Goddard

NASA’s Nancy Grace Roman Space Telescope is one giant step closer to unlocking the mysteries of the universe. The mission has now received its final major delivery: the Optical Telescope Assembly, which includes a 7.9-foot (2.4-meter) primary mirror, nine additional mirrors, and supporting structures and electronics. The assembly was delivered Nov. 7. to the largest clean room at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, where the observatory is being built.

The telescope will focus cosmic light and send it to Roman’s instruments, revealing many billions of objects strewn throughout space and time. Using the mission’s Wide Field Instrument, a 300-megapixel infrared camera, astronomers will survey the cosmos all the way from the outskirts of our solar system toward the edge of the observable universe. Scientists will use Roman’s Coronagraph Instrument to test new technologies for dimming host stars to image planets and dusty disks around them in far better detail than ever before.

“We have a top-notch telescope that’s well aligned and has great optical performance at the cold temperatures it will see in space,” said Bente Eegholm, optics lead for Roman’s Optical Telescope Assembly at NASA Goddard. “I am now looking forward to the next phase where the telescope and instruments will be put together to form the Roman observatory.”

Designed and built by L3Harris Technologies in Rochester, New York, the assembly incorporates key optics (including the primary mirror) that were made available to NASA by the National Reconnaissance Office. The team at L3Harris then reshaped the mirror and built upon the inherited hardware to ensure it would meet Roman’s specifications for expansive, sensitive infrared observations.

“The telescope will be the foundation of all of the science Roman will do, so its design and performance are among the largest factors in the mission’s survey capability,” said Josh Abel, lead Optical Telescope Assembly systems engineer at NASA Goddard.

The team at Goddard worked closely with L3Harris to ensure these stringent requirements were met and that the telescope assembly will integrate smoothly into the rest of the Roman observatory.

The assembly’s design and performance will largely determine the quality of the mission’s results, so the manufacturing and testing processes were extremely rigorous. Each optical component was tested individually prior to being assembled and assessed together earlier this year. The tests helped ensure that the alignment of the telescope’s mirrors will change as expected when the telescope reaches its operating temperature in space.

Then, the telescope was put through tests simulating the extreme shaking and intense sound waves associated with launch. Engineers also made sure that tiny components called actuators, which will adjust some of the mirrors in space, move as predicted. And the team measured gases released from the assembly as it transitioned from normal air pressure to a vacuum –– the same phenomenon that has led astronauts to report that space smells gunpowdery or metallic. If not carefully controlled, these gases could contaminate the telescope or instruments.

Finally, the telescope underwent a month-long thermal vacuum test to ensure it will withstand the temperature and pressure environment of space. The team closely monitored it during cold operating conditions to ensure the telescope’s temperature will remain constant to within a fraction of a degree. Holding the temperature constant allows the telescope to remain in stable focus, making Roman’s high-resolution images consistently sharp. Nearly 100 heaters on the telescope will help keep all parts of it at a very stable temperature.

“It is very difficult to design and build a system to hold temperatures to such a tight stability, and the telescope performed exceptionally,” said Christine Cottingham, thermal lead for Roman’s Optical Telescope Assembly at NASA Goddard.

Now that the assembly has arrived at Goddard, it will be installed onto Roman’s Instrument Carrier, a structure that will keep the telescope and Roman’s two instruments optically aligned. The assembly’s electronics box –– essentially the telescope’s brain –– will be mounted within the spacecraft along with Roman’s other electronics.

With this milestone, Roman remains on track for launch by May 2027.

“Congratulations to the team on this stellar accomplishment!” said J. Scott Smith, the assembly’s telescope manager at NASA Goddard. “The completion of the telescope marks the end of an epoch and incredible journey for this team, and yet only a chapter in building Roman. The team’s efforts have advanced technology and ignited the imaginations of those who dream of exploring the stars.”

TOP IMAGE: Upon arrival at NASA's Goddard Space Flight Center, the Optical Telescope Assembly for the agency's Nancy Grace Roman Space Telescope was lifted out of the shipping fixture and placed with other mission hardware in Goddard's largest clean room. Now, it will be installed onto Roman's Instrument Carrier, a structure that will keep the telescope and Roman's two instruments optically aligned. The assembly's electronics box –– essentially the telescope's brain –– will be mounted within the spacecraft along with Roman's other electronics. Credit NASA/Chris Gunn

CENTRE IMAGE: In this photo, optical engineer Bente Eegholm inspects the surface of the primary mirror for NASA's Nancy Grace Roman Space Telescope. This 7.9-foot (2.4-meter) mirror is a major component of the Optical Telescope Assembly, which also contains nine additional mirrors and supporting structures and electronics. Credit NASA/Chris Gunn

BOTTOM IMAGE: This photo shows the Optical Telescope Assembly for NASA's Nancy Grace Roman Space Telescope, which was recently delivered to the largest clean room at the agency's Goddard Space Flight Center in Greenbelt, Md. Credit NASA/Chris Gunn

[galetech]

Top Wholesale Surveillance CCTV Camera Brands in India

In India, the demand for surveillance CCTV cameras has been steadily increasing due to the growing awareness of security needs in both residential and commercial settings. With numerous brands competing in the market, let's explore some of the top wholesale surveillance CCTV camera brands in India:

Hikvision: Hikvision is one of the most well-known and trusted brands in the surveillance industry. They offer a wide range of CCTV cameras, including IP cameras, dome cameras, bullet cameras, and PTZ cameras. Hikvision is known for its high-quality products, advanced features, and reliable performance, making them a popular choice for wholesale purchases.

Dahua Technology: Dahua is another prominent player in the Indian surveillance market. They are recognized for their innovative solutions, such as AI-powered cameras, thermal cameras, and advanced video analytics. Dahua's products cater to various industry needs, making them a preferred option for wholesalers and system integrators.

CP Plus: CP Plus is an Indian brand that has gained significant popularity in the surveillance domain. They offer a wide range of cameras, including HD cameras, IP cameras, and wireless cameras, along with DVRs and NVRs. CP Plus focuses on affordability without compromising on quality, which has contributed to its success in the wholesale market.

Bosch Security Systems: Bosch is a global player with a strong presence in the Indian market. Their surveillance cameras are known for their durability, advanced technology, and seamless integration with other security systems. Bosch caters to various applications, from small businesses to large enterprises.

Evoke Hi Tech: Evoke Hi Tech is a renowned brand in the electronics industry and has a significant share in the surveillance camera market. They provide high-resolution cameras, low-light cameras, and advanced PTZ cameras suitable for various surveillance needs. Evoke Hi Tech's cameras are preferred for their image quality and reliability.

Samsung: Samsung, a well-known consumer electronics brand, also offers a range of surveillance cameras in India. Their cameras come equipped with advanced features like digital image stabilization, thermal imaging, and smart analytics, making them an attractive choice for wholesale buyers.

Honeywell: Honeywell is a global conglomerate with a strong presence in the security and surveillance sector. They offer a diverse range of CCTV cameras, including dome cameras, bullet cameras, and panoramic cameras. Honeywell's cameras are known for their rugged design and cutting-edge technology.

These brands have earned their reputation in the Indian market by consistently delivering high-quality, reliable surveillance solutions. When purchasing wholesale CCTV cameras, it's essential to consider factors like camera type, resolution, lens options, and additional features to ensure they meet specific security requirements.