The thread for space cadets!

Enceladus’s oceans may be the right saltiness to sustain life

The way ice covers the surface of Saturn’s moon Enceladus suggests that the oceans trapped beneath it may be only a little less salty than Earth’s oceans. The finding adds to the possibility that this moon might be able to sustain life.

The surface of Enceladus is encased in clean, bright ice. Wanying Kang at Massachusetts Institute of Technology and her colleagues wanted to determine what the characteristics of this ice shell indicate about the ocean beneath it.

Samples taken by the Cassini spacecraft of geyser-like jets of water from Enceladus’s surface previously showed that there is some organic matter that could sustain potential life on the icy moon. Considering the waters under Enceladus’s ice was the logical next step for inferring its habitability, says Kang.

The team devised a theoretical model detailing how ocean salinity, ocean currents and ice geometry affect each other on a planet or a moon, then tweaked it to best reproduce the properties of Enceladus’s ice.

The researchers found that saltier subsurface oceans correspond to thicker ice on a planet’s poles than over its equator and vice versa for less salty water. On Enceladus, the ice over the poles is thinner than the ice over the equator. The specific variation in thickness suggests that the ocean’s salinity could be as high as 30 grams of salt in a kilogram of water. For comparison, Earth’s oceans have a salinity of 35 grams of salt per kilogram of water.

The researchers also determined details of water circulation under the moon’s ice. These currents are related to temperature differences in the water so understanding them is also important for determining habitability, says Kang.

The team found that some heat emanates from the bottom of Enceladus’s ocean, possibly indicating the existence of heat vents in the ocean floor. Kang says that some astrobiologists have previously suggested that, like on Earth, such hydrothermal vents could be where life is found in the future.​

Writeup Paper

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Disco ball vs Einstein

A newly launched satellite aims to measure how Earth’s rotation drags the fabric of space-time around itself — an effect of Einstein’s general theory of relativity — ten times more accurately than ever before.​
The Laser Relativity Satellite 2 (LARES-2) launched from the European Space Agency’s (ESA) spaceport in Kourou, French Guiana, on 13 July. It was built by the Italian Space Agency (ASI) at a cost of around €10 million (US$10.2 million), and lifted off on the maiden flight of an upgraded version of the European Vega rocket, called Vega C.​
LARES-2’s structure is disarmingly simple: it is a sphere of metal covered with 303 reflectors, with no on-board electronics or navigation control.​
LARES-2 packs around 295 kilograms of material into a sphere less than 50 centimetres across. Its density minimizes the effects of phenomena such as radiation pressure from sunlight or the feeble drag from Earth’s atmosphere at high altitudes, says aerospace engineer Antonio Paolozzi of Sapienza University in Rome. After experimenting with custom high-density materials, the team opted for an off-the-shelf nickel alloy. This had acceptable density and enabled LARES-2 to qualify for the Vega C maiden flight without expensive flight-certification tests.​
Using an existing global network of laser-ranging stations, Ciufolini and his colleagues plan to track the orbit of LARES-2 for several years. This kind of probe can continue to provide data for decades. “You can just sit back and send laser beams to it,” Will says. “In terms of cost it’s a cheap, good thing to do.”​
According to Newtonian gravity, an object orbiting a perfectly spherical planet should keep tracing the same ellipse, eon after eon. But in 1913, Albert Einstein and his collaborator Michele Besso used a preliminary version of general relativity to suggest that if such a planet were rotating, it should cause the satellite’s orbit to shift slightly. The precise mathematics of the effect was calculated in 1918 by Austrian physicists Josef Lense and Hans Thirring. Modern calculations predict that the Lense–Thirring effect, a kind of relativistic ‘frame dragging’, should make the plane of the orbit precess, or rotate, around the Earth’s axis, by 8.6 millionths of a degree per year.​
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Pictures of Mars' Grand Canyon

Though calling Valles Marineris the "Grand Canyon" kind of plays it down. At 4000 km long, 200 km wide and up to 7 km deep, Valles Marineris is almost ten times longer, 20 times wider and five times deeper than the Grand Canyon. As the largest canyon system in the Solar System, it would span the distance from the northern tip of Norway to the southern tip of Sicily.

Mars Express has been orbiting the Red Planet since 2003, imaging Mars’ surface, mapping its minerals, identifying the composition and circulation of its tenuous atmosphere, probing beneath its crust, and exploring how various phenomena interact in the martian environment.

The mission’s High Resolution Stereo Camera (HRSC), responsible for these new images, has revealed much about Mars’ diverse surface features, with recent images showing everything from wind-sculpted ridges and grooves through impact craters and channels that once carried liquid water to volcanoes, tectonic faults, river channels and ancient lava pools.

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NASA finds clangers homes on moon are a comfortable temperature

NASA-funded scientists have discovered shaded locations within pits on the Moon that always hover around a comfortable 63 F (about 17 C) using data from NASA’s Lunar Reconnaissance Orbiter (LRO) spacecraft and computer modeling.​
The pits, and caves to which they may lead, would make thermally stable sites for lunar exploration compared to areas at the Moon’s surface, which heat up to 260 F (about 127 C) during the day and cool to minus 280 F (about minus 173 C) at night.​

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Clangers home
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NASA images of moon
 
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Four revelations from the Webb telescope about distant galaxies

There are an awful lot of galaxies way out there

Because Webb detects infrared light, and because the expansion of the cosmos stretches light to redder wavelengths, the telescope is well suited to spotting galaxies that formed early in the Universe’s history. In its first observing programmes, which kicked off in June, Webb discovered many distant galaxies that lie beyond the reach of other observatories, such as the Hubble Space Telescope.​
One study combed through data from many of the distant galaxy fields Webb has observed so far, to analyse the rate at which stars formed in the early Universe. It found 44 previously unknown galaxies stretching back to within 300 million years of the Big Bang. Combined with 11 previously known galaxies, the findings show that there was a significant population of galaxies forming stars in the early Universe​
Many galaxies are competing for the ‘most distant’ title

Perhaps the highest-profile rush is the stampede of research teams vying to identify the most distant galaxy in the Webb data. A number of candidates have been spotted that will need to be confirmed through further studies, but all of them would break Hubble’s record for the most-distant galaxy, which dates to around 400 million years after the Big Bang.​
Some early galaxies are surprisingly complex
Webb’s distant galaxies are also turning out to have more structure than astronomers had expected.​
One study of Webb’s first deep-field image found a surprisingly large number of distant galaxies that are shaped like disks. Using Hubble, astronomers had concluded that distant galaxies are more irregularly shaped than nearby ones, which, like the Milky Way, often display regular forms such as disks. The theory was that early galaxies were more often distorted by interactions with neighbouring galaxies. But the Webb observations suggest there are up to 10 times as many distant disk-shaped galaxies as previously thought.​
Closer galaxies are smaller than expected

The surprises from Webb continue even a little later in the Universe’s evolution. One study looked at Webb’s observations of ‘cosmic noon’, the period approximately 3 billion years after the Big Bang. This is when star formation peaked in the Universe, and the most light was created.​
Wren Suess, an astronomer at the University of California, Santa Cruz, compared Hubble images of galaxies at cosmic noon with Webb images of the same galaxies. At the infrared wavelengths detected by Webb, most of the massive galaxies looked much smaller than they did in Hubble images. “It potentially changes our whole view of how galaxy sizes evolve over time,” Suess says. Hubble studies suggested that galaxies start out small and grow bigger over time, but the Webb findings hint that Hubble didn't have the whole picture, and so galaxy evolution might be more complicated than scientists had anticipated.​
 
Firm’s new tech could make space more accessible

After nearly six years of closed door research and development, Albuquerque-based X-Bow Systems publicly debuted ground-breaking rocket motor technology this year that could shake up the space-launch industry.
X-Bow (pronounced “crossbow”), which originally formed in 2016, burst out of stealth mode last April, unveiling a newly developed family of suborbital and orbital launch vehicles, along with a new, potentially revolutionary, automated process for making solid state propellant for rocket motors. That additive manufacturing process may represent the biggest technological leap in solid fuel rocket-motors in 50 years, possibly allowing radical reduction in costs for vehicle launches and greater flight frequency.

“Our solid rocket motor manufacturing process is an emerging disrupter for the aerospace industry,” X-Bow founder and CEO Jason Hundley told the Journal. “It’s a new, patent-pending ‘energetics’ technology.”
X-Bow’s proprietary procedure for “additive manufacturing of solid propellants,” or AMSP, marks the first time a company has successfully applied 3D printing to solid-state fuel for rocket motors. Other manufacturers do use 3D printing for the motors themselves, but only a couple of commercial companies currently make solid-state rocket motor fuel, and they use a decades-old, time consuming process that normally lasts six to eight weeks before delivery to customers, Hundley said. The traditional fuel making procedure begins with a slow mixing of chemicals, which can take up to five days. After that, the mixture is poured into a giant steel casting pit, where it remains for 10-15 days for the ingredients to slowly harden. Then, when the solid state fuel is ready for removal, it gets put through intensive post-inspection. And only after that is the propellant finally shipped onto the last stage of manufacturing, whereby the fuel gets integrated into the rocket motor assembly process itself.

In contrast, X-Bow’s additive manufacturing compresses the entire mixing-and-curing procedure into a threeday process, with all the automated technology installed inside compact shipping containers that X-Bow calls a “Rocket Factory in a Box.” In addition, the company has developed proprietary rocket motors that are designed to be integrated with the fuel through a simple, snap-in procedure using cartridges the encapsulate the propellant.
“It’s a cartridge-based approach,” Hundley said. “We put the energetics (propellant) in the bottom of the rocket motor and screw in the nozzle on the back.”

The overall, end result is a far simpler, more efficient process that significantly lowers the manufacturing footprint, immensely speeding the timeline and reducing the costs for making both the solid-state propellant and the fully-assembled rocket motors themselves. “We can produce about 700 pounds of grain (propellant) in about four hours, with one-to-two days for curing before it’s dispensed out of the system,” Hundley said. “That means we can make between 1,500 and 2,000 pounds of energetics in a week.” X-Bow hadn’t considered creating new propellant making technology when it originally launched six years ago. Rather, Hundley and a group of veteran aerospace industry colleagues founded the company to build a new family of launch vehicles that X-Bow originally developed in cooperation with Sandia National Laboratories and the Air Force Research Laboratory at Kirtland Air Force Base. That new vehicle, dubbed the “Bolt Rocket,” is designed for flexible construction to accommodate different sizes and capabilities for suborbital and orbital launches, with corresponding alterations in rocker-motor configuration depending on the mission, Hundley said.

“We can go from junior size all the way to super high-end vehicles,” Hundley said. “It’s a family of vehicles with a common front-end chassis and rocket motor foundation.” X-Bow originally expected to use commercial suppliers for its solid-state rocket motor propellant. But the procurement process turned out so slow and costly, the company decided to create its own fuel-making technology. And that, together with its Bolt Rocket and proprietary rocket motor design, has substantially broadened X-Bow’s commercial opportunities beyond its original focus on launch services for government and private-sector clients. Space payload flights for customers remain central to X-Bow’s business offerings, but its proprietary solid-state rocket motors can be adapted for other uses such as missiles, including emerging hypersonic technology. “We’ll do space launches as a service, but we can also tune the factory design to provide rocket motors for other applications,” Hundley said. “Every tactical missile, for example, has a solid rocket motor.”

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X-Bow Systems “Rocket Factory in a Box” facility. The Albuquerque-based company uses its own additive-manufacturing process to produce solid-state fuel in a compressed timeline, a process that takes place in customized shipping containers. COURTESY OF X-BOW SYSTEMS

It could also become a commercial supplier of rocket-motor propellant, working with clients to adapt the particular fuel mixtures needed for other rocket-motor designs. And, given its hyper-fast propellant-production process — plus its varying mission-specific rocket and motor designs — the company could offer some of the fastest project turn-around times in the aerospace industry.
“We’ve developed almost a ‘just-in-time’ capability for suborbital and orbital systems,” Hundley said.

Thanks to its breakthrough technology, the company has already developed a formidable customer base in both government and commercial sectors, despite only just emerging from stealth mode. It earned about $7 million in revenue in 2021, and projects between $15 million and $20 million this year. It also closed on a $27 million round of private equity in April with institutional and corporate venture funds, including Lockheed Martin Ventures.
The company was originally based in Huntsville, Alabama, although it’s maintained a substantial presence in New Mexico since launching.

In 2019, however, X-Bow moved its corporate headquarters and all its central operations to Albuquerque. It now leases a 5,000-squarefoot facility in Uptown, and it’s established a manufacturing researchand- development complex in Socorro at the New Mexico Institute for Mining and Technology’s Energetic Materials Research and Testing Center. It currently employs about 70 people, more than half of them in New Mexico, with projected growth to 100 this year, depending on public and commercial contracts now under negotiation. And it maintains close links with many local businesses and public entities here. It’s
New tech makes space accessible contracted directly, for example, with two New Mexico-based engineering firms to provide products and services.

“We’ve had multiple New Mexico businesses involved with our operations, and we intend to keep them involved in future missions,” Hundley said. In fact, Central New Mexico Community College has a vested interest in X-Bow through CNM Ingenuity, which manages all of CNM’’s commercial endeavors. The Ingenuity Venture Fund and the ABQid business accelerator investment fund — which is also run by CNM Ingenuity — jointly contributed to a $2.4 million seed round of investment in X-Bow three years ago, said T.J. Cook, who manages both funds.

“X-Bow has really created a paradigm shift in the world of propellants,” Cook told the Journal. “The company has developed platform technology for not only rocket launches, but many other applications.
It now has many business inroads in place to excel in the market.”

Kevin Robinson-Avila covers technology, energy, venture capital and utilities for the Journal. He can be reached at krobinson-avila@abqjournal. com.
 
Cartwheel galaxy caused by galactic crash (paywalled)

The Cartwheel galaxy is about 500 million light years away and measures about 150,000 light years across. Researchers believe that it was most likely a spiral galaxy similar to the Milky Way before one of its companion galaxies blasted through it like a bullet through a target, sending waves of stars and gas rippling out from the galaxy’s centre and creating the nested ring shapes that we see today.​
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Spoiler Full text :
The James Webb Space Telescope (JWST) has taken a picture of one of the strangest galaxies in the universe. The details of the Cartwheel galaxy are obscured by dust, which has made studying it difficult, but the new images from JWST peer through to reveal this weird galaxy in more detail than ever before.

The Cartwheel galaxy is about 500 million light years away and measures about 150,000 light years across. Researchers believe that it was most likely a spiral galaxy similar to the Milky Way before one of its companion galaxies blasted through it like a bullet through a target, sending waves of stars and gas rippling out from the galaxy’s centre and creating the nested ring shapes that we see today.

The inner ring that surrounds the relatively old stars at the centre of the galaxy is made mostly of hot, bright dust, along with some huge clusters of young stars. The outer ring is just as dynamic if not even more so – as it expands outward, it smashes through the gas surrounding the galaxy and triggers bursts of star formation, which light up the surrounding dust.

There are also areas of intense star formation in the spokes connecting the two rings, which seem to be remnants of the galaxy’s spiral arms. “This dust is lighting up the spokes as well as the rim of the wheel, and that’s very neat to see,” says Karl Gordon at the Space Telescope Science Institute in Maryland. “It’s telling us there’s lots of star formation going on, maybe even more than we thought.”

This image also revealed a region of star formation at the bottom right of the galaxy that is much brighter than researchers expected. As they continue to analyse the image, they will gain more insight into how the Cartwheel galaxy is evolving and what it might look like in the future as the aftermath of its titanic collision settles down.
 
The SLS rocket might actually launch in two weeks. It would be an uncrewed mission that would last for 39-42 days, with the Orion spacecraft flying around the Moon.

https://arstechnica.com/science/202...ace-launch-system-rocket-is-now-ready-to-fly/

NASA continues to target three dates to attempt the Artemis I launch: August 29, September 2, and September 5.

...

Each of the three upcoming launch opportunities would allow for a "long-class" mission for the Orion spacecraft, which will be uncrewed and fly into lunar orbit for several weeks before returning to Earth and splashing down in the Pacific Ocean. The missions would range in length from 39 to 42 days.
 
Northern lights may be visible as far south as New York, Chicago, and Portland

A plume of "dark plasma" hurled from the sun will be engulfed to form a "cannibal" coronal mass ejection which will sideswipe the Earth on Thursday (Aug. 18), causing a strong G3 geomagnetic storm.​
The "dark plasma explosion" was first spotted by solar observers on Sunday (Aug. 14) as it erupted from a sunspot on the sun's surface at a speed of roughly 1.3 million mph (2.1 million km/h), tearing "through the sun's atmosphere, creating a coronal mass ejection (CME)," or explosive jets of solar material, spaceweather.com wrote in an update (opens in new tab). Then, on Monday (Aug. 15), another CME, created by the collapse of a gigantic magnetic filament, was launched from the sun.​
The two eruptions together will merge to form a cannibal coronal mass ejection, according to National Oceanic and Atmospheric Administration (NOAA) forecasts (opens in new tab). Cannibal CMEs occur when one fast-moving solar eruption overtakes an earlier eruption in the same region of space, gobbling up the charged particles to form a giant, combined wavefront that, upon reaching Earth, triggers a powerful geomagnetic storm.​
They're all expected to arrive at about 1 a.m. ET on Thursday, possibly triggering stunning, highly active auroras as far south as Pennsylvania, Iowa, and Oregon, according to the Space Weather Prediction Center, a branch of the National Weather Service.​
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an aurora over Whitehorse, Yukon on the night of September 3, 2012
 
In space, you can hear black holes scream

As long as they are in a galaxy cluster that has enough gas to pick up actual sound.

Since 2003, the black hole at the center of the Perseus galaxy cluster has been associated with sound. This is because astronomers discovered that pressure waves sent out by the black hole caused ripples in the cluster’s hot gas that could be translated into a note – one that humans cannot hear some 57 octaves below middle C. Now a new sonification brings more notes to this black hole sound machine. This new sonification – that is, the translation of astronomical data into sound – is being released for NASA’s Black Hole Week this year.​
In some ways, this sonification is unlike any other done before (1, 2, 3, 4) because it revisits the actual sound waves discovered in data from NASA's Chandra X-ray Observatory. The popular misconception that there is no sound in space originates with the fact that most of space is essentially a vacuum, providing no medium for sound waves to propagate through. A galaxy cluster, on the other hand, has copious amounts of gas that envelop the hundreds or even thousands of galaxies within it, providing a medium for the sound waves to travel.​
In this new sonification of Perseus, the sound waves astronomers previously identified were extracted and made audible for the first time. The sound waves were extracted in radial directions, that is, outwards from the center. The signals were then resynthesized into the range of human hearing by scaling them upward by 57 and 58 octaves above their true pitch. Another way to put this is that they are being heard 144 quadrillion and 288 quadrillion times higher than their original frequency. (A quadrillion is 1,000,000,000,000,000.) The radar-like scan around the image allows you to hear waves emitted in different directions. In the visual image of these data, blue and purple both show X-ray data captured by Chandra.​
 
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The SLS rocket might actually launch in two weeks. It would be an uncrewed mission that would last for 39-42 days, with the Orion spacecraft flying around the Moon.

https://arstechnica.com/science/202...ace-launch-system-rocket-is-now-ready-to-fly/
Yup, launching tomorrow! :please:


At $2 billion per launch, it can get 50% more cargo into space than SpaceX for only x13 more money.

It will fly the moon spacecraft Orion backwards around the moon for 6 days and get within 16 miles (around 25km) of it on a very strange path.
Then Orion will come back to Earth and splashdown in the ocean.

Over 300ft. tall (99m) :D
Supposed to more powerful than the Saturn V rocket by 15%.
 
Heart of the Phantom Galaxy

This image from the NASA/ESA/CSA James Webb Space Telescope shows the heart of M74, otherwise known as the Phantom Galaxy. Webb’s sharp vision has revealed delicate filaments of gas and dust in the grandiose spiral arms which wind outwards from the centre of this image. A lack of gas in the nuclear region also provides an unobscured view of the nuclear star cluster at the galaxy's centre.​
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Yup, launching tomorrow! :please:


At $2 billion per launch, it can get 50% more cargo into space than SpaceX for only x13 more money.

It will fly the moon spacecraft Orion backwards around the moon for 6 days and get within 16 miles (around 25km) of it on a very strange path.
Then Orion will come back to Earth and splashdown in the ocean.

Over 300ft. tall (99m) :D
Supposed to more powerful than the Saturn V rocket by 15%.
It did not launch.

The temperature reading on engine 3 was ??? and injecting while too hot, well, the skyscraper of cryogenic rocket fuel might have had a bad day.

NASA is working on a plan to launch it Saturday safely without knowing the actual temperature on engine 3. :eekdance:

 
It did not launch.

The temperature reading on engine 3 was ??? and injecting while too hot, well, the skyscraper of cryogenic rocket fuel might have had a bad day.

NASA is working on a plan to launch it Saturday safely without knowing the actual temperature on engine 3. :eekdance:

Things are not going well.


As the sun rose, an over-pressure alarm sounded and the tanking operation was briefly halted, but no damage occurred and the effort resumed. But minutes later, hydrogen fuel began leaking from the engine section at the bottom of the rocket. NASA halted the operation, while engineers scrambled to plug what was believed to be a gap around a seal in the supply line.

The countdown clocks continued ticking toward an afternoon liftoff; NASA had two hours Saturday to get the rocket off.

I think they said 400,000 people would watch today?
No pressure...

Should go up at 2 P.M. U.S. eastern time zone.
Billions of dollars and our future moon missions!

 
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James Web takes real pictures of an exoplanet!!!

The James Webb Space Telescope has taken its first picture of a planet beyond the Solar System — opening a window to understanding other worlds and underscoring the telescope’s immense capabilities.​

The image is of a planet called HIP 65426 b, an object similar to Jupiter, but younger and hotter, that lies 107 parsecs from Earth in the constellation Centaurus. It is the first exoplanet image ever taken at deep infrared wavelengths, which allow astronomers to study the full range of a planet’s brightness and what it is made of.​
HIP 65426 b is probably around 14 million years old, making it “a baby Jupiter”, Biller says. It’s “like Jupiter, but right after it formed”. Our Solar System is around 4.5 billion years old.​
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The Webb telescope imaged HIP 65426 b at multiple infrared wavelengths (from left to right: 3.00, 4.44, 11.4 and 15.5 micrometres).
 
James Web takes real pictures of an exoplanet!!!

The James Webb Space Telescope has taken its first picture of a planet beyond the Solar System — opening a window to understanding other worlds and underscoring the telescope’s immense capabilities.​

The image is of a planet called HIP 65426 b, an object similar to Jupiter, but younger and hotter, that lies 107 parsecs from Earth in the constellation Centaurus. It is the first exoplanet image ever taken at deep infrared wavelengths, which allow astronomers to study the full range of a planet’s brightness and what it is made of.​
HIP 65426 b is probably around 14 million years old, making it “a baby Jupiter”, Biller says. It’s “like Jupiter, but right after it formed”. Our Solar System is around 4.5 billion years old.​
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The Webb telescope imaged HIP 65426 b at multiple infrared wavelengths (from left to right: 3.00, 4.44, 11.4 and 15.5 micrometres).
What a fatty :)

Pretty cool we can see any planet at all 300 light years away.
 
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Gerald Rhemann has been named the overall winner of Astronomy Photographer of the Year 2022 for his photograph Disconnection Event. The remarkable image shows Comet C/2021 A1, commonly known as Comet Leonard, which was first discovered in January 2021 by astronomer Greg Leonard.
 
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