Close-up of Pandora

Pandora

Cool image time! The image on the right, cropped and reduced to show here, is that of Saturn’s small moon Pandora. The full resolution image was taken on December 18, 2016 during Cassini’s closest fly-by of the Moon ever. It was taken from a distance of 25,200 miles, and has a resolution of 787 feet per pixel.

Note the pooling of dust-like material in the crater. Note also the brighter exposed surfaces on the inner crater rim above that pooled material. It appears to my eye almost as if the dust that had coated the higher elevations of this inner rim has for some unknown reason suddenly settled into the crater’s floor.

Pandora orbits just outside Saturn’s F ring, which means it is well exposed to the material in the ring. I would also expect that much of its surface is well coated with particles from the rings.

Fatal clinical drug trial failed because company did not review all data

The company that conducted a fatal French clinical drug trial that killed one and left four permanently damaged has revealed that it did not review all the available data before administering increased dosages to patients.

Not only is it astonishing that they failed to use all the available data, it is even more amazing that the company itself admits to this.

As I noted when this story first broke in February, this is a big deal, and should get major coverage by news organizations.

…it is disturbing that a research company could be so cavalier about the lives of the human beings it is using as test subjects.

This story also illustrates indirectly the significant decline in the state of today’s modern mainstream press as well as the greater interests of the general public. This is a major science story. For a clinical drug study to kill one of its test subjects is a big deal. Yet I am certain that this will get no coverage in any cable news outlet. (If anyone see a video story about this, please let me know.) The written news outlets on the web will likely do a story, but it will not give it wide exposure.

As far as I can tell, this story got no coverage in the press then, and I expect none now. A dark age is surely coming.

Computer modeling suggests light fluctuations at Tabby’s Star are natural

A computer analysis of the light fluctuations of Tabby’s Star suggest to astronomers that the changes are not caused by objects blocking the star (such as an alien Dyson Sphere under construction) but are instead natural variations caused as the star evolves.

This conclusion is decidedly uncertain. They do not know the nature of this stellar evolution. And they are applying avalanche models to the star to come to this conclusion.

The squealing of pigs

Back in October 2010, just days before the mid-term elections, I wrote the following:

For the sake of argument, let’s assume that, come Tuesday, the Republicans take both houses, in a stunning landslide not seen in more than a century. Let’s also assume that the changes in Congress are going to point decidedly away from the recent liberal policies of large government (by both parties). Instead, every indication suggests that the new Congress will lean heavily towards a return to the principles of small government, low taxes, and less regulation.

These assumptions are not unreasonable. Not only do the polls indicate that one or both of the houses of Congress will switch from Democratic to Republican control, the numerous and unexpected primary upsets of established incumbents from both parties — as well the many protests over the past year by large numbers of ordinary citizens — make it clear that the public is not interested in half measures. Come January, the tone and direction of Congress is going to undergo a shocking change.

Anyway, based on these assumptions, we should then expect next year’s Congress to propose unprecedented cuts to the federal budget, including the elimination of many hallowed programs. The recent calls to defund NPR and the Corporation for Public Broadcastings are only one example.

When Congress attempts this, however, the vested interests that have depended on this funding for decades are not going to take the cuts lightly. Or to put it more bluntly, they are going to squeal like pigs, throwing temper tantrums so loud and insane that they will make the complaints of a typical three-year-old seem truly statesman-like. And they will do so in the hope that they will garner sympathy and support from the general voting public, thereby making the cuts difficult to carry out.

The real question then is not whether the new Congress will propose the cuts required to bring the federal government under control, but whether they, as well as the public, will have the courage to follow through, to defy the howls from these spoiled brats, and do what must be done.

The legislative situation with NASA over the summer and fall might give us a hint about whether the next Congress will have the courage to make the cuts that are necessary. In this case Obama actually proposed doing something close to what conservatives have dreamed of for decades: take NASA (and the government) out of the business of building rockets and spacecraft and pass it over to the private sector.

Moreover, despite the strong dislike the right has for Obama and his leftist policies, many conservative pundits both inside and outside of the space activist community publicly supported the President in this effort.

Nonetheless, these policies were not accepted by Congress. Instead, the legislative body passed an authorization bill that requires NASA to build a new heavy-lift rocket and the manned capsule to go with it. Congress did this partly for national security reasons, but mostly because they wanted to protect the jobs in Houston, Florida, and elsewhere that NASA provides, and thus bring home the bacon to their constituents. And they did this because those constituents had squealed at them about the threatened loss of funding.

In other words, elected officials from both parties had teamed up to authorize this pork-laden program in order to keep the pigs quiet. In other words, NASA’s legislative history this past year does not give us an encouraging view of the future. It appears that Congress will give us the same-old same-old, when asked.

More than six years have passed, and my analysis of the situation in 2010 appears almost perfect. While the Republicans did not win both houses of Congress in 2010, they did in 2014. Despite these victories from voters who clearly wanted them to cut back on the power of government, they did exactly what I expected, based on their actions in connection with NASA and SLS: maintain the pork and chicken out whenever challenged by Obama, the Democrats, the press (I repeat myself), and too many spoiled members of the general public.

After the 2016 elections, things have moved even more to the right. The Republicans not only control both houses of Congress, they have a Republican president (though a very unpredictable one) and the leftwing mainstream press has been discredited and no longer monopolizes the distribution of information. What will happen in the coming years?
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“Anomalous readings” detected during testing of Webb telescope

During standard vibration testing to simulate launch, engineers have detected what they call “anomalous readings” in the James Webb Space Telescope.

During the vibration testing on December 3, at Goddard Space Flight Center in Greenbelt, Maryland, accelerometers attached to the telescope detected anomalous readings during a particular test. Further tests to identify the source of the anomaly are underway. The engineering team investigating the vibe anomaly has made numerous detailed visual inspections of the Webb telescope and has found no visible signs of damage.

It is a good sign that they have found no damage. It is also a good thing that they detected these issues now, on the ground, where they can fix them. Webb, almost a decade behind schedule and $8 billion over budget, will be placed at a point a million miles from Earth, where no repair crew will be able to reach it.

Betelgeuse might have eaten a star

Because the red giant star Betelgeuse rotates far faster than it should, astronomers are now theorizing that when it expanded into its present red giant phase about 100,000 years ago it swallowed a companion star which contributed its own angular momentum to the system to speed up the rotation.

This theory is bolstered by evidence of a shell of matter surrounding Betelgeuse that is possibly a remnant of that destroyed star.

Flying over Occator Crater on Ceres

Cool movie time! Using data from Dawn the German Aerospace Center (DLR) has produced a short animation that gives a 3D flyover of Occator Crater on Ceres.

The animated flyover includes topographic and enhanced-color views of the crater, highlighting the central dome feature. The central area has been named Cerealia Facula. Occator’s secondary group of bright spots is called Vinalia Faculae.

The movie is definitely worth watching, especially the sections that show in close-up the bright areas near the crater’s center.

Lots of ice on Ceres

New data from Dawn now suggests that Ceres contains a large amount of ice on or near its surface.

“On Ceres, ice is not just localized to a few craters. It’s everywhere, and nearer to the surface with higher latitudes,” said Thomas Prettyman, principal investigator of Dawn’s gamma ray and neutron detector (GRaND), based at the Planetary Science Institute, Tucson, Arizona. Researchers used the GRaND instrument to determine the concentrations of hydrogen, iron and potassium in the uppermost yard (or meter) of Ceres. GRaND measures the number and energy of gamma rays and neutrons coming from Ceres. Neutrons are produced as galactic cosmic rays interact with Ceres’ surface. Some neutrons get absorbed into the surface, while others escape. Since hydrogen slows down neutrons, it is associated with a fewer neutrons escaping. On Ceres, hydrogen is likely to be in the form of frozen water (which is made of two hydrogen atoms and one oxygen atom).

Rather than a solid ice layer, there is likely to be a porous mixture of rocky materials in which ice fills the pores, researchers found. The GRaND data show that the mixture is about 10 percent ice by weight.

Juno completes third Jupiter flyby

On December 11 Juno successfully completed its third close flyby of Jupiter.

They have released one quite spectacular image taken during the close approach. Expect more to follow soon.

Though they continue to say that they are still considering firing the spacecraft’s main engine to lower and shorten the orbit, I am getting the impression that they are increasingly leaning to leaving things as they are. While this longer orbit will produce larger gaps in their data of the gas giant’s atmosphere (53 days between close approaches versus 14 days), it will also allow them to tract changes over a much longer time period. Considering the risk of a catastrophic failure should they fire the questionable engine, this choice seems quite reasonable.

OSIRIS-REx to search for Earth’s Trojan asteroids

As it heads outward for a rendezvous with the asteroid Bennu, OSIRIS-REx will turn on its instruments for 12 days in February 2017 to hunt for the Trojan asteroids that likely orbit the Sun in the Earth’s orbit 60 degrees ahead and behind it.

Six planets in our solar system are known to harbor Trojan asteroids — Jupiter, Neptune, Mars, Venus, Uranus and Earth. Although more than 6,000 Trojan asteroids are known to be orbiting along with Jupiter, scientists have discovered only one Earth Trojan to date: 2010 TK7, found by NASA’s NEOWISE project in 2010. Scientists predict that there should be more Trojans orbiting Earth, but these asteroids are difficult to detect because they appear close to the sun from Earth’s point of view. In mid-February 2017, however, the OSIRIS-REx spacecraft will be ideally positioned to undertake a survey of the stable point in front of Earth.

Over 12 days, the OSIRIS-REx Earth-Trojan asteroid search will employ the spacecraft’s MapCam imager to methodically scan the space where Earth Trojans are expected to exist. MapCam is part of the OSIRIS-REx Camera Suite, or OCAMS, which was designed and built by researchers at the UA’s Lunar and Planetary Laboratory.

Did a giant black hole eat a star?

New data now suggests that what astronomers had thought was the brightest supernova ever detect might have instead been the ripping apart of a star as it passed too close to a supermassive black hole.

In this scenario, the extreme gravitational forces of a supermassive black hole, located in the centre of the host galaxy, ripped apart a Sun-like star that wandered too close — a so-called tidal disruption event, something so far only observed about 10 times. In the process, the star was “spaghettified” and shocks in the colliding debris as well as heat generated in accretion led to a burst of light. This gave the event the appearance of a very bright supernova explosion, even though the star would not have become a supernova on its own as it did not have enough mass. The team based their new conclusions on observations from a selection of telescopes, both on the ground and in space. Among them was the NASA/ESA Hubble Space Telescope, the Very Large Telescope at ESO’s Paranal Observatory and the New Technology Telescope at ESO’s La Silla Observatory

Curiosity cleared to move but not drill

Engineers have cleared Curiosity to move once again, but have not yet cleared the rover to use its balky drill.

This morning we received downlink that indicated operation of the drill feed using standard commands. This is great news, and the anomaly response team has cleared the rover for use of the arm and driving (but not yet drilling).

It is not known when they will drill again, but the news suggests that they will do so eventually, once they get a full understanding of what prevented normal operations this last time. For moment, at least, they no longer have a need to keep the rover motionless so they could assess the situation.

First dinosaur tail found, preserved in amber

Paleontologists have discovered the first completely preserved dinosaur tail, feathers and all, preserved in amber.

Inside the lump of resin is a 1.4-inch appendage covered in delicate feathers, described as chestnut brown with a pale or white underside. CT scans and microscopic analysis of the sample revealed eight vertebrae from the middle or end of a long, thin tail that may have been originally made up of more than 25 vertebrae. Based on the structure of the tail, researchers believe it belongs to a juvenile coelurosaur, part of a group of theropod dinosaurs that includes everything from tyrannosaurs to modern birds.

Juno’s upcoming December 11 Jupiter flyby

The Juno science team prepares for the next close flyby of Jupiter on December 11.

At the time of closest approach (called perijove), Juno will be about 2,580 miles (4,150 kilometers) above the gas giant’s roiling cloud tops and traveling at a speed of about 129,000 mph (57.8 kilometers per second) relative to the planet. Seven of Juno’s eight science instruments will be energized and collecting data during the flyby. “This will be the first time we are planning to operate the full Juno capability to investigate Jupiter’s interior structure via its gravity field,” said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio. “We are looking forward to what Jupiter’s gravity may reveal about the gas giant’s past and its future.”

Mission managers have decided not to collect data with the Jovian Infrared Auroral Mapper (JIRAM) instrument during the December flyby, to allow the team to complete an update to the spacecraft software that processes JIRAM’s science data. A software patch allowing JIRAM’s operation is expected to be available prior to the next perijove pass (PJ4) on Feb. 2, 2017.

It increasingly appears they do not want to risk firing the spacecraft’s main engine to shorten the 53 day orbit to 14 days because of a fear that the burn could fail catastrophically. This means that Juno’s mission will be extended significantly because it will take longer to gather data with such a long orbit.

Jupiter’s chaotic storms

Jupiter's storms, as seen by Juno after processing

Cool image time! The image on the right shows what anyone can do if they want to play with images that have been taken by the Juno spacecraft. On top is the raw Juno image of a storm on Jupiter. On the bottom is that same storm after significant processing by an ordinary citizen. A larger version can be seen here.

While the Juno science team’s policy of making all their raw images available to the public is routine for a NASA mission, they are doing something a bit different by allowing the public to play with the images and then upload them on a Juno website for everyone to see. While some of the subsequent images have been a little silly, the image on the right illustrates how this policy can help scientists (and the public) better study the atmosphere on Jupiter. The processing has brought out all the storm’s swirls and twirls, and shown clearly how chaotic the storms are in Jupiter’s high latitudes.

The scientists don’t have the resources or the time to do this kind of processing on every image, or even every piece of every image. Allowing the public to do it will increase the variety of results and make it more likely for everyone to gain some understanding of what is going on in the gas giant’s atmosphere. Or not, but then that’s okay, as a realization that we don’t understand something is the first step towards wisdom and real knowledge.

Mars rover update: December 8, 2016

Curiosity

Mars' dusty sky

For the overall context of Curiosity’s travels, see Pinpointing Curiosity’s location in Gale Crater.

Since my last rover update on November 14th, Curiosity moved relatively little. They drove a short distance to the southeast to a point where they wanted to drill, but have not moved from this location for the past two weeks because of drill issues.

While the engineers study the drill problem, which requires them to not move either the rover or the drill arm, the scientists have still used Curiosity to take images of the dust in the sky, to take hourly images of the dust on the ground (to see how it is changed by the wind), and to take images of nearby interesting nearby features (below the fold).
» Read more

Two new studies say different things about Greenland’s icecap history

The uncertainty of science: Two new studies of Greenland’s icecap suggest completely opposite histories, with one saying that Greenland was ice free at least once in the past 2.6 million years, with the other saying that the icecap covered Greenland continuously for the past 7.5 million years.

Evidence buried in Greenland’s bedrock shows the island’s massive ice sheet melted nearly completely at least once in the last 2.6 million years. This suggests that Greenland’s ice may be less stable than previously believed. “Our study puts Greenland back on the endangered ice-sheet map,” says Joerg Schaefer, a palaeoclimatologist at the Lamont-Doherty Earth Observatory in Palisades, New York, and co-author of a paper published on 7 December in Nature.

A second paper in the same issue paints a slightly different view of the ice sheet’s past stability. A group led by Paul Bierman, a geomorphologist at the University of Vermont in Burlington, found that ice covered eastern Greenland for all of the past 7.5 million years. Experts say the two papers do not necessarily contradict one another: at times, nearly all of Greenland’s ice could have melted (as seen by Schaefer’s team) while a frosty cap remained in the eastern highlands (as seen by Bierman’s group).

If all of Greenland’s ice melted, it would raise sea levels by seven metres. Models suggest that Greenland could become ice-free as soon as 2,500 years from now, depending on the concentration of greenhouse gases in the atmosphere. [emphasis mine]

This story is a perfect example of how the passionate belief in a theory (that global warming is happening, is a threat, and will melt the icecaps) can warp a scientist’s thinking. Both studies used a single drilled ice core, with the first from Greenland’s central region and the second from Greenland’s eastern region. Thus, there is no reason to say that the entire Greenland icecap had melted, as noted in the highlighted text that describes the first study. What the data merely suggests is that these two regions might have had different histories.

Instead, the article, in its effort to confirm the possibility that Greenland’s icecap could melt entirely and thus pose a threat of a big sea level rise, ignores this simple detail and struggles to justify the concept that the entire cap certainly melted in the past, even though one study suggests otherwise. This causes everyone to misunderstand the results, and draw conclusions that are uncalled for, based on the available data.

Design flaw in India’s Mars Orbiter

According to American researchers, a fundamental design flaw in the primary scientific instrument on India’s Mangalyaan Mars orbiter prevents it from carrying out its mission of measuring the methane in the Martian atmosphere.

“They did not design this properly for the detection of methane on Mars,” Michael Mumma, senior scientist at NASA’s Goddard Space Flight Center, told Seeker. In 2003, Mumma led a team that made the first definitive measurements of methane on Mars using an infrared telescope in Hawaii. The methane, which appeared in plumes over specific regions of Mars, reached a maximum density of about 60 parts per billion. “The (MOM) instrument is beautifully engineered, but not for the methane task. It has other value, but unfortunately they will not be able to provide measurements of methane at the levels needed to sample even the plumes we saw,” Mumma said.

They are re-purposing the instrument to measure the reflected sunlight coming off the Martian surface, useful data to be sure but hardly worth an entire space mission.

The weird south pole of Mars

Mars' south pole region

Cool image time (literally)! The photo above, cropped slightly to show here, was taken by Mars Reconnaissance Orbit (MRO) in August 2016 and was released today as part of the monthly release of captioned images. And though it looks like a fractal computer-generated animation still, it is instead real, showing the strange and quite alien terrain that routinely forms at the carbon dioxide ice cap there.

The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this this coolest landscape on Earth and Mars combined!

This region is about 4 degrees north of the south pole itself.

ExoMars’ Trace Gas Orbiter images Phobos

As part of its checkout, Europe’s ExoMars’ Trace Gas Orbiter has taken test images of the Martian moon Phobos.

The camera imaged the moon on 26 November from a distance of 7700 km, during the closest part of the spacecraft’s orbit around Mars. TGO’s elliptical orbit currently takes it to within 230–310 km of the surface at its closest point and around 98 000 km at its furthest every 4.2 days. A colour composite has been created from several individual images taken through several filters. The camera’s filters are optimised to reveal differences in mineralogical composition, seen as ‘bluer’ or ‘redder’ colours in the processed image. An anaglyph created from a stereo pair of images captured is also presented, and can be viewed using red–blue 3D glasses.

The images were done to test the spacecraft’s operation, and have apparently shown that it is functioning well.

First images from Cassini’s first Saturn ring flyby

Saturn's polar vortex

Cool image time! And this is only the start. The Cassini science team has released the first images taken by Cassini during its first of 42 close flybys of the rings of Saturn. The image on the right, cropped from the full image, shows Saturn’s north polar vortex. The storm at the polar really does look like a whirlpool that is descending down into the gas giant’s depth.

I must emphasize that photography was not the focus of this first flyby. These images were taken the two days before the flyby on December 4. Later flybys are going to produce far better images, as they will be taking pictures throughout.

Sunspot activity continues to drop

NOAA yesterday posted its monthly update of the solar cycle, covering sunspot activity for November. Below is my monthly annotated version of that update.

November 2016 Solar Cycle graph

The graph above has been modified to show the predictions of the solar science community. The green curves show the community’s two original predictions from April 2007, with half the scientists predicting a very strong maximum and half predicting a weak one. The red curve is their revised May 2009 prediction.

In November sunspot activity dropped again, to the second lowest point seen since 2010. Essentially, activity today is about where it was in 2010 when the solar minimum was finally ending. Now, the solar maximum is ending and we are beginning the next solar minimum.

Throughout the entire just completed solar maximum, the Sun continuously under-performed all predictions. Even now, despite following almost precisely the prediction of the 2007 low prediction during 2014 and 2015, in 2016 the ramp down has begun to slip below that prediction. The trend continues to suggest the arrival of solar minimum will be early, possibly as early as sometime late next year.

Drill issues at Curiosity

The recent failure by Curiosity to drill has caused engineers to stop the rover in its tracks while they analyze the cause of the problem.

The rover team learned Dec. 1 that Curiosity did not complete the commands for drilling. The rover detected a fault in an early step in which the “drill feed” mechanism did not extend the drill to touch the rock target with the bit. “We are in the process of defining a set of diagnostic tests to carefully assess the drill feed mechanism. We are using our test rover here on Earth to try out these tests before we run them on Mars,” Curiosity Deputy Project Manager Steven Lee, at NASA’s Jet Propulsion Laboratory in Pasadena, California, said Monday. “To be cautious, until we run the tests on Curiosity, we want to restrict any dynamic changes that could affect the diagnosis. That means not moving the arm and not driving, which could shake it.”

Two among the set of possible causes being assessed are that a brake on the drill feed mechanism did not disengage fully or that an electronic encoder for the mechanism’s motor did not function as expected. Lee said that workarounds may exist for both of those scenarios, but the first step is to identify why the motor did not operate properly last week.

Though they do not say so, the problem is almost certainly related to a fundamental design flaw in the drill’s design that causes intermittent short-circuits when they use it, and has the possibility of shorting out the entire rover if they are not careful.

Cassini makes its first close ring flyby of Saturn

Cassini has begun its last year at Saturn, making its first close fly-by of the gas giant’s rings yesterday.

Cassini’s imaging cameras obtained views of Saturn about two days before crossing through the ring plane, but not near the time of closest approach. The focus of this first close pass was the engine maneuver and observations by Cassini’s other science instruments. Future dives past the rings will feature some of the mission’s best views of the outer regions of the rings and small, nearby moons.

Each of Cassini’s orbits for the remainder of the mission will last one week. The next pass by the rings’ outer edges is planned for Dec. 11. The ring-grazing orbits — 20 in all — will continue until April 22, when the last close flyby of Saturn’s moon Titan will reshape Cassini’s flight path. With that encounter, Cassini will leap over the rings, making the first of 22 plunges through the 1,500-mile-wide (2,400-kilometer) gap between Saturn and its innermost ring on April 26.

On Sept. 15, the mission will conclude with a final plunge into Saturn’s atmosphere. During the plunge, Cassini will transmit data on the atmosphere’s composition until its signal is lost.

Now for a bit of reality: When Cassini’s mission ends on September 15, 2017, it will likely be a minimum of 20 years before another spacecraft returns.

The beginning of Cassini’s final year at Saturn

Link here. The article does a nice job of outlining, with videos, what will happen as the spacecraft makes multiple dives inside rings.

Cassini’s final acts, which will play out over the next year. That pass placed Cassini in a high-inclination orbit tilted 60° relative to the ring plane. Cassini will perform 20 passes just 620 miles (1000 kilometers) outside the F ring of Saturn in a phase known as the Ring-Grazing Orbits, which runs from late November 2016 through April 2017.

Cassini already reached apoapse, or its farthest point from Saturn, on Wednesday, November 30th. The first ring crossing is coming right up this weekend on Sunday, December 4th, at 7:09 a.m. EST / 13:09 UT. During the first periapse pass on Sunday, Cassini will also burn its main engine for the 183rd and final time for the mission. All later fine course corrections will be made using thrusters only.

Things get even more interesting after April, when the series of Grand Finale Orbits will begin, taking the spacecraft through the 1240-mile-wide (2000-kilometer-wide) gap between the planet’s cloud tops and rings for 22 final orbits. The Grand Finale Orbits start with the spacecraft’s 126th and final pass near Titan, which will set the spacecraft up for much tighter final orbits.

ESA approves ExoMars 2020 funding

Despite the failure of the Schiaparelli lander on ExoMars 2016, the European Space Agency today approved funds to build and fly the ExoMars 2020 rover mission.

At a meeting of European government ministers in Lucerne, Switzerland, on 1 and 2 December, ESA member states agreed to provide an extra €339 million for ExoMars 2020. ESA also announced that it will find a further €97 million by moving funds internally. Speaking at a press briefing after the meeting, ESA director-general Jan Wörner said this would be done “without detriment” to ESA’s wider science budget.

But not all projects were so fortunate. Member states did not commit the €250 million needed to fund a plan for ESA to participate in a mission to deflect the moon of an asteroid, although they left door open to future, similar projects.

I am not at present sure how they are going to divide up the work between Europe and Russia. Earlier it was my understanding that Russia would provide the roving technology, but right now I am very unsure about this.

One side note: At this same meeting ESA committed to sticking with ISS through 2024.

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