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DuckDuckGo, a privacy-focused tech company, today launched something called Tracker Radar—an open-source, automatically generated and continually updated list that currently contains more than 5,000 domains that more than 1,700 companies use to track people online.
The idea behind Tracker Radar, first reported by CNET, is to share the data DuckDuckGo has collected to create a better set of tracker blockers. DuckDuckGo says that the majority of existing tracker data falls into two types: block lists and in-browser tracker identification. The issue is the former relies on crowd-sourcing and manual maintenance. The latter is difficult to scale and also can be potentially abused due to the fact it's generating a list based on your actual browsing habits. Tracker Radar supposedly gets around some of these issues by looking at the most common cross-site trackers and including a host of information about their behavior, things like prevalence, fingerprinting, cookies, and privacy policies, among other considerations.
See DuckDuckGo's Tracker Radar GitHub page for the list and other tools.
Obligatory alt-aristarchus comment: If it walks like a duckduckgo, and it quacks like a duckduckgo, it's got privacy like a duckduckgo! Thanks, Google!
Proposed US law is "Trojan horse" to stop online encryption, critics say:
Two Republicans and two Democrats in the US Senate have proposed a law that aims to combat sexual exploitation of children online, but critics of the bill call it a "Trojan horse" that could harm Americans' security by reducing access to encryption. The EARN IT (Eliminating Abusive and Rampant Neglect of Interactive Technologies) Act "would create incentives for companies to 'earn' liability protection for violations of laws related to online child sexual abuse material," an announcement by the bill's supporters said today.
Under current law, Section 230 of the Communications Decency Act provides website operators broad legal immunity for hosting third-party content. A 2018 law known as FOSTA-SESTA chipped away at that immunity for content related to prostitution and sex trafficking, and the EARN IT Act would further weaken immunity for website operators who fail to take certain to-be-determined measures to find and remove child sexual-abuse material.
In a related development today, US Attorney General William Barr gave a speech calling for an analysis of how Section 230 affects "incentives for platforms to address [child sexual exploitation] crimes and the availability of civil remedies to the victims."
[...] Stewart Baker, who was formerly assistant secretary for policy at the Department of Homeland Security and general counsel at the National Security Agency, wrote in a blog post that "there is nothing radical" about the bill. "The risk of liability isn't likely to kill encryption or end Internet security," Baker wrote. But Baker acknowledged that the bill will likely make the decision to offer encryption a more difficult one for tech companies
Related:
U.S. Congress Passes SESTA/FOSTA Law
DoJ Lets Cops Know SESTA/FOSTA Is For Shutting Down Websites, Not Busting Sex Traffickers
Crypto Wars: US AG William Barr and UK Home Secretary Priti Patel Shake Fists at Facebook
Senate Judiciary Committee Interrogates Apple, Facebook about Crypto
Caffeine boosts problem-solving ability but not creativity, study indicates:
"In Western cultures, caffeine is stereotypically associated with creative occupations and lifestyles, from writers and their coffee to programmers and their energy drinks, and there's more than a kernel of truth to these stereotypes," wrote Darya Zabelina, assistant professor of psychology and first author of the study recently published in the journal Consciousness and Cognition.
While the cognitive benefits of caffeine -- increased alertness, improved vigilance, enhanced focus and improved motor performance -- are well established, she said, the stimulant's affect on creativity is less known.
In the paper, Zabelina differentiates "convergent" from "divergent" thinking. The former is defined as seeking a specific solution to a problem, for example, the "correct" answer. The latter is characterized by idea generation where a large set of apt, novel or interesting responses would be suitable. Caffeine was shown to improve convergent thinking in the study, while consuming it had no significant impact on divergent thinking.
Journal Reference:
Darya L. Zabelina, Paul J. Silvia. Percolating ideas: The effects of caffeine on creative thinking and problem solving. Consciousness and Cognition, 2020; 79: 102899 DOI: 10.1016/j.concog.2020.102899
I wonder if she drank coffee to help her come up with that conclusion?
The Australian government is investigating implementing age verification to access porn online following a failed UK age verification scheme. Children's charity eChildhood claims that "a third of students aged eight and under attempted to access online pornography in the past six months" including through advertising popups. No mention has been made about how effective the Australian plan will be and what exact measures may be taken to block access online.
The UK proposed making users visiting porn sites prove they were 18. The government abandoned the plan in October after a series of major technical issues.
The Australian report said three "crucial factors" needed to be sorted out to succeed where the UK scheme failed.
These included ensuring a level playing field for regulation, making age verification easy for consumers to use and raising public awareness of the need for age verification.
[...]Advocacy group Collective Shout said UK research found 28 per cent [of] children aged 11 to 12 had seen pornography online. In the 15 to 16 age group, the number jumped to 65 per cent.
The Internet routes around damage.
Surprise! Students get an unexpected glimpse of a black hole 30,000 light-years away:
Peering into deep space with an instrument they built, a group of students and researchers caught a surprising glimpse of a newly discovered black hole 30,000 light-years from Earth.
In the fall of 2019, students and researchers from the Massachusetts Institute of Technology and Harvard University were working with an instrument that they designed and now operate, the Regolith X-Ray Imaging Spectrometer (REXIS), which is on board NASA's OSIRIS-REx spacecraft. While using the shoebox-size instrument to observe the asteroid Bennu, the spacecraft's destination, the team made an unexpected detection: a new black hole in the constellation Columba.
REXIS measures X-rays that are emitted from objects like Bennu in response to solar radiation. On Nov. 11, 2019, the collaborative group of researchers and students spotted X-rays radiating from a point off the edge of Bennu.
[...] Upon further analysis, the team found that the X-rays seen off the edge of Bennu were coming from a newly flaring black hole X-ray binary. The black hole, known as MAXI J0637-430, was discovered just a week before these observations by researchers using Japan's MAXI telescope, which operates from aboard the International Space Station. The X-rays were also detected by NASA's Neutron Star Interior Composition Explorer (NICER) telescope, which is also on the space station. Although both telescopes were able to detect the X-rays from low Earth orbit, REXIS detected the event while millions of miles from Earth. This observation marks the first time that such an outburst has been detected from interplanetary space, according to the statement.
Methane emitted by humans vastly underestimated:
University of Rochester researchers Benjamin Hmiel, a postdoctoral associate in the lab of Vasilii Petrenko, a professor of earth and environmental sciences, and their collaborators, measured methane levels in ancient air samples and found that scientists have been vastly underestimating the amount of methane humans are emitting into the atmosphere via fossil fuels. In a paper published in Nature, the researchers indicate that reducing fossil fuel use is a key target in curbing climate change.
[...] Methane is the second largest anthropogenic -- originating from human activity -- contributor to global warming, after carbon dioxide. But, compared to carbon dioxide, as well as other heat-trapping gases, methane has a relatively short shelf-life; it lasts an average of only nine years in the atmosphere, while carbon dioxide, for instance, can persist in the atmosphere for about a century. That makes methane an especially suitable target for curbing emission levels in a short time frame.
"If we stopped emitting all carbon dioxide today, high carbon dioxide levels in the atmosphere would still persist for a long time," Hmiel says. "Methane is important to study because if we make changes to our current methane emissions, it's going to reflect more quickly."
[...] In order to more accurately separate the natural and anthropogenic components, Hmiel and his colleagues turned to the past, by drilling and collecting ice cores from Greenland. The ice core samples act like time capsules: they contain air bubbles with small quantities of ancient air trapped inside. The researchers use a melting chamber to extract the ancient air from the bubbles and then study its chemical composition.
Hmiel's research focused on measuring the composition of air from the early 18th century -- before the start of the Industrial Revolution -- to the present day. Humans did not begin using fossil fuels in significant amounts until the mid-19th century. Measuring emission levels before this time period allows researchers to identify the natural emissions absent the emissions from fossil fuels that are present in today's atmosphere. There is no evidence to suggest natural fossil methane emissions can vary over the course of a few centuries.
[...] By measuring the carbon-14 isotopes in air from more than 200 years ago, the researchers found that almost all of the methane emitted to the atmosphere was biological in nature until about 1870. That's when the fossil component began to rise rapidly. The timing coincides with a sharp increase in the use of fossil fuels.
The levels of naturally released fossil methane are about 10 times lower than previous research reported. Given the total fossil emissions measured in the atmosphere today, Hmiel and his colleagues deduce that the manmade fossil component is higher than expected -- 25-40 percent higher, they found.
I have a couple things to bring to the attention of the community concerning site funding and comment moderations. As always, if you are not interested in these matters, feel free to skip past this one; another story will be along shortly. Otherwise read beyond the fold for an update.
Finances:
A recent comment to a journal article about SoylentNews now having a privacy policy prompted me to pursue something that had been nagging at me for a long while.
In short, I have learned it costs more to run this site than I had estimated. We have actually been operating at a loss for the past couple years. I have, therefore, provided a revised fundraising goal of $3500.00 for the first half of this calendar year in the "Site News" slashbox (that appears on the right-hand-side of the main page).
I have been advised our current funds on hand can support the site for just six months.
For those who have been around for a while, it will come as no surprise to learn that I try to keep a handle on subscription income for this site. Further, I have been maintaining what we affectionately refer to here as the "Beg-O-Meter' that appears in the "Site News" slashbox. It provides a running tally of our financial goal for the period and how far along we are towards attaining that goal. Lastly, I have posted stories in the past apprising the community as to our progress towards those goals.
We are an entirely volunteer organization (no staff member has ever been paid anything for their work on SoylentNews). All funding for the site comes entirely from the community (we have never run advertisements and are strongly resistant to any suggestion to do so). The vast majority of our funding comes from subscriptions.
My prior estimates of $4000.00 per year were based on the only information I had available at that time. Our monthly web hosting costs ($260/month), the fact that we needed to file and pay taxes, and that we paid an accountant to prepare them. Twelve months at $260/month works out to $2160 per year. I reasoned a goal of $3000 for the year would give us about $840 for those other expenses... that should do it, right?
Apparently not.
Thanks to the above-referenced comment, I reached out to a member of our board of directors and inquired as to our financial status. In very short order I received a pile of PDF files. A separate file for each fiscal year's Profit and Loss Statement and a separate file for each year's Balance Sheet. It took a surprising amount of effort, but thanks to the concerted effort of a few staff members, these have been uploaded to our Wiki and can now be accessed through the SoylentNews Finance page.
A couple things bear explanation. You may notice that there are expenses associated with subscriptions. The amount of a subscription made to SoylentNews is a gross amount. From that, Stripe or PayPal charge a processing fee for each subscription. These fees do add up and amount to the aforementioned expense.
Also, why is a Delaware company paying Massachusetts state taxes? I reached out for an answer from a board member, and here is his reply:
We pay Massachusetts income tax (since we are not profitable, we pay the minimum amount of $456 each year, but if we ever become profitable, we will have to pay more) because we are physically located in MA (through me). A physical address was required to open our checking account with BoA[*], and for various other things. For example, we need a physical address to sign the engagement letter with our accountant every year. Note that we are not required to pay Delaware income tax because we are not physically located in DE. The tax that we pay to Delaware each year is technically a franchise tax that we pay for the privilege of being incorporated in Delaware (allowing us to be a Public Benefit Corporation, among other benefits).
[*] BoA - Bank of America.
I will keep the community appraised should I learn anything more.
Moderations:
We had had a discussion on the site a few months ago about moderation on the site. I have been pursuing a possible implementation of one of the suggestions raised there: adding a "-1 Ad Hominem" moderation. Discussion among staff has suggested we would need a counter moderation should a "-1 Ad Hominem" be perceived to have been in error. That wold mean the addition of a "+1 Not Ad Hominem" moderation, too. (In proper geek fashion, they nicely abbreviate to: "-1 AH" and "+1 NAH"!) There is more to its implementation than just adding these options to the moderation table; coding changes would also be needed. This, in turn, would require the modifications be submitted through GitHub as a pull request, then testing, and finally a rollout to the community. It is important to note that this would be on a trial basis! If it proves to NOT be workable, we need to be able to roll that back. This is easier said than done! The previous moderations will need to remain in the system (what's done is done) but future moderations must be able to be blocked... and the code is not designed for this at all.
It bears mentioning that our goal is to provide a forum for the community to comment on stories and to moderate those comments. We strive to be as hands-off about these matters as we reasonably can.
In short, this is mostly an announcement that AH moderations have not been forgotten, design work is in progress, and that when time and developer availability permits, we hope to be rolling this out for a test run. I would not expect anything to happen in the next month, but wanted to provide as much advance notice as to the intention as possible so as to encourage any feedback, discussion, etc. that could help inform our implementation.
<Note class="TMB">
s/next month/next few months/
Contractor woes (just because I technically can do everything doesn't mean it's always the wisest idea) wound up pushing move-in date on the church I've been remodeling back a couple months (end of April is what we're currently shooting for as a best case scenario) and I don't want anything hitting production servers that hasn't had at least two weeks worth of testing on our dev server after me calling it done, because I'm quite often wrong about that. The end of May is the soonest anything is likely to hit production servers, with some time in June being far more likely.
</Note>
The force is strong in neutron stars:
[...] physicists at MIT and elsewhere have for the first time characterized the strong nuclear force, and the interactions between protons and neutrons, at extremely short distances.
[...] "This is the first very detailed look at what happens to the strong nuclear force at very short distances," says Or Hen, assistant professor of physicist at MIT. "This has huge implications, primarily for neutron stars and also for the understanding of nuclear systems as a whole."
[...] Ultra-short-distance interactions between protons and neutrons are rare in most atomic nuclei. Detecting them requires pummeling atoms with a huge number of extremely high-energy electrons, a fraction of which might have a chance of kicking out a pair of nucleons (protons or neutrons) moving at high momentum -- an indication that the particles must be interacting at extremely short distances.
"To do these experiments, you need insanely high-current particle accelerators," Hen says. "It's only recently where we have the detector capability, and understand the processes well enough to do this type of work."
Hen and his colleagues looked for the interactions by mining data previously collected by CLAS[*], a house-sized particle detector at Jefferson Laboratory; the JLab accelerator produces unprecedently high intensity and high-energy beams of electrons. The CLAS detector was operational from 1988 to 2012, and the results of those experiments have since been available for researchers to look through for other phenomena buried in the data.
In their new study, the researchers analyzed a trove of data, amounting to some quadrillion electrons hitting atomic nuclei in the CLAS detector. The electron beam was aimed at foils made from carbon, lead, aluminum, and iron, each with atoms of varying ratios of protons to neutrons. When an electron collides with a proton or neutron in an atom, the energy at which it scatters away is proportional to the energy and momentum of the corresponding nucleon.
[...] With this general approach, the team looked through the quadrillion electron collisions and managed to isolate and calculate the momentum of several hundred pairs of high-momentum nucleons. Hen likens these pairs to "neutron star droplets," as their momentum, and their inferred distance between each other, is similar to the extremely dense conditions in the core of a neutron star.
They treated each isolated pair as a "snapshot" and organized the several hundred snapshots along a momentum distribution. At the low end of this distribution, they observed a suppression of proton-proton pairs, indicating that the strong nuclear force acts mostly to attract protons to neutrons at intermediate high-momentum, and short distances.
Further along the distribution, they observed a transition: There appeared to be more proton-proton and, by symmetry, neutron-neutron pairs, suggesting that, at higher momentum, or increasingly short distances, the strong nuclear force acts not just on protons and neutrons, but also on protons and protons and neutrons and neutrons. This pairing force is understood to be repulsive in nature, meaning that at short distances, neutrons interact by strongly repelling each other.
[...] "People assumed that the system is so dense that it should be considered as a soup of quarks and gluons," Hen explains. "But we find even at the highest densities, we can describe these interactions using protons and neutrons; they seem to keep their identities and don't turn into this bag of quarks. So the cores of neutron stars could be much simpler than people thought. That's a huge surprise."
[*] CLAS: CEBAF Large Acceptance Spectrometer.
CEBAF: Continuous Electron Beam Accelerator Facility.
Journal Reference:
A. Schmidt, et al. Probing the core of the strong nuclear interaction. Nature, 2020; 578 (7796): 540 DOI: 10.1038/s41586-020-2021-6
Arthur T Knackerbracket has found the following story:
ARM CPU vendor Ampere announced an 80-core CPU called the Altra on Tuesday. If the core count didn't clue you in already, the Altra is aimed at data-center computing rather than home or even typical business needs. The Altra's 80 cores do not offer hyperthreading, so 80 cores here means 80 threads as well.
Before we go into too much detail about the Altra—which is currently sampling but is not yet generally available and does not have any third-party benchmarks—it's instructive to take a look slightly backward to its little sibling, the 32-core eMAG 8180.
The Altra is not Ampere's first entry into data-center ARM computing. Its last processor, the eMAG 8180, is a 32-core part running at up to 3.3GHz turbo. The eMAG 8180 is available in packet.net's c2.large.arm package, in the form of Lenovo's ThinkSystem HR330A 1u single-socket systems.
Kinvolk, a Berlin-based Linux development company, did some pretty extensive benchmarking of a single-socket eMAG 8180 system—comparing it to a 24-core AMD Epyc 7401P (24c/48t) and a dual-socket Xeon Gold 5120 (28c/56t total).
[...] Like the eMAG, the Altra does not offer SMT (Simultaneous Multi Threading), so its 80 cores mean 80 threads. Unlike the eMAG, the Altra is designed for either single or dual-socket operation—so we can expect to see 160-core Altra-powered systems later in 2020. We know that there will be multiple SKUs, with a TDP range the data sheet specifies at 45W to 210W. But we don't know their individual details.
The fine print in Altra's slide deck claims 80 cores and 180W for the Altra under test, not 210W. This may imply adjustable thermal performance configurations similar to what one might see in laptop CPUs, but at this point it's just too soon to tell. The company claims—presumably, with dual-socket builds of the 80-core SKU—the highest rack density in the industry, at up to 3,500 cores per rack.
It's important to note that these performance numbers are thin at best. Not only are they Ampere-internal, they're "projected," not real. Further, the AMD and Intel performance numbers have been artificially decreased, to account for the fact that the Altra is using binaries compiled with GCC. Meanwhile, the AMD and Intel numbers were generated with CPU-optimized compilers. This drops the Epyc down to 83.5 percent of its real performance and the Xeon down to 76 percent of its.
This isn't sketchy, exactly—it's a fairly common industry practice, and Ampere disclosed it clearly enough in the presentation. But it's likely not what many people would expect. We should point out that the only performance numbers given here are SPECrate 2017_int_base—which is an extremely narrow integer math performance benchmark.
Arthur T Knackerbracket has found the following story:
Organic compounds called thiophenes are found on Earth in coal, crude oil and oddly enough, in white truffles, the mushroom beloved by epicureans and wild pigs.
Thiophenes were also recently discovered on Mars, and Washington State University astrobiologist Dirk Schulze-Makuch thinks their presence would be consistent with the presence of early life on Mars.
Schulze-Makuch and Jacob Heinz with the Technische Universität in Berlin explore some of the possible pathways for thiophenes' origins on the red planet in a new paper published in the journal Astrobiology. Their work suggests that a biological process, most likely involving bacteria rather than a truffle though, may have played a role in the organic compound's existence in the Martian soil.
"We identified several biological pathways for thiophenes that seem more likely than chemical ones, but we still need proof," Dirk Schulze-Makuch said. "If you find thiophenes on Earth, then you would think they are biological, but on Mars, of course, the bar to prove that has to be quite a bit higher."
Thiophene molecules have four carbon atoms and a sulfur atom arranged in a ring, and both carbon and sulfur, are bio-essential elements. Yet Schulze-Makuch and Heinz could not exclude non-biological processes leading to the existence of these compounds on Mars.
Meteor impacts provide one possible abiotic explanation. Thiophenes can also be created through thermochemical sulfate reduction, a process that involves a set of compounds being heated to 248 degrees Fahrenheit (120 degrees Celsius) or more.
In the biological scenario, bacteria, which may have existed more than three billion years ago when Mars was warmer and wetter, could have facilitated a sulfate reduction process that results in thiophenes. There are also other pathways where the thiophenes themselves are broken down by bacteria.
While the Curiosity Rover has provided many clues, it uses techniques that break larger molecules up into components, so scientists can only look at the resulting fragments.
Further evidence should come from the next rover, the Rosalind Franklin, which is expected to launch in July 2020. It will be carrying a Mars Organic Molecule Analyzer, or MOMA, which uses a less destructive analyzing method that will allow for the collection of larger molecules.
Schulze-Makuch and Heinz recommend using the data collected by the next rover to look at carbon and sulfur isotopes. Isotopes are variations of the chemical elements that have different numbers of neutrons than the typical form, resulting in differences in mass.
"Organisms are 'lazy'. They would rather use the light isotope variations of the element because it costs them less energy," he said.
Organisms alter the ratios of heavy and light isotopes in the compounds they produce that are substantially different from the ratios found in their building blocks, which Schulze-Makuch calls "a telltale signal for life."
Yet even if the next rover returns this isotopic evidence, it may still not be enough to prove definitively that there is, or once was, life on Mars.
"As Carl Sagan said 'extraordinary claims require extraordinary evidence,'" Schulze-Makuch said. "I think the proof will really require that we actually send people there, and an astronaut looks through a microscope and sees a moving microbe."
More information: Jacob Heinz et al, Thiophenes on Mars: Biotic or Abiotic Origin?, Astrobiology (2020). DOI: 10.1089/ast.2019.2139
I-Programmer runs a story [0] which says it might not be math chops, but language skills that make a good programmer.
This makes sense, at least to me. I'm a fair coder, and can certainly count, but would not consider my math skills to be high level. As a teenager, C.L. Dogson's Symbolic Logic/Game of Logic [1] was a great read, but wading through formulas and proofs has always made me feel like a 4 year old.
To each his own. For my main "Human" language - English - I'm a pretty good communicator, and that also reflects in the dozen or so coding "dialects" I've kept up with over the years. In basic training I was surprised to test very high at language skills when I absolutely detested spanish in high school (the teacher had something to do with it) and even after living with a German gal for quite some time now have only the rudiments of that language.
This story resonated because I agree with it, coming around to thinking a good thirty years ago that programming is more of a language than a math skill - just not specifically one for a "human" language.
I treat coding like writing a story, itself a variation of the scientific method: 1) first draft, 2 revise, 3 go to 2 until the screen's output matches what's in my head as closely as possible.
So, at least in my case, language skills being much better than math skills result in a fair ability to program.
The folks at Stack Overflow [2] had a long thread on a similar subject some time back. Soylentils, what do you think?
[0] https://www.i-programmer.info/news/99/13517.html
[1] https://en.wikipedia.org/wiki/The_Game_of_Logic
[2] https://stackoverflow.com/questions/157354/is-mathematics-necessary-for-programming
Anthony Levandowski ordered to pay $179 million to Google:
Anthony Levandowski, the engineer and autonomous vehicle startup founder who was at the center of a trade secrets lawsuit between Uber and Waymo, has been ordered to pay $179 million to end a contract dispute over his departure from Google.
Reuters was the first to report the court order.
An arbitration panel ruled in December that Levandowski [...] had engaged in unfair competition and breached [his] contract with Google when [he] left the company to start a rival autonomous vehicle company focused on trucking, called Otto. Uber acquired Otto in 2017. A San Francisco County court confirmed Wednesday the panel's decision.
[...] Levandowski, had disputed the ruling. The San Francisco County Superior Court denied his petition today, granting Google's petition to hold Levandowski to the arbitration agreement under which he was liable.
[...] Levandowski personally filed today for Chapter 11 bankruptcy, stating that the presumptive $179M debt quite exceeds his assets, which he estimates at somewhere between $50M and $100M.
TSMC & Broadcom Develop 1,700 mm2 CoWoS Interposer: 2X Larger Than Reticles
TSMC and Broadcom have also been playing with the idea of oversized chips, and this week they've announced their plans to develop a supersized interposer to be used in Chip-on-Wafer-on-Substrate (CoWoS) packaging.
Overall, the proposed 1,700 mm² interposer is twice the size of TSMC's 858 mm² reticle limit. Of course, TSMC can't actually produce a single interposer this large all in one shot – that's what the reticle limit is all about – so instead the company is essentially stitching together multiple interposers, building them next to each other on a single wafer and then connecting them. The net result is that an oversized interposer can be made to function without violating reticle limits.
The new CoWoS platform will initially be used for a new processor from Broadcom for the HPC market, and will be made using TSMC's EUV-based 5 nm (N5) process technology. This system-in-package product features 'multiple' SoC dies as well as six HBM2 stacks with a total capacity of 96 GB. According to Broadcom's press release, the chip will have a total bandwidth of up to 2.7 TB/s, which is in line with what Samsung's latest HBM2E chips can offer.
Also at Guru3D.
Previously: TSMC Shows Off Gigantic Silicon Interposer
It is time for a quiz slightly biased toward older, larger systems giving old farts an unfair advantage.
Remember: googling the answers is cheating but we have no way of enforcing it. But it is less fun.
1. What is the advantage of unidirectional printing on a dot-matrix printer?
2. What is the distance between the black marks on a thick yellow ethernet cable (10BASE5)?
3. Which CPU did the SuperMAX from DDE have? (trick question)
4. How do you exit from a DOS program (interrupt number + subfunction)
5. Which interactive game from 1986 had the settings tame..lewd, and a scratch'n'sniff card was in the box?
6. Why is a memory dump called a "core" dump?
7. Which CPU did the Siemens PC-D have?
8. Which new features were in the file system in DOS 2.x when compared to DOS 1.x ?
9. What is the visual administration tool in AIX called?
10. Name the file server in the Amoeba OS.
11. What is the biggest difference between C64 joysticks and PC-joysticks (we are talking about the original ones that had to connect to a game port)?
12. What is the maximum line length in COBOL? (trick question)
13. Where is the main office of the Sirius Cybernetics Complaints Department located?
14. "eioio" instruction on Power. What does it do?
15. Before Borland introduced their TurboVision, which toolkit was widespread for implementing windows/ISAM-files in Turbo Pascal?
16. Why is the Unix function for creating a file called "creat" and not "create"?
17. When was SMP supported by Windows? And OS/2?
18. Which number did the Fidonet nets have in your country? (bonus point if you remember your matrix address)
19. How do you mark a block in Wordstar?
20. Which came first: Amiga, Norton Commander, or HP Laserjet?
[20200306_005148 UTC; Updated to add:
Please, when posting a reply, bracket your answer in spoiler tags, like so:
<p>My answer to question #n is:</p>
<spoiler>
Write your answer here.
</spoiler>Which, when presented on the site, will look like:
My answer to question #n is:
Write your answer here.
Thank You! --martyb]
WFIRST, proposed for cancellation, is approved for development
NASA has approved a major astrophysics mission to go into the next phase of its development even as the administration seeks once again to cancel it.
NASA announced March 2 that the Wide Field Infrared Survey Telescope (WFIRST) has passed a review known as Key Decision Point C, which confirms development plans for the mission and allows it to move into full-scale hardware production and testing.
That milestone is when the agency also sets a baseline cost and schedule commitment for the mission. NASA said in its statement about the review that the mission would cost $3.2 billion through its launch, a cost cap previously set by NASA. The cost when including five years of science operations, as well as a coronagraph instrument deemed a technology demonstration by NASA, increases to $3.934 billion.
However, NASA did not announce a launch date for the mission because its fiscal year 2021 budget request proposes to cancel WFIRST. "The Administration is not ready to proceed with another multi-billion-dollar telescope until Webb has been successfully launched and deployed," NASA said in its statement, a reference to the James Webb Space Telescope scheduled for launch in March 2021. NASA used the same statement in its 2021 budget request to explain why it sought no funding for the mission.
Wide Field Infrared Survey Telescope (WFIRST).
Previously:
WFIRST Space Observatory Could be Scaled Back Due to Costs
Trump Administration Budget Proposal Would Cancel WFIRST
NASA Gets Money it Didn't Ask for to Fund Second SLS Mobile Launcher; WFIRST Mission Receives Funds
Launch of James Webb Space Telescope Delayed Again, This Time to March 2021, Cost at $9.66 Billion
NASA Administrator at House Hearing: WFIRST Could be Delayed to Help Pay for JWST