Tweet This! :)

Thursday, November 20, 2025

‘Secret Communication System’ truly ahead of its time

@Mark Ollig

Hollywood actress Hedy Lamarr and American composer George Antheil filed a US patent application June 10, 1941, Serial No. 397,412, titled “Secret Communication System.”

Issued as US Patent No. 2,292,387 Aug. 11, 1942, during the height of World War II, their invention described a system designed to make radio communications difficult to discover or decipher.

On the patent, Lamarr was listed as Hedy Kiesler Markey, her legal name at the time, which blended her maiden surname with her married name.

They proposed a frequency-hopping system in which the transmitter and receiver switched in sync among as many as 88 preset frequencies.

This rapid, synchronized hopping, with both ends changing in the same order at the same time, kept their link in step and, in principle, would make the intended torpedo control signals much harder to jam or intercept.

The patent states, “This invention relates broadly to secret communication systems involving the use of carrier waves of different frequencies, and is especially useful in the remote control of dirigible craft, such as torpedoes.”

It continues, “An object of the invention is to provide a method of secret communication which is relatively simple and reliable in operation, but at the same time is difficult to discover or decipher.”

As a child in Vienna, Lamarr’s father taught her about machines, such as streetcars and printing presses, which sparked her technical interest in inventing and solving problems.

While still in her teens, Lamarr studied acting in Vienna and caught the attention of pioneering theater director Max Reinhardt, who helped launch her professional stage and film career.

In 1933, Lamarr married industrialist Fritz Mandl, attending his meetings with scientists and defense experts, where she gained knowledge about weapons and radio technology, including how jamming could disrupt radio connections.

In 1937, just before World War II erupted in Europe, she met Louis B. Mayer in London.

He was the head of Metro-Goldwyn-Mayer (MGM), a Hollywood studio based in Culver City, CA, known for its high-quality films and roster of major stars.

She accepted an MGM contract during the ocean voyage to the United States and then moved to Hollywood to begin her new career under the stage name Hedy Lamarr.

Hedy Lamarr starred in films like “Algiers” (1938), “Ziegfeld Girl” (1941), and “Samson and Delilah” (1949).

During her movie career, she became interested in a specific wartime issue: how to keep enemy forces from jamming the radio signals used to guide Allied radio-controlled torpedoes.

In 1940, while war raged in Europe and the United States had not yet entered the conflict, Lamarr met composer George Antheil at a Hollywood dinner party.

She was quoted as having discussed her discomfort with making money while Europe was in crisis.
Lamarr and Antheil’s later conversations turned to the use of radio control and jamming techniques, which led to a design for protecting radio-guided torpedoes from interference.

As World War II unfolded in Europe, they worked together on a frequency-hopping control method to counter Axis jamming of Allied radio-guided torpedoes.

Antheil, a pioneering composer, explored the idea of syncing several player pianos playing simultaneously via perforated paper rolls during his live performances.

His most famous work, Ballet Mécanique, was originally scored for 16 synchronized player pianos.

That work gave him a practical sense of timing, coordination, and expertise to control multiple machines simultaneously.

He drew on that experience when he helped Lamarr design the patent’s synchronization mechanism for the frequency-hopping system, using as many as 88 preset frequencies, matching the 88 keys on a piano keyboard.

Lamarr and Antheil developed a method to rapidly switch between preset radio frequencies, with only the sender and receiver aware of the pattern.

Their idea used matching perforated paper rolls in both the transmitter and receiver, each programmed with the same hopping sequence, a preset pattern of frequency changes, ensuring both sides remained in step as the radio frequency changed.

As the rolls moved forward together, the connection stayed in sync even as the carrier frequency changed.

This coordinated hopping pattern is often cited as an early analog example of what is now known as spread-spectrum signaling, a concept that later engineers adapted into electronic and digital forms.

The Navy rejected it in 1942 because the paper-roll synchronization mechanism was too cumbersome for a torpedo.

It is also clear to me that the vacuum-tube electronics of that era would have added unnecessary size and complexity to any practical version of their device meant for use inside a torpedo.

Lamarr and Antheil’s patent was granted during World War II, but it wasn’t until transistor technology emerged in the 1950s that their idea became practical for use in compact electronic devices.

In 1957, during the Cold War, as solid-state electronics progressed, engineers at Sylvania explored developing a version of Lamarr and Antheil’s patented system using solid-state transistors.

In the following years, as new technologies matured, the military began implementing spread-spectrum and frequency-hopping techniques.

The development of spread-spectrum and frequency-hopping technologies paved the way for Bluetooth, invented in 1994, which uses frequency-hopping spread spectrum (FHSS) in the 2.4 gigahertz band to reduce interference.

The Global Positioning System (GPS), which became fully operational in the mid-1990s, also uses direct-sequence spread spectrum (DSSS) for improved signal reception.

The first Wi-Fi standard, the Institute of Electrical and Electronics Engineers (IEEE) 802.11 specification, released in 1997, employed methods such as frequency hopping and DSSS.

In 1999, IEEE 802.11a introduced orthogonal frequency-division multiplexing (OFDM) in the 5 gigahertz band for faster data rates.

This evolution of wireless standards continues to this day.

As of this year, Wi-Fi 6 (using the 2.4 and 5 GHz bands) and Wi-Fi 6E (which adds the 6 GHz band) are commonly found in new routers, offering maximum theoretical speeds of approximately 9.6 Gbps.

Also, Wi-Fi 7 (IEEE 802.11be) is now available in high-end devices, offering multi-gigabit speeds with peak data rates of around 40 Gbps under optimal conditions.

Lamarr and Antheil’s collaboration played a key role in shaping the “truly ahead of its time” wireless technologies we rely on today.

George Johann Carl Antheil was born July 8, 1900, in Trenton, NJ, and died Feb. 12, 1959, in New York City, NY, at age 58.

Hedy Lamarr, born Hedwig Eva Maria Kiesler Nov. 9, 1914, in Vienna, Austria, died Jan. 19, 2000, in Casselberry, FL, at age 85.

















Thursday, November 13, 2025

AI helps retired telecom tech

@Mark Ollig

The other evening, I turned on my LG smart TV and opened the YouTube TV app to watch some live-streaming channels.

Lately, the video had been a bit blurry and choppy.

That night, it froze after about a minute, and all I saw was a spinning icon circle; it felt like seeing the Windows “blue screen of death.”

I could hear “Star Trek’s” Dr. Leonard McCoy saying, “The YouTube TV app is dead, Jim.”

As a retired telecom engineer, I used to resolve complex hardware and call routing problems involving multimillion-dollar digital and optical signaling network systems.

Before retirement, I diagnosed issues in Voice over Internet Protocol (VoIP) switching environments.

But there I was, in my living room, staring at a frozen YouTube TV video stream.

My other smart TV apps, Netflix, Prime Video, and Paramount+, all worked fine.

I also verified that the YouTube TV app played smoothly on my Hewlett-Packard laptop, my Google Assistant smart display, and my Samsung Galaxy smartphone.

All devices were connected, including my smart TV, via Wi-Fi through a wireless local area network (WLAN) on my Verizon 5G Home Internet gateway, the router in my home.

Since I have written about artificial intelligence (AI), I asked ChatGPT-5 from OpenAI for assistance.

I typed out the problem, listed what I had tried, and uploaded photos from the LG manual, the smart TV model label, the LG remote, and the on-screen messages I was seeing.

ChatGPT identified a likely adaptive bitrate (ABR) representation switch issue in the YouTube TV app’s webOS media player.

LG’s webOS is a Linux-based operating system.

When the app tried to improve video quality on my smart TV, it likely switched to a higher-bitrate segment of the same codec at a keyframe, known as an Instantaneous Decoder Refresh (IDR) frame.

Most video frames store only changes from prior frames, but a keyframe contains the complete picture.

When the video player encounters an IDR keyframe during an adaptive-bitrate (ABR) switch, it can discard older data, reset the decoder, and start again from that point without visual glitches or interruptions.

At that moment, the TV’s video pipeline should clear any buffered video data and reset the decoder. It should then load the next segment and continue playing.

A recent update to webOS or the YouTube TV app may have caused the playback issue, as the app froze during an adaptive-bitrate (ABR) transition because the reset did not complete.

And yes, I had deleted and reinstalled the YouTube TV app and reset the smart TV, but this did not immediately resolve the problem.

After completing a clean reinstall and full power reset, the newly installed app replaced the previous install, which a background update likely left in a bad state.

Reinstalling cleared cached files and settings, and the power reset cleared the TV’s memory and video decoder.

With a clean start, the player pulled a fresh playlist, picked a stable bitrate, and the video resumed.
The channels on the YouTube TV app played smoothly again on my LG smart TV.

Video playback for the YouTube TV app has been stable at high definition (HD) 720p and 60 frames per second (fps).

The smart TV is now set to auto update, which lets webOS refresh the system software and individual apps automatically.

I did some research on the history of smart TVs, with a focus on LG and its operating system, webOS.

Released in 2008, Samsung’s Series 7 (PAVV Bordeaux 750) was among the earliest connected TVs.

In 2009, Samsung added Yahoo-powered Internet@TV widgets (news, weather, stock) on select models.

It was the forerunner to today’s smart TVs.

Samsung introduced its Yahoo-powered “Internet@TV” widgets in 2009 on select models, offering on-screen apps like weather, news, and videos.

Google introduced Google TV, a smart TV platform, in May 2010.

“We want to use the internet to change the television experience. We’re putting a browser in the TV to enable a whole bunch of things,” said Vincent Dureau, Google’s head of TV technology, in the Aug. 19, 2010, Minneapolis Star Tribune.

Sony introduced the first high-definition TVs (HDTVs) powered by Google TV in October 2010.

LG’s history began in 1947 with the founding of Lucky Chemical Industrial Corporation by Koo In-hwoi (1907 to 1969).

In 1958, 11 years after founding his first company, In-hwoi started GoldStar Co., Ltd., marking his entry into the electronics industry.

For many years, Lucky Chemical focused on chemicals, while GoldStar focused on electronics.

In 1983, the parent company officially adopted the name Lucky-Goldstar, bringing Lucky Chemical and GoldStar together under one brand, now known as LG.

In 2009, Palm developed webOS, a Linux-based operating system, in Sunnyvale, CA. Hewlett-Packard acquired Palm in 2010 for $1.2 billion.

LG’s early NetCast smart TVs gained popularity by 2009, and the LG Smart TV brand was officially launched at CES 2011.

In 2013, LG acquired webOS from Hewlett-Packard and integrated it into its TV platform in 2014.

LG’s main office is in the LG Twin Towers in Seoul, South Korea.

I’m writing this four days after the clean reinstall and power reset, and the YouTube TV app continues to run smoothly on my smart TV.

With a bit of help from AI, this retired telecom tech solved one more problem.



Friday, November 7, 2025

Significant milestones in space and technology

@Mark Ollig

As November begins, I’d like to reflect on some of the early historical milestones associated with this month.

First commercial telegraph line

The first telegraph line in North America opened for regular commercial service between Buffalo and Lockport, New York, Nov. 7, 1845.

The single-wire circuit transmitted messages in Morse code over pole-mounted conductors.

The line was built under the direction of Orrin S. Wood, following Samuel F. B. Morse’s system, and marked the start of commercial telegraphy in the United States.

Gemini 12’s spacewalk lessons

Gemini 12 launched on Nov. 11, 1966, with astronauts James Lovell and Edwin “Buzz” Aldrin aboard.

Aldrin performed three extravehicular activities (EVAs) totaling about five hours and 30 minutes, using handholds and footholds attached to the Gemini spacecraft.

Lovell and Aldrin also completed a rendezvous and docking with the Agena Target Vehicle in Earth orbit.

As the final Gemini mission, Gemini 12 validated EVA techniques and rendezvous procedures later used for Apollo lunar module rendezvous and docking.

Surveyor 6 lands and hops on the Moon

Surveyor 6 launched Nov. 7, 1967, and landed in Sinus Medii Nov. 10. It transmitted 29,952 television pictures of the lunar surface.

Surveyor 6 performed the first remote-controlled “hop” on another world Nov. 17, 1967, rising about 10 to 12 feet above the surface and landing about eight feet away under commands from NASA controllers.

Its data showed the lunar surface could support the Apollo Lunar Module and helped identify future landing sites.

Apollo 4 and the first Saturn V flight

Apollo 4 launched Nov. 9, 1967, from Kennedy Space Center’s Launch Complex 39A, marking the first flight of the Saturn V rocket.

This uncrewed mission tested all three stages of the rocket, along with the command and service module.

The mission simulated a high-speed lunar return when the command module reentered Earth’s atmosphere at nearly 25,000 miles per hour, successfully validating the heat shield’s performance.

Mariner 9 arrives at Mars

NASA’s Mariner 9 became the first spacecraft to orbit another planet when it entered orbit around Mars Nov. 13, 1971 (CST).

A global dust storm initially obscured the surface, but once it cleared, Mariner 9 revealed volcanoes, valleys, and ancient riverbeds, including Olympus Mons and Valles Marineris.

The orbiter mapped about 85% of the planet’s surface and returned 7,329 images before the mission completed Oct. 27, 1972.

Voyager 1 Saturn flyby

NASA’s Voyager 1 space probe launched Sept. 5, 1977.

It made its closest approach to Saturn Nov. 12, 1980, at a distance of about 78,000 miles from the planet’s cloud tops and captured images of Saturn’s rings, moons, and Titan.

Now traveling through interstellar space, Voyager 1 is about 15.7 billion miles from Earth and continues to transmit data to NASA’s Deep Space Network.

STS-2: First reuse of a shuttle

NASA launched the Space Transportation System (STS) Space Shuttle Columbia Nov. 12, 1981, marking the first reuse of a space shuttle orbiter since STS-1 April 12, 1981.

Astronauts Joe Engle and Richard Truly spent two days testing shuttle systems, including the Office of Space and Terrestrial Applications (OSTA-1), which carried the first scientific payload aboard the Space Shuttle.

Microsoft announces Windows

Microsoft founder Bill Gates introduced Windows, a groundbreaking graphical user interface, at the Helmsley Palace Hotel in New York City, NY, Nov. 10, 1983.

Windows 1.0 was released to customers in November 1985, marking the launch of a new era in personal computing.

The birth of AOL

Quantum Link (Q-Link) launched Nov. 5, 1985, for Commodore 64 and 128 users.

It featured graphical menus and icons, offering services like email, chat rooms, forums, and file libraries.

Users could play online games, such as Island of Kesmai and Habitat, which included avatars.

Most dial-up connections were at speeds of 300 to 2,400 bits per second.

Q-Link evolved into America Online in October 1989.

AOL discontinued its dial-up service Sept. 30, 2025.

First internet radio simulcast

WXYC-FM 89.3 at UNC-Chapel Hill became the first traditional radio station to stream live on the internet Nov. 7, 1994.

Listeners installed Cornell’s CU-SeeMe program on their computer, typed in the UNC SunSITE server address, and listened through that connection.

WREK 91.1 FM in Atlanta also streamed that day in a beta test. KJHK 90.7 FM at the University of Kansas began broadcasting a public stream Dec. 3, 1994.

Apple iPod goes on sale

Apple introduced the iPod Oct. 23, 2001, with a five-gigabyte, 1.8-inch hard drive. The first model could hold about 1,000 songs.

It went on sale Nov. 10, 2001, and synced with iTunes on an Apple Mac computer over a FireWire cable, which also charged the iPod.

Firefox 1 release

Millions of users quickly adopted Mozilla’s Firefox web browser after its release Nov. 9, 2004.

Its open-source model and tabbed browsing gave people a fresh choice beyond Internet Explorer and revived competition on the web.

Rosetta’s Philae lands on a comet

The Philae lander, carried by the European Space Agency’s Rosetta spacecraft, touched down on comet 67P/Churyumov–Gerasimenko on Nov. 12, 2014.

Its grappling-hook harpoons, designed to anchor the lander, failed to fire, and Philae bounced twice before coming to rest in shadow.

Philae returned images and instrument data before its batteries depleted.

Rosetta remained in orbit from Aug. 6, 2014, until a controlled descent concluded the mission Sept. 30, 2016.

Philae became the first spacecraft to land on a comet.

Twitter expands to 280 characters

Twitter increased the character limit on its website from 140 to 280 characters Nov. 7, 2017.

The change was intended to solve “cramming,” a problem where users frequently hit the 140-character limit and needed to shorten the words used in their tweets (posts).

AI web browsers

The Browser Company’s Dia announced an integrated AI web browser Nov. 3, 2025.

Opera Limited, majority-owned by Kunlun Tech, released the Neon AI browser Sept. 30.

In October, there were AI updates to its Opera and Opera GX web browsers.

Major technological milestones have progressed from the first commercial telegraph to space exploration and now AI-powered web browsers.



Thursday, October 30, 2025

Lunar Orbiter 1: NASA’s first Moon survey mission

@Mark Ollig

“I believe that this nation should commit itself to achieving the goal, before this decade is out, of landing a man on the Moon and returning him safely to the Earth.”

President John F. Kennedy spoke those words to a joint session of Congress May 25, 1961.

Just over a month earlier, April 12, 1961, Soviet cosmonaut Yuri Gagarin became the first human to orbit Earth in the Vostok 1 capsule, completing a 108-minute flight.

Shortly afterward, NASA launched astronaut Alan Shepard in the Mercury spacecraft Freedom 7 May 5, 1961, completing a 15-minute suborbital flight.

Unlike Gagarin’s mission, Shepard’s did not involve orbiting Earth.

US fears of Soviet technological superiority in space began Oct. 4, 1957, with the launch of the “beeping” Sputnik 1, the first artificial satellite to orbit Earth.

The United States attempted its first satellite launch Dec. 6, 1957, with Vanguard TV-3 (Test Vehicle-Three), which rose about four feet off the launch pad before losing thrust and exploding.

NASA launched the Lunar Orbiter program Aug. 30, 1963, to create detailed maps of the Moon’s surface so future crewed spacecraft could land safely, since Earth-based telescopic images lacked the needed resolution.

An uncrewed equipped spacecraft would travel to the Moon and take high-resolution photographs of its surface.

President Kennedy was assassinated in Dallas, TX, Nov. 22, 1963.

By this time, NASA had begun developing the technology, rockets, and spacecraft to send American astronauts to the moon.

NASA awarded the Boeing Company a contract May 7, 1964, to build five robotic lunar orbiter spacecraft to be sent to the moon between 1966 and 1967, starting with Lunar Orbiter 1.

The lunar orbiters were produced at Boeing’s missile production center in Seattle, WA.

Lunar Orbiter 1 weighed 853 pounds and featured a 150-pound film imaging system developed by Eastman Kodak, which handled the exposure, scanning, and development of 70-millimeter film.

The spacecraft’s camera system included two lenses: a high-resolution 610 mm Panoramic lens and a medium-resolution 80 mm wide-angle Xenotar lens.

This system enabled both detailed close-ups and broader background images during each exposure.

NASA launched Lunar Orbiter 1 from Cape Kennedy, FL, using an Atlas rocket with an Agena D upper stage Aug. 10, 1966, at 2:31 p.m. CDT.

Translunar injection was completed by Agena D’s upper-stage engine at 3:04 p.m. CDT, setting Lunar Orbiter 1 on its path to the moon.

A 100-pound thrust bipropellant engine using nitrogen tetroxide and Aerozine-50 adjusted the spacecraft’s course and orbit.

Lunar Orbiter 1 was powered by solar panels, with a battery for periods when the orbiter was on the far side of the Moon and hidden from sunlight.

The onboard Canopus star tracker allowed the orbiter to orient itself by locking onto the bright star Canopus, providing a stable celestial reference for attitude control.

Lunar Orbiter 1 communicated by radio on the S-band, a microwave frequency around 2,295 megahertz, through NASA’s Deep Space Network stations at Goldstone, CA; Madrid, Spain; and Woomera, Australia.

The orbiter also measured radiation, the energy emitted by space particles, and recorded the density of micrometeorites impacting its surface.

The Aug. 11, 1966, Minneapolis Star newspaper headline read “Lunar Orbiter Speeds Towards Its Target.”
Lunar Orbiter 1 reached the Moon Aug. 14, 1966. It completed one orbit every three hours and 37 minutes.

Its cameras capturing high- and medium-resolution photos.

Scientists analyzed these images to map craters, slopes, and rocky areas, aiding in avoiding these hazards and selecting the safest Apollo mission landing sites.

From Aug. 18 to Aug. 29, 1966, Lunar Orbiter 1 transmitted 205 image frames to Earth, some 240,000 miles away.

After a small orbital correction Aug. 21, Lunar Orbiter 1 lowered its path to about 35 miles above the Moon’s surface to obtain higher-resolution, including stereo pairs (two photos of the same area taken from slightly different angles).

NASA confirmed that these stereographic photos, with a resolution as fine as three feet, provided needed 3D data for planning future lunar landing sites.

The orbiter’s camera continued sending pictures to Earth through September.

During its 577th lunar orbit Oct. 29, 1966, NASA commanded Lunar Orbiter 1, which was at its mission end, to impact the Moon’s far side at six degrees, 42 minutes north latitude and 162 degrees east longitude.

The Minneapolis Star reported, also on Oct. 29, 1966, that the Soviet Union’s Luna-12 spacecraft had entered lunar orbit Oct. 25 and began sending photographs of the moon’s surface to Earth shortly after.

“The feat moved Russia a step closer to a manned moon landing,” the article stated.

By 1966, the US and the Soviet Union were in a fierce competition to showcase their achievements in space exploration, especially in the space race to land humans on the moon first.

NASA’s Lunar Orbiter program produced high-quality photographs that were used to identify safe landing sites for the Apollo missions, and it played a leading role in advancing lunar imaging technology.

American astronauts Neil Armstrong and Edwin “Buzz” Aldrin successfully landed on the Moon July 20, 1969, explored its surface, and returned safely to Earth.

This achievement fulfilled President Kennedy’s goal to “land a man on the Moon and return him safely to the Earth” before the end of the decade.

Lunar Orbiter 1 took a photograph of a crescent Earth above the lunar horizon Aug. 23, 1966.

The image was developed, scanned, and transmitted to Earth as an analog signal.

The Lunar Orbiter Image Recovery Project at NASA’s Ames Research Center in Moffett Field, CA, later digitized and enhanced the image, releasing it Nov. 13, 2008.

You can see it here: https://www.nasa.gov/wp-content/uploads/2020/12/lunar_orbiter_1_photo_of_earth_aug_23_1966_original_and_remastered_loirp.jpg.


Friday, October 24, 2025

MCM/70: Canada’s early player in the computer era

@Mark Ollig

While many of my past columns have highlighted computers built in this country, some credit for their early innovation also belongs to our neighbors to the north.

Merslau “Mers” Kutt, born in 1933 in Ontario, Canada, was a mathematics professor at Queen’s University in Kingston, Ontario.

In the fall of 1971, he met software engineer Gordon Ramer in Toronto to explore new computer technologies.

Kutt Systems Inc. was founded in Toronto Dec. 28, 1971, and secured financial backing from local investors.

In mid-1972, the company assembled its first working microcomputer prototype using Intel’s SIM8-01 single-board development system.

The SIM8-01 was a low-cost kit for Intel’s 8008 central processing unit (CPU), released in 1972, and was widely used in early microcomputer prototyping.

That prototype evolved into the MCM/70 microcomputer late in 1972, when Kutt Systems was renamed Micro Computer Machines (MCM) and Mers Kutt became president.

In November 1972, MCM demonstrated a rack-mounted, wire-wrapped MCM/70 prototype to shareholders in Kingston.

The 1973 MCM/70 delivered interactive A Programming Language (APL) capability in a portable microcomputer with software in read-only memory (ROM), using dual cassette tape drives for its virtual memory.

It offered this capability before mainstream personal computers (PCs) were available, when businesses and organizations relied on large computer mainframes.

The MCM/70, an early portable microcomputer, used Intel’s 8008 microprocessor, operating at about 0.8 megahertz (MHz).

It operated two ROM modules: EASY (External Allocation System), which managed cassette input/output, and AVS (A Virtual System), which provided cassette-based virtual memory of about 200 kilobytes (KB).

APL programs did not use traditional files; instead, all user-defined elements, such as numbers, arrays, and functions, were kept together in what APL called a workspace.

The MCM/70 would automatically perform an orderly shutdown during a power loss, writing the users’ workspace data to cassette tape.

When its internal memory filled up, the MCM/70 could offload parts of the workspace to cassette tape, extending usable random-access memory (RAM).

The company announced Sept. 25, 1973, the fully working MCM/70 at the Royal York Hotel in downtown Toronto, with demonstrations in New York Sept. 27 and Boston Sept. 28.

Delivered to resale dealers in 1974, the MCM/70 preceded the Altair 8800 by about a year, and the Apple II and IBM PC by several years.

Ads and the press compared the MCM/70 to a typewriter, saying it was easy to carry and set on a desk to use.

Users solved tasks such as portfolio rebalancing and inventory forecasts with the MCM/70.

When dealer shipments started in late 1974, the MCM/70 usually came with two to eight kilobytes of RAM, expandable with cassette-backed virtual memory for larger workspaces.

The MCM/70 was designed for professional users in business, laboratory, and government settings, rather than the mass market.

The original MCM/70 model featured a built-in keyboard with an APL layout based on IBM 2741 terminals, a single-line gas-plasma display screen, and support for up to two cassette tape drives.

Today, APL primarily survives in specialized domains, including finance, research, and engineering, with commercial tools such as Dyalog and open-source options.

The machine, the Micro Computer Machines/70 (MCM/70), connected to printers and other peripherals through input/output (I/O) ports.

These included the MCP-132 printer/plotter (an MCM-branded Diablo Systems HyType I) and the PMR-400 punched-card reader.

It also supported the SCI-1200 communications subsystem, allowing users to send and receive data by modem.

From 1974 to 1980, connections commonly included IBM System/360 and compatible System/370 mainframes, Digital Equipment Corporation (DEC) systems, and other MCM computers.

By 1979 and 1980, users also dialed early bulletin board systems (BBSs).

The MCM/70 operated on AC power, with a small internal battery for memory preservation and orderly shutdown during power outages.

Early 1970s materials described the MCM/70 as a portable microcomputer that could be carried like a small typewriter. It weighed about 20 pounds.

When production and dealer shipments began in earnest in late 1974, MCM/70 model prices ranged roughly from $4,700 to $9,800, depending on options and memory.

Today, that would amount to about $29,800 to $62,100.

The MCM/70 was marketed to businesses, laboratories, and government agencies that needed interactive, programmable data analysis

By 1976, customers included Chevron, Firestone, Mutual Life of Canada, Ontario Hydro, NASA’s Goddard Space Flight Center, and the United States Army.

MCM’s computer product line included the MCM/70 in 1974, the MCM/700 in 1975, the MCM/800 in 1976, the MCM/900 in 1978, and the MCM/1000 (MCM Power) in 1980.

The original MCM/70 used an APL keyboard; however, later MCM computer models used standard QWERTY keyboards for general office use.

In 1981, Kutt founded All Computers Inc. and developed the MCM MicroPower, a small single-user computing machine.

Lower-priced personal computers, including the Apple II and later the IBM PC, ultimately eroded MCM’s market share, and the company ceased operations in 1983.

In September 2003, The Globe and Mail newspaper in Canada featured a story that referred to Kutt as the “father of the personal computer (PC).”

In 2019, Kutt filed a patent infringement lawsuit in the US District Court for the Eastern District of Texas involving his US Patent 5,450,574 and US Patent 5,506,981.

He sued Apple Inc. and more than 40 other companies for $350 billion in damages Sept. 20, 2019.

The district court dismissed the case with prejudice on March 23, 2020.

The US Court of Appeals for the Federal Circuit confirmed the lower court’s dismissal Nov. 9, 2022.

No damages were awarded.

My latest research shows that Merslau “Mers” Kutt is still living.

A photo of a working MCM/70 with the APL keyboard at the York University Computer Museum exhibit can be seen here: https://bit.ly/3IL42vP.


Thursday, October 16, 2025

Viking 1: the Mars lander that set the standard

@ Mark Ollig

The Soviet Union’s Mars 3 spacecraft soft-landed on Mars Dec. 2, 1971, but its surface signal lasted only about 20 seconds.

It transmitted the first lines of a TV frame, a featureless gray field, before the signal failed.

Viking 1 lifted off Aug. 20, 1975, aboard a Titan IIIE/Centaur rocket from Cape Canaveral toward Mars, about 160 million miles away.

The Centaur was a high-energy stage using twin RL-10 engines that burned liquid hydrogen and liquid oxygen, known for their reliability and performance.

Because of its looping trajectory around the sun, Viking 1 traveled more than 400 million miles to reach Mars.

Viking 1 was a two-part spacecraft consisting of the Viking 1 orbiter (which would circle Mars) and the Viking 1 lander (designed to land on the surface).

The Titan IIIE core and solid boosters placed the Viking 1 spacecraft in a 104-mile parking orbit around Earth, a temporary holding orbit before departure to Mars.

The Centaur upper stage then restarted from that orbit to perform the trans-Mars injection, sending the spacecraft on its way.

Approximately four minutes later, the upper stage successfully separated from the Viking 1 spacecraft.

As Viking 1 moved outward toward Mars, its speed around the sun fell from about 73,000 mph near Earth’s orbit to roughly 48,000 mph near Mars’ orbit.

The spacecraft performed three trajectory-correction maneuvers on its journey to Mars: Aug. 27, 1975; June 10, 1976; and June 15, 1976.

During its 11-month journey to the Red Planet, the Viking 1 lander was secured in a protective aeroshell that acted as a heat shield.

It was connected to the Viking 1 orbiter via mechanical latches and an electrical umbilical for power and signals.

The Viking 1 spacecraft entered Mars orbit June 19, 1976.

For the next four weeks, mission controllers from Earth observed images of the Mars surface from the Viking 1 orbiter and confirmed a safe landing site for the Viking 1 lander.

A timed sequence then triggered the release of the lander using pyrotechnic devices, while springs pushed it onto its descent path.

The Viking 1 lander touched down in Chryse Planitia July 20, 1976.

Because radio signals take time to travel between Earth and Mars, the lander relied on its onboard computer for many tasks.

It drew power from two radioisotope thermoelectric generators (RTGs, which convert heat from radioactive decay into electricity), while the orbiter used solar power.

The lander carried twin panoramic cameras and three biology experiments, returning the first US photos from the Martian surface and conducting the first life-detection experiments (searching for signs of life) on another planet.

Its weather package measured temperature, pressure, and wind, giving Earth the first day-to-day weather reports from Mars.

I recall hearing it said on a 1976 television news broadcast, “Today, the temperature reached 72 degrees Fahrenheit in the northern equatorial region on the planet Mars.”

Viking 1 operated until November 1982. The Viking 1 orbiter ended its mission July 25, 1978; the Viking 1 orbiter ended Aug. 17, 1980.

Decades after Viking, another milestone arrived; 45 years later, NASA’s Perseverance rover touched down in Jezero Crater Feb. 18, 2021.

Perseverance operates autonomously to handle communication delays with Earth efficiently.

It uses AutoNav on the Vision Compute Element (VCE) to navigate and avoid obstacles, while AEGIS helps select targets and gather SuperCam data.

The rover is powered by a plutonium Multi-Mission Radioisotope Thermoelectric Generator (MMRTG).
Ingenuity, a helicopter carried by Perseverance, first flew April 19, 2021.

It is solar-powered and uses a Qualcomm Snapdragon 801 processor to navigate autonomously.

In 72 flights, Ingenuity traveled more than 10 miles, took more than 18,000 images, reached about 79 feet in altitude, and flew up to 2,300 feet in one flight.

Ingenuity’s final flight on Mars took place Jan. 18, 2024.

Looking to the future, Mars Sample Return, a joint NASA-European Space Agency campaign, is being replanned; NASA expects to confirm the mission design in 2026 and target robotic sample delivery in the 2030s.

The Perseverance rover captured images of a streak of light in the Martian sky, sparking speculation about the interstellar comet 3I/ATLAS.

However, NASA has not yet confirmed the sighting as comet 3I/ATLAS.

The European Space Agency released official images of comet 3I/ATLAS from its Mars orbiters, the ExoMars Trace Gas Orbiter and the Mars Express, around the same time.

Ultimately, the Perseverance mission supports NASA’s broader goal of preparing for future human exploration of Mars, which builds upon the Artemis program’s mission to the moon.

Artemis II will send four astronauts around the moon on a roughly 10-day flight to test Orion’s systems.

The Artemis III mission will be the first south-polar landing of astronauts since Dec. 11, 1972.

NASA aims for the first crewed missions to Mars sometime in the 2030s.

Hurry up, NASA. I’m not getting any younger.

Viking 1 is remembered as the mission that set the standard for future missions to Mars – and beyond.




Friday, October 10, 2025

Space law in the age of AI

@Mark Ollig


The Outer Space Treaty (OST) opened for signatures in Washington, London, and Moscow Jan. 27, 1967.

By the time it took effect Oct. 10, 1967, 61 countries had signed it.

The treaty established fundamental principles for space activity, including the banning of national ownership of outer space and the guarantee of freedom for peaceful exploration.

It also prohibited the placement of nuclear weapons or other weapons of mass destruction (WMD) in Earth orbit, on the Moon, or on other celestial bodies.

Of course, the 1967 Outer Space Treaty does not mention artificial intelligence (AI).

The United Nations Office for Outer Space Affairs (UNOOSA) promotes discussions about safety and responsibility in the use of AI.

UNOOSA also maintains the official status of the five core United Nations (UN) space treaties.

The 1967 OST allows all countries to explore and use space freely, but it does not let any nation claim ownership of celestial bodies.

Its Articles X to XII promote openness by allowing visits to these objects in space and the sharing of information.

However, I noted the 1967 treaty permits military personnel to carry out peaceful scientific activities, and it does not expressly prohibit placing conventional weapons in Earth orbit.

New agreements and updates are helping to address complex problems that modern satellites and spacecraft create for the current 1967 OST.

The Agreement on the Rescue of Astronauts (1968) requires countries to help distressed astronauts and return them safely to Earth.

The Convention on International Liability for Damage Caused by Space Objects (1972) makes the launching state liable for any damage caused by falling space debris on the surface of the Earth or to aircraft in flight.

The Convention on Registration of Objects Launched into Outer Space (1975) requires countries to submit basic details of space objects launched into outer space to the United Nations.

The Agreement Governing the Activities of States on the Moon and Other Celestial Bodies (1979) extends OST principles to the Moon and urges an international regime for its resource use.

The treaty strongly emphasizes that countries may not place nuclear weapons or other WMD in Earth orbit.

Military bases, weapons testing, and military maneuvers are not allowed on the Moon or other celestial bodies.

However, military personnel can participate in peaceful scientific activities there.

The Artemis Accords, introduced in 2020, enhance the 1967 Outer Space Treaty by emphasizing transparency, collaboration, and the responsible use of resources in space exploration.

Originally signed by eight countries, the Accords have expanded to 56 countries, including Senegal, which joined July 24 of this year.

In September of this year, UNOOSA issued a policy brief titled “Ensuring Responsible AI in Space and Earth Observation.”

The brief emphasizes that ethical and transparent AI is essential in space.

It requires a clear understanding and monitoring of AI actions, as well as human oversight in major decisions, particularly for deep-space missions. Read it here: https://bit.ly/47909Kf.

Launched Dec. 18, 2019, the European Space Agency’s (ESA) Optical Payload for the Satellite with Amateur Transceiver (OPS-SAT) was an orbiting AI lab about 320 miles above Earth.

Using neural networks installed on the satellite system, it analyzed images directly onboard, while its machine-learning models handled power, temperature, and orientation adjustments instantly.

The mission ended May 22, 2024, when OPS-SAT reentered Earth’s atmosphere and burned up.

NASA managed the Starling 1.5 experiment this year, testing autonomous satellite coordination with SpaceX’s Starlink network.

The experiment showcased AI-assisted space traffic coordination, including automated screening of trajectories and the assignment of maneuver responsibility.

The European Space Agency’s (ESA) PhiSat-1 launched in early September 2020 on a Vega rideshare from Kourou, French Guiana.

It uses onboard AI to filter cloud-covered images and send only clear images to Earth.

The PhiSat-2 satellite was launched Aug. 16, 2024, carrying a multispectral imager and advanced AI capabilities.

Its AI helps sort data quickly so teams can make fast decisions during disasters, find ships, track wildfires, and protect the environment.

PhiSat-2 quickly turns raw images into near-real-time street maps, giving emergency teams and maritime groups instant information about what is happening.

By the end of October 1967, about 1,090 objects had been launched into Earth orbit since Sputnik 1 in 1957.

In 1967, the United States launched 87 spacecraft, according to NASA.

Most launches to that date were by the United States and the Soviet Union; others with satellites included the United Kingdom, Canada, Italy, and France, with France the only one to reach orbit on its own.

As of February 2024, NASA reports that roughly 9,300 satellites are currently orbiting Earth.

NASA also reports that more than 45,000 human-made space objects orbit the planet, including debris and nonoperational satellite hardware.

UNOOSA leads discussions on international space law through the Committee on the Peaceful Uses of Outer Space.

For the latest updates on the status of outer space treaties and new developments, see UNOOSA: https://bit.ly/4nBUOBe.