Great Australians — Anthony Michell

We Australians excel at remembering and celebrating our sporting heroes, from cricketers to particularly successful race horses, but are not so good at celebrating the great people who helped build our civilization, particularly when those builders are Australian. Today, I want to celebrate the birthday of a revolutionary Australian engineer, A. G. M. Michell.


Innovator and Inventor

Anthony George Maldon Michell was an Australian engineer who made enormous contributions to a wide range of engineering sciences, from publishing the seminal work on structural optimization, to the invention of the Fluid-film Thrust Bearing. Michell’s inventions operate quietly in the background, but have made a huge impact on our every-day lives.

That's the guy.

Anthony George Maldon Michell (21 June 1870 – 17 February 1959) — engineer

Early life and education

Michell was born in London in 1870 while his parents were visiting from Australia, but grew up and attended primary school in Victoria. He returned to England to attend Grammar school and spent a year studying at Cambridge. He returned to Australia in 1889 to study engineering at the University of Melbourne.

Bearing the load

Of all of Michell’s inventions and innovations, the one that has had the greatest impact is the Michell Bearing, or Fluid-film Thrust Bearing, which he patented in 1905. Michell created a bearing with tilting load-pads that would maintain a thin film of lubricating oil between the metal surfaces. He mathematically derived the pressure distribution in the oil so that the pivot for the tilting pads could be optimally placed to ensure that the pads tilt automatically, under varying load, to the most efficient geometry. At the start of the 20th century, this bearing was revolutionary (pun intended). It could sustain enormous thrust loads with minimal wear and without overheating, while being only one tenth of the size of the bearings it replaced.

Under pressure, do do do didi do do...

Michell thrust bearing — the pads tilt automatically to the most efficient geometry

The low-friction of Michell’s bearings made them much more efficient. Within a decade they had found almost universal application in generators and ships’ thrust blocks. There was some reluctance by the British to adopt Michell Bearings in their ships, until the discovery that the German Navy were using Michell Bearings in their WWI U-Boats, which gave the U-Boats a range and speed that surprised the Royal Navy.

As well as being efficient, the low-wear of Michell Bearings mean they need little maintenance and are very reliable. A Michell Bearing installed at the Holtwood Hydroelectric Power Plant in Pennsylvania in 1912, supporting 165 tonnes of turbine and 40 tonnes of water pressure, is still in operation today. That bearing has been estimated to have a maintenance-free life of over 1000 years.

Michell Bearings, for their strength, efficiency, and reliability are still used on all large ships, power plants and turbines today.

Going with the flow

Another of Michell’s brilliant inventions is the Cross-flow turbine, which has found applications in hydroelectricity generation. This turbine is not used as often as the more common Kaplan, Francis, or Pelton type turbines because it has a lower maximum efficiency. However, cross-flow turbines have a much better efficiency than any of these three when operating at partial load. This gives cross-flow turbines an advantage in small-scale hydroelectric power generation, in situations, such as small rivers, where water flow and pressure can vary widely over the year. Cross-flow turbines are also easier to build, are easier to maintain, and are partially self-cleaning due to the way in which water flows through the blades of the rotor.

Does that count as giving credit?

Cross-flow turbine — image blatantly stolen from Wikipedia

Other innovations

Michell’s other notable innovations include the first published work on structural optimization. Unfortunately, Michell was ahead of his time and this field of research did not gain momentum until computers became a useful research tool some half-century later.

Michell also designed a crankless engine that drew on his work on the thrust bearing and used slipper-blocks on a slanted wobble-plate to convert the reciprocal motion of the pistons into rotary motion of an output shaft. By eliminating the crankshaft, connecting rods, and associated bearings, Michell’s crankless engines could be lighter and more compact than conventional automotive and stationary engines. Proper dynamic design of the wobble-plate also made the engine very low in vibration. Despite successful demonstrations, improved efficiency, and several licensed derivatives, the crankless engine failed to gain wide-spread acceptance and the company formed to produce and market the technology was placed into receivership.

Might be pushing it a bit there...

Michell’s crankless engine — image stolen from somewhere else

Later life

Michell was elected a Fellow of the Royal Society and received several prestigious awards including the Kernot Memorial Medal for distinguished engineering achievement in Australia, and the James Watt International Medal. He continued to make major contributions in engineering research until his death in 1959 at the age of 88.


When asked to list great Australian inventions, most Australians might include the Hills Hoist, Vegemite, the Victa lawnmower, and not much else. Michell, and his bearings that transformed movement and power in the 20th century, deserve to be amongst the first things a proud Australian should include on their list.

Great Australians — Ruby Payne-Scott

We Australians excel at remembering and celebrating our sporting heroes, from cricketers to particularly successful race horses, but are not so good at celebrating the great people who helped build our civilization, particularly when those builders are Australian. Today, I want to celebrate the birthday of a brilliant Australian scientist, Ruby Payne-Scott.


Southern Star

Ruby Payne-Scott is remembered as one of Australia’s most outstanding physicists. As well as contributing to other sciences, she was a pioneer of radio astronomy and made major discoveries about the nature of radio emissions from the Sun. Payne-Scott also has the distinction of being the first female radio astronomer.

Ruby Payne-Scott (28 May 1912 – 25 May 1981) — Physicist, pioneering astronomer

Ruby Payne-Scott (28 May 1912 – 25 May 1981) — Physicist, pioneering astronomer

Early life and education

Ruby was born in 1912 in the town of Grafton, NSW. She demonstrated remarkable talent at school and moved to live with her aunt in Sydney, where she could get a better education. She was awarded honours in mathematics and botany, and won two scholarships to the University of Sydney where she studied physics, chemistry, mathematics, and botany. As was typical of the era, Ruby was often the only woman in her classes.


Despite the prejudice and difficulty in getting a job that female physicists faced at the time (compounded by the Great Depression), Ruby’s excellent academic performance landed her a job as a physicist on the University of Sydney’s new cancer research project. One project she worked on was to determine the effect that the Earth’s magnetic field had on the vital processes of living beings. Working with William Love she cultivated chick embryos in magnetic fields up to 5000 times stronger than the Earth’s field. They found no observable differences in the chicks and determined that the magnetism of the Earth had little or no effect on living creatures.

The cancer research project closed down in 1935, and Ruby was forced to take one of the few career options open to educated women at the time, teaching. She completed a diploma of teaching and started working at a school in South Australia. Ruby was constantly alert for ways to get back into physics and eventually managed to land a job with Australian Wireless Amalgamated, a major hirer of physicists. Although she was hired as a librarian, Ruby managed to get involved in some research projects in the company’s standards laboratory and eventually worked her way into full-time research.

In 1939, Australia, following Britain’s lead, declared war on Germany. The CSIR (the precursor to the CSIRO) was charged with developing an Australian radar capability. As happened in Britain and the USA, mobilization for war created a shortage of trained men and provided women with the opportunity to break into jobs and careers they were previously bared from. Ruby and another woman, Joan Freeman, managed to get hired to work as researchers in the CSIR’s new Radiophysics laboratory. The women excelled in their roles, under the leadership of another great Australian physicist, Joe Pawsey, and both Ruby and Joan later commented that their colleagues treated them as “one of the boys”. The two women mainly had to deal with discrimination from administrators and petty bureaucrats who imposed absurd and unfair rules such as banning women from smoking or wearing shorts, rules which Ruby took the lead in breaking. Ruby even married her Husband, Bill Holman Hall, in secret in 1944 because married women were not allowed to hold permanent positions in government agencies.

Wartime radar research in Britain had discovered that the Sun occasionally produced significant amounts of radio waves. Excited by this, in their spare time Ruby and Joe Pawsey ran some experiments to follow up on this discovery, but did not have the right equipment to make the observations. When the war ended the Radio Physics laboratory was due to be scrapped, so the team put together an application to continue as a radio physics research division, concentrating on rain making and radio astronomy. At the time, radio astronomy was a very new field of research and the astronomy community showed very little interest. Despite this, the CSIR decided to fund radio physics and Australia remains a world leader in radio astronomy to this day.

Along with Joe Pawsey and Lindsay McCready, Payne-Scott used decommissioned radar equipment to make detailed radio-frequency observations of the Sun. This small team was the first to construct a radio-astronomy interferometer. Radio interferometers greatly increase the resolution of their observations by using a long baseline between two or more radio antennas. The CSIR team managed to construct an interferometer using only one antenna.

Great TV reception... Just had to wait for Australia to get TV.

Decommissioned radar antenna at Dover Heights, run by CSIR Radiophysics.

The radar antenna they were using was a coastal installation mounted on a sea-cliff. The antenna received radio signals directly from the Sun but also from reflections off the sea below. This simulated a baseline of around 200 metres between two antennas and allowed Payne-Scott, Pawsey and McCready to determine that solar radio radiation was coming from patches of the Sun that had sun-spots, a major discovery that boosted Australia’s international scientific reputation. The team also showed that the Sun’s corona has a temperature of over a million degrees centigrade, a phenomenon that remains a mystery to astrophysicists. Payne-Scott is also credited with the discovery of type I and type III solar outbursts.

Built to defend against the land of the rising Sun.

Dover heights sea-cliff interferometer — used to study the Sun

Workplace activist and career cut short

Throughout her time at the CSIR and its successor the CSIRO, Payne-Scott was an active advocate of equal rights and pay for women. She fearlessly and vocally opposed women’s workplace restrictions and pay reductions, clashing with CSIRO chairman Sir Ian Clunies Ross on several occasions. Eventually her secret marriage was discovered by CSIRO administrators and she was demoted to a temporary position. Payne-Scott left the CSIRO for good in 1951 (aged 39) to give birth to her son Peter.

Later life

Payne-Scott had a second child, a daughter named Fiona, and in 1963 returned to teaching. She retired in 1974 and died in 1981 at the age of 69.

Today, Ruby’s legacy is remembered in the CSIRO by the Payne-Scott award which is given to support the careers of women researchers. Her influence on radio astronomy and her discoveries means that her name is known by a large section of the Australian astronomy community, though they may not be completely aware of how hard Ruby had to fight to be able to do her ground-breaking research.

Who comes up with these Google doodles?

Google celebrated Ruby’s 100th birthday.

In 2012, on what would have been her 100th birthday, Ruby Payne-Scott was celebrated with a Google doodle. However, this great Australian is still completely unknown to the majority of Australian people. Ruby, her research, and her fight for women’s rights deserves greater recognition.

More information on the life and work of Ruby Payne-Scott can be found at the CSIRO Staff Association, National Archives, or Payne-Scott’s Wikipedia page.