Category Archives: General

Understanding radioactive dose

If someone says something is “very radioactive”, what do they actually mean? How do you measure “radioactiveness”? There are many terms used in physics to describe radioactive decay and each has a specific use.

(Throughout this post I’ll be using polonium-210 as an example. Polonium-210 is most famous as the radioactive poison used to murder Russian dissident Alexander Litvinenko.)

The activity of a radioactivity substance is the number of decays that it undergoes per second: one becquerel (Bq) is one decay per second. Polonium-210 has an activity of 166 terabecquerels per gram (166 TBq/g) which means that each gram of Po-210 undergoes 166 trillion decays per second. But knowing how many radioactive decays a substance undergoes isn’t going to tell us how dangerous it is. Standing one kilometre away from a 1 TBq source is very different to standing one metre away from a 1 TBq source.

The absorbed dose, measured in grays* (Gy), is a measure of the amount of energy deposited by a radioactive source into each kilogram of mass (one gray is one joule per kilogram).

Every time a Po-210 nucleus decays it emits a particle with an energy of 5.3 MeV, which is equivalent to 8.50×10−13 joules. 1 gram of polonium-210, emitting 166 trillion of these particles per second is equivalent to 141 watts, easily enough to run a laptop or two standard 60 W lightbulbs. After a day one one-thousandth of a gram of polonium-210 would have released 12 200 joules of energy, about the same amount of energy as a twenty-five kilogram mass travelling at 70 mph. This 12 200 joules, divided evenly amongst the mass of an 80 kg human being would be more than 150 Gy, where anything more than 5 Gy at any one time is usually fatal.

Absorbed dose isn’t perfect for measuring the danger posed by a radioactive source as it doesn’t take into account where the radiation is absorbed, nor the type of radiation.

The equivalent dose only takes into account the organ or tissue being affected but the effective dose, measured in sieverts† (Sv) is designed to compensate for these failings and attempts to reflect the biological rather than the physical effects of radiation. It is calculated by combining the absorbed dose and two dimensionless factors: one to account for the type of radiation and one to account for the organ or tissue being irradiated. These factors, Q and N, combined together are called the radiation weighting factor.

Q (sometimes called the quality factor) accounts for the type of radiation being absorbed. It is equal to 1.0 for all photons, electrons, positrons and muons; 2.0 for protons and pions; 5.0 to 20 for neutrons according to their energy; and 20 for alpha particles and the heavier products of nuclear fission. N accounts for the tissue or organ that is being irradiated. N is greatest for bone marrow, the colon, the lungs, heart or stomach; and lowest for the skin.

Looking back at the 150 Gy absorbed dose for one milligram of Po-210 we end up with a table that looks like this:

150 Gy of alpha radiation incident upon the lungs or stomach (360 Sv) is approximately 250 times more damaging biologically than 150 Gy of electron or positron radiation received to the skin (1.5 Sv). For comparison, the average dose for a resident of the UK, due to natural background sources is about 2.6 millisieverts and a dose of more than 3 Sv kills fifty percent of people within thirty days.

* The gray is named after Hal Gray, a British physicist who created the field of radiobiology.
† The sievert is named after Rolf Maximilian Sievert, a Swedish medical physicist who studied the biological effects of radiation.

Interferometry data from Christchurch earthquake

The PALSAR instrument aboard the Japanese Advanced Land Observing Satellite (ALOS) has produced some imagery of the Christchurch earthquake.

The ALOS-PALSAR instrument is an interferometer (technically an InSAR instrument) that measures the height between the satellite and the ground. The coloured bands show the variation in the height of the ground. One complete cycle of colour shows a displacement of the ground from −6 cm to +6 cm from the position it “should” be in.

Where bands are closely packed together the displacement of the ground is varying a great deal in a small distance, usually leading to greater destruction.

Programme for International Student Assessment

The Programme for International Student Assessment (PISA) study is conducted every three years by the Organisation for Economic Cooperation and Development (OECD). The OECD is a group of thirty-four countries with “advanced economies”, which basically translates to “club for rich countries”.

The PISA study gives 470 000 15 year-olds a test in literacy, numeracy and science and has just released the results of the 2009 study. The UK comes out above average in science and reading, but below average in mathematics.

I was quite interested in the correlation between between scores:

  • Between science and mathematics was 97.1%
  • Between science and reading was 98.1%
  • Between reading and mathematics was 94.8%

I had expected the highest degree of correlation to be between science and mathematics, but that is probably a physicist’s bias, as maths is such an important part of physics.

Penrose tiling

Sir Roger Penrose is a mathematical physicist best known for his work on theories of general relativity and cosmology. He won the Wolf Prize in 1988 with Stephen Hawking for his work on singularities and black holes; the Institute of Physics’s Paul Dirac Medal and Prize in 1989; and the Royal Society’s Copley Medal in 2008 for “his beautiful and original insights into many areas of mathematics and mathematical physics.”

He is also the inventor of Penrose Tiling, a unique tiling pattern with five-fold symmetry, so I was delighted to discover this building as part of the Greenwich Peninsula complex outside the O2 Millenium Dome.

Almost the entire surface of the Ravensbourne College of Design and Communication building is covered with a Penrose-inspired pattern. Penrose previously sued Kleenex for using his tiling pattern on their quilted toilet paper, but I imagine that Ravensbourne’s architects, Foreign Office, checked with him first.

Time on the Moon

I was surprised to find that the amount of time spent on the Moon by Neil Armstrong and “Buzz” Aldrin on the Apollo 11 mission was really quite small when compared with the time spent by astronauts on subsequent Apollo missions.

Only 12 people (all men, unfortunately) have ever set foot on the Moon. The person to spend the most time on the Moon is Gene Cernan, the commander of the Apollo 17 mission. He left the Apollo lander before the Apollo 17 Lunar Module pilot, NASA geologist Harrison Schmitt, and re-entered the lander after Schmitt. He is therefore also the last person to set foot on the Moon, all the way back in 1972.

Gene Cernan cruising the lunar surface in the lunar rover

Cernan also co-holds (with Thomas Stafford and John Young) the record for the fastest speed achieved by a human being, as the Apollo 10 probe on which he was a passenger reached a speed of 11.1 kilometres per second (24 790 mph) on its return to Earth after orbiting the Moon. The Apollo 10 Command Module is now on display at the Science Museum in London.