significant heat, generally when they were fired in a kiln. Other methods Other methods include: Argon–argon (Ar–Ar) Iodine–xenon (I–Xe) Lanthanum–barium (La–Ba) Lead–lead (Pb–Pb) Lutetium–hafnium (Lu–Hf) Hafnium–tungsten dating (Hf-W) Potassium–calcium (K–Ca) Rhenium–osmium (Re–Os) Uranium–uranium (U–U) Krypton–krypton (Kr–Kr) Beryllium (10Be–9Be) Dating with decay products of short-lived extinct radionuclides Absolute radiometric dating requires a measurable fraction of parent nucleus to remain in the sample rock. For rocks dating back to the beginning of the solar system, this requires extremely long-lived parent isotopes, making measurement of such rocks' exact ages imprecise. To be able to distinguish the relative ages of rocks from such old material, and to get a better time resolution than that available from long-lived isotopes, short-lived isotopes that are no longer present in the rock can be used. At the beginning of the solar system, there were several relatively short-lived radionuclides like 26Al, 60Fe, 53Mn, and 129I present within the solar nebula. These radionuclides—possibly produced by the explosion of a supernova—are extinct today, but their decay products can be detected in very old material, such as that which constitutes meteorites. By measuring the decay products of extinct radionuclides with a mass spectrometer and using isochronplots, it is possible to determine relative ages of different events in the early history of the solar system. Dating methods based on extinct radionuclides can also be calibrated with the U-Pb method to give absolute ages. Thus both the approximate age and a high time resolution can be obtained. Generally a shorter half-life leads to a higher time resolution at the expense of timescale. The 129I – 129Xe chronometer beta-decays to with a half-life of 16 million years. The iodine-xenon chronometer is an isochron technique. Samples are exposed to neutrons in a nuclear reactor. This converts the only stable isotope of iodine () into via neutron capture followed by beta decay (of ). After irradiation, samples are heated in a series of steps and the xenon isotopic signature of the gas evolved in each step is analysed. When a consistent / ratio is observed across several consecutive temperature steps, it can be interpreted as corresponding to a time at which the sample stopped losing xenon. Samples of a meteorite called Shallowater are usually included in the irradiation to monitor the conversion efficiency from to . The difference between the measured / ratios of the sample and Shallowater then corresponds to the different ratios of / when