Neptunium (Np)

Discovery & history

Discovered: 1940 · Edwin McMillan

When the first periodic table of the elements was published by Dmitri Mendeleev in the early 1870s, it showed a " — " in place after uranium similar to several other places for then-undiscovered elements. Other subsequent tables of known elements, including a 1913 publication of the known radioactive isotopes by Kasimir Fajans, also show an empty place after uranium, element 92. Up to and after the discovery of the final component of the atomic nucleus, the neutron in 1932, most scientists did not seriously consider the possibility of elements heavier than uranium. While nuclear theory at the time did not explicitly prohibit their existence, there was little evidence to suggest that they did. However, the discovery of induced radioactivity by Irène and Frédéric Joliot-Curie in late 1933 opened up an entirely new method of researching the elements and inspired a small group of Italian sci

Uses & applications

The longest-lived isotope of neptunium, 237Np, has a half-life of 2.14 million years, which is more than 2,000 times shorter than the age of the Earth. Therefore, any primordial neptunium would have decayed in the distant past. After only about 80 million years, the concentration of even the longest-lived isotope, 237Np, would have been reduced to less than one-trillionth (10−12) of its original amount. Thus neptunium is present in nature only in negligible amounts produced as intermediate decay products of other isotopes. Trace amounts of the neptunium isotopes neptunium-237 and -239 are found naturally as decay products from transmutation reactions in uranium ores. 239Np and 237Np are the most common of these isotopes; they are directly formed from neutron capture by uranium-238 atoms. These neutrons come from the spontaneous fission of uranium-238, naturally neutron-induced fission of

Isotopes

All nuclear data not otherwise stated is from the standard source: Twenty-four neptunium radioisotopes have been characterized, with the most stable being 237Np with a half-life of 2.144 million years, 236Np with a half-life of 153,000 years, and 235Np with a half-life of 396.1 days. All of the remaining radioactive isotopes have half-lives that are less than 5 days. Isotopes lighter than the most stable one, 237Np, decay primarily by electron capture, although some also decay by alpha emission to become protactinium. 237Np itself, being the beta-stable isobar of mass number 237, decays by alpha to 233Pa, with very rare spontaneous fission. Heavier isotopes generally decay by beta emission. The decay of 237Np eventually yields bismuth-209 and thallium-205, unlike most other common heavy nuclei which decay into isotopes of lead. This decay chain is known as the neptunium series. This deca