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Astatine

Astatine is a chemical element; it has symbol At and atomic number 85. It is the rarest naturally occurring element in the Earth's crust, occurring only as the decay product of various heavier elements. All of astatine's isotopes are short-lived; the most stable is astatine-210, with a half-life of 8.1 hours. Consequently, a solid sample of the element has never been seen, because any macroscopic specimen would be immediately vaporized by the heat of its radioactivity.

Astatine, 85At
Astatine
Pronunciation/ˈæstətn, -tɪn/ (ASS-tə-teen, -⁠tin)
Appearanceunknown, probably metallic
Mass number[210]
Astatine in the periodic table
Hydrogen Helium
Lithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine Neon
Sodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine Argon
Potassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine Krypton
Rubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine Xenon
Caesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury (element) Thallium Lead Bismuth Polonium Astatine Radon
Francium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson
 I 

At

Ts
poloniumastatineradon
Atomic number (Z)85
Groupgroup 17 (halogens)
Periodperiod 6
Block  p-block
Electron configuration[Xe] 4f14 5d10 6s2 6p5
Electrons per shell2, 8, 18, 32, 18, 7
Physical properties
Phase at STPsolid (predicted)
Density (near r.t.)8.91–8.95 g/cm3 (estimated)[1]
Molar volume23.6 cm3/mol (estimated)[1]
Atomic properties
Oxidation states−1, +1, +3, +5, +7[2]
Ionization energies
  • 1st: 899.003 kJ/mol[3]
Other properties
Natural occurrencefrom decay
Crystal structureface-centered cubic (fcc)

(predicted)[4]
CAS Number7440-68-8
History
Namingfrom Ancient Greek ἄστατος (ástatos) 'unstable'
DiscoveryDale R. Corson, Kenneth Ross MacKenzie, Emilio Segrè (1940)
Isotopes of astatine
Main isotopes[5] Decay
abun­dance half-life (t1/2) mode pro­duct
209At synth 5.41 h β+ 209Po
α 205Bi
210At synth 8.1 h β+ 210Po
α 206Bi
211At synth 7.21 h ε 211Po
α 207Bi
 Category: Astatine
| references

The bulk properties of astatine are not known with certainty. Many of them have been estimated from its position on the periodic table as a heavier analog of fluorine, chlorine, bromine, and iodine, the four stable halogens. However, astatine also falls roughly along the dividing line between metals and nonmetals, and some metallic behavior has also been observed and predicted for it. Astatine is likely to have a dark or lustrous appearance and may be a semiconductor or possibly a metal. Chemically, several anionic species of astatine are known and most of its compounds resemble those of iodine, but it also sometimes displays metallic characteristics and shows some similarities to silver.

The first synthesis of astatine was in 1940 by Dale R. Corson, Kenneth Ross MacKenzie, and Emilio G. Segrè at the University of California, Berkeley. They named it from the Ancient Greek ἄστατος (astatos) 'unstable'. Four isotopes of astatine were subsequently found to be naturally occurring, although much less than one gram is present at any given time in the Earth's crust. Neither the most stable isotope, astatine-210, nor the medically useful astatine-211 occur naturally; they are usually produced by bombarding bismuth-209 with alpha particles.

Characteristics edit

Astatine is an extremely radioactive element; all its isotopes have half-lives of 8.1 hours or less, decaying into other astatine isotopes, bismuth, polonium, or radon. Most of its isotopes are very unstable, with half-lives of seconds or less. Of the first 101 elements in the periodic table, only francium is less stable, and all the astatine isotopes more stable than the longest-lived francium isotopes (205–211At) are in any case synthetic and do not occur in nature.[6]

The bulk properties of astatine are not known with any certainty.[7] Research is limited by its short half-life, which prevents the creation of weighable quantities.[8] A visible piece of astatine would immediately vaporize itself because of the heat generated by its intense radioactivity.[9] It remains to be seen if, with sufficient cooling, a macroscopic quantity of astatine could be deposited as a thin film.[4] Astatine is usually classified as either a nonmetal or a metalloid;[10][11] metal formation has also been predicted.[4][12]

Physical edit

Most of the physical properties of astatine have been estimated (by interpolation or extrapolation), using theoretically or empirically derived methods.[13] For example, halogens get darker with increasing atomic weight – fluorine is nearly colorless, chlorine is yellow-green, bromine is red-brown, and iodine is dark gray/violet. Astatine is sometimes described as probably being a black solid (assuming it follows this trend), or as having a metallic appearance (if it is a metalloid or a metal).[14][15][16]

Astatine sublimes less readily than iodine, having a lower vapor pressure.[8] Even so, half of a given quantity of astatine will vaporize in approximately an hour if put on a clean glass surface at room temperature.[a] The absorption spectrum of astatine in the middle ultraviolet region has lines at 224.401 and 216.225 nm, suggestive of 6p to 7s transitions.[18][19]

The structure of solid astatine is unknown.[20] As an analog of iodine it may have an orthorhombic crystalline structure composed of diatomic astatine molecules, and be a semiconductor (with a band gap of 0.7 eV).[21][22] Alternatively, if condensed astatine forms a metallic phase, as has been predicted, it may have a monatomic face-centered cubic structure; in this structure, it may well be a superconductor, like the similar high-pressure phase of iodine.[4] Metallic astatine is expected to have a density of 8.91–8.95 g/cm3.[1]

Evidence for (or against) the existence of diatomic astatine (At2) is sparse and inconclusive.[23][24][25][26][27] Some sources state that it does not exist, or at least has never been observed,[28][29] while other sources assert or imply its existence.[30][31][32] Despite this controversy, many properties of diatomic astatine have been predicted;[33] for example, its bond length would be 300±10 pm, dissociation energy 83.7±12.5 kJ/mol,[34] and heat of vaporization (∆Hvap) 54.39 kJ/mol.[35] Many values have been predicted for the melting and boiling points of astatine, but only for At2.[36]

Chemical edit

The chemistry of astatine is "clouded by the extremely low concentrations at which astatine experiments have been conducted, and the possibility of reactions with impurities, walls and filters, or radioactivity by-products, and other unwanted nano-scale interactions".[21] Many of its apparent chemical properties have been observed using tracer studies on extremely dilute astatine solutions,[32][37] typically less than 10−10 mol·L−1.[38] Some properties, such as anion formation, align with other halogens.[8] Astatine has some metallic characteristics as well, such as plating onto a cathode,[b] and coprecipitating with metal sulfides in hydrochloric acid.[40] It forms complexes with EDTA, a metal chelating agent,[41] and is capable of acting as a metal in antibody radiolabeling; in some respects, astatine in the +1 state is akin to silver in the same state. Most of the organic chemistry of astatine is, however, analogous to that of iodine.[42] It has been suggested that astatine can form a stable monatomic cation in aqueous solution.[40][43]

Astatine has an electronegativity of 2.2 on the revised Pauling scale – lower than that of iodine (2.66) and the same as hydrogen. In hydrogen astatide (HAt), the negative charge is predicted to be on the hydrogen atom, implying that this compound could be referred to as astatine hydride according to certain nomenclatures.[44][45][46][47] That would be consistent with the electronegativity of astatine on the Allred–Rochow scale (1.9) being less than that of hydrogen (2.2).[48][c] However, official IUPAC stoichiometric nomenclature is based on an idealized convention of determining the relative electronegativities of the elements by the mere virtue of their position within the periodic table. According to this convention, astatine is handled as though it is more electronegative than hydrogen, irrespective of its true electronegativity. The electron affinity of astatine, at 233 kJ mol−1, is 21% less than that of iodine.[50] In comparison, the value of Cl (349) is 6.4% higher than F (328); Br (325) is 6.9% less than Cl; and I (295) is 9.2% less than Br. The marked reduction for At was predicted as being due to spin–orbit interactions.[38] The first ionization energy of astatine is about 899 kJ mol−1, which continues the trend of decreasing first ionization energies down the halogen group (fluorine, 1681; chlorine, 1251; bromine, 1140; iodine, 1008).[3]

Compounds edit

Less reactive than iodine, astatine is the least reactive of the halogens;[51] the chemical properties of tennessine, the next-heavier group 17 element, have not yet been investigated, however.[52] Astatine compounds have been synthesized in nano-scale amounts and studied as intensively as possible before their radioactive disintegration. The reactions involved have been typically tested with dilute solutions of astatine mixed with larger amounts of iodine. Acting as a carrier, the iodine ensures there is sufficient material for laboratory techniques (such as filtration and precipitation) to work.[53][54][d] Like iodine, astatine has been shown to adopt odd-numbered oxidation states ranging from −1 to +7.[57]

Only a few compounds with metals have been reported, in the form of astatides of sodium,[9] palladium, silver, thallium, and lead.[58] Some characteristic properties of silver and sodium astatide, and the other hypothetical alkali and alkaline earth astatides, have been estimated by extrapolation from other metal halides.[59]

 
Hydrogen astatide space-filling model

The formation of an astatine compound with hydrogen – usually referred to as hydrogen astatide – was noted by the pioneers of astatine chemistry.[60] As mentioned, there are grounds for instead referring to this compound as astatine hydride. It is easily oxidized; acidification by dilute nitric acid gives the At0 or At+ forms, and the subsequent addition of silver(I) may only partially, at best, precipitate astatine as silver(I) astatide (AgAt). Iodine, in contrast, is not oxidized, and precipitates readily as silver(I) iodide.[8][61]

Astatine is known to bind to boron,[62] carbon, and nitrogen.[63] Various boron cage compounds have been prepared with At–B bonds, these being more stable than At–C bonds.[64] Astatine can replace a hydrogen atom in benzene to form astatobenzene C6H5At; this may be oxidized to C6H5AtCl2 by chlorine. By treating this compound with an alkaline solution of hypochlorite, C6H5AtO2 can be produced.[65] The dipyridine-astatine(I) cation, [At(C5H5N)2]+, forms ionic compounds with perchlorate[63] (a non-coordinating anion[66]) and with nitrate, [At(C5H5N)2]NO3.[63] This cation exists as a coordination complex in which two dative covalent bonds separately link the astatine(I) centre with each of the pyridine rings via their nitrogen atoms.[63]

With oxygen, there is evidence of the species AtO and AtO+ in aqueous solution, formed by the reaction of astatine with an oxidant such as elemental bromine or (in the last case) by sodium persulfate in a solution of perchloric acid.[8][67] The species previously thought to be AtO2 has since been determined to be AtO(OH)2, a hydrolysis product of AtO+ (another such hydrolysis product being AtOOH).[68] The well characterized AtO3 anion can be obtained by, for example, the oxidation of astatine with potassium hypochlorite in a solution of potassium hydroxide.[65][69] Preparation of lanthanum triastatate La(AtO3)3, following the oxidation of astatine by a hot Na2S2O8 solution, has been reported.[70] Further oxidation of AtO3, such as by xenon difluoride (in a hot alkaline solution) or periodate (in a neutral or alkaline solution), yields the perastatate ion AtO4; this is only stable in neutral or alkaline solutions.[71] Astatine is also thought to be capable of forming cations in salts with oxyanions such as iodate or dichromate; this is based on the observation that, in acidic solutions, monovalent or intermediate positive states of astatine coprecipitate with the insoluble salts of metal cations such as silver(I) iodate or thallium(I) dichromate.[65][72]

Astatine may form bonds to the other chalcogens; these include S7At+ and At(CSN)2 with sulfur, a coordination selenourea compound with selenium, and an astatine–tellurium colloid with tellurium.[73]

 
Structure of astatine monoiodide, one of the astatine interhalogens and the heaviest known diatomic interhalogen

Astatine is known to react with its lighter homologs iodine, bromine, and chlorine in the vapor state; these reactions produce diatomic interhalogen compounds with formulas AtI, AtBr, and AtCl.[55] The first two compounds may also be produced in water – astatine reacts with iodine/iodide solution to form AtI, whereas AtBr requires (aside from astatine) an iodine/iodine monobromide/bromide solution. The excess of iodides or bromides may lead to AtBr2 and AtI2 ions,[55] or in a chloride solution, they may produce species like AtCl2 or AtBrCl via equilibrium reactions with the chlorides.[56] Oxidation of the element with dichromate (in nitric acid solution) showed that adding chloride turned the astatine into a molecule likely to be either AtCl or AtOCl. Similarly, AtOCl2 or AtCl2 may be produced.[55] The polyhalides PdAtI2, CsAtI2, TlAtI2,[74][75][76] and PbAtI[77] are known or presumed to have been precipitated. In a plasma ion source mass spectrometer, the ions [AtI]+, [AtBr]+, and [AtCl]+ have been formed by introducing lighter halogen vapors into a helium-filled cell containing astatine, supporting the existence of stable neutral molecules in the plasma ion state.[55] No astatine fluorides have been discovered yet. Their absence has been speculatively attributed to the extreme reactivity of such compounds, including the reaction of an initially formed fluoride with the walls of the glass container to form a non-volatile product.[e] Thus, although the synthesis of an astatine fluoride is thought to be possible, it may require a liquid halogen fluoride solvent, as has already been used for the characterization of radon fluoride.[55][71]

History edit

 
 
Dmitri Mendeleev's table of 1871, with an empty space at the eka-iodine position

In 1869, when Dmitri Mendeleev published his periodic table, the space under iodine was empty; after Niels Bohr established the physical basis of the classification of chemical elements, it was suggested that the fifth halogen belonged there. Before its officially recognized discovery, it was called "eka-iodine" (from Sanskrit eka – "one") to imply it was one space under iodine (in the same manner as eka-silicon, eka-boron, and others).[81] Scientists tried to find it in nature; given its extreme rarity, these attempts resulted in several false discoveries.[82]

The first claimed discovery of eka-iodine was made by Fred Allison and his associates at the Alabama Polytechnic Institute (now Auburn University) in 1931. The discoverers named element 85 "alabamine", and assigned it the symbol Ab, designations that were used for a few years.[83][84][85] In 1934, H. G. MacPherson of University of California, Berkeley disproved Allison's method and the validity of his discovery.[86] There was another claim in 1937, by the chemist Rajendralal De. Working in Dacca in British India (now Dhaka in Bangladesh), he chose the name "dakin" for element 85, which he claimed to have isolated as the thorium series equivalent of radium F (polonium-210) in the radium series.[87] The properties he reported for dakin do not correspond to those of astatine,[87] and astatine's radioactivity would have prevented him from handling it in the quantities he claimed.[88] Moreover, astatine is not found in the thorium series, and the true identity of dakin is not known.[87]

In 1936, the team of Romanian physicist Horia Hulubei and French physicist Yvette Cauchois claimed to have discovered element 85 by observing its X-ray emission lines. In 1939, they published another paper which supported and extended previous data. In 1944, Hulubei published a summary of data he had obtained up to that time, claiming it was supported by the work of other researchers. He chose the name "dor", presumably from the Romanian for "longing" [for peace], as World War II had started five years earlier. As Hulubei was writing in French, a language which does not accommodate the "ine" suffix, dor would likely have been rendered in English as "dorine", had it been adopted. In 1947, Hulubei's claim was effectively rejected by the Austrian chemist Friedrich Paneth, who would later chair the IUPAC committee responsible for recognition of new elements. Even though Hulubei's samples did contain astatine-218, his means to detect it were too weak, by current standards, to enable correct identification; moreover, he could not perform chemical tests on the element.[88] He had also been involved in an earlier false claim as to the discovery of element 87 (francium) and this is thought to have caused other researchers to downplay his work.[89]

 
Emilio Segrè, one of the discoverers of the main-group element astatine

In 1940, the Swiss chemist Walter Minder announced the discovery of element 85 as the beta decay product of radium A (polonium-218), choosing the name "helvetium" (from Helvetia, the Latin name of Switzerland). Berta Karlik and Traude Bernert were unsuccessful in reproducing his experiments, and subsequently attributed Minder's results to contamination of his radon stream (radon-222 is the parent isotope of polonium-218).[90][f] In 1942, Minder, in collaboration with the English scientist Alice Leigh-Smith, announced the discovery of another isotope of element 85, presumed to be the product of thorium A (polonium-216) beta decay. They named this substance "anglo-helvetium",[91] but Karlik and Bernert were again unable to reproduce these results.[53]

Later in 1940, Dale R. Corson, Kenneth Ross MacKenzie, and Emilio Segrè isolated the element at the University of California, Berkeley. Instead of searching for the element in nature, the scientists created it by bombarding bismuth-209 with alpha particles in a cyclotron (particle accelerator) to produce, after emission of two neutrons, astatine-211.[92] The discoverers, however, did not immediately suggest a name for the element. The reason for this was that at the time, an element created synthetically in "invisible quantities" that had not yet been discovered in nature was not seen as a completely valid one; in addition, chemists were reluctant to recognize radioactive isotopes as legitimately as stable ones.[93] In 1943, astatine was found as a product of two naturally occurring decay chains by Berta Karlik and Traude Bernert, first in the so-called uranium series, and then in the actinium series.[94][95] (Since then, astatine was also found in a third decay chain, the neptunium series.[96]) Friedrich Paneth in 1946 called to finally recognize synthetic elements, quoting, among other reasons, recent confirmation of their natural occurrence, and proposed that the discoverers of the newly discovered unnamed elements name these elements. In early 1947, Nature published the discoverers' suggestions; a letter from Corson, MacKenzie, and Segrè suggested the name "astatine"[93] coming from the Ancient Greek αστατος (astatos) meaning 'unstable', because of its propensity for radioactive decay, with the ending "-ine", found in the names of the four previously discovered halogens. The name was also chosen to continue the tradition of the four stable halogens, where the name referred to a property of the element.[97]

Corson and his colleagues classified astatine as a metal on the basis of its analytical chemistry.[98] Subsequent investigators reported iodine-like,[99][100] cationic,[101][102] or amphoteric behavior.[103][104] In a 2003 retrospective, Corson wrote that "some of the properties [of astatine] are similar to iodine ... it also exhibits metallic properties, more like its metallic neighbors Po and Bi."[97]

Isotopes edit

Alpha decay characteristics for sample astatine isotopes[g]
Mass
number
Half-life[6] Probability
of alpha
decay[6]
Alpha
decay
half-life
207 1.80 h 8.6% 20.9 h
208 1.63 h 0.55% 12.3 d
209 5.41 h 4.1% 5.5 d
210 8.1 h 0.175% 193 d
211 7.21 h 41.8% 17.2 h
212 0.31 s ≈100% 0.31 s
213 125 ns 100% 125 ns
214 558 ns 100% 558 ns
219 56 s 97% 58 s
220 3.71 min 8% 46.4 min
221 2.3 min experimentally
alpha stable

There are 41 known isotopes of astatine, with mass numbers of 188 and 190–229.[105][106] Theoretical modeling suggests that about 37 more isotopes could exist.[105] No stable or long-lived astatine isotope has been observed, nor is one expected to exist.[107]

Astatine's alpha decay energies follow the same trend as for other heavy elements.[107] Lighter astatine isotopes have quite high energies of alpha decay, which become lower as the nuclei become heavier. Astatine-211 has a significantly higher energy than the previous isotope, because it has a nucleus with 126 neutrons, and 126 is a magic number corresponding to a filled neutron shell. Despite having a similar half-life to the previous isotope (8.1 hours for astatine-210 and 7.2 hours for astatine-211), the alpha decay probability is much higher for the latter: 41.81% against only 0.18%.[6][h] The two following isotopes release even more energy, with astatine-213 releasing the most energy. For this reason, it is the shortest-lived astatine isotope.[107] Even though heavier astatine isotopes release less energy, no long-lived astatine isotope exists, because of the increasing role of beta decay (electron emission).[107] This decay mode is especially important for astatine; as early as 1950 it was postulated that all isotopes of the element undergo beta decay,[108] though nuclear mass measurements indicate that 215At is in fact beta-stable, as it has the lowest mass of all isobars with A = 215.[6] A beta decay mode has been found for all other astatine isotopes except for astatine-213, astatine-214, and astatine-216m.[6] Astatine-210 and lighter isotopes exhibit beta plus decay (positron emission), astatine-216 and heavier isotopes exhibit beta minus decay, and astatine-212 decays via both modes, while astatine-211 undergoes electron capture.[6]

The most stable isotope is astatine-210, which has a half-life of 8.1 hours. The primary decay mode is beta plus, to the relatively long-lived (in comparison to astatine isotopes) alpha emitter polonium-210. In total, only five isotopes have half-lives exceeding one hour (astatine-207 to -211). The least stable ground state isotope is astatine-213, with a half-life of 125 nanoseconds. It undergoes alpha decay to the extremely long-lived bismuth-209.[6]

Astatine has 24 known nuclear isomers, which are nuclei with one or more nucleons (protons or neutrons) in an excited state. A nuclear isomer may also be called a "meta-state", meaning the system has more internal energy than the "ground state" (the state with the lowest possible internal energy), making the former likely to decay into the latter. There may be more than one isomer for each isotope. The most stable of these nuclear isomers is astatine-202m1,[i] which has a half-life of about 3 minutes, longer than those of all the ground states bar those of isotopes 203–211 and 220. The least stable is astatine-214m1; its half-life of 265 nanoseconds is shorter than those of all ground states except that of astatine-213.[6][105]

Natural occurrence edit

 
Neptunium series, showing the decay products, including astatine-217, formed from neptunium-237

Astatine is the rarest naturally occurring element.[j] The total amount of astatine in the Earth's crust (quoted mass 2.36 × 1025 grams)[109] is estimated by some to be less than one gram at any given time.[8] Other sources estimate the amount of ephemeral astatine, present on earth at any given moment, to be up to one ounce[110] (about 28 grams).

Any astatine present at the formation of the Earth has long since disappeared; the four naturally occurring isotopes (astatine-215, -217, -218 and -219)[111] are instead continuously produced as a result of the decay of radioactive thorium and uranium ores, and trace quantities of neptunium-237. The landmass of North and South America combined, to a depth of 16 kilometers (10 miles), contains only about one trillion astatine-215 atoms at any given time (around 3.5 × 10−10 grams).[112] Astatine-217 is produced via the radioactive decay of neptunium-237. Primordial remnants of the latter isotope—due to its relatively short half-life of 2.14 million years—are no longer present on Earth. However, trace amounts occur naturally as a product of transmutation reactions in uranium ores.[113] Astatine-218 was the first astatine isotope discovered in nature.[114] Astatine-219, with a half-life of 56 seconds, is the longest lived of the naturally occurring isotopes.[6]

Isotopes of astatine are sometimes not listed as naturally occurring because of misconceptions[103] that there are no such isotopes,[115] or discrepancies in the literature. Astatine-216 has been counted as a naturally occurring isotope but reports of its observation[116] (which were described as doubtful) have not been confirmed.[117]

Synthesis edit

Formation edit

Possible reactions after bombarding bismuth-209 with alpha particles
Reaction[k] Energy of alpha particle
209
83
Bi
+ 4
2
He
211
85
At
+ 2 1
0
n
26 MeV[53]
209
83
Bi
+ 4
2
He
210
85
At
+ 3 1
0
n
40 MeV[53]
209
83
Bi
+ 4
2
He
209
85
At
+ 4 1
0
n
60 MeV[118]

Astatine was first produced by bombarding bismuth-209 with energetic alpha particles, and this is still the major route used to create the relatively long-lived isotopes astatine-209 through astatine-211. Astatine is only produced in minuscule quantities, with modern techniques allowing production runs of up to 6.6 gigabecquerels[119] (about 86 nanograms or 2.47×1014 atoms). Synthesis of greater quantities of astatine using this method is constrained by the limited availability of suitable cyclotrons and the prospect of melting the target.[119][120][l] Solvent radiolysis due to the cumulative effect of astatine decay[122] is a related problem. With cryogenic technology, microgram quantities of astatine might be able to be generated via proton irradiation of thorium or uranium to yield radon-211, in turn decaying to astatine-211. Contamination with astatine-210 is expected to be a drawback of this method.[123]

The most important isotope is astatine-211, the only one in commercial use. To produce the bismuth target, the metal is sputtered onto a gold, copper, or aluminium surface at 50 to 100 milligrams per square centimeter. Bismuth oxide can be used instead; this is forcibly fused with a copper plate.[124] The target is kept under a chemically neutral nitrogen atmosphere,[125] and is cooled with water to prevent premature astatine vaporization.[124] In a particle accelerator, such as a cyclotron,[126] alpha particles are collided with the bismuth. Even though only one bismuth isotope is used (bismuth-209), the reaction may occur in three possible ways, producing astatine-209, astatine-210, or astatine-211. In order to eliminate undesired nuclides, the maximum energy of the particle accelerator is set to a value (optimally 29.17 MeV)[127] above that for the reaction producing astatine-211 (to produce the desired isotope) and below the one producing astatine-210 (to avoid producing other astatine isotopes).[124]

Separation methods edit

Since astatine is the main product of the synthesis, after its formation it must only be separated from the target and any significant contaminants. Several methods are available, "but they generally follow one of two approaches—dry distillation or [wet] acid treatment of the target followed by solvent extraction." The methods summarized below are modern adaptations of older procedures, as reviewed by Kugler and Keller.[128][m] Pre-1985 techniques more often addressed the elimination of co-produced toxic polonium; this requirement is now mitigated by capping the energy of the cyclotron irradiation beam.[119]

Dry edit

The astatine-containing cyclotron target is heated to a temperature of around 650 °C. The astatine volatilizes and is condensed in (typically) a cold trap. Higher temperatures of up to around 850 °C may increase the yield, at the risk of bismuth contamination from concurrent volatilization. Redistilling the condensate may be required to minimize the presence of bismuth[130] (as bismuth can interfere with astatine labeling reactions). The astatine is recovered from the trap using one or more low concentration solvents such as sodium hydroxide, methanol or chloroform. Astatine yields of up to around 80% may be achieved. Dry separation is the method most commonly used to produce a chemically useful form of astatine.[120][131]

Wet edit

The irradiated bismuth (or sometimes bismuth trioxide) target is first dissolved in, for example, concentrated nitric or perchloric acid. Following this first step, the acid can be distilled away to leave behind a white residue that contains both bismuth and the desired astatine product. This residue is then dissolved in a concentrated acid, such as hydrochloric acid. Astatine is extracted from this acid using an organic solvent such as dibutyl ether, diisopropyl ether (DIPE), or thiosemicarbazide. Using liquid-liquid extraction, the astatine product can be repeatedly washed with an acid, such as HCl, and extracted into the organic solvent layer. A separation yield of 93% using nitric acid has been reported, falling to 72% by the time purification procedures were completed (distillation of nitric acid, purging residual nitrogen oxides, and redissolving bismuth nitrate to enable liquid–liquid extraction).[132][133] Wet methods involve "multiple radioactivity handling steps" and have not been considered well suited for isolating larger quantities of astatine. However, wet extraction methods are being examined for use in production of larger quantities of astatine-211, as it is thought that wet extraction methods can provide more consistency.[133] They can enable the production of astatine in a specific oxidation state and may have greater applicability in experimental radiochemistry.[119]

Uses and precautions edit

Several 211At-containing molecules and their experimental uses[134]
Agent Applications
[211At]astatine-tellurium colloids Compartmental tumors
6-[211At]astato-2-methyl-1,4-naphtaquinol diphosphate Adenocarcinomas
211At-labeled methylene blue Melanomas
Meta-[211At]astatobenzyl guanidine Neuroendocrine tumors
5-[211At]astato-2'-deoxyuridine Various
211At-labeled biotin conjugates Various pretargeting
211At-labeled octreotide Somatostatin receptor
211At-labeled monoclonal antibodies and fragments Various
211At-labeled bisphosphonates Bone metastases

Newly formed astatine-211 is the subject of ongoing research in nuclear medicine.[134] It must be used quickly as it decays with a half-life of 7.2 hours; this is long enough to permit multistep labeling strategies. Astatine-211 has potential for targeted alpha-particle therapy, since it decays either via emission of an alpha particle (to bismuth-207),[135] or via electron capture (to an extremely short-lived nuclide, polonium-211, which undergoes further alpha decay), very quickly reaching its stable granddaughter lead-207. Polonium X-rays emitted as a result of the electron capture branch, in the range of 77–92 keV, enable the tracking of astatine in animals and patients.[134] Although astatine-210 has a slightly longer half-life, it is wholly unsuitable because it usually undergoes beta plus decay to the extremely toxic polonium-210.[136]

The principal medicinal difference between astatine-211 and iodine-131 (a radioactive iodine isotope also used in medicine) is that iodine-131 emits high-energy beta particles, and astatine does not. Beta particles have much greater penetrating power through tissues than do the much heavier alpha particles. An average alpha particle released by astatine-211 can travel up to 70 µm through surrounding tissues; an average-energy beta particle emitted by iodine-131 can travel nearly 30 times as far, to about 2 mm.[124] The short half-life and limited penetrating power of alpha radiation through tissues offers advantages in situations where the "tumor burden is low and/or malignant cell populations are located in close proximity to essential normal tissues."[119] Significant morbidity in cell culture models of human cancers has been achieved with from one to ten astatine-211 atoms bound per cell.[137]

Astatine ... [is] miserable to make and hell to work with.[138]

P Durbin, Human Radiation Studies: Remembering the Early Years, 1995

Several obstacles have been encountered in the development of astatine-based radiopharmaceuticals for cancer treatment. World War II delayed research for close to a decade. Results of early experiments indicated that a cancer-selective carrier would need to be developed and it was not until the 1970s that monoclonal antibodies became available for this purpose. Unlike iodine, astatine shows a tendency to dehalogenate from molecular carriers such as these, particularly at sp3 carbon sites[n] (less so from sp2 sites). Given the toxicity of astatine accumulated and retained in the body, this emphasized the need to ensure it remained attached to its host molecule. While astatine carriers that are slowly metabolized can be assessed for their efficacy, more rapidly metabolized carriers remain a significant obstacle to the evaluation of astatine in nuclear medicine. Mitigating the effects of astatine-induced radiolysis of labeling chemistry and carrier molecules is another area requiring further development. A practical application for astatine as a cancer treatment would potentially be suitable for a "staggering" number of patients; production of astatine in the quantities that would be required remains an issue.[123][139][o]

Animal studies show that astatine, similarly to iodine—although to a lesser extent, perhaps because of its slightly more metallic nature[110]—is preferentially (and dangerously) concentrated in the thyroid gland. Unlike iodine, astatine also shows a tendency to be taken up by the lungs and spleen, possibly because of in-body oxidation of At to At+.[42] If administered in the form of a radiocolloid it tends to concentrate in the liver. Experiments in rats and monkeys suggest that astatine-211 causes much greater damage to the thyroid gland than does iodine-131, with repetitive injection of the nuclide resulting in necrosis and cell dysplasia within the gland.[140] Early research suggested that injection of astatine into female rodents caused morphological changes in breast tissue;[141] this conclusion remained controversial for many years. General agreement was later reached that this was likely caused by the effect of breast tissue irradiation combined with hormonal changes due to irradiation of the ovaries.[138] Trace amounts of astatine can be handled safely in fume hoods if they are well-aerated; biological uptake of the element must be avoided.[142]

See also edit

Notes edit

  1. ^ This half-vaporization period grows to 16 hours if it is instead put on a gold or platinum surface; this may be caused by poorly understood interactions between astatine and these noble metals.[17]
  2. ^ It is also possible that this is sorption on a cathode.[39]
  3. ^ The algorithm used to generate the Allred-Rochow scale fails in the case of hydrogen, providing a value that is close to that of oxygen (3.5). Hydrogen is instead assigned a value of 2.2. Despite this shortcoming, the Allred-Rochow scale has achieved a relatively high degree of acceptance.[49]
  4. ^ Iodine can act as a carrier despite it reacting with astatine in water because these reactions require iodide (I), not (only) I2.[55][56]
  5. ^ An initial attempt to fluoridate astatine using chlorine trifluoride resulted in formation of a product which became stuck to the glass. Chlorine monofluoride, chlorine, and tetrafluorosilane were formed. The authors called the effect "puzzling", admitting they had expected formation of a volatile fluoride.[78] Ten years later, the compound was predicted to be non-volatile, out of line with the lighter halogens but similar to radon fluoride;[79] by this time, the latter had been shown to be ionic.[80]
  6. ^ In other words, some other substance was undergoing beta decay (to a different end element), not polonium-218.
  7. ^ In the table, "alpha decay half-life" refers to the half-life if decay modes other than alpha are omitted.
  8. ^ This means that, if decay modes other than alpha are omitted, then astatine-210 has an alpha decay half-life of 4,628.6 hours (128.9 days) and astatine-211 has one of only 17.2 hours (0.7 days). Therefore, astatine-211 is very much less stable toward alpha decay than astatine-210.
  9. ^ "m1" means that this state of the isotope is the next possible one above – with an energy greater than – the ground state. "m2" and similar designations refer to further higher energy states. The number may be dropped if there is only one well-established meta state, such as astatine-216m. Other designation techniques are sometimes used.
  10. ^ Emsley[9] states that this title has been lost to berkelium, "a few atoms of which can be produced in very-highly concentrated uranium-bearing deposits"; however, his assertion is not corroborated by any primary source.
  11. ^ A nuclide is commonly denoted by a symbol of the chemical element this nuclide belongs to, preceded by a non-spaced superscript mass number and a subscript atomic number of the nuclide located directly under the mass number. (Neutrons may be considered as nuclei with the atomic mass of 1 and the atomic charge of 0, with the symbol being n.) With the atomic number omitted, it is also sometimes used as a designation of an isotope of an element in isotope-related chemistry.
  12. ^ See however Nagatsu et al.[121] who encapsulate the bismuth target in a thin aluminium foil and place it in a niobium holder capable of holding molten bismuth.
  13. ^ See also Lavrukhina and Pozdnyakov.[129]
  14. ^ In other words, where carbon's one s atomic orbital and three p orbitals hybridize to give four new orbitals shaped as intermediates between the original s and p orbitals.
  15. ^ "Unfortunately, the conundrum confronting the … field is that commercial supply of 211At awaits the demonstration of clinical efficacy; however, the demonstration of clinical efficacy requires a reliable supply of 211At."[119]

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Bibliography edit

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External links edit

astatine, chemical, element, symbol, atomic, number, rarest, naturally, occurring, element, earth, crust, occurring, only, decay, product, various, heavier, elements, astatine, isotopes, short, lived, most, stable, astatine, with, half, life, hours, consequent. Astatine is a chemical element it has symbol At and atomic number 85 It is the rarest naturally occurring element in the Earth s crust occurring only as the decay product of various heavier elements All of astatine s isotopes are short lived the most stable is astatine 210 with a half life of 8 1 hours Consequently a solid sample of the element has never been seen because any macroscopic specimen would be immediately vaporized by the heat of its radioactivity Astatine 85AtAstatinePronunciation ˈ ae s t e t iː n t ɪ n wbr ASS te teen tin Appearanceunknown probably metallicMass number 210 Astatine in the periodic tableHydrogen HeliumLithium Beryllium Boron Carbon Nitrogen Oxygen Fluorine NeonSodium Magnesium Aluminium Silicon Phosphorus Sulfur Chlorine ArgonPotassium Calcium Scandium Titanium Vanadium Chromium Manganese Iron Cobalt Nickel Copper Zinc Gallium Germanium Arsenic Selenium Bromine KryptonRubidium Strontium Yttrium Zirconium Niobium Molybdenum Technetium Ruthenium Rhodium Palladium Silver Cadmium Indium Tin Antimony Tellurium Iodine XenonCaesium Barium Lanthanum Cerium Praseodymium Neodymium Promethium Samarium Europium Gadolinium Terbium Dysprosium Holmium Erbium Thulium Ytterbium Lutetium Hafnium Tantalum Tungsten Rhenium Osmium Iridium Platinum Gold Mercury element Thallium Lead Bismuth Polonium Astatine RadonFrancium Radium Actinium Thorium Protactinium Uranium Neptunium Plutonium Americium Curium Berkelium Californium Einsteinium Fermium Mendelevium Nobelium Lawrencium Rutherfordium Dubnium Seaborgium Bohrium Hassium Meitnerium Darmstadtium Roentgenium Copernicium Nihonium Flerovium Moscovium Livermorium Tennessine Oganesson I At Tspolonium astatine radonAtomic number Z 85Groupgroup 17 halogens Periodperiod 6Block p blockElectron configuration Xe 4f14 5d10 6s2 6p5Electrons per shell2 8 18 32 18 7Physical propertiesPhase at STPsolid predicted Density near r t 8 91 8 95 g cm3 estimated 1 Molar volume23 6 cm3 mol estimated 1 Atomic propertiesOxidation states 1 1 3 5 7 2 Ionization energies1st 899 003 kJ mol 3 Other propertiesNatural occurrencefrom decayCrystal structure face centered cubic fcc predicted 4 CAS Number7440 68 8HistoryNamingfrom Ancient Greek ἄstatos astatos unstable DiscoveryDale R Corson Kenneth Ross MacKenzie Emilio Segre 1940 Isotopes of astatineveMain isotopes 5 Decayabun dance half life t1 2 mode pro duct209At synth 5 41 h b 209Poa 205Bi210At synth 8 1 h b 210Poa 206Bi211At synth 7 21 h e 211Poa 207Bi Category Astatineviewtalkedit referencesThe bulk properties of astatine are not known with certainty Many of them have been estimated from its position on the periodic table as a heavier analog of fluorine chlorine bromine and iodine the four stable halogens However astatine also falls roughly along the dividing line between metals and nonmetals and some metallic behavior has also been observed and predicted for it Astatine is likely to have a dark or lustrous appearance and may be a semiconductor or possibly a metal Chemically several anionic species of astatine are known and most of its compounds resemble those of iodine but it also sometimes displays metallic characteristics and shows some similarities to silver The first synthesis of astatine was in 1940 by Dale R Corson Kenneth Ross MacKenzie and Emilio G Segre at the University of California Berkeley They named it from the Ancient Greek ἄstatos astatos unstable Four isotopes of astatine were subsequently found to be naturally occurring although much less than one gram is present at any given time in the Earth s crust Neither the most stable isotope astatine 210 nor the medically useful astatine 211 occur naturally they are usually produced by bombarding bismuth 209 with alpha particles Contents 1 Characteristics 1 1 Physical 1 2 Chemical 2 Compounds 3 History 4 Isotopes 5 Natural occurrence 6 Synthesis 6 1 Formation 6 2 Separation methods 6 2 1 Dry 6 2 2 Wet 7 Uses and precautions 8 See also 9 Notes 10 References 11 Bibliography 12 External linksCharacteristics editAstatine is an extremely radioactive element all its isotopes have half lives of 8 1 hours or less decaying into other astatine isotopes bismuth polonium or radon Most of its isotopes are very unstable with half lives of seconds or less Of the first 101 elements in the periodic table only francium is less stable and all the astatine isotopes more stable than the longest lived francium isotopes 205 211At are in any case synthetic and do not occur in nature 6 The bulk properties of astatine are not known with any certainty 7 Research is limited by its short half life which prevents the creation of weighable quantities 8 A visible piece of astatine would immediately vaporize itself because of the heat generated by its intense radioactivity 9 It remains to be seen if with sufficient cooling a macroscopic quantity of astatine could be deposited as a thin film 4 Astatine is usually classified as either a nonmetal or a metalloid 10 11 metal formation has also been predicted 4 12 Physical edit Most of the physical properties of astatine have been estimated by interpolation or extrapolation using theoretically or empirically derived methods 13 For example halogens get darker with increasing atomic weight fluorine is nearly colorless chlorine is yellow green bromine is red brown and iodine is dark gray violet Astatine is sometimes described as probably being a black solid assuming it follows this trend or as having a metallic appearance if it is a metalloid or a metal 14 15 16 Astatine sublimes less readily than iodine having a lower vapor pressure 8 Even so half of a given quantity of astatine will vaporize in approximately an hour if put on a clean glass surface at room temperature a The absorption spectrum of astatine in the middle ultraviolet region has lines at 224 401 and 216 225 nm suggestive of 6p to 7s transitions 18 19 The structure of solid astatine is unknown 20 As an analog of iodine it may have an orthorhombic crystalline structure composed of diatomic astatine molecules and be a semiconductor with a band gap of 0 7 eV 21 22 Alternatively if condensed astatine forms a metallic phase as has been predicted it may have a monatomic face centered cubic structure in this structure it may well be a superconductor like the similar high pressure phase of iodine 4 Metallic astatine is expected to have a density of 8 91 8 95 g cm3 1 Evidence for or against the existence of diatomic astatine At2 is sparse and inconclusive 23 24 25 26 27 Some sources state that it does not exist or at least has never been observed 28 29 while other sources assert or imply its existence 30 31 32 Despite this controversy many properties of diatomic astatine have been predicted 33 for example its bond length would be 300 10 pm dissociation energy 83 7 12 5 kJ mol 34 and heat of vaporization Hvap 54 39 kJ mol 35 Many values have been predicted for the melting and boiling points of astatine but only for At2 36 Chemical edit The chemistry of astatine is clouded by the extremely low concentrations at which astatine experiments have been conducted and the possibility of reactions with impurities walls and filters or radioactivity by products and other unwanted nano scale interactions 21 Many of its apparent chemical properties have been observed using tracer studies on extremely dilute astatine solutions 32 37 typically less than 10 10 mol L 1 38 Some properties such as anion formation align with other halogens 8 Astatine has some metallic characteristics as well such as plating onto a cathode b and coprecipitating with metal sulfides in hydrochloric acid 40 It forms complexes with EDTA a metal chelating agent 41 and is capable of acting as a metal in antibody radiolabeling in some respects astatine in the 1 state is akin to silver in the same state Most of the organic chemistry of astatine is however analogous to that of iodine 42 It has been suggested that astatine can form a stable monatomic cation in aqueous solution 40 43 Astatine has an electronegativity of 2 2 on the revised Pauling scale lower than that of iodine 2 66 and the same as hydrogen In hydrogen astatide HAt the negative charge is predicted to be on the hydrogen atom implying that this compound could be referred to as astatine hydride according to certain nomenclatures 44 45 46 47 That would be consistent with the electronegativity of astatine on the Allred Rochow scale 1 9 being less than that of hydrogen 2 2 48 c However official IUPAC stoichiometric nomenclature is based on an idealized convention of determining the relative electronegativities of the elements by the mere virtue of their position within the periodic table According to this convention astatine is handled as though it is more electronegative than hydrogen irrespective of its true electronegativity The electron affinity of astatine at 233 kJ mol 1 is 21 less than that of iodine 50 In comparison the value of Cl 349 is 6 4 higher than F 328 Br 325 is 6 9 less than Cl and I 295 is 9 2 less than Br The marked reduction for At was predicted as being due to spin orbit interactions 38 The first ionization energy of astatine is about 899 kJ mol 1 which continues the trend of decreasing first ionization energies down the halogen group fluorine 1681 chlorine 1251 bromine 1140 iodine 1008 3 Compounds editMain article Astatine compounds Less reactive than iodine astatine is the least reactive of the halogens 51 the chemical properties of tennessine the next heavier group 17 element have not yet been investigated however 52 Astatine compounds have been synthesized in nano scale amounts and studied as intensively as possible before their radioactive disintegration The reactions involved have been typically tested with dilute solutions of astatine mixed with larger amounts of iodine Acting as a carrier the iodine ensures there is sufficient material for laboratory techniques such as filtration and precipitation to work 53 54 d Like iodine astatine has been shown to adopt odd numbered oxidation states ranging from 1 to 7 57 Only a few compounds with metals have been reported in the form of astatides of sodium 9 palladium silver thallium and lead 58 Some characteristic properties of silver and sodium astatide and the other hypothetical alkali and alkaline earth astatides have been estimated by extrapolation from other metal halides 59 nbsp Hydrogen astatide space filling modelThe formation of an astatine compound with hydrogen usually referred to as hydrogen astatide was noted by the pioneers of astatine chemistry 60 As mentioned there are grounds for instead referring to this compound as astatine hydride It is easily oxidized acidification by dilute nitric acid gives the At0 or At forms and the subsequent addition of silver I may only partially at best precipitate astatine as silver I astatide AgAt Iodine in contrast is not oxidized and precipitates readily as silver I iodide 8 61 Astatine is known to bind to boron 62 carbon and nitrogen 63 Various boron cage compounds have been prepared with At B bonds these being more stable than At C bonds 64 Astatine can replace a hydrogen atom in benzene to form astatobenzene C6H5At this may be oxidized to C6H5AtCl2 by chlorine By treating this compound with an alkaline solution of hypochlorite C6H5AtO2 can be produced 65 The dipyridine astatine I cation At C5H5N 2 forms ionic compounds with perchlorate 63 a non coordinating anion 66 and with nitrate At C5H5N 2 NO3 63 This cation exists as a coordination complex in which two dative covalent bonds separately link the astatine I centre with each of the pyridine rings via their nitrogen atoms 63 With oxygen there is evidence of the species AtO and AtO in aqueous solution formed by the reaction of astatine with an oxidant such as elemental bromine or in the last case by sodium persulfate in a solution of perchloric acid 8 67 The species previously thought to be AtO 2 has since been determined to be AtO OH 2 a hydrolysis product of AtO another such hydrolysis product being AtOOH 68 The well characterized AtO 3 anion can be obtained by for example the oxidation of astatine with potassium hypochlorite in a solution of potassium hydroxide 65 69 Preparation of lanthanum triastatate La AtO3 3 following the oxidation of astatine by a hot Na2S2O8 solution has been reported 70 Further oxidation of AtO 3 such as by xenon difluoride in a hot alkaline solution or periodate in a neutral or alkaline solution yields the perastatate ion AtO 4 this is only stable in neutral or alkaline solutions 71 Astatine is also thought to be capable of forming cations in salts with oxyanions such as iodate or dichromate this is based on the observation that in acidic solutions monovalent or intermediate positive states of astatine coprecipitate with the insoluble salts of metal cations such as silver I iodate or thallium I dichromate 65 72 Astatine may form bonds to the other chalcogens these include S7At and At CSN 2 with sulfur a coordination selenourea compound with selenium and an astatine tellurium colloid with tellurium 73 nbsp Structure of astatine monoiodide one of the astatine interhalogens and the heaviest known diatomic interhalogenAstatine is known to react with its lighter homologs iodine bromine and chlorine in the vapor state these reactions produce diatomic interhalogen compounds with formulas AtI AtBr and AtCl 55 The first two compounds may also be produced in water astatine reacts with iodine iodide solution to form AtI whereas AtBr requires aside from astatine an iodine iodine monobromide bromide solution The excess of iodides or bromides may lead to AtBr 2 and AtI 2 ions 55 or in a chloride solution they may produce species like AtCl 2 or AtBrCl via equilibrium reactions with the chlorides 56 Oxidation of the element with dichromate in nitric acid solution showed that adding chloride turned the astatine into a molecule likely to be either AtCl or AtOCl Similarly AtOCl 2 or AtCl 2 may be produced 55 The polyhalides PdAtI2 CsAtI2 TlAtI2 74 75 76 and PbAtI 77 are known or presumed to have been precipitated In a plasma ion source mass spectrometer the ions AtI AtBr and AtCl have been formed by introducing lighter halogen vapors into a helium filled cell containing astatine supporting the existence of stable neutral molecules in the plasma ion state 55 No astatine fluorides have been discovered yet Their absence has been speculatively attributed to the extreme reactivity of such compounds including the reaction of an initially formed fluoride with the walls of the glass container to form a non volatile product e Thus although the synthesis of an astatine fluoride is thought to be possible it may require a liquid halogen fluoride solvent as has already been used for the characterization of radon fluoride 55 71 History edit nbsp nbsp Dmitri Mendeleev s table of 1871 with an empty space at the eka iodine position In 1869 when Dmitri Mendeleev published his periodic table the space under iodine was empty after Niels Bohr established the physical basis of the classification of chemical elements it was suggested that the fifth halogen belonged there Before its officially recognized discovery it was called eka iodine from Sanskrit eka one to imply it was one space under iodine in the same manner as eka silicon eka boron and others 81 Scientists tried to find it in nature given its extreme rarity these attempts resulted in several false discoveries 82 The first claimed discovery of eka iodine was made by Fred Allison and his associates at the Alabama Polytechnic Institute now Auburn University in 1931 The discoverers named element 85 alabamine and assigned it the symbol Ab designations that were used for a few years 83 84 85 In 1934 H G MacPherson of University of California Berkeley disproved Allison s method and the validity of his discovery 86 There was another claim in 1937 by the chemist Rajendralal De Working in Dacca in British India now Dhaka in Bangladesh he chose the name dakin for element 85 which he claimed to have isolated as the thorium series equivalent of radium F polonium 210 in the radium series 87 The properties he reported for dakin do not correspond to those of astatine 87 and astatine s radioactivity would have prevented him from handling it in the quantities he claimed 88 Moreover astatine is not found in the thorium series and the true identity of dakin is not known 87 In 1936 the team of Romanian physicist Horia Hulubei and French physicist Yvette Cauchois claimed to have discovered element 85 by observing its X ray emission lines In 1939 they published another paper which supported and extended previous data In 1944 Hulubei published a summary of data he had obtained up to that time claiming it was supported by the work of other researchers He chose the name dor presumably from the Romanian for longing for peace as World War II had started five years earlier As Hulubei was writing in French a language which does not accommodate the ine suffix dor would likely have been rendered in English as dorine had it been adopted In 1947 Hulubei s claim was effectively rejected by the Austrian chemist Friedrich Paneth who would later chair the IUPAC committee responsible for recognition of new elements Even though Hulubei s samples did contain astatine 218 his means to detect it were too weak by current standards to enable correct identification moreover he could not perform chemical tests on the element 88 He had also been involved in an earlier false claim as to the discovery of element 87 francium and this is thought to have caused other researchers to downplay his work 89 nbsp Emilio Segre one of the discoverers of the main group element astatineIn 1940 the Swiss chemist Walter Minder announced the discovery of element 85 as the beta decay product of radium A polonium 218 choosing the name helvetium from Helvetia the Latin name of Switzerland Berta Karlik and Traude Bernert were unsuccessful in reproducing his experiments and subsequently attributed Minder s results to contamination of his radon stream radon 222 is the parent isotope of polonium 218 90 f In 1942 Minder in collaboration with the English scientist Alice Leigh Smith announced the discovery of another isotope of element 85 presumed to be the product of thorium A polonium 216 beta decay They named this substance anglo helvetium 91 but Karlik and Bernert were again unable to reproduce these results 53 Later in 1940 Dale R Corson Kenneth Ross MacKenzie and Emilio Segre isolated the element at the University of California Berkeley Instead of searching for the element in nature the scientists created it by bombarding bismuth 209 with alpha particles in a cyclotron particle accelerator to produce after emission of two neutrons astatine 211 92 The discoverers however did not immediately suggest a name for the element The reason for this was that at the time an element created synthetically in invisible quantities that had not yet been discovered in nature was not seen as a completely valid one in addition chemists were reluctant to recognize radioactive isotopes as legitimately as stable ones 93 In 1943 astatine was found as a product of two naturally occurring decay chains by Berta Karlik and Traude Bernert first in the so called uranium series and then in the actinium series 94 95 Since then astatine was also found in a third decay chain the neptunium series 96 Friedrich Paneth in 1946 called to finally recognize synthetic elements quoting among other reasons recent confirmation of their natural occurrence and proposed that the discoverers of the newly discovered unnamed elements name these elements In early 1947 Nature published the discoverers suggestions a letter from Corson MacKenzie and Segre suggested the name astatine 93 coming from the Ancient Greek astatos astatos meaning unstable because of its propensity for radioactive decay with the ending ine found in the names of the four previously discovered halogens The name was also chosen to continue the tradition of the four stable halogens where the name referred to a property of the element 97 Corson and his colleagues classified astatine as a metal on the basis of its analytical chemistry 98 Subsequent investigators reported iodine like 99 100 cationic 101 102 or amphoteric behavior 103 104 In a 2003 retrospective Corson wrote that some of the properties of astatine are similar to iodine it also exhibits metallic properties more like its metallic neighbors Po and Bi 97 Isotopes editMain article Isotopes of astatine Alpha decay characteristics for sample astatine isotopes g Massnumber Half life 6 Probabilityof alphadecay 6 Alphadecayhalf life207 1 80 h 8 6 20 9 h208 1 63 h 0 55 12 3 d209 5 41 h 4 1 5 5 d210 8 1 h 0 175 193 d211 7 21 h 41 8 17 2 h212 0 31 s 100 0 31 s213 125 ns 100 125 ns214 558 ns 100 558 ns219 56 s 97 58 s220 3 71 min 8 46 4 min221 2 3 min experimentallyalpha stable There are 41 known isotopes of astatine with mass numbers of 188 and 190 229 105 106 Theoretical modeling suggests that about 37 more isotopes could exist 105 No stable or long lived astatine isotope has been observed nor is one expected to exist 107 Astatine s alpha decay energies follow the same trend as for other heavy elements 107 Lighter astatine isotopes have quite high energies of alpha decay which become lower as the nuclei become heavier Astatine 211 has a significantly higher energy than the previous isotope because it has a nucleus with 126 neutrons and 126 is a magic number corresponding to a filled neutron shell Despite having a similar half life to the previous isotope 8 1 hours for astatine 210 and 7 2 hours for astatine 211 the alpha decay probability is much higher for the latter 41 81 against only 0 18 6 h The two following isotopes release even more energy with astatine 213 releasing the most energy For this reason it is the shortest lived astatine isotope 107 Even though heavier astatine isotopes release less energy no long lived astatine isotope exists because of the increasing role of beta decay electron emission 107 This decay mode is especially important for astatine as early as 1950 it was postulated that all isotopes of the element undergo beta decay 108 though nuclear mass measurements indicate that 215At is in fact beta stable as it has the lowest mass of all isobars with A 215 6 A beta decay mode has been found for all other astatine isotopes except for astatine 213 astatine 214 and astatine 216m 6 Astatine 210 and lighter isotopes exhibit beta plus decay positron emission astatine 216 and heavier isotopes exhibit beta minus decay and astatine 212 decays via both modes while astatine 211 undergoes electron capture 6 The most stable isotope is astatine 210 which has a half life of 8 1 hours The primary decay mode is beta plus to the relatively long lived in comparison to astatine isotopes alpha emitter polonium 210 In total only five isotopes have half lives exceeding one hour astatine 207 to 211 The least stable ground state isotope is astatine 213 with a half life of 125 nanoseconds It undergoes alpha decay to the extremely long lived bismuth 209 6 Astatine has 24 known nuclear isomers which are nuclei with one or more nucleons protons or neutrons in an excited state A nuclear isomer may also be called a meta state meaning the system has more internal energy than the ground state the state with the lowest possible internal energy making the former likely to decay into the latter There may be more than one isomer for each isotope The most stable of these nuclear isomers is astatine 202m1 i which has a half life of about 3 minutes longer than those of all the ground states bar those of isotopes 203 211 and 220 The least stable is astatine 214m1 its half life of 265 nanoseconds is shorter than those of all ground states except that of astatine 213 6 105 Natural occurrence edit nbsp Neptunium series showing the decay products including astatine 217 formed from neptunium 237Astatine is the rarest naturally occurring element j The total amount of astatine in the Earth s crust quoted mass 2 36 1025 grams 109 is estimated by some to be less than one gram at any given time 8 Other sources estimate the amount of ephemeral astatine present on earth at any given moment to be up to one ounce 110 about 28 grams Any astatine present at the formation of the Earth has long since disappeared the four naturally occurring isotopes astatine 215 217 218 and 219 111 are instead continuously produced as a result of the decay of radioactive thorium and uranium ores and trace quantities of neptunium 237 The landmass of North and South America combined to a depth of 16 kilometers 10 miles contains only about one trillion astatine 215 atoms at any given time around 3 5 10 10 grams 112 Astatine 217 is produced via the radioactive decay of neptunium 237 Primordial remnants of the latter isotope due to its relatively short half life of 2 14 million years are no longer present on Earth However trace amounts occur naturally as a product of transmutation reactions in uranium ores 113 Astatine 218 was the first astatine isotope discovered in nature 114 Astatine 219 with a half life of 56 seconds is the longest lived of the naturally occurring isotopes 6 Isotopes of astatine are sometimes not listed as naturally occurring because of misconceptions 103 that there are no such isotopes 115 or discrepancies in the literature Astatine 216 has been counted as a naturally occurring isotope but reports of its observation 116 which were described as doubtful have not been confirmed 117 Synthesis editFormation edit Possible reactions after bombarding bismuth 209 with alpha particles Reaction k Energy of alpha particle20983 Bi 42 He 21185 At 2 10 n 26 MeV 53 20983 Bi 42 He 21085 At 3 10 n 40 MeV 53 20983 Bi 42 He 20985 At 4 10 n 60 MeV 118 Astatine was first produced by bombarding bismuth 209 with energetic alpha particles and this is still the major route used to create the relatively long lived isotopes astatine 209 through astatine 211 Astatine is only produced in minuscule quantities with modern techniques allowing production runs of up to 6 6 gigabecquerels 119 about 86 nanograms or 2 47 1014 atoms Synthesis of greater quantities of astatine using this method is constrained by the limited availability of suitable cyclotrons and the prospect of melting the target 119 120 l Solvent radiolysis due to the cumulative effect of astatine decay 122 is a related problem With cryogenic technology microgram quantities of astatine might be able to be generated via proton irradiation of thorium or uranium to yield radon 211 in turn decaying to astatine 211 Contamination with astatine 210 is expected to be a drawback of this method 123 The most important isotope is astatine 211 the only one in commercial use To produce the bismuth target the metal is sputtered onto a gold copper or aluminium surface at 50 to 100 milligrams per square centimeter Bismuth oxide can be used instead this is forcibly fused with a copper plate 124 The target is kept under a chemically neutral nitrogen atmosphere 125 and is cooled with water to prevent premature astatine vaporization 124 In a particle accelerator such as a cyclotron 126 alpha particles are collided with the bismuth Even though only one bismuth isotope is used bismuth 209 the reaction may occur in three possible ways producing astatine 209 astatine 210 or astatine 211 In order to eliminate undesired nuclides the maximum energy of the particle accelerator is set to a value optimally 29 17 MeV 127 above that for the reaction producing astatine 211 to produce the desired isotope and below the one producing astatine 210 to avoid producing other astatine isotopes 124 Separation methods edit Since astatine is the main product of the synthesis after its formation it must only be separated from the target and any significant contaminants Several methods are available but they generally follow one of two approaches dry distillation or wet acid treatment of the target followed by solvent extraction The methods summarized below are modern adaptations of older procedures as reviewed by Kugler and Keller 128 m Pre 1985 techniques more often addressed the elimination of co produced toxic polonium this requirement is now mitigated by capping the energy of the cyclotron irradiation beam 119 Dry edit The astatine containing cyclotron target is heated to a temperature of around 650 C The astatine volatilizes and is condensed in typically a cold trap Higher temperatures of up to around 850 C may increase the yield at the risk of bismuth contamination from concurrent volatilization Redistilling the condensate may be required to minimize the presence of bismuth 130 as bismuth can interfere with astatine labeling reactions The astatine is recovered from the trap using one or more low concentration solvents such as sodium hydroxide methanol or chloroform Astatine yields of up to around 80 may be achieved Dry separation is the method most commonly used to produce a chemically useful form of astatine 120 131 Wet edit The irradiated bismuth or sometimes bismuth trioxide target is first dissolved in for example concentrated nitric or perchloric acid Following this first step the acid can be distilled away to leave behind a white residue that contains both bismuth and the desired astatine product This residue is then dissolved in a concentrated acid such as hydrochloric acid Astatine is extracted from this acid using an organic solvent such as dibutyl ether diisopropyl ether DIPE or thiosemicarbazide Using liquid liquid extraction the astatine product can be repeatedly washed with an acid such as HCl and extracted into the organic solvent layer A separation yield of 93 using nitric acid has been reported falling to 72 by the time purification procedures were completed distillation of nitric acid purging residual nitrogen oxides and redissolving bismuth nitrate to enable liquid liquid extraction 132 133 Wet methods involve multiple radioactivity handling steps and have not been considered well suited for isolating larger quantities of astatine However wet extraction methods are being examined for use in production of larger quantities of astatine 211 as it is thought that wet extraction methods can provide more consistency 133 They can enable the production of astatine in a specific oxidation state and may have greater applicability in experimental radiochemistry 119 Uses and precautions editSeveral 211At containing molecules and their experimental uses 134 Agent Applications 211At astatine tellurium colloids Compartmental tumors6 211At astato 2 methyl 1 4 naphtaquinol diphosphate Adenocarcinomas211At labeled methylene blue MelanomasMeta 211At astatobenzyl guanidine Neuroendocrine tumors5 211At astato 2 deoxyuridine Various211At labeled biotin conjugates Various pretargeting211At labeled octreotide Somatostatin receptor211At labeled monoclonal antibodies and fragments Various211At labeled bisphosphonates Bone metastases Newly formed astatine 211 is the subject of ongoing research in nuclear medicine 134 It must be used quickly as it decays with a half life of 7 2 hours this is long enough to permit multistep labeling strategies Astatine 211 has potential for targeted alpha particle therapy since it decays either via emission of an alpha particle to bismuth 207 135 or via electron capture to an extremely short lived nuclide polonium 211 which undergoes further alpha decay very quickly reaching its stable granddaughter lead 207 Polonium X rays emitted as a result of the electron capture branch in the range of 77 92 keV enable the tracking of astatine in animals and patients 134 Although astatine 210 has a slightly longer half life it is wholly unsuitable because it usually undergoes beta plus decay to the extremely toxic polonium 210 136 The principal medicinal difference between astatine 211 and iodine 131 a radioactive iodine isotope also used in medicine is that iodine 131 emits high energy beta particles and astatine does not Beta particles have much greater penetrating power through tissues than do the much heavier alpha particles An average alpha particle released by astatine 211 can travel up to 70 µm through surrounding tissues an average energy beta particle emitted by iodine 131 can travel nearly 30 times as far to about 2 mm 124 The short half life and limited penetrating power of alpha radiation through tissues offers advantages in situations where the tumor burden is low and or malignant cell populations are located in close proximity to essential normal tissues 119 Significant morbidity in cell culture models of human cancers has been achieved with from one to ten astatine 211 atoms bound per cell 137 Astatine is miserable to make and hell to work with 138 P Durbin Human Radiation Studies Remembering the Early Years 1995 Several obstacles have been encountered in the development of astatine based radiopharmaceuticals for cancer treatment World War II delayed research for close to a decade Results of early experiments indicated that a cancer selective carrier would need to be developed and it was not until the 1970s that monoclonal antibodies became available for this purpose Unlike iodine astatine shows a tendency to dehalogenate from molecular carriers such as these particularly at sp3 carbon sites n less so from sp2 sites Given the toxicity of astatine accumulated and retained in the body this emphasized the need to ensure it remained attached to its host molecule While astatine carriers that are slowly metabolized can be assessed for their efficacy more rapidly metabolized carriers remain a significant obstacle to the evaluation of astatine in nuclear medicine Mitigating the effects of astatine induced radiolysis of labeling chemistry and carrier molecules is another area requiring further development A practical application for astatine as a cancer treatment would potentially be suitable for a staggering number of patients production of astatine in the quantities that would be required remains an issue 123 139 o Animal studies show that astatine similarly to iodine although to a lesser extent perhaps because of its slightly more metallic nature 110 is preferentially and dangerously concentrated in the thyroid gland Unlike iodine astatine also shows a tendency to be taken up by the lungs and spleen possibly because of in body oxidation of At to At 42 If administered in the form of a radiocolloid it tends to concentrate in the liver Experiments in rats and monkeys suggest that astatine 211 causes much greater damage to the thyroid gland than does iodine 131 with repetitive injection of the nuclide resulting in necrosis and cell dysplasia within the gland 140 Early research suggested that injection of astatine into female rodents caused morphological changes in breast tissue 141 this conclusion remained controversial for many years General agreement was later reached that this was likely caused by the effect of breast tissue irradiation combined with hormonal changes due to irradiation of the ovaries 138 Trace amounts of astatine can be handled safely in fume hoods if they are well aerated biological uptake of the element must be avoided 142 See also edit nbsp Chemistry portalRadiation protectionNotes edit This half vaporization period grows to 16 hours if it is instead put on a gold or platinum surface this may be caused by poorly understood interactions between astatine and these noble metals 17 It is also possible that this is sorption on a cathode 39 The algorithm used to generate the Allred Rochow scale fails in the case of hydrogen providing a value that is close to that of oxygen 3 5 Hydrogen is instead assigned a value of 2 2 Despite this shortcoming the Allred Rochow scale has achieved a relatively high degree of acceptance 49 Iodine can act as a carrier despite it reacting with astatine in water because these reactions require iodide I not only I2 55 56 An initial attempt to fluoridate astatine using chlorine trifluoride resulted in formation of a product which became stuck to the glass Chlorine monofluoride chlorine and tetrafluorosilane were formed The authors called the effect puzzling admitting they had expected formation of a volatile fluoride 78 Ten years later the compound was predicted to be non volatile out of line with the lighter halogens but similar to radon fluoride 79 by this time the latter had been shown to be ionic 80 In other words some other substance was undergoing beta decay to a different end element not polonium 218 In the table alpha decay half life refers to the half life if decay modes other than alpha are omitted This means that if decay modes other than alpha are omitted then astatine 210 has an alpha decay half life of 4 628 6 hours 128 9 days and astatine 211 has one of only 17 2 hours 0 7 days Therefore astatine 211 is very much less stable toward alpha decay than astatine 210 m1 means that this state of the isotope is the next possible one above with an energy greater than the ground state m2 and similar designations refer to further higher energy states The number may be dropped if there is only one well established meta state such as astatine 216m Other designation techniques are sometimes used Emsley 9 states that this title has been lost to berkelium a few atoms of which can be produced in very highly concentrated uranium bearing deposits however his assertion is not corroborated by any primary source A nuclide is commonly denoted by a symbol of the chemical element this nuclide belongs to preceded by a non spaced superscript mass number and a subscript atomic number of the nuclide located directly under the mass number Neutrons may be considered as nuclei with the atomic mass of 1 and the atomic charge of 0 with the symbol being n With the atomic number omitted it is also sometimes used as a designation of an isotope of an element in isotope related chemistry See however Nagatsu et al 121 who encapsulate the bismuth target in a thin aluminium foil and place it in a niobium holder capable of holding molten bismuth See also Lavrukhina and Pozdnyakov 129 In other words where carbon s one s atomic orbital and three p orbitals hybridize to give four new orbitals shaped as intermediates between the original s and p orbitals Unfortunately the conundrum confronting the field is that commercial supply of 211At awaits the demonstration of clinical efficacy however the demonstration of clinical efficacy requires a reliable supply of 211At 119 References edit a b c Arblaster JW ed 2018 Selected Values of the Crystallographic Properties of Elements Materials Park Ohio ASM International p 604 ISBN 978 1 62708 154 2 Greenwood Norman N Earnshaw Alan 1997 Chemistry of the Elements 2nd ed Butterworth Heinemann p 28 ISBN 978 0 08 037941 8 a b Rothe S Andreyev A N Antalic S Borschevsky A Capponi L Cocolios T E De Witte H Eliav E et al 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of astatine Nature Communications 11 1 3824 arXiv 2002 11418 Bibcode 2020NatCo 11 3824L doi 10 1038 s41467 020 17599 2 PMC 7393155 PMID 32733029 Anders E 1959 Technetium and astatine chemistry Annual Review of Nuclear Science 9 203 220 Bibcode 1959ARNPS 9 203A doi 10 1146 annurev ns 09 120159 001223 subscription required Superheavy Element 117 Confirmed On the Way to the Island of Stability GSI Helmholtz Centre for Heavy Ion Research Archived from the original on 3 August 2018 Retrieved 26 July 2015 a b c d Nefedov V D Norseev Yu V Toropova M A Khalkin Vladimir A 1968 Astatine Russian Chemical Reviews 37 2 87 98 Bibcode 1968RuCRv 37 87N doi 10 1070 RC1968v037n02ABEH001603 S2CID 250775410 subscription required Aten A H W Jr Doorgeest T Hollstein U Moeken H P 1952 Section 5 Radiochemical Methods Analytical Chemistry of Astatine Analyst 77 920 774 777 Bibcode 1952Ana 77 774A doi 10 1039 AN9527700774 subscription required a b c d e f Zuckerman amp Hagen 1989 p 31 a b Zuckerman amp Hagen 1989 p 38 Chatterjee Sayandev Czerwinski Kenneth R Fitzgerald Hilary A Lakes Andrew L Liao Zuolei Ludwig Russell C McBride Katie M Vlasenko Vladislav P 2020 Novel Platforms for Drug Delivery Applications Woodhead Publishing Series in Biomaterials Woodhead Publishing Subchapter 16 4 2 Redox behavior doi 10 1016 B978 0 323 91376 8 00012 4 Kugler amp Keller 1985 pp 213 214 Kugler amp Keller 1985 pp 214 218 Kugler amp Keller 1985 p 211 Kugler amp Keller 1985 pp 109 110 129 213 Davidson M 2000 Contemporary boron chemistry Royal Society of Chemistry p 146 ISBN 978 0 85404 835 9 a b c d Zuckerman amp Hagen 1989 p 276 Elgqvist J Hultborn R Lindegren S Palm S 2011 Ovarian cancer background and clinical perspectives In Speer S ed Targeted Radionuclide Therapy Lippincott Williams amp Wilkins pp 380 396 383 ISBN 978 0 7817 9693 4 a b c Zuckerman amp Hagen 1989 pp 190 191 Brookhart M Grant B Volpe A F 1992 3 5 CF3 2C6H3 4B H OEt2 2 a convenient reagent for generation and stabilization of cationic highly electrophilic organometallic complexes Organometallics 11 11 3920 3922 doi 10 1021 om00059a071 Kugler amp Keller 1985 p 111 Sergentu Dumitru Claudiu Teze David Sabatie Gogova Andrea Alliot Cyrille Guo Ning Bassel Fadel Da Silva Isidro Deniaud David Maurice Remi Champion Julie Galland Nicolas Montavon Gilles 2016 Advances on the Determination of the Astatine Pourbaix Diagram Predomination of AtO OH 2 over At in Basic Conditions Chem Eur J 22 9 2964 71 doi 10 1002 chem 201504403 PMID 26773333 Kugler amp Keller 1985 p 222 Lavrukhina amp Pozdnyakov 1970 p 238 a b Kugler amp Keller 1985 pp 112 192 193 Kugler amp Keller 1985 p 219 Zuckerman amp Hagen 1989 pp 192 193 Zuckerman amp Hagen 1990 p 212 Brinkman G A Aten H W 1963 Decomposition of Caesium Diiodo Astatate I CsAtI2 Radiochimica Acta 2 1 48 doi 10 1524 ract 1963 2 1 48 S2CID 99398848 Zuckerman amp Hagen 1990 p 60 Zuckerman amp Hagen 1989 p 426 Appelman E H Sloth E N Studier M H 1966 Observation of Astatine Compounds by Time of 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Bibcode 1975JChEd 52 585T doi 10 1021 ed052p585 subscription required MacPherson H G 1934 An Investigation of the Magneto optic Method of Chemical Analysis Physical Review 47 4 310 315 Bibcode 1935PhRv 47 310M doi 10 1103 PhysRev 47 310 a b c Mellor J W 1965 A Comprehensive Treatise on Inorganic and Theoretical Chemistry Longmans Green p 1066 OCLC 13842122 a b Burdette S C Thornton B F 2010 Finding Eka Iodine Discovery Priority in Modern Times PDF Bulletin for the History of Chemistry 35 86 96 Archived PDF from the original on 9 October 2022 Scerri E 2013 A Tale of 7 Elements Google Play ed Oxford University Press pp 188 190 206 ISBN 978 0 19 539131 2 Karlik B Bernert T 1942 Uber Eine Vermutete b Strahlung des Radium A und die Naturliche Existenz des Elementes 85 About a Suspected b radiation of Radium A and the Natural Existence of the Element 85 Naturwissenschaften in German 30 44 45 685 686 Bibcode 1942NW 30 685K doi 10 1007 BF01487965 S2CID 6667655 subscription required Leigh Smith A Minder W 1942 Experimental Evidence of the Existence of Element 85 in the Thorium Family Nature 150 3817 767 768 Bibcode 1942Natur 150 767L doi 10 1038 150767a0 S2CID 4121704 subscription required Corson MacKenzie amp Segre 1940 a b Davis Helen Miles 1959 The Chemical Elements PDF 2nd ed Science Service Ballantine Books p 29 Archived from the original PDF on 23 August 2017 Retrieved 14 August 2016 Karlik B Bernert T 1943 Eine Neue Naturliche a Strahlung A New Natural a radiation Naturwissenschaften in German 31 25 26 298 299 Bibcode 1943NW 31 298K doi 10 1007 BF01475613 S2CID 38193384 subscription required Karlik B Bernert T 1943 Das Element 85 in den Naturlichen Zerfallsreihen The Element 85 in the Natural Decay Chains Zeitschrift fur Physik in German 123 1 2 51 72 Bibcode 1944ZPhy 123 51K doi 10 1007 BF01375144 S2CID 123906708 subscription required Lederer C M Hollander J M Perlman I 1967 Table of Isotopes 6th ed John Wiley amp Sons pp 1 657 a b Corson D R 2003 Astatine Chemical amp Engineering News 81 36 158 doi 10 1021 cen v081n036 p158 Corson MacKenzie amp Segre 1940 pp 672 677 Hamilton J G Soley M H 1940 A Comparison of the Metabolism of Iodine and of Element 85 Eka Iodine Proceedings of the National Academy of Sciences 26 8 483 489 Bibcode 1940PNAS 26 483H doi 10 1073 pnas 26 8 483 PMC 1078214 PMID 16588388 Neumann H M 1957 Solvent Distribution Studies of the Chemistry of Astatine Journal of Inorganic and Nuclear Chemistry 4 5 6 349 353 doi 10 1016 0022 1902 57 80018 9 Johnson G L Leininger R F Segre E 1949 Chemical Properties of Astatine I Journal of Chemical Physics 17 1 1 10 Bibcode 1949JChPh 17 1J doi 10 1063 1 1747034 hdl 2027 mdp 39015086446914 S2CID 95324453 Dreyer I Dreyer R Chalkin V A 1979 Cations of Astatine in Aqueous Solutions Production and some Characteristics Radiochemical and Radioanalytical Letters in German 36 6 389 398 a b Aten A H W Jr 1964 The Chemistry of Astatine Advances in Inorganic Chemistry and Radiochemistry Vol 6 pp 207 223 doi 10 1016 S0065 2792 08 60227 7 ISBN 978 0 12 023606 0 Nefedov V D Norseev Yu V Toropova M A Khalkin V A 1968 Astatine Russian Chemical Reviews 37 2 87 98 Bibcode 1968RuCRv 37 87N doi 10 1070 RC1968v037n02ABEH001603 S2CID 250775410 a b c Fry C Thoennessen M 2013 Discovery of the astatine radon francium and radium isotopes Atomic Data and Nuclear Data Tables 09 5 497 519 arXiv 1205 5841 Bibcode 2013ADNDT 99 497F doi 10 1016 j adt 2012 05 003 S2CID 12590893 Kokkonen Henna Decay properties of the new isotopes 188At and 190At PDF University of Jyvaskyla Retrieved 8 June 2023 a b c d Lavrukhina amp Pozdnyakov 1970 p 229 Rankama K 1956 Isotope Geology 2nd ed Pergamon Press p 403 ISBN 978 0 470 70800 2 Lide D R ed 2004 CRC Handbook of Chemistry and Physics 85th ed CRC Press pp 14 10 ISBN 978 0 8493 0485 9 a b Stwertka Albert A Guide to the Elements Oxford University Press 1996 p 193 ISBN 0 19 508083 1 Lavrukhina amp Pozdnyakov 1970 p 228 229 Asimov I 1957 Only a Trillion Abelard Schuman p 24 Kolthoff I M Elving P J eds 1964 Treatise on Analytical Chemistry Part II Analytical Chemistry of the Elements Vol 4 New York Interscience Encyclopedia p 487 Kugler amp Keller 1985 p 4 Maiti M Lahiri S 2011 Production cross section of At radionuclides from 7Li natPb and 9Be natTl reactions Physical Review C 84 6 07601 07604 07601 arXiv 1109 6413 Bibcode 2011PhRvC 84f7601M doi 10 1103 PhysRevC 84 067601 S2CID 115321713 Greenwood amp Earnshaw 2002 p 796 Kugler amp Keller 1985 p 5 Barton G W Ghiorso A Perlman I 1951 Radioactivity of Astatine Isotopes Physical Review 82 1 13 19 Bibcode 1951PhRv 82 13B doi 10 1103 PhysRev 82 13 hdl 2027 mdp 39015086480574 subscription required a b c d e f Zalutsky M R Pruszynski M 2011 Astatine 211 Production and Availability Current Radiopharmaceuticals 4 3 177 185 doi 10 2174 1874471011104030177 PMC 3503149 PMID 22201707 a b Larsen R H Wieland B W Zalutsky M R J 1996 Evaluation of an Internal Cyclotron Target for the Production of 211At via the 209Bi a 2n 211At reaction Applied Radiation and Isotopes 47 2 135 143 doi 10 1016 0969 8043 95 00285 5 PMID 8852627 Nagatsu K Minegishi K H Fukada M Suzuki H Hasegawa S Zhang M 2014 Production of 211At by a vertical beam irradiation method Applied Radiation and Isotopes 94 363 371 doi 10 1016 j apradiso 2014 09 012 PMID 25439168 Barbet J Bourgeois M Chatal J 2014 Cyclotron Based Radiopharmaceuticals for Nuclear Medicine Therapy In R P Baum eds Therapeutic Nuclear Medicine Springer pp 95 104 99 ISBN 978 3 540 36718 5 a b Wilbur D S 2001 Overcoming the Obstacles to Clinical Evaluation of 211At Labeled Radiopharmaceuticals The Journal of Nuclear Medicine 42 10 1516 1518 PMID 11585866 a b c d Lavrukhina amp Pozdnyakov 1970 p 233 Gopalan R 2009 Inorganic Chemistry for Undergraduates Universities Press p 547 ISBN 978 81 7371 660 7 Stigbrand T Carlsson J Adams G P 2008 Targeted Radionuclide Tumor Therapy Biological Aspects Springer p 150 ISBN 978 1 4020 8695 3 Gyehong G Chun K Park S H Kim B 2014 Production of a particle emitting 211At using 45 MeV a beam Physics in Medicine and Biology 59 11 2849 2860 Bibcode 2014PMB 59 2849K doi 10 1088 0031 9155 59 11 2849 PMID 24819557 S2CID 21973246 Kugler amp Keller 1985 pp 95 106 133 139 Lavrukhina amp Pozdnyakov 1970 pp 243 253 Kugler amp Keller 1985 p 97 Lindegren S Back T Jensen H J 2001 Dry distillation of Astatine 211 from Irradiated Bismuth Targets A Time saving Procedure with High Recovery Yields Applied Radiation and Isotopes 55 2 157 160 doi 10 1016 S0969 8043 01 00044 6 PMID 11393754 Yordanov A T Pozzi O Carlin S Akabani G J Wieland B Zalutsky M R 2005 Wet Harvesting of No carrier added 211At from an Irradiated 209Bi Target for Radiopharmaceutical Applications Journal of Radioanalytical and Nuclear Chemistry 262 3 593 599 doi 10 1007 s10967 005 0481 7 S2CID 93179195 a b Balkin Ethan Hamlin Donald Gagnon Katherine Chyan Ming Kuan Pal Sujit Watanabe Shigeki Wilbur D 18 September 2013 Evaluation of a Wet Chemistry Method for Isolation of Cyclotron Produced 211At Astatine Applied Sciences 3 3 636 655 CiteSeerX 10 1 1 383 1903 doi 10 3390 app3030636 ISSN 2076 3417 a b c Vertes Nagy amp Klencsar 2003 p 337 Zalutsky Michael Vaidyanathan Ganesan 1 September 2000 Astatine 211 Labeled Radiotherapeutics An Emerging Approach to Targeted Alpha Particle Radiotherapy Current Pharmaceutical Design 6 14 1433 1455 doi 10 2174 1381612003399275 PMID 10903402 Wilbur D Scott 20 February 2013 Enigmatic astatine Nature Chemistry 5 3 246 Bibcode 2013NatCh 5 246W doi 10 1038 nchem 1580 PMID 23422568 Vertes Nagy amp Klencsar 2003 p 338 a b Fisher D 1995 Oral History of Dr Patricia Wallace Durbin PhD Human Radiation Studies Remembering the Early Years United States Department of Energy Office of Human Radiation Experiments Retrieved 25 March 2015 Vaidyanathan G Zalutsky M R 2008 Astatine Radiopharmaceuticals Prospects and Problems Current Radiopharmaceuticals 1 3 177 196 doi 10 2174 1874471010801030177 PMC 2818997 PMID 20150978 Lavrukhina amp Pozdnyakov 1970 pp 232 233 Odell T T Jr Upton A C 2013 Softcover reprint of the hardcover 1st edition 1961 Late Effects of Internally Deposited Radioisotopes In Schwiegk H Turba F eds Radioactive Isotopes in Physiology Diagnostics and Therapy Radioaktive Isotope in Physiologie Diagnostik Und Therapie Springer Verlag pp 375 392 385 ISBN 978 3 642 49477 2 Keller Cornelius Wolf Walter Shani Jashovam Radionuclides 2 Radioactive Elements and Artificial Radionuclides Ullmann s Encyclopedia of Industrial Chemistry Weinheim Wiley VCH doi 10 1002 14356007 o22 o15 ISBN 978 3527306732 Bibliography editCorson D R MacKenzie K R Segre E 1940 Artificially Radioactive Element 85 Physical Review 58 8 672 678 Bibcode 1940PhRv 58 672C doi 10 1103 PhysRev 58 672 subscription required Greenwood N N Earnshaw A 2002 Chemistry of the Elements 2nd ed Butterworth Heinemann ISBN 978 0 7506 3365 9 Kugler H K Keller C 1985 At Astatine System No 8a Gmelin Handbook of Inorganic and Organometallic Chemistry Vol 8 8th ed Springer Verlag ISBN 978 3 540 93516 2 Lavrukhina Avgusta Konstantinovna Pozdnyakov Aleksandr Aleksandrovich 1970 Analytical Chemistry of Technetium Promethium Astatine and Francium Translated by R Kondor Ann Arbor Humphrey Science Publishers ISBN 978 0 250 39923 9 Scerri Eric 2013 A Tale of Seven Elements Oxford University Press ISBN 9780195391312 Vertes A Nagy S Klencsar Z 2003 Handbook of Nuclear Chemistry Vol 4 Springer ISBN 978 1 4020 1316 4 Zuckerman J J Hagen A P 1989 Inorganic Reactions and Methods Volume 3 The Formation of Bonds to Halogens Part 1 John Wiley amp Sons ISBN 978 0 471 18656 4 Zuckerman J J Hagen A P 1990 Inorganic Reactions and Methods Volume 4 The Formation of Bonds to Halogens Part 2 John Wiley amp Sons ISBN 978 0 471 18657 1 External links editAstatine at Wikipedia s sister projects nbsp Definitions from Wiktionary nbsp Media from Commons nbsp Resources from Wikiversity Astatine at The Periodic Table of Videos University of Nottingham Astatine Halogen or Metal Retrieved from https en wikipedia org w index php title Astatine amp oldid 1203383901, wikipedia, wiki, book, books, library,

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