Einsteinium (Es)
actinideSolid
표준 원자량
[252]전자 배치
[Rn] 7s2 5f11녹는점
859.85 °C끓는점
해당 없음밀도
8840 kg/m³산화 상태
+2, +3, +4전기 음성도(Pauling)
1.3제1 이온화 에너지
6.3684 eV발견 연도
1952원자 반지름
해당 없음상세 정보
Einsteinium is a synthetic actinide with atomic number 99. It was first identified in debris from a thermonuclear test, and it is now made only in minute amounts by intense neutron irradiation of lighter actinides. Its chemistry is dominated by the +3 oxidation state and resembles that of neighboring trivalent actinides and lanthanides. The element is important mainly as a research material and as a target for producing still heavier elements.
Einsteinium does not occur naturally in the Earth’s crust. It was first identified in December 1952 by American scientists from the Argonne National Laboratory near Chicago, Illinois, the Los Alamos National Laboratory in Los Alamos, New Mexico, and The University of California Laboratory in Berkeley, California in the debris of thermonuclear weapons. The element was named for Albert Einstein (Fig. IUPAC.99.1). 253Es was the first isotope identified; it has a half-life of 20.47 days. The isotope with the longest half-life is 252Es, with a half-life of 472 days [630], [631].
There are no uses for isotopes of einsteinium outside of basic scientific research for the production of higher transuranic elements and studies of actinide science. Due to the radiation and heat given off by einsteinium isotopes, it is difficult to use them in experiments and studies [631].
Tracer studies using 253Es show that einsteinium has chemical properties typical of a heavy trivalent, actinide element. Oxidation states of II and III for einsteinium have been reported and oxidation state IV has been postulated from vapor transport studies but not established unequivocally. Einsteinium is the first divalent metal in the actinide series (two bonding electrons rather than three). The self-irradiation properties of einsteinium make it extremely difficult, for example, to obtain x-ray crystallographic data. The intense gamma and x-rays from einsteinium decay to daughter products over-exposes the x-ray film/detector. This intense self-irradiation can be exploited however to study accelerated aging and radiation damage studies, and for targeted radiation medical treatments. An example of einsteinium chemical studies is the chemical consequences of radioactive decay. With the relatively short half-life of Es-253 (20.47 days) one can study the in-growth of daughter Bk-249 (half-life 330 days) and grand-daughter Cf-249 (half-life 351 years). Evidence suggests that divalent Es might decay into a divalent Bk daughter and subsequently into as of yet unknown divalent Cf. There are no commercial uses for einsteinium however it is the heaviest element for which bulk studies can be performed that allows for fundamental studies of the role of 5-f electrons in actinide systematics.
Further reading:
Richard G. Haire (2006) Chapter 12, The Chemistry of the Actinide and Transactinide Elements, Third Edition, L. R. Morss, J. Fuger, and N. M. Edelstein, Eds, Springer Publishers.
This element reviewed and Updated by Dr. David Hobart, 2011
Einsteinium was discovered by a team of scientists led by Albert Ghiorso in 1952 while studying the radioactive debris produced by the detonation of the first hydrogen bomb. The isotope they discovered, einsteinium-253, has a half-life of about 20 days and was produced by combining 15 neutrons with uranium-238, which then underwent seven beta decays. Today, einsteinium is produced though a lengthy chain of nuclear reactions that involves bombarding each isotope in the chain with neutrons and then allowing the resulting isotope to undergo beta decay. Einsteinium's most stable isotope, einsteinium-252, has a half-life of about 471.7 days. It decays into berkelium-248 through alpha decay or into californium-252 through electron capture.
Einsteinium, the seventh transuranic element of the actinide series to be discovered, was identified by Ghiorso and co-workers at Berkeley in December 1952 in debris from the first large thermonuclear explosion, which took place in the Pacific in November, 1952. The 20-day 253Es isotope was produced. It was named after Albert Einstein.
In 1961, enough einsteinium was produced to separate a macroscopic amount of 253Es. This sample weighted about 0.01µg and was measured using a special magnetic-type balance. 253Es so produced was used to produce mendelevium (Element 101) by neutron bombardment.
About 3 µg of einsteinium has been produced in the High Flux Isotope Reactor (HFIR) at Oak Ridge National Laboratories by:
▸ irradiating kilogram quantities of 239Pu in a reactor for several years to produce 242Pu,
▸ fabricating the 242Pu into pellets of plutonium oxide and aluminum powder,
▸ loading the pellets into target rods for an initial 1-year irradiation at the Savannah River Plant, and,
▸ irradiating the targets for another 4 months in the HFIR.
The targets were then removed for chemical separation of the einsteinium from californium daughter products. About 2 milligrams of einsteinium can be present in special HFIR campaigns.
Only microgram-scale samples have been isolated, so ordinary bulk appearance is not well established. Metallic einsteinium has not been characterized like common metals; many physical properties are measured with difficulty or inferred from very small samples.
Einsteinium has no commercial use. Its main use is in nuclear and chemical research, especially in studies of heavy-actinide chemistry and radiation effects in solids. ²⁵³Es has been used as a target material for producing mendelevium and other heavier nuclei in accelerator experiments. Because it is scarce, intensely radioactive, and self-heating, its use is limited to specialized laboratories with radiochemical facilities.
Since only small amounts of einsteinium have ever been produced, it currently has no uses outside of basic scientific research.
Einsteinium chemistry is known from tracer and microgram-scale work. The most stable common oxidation state in solution is Es³⁺, which forms salts and coordination complexes broadly similar to those of other trivalent actinides. Reported compounds include einsteinium(III) chloride, EsCl₃, einsteinium(III) bromide, EsBr₃, and einsteinium(III) oxide, Es₂O₃. A divalent state has been observed under reducing conditions in some systems, but +3 remains the principal aqueous and solid-state chemistry.
See more information at the Einsteinium compound page.
All einsteinium isotopes are radioactive, and hazards depend strongly on the isotope and amount. Important risks include external gamma or X-ray exposure from associated decay products, internal alpha exposure if material is inhaled or ingested, and heat generation in concentrated samples. Handling requires shielded, contamination-controlled radiochemical equipment. No biological role is known.
Einsteinium has no meaningful natural environmental cycle. Any natural occurrence would be transient and extraordinarily rare, produced by neutron capture in exceptional nuclear events and quickly lost by radioactive decay. Environmental releases are associated only with nuclear activities or laboratory material, where behavior is governed by actinide chemistry, sorption to minerals, complexation, and isotope-specific decay.
Einsteinium is not a commodity and has no normal market. It is produced in specialized high-flux reactors by prolonged neutron irradiation of plutonium, curium, or other actinide targets, followed by difficult radiochemical separation from neighboring transplutonium elements. Production yields are tiny, and the material decays during and after processing. Supply is therefore episodic, institutionally controlled, and directed almost entirely to research experiments rather than industrial demand.
Made by bombarding uranium with neutrons.
Einsteinium is not a primordial element and has no stable isotopes. In the universe it can be formed only in environments with intense neutron capture, such as nuclear explosions or possibly extreme astrophysical r-process events, but any atoms produced decay on short geological timescales. It is not expected to persist in planets, meteorites, or stellar material except as a transient radionuclide.
- The first einsteinium atoms were found in fallout from the 1952 Ivy Mike thermonuclear test.
- ²⁵³Es is often the most useful isotope for chemistry because it can be made in measurable microgram quantities.
- Self-irradiation damages einsteinium compounds and can alter measurements during an experiment.
- Einsteinium helped enable the first synthesis of mendelevium.
- Separation from californium and other neighboring actinides is one of the main practical difficulties.
이미지
특성
물리적 특성
- 반데르발스 반지름
- 245 pm 모든 원소의 반데르발스 반지름 비교 →
- 밀도
- 8840 kg/m³ 모든 원소의 밀도 비교 →
- STP에서의 상
- 고체 모든 원소의 STP에서의 상 비교 →
- 녹는점
- 859.85 °C 모든 원소의 녹는점 비교 →
화학적 특성
- 전기 음성도(Pauling)
- 1.3 모든 원소의 전기 음성도(Pauling) 비교 →
- 전자 친화도
- -0.3 eV (음수 값 — 추가 전자를 결합하지 않을 것으로 예측됨)
- 제1 이온화 에너지
- 6.3684 eV 모든 원소의 제1 이온화 에너지 비교 →
- 제2 이온화 에너지
- 12.200042 eV 모든 원소의 제2 이온화 에너지 비교 →
- 제3 이온화 에너지
- 22.700078 eV 모든 원소의 제3 이온화 에너지 비교 →
- 제4 이온화 에너지
- 38.800134 eV 모든 원소의 제4 이온화 에너지 비교 →
- 제5 이온화 에너지
- 54.100186 eV 모든 원소의 제5 이온화 에너지 비교 →
- 산화 상태
- +2, +3, +4 모든 원소의 산화 상태 비교 →
- 원자가 전자
- 3 모든 원소의 원자가 전자 비교 →
- 전자 배치
- [Rn] 7s2 5f11
열역학적 특성
- 승화열
- 3.990258 eV
- 원자화열
- 3.990258 eV
- 원자화 엔탈피
- 1.378453 eV
핵 특성
- 양성자 수
- 99 모든 원소의 양성자 수 비교 →
- 중성자 수
- 153 모든 원소의 중성자 수 비교 →
- 알려진 동위원소 수
- 20 모든 원소의 알려진 동위원소 수 비교 →
- 안정 동위원소 수
- 0 모든 원소의 안정 동위원소 수 비교 →
- 질량수(가장 안정한 동위원소)
- 252
- 가장 안정한 동위원소
- Es-252
- 발견 연도
- 1952
존재비
해당 없음
결정 구조
해당 없음
전자 구조
- 전자껍질별 전자 수
- 2, 8, 18, 32, 29, 8, 2 모든 원소의 전자껍질별 전자 수 비교 →
식별자
- CAS 등록 번호
- 7429-92-7 모든 원소의 CAS 등록 번호 비교 →
- 항 기호
- 4I°15/2
- InChI
- InChI=1S/Es
- InChI 키
- CKBRQZNRCSJHFT-UHFFFAOYSA-N
전자 배치 측정값
Es: 5f¹¹ 7s²[Rn] 5f¹¹ 7s²1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 5s² 5p⁶ 4f¹⁴ 5d¹⁰ 6s² 6p⁶ 5f¹¹ 7s²원자 모형
동위원소에 따라 중성자 수, 질량, 안정성은 달라지지만, 중성 원자의 전자 배치는 달라지지 않습니다.
개략적인 원자 모형이며 실제 비율과 다릅니다.
원자 지문
방출 / 흡수 스펙트럼
동위원소 분포
안정 동위원소가 없습니다.
| 질량수 | 원자 질량(u) | 천연 존재비 | 반감기 |
|---|---|---|---|
| 252 방사성 | 252.08298 ± 0.000054 | 해당 없음 | 471.7 일 |
| 254 방사성 | 254.0880222 ± 0.0000045 | 해당 없음 | 275.7 일 |
| 249 방사성 | 249.076411 ± 0.000032 | 해당 없음 | 102.2 분 |
| 255 방사성 | 255.090275 ± 0.000012 | 해당 없음 | 39.8 일 |
| 244 방사성 | 244.07088 ± 0.0002 | 해당 없음 | 37 초 |
상 / 상태
이유: 승화점(859.85 °C)보다 834.9 °C 낮음
개략도이며 실제 비율과 다름
상전이점
전이 에너지
승화점에서 1 mol을 승화시키는 데 필요한 에너지
밀도
표준 조건에서
표준 조건에서
원자 스펙트럼
전체 99개 중 10개를 표시합니다. 이온 전하순으로 정렬되었습니다(오름차순).
보유 에너지 준위 데이터 ?
| 이온 | 전하 | 준위 |
|---|---|---|
| Es I | 0 | 2 |
| Es II | +1 | 2 |
| Es III | +2 | 2 |
| Es IV | +3 | 2 |
| Es V | +4 | 2 |
| Es VI | +5 | 2 |
| Es VII | +6 | 2 |
| Es VIII | +7 | 2 |
| Es IX | +8 | 2 |
| Es X | +9 | 2 |
결정 구조 데이터 없음
이온 반지름
| 전하 | 배위 | 스핀 | 반지름 |
|---|---|---|---|
| +3 | 9 | 해당 없음 | 111.6 pm |
화합물
동위원소 (5)
Sixteen isotopes with three isomers ranging in atomic mass from 241 to 256 are now recognized for einsteinium. 252Es has the longest half-life (472 days) but is only available in minute quantities. The isotopes 253Es and 254Es are the isotopes of choice for physicochemical studies because of their availability and reasonable half-lives. However, usually only a few micrograms of einsteinium isotopes are used in experiments to reduce worker exposure and to minimize the intense self-irradiation effects.
| 질량수 | 원자 질량(u) | 천연 존재비 | 반감기 | 붕괴 방식 | |
|---|---|---|---|---|---|
| 252 방사성 | 252.08298 ± 0.000054 | 해당 없음 | 471.7 일 | α =78±0.2%ε =22±0.2% | |
| 254 방사성 | 254.0880222 ± 0.0000045 | 해당 없음 | 275.7 일 | α ≈100%ε ?β- =1.74e-4±0.8% | |
| 249 방사성 | 249.076411 ± 0.000032 | 해당 없음 | 102.2 분 | β+ ≈100%α =0.57±0.8% | |
| 255 방사성 | 255.090275 ± 0.000012 | 해당 없음 | 39.8 일 | β- =92.0±0.4%α =8.0±0.4%SF =0.0041±0.2% | |
| 244 방사성 | 244.07088 ± 0.0002 | 해당 없음 | 37 초 | β+ =95±0.3%α =5±0.3%β+SF =0.011±0.4% |
확장 특성
공유 결합 반지름(확장)
- 공유 결합 반지름(Pyykkö)
- 165 pm
- 공유 결합 반지름(Pyykkö, 이중 결합)
- 140 pm
반데르발스 반지름
- Alvarez
- 270 pm
- UFF
- 329.9 pm
번호 척도
- Mendeleev
- 34
- Pettifor
- 38
- Glawe
- 43
전기 음성도 척도
- Ghosh
- 0
분극률 및 분산
- 쌍극자 분극률
- 118 a.u.
- 쌍극자 분극률(불확도)
- 20 a.u.
상전이 및 동소체
| 녹는점 | 1133.15 K |
산화 상태 분류
심화 참고 데이터
결정 반지름 상세 정보 (1)
| 전하 | CN | 스핀 | rcrystal (pm) | 기원 |
|---|---|---|---|---|
| 3 | IX | — | 125.6 |
동위원소 붕괴 방식 (51)
| 동위원소 | 모드 | 세기 |
|---|---|---|
| 239 | A | — |
| 239 | B+ | — |
| 239 | SF | — |
| 240 | A | 70% |
| 240 | B+ | 30% |
| 240 | B+SF | 0.2% |
| 241 | A | 100% |
| 241 | B+ | — |
| 242 | A | 57% |
| 242 | B+ | 43% |
추가 데이터
Estimated Crustal Abundance
The estimated element abundance in the earth's crust.
Not Applicable
참고 문헌 (1)
- [5] Einsteinium https://education.jlab.org/itselemental/ele099.html
Estimated Oceanic Abundance
The estimated element abundance in the earth's oceans.
Not Applicable
참고 문헌 (1)
- [5] Einsteinium https://education.jlab.org/itselemental/ele099.html
참고 문헌
(9)
Data deposited in or computed by PubChem
The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.
Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.
The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.
Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/
The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.
The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database
This section provides all form of data related to element Einsteinium.
The element property data was retrieved from publications.
