From English Wikipedia @ Freddythechick
Chemical element with atomic number 112 (Cn)
Copernicium, 112 Cn Pronunciation (KOH -pər-NISS -ee-əm ) Mass number [285]
Atomic number (Z ) 112 Group group 12 Period period 7 Block d-block Electron configuration [Rn ] 5f14 6d10 7s2 (predicted) [1] Electrons per shell 2, 8, 18, 32, 32, 18, 2 (predicted) Phase at STP liquid (predicted) [2] [3] Melting point 283 ± 11 K (10 ± 11 °C, 50 ± 20 °F) (predicted) [3] Boiling point 340 ± 10 K (67 ± 10 °C, 153 ± 18 °F)[3] (predicted )Density (near r.t. ) 14.0 g/cm3 (predicted) [3] Triple point 283 K, 25 kPa (predicted) [3] Oxidation states 0 , (+1), +2 , (+4), (+6) (parenthesized: prediction )[1] [4] [5] [6] Ionization energies 1st: 1155 kJ/mol 2nd: 2170 kJ/mol 3rd: 3160 kJ/mol (more ) (all estimated) [1] Atomic radius calculated: 147 pm [1] [5] (predicted) Covalent radius 122 pm (predicted) [7] Natural occurrence synthetic Crystal structure hexagonal close-packed (hcp)(predicted) [3] CAS Number 54084-26-3 Naming after Nicolaus Copernicus Discovery Gesellschaft für Schwerionenforschung (1996)
Category: Copernicium | references
child table, as reused in {IB-Cn}
References
These references will appear in the article, but this list appears only on this page.
^ 1.0 1.1 1.2 1.3 Hoffman, Darleane C.; Lee, Diana M.; Pershina, Valeria (2006). "Transactinides and the future elements". In Morss; Edelstein, Norman M.; Fuger, Jean (eds.). The Chemistry of the Actinide and Transactinide Elements (3rd ed.). Dordrecht, The Netherlands: Springer Science+Business Media . ISBN 978-1-4020-3555-5 .
^ Soverna S 2004, 'Indication for a gaseous element 112,' in U Grundinger (ed.), GSI Scientific Report 2003, GSI Report 2004-1, p. 187, ISSN 0174-0814
^ 3.0 3.1 3.2 3.3 3.4 3.5 Mewes, J.-M.; Smits, O. R.; Kresse, G.; Schwerdtfeger, P. (2019). "Copernicium is a Relativistic Noble Liquid" . Angewandte Chemie International Edition . doi :10.1002/anie.201906966 .
^ Gäggeler, Heinz W.; Türler, Andreas (2013). "Gas Phase Chemistry of Superheavy Elements" . The Chemistry of Superheavy Elements . Springer Science+Business Media . pp. 415–483. doi :10.1007/978-3-642-37466-1_8 . ISBN 978-3-642-37465-4 . Retrieved 2018-04-21 .
^ 5.0 5.1 Fricke, Burkhard (1975). "Superheavy elements: a prediction of their chemical and physical properties" . Recent Impact of Physics on Inorganic Chemistry . Structure and Bonding. 21 : 89–144. doi :10.1007/BFb0116498 . ISBN 978-3-540-07109-9 . Retrieved 4 October 2013 .
^ Hu, Shu-Xian; Zou, Wenli (23 September 2021). "Stable copernicium hexafluoride (CnF6 ) with an oxidation state of VI+". Physical Chemistry Chemical Physics . 2022 (24): 321–325. doi :10.1039/D1CP04360A . PMID 34889909 .
^ Chemical Data. Copernicium - Cn , Royal Chemical Society
^ 8.0 8.1 Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021). "The NUBASE2020 evaluation of nuclear properties" (PDF) . Chinese Physics C . 45 (3): 030001. doi :10.1088/1674-1137/abddae .
^ 9.0 9.1 Oganessian, Yu. Ts.; Utyonkov, V. K.; Ibadullayev, D.; et al. (2022). "Investigation of 48 Ca-induced reactions with 242 Pu and 238 U targets at the JINR Superheavy Element Factory". Physical Review C . 106 (24612). Bibcode :2022PhRvC.106b4612O . doi :10.1103/PhysRevC.106.024612 . S2CID 251759318 .
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