Nipponium as a new element (Z=75) separated by the Japanese chemist, Masataka Ogawa: a scientific and science historical re-evaluation

Ниппоний как новый элемент (Z = 75), выделенный японским химиком Масатакой Огавой: научная и историко-научная переоценка
H. Kenji Yoshihara
2008-01-01

Element 75NipponiumOptical spectraRheniumX-ray spectra
This review article deals with a new element 'nipponium' reported by Masataka Ogawa in 1908, and with its scientific and science historical background. Ogawa positioned nipponium between molybdenum and ruthenium in the periodic table. From a modern chemical viewpoint, however, nipponium is ascribable to the element with Z=75, namely rhenium, which was unknown in 1908. The reasons for this corrected assignment of nipponium are (1) its optical spectra, (2) its atomic weight when corrected, (3) its relative abundance in molybdenite, the same being true with rhenium. Recently some important evidence was found among the Ogawa's personal collection preserved by his family. Deciphering the X-ray spectra revealed that the measured spectra of the nipponium sample that Ogawa brought from University College, London clearly showed the presence of the element 75 (rhenium). Thus was resolved the mysterious story of nipponium, which had continued for almost a century. It is concluded that nipponium was identical to rhenium.
1
Masataka Ogawa reported nipponium in 1908 and positioned it between molybdenum and ruthenium in the periodic table.
2
Modern chemical analysis reassigns nipponium to element Z=75, rhenium, based on optical spectra, corrected atomic weight, and molybdenite abundance.
3
Recently examined X-ray spectra from Ogawa’s preserved nipponium sample clearly demonstrated the presence of element 75 (rhenium).
4
The historical mystery of nipponium was resolved: Ogawa’s nipponium was identical to rhenium, which was unknown in 1908.

Masataka Ogawa’s reported element “nipponium” (Z=75), identified as rhenium

The scientific identity and historical reassignment of nipponium to rhenium based on optical and X-ray spectra, corrected atomic weight, and abundance in molybdenite

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2008-01-01
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H. Kenji Yoshihara
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