| Abstract: | Abstract Tellurium is a sort of scattered rare element on the earth. Its concentration is very low in earth's crust, only 1.0 ng/g. However, it has extremely high abundance in Co‐rich crusts, marine polymetallic nodules, deep‐sea sediments and aerolites. To find out the origin of tellurium enrichment in deep‐sea sediments, we analyzed and compared tellurium concentrations and helium isotope compositions in the magnetic parts and those in the bulk parts of deep‐sea sediments. The result indicates that the helium content, 3He/4He ratio and tellurium concentration are obviously higher in the magnetic parts than those in the bulk parts. The 3He abundance varies synchronously with the tellurium concentration. 3He and Te have a distinct positive correlation with each other. It is the first time that the paper brings forward that the extreme enrichment of tellurium in deep‐sea sediments, like helium isotope anomalies, probably results from the input of interplanetary dust particles (IDPs). Similarly, the extreme enrichment of tellurium in marine polymetallic nodules and Co‐rich crusts is possibly related to IDPs. |
