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Decrease in male mouse fertility by hydrogen sulfide and/or ammonia can Be inheritable.

Authors :
Zhang, Weidong
Zhao, Yong
Zhang, Pengfei
Hao, Yanan
Yu, Shuai
Min, Lingjiang
Li, Lan
Ma, Dongxue
Chen, Liang
Yi, Bao
Tang, Xiangfang
Meng, Qingshi
Liu, Lei
Wang, Shukun
Shen, Wei
Zhang, Hongfu
Source :
Chemosphere. Mar2018, Vol. 194, p147-157. 11p.
Publication Year :
2018

Abstract

Numerous epidemiological studies suggest that air pollutants cause a decline in the quality of human spermatozoa and thus a reduction in fertility. However, the exact cause of infertility remains unknown. Air pollution gases, such as NH 3 and H 2 S are either free or bound to airborne particular materials (PM) and are abundant and reactive. The aim of this current investigation was to explore the impacts of NH 3 and/or H 2 S on male fertility and the underlying mechanisms. Male mouse exposed to H 2 S and/or NH 3 and after two generations were used to evaluate the impacts on fertility. The fertility, and spermatozoa quality parameters and proteins involved in spermatogenesis were investigated. Our current investigation demonstrates: i) H 2 S and/or NH 3 decrease male fertility by 20–30%, reduce the spermatozoa concentration about 20–40%, decrease 10–20%, increase around 30%; ii) the reduction in male fertility by H 2 S and/or NH 3 can be inheritable; iii) H 2 S and/or NH 3 can diminish male fertility through the disruption of spermatogenesis without affecting other body parameters such as body weight and organ index. One component of air pollutants, for example NH 3 , does not have a severe impact; however, two or more pollutants such as H 2 S and NH 3 combined can cause serious health problems, especially with regard to male fertility. We suggest that greater attention should be paid to these air pollutants to improve human health and fertility. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00456535
Volume :
194
Database :
Academic Search Index
Journal :
Chemosphere
Publication Type :
Academic Journal
Accession number :
126946911
Full Text :
https://doi.org/10.1016/j.chemosphere.2017.11.164