Integrated system approach to dark fermentative biohydrogen production for enhanced yield, energy efficiency and substrate recovery

2018 ◽  
Vol 17 (3) ◽  
pp. 501-529 ◽  
Author(s):  
Patrick T. Sekoai ◽  
Kelvin O. Yoro ◽  
Michael O. Bodunrin ◽  
Augustine O. Ayeni ◽  
Michael O. Daramola
2003 ◽  
Vol 2 (1) ◽  
pp. 35-39 ◽  
Author(s):  
S. Franck ◽  
M. Cuntz ◽  
W. von Bloh ◽  
C. Bounama

In a previous paper, we showed that Earth-type habitable planets around 47 UMa are in principle possible if a distinct set of conditions is warranted. These conditions include that the Earth-type planets have successfully formed and are orbitally stable and, in addition, that the 47 UMa star–planet system is relatively young ([lsim ]6 Gyr). We now extend this study by considering Earth-like planets with different land/ocean coverages. This study is again based on the so-called integrated system approach, which describes the photosynthetic biomass production taking into account a variety of climatological, biogeochemical and geodynamical processes. This approach implies a special characterization of the habitable zone defined for a distinct type of planet. We show that the likelihood of finding a habitable Earth-like planet on a stable orbit around 47 UMa critically depends on the percentage of the planetary land/ocean coverage. The likelihood is significantly increased for planets with a very high percentage of ocean surface (‘water worlds’).


2015 ◽  
Vol 162 ◽  
pp. 583-592 ◽  
Author(s):  
Fredrik Gunnarsson ◽  
Moa Z. Granlund ◽  
Mattias Englund ◽  
Jazaer Dawody ◽  
Lars J. Pettersson ◽  
...  

1973 ◽  
Vol R-22 (1) ◽  
pp. 2-12 ◽  
Author(s):  
Stephen A. Szygenda ◽  
Michael J. Flynn

2020 ◽  
Author(s):  
Paolo Re ◽  
Francesco Lamboglia ◽  
Giorgio Missiaggia

2018 ◽  
Vol 159 ◽  
pp. 332-345 ◽  
Author(s):  
Cynthia Regnier ◽  
Kaiyu Sun ◽  
Tianzhen Hong ◽  
Mary Ann Piette

Sign in / Sign up

Export Citation Format

Share Document