The maximum stellar mass that can exist as a white dwarf is about 1.4 solar masses and is known as the Chandrasekhar limit.
Preliminary experiments to derive aerosol deposition rate on a flat plate and the maximum feasible liquid mass that may be accumulated on a near-spherical envelope are briefly described.
In order to determine the maximum amount of cell mass that could be efficiently digested by a 13% sodium hypochlorite solution, small-scale extraction experiments were carried out at first.
This paper describes the methodology for setting the minimum number of mass exchange units target and a procedure for designing a maximum mass recovery network that features the minimum utility targets.
If say the feeding rate is 4%, the value does not fluctuate with the amount of crude protein contained in the feed, but is fixed as the preferably maximum mass of feed that can be consumed by an individual fish per day.
Calculate the maximum mass of magnesium oxide that can be formed from 4.8 g of magnesium.
Electrodeposition mechanism of manganese oxide is discussed with the help of electrochemical quartz crystal microbalance (EQCM) study and it reveals that maximum mass deposited on the electrode surface occurs at 0.85 V vs SCE.
If, instead, it became a hypermassive neutron star, it should have been rotating extremely rapidly, as a large amount of angular momentum could raise that maximum mass limit by 10-15%.
This has been inferred to be an object with a maximum mass of 6 times that of Jupiter and an orbital radius of 3.3 AU.
