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The mass accretion rate (solar mass per year).
The present rate of star formation is about one solar mass per year in the entire Galaxy, which contains something like 2 × 109 solar masses of gas.
The corresponding mass-loss rates approach and sometimes exceed one hundred-thousandth of a solar mass per year, which means that one entire solar mass (perhaps a tenth of the total mass of the star) is carried away into space in a relatively short span of 100,000 years.
Low bone turnover particularly in the long bones of the leg (≤1 % of bone mass per year) favours the accumulation of microdamage eventually leading to overt bone failure / fracture [10].
Courtship display, ejaculate size, number of eggs laid and body mass per year were analysed to assess change in breeding values over time.
For example, a difference of 5 kg in lean body mass translates to a difference in energy expenditure of 100 kcal/day (equivalent to 4.7 kg fat mass per year).
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Fuel = Mass or volume of the fuel combusted, either from company records or directly measured by a fuel flow meter, as applicable (mass or volume per year).
It probably also triggers the episodic mass loss at rates of 10−7 to 10−5 solar masses per year.
Over the past 3 years the mass accretion rate has steadily decreased from about 5x10-6 to 3x10-8 solar masses per year.
With an average past star-formation rate of 600 to 3,000 solar masses per year, this galaxy was among the most vigorous star-forming galaxies in the Universe.
As the gas cools, the central galaxy draws the material inward at inferred rates that often exceed 100 solar masses per year.
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