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A new estimate for an older accretion time of the limestone based on new data from associated clastic rocks would require even higher apparent plate motions (Wakabayashi 2015).
We have simulated different formation scenarios of Varuna by varying the accretion time, accretion rate, and a fraction of impact kinetic energy converted into heat.
Up to a mass of about 10 M⊙, the accretion time (t_{mathrm{acc}}=M_/dot{M}_), where (M_) is the mass of the protostar, is smaller than the Kelvin-Helmholtz time (t_{mathrm{KH}}=GM_^{2}/ (R_L_ )), where (L_) is the luminosity of the protostar.
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The time-scale for the 'flipping' is the accretion time-scale of the inner part of the disc which is expected to be much less than the evolution time of the star's magnetic field.
Given that accretion times are on the order of 10 Myr (Brasser 2013), the scaling places the inner core's (and thus its magnetic field's) onset time before accretion's end and requires inner core growth during accretion and during growth of the core itself.
The Jovian subnebula may have been relatively "gas-starved" when the Galilean satellites formed; this would have allowed for the lengthy accretion times required for Callisto.
Any work of art is an accretion – of time, of learning, of the histories that have gone before it.
In general, at the start of accretion, the time intervals between impacts are relatively short.
In the longitudinal analysis, the baseline REE adjusted for baseline FFM was not predictive of FM accretion over time (p=0.8).
Long-term plots provide an excellent source of information on biomass accretion over time where plots have been maintained and re-measured.
There is a discussion that the lifetime of dense clouds (or the recycling time-scale of dense gas) should be longer than the accretion growth time-scale for an efficient dust growth (Zhukovska et al., 2008; Dwek and Cherchneff, 2011).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com