Autumn Spring by Shelley Thrasher

By Shelley Thrasher

Bree significant and Linda Morton have sacrificed their own lives for profession and family members. Now, in her overdue sixties, Bree is pressured to come back to her place of birth in East Texas, the place she starts off to find issues approximately herself she has refused to recognize for 50 years. Do either she and Linda—who is ultimately out and proud—have the braveness to assert the kind of lifestyles they’ve by no means allowed themselves to include?

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1979; Cowan et al. 1983). 1 Age Determinations 100 --- a-decay 96 --1 spontaneous fiSSion / 96 z 235U/+/ • / ;+-x+ /*x /. '~ XII ' // 244pu 94 92 /. / /+I ;+ /+" l" / / / 61/+ I 232Th e6 ~ GJ GJ GJ 66 64 ~ 62 60 140 + ES· -4 9 --1 I // 23eU /1 GJ

Acta 40, 617 (1976); cf. also Kirsten 1978] 206 Pb /204Pb iD _ (iD ) = Kp (eu-i) . 2) In a plot of iD/jD vs. Kp/jD, this is a straight line with a slope tana = (eu -1), if (KpßD) is variable, and (1JßD)o is constant. This is the case for pieces of a meteorite or of a rock, if iD and jD are different isotopes of the same chemical element. Initial isotopic ratios should be equal in different probes ("separates") of one rock, since chemical fractionation cannot change these ratios. Thus one can expect eD/jD)o to be constant.

15). When A = 4/27 and K = + 1 there is the possibility of a static solution, the "Einstein Universe" , with a constant radius XE = (~) - 1/3 = 3/2. e. ° ° ° ° R E =(A)-1I2. A small change in A leads from the static universe to an expanding solution. There is a solution starting from x = 0, and "creeping" towards XE, while a third solution starts expanding from the finite radius XE (the "Eddington-Lemaitre Universe") (Fig. 16). -L. case (Fig. 17). L. t L------------~t X Fig. 16. x vs. T for the static Einstein, and the Eddington-Lemaitre model Fig.

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