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ORNL-4191 - the Molten Salt Energy Technologies Web Site

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Fig. 18.2.<br />

carbides. 1000~.<br />

carbides. Figure 18.4 shows <strong>the</strong> correspondence<br />

between <strong>the</strong> morphologies of <strong>the</strong> extracted precipitate<br />

and that indicated by <strong>the</strong> autoradiograph.<br />

A selected area diffraction pattern and an electron<br />

probe microanalyzer trace are also included.<br />

This type of precipitate has not yet been identified,<br />

but <strong>the</strong> diffraction pattern does not correspond<br />

to MbC. A comparison of <strong>the</strong> microprobe<br />

results with standards shows that <strong>the</strong> noncarbon<br />

constituents are about 90% Mo and 10% Cr. However,<br />

some M,C carbides are also present after<br />

high-temperature anneals and exist in several<br />

morphologies.<br />

We are concluding our investigation of precipitation<br />

in standard Hastelloy N and will be evaluating<br />

<strong>the</strong> information generated and attempting<br />

to relate our observations to observed changes in<br />

mechanical properties.<br />

Because of <strong>the</strong> attractive in-reactor properties<br />

of <strong>the</strong> titanium-modified Hastelloy N, we are expanding<br />

our studies to include this material. Optical<br />

metallography shows <strong>the</strong> alloy to be quitc<br />

free of precipitate. Initial electron microscopy<br />

studies of two experimental heats revealed that<br />

220<br />

Extraction Replica from Hastelloy N (Heat 5065)Aged 4 hr at 1600OF. All precipitates are M 6 C<br />

a considerable amount of very thin, fine precip-<br />

itate was present in <strong>the</strong> grain boundaries. This<br />

was rarely detected in thin-foil transmission mi-<br />

croscopy but was readily seen by <strong>the</strong> extractim<br />

replica technique.<br />

Selected area electron diffraction studies on<br />

<strong>the</strong> fine grain-boundary precipitates have revealed<br />

at least two phases, which exist in many mor-<br />

phologies. Although <strong>the</strong>se precipitates have not<br />

been positively identified, indications are quite<br />

good that Ti,O is one phase and that it is present<br />

in conjunction with <strong>the</strong> second type. The o<strong>the</strong>r<br />

phase has a face-centered cubic structure with a<br />

lattice parameter of about 4.27 A and may exist<br />

independently of <strong>the</strong> former. Considering chemical<br />

composition, TIC seems to be <strong>the</strong> most likely com-<br />

position of <strong>the</strong> second phase. However, <strong>the</strong> re-<br />

ported lattice parameter for Tic is 4.33 A, com-<br />

pared with our measured value of 4.27 A. TiN and<br />

TiB have lattice parameters more closely related<br />

to <strong>the</strong> measured value; however, chemical analyses<br />

of <strong>the</strong> heats involved show <strong>the</strong> boron and nitrogen<br />

contents to be extremely low.

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