Previous investigations of goethite revealed a substantial variation of col
or and diffuse reflectance spectra (DRS) in the extended visible range (350
-2200 nm). To better understand the causes of this variability and to asses
s the potential of DRS as a mineralogical tool, we investigated the DRS of
pure and A1-substituted goethite. alpha-Fe1-xAlxOOH with x from 0 to 0.33,
and mean crystal lengths (MCL) from 170 to 1800 nm. The strongly overlappin
g ligand field bands were extracted by fitting the single-electron transiti
ons (6)A(1) --> T-4(1), (6)A(1) --> T-4(2), (6)A(1) --> (E-4; (4)A(1)), and
(6)A(1) --> E-4(D-4) as functions of the ligand field splitting energy, 10
Dq, and the interelectronic repulsion parameters, Racah-B and -C. With x i
ncreasing from 0 to 0.33, (6)A(1) --> T-4(1) decreased from 10,590 to 10,15
0 cm(-1) (944 to 958 nm), and (6)A(1) --> T-4(2) decreased from 15,310 to 1
4,880 cm(-1) (653 to 672 nm), while 10 Dq increased from 15,770 to 16,220 c
m-l. From the change of 10 Dq we calculated a decrease of the Fe-(O,OH) dis
tances from 202.0 to 200.9 pm (-0.5%). This decrease is smaller than the av
erage decrease of all (Al,Fe)-(O,OH) distances (-1.8%) calculated from the
change of the unit-cell lengths (UCL). That is, there remains a substantial
difference in size between the larger Fe- and the smaller Al-occupied octa
hedra in the solid solution which may indicate the existence of diaspore cl
usters within the goethite structure. The increasing strain in the crystal
structure due to the size mismatch and limited contractibility of the oxyge
n cage around Fe may be the primary reason for Al substitution being restri
cted to x < 0.33. The bands (6)A(1) --> (E-4; (4)A(1)) and (6)A(1) --> E-4(
D-4) did not shift, indicating a constant covalency of the Fe-(O,OH) bonds
with B = 628 cm(-1) and C = 5.5B. Whereas variation of band energies could
be explained in terms of the Fe-(O,OH) ligand held, the variation of color
and band intensities was mainly determined by crystal size. Although our st
udy confirmed the potential of DRS for mineralogical investigations, there
is still a gap between the fundamental theory and the explanation of some s
pectral features.