A 13C-n.m.r. study of the tungstate and molybdate complexes of perseitol, galactitol, and d -mannitol

A 13C-n.m.r. study of the tungstate and molybdate complexes of perseitol, galactitol, and d -mannitol

279 Carbohydrate Research, 211 (1991) 279~~286 Elsevier Science Publishers B.V., Amsterdam A 13C-n.m.r. study of the tungstate and molybdate complex...

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279

Carbohydrate Research, 211 (1991) 279~~286 Elsevier Science Publishers B.V., Amsterdam

A 13C-n.m.r. study of the tungstate and molybdate complexes of perseitol, galactitol, and D-mannitol* Stella Chapellet Lahoratoire

de R.M.N.

de I’UniversitG de Rouen,

76134 Mont-Saint-Aignan

and Jean-Francois U.R.A.

U.R.A.

464 du C.N.R.S.,

Faculth des Sciences,

B P. 118,

iFrance)

Verchtre

500 du C.N.R.S.,

UniwrsitP

de Rouen,

Fmul~k dcs Sciences,

i3.P. 118, 76/34 Mont-Saint-Aignan

(France) (Received

June

18th, 1990; accepted

for pubkation,

September

7th, 1990)

ABSTRACT

Perseitol stability

(D-gl~cero-D-galucto-heptitol)

higher than those of galactitol

magnitude

higher

complexes

had similar

than those for molybdate.

the galucto group D-Mannitol reversed

structures

in galactitol

and perseitol

formed

forms

and D-mannitol,

dinuclear

The ‘?C-n.m.r.

that involved and perseitol,

complexes

data showed

four vicinal hydroxyl complexes

that

have

a

are three orders of and molybdate

The sites of chelation

HO-3.45

that involved

tungstate

constants

that the tungstate

groups.

and the arahino group

pairs of isomeric

with

and all ofthe formation

and HO-6

involved

in D-mannitol.

the same site of chelatton

but in

orientations.

INTROI>UCTION

Alditols are well-known complexing agents for molybdate MOO,*- and tungstate WO,‘~ ions in aqueous acidic solution. Dinuclear anionic complexes are formed as indicated by a series of polarimetric and potentiometric studies’~“. The crystal structures of D-mannitol”.“’ and erythritol” molybdate complexes showed that the chelation involved four vicinal hydroxyl groups. ‘3C-N.m.r. studies demonstrated that themolybdate complexes of most polyols retained this structure in solution, and attempts were made to classify different types of tungstate’ and molybdate”~” complexes. y5Mo-N.m.r. spectroscopy revealed two non-equivalent MO atoms I4 in complexes of aldoses of the I~xoPmannn series, which chelated molybdate as tetradentate donors. Tungstate complexes have been used for the chromatographic separation of carbohydrates”, and alditols are useful complexing agents in the acidimetric titration of tungstate”‘. The thermodynamic data showed that the most stable complex was formed with perseitol (D-glycero-D-ga/acto-heptitol). We now report on the stabilities and structures of the molybdate and tungstate complexes of perseitol. Since two tetritol

* Communicated in part at the First Mediterranean 21-23, 1990. +Author for correspondence. 0008-6215/91/$03.50

@ 1991 - Elsevier

Conference

Science Publishers

on Carbohydrates,

B.V.

Avignon,

France,

May

280

S. < fihl'l~1.l.l..J.-f-. VI

K('fWKI

TUNGSTATE

TABLE

AND MOLYBDATE

COMPLEXES

281

II

100.62-MHz “C-n.m.r. complexes of galactitol

chemical

shifts (6 in p.p.m.) and ‘J,.,H values (Hz) for the tungstate

C-l

” ‘J,,u 141 Hz for C-I/6:

TABLE

OF ALDITOLS

c-2

c-3

C-4

C-5

and molybdate

C-6

65.5

71.5

72.1

72.1

71.5

65.5

65.3 143 -0.2

79.0 147 7.5

91.4 150 19.3

82.9 150 10.8

82.4 141 10.9

64.5 142 - 1.0

64.7 143 -0.X

19.4 144 7.9

91.8 149 19.7

83.7 I47 Il.6

83.3 146 11.8

65.5 143 0.0

6 assigned

from the literature”.

Accuracy:

J kO.1 p.p,m.;

J *I

Hz. ’ Ref. 13.

III

100.62-MHz “C-n.m.r. chemical complexes of u-mannitol

shifts (6 in p.p.m.)

C-I

and ‘J(.H values (Hz) for the tungstate

c-2

c-3

c-4

c-5

and molybdate

C-6

65.8

74.2

71.6

71.6

74.2

65.3 143 -0.5

72.9 143 - 1.3

81.9 147 10.3

82.7 150 Il.1

92.5 150 18.3

71.0 145 5.2

65.1 143 -0.7

73.7 143 -0.5

79.1 144 7.5

91.6 150 20.0

82.7 150 8.5

73.1 147 7.3

65.4 142

73.1 142

83.3 145

83.8 149

93.1 148

‘71.7 145

-0.4

-0.9

11.7

12.2

18.9

5.9

65.9 142 0.1

74.1 142 -0.1

80.3 143 x.7

92.3 148 20.7

83.8 149 9.6

‘74.1 1,45 8.3

” ‘JCH 141 Hz for C-1:6; b assigned

from the literature”.

Accuracy:

6 kO.1 p.p.m.;

65.8

J k 1 Hz. h Ref. 13.

complexes (M, and MJ that involved the arc&no group HO-3,4,5 and HO-6. The deshielding pattern characteristic of the galactitol species (i.e., 7-2tSlO-10 p.p.m.) was also observed for the D-mannitol complexes. However, for a given pair of complexes, these patterns were reversed, which suggested that the isomerism was due to the asymmetry of the chelating site, in which C-3,6 bore different substituents, in contrast to

hi

3

61.1 133 0 I

TUNGSTATE

AND MOLYBDATE

COMPLEXES

For the pair of molybdate matched

those reported”,

had been assigned and HO-3,4,5,6 unlikely, molybdate

the assignments

from ‘H- and ‘%-n.m.r.

since it was shown

Unambiguous

assignments

pair of perseitol

that

complexes

our spectra

The complexing

data as HO-2,3,4,5 t,-mannitol

The carbon-chain assignments

for P?. No evidence

closely

sites of perseitol

(the galucto group) in P,

did not complex

for the Pz molybdate

the proposed

assignment

differed.

IV), although

but with the galucto-like

experiments.

data. However,

above tentative

(Table

in Pz (see Fig. 1). The second assignment

above

by its munno group,

clear 2D-‘H-n.m.r. literature

complexes

(the manno group)

283

OF ALDITOLS

appeared

tungstate

or

group HO-3,4,5,6.

complex were made by homonusequence

was in agreement

were reversed

was obtained

differed from those formed

in order to verify the

to indicate

by alditols

with

that the P,-P,

that possess related

complexing sites such as D-arabinitol, D-mannitol, and D-glucitol”. Using an excess of molybdate, the 95Mo-n.m.r. spectra of perseitol-molybdateHCI mixtures contained a sharp signal for free molybdate at 6 -0 and a new broad

CH,OH

galacto

CH,OH Perseitol

Fig. 1. Schematic representation of the chelation of the dimolybdate anion by four vicinal hydroxyl groups of an alditol molecule; R and R’ are CH,OH in galactitol, H and CHOH-CH20H in u-mannitol, and CH20H and CWOH-CH20H in perseitol. When R + R’, a pair of isomers is formed. The dimolybdate structure is that characterised in the complexes of wmannitol’.‘” and erythritol”.

2x3

\.

(

tlAI’l~1.I.l

I.-f.

\.I K(~FII:KI:

TUNGSTATE

should

AND MOLYBDATE

COMPLEXES

285

OF ALDITOLS

have been much higher if complex

P? (40% of total) had involved

group. These results accord with the finding that molybdate goups of D-mannitol

and perseitol.

Determination quantitative

of the formation

support

molybdate-catalysed active

molybdate

Published

constants

for the interpretation epimerisation

species

of the molybdate

of recent results”

of aldoses.

by complexation,

It is believed thereby

data on the relative yields of the reaction

h, 90’) indicated

the manno

is not chelated by the manno

the order of stability

to be perseitol

that alditols

reducing

D-glucose

complexes

provides

on the inhibition

of the

scavenge

the

the rate of reaction.

-+ D-mannose

> galactitol

(pH 3.5, 3

> D-mannitol

>

D-arabinitol > ribitol, in excellent agreement with the results in Table I and earlier results for D-arabinitol and ribitol”, and confirm that the dinuclear molybdate complexes are the species responsible for the reported decrease in the rate of epimerisation. EXPERIMENTAL

All chemicals were of analytical grade and perseitol supplied. Water was de-ionised in a Millipore apparatus.

(Aldrich)

was used

as

Formation constants were determined by potentiometry’4x’6, based on the determination of the half-equivalence pH, ,2values in acidimetric (HCl) titrations of disodium molybdate

or tungstate

solutions

of known

concentration

that

contained

various

amounts of alditol. Measurements were made at constant ionic strength (KCl, 0.1~). All ID- and 2D-n.m.r. spectra were recorded with a Bruker AM 400 spectrometer equipped with a 5-mm multinuclear probe. Solutions contained alditol(0.5 mmol) and disodium molybdate or tungstate dihydrate (1.5 mmol) in DzO (0.5 cm”). Cont. HCl (0.75 mmol) was added last, in order to avoid the precipitation of tungsten trioxide. The ‘5Mo-n.m.r.

measurements

were made as described’3,‘4.

For the “C-n.m.r.

experiments, the proton-coupled and -decoupled spectra were obtained with n.0.e. The chemical shifts were determined by the substitution method’“, using the trimethylsilylphosphate reference signal in DzO. ZD-Heteronuclear experiments were performed*’ with polarisation transfer from ‘H to 13C, the number of experiments being 64 x 1k. Initial assignments of ‘H spectra of mixtures of complexes required 2D-homonuclear experiments

(COSY-45)22,‘3.

REFERENCES I 2 3 4 5 6 7 8 9 IO

I1

N. K. Richtmyer and C. S. Hudson, J. Am. Chum. SW.. 73 (1951) 2249 -2250. E. J. Bourne, D. H. Hutson, and H. Weigel, J. Chem. Sot.. (1961) 35-38. H. J. F. Angus and H. Weigel, J. Chem. Sot., (1964) 3994-4000. H. J. F. Angus, E. J. Bourne, and H. Weigel, d. Chem. SW., (1965) 21 -26. W. Voelter, E. Bayer, R. Records. E. Bunnenberg. and C. Djerassi, Chem. Bet-., 102 (1969) 1005-1019. L. Pettersson, Acta Chem. &and., 26 (1972) 4067-4083. M. Mikesova and M. Bartusek. Collect. Czech. Chem. Commun., 43 (1978) 1867-1877. E. Llopis, J. A. Ramirez, and A. Cervilla, Polyhedron, 5 (1986) 2069-2074. J. E. Godfrey and J. M. Waters, Cryst. Strut. Commun., 4 (1975) S-8. B. Hedman, Acta Cr~sfallogr., Sect. E, 33 (1977) 3077-3083. L. Ma, S. Liu, and J. Zubieta. Polyhedron, 8 (1989) 1571-1573.