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accompanied by a much smaller peak of H2, were observed between
position of adsorbed or slightly polymerized C2H4 species. At higher
(all centered at around 530 ◦C) were associated with the decompo-
sition of acetate species [37,38], which accumulated on the catalyst
surface during reaction.
Fig. 16b presents the TPH profiles of the used catalyst which
were also performed at a space-time of 0.20 mg min/ml. As shown,
the main evolution peaks observed were C2H4 (maxima at around
350 ◦C), CH4 (510 ◦C) and CO (550 ◦C), suggesting again that the
carbon species deposited during ESR are C2H4 intermediates and
acetate species. The fact that there was almost no CO2 detected
in this case suggests that the generation of CO2 is not favored in
the reducing atmosphere. Besides, no CH4 was observed in the low
temperature region (< 400 ◦C) [39], implying that almost no CHx is
generated or remained on the catalyst surface under the conditions
applied.
Fig. 16c shows the TP-D2 profiles of the used catalyst performed
at the highest space-time for more than 16 h. As illustrated, the
most abundant desorption peak evolving at temperatures <400 ◦C
was HD (m/e 3), indicating that huge amount of H species remained
on the catalyst surface after test. Meanwhile, the evolution peaks of
CH3D (m/e 17), CH2D2 (m/e 18) and CHD3 (m/e 19) (centered around
200 ◦C) were detected simultaneously, confirming the presence of
CHx group on the catalyst surface. Besides, a trace peak assigned to
CO2 was observed, and can be attributed to the decomposition of
carbonate species formed during reaction. At higher temperatures,
a pronounced peak of CH2D2 (m/e 18, centered at around 620 ◦C)
was accompanied by a much smaller peak of CHD3 (m/e 19) as well
as a trace peak of CH4 (m/e 16). Moreover, significant formation
of HD (m/e 3) and CO were observed in the closely followed tem-
perature region. Together, these observations at high temperature
range again confirm the deposition of acetate species during reac-
tion and its decomposition to form CHx, H2 and CO during heating.
Furthermore, the most abundant CH2D2 (m/e 18) detected among
the CHx derivatives is likely correlated with the stability of CH2
species among the CHx group formed right after the decomposition
of acetate species, further indicating that the C–C bond breaking
may occur through CH2–CO species [40].
which means the co-fed H2 may directly affect the adsorption
and conversion of C2H5OH, especially the dehydrogenation reac-
tion.
Even though 2 wt.% Ni may be too little to maintain suffi-
cient C–C bond rupture activity for syngas formation under the
concerning the reaction scheme and the effect of Ni2+ addition to
Mg(Al)O. Di Cosimo et al. have previously studied the effect of Al
incorporation on MgO on the surface basicity and ethanol conver-
sion [43,44]. They reported that there are surface sites of low (OH−
group), medium (Mn+–O2−), and strong (O2− anions) basic centers
in the surface of Mg(Al)O mixed oxide with 5 > Mg/Al > 1. They fur-
ther reported that the dehydrogenation of C2H5OH to CH3CHO is
favored on the Mg-rich Mg(Al)O oxides because these samples con-
tain a large number of properly positioned Al3+ Lewis acid sites and
Mg2+–O2− basic pairs, which are required for H abstraction steps
leading to ethoxy formation. On the other hand, the dehydration
of C2H5OH also involves the initial surface ethoxy formation on a
weak Lewis acid-strong base pair site. Recently, Jensen et al. [45]
investigated the acid-base property of 2 wt.% Ni/Mg(Al)O catalyst
and concluded that the sample has an intermediate basic strength
of O2− sites and Mn+–O2− pairs and acidic Lewis sites in comparison
with Ni/CaO, Ni/MgO and Ni/Al2O3. Therefore, the ethanol dehy-
drogenation and dehydration could proceed simultaneously and
might also share common steps for H abstraction from C2H5OH (the
ethoxy species) since O2− sites and Mn+–O2− pairs and acidic Lewis
sites exist together over the Ni/Mg(Al)O catalyst. In the current
study, kinetic investigation suggests that CH3CHO and C2H4 are
primary products which are formed in parallel on different active
sites. H2, C2H5OH and H2O compete for the same active sites on
the catalyst surface. Moreover, TPD experiment suggests that C2H4
and H2 are formed via a common intermediate. On the basis of these
observations, it is reasonable that dehydrogenation and dehydra-
tion share the same elementary steps for ethoxy species formation
(C2H5OH ↔ C2H5OH* ↔ C2H5O* + H*).
Although dehydrogenation and dehydration could proceed
simultaneously, much higher selectivities to CH3CHO were
achieved at low space-time region, as shown in Fig. 7. Interest-
ingly, this result is quite different from that obtained for Mg(Al)O
without incorporation of Ni2+ (Fig. S9). As shown, C2H4 selectiv-
ity is always higher than that of CH3CHO. Increasing space-time
increased the selectivity to C2H4, while its value varied lightly with
ethanol conversion at a fixed space-time. A comparison between
the selectivity versus ethanol conversion curves obtained over
Mg(Al)O (Fig. S9) and Ni/Mg(Al)O (Fig. 7), respectively, at differ-
ent space-times reveal two additional differences. First, the C2H4
and CH3CHO selectivities varied with deactivation over Ni/Mg(Al)O
but not over Mg(Al)O. This result suggests that the selective deac-
tivation of the Ni/Mg(Al)O sample is related to catalytic sites which
are created by Ni addition to Mg(Al)O, and that those sites favor
CH3CHO formation. On the other hand, Mg(Al)O deactivated very
little during 1000 min on-stream. Second, Mg(Al)O was selective
towards C2H4, and yielded C2H4:CH3CHO ratios in the range 1.5–3
(Fig. S9), while Ni/Mg(Al)O was selective towards CH3CHO, and
yielded C2H4:CH3CHO ratios in the range 0.33–1 (Fig. 7) under
the same conditions. The opposite selectivity trend observed for
the two materials strongly suggest that sites involving Ni domi-
nate product formation over the Ni/Mg(Al)O material. This effect
is likely related to either a) the abstraction of Ni from the original
hydrotalcite-like precursor during calcination creates defects on
the Mg(Al,Ni)O support which facilitate the adsorption of ethanol
and the activation of H2O to OH− or O2-, or b) partial substitution of
Mg2+ (72 pm) by smaller Ni2+ (69 pm) modifies the abundance of
4. Overall discussion
The Ni/Mg(Al)O catalyst used in this study has previously been
successfully tested as catalyst for the dry reforming of propane
to syngas (CO and H2) at 600 ◦C [26]. A major observation from
the test data presented in this study is that the same Ni/Mg(Al)O
catalyst was barely active for syngas formation from ethanol and
water at 500 ◦C. It mainly produced C2H4, CH3CHO, H2 (and H2O)
the effluent only at the highest space-time employed (Fig. 6 and
8). The reason could be that metallic Ni was rapidly covered
and deactivated by coke, as suggested by the poor initial carbon
mass balance (Fig. 5), or that Ni was mainly present in an oxi-
improving the catalyst performance, H2 addition (Fig. 4) signif-
icantly reduced the ethanol conversion in terms of suppressing
C2H4 and, even more strongly, CH3CHO generation. Laosiripojana
et al. [41,42] studied the effect of co-fed H2 on ESR and CH4 dry
reforming reactions. They attributed the negative effect of H2 on
CH4 conversion to inhibition of the hydrocarbon - lattice oxygen
interaction, and to possible coverage of active Ni sites by hydrogen.
In our case, the negative impacts of H2 co-feed on ethanol conver-
sion and product distribution are probably due to the competition
for the same active sites with C2H5OH and H2O. Another possi-
ble explanation is the consumption of surface OH-/O2− species,
M
n+–O2− pair sites that promote dehydrogenation. However, this
advantage can be diluted by increasing space-time, since much
more acid-base pair sites are available for ethanol conversion,
Please cite this article in press as: G. Zeng, et al., Kinetic and process study of ethanol steam reforming over Ni/Mg(Al)O catalysts: The