Szymon
Jarzyński
a,
Cyprian
Doroszko
a,
Daria
Jamroz
a,
Kinga
Stefanowska-Kątna
b,
Jędrzej
Walkowiak
b,
Sławomir
Wojtulewski
c,
Janusz
Zakrzewski
a and
Bogna
Rudolf
*a
aUniversity of Lodz, Faculty of Chemistry, Department of Organic Chemistry, Tamka 12, 91-403 Lodz, Poland. E-mail: bogna.rudolf@chemia.uni.lodz.pl
bCenter for Advanced Technologies, Adam Mickiewicz University, Uniwersytetu Poznańskiego 10, 61-614 Poznań, Poland
cDepartment of Structural Chemistry, Faculty of Chemistry, University of Bialystok, Ciołkowskiego 1K, 15-245 Bialystok, Poland
First published on 17th March 2025
The visible-light irradiation of solutions of CpFe(CO)2I (Cp = (η5-C5H5)), acetylacetone (or other β-diketones), and diisopropylamine in toluene led to the substitution of all ligands with β-diketonate anions and the oxidation of FeII to FeIII. The only product was Fe(β-diketonate)3, which exclusively formed even when using an equimolar ratio of CpFe(CO)2I and diketone. The reaction occurred under both anaerobic and aerobic conditions. The proposed reaction mechanism assigns the key role to the non-innocent behavior of the β-diketonate ligands. Dioxygen or the acetylacetone acts as oxidant. The ruthenium complex CpRu(CO)2I reacts with acetylacetone in a similar way to the corresponding iron complex, but irradiation with UV light is required to assure an acceptable yield of the product. All obtained complexes were analyzed by NMR, FT-IR, and ESI-MS, and one was subjected to single-crystal and powder X-ray diffraction analysis, which revealed its mer stereochemistry.
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| Scheme 1 Photochemical transformations of CpFe(CO)2X: (a) CO ligand exchange,1,2,6,7,9 (b) photolysis in the presence of acidic NH compounds,11–16 and (c) photolysis in the presence of Bu4N+Y− with and without PPh3.17 | ||
These easy and efficient photochemical substitutions of iodido in 1a by anions of N–H acids encouraged us to explore similar reactions using β-diketones, which also contain relatively acidic protons and exhibit rich coordination chemistry.19,20 Surprisingly, we observed that the irradiation of solutions of 1a, acetylacetone (Hacac, 2a), and DIPA in toluene led to the substitution of all ligands with β-diketonate anions, giving Fe(acac)3.
:
2a = 1
:
3) and an excess of DIPA achieved practically complete consumption of 1a, and 3a was isolated in 73% yield (Table 1, entry 5).
| Entry | Deviation from general conditions | Yield 3ab |
|---|---|---|
| a General conditions: CpFe(CO)2I 1a (1 mmol), acetylacetone 2a (3 mmol), DIPA (6 mmol), toluene (10 mL), four 100 W tungsten lamps, 1 h, 0 °C. b Yield was based on isolated product. c N.R. = no reaction. | ||
| 1 | None | 82% |
| 2 | No light | N.R.c |
| 3 | No light, without DIPA | N.R.c |
| 4 | Sunlight | 24% |
| 5 | Under argon | 73% |
| 6 | 1 equiv. of 2a instead of 3 equiv. | 62% |
| 7 | 3 equiv. of DIPA instead of 6 equiv. | 69% |
| 8 | Et3N instead of DIPA | 43% |
| 9 | DBU instead of DIPA | 34% |
| 10 | DIPEA instead of DIPA | 69% |
| 11 | Pyrrolidine instead of DIPA | 58% |
| 12 | THF instead of toluene | 47% |
| 13 | EtOAc instead of toluene | 52% |
| 14 | MeOH instead of toluene | 28% |
As the reaction involved oxidation of FeII → FeIII, we tested whether it would proceed in an oxidizing atmosphere (i.e., air). The presence of air had practically no effect on the course of the reaction or the yield of 3a (Table 1, entry 1). Therefore, all subsequent experiments were carried out in air. DIPA could be replaced by other amines (e.g., Et3N, 1,8-diazabicyclo[5.4.0]undec-7-ene (DBU), N,N-diisopropylethylamine (DIPEA), or pyrrolidine) (Table 1, entries 8–11), but they worked less efficiently. The reaction could also proceed in some other solvents, but less efficiently (Table 1, entries 12–14).
Reactions under aerobic conditions would clearly have dioxygen as the oxidant, with a reduction potential, Ered0 = −0.6 V (O2/O2˙− in DMF vs. a normal hydrogen electrode).21 However, the control experiment showed that oxygen is not capable of oxidizing 1a in either its ground or excited state: the irradiation of this complex in aerated toluene resulted only in its practically quantitative recovery. Hacac displayed even weaker oxidizing properties (Ered0 = −2.2 V in DMF vs. SCE),22 corresponding to its reduction to acac− and ½ H2. This means that the FeII → FeIII oxidation step did not involve 1a; instead, an intermediate was formed during the reaction. Oxygen is most likely the oxidant in aerobic reactions, while in its absence the weaker oxidant Hacac fulfills this function.
We also used ultraviolet (UV)–visible (vis) and infrared (IR) spectroscopy to observe the solutions of photolyzed aerated 1a in toluene with Hacac and DIPA in an effort to detect possible intermediates. However, the exclusive formation of 3a at an equimolar ratio of 1a and Hacac (Table 1, entry 6) suggests a very rapid transformation of the primary photolysis product with respect to its formation rate.
The spectra in Fig. 1 clearly show that 1a (λmax = 346 nm) transformed into 3a (λmax = 354 nm and λmax = 436 nm). The presence of isosbestic points23 at 389 and 555 nm indicates that during the whole process, the photolyzed solution contained only these two iron-containing components. The spectra also intersect at about 340 nm, but without an isosbestic point. The lack of such a point is most likely related to the influence of absorption in this range by Hacac and acac− (λmax = 270–290 nm), whose concentrations changed during photolysis.
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| Fig. 1 Changes in UV–vis spectra during visible irradiation of an aerated solution of 1a (0.3 mM), 2a (0.9 mM), and DIPA (1.8 mM) in toluene at 0 °C; stars denote isosbestic points. | ||
The in situ IR study led to the same conclusion. The photolysis caused the disappearance of the absorption bands for the CO ligand of 1a (2040 and 1995 cm−1) and the appearance of intense absorption bands for 3a (1555 and 1518 cm−1; Fig. 2). The disappearance of the CO ligand bands was not accompanied by the appearance of any new absorption band in this spectral range. Fig. 3 shows the decay of 1a (as represented by the bands at 2040 and 1995 cm−1) and the formation of 3a (via bands at 1555 and 1518 cm−1). The sum of the intensities of both sets of bands shows little change with time, indicating that the reaction proceeded with no detectable intermediate. We believe that the reaction involved the rapid stepwise substitution of the ligands in 1a with acac ligands (Scheme 3).
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| Fig. 3 Temporal evolution of the conversion of 1a to 3a during photolysis, as measured by the intensities of the bands at 2040 and 1995 cm−1 (1a) and those at 1555 and 1518 cm−1 (3a). | ||
The first step of the reaction is the photochemical replacement of the iodido ligand with an acac anion to form complex I. The feasibility of the substitution is strongly supported by previous reports on similar photochemical substitutions of the iodido ligand in 1a with anionic nitrogen ligands.12,13,16,17,24,25 The suggested next step is intramolecular CO substitution, resulting in the formation of complex II with acac chelation (Scheme 3). The chelating acac ligand has been previously reported to behave as a non-innocent redox ligand.26,27 This means that it can accept additional electron density from the metal to increase its formal oxidation state.28–33 Therefore, it can be assumed that complex II is in equilibrium with its valence tautomer IIa, which contains an FeIII center and reactive acac2− anion radical.34 This increase in electron density on the acac ligand might strengthen its reducing power to allow its oxidation by dioxygen or Hacac.
In the next step of the reaction the remaining CO ligand is replaced by the η1-acac ligand, leading to complex IV and starting the sequence IV → V → VI → 3a. This substitution is accompanied by the η5-η3-η1 slippage of the Cp ligand.35
We also tested the reaction using the ruthenium analogue of 1a, CpRu(CO)2I (1b), and 2a. In this case, however, the aerobic reaction under irradiation with visible light was slow and only 16% of the ruthenium(III) acetylacetonate 4 was isolated after 6 h. A higher yield was obtained in the reaction using UV light (350 nm). After 3h of irradiation, complex 4 was isolated in 37% yield (Scheme 5). Comparison of UV–vis absorption spectra of 1a and 1b provides a plausible explanation for the different photochemical reactivity of these compounds (Fig. 4). The spectrum of 1a shows weak broad long-lying absorption bands with maxima at 500 and 648 nm, which were assigned to the symmetry-forbidden d–d transition.16,17 Irradiation into these bands induces substitution of the iodido ligand in 1a with the pyrrolyl anion. In contrast, the spectrum of 1b shows negligible absorption in the range of 500–700 nm. Its lowest-energy band is observed at 423 nm, tailing into the UV region. Therefore, in this case UV irradiation is more strongly absorbed and more efficient.
Optimization of the reaction conditions is shown in Table 2.
| Entry | Deviation from general conditions | Yield 4b |
|---|---|---|
| a General conditions: 1b (1 mmol), 2a (3 mmol), DIPA (6 mmol), toluene (10 mL), 3 h, 0 °C. b Yield was based on isolated product. c N.R. = no reaction. d Time of reaction was 6 h. | ||
| 1 | None | 37% |
| 2 | No light | N.R.c |
| 3 | Visible light | 16%d |
| 4 | Et3N instead of DIPA | 13% |
| 5 | DIPEA instead of DIPA | 21% |
| 6 | THF instead of toluene | 28% |
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| Fig. 5 Molecular structure of crystalline 3f. Displacement ellipsoids are drawn at the 50% probability level. | ||
| Identification code | 3f |
|---|---|
| Empirical formula | C33H33O9Fe |
| Formula weight | 629.44 |
| Crystal system | Monoclinic |
| Space group | P21/c |
| a | 14.2832(7) Å |
| b | 15.6780(8) Å |
| c | 13.2979(5) Å |
| β | 97.346(4)° |
| Volume | 2953.4(2) Å3 |
| Z | 4 |
| ρ calc | 1.416 g cm−3 |
| μ | 0.566 mm−1 |
| F(000) | 1316 |
| 2Θ range for data collection | 5.18° to 58.256° |
| Index ranges | −19 ≤ h ≤ 19, −21 ≤ k ≤ 21, −16 ≤ l ≤ 18 |
| Reflections collected/independent | 33 711/7948 [Rint = 0.0405, Rsigma = 0.0346] |
| Data/restraints/parameters | 7948/0/394 |
| Goodness-of-fit on F2 | 1.086 |
| Final R indexes [I> = 2σ(I)] | R 1 = 0.0668, wR2 = 0.1732 |
| Final R indexes [all data] | R 1 = 0.0850, wR2 = 0.1857 |
| Largest diff. peak/hole | 0.62/−0.45 e Å−3 |
| CCDC no. | 2371792† |
Additionally, a powder X-ray diffraction experiment conducted on a polycrystalline sample and a randomly selected bulk sample support that statement.
Fig. 6 presents a compilation of diffractograms for the single polycrystalline rosette, the crushed crystallites and the single crystal, calculated from the CIF file. The compilation is accompanied by photographs of the samples. A comparison of the measurements of the polycrystalline samples a and b reveals their phase to be identical. Moreover, a comparison with the calculated diffractogram demonstrates the corresponding order and size of the dominant reflections. The slight discrepancy in their positions can be attributed to the difference in measurement temperature; the monocrystal of the compound was measured at 100 K, while the polycrystals were measured at room temperature. The reduction in crystal lattice magnitude under low-temperature conditions resulted in an observed shift of the reflections by a few hundredths of angle 2Θ towards higher values, as would be expected.
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| Fig. 6 The diffractograms of 3f: a – single polycrystalline rosette; b – ground crystallites; c – calculated from the cif file of monocrystal measurements. | ||
The overall coordination sphere can be described as a slightly distorted octahedron. The lengths of the Fe–O bonds are relatively constant (approximately 2.0 Å), with differences of less than 0.01 Å. Nevertheless, the coordination sphere is slightly distorted with regard to the O–Fe–O valence angles. Ligand C shows the greatest deviation from a right angle of approximately 5°, while ligands A and B exhibit an O–Fe–O valence angle of about 87°. As a result, the nominally linear arrangements of O1A–Fe1–O2C, O2A–Fe1–O2B, and O1B–Fe1–O1C showed slight deviations, with valence angles of approximately 177°, 171°, and 169°, respectively.
CpFe(CO)2I (1a) and CpRu(CO)2I (1b) were synthesized according to a previously published procedure.38
The initial black color of the solution became red upon irradiation. After the reaction was completed (1–8 h), silica gel was added to the mixture. The solvent was evaporated in vacuo, and the crude reaction mixture was purified by flash column chromatography (![[C with combining low line]](https://www.rsc.org/images/entities/char_0043_0332.gif)
; dry packing, hexane/dichloromethane/methanol eluent) to afford the corresponding product.
:
5). For the 1H NMR spectrum see ESI Fig. S5.†IR (KBr, cm−1) 2961, 2920, 1565, 1517, 1420, 1350, 1271, 1189, 1011, 927, 770, 665, 549. ESI-MS (m/z): 254.20 ([M-ligand]+). Anal. calcd for C15H21FeO6 (353.17): C 51.01, H 5.99; found: C 51.11, H 5.95.
:
9). For the 1H NMR spectrum see ESI Fig. S6.†IR (KBr, cm−1) 2965, 2930, 2871, 1562, 1532, 1500, 1404, 1298, 1159, 1093, 922, 789, 690, 585. ESI-MS (m/z): 366.40 ([M-ligand]+), 544.5 ([M + Na]+). Anal. calcd for C27H45FeO6: C 62.19, H 8.70; found: C 62.09, H 8.66.
:
1). For the 1H NMR spectrum see ESI Fig. S7.†IR (KBr, cm−1) 2964, 2905, 2866, 1546, 1506, 1454, 1394, 1352, 1246, 1226, 1177, 1144, 872, 797, 623, 503. ESI-MS (m/z): 606.5 ([M + H]+), 628.60 ([M + Na]+). Anal. calcd for C33H57FeO6: C 65.44, H 9.49; found: C 65.47, H 9.54.
:
1). For the 1H NMR spectrum see ESI Fig. S8.†IR (KBr, cm−1) 2934, 1606, 1523, 1506, 1452, 1365, 1283, 1225, 1192, 1130, 948, 861, 788, 729, 581, 502. ESI-MS (m/z): 538.20 ([M + Na]+). Anal. calcd for C15H12F9FeO6: C 34.98, H 2.35; found: C 34.93, H 2.37.
:
9). For the 1H NMR spectrum see ESI Fig. S9.†IR (KBr, cm−1) 3058, 2993, 2964, 1588, 1544, 1508, 1487, 1449, 1378, 1357, 1306, 1292, 1207, 1180, 999, 959, 773, 715, 684, 576, 447. ESI-MS (m/z): 378.40 ([M-ligand]+). Anal. calcd for C30H27FeO6: C 66.80, H 5.05; found: C 66.83, H 4.98.
:
9). For the 1H NMR spectrum see ESI Fig. S10.†IR (neat, cm−1) 2924, 2840, 1583, 1521, 1492, 1417, 1352, 1291, 1250, 1169, 1113, 1024, 959, 842, 776, 637, 506. ESI-MS (m/z): 438.08 ([M-ligand]+). Anal. calcd for C33H33FeO9: C 62.97, H 5.28; found: C 62.90, H 5.29.
:
9). For the 1H NMR spectrum see ESI Fig. S11.†IR (neat, cm−1) 3006, 2971, 1580, 1509, 1483, 1404, 1354, 1294, 1173, 1091, 1011, 998, 956, 850, 779, 752, 594. ESI-MS (m/z): 446.20 ([M-ligand]+). Anal. calcd for C30H24Cl3FeO6: C 56.06, H 3.76; found: C 56.19, H 3.79.
:
1). For the 1H NMR spectrum see ESI Fig. S12.†IR (KBr, cm−1) 3140, 3066, 1596, 1570, 1453, 1323, 1294, 1251, 1197, 1142, 1073, 942, 776, 699, 638, 592, 538. HRMS (ESI)m/z calcd for C30H19F9FeO6+ ([M + H]+): 702.0387; found: 702.0387. Anal. calcd for C30H18F9FeO6: C 51.38, H 2.59; found: C 51.42, H 2.62.
:
95). For the 1H NMR spectrum see ESI Fig. S13.†IR (KBr, cm−1) 3113, 1567, 1540, 1508, 1404, 1350, 1308, 1255, 1232, 1192, 1136, 1066, 1014, 933, 862, 798, 730, 647, 588. ESI-MS (m/z): 498.20 ([M-ligand]+), 742.30 ([M + Na]+). Anal. calcd for C24H12F9FeO6S3: C 40.07, H 1.68; found: C 40.10, H 1.56.
:
9). For the 1H NMR spectrum see ESI Fig. S14.†IR (KBr, cm−1) 3153, 3125, 1593, 1574, 1458, 1437, 1311, 1261, 1199, 1150, 1138, 1097, 1018, 945, 883, 862, 772, 679, 591. ESI-MS (m/z): 466.20 ([M-ligand]+), 694.20 ([M + Na]+). Anal. calcd for C24H12 F9FeO9: C 42.95, H 1.80; found: C 43.01, H 1.65.
:
9). For the 1H NMR spectrum see ESI Fig. S15.†IR (KBr, cm−1) 3055, 3025, 2964, 1590, 1529, 1522, 1478, 1452, 1380, 1359, 1315, 1225, 1180, 1066, 1024, 939, 757, 721, 686, 621, 548. HRMS (ESI)m/z calcd for C45H34FeO6+ ([M + H]+): 726.1705; found: 726.1722. Anal. calcd for C45H33FeO6: C 74.49, H 4.58; found: C 74.60, H 4.51.
:
9). For the 1H NMR spectrum see ESI Fig. S16.†IR (neat, cm−1) 2955, 2924, 2853, 1601, 1586, 1519, 1498, 1476, 1447, 1374, 1355, 1298, 1253, 1222, 1169, 1022, 936, 842, 789, 711, 691, 603, 531. HRMS (ESI)m/z calcd for C48H40FeO6+ ([M + H]+): 816.2022; found: 816.2003. Anal. calcd for C48H39FeO9: C 70.68, H 4.82; found: C 70.64, H 4.86.
:
9). For the 1H NMR spectrum see ESI Fig. S17.†IR (neat, cm−1) 3056, 3030, 1737, 1587, 1511, 1475, 1446, 1403, 1351, 1311, 1295, 1221, 1090, 1011, 937, 793, 763, 685, 636, 535. ESI-MS (m/z): 570.30 ([M-ligand]+). Anal. calcd for C45H30Cl3FeO6: C 65.20, H 3.65; found: C 65.13, H 3.52.
:
5). For the 1H NMR spectrum see ESI Fig. S19.†IR (KBr, cm−1) 2997, 2919, 1541, 1516, 1375, 1364, 1268, 1018, 934, 778, 622, 454 cm−1. ESI-MS (m/z): 400.30 ([M + H]+). Anal. calcd for C15H21RuO6: C 45.22, H 5.31; found: C 45.05, H 5.24.
The non-hydrogen atoms were refined anisotropically. Hydrogen atoms were introduced in calculated positions with idealized geometry and constrained using a rigid-body model with isotropic displacement parameters equal to 1.2 and 1.5 in the case of CH and CH3 hydrogen atoms, respectively. Table 3 summarizes the relevant crystallographic data.
Footnote |
| † Electronic supplementary information (ESI) available: Synthesis of β-diketones, crystallographic data and 1H NMR spectra of compounds 3a–n and 4. CCDC 2371792. For ESI and crystallographic data in CIF or other electronic format see DOI: https://doi.org/10.1039/d5dt00294j |
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