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一种包含六个紧密堆积的钆(III)离子的星爆状异金属化合物。

A starburst-shaped heterometallic compound incorporating six densely packed gd(3+) ions.

作者信息

Livramento João Bruno, Sour Angélique, Borel Alain, Merbach André E, Tóth Eva

机构信息

Laboratoire de Chimie Inorganique et Bioinorganique, Ecole Polytechnique Fédérale de Lausanne, EPFL-BCH, 1015 Lausanne, Switzerland.

出版信息

Chemistry. 2006 Jan 23;12(4):989-1003. doi: 10.1002/chem.200500969.

Abstract

The heterotritopic ligand [bpy(DTTA)2]8- has two diethylenediamine-tetraacetate units for selective lanthanide(III) coordination and one bipyridine function for selective Fe(II) coordination. In aqueous solution and in the presence of these metals, the ligand is capable of self-assembly to form a rigid supramolecular metallostar structure, [Fe[Gd2bpy(DTTA)2(H2O)4]3]4-. We report here the physicochemical characterization of the dinuclear complex [Gd2bpy(DTTA)2(H2O)4]2- and the metallostar [Fe[Gd2bpy(DTTA)2(H2O)4]3]4- with regard to potential MRI contrast agent applications. A combination of pH potentiometry and 1H NMR spectroscopy has been used to determine protonation constants for the ligand [bpy(DTTA)2]8- and for the complexes [Fe[bpy(DTTA)2]3]22- and [Y2bpy(DTTA)2]2-. In addition, stability constants have been measured for the dinuclear chelates [M2bpy(DTTA)2]n- formed with M = Gd3+ and Zn2+ (log K(GdL) = 18.2; log K(ZnL) = 18.0; log K(ZnHL) = 3.4). A multiple field, variable-temperature 17O NMR and proton relaxivity study on [Gd2bpy(DTTA)2(H2O)4]2- and Fe[Gd2bpy(DTTA)2(H2O)4]3 yielded the parameters for water exchange and the rotational dynamics. The 17O chemical shifts are indicative of bishydration of the lanthanide ion. The exchange rates of the two inner-sphere water molecules are very similar in the dinuclear [Gd2bpy(DTTA)2(H2O)(4)]2- and in the metallostar (k(ex)298 = 8.1 +/- 0.3 x 10(6) and 7.4 +/- 0.2 x 10(6) s(-1), respectively), and are comparable to k(ex)298 for similar Gd(III) poly(amino carboxylates). The rotational dynamics of the metallostar has been described by means of the Lipari-Szabo approach, which involves separating global and local motions. The difference between the local and global rotational correlation times, tau(lO)298 = 190 +/- 15 ps and tau(gO)298 = 930 +/- 50 ps, respectively, shows that the metallostar is not completely rigid. However, the relatively high value of S2 = 0.60 +/- 0.04, describing the restriction of the local motions with regard to the global one, points to a limited flexibility compared with previously reported macromolecules such as dendrimers. As a result of the two inner-sphere water molecules, with their near-optimal exchange rate, and the limited flexibility, the metallostar has a remarkable molar proton relaxivity, particularly at high magnetic fields (r1 = 33.2 and 16.4 mM(-1) s(-1) at 60 and 200 MHz, respectively, at 25 degrees C). It packs six efficiently relaxing Gd(III) ions into a small molecular space, which leads, to the best of our knowledge, to the highest relaxivity per molecular mass ever reported for a Gd(III) complex. The [bpy(DTTA)2]8- ligand is also a prime candidate as a terminal ligand for constructing larger sized, Fe(II) (or Ru(II))-based metallostars or metallodendrimers loaded with Gd(III) on the surface.

摘要

异三齿配体[bpy(DTTA)₂]⁸⁻有两个二乙撑三胺五乙酸单元用于选择性镧系元素(III)配位,还有一个联吡啶官能团用于选择性铁(II)配位。在水溶液中且有这些金属存在时,该配体能够自组装形成刚性超分子金属星结构[Fe[Gd₂bpy(DTTA)₂(H₂O)₄]₃]⁴⁻。我们在此报告双核配合物[Gd₂bpy(DTTA)₂(H₂O)₄]²⁻和金属星[Fe[Gd₂bpy(DTTA)₂(H₂O)₄]₃]⁴⁻在潜在磁共振成像造影剂应用方面的物理化学表征。结合使用pH电位滴定法和¹H核磁共振光谱法来测定配体[bpy(DTTA)₂]⁸⁻以及配合物[Fe[bpy(DTTA)₂]₃]²²⁻和[Y₂bpy(DTTA)₂]²⁻的质子化常数。此外,还测量了与M = Gd³⁺和Zn²⁺形成的双核螯合物[M₂bpy(DTTA)₂]ⁿ⁻的稳定常数(log K(GdL) = 18.2;log K(ZnL) = 18.0;log K(ZnHL) = 3.4)。对[Gd₂bpy(DTTA)₂(H₂O)₄]²⁻和Fe[Gd₂bpy(DTTA)₂(H₂O)₄]₃进行的多场、变温¹⁷O核磁共振和质子弛豫率研究得出了水交换和旋转动力学的参数。¹⁷O化学位移表明镧系离子的双水合作用。双核[Gd₂bpy(DTTA)₂(H₂O)₄]²⁻和金属星中两个内球水分子的交换速率非常相似(k(ex)₂₉₈分别为8.1±0.3×10⁶和7.4±0.2×10⁶ s⁻¹),与类似的Gd(III)聚氨基羧酸盐的k(ex)₂₉₈相当。金属星的旋转动力学已通过Lipari-Szabo方法进行描述,该方法涉及分离整体运动和局部运动。局部和整体旋转相关时间的差异,τ(lO)₂₉₈ = 190±15 ps和τ(gO)₂₉₈ = 930±50 ps,分别表明金属星并非完全刚性。然而,描述局部运动相对于整体运动限制的S₂ = 0.60±0.04的相对较高值表明,与之前报道的大分子如树枝状大分子相比,其灵活性有限。由于两个内球水分子具有接近最佳的交换速率以及有限的灵活性,金属星具有显著的摩尔质子弛豫率,特别是在高磁场下(在25℃时,60和200 MHz下的r1分别为33.2和16.4 mM⁻¹ s⁻¹)。它将六个有效弛豫的Gd(III)离子堆积到一个小分子空间中,据我们所知,这导致了Gd(III)配合物每分子质量的弛豫率是有史以来报道的最高值。[bpy(DTTA)₂]⁸⁻配体也是构建表面负载Gd(III)的更大尺寸的基于Fe(II)(或Ru(II))的金属星或金属树枝状大分子的末端配体的主要候选物。

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