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星形胶质细胞对乙酸盐的优先利用归因于转运。

Preferential utilization of acetate by astrocytes is attributable to transport.

作者信息

Waniewski R A, Martin D L

机构信息

Wadsworth Center, New York State Department of Health, Albany, New York 12201-0509, USA.

出版信息

J Neurosci. 1998 Jul 15;18(14):5225-33. doi: 10.1523/JNEUROSCI.18-14-05225.1998.

Abstract

Exogenous acetate is preferentially metabolized by astrocytes in the CNS, but the biochemical basis for this selectivity is unknown. We observed that rat cortical astrocytes produce 14CO2 from 0.2 mM [14C]acetate at a rate of 0.43 nmol/min per milligram of protein, 18 times faster than cortical synaptosomes. Subsequent studies examined whether this was attributable to cellular differences in the transport or metabolism of acetate. The activity of acetyl-CoA synthetase, the first enzymatic step in acetate utilization, was greater in synaptosomes than in astrocytes (5.0 and 2.9 nmol/min per milligram of protein), indicating that slower metabolism in synaptosomes cannot be attributed to lack of enzymatic activity. [14C]Acetate uptake in astrocytes is rapid and time-dependent and follows saturation kinetics (Vmax, 498 nmol/min per milligram of protein; Km, 9.3 mM). Uptake is inhibited stereospecifically by L-lactate as well as by pyruvate, fluoroacetate, propionate, and alpha-cyano-4-hydroxycinnamate (CHC). Preloading astrocytes with L-lactate or acetate, but not D-lactate, pyruvate, or glyoxylate, transaccelerates [14C]acetate uptake. Acetate uptake by astrocytes appears to be mediated by a carrier with properties similar to that of monocarboxylate transport. In contrast, studies with synaptosomes provided no evidence for time-dependent, saturable, transaccelerated, or CHC-inhibitable uptake of [14C]acetate. The high rate of transport in astrocytes compared with synaptosomes explains the rapid incorporation of [14C]acetate into brain glutamine over glutamate. These findings provide support for the use of acetate as a marker for glial metabolism and suggest that extracellular acetate in the brain generated from acetylcholine and ethanol metabolism is accumulated first by astrocytes.

摘要

外源性乙酸盐在中枢神经系统中优先被星形胶质细胞代谢,但这种选择性的生化基础尚不清楚。我们观察到,大鼠皮质星形胶质细胞以0.43 nmol/分钟每毫克蛋白质的速率从0.2 mM [14C]乙酸盐产生14CO2,比皮质突触体快18倍。随后的研究检查了这是否归因于乙酸盐转运或代谢的细胞差异。乙酰辅酶A合成酶是乙酸盐利用的第一步酶促反应,其活性在突触体中比在星形胶质细胞中更高(5.0和2.9 nmol/分钟每毫克蛋白质),这表明突触体中代谢较慢不能归因于酶活性的缺乏。星形胶质细胞对[14C]乙酸盐的摄取迅速且具有时间依赖性,并遵循饱和动力学(Vmax,498 nmol/分钟每毫克蛋白质;Km,9.3 mM)。摄取受到L-乳酸以及丙酮酸、氟乙酸盐、丙酸盐和α-氰基-4-羟基肉桂酸酯(CHC)的立体特异性抑制。用L-乳酸或乙酸盐预加载星形胶质细胞,但不是D-乳酸、丙酮酸或乙醛酸,可以加速[14C]乙酸盐的摄取。星形胶质细胞对乙酸盐的摄取似乎是由一种具有与单羧酸转运相似性质的载体介导的。相比之下,对突触体的研究没有提供[14C]乙酸盐的时间依赖性、可饱和、加速或CHC抑制性摄取的证据。与突触体相比,星形胶质细胞中乙酸盐的高转运速率解释了[14C]乙酸盐优先快速掺入脑谷氨酰胺而非谷氨酸中。这些发现支持将乙酸盐用作胶质细胞代谢的标志物,并表明由乙酰胆碱和乙醇代谢产生的脑内细胞外乙酸盐首先被星形胶质细胞积累。

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