Easily identified by the spectacular band of dark dust that partially obscures its bright core, Messier 64, or the Black Eye Galaxy, is characterized by its bizarre internal motion.NASA, CSA, ESA, F. Belfiore (European Southern Observatory – Germany), J. Lee (Space Telescope Science Institute), A. Leroy (The Ohio State University), and D. Thilker (The Johns Hopkins University); Processing: Gladys Kober (NASA/Catholic University of America)
Messier 64，即黑洞星系，因其部分遮蔽明亮核心的壮观暗尘带而易于辨认，其内部运动特征极为奇特。NASA、CSA、ESA、F. Belfiore（欧洲南方天文台—德国）、J. Lee（太空望远镜科学研究所）、A. Leroy（俄亥俄州立大学）和 D. Thilker（约翰斯·霍普金斯大学）；图像处理：Gladys Kober（NASA/天主教美国大学）
This March 20, 2026, image of Messier 64, or the Black Eye Galaxy, is a composite view from NASA’s Hubble Space Telescope and James Webb Space Telescope. It shows Messier 64 captured at near- and mid-infrared wavelengths by Webb, while Hubble’s image shows the galaxy in ultraviolet, visible, and near-infrared light.
这张拍摄于2026年3月20日的Messier 64（黑洞星系）图像，是由NASA哈勃空间望远镜与詹姆斯·韦伯空间望远镜合成的复合视图。其中，韦伯望远镜以近红外和中红外波段捕捉了该星系，而哈勃望远镜则展示了其在紫外、可见光及近红外波段的光谱。
NASA · Public Domain