The sharp Hubble data also reveal more distant background galaxies seen right through NGC 2442's star clusters and nebulae.
敏锐的哈勃数据还暴露了更多遥远的背景星系，右边透过NGC 2442的星团和星云可见。
The many energetic star-forming regions along NGC 300's spiral arms are visible in the picture as red and pink clouds.
我们可以看到许多位于NGC 300星系的螺旋腕上的高能量恒星在图片里呈现红色、粉红色。
The debris trail that joins them, along with NGC 5218's comma-shaped extension and the distorted arms of NGC 5216, are a consequence of mutual gravitational tides.
连接它们的余迹，沿着NGC 5218逗号形状延伸至NGC 5216扭曲的旋臂，是引潮力互相作用的结果。
Broader than the disk, NGC 660's ring spans about 40, 000 light-years.
NGC 660的环比盘更为宽广，直径大约为40000光年。
NGC 770's fuzzy, elliptical appearance contrasts nicely with a spiky foreground Milky Way star in matching yellowish hues.
NGC 770朦胧的椭圆形状与前景中银河系黄色恒星的芒角状形成了显明对比。
NGC 770's fuzzy, elliptical appearance contrasts nicely with a spiky foreground Milky Way star in matching yellowish hues.
NGC 770朦胧的椭圆形状与前景中银河系黄色恒星的芒角状形成了显明对比。
应用推荐