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"The nebula appears to have distinct regions that capture different phases of its evolution — an outer shell of gas that was blown off first and consists mostly of hydrogen, and an inner cloud with more structure that contains a mix of different gases," NASA's blog post reads. The dark line that runs vertically through the nebula, giving it the cranial appearance, could be the result of "an outburst or outflow from the central star, which typically occurs as twin jets burst out in opposite directions." Both Webb's Near-Infrared Camera (NIRCam) and its Mid-Infrared Instrument (MIRI) were used to document the nebula.，推荐阅读爱思助手下载最新版本获取更多信息
主屏幕编辑菜单的液态玻璃透明度进一步提升，玻璃质感更明显，但在部分背景下会导致文字与图标的对比度下降，导致可读性变差；深色模式下的控制中心弹窗背景也同步变得更暗。。一键获取谷歌浏览器下载对此有专业解读