Jones-Emberson 1
2023-02-24
浏览次数: 15
行星状星云琼斯-艾伯森1号是一颗垂死的类太阳恒星的死亡裹尸布。它位于距离地球1600光年的山猫星座。大约4光年宽,这颗垂死的恒星的大气层的残余正在膨胀,被甩到星际空间中,因为这颗恒星用于聚变的氢和氦的中心供应在数十亿年后终于耗尽了。在行星状星云的中心附近可以看到恒星核心的残骸,一颗蓝热的白矮星。这个星云也被称为PK 164 +31.1,它很暗,很难用望远镜的目镜瞥见。但这张包含22小时曝光时间的深度宽带图像确实以非凡的细节展示了它。我们银河系内的恒星以及宇宙中的背景星系分散在清晰的视野中。琼斯-艾伯森1号在宇宙舞台上转瞬即逝,将在未来几千年逐渐消失。它炽热的中央白矮星需要数十亿年才能冷却下来。
查看原文解释
Planetary nebula Jones-Emberson 1 is the death shroud of a dying Sun-like star. It lies some 1,600 light-years from Earth toward the sharp-eyed constellation Lynx. About 4 light-years across, the expanding remnant of the dying star's atmosphere was shrugged off into interstellar space, as the star's central supply of hydrogen and then helium for fusion was finally depleted after billions of years. Visible near the center of the planetary nebula is what remains of the stellar core, a blue-hot white dwarf star. Also known as PK 164 +31.1, the nebula is faint and very difficult to glimpse at a telescope's eyepiece. But this deep broadband image combining 22 hours of exposure time does show it off in exceptional detail. Stars within our own Milky Way galaxy as well as background galaxies across the universe are scattered through the clear field of view. Ephemeral on the cosmic stage, Jones-Emberson 1 will fade away over the next few thousand years. Its hot, central white dwarf star will take billions of years to cool.
© Serge Brunier, Jean-François Bax, David Vernet