Cosmic Dust Clouds and Nebulae in the Cepheus Flare

According to NASA News Releases, the image displays cosmic dust clouds that are visible through dimly reflected starlight, appearing as spooky shapes within the dusty expanse of the royal constellation Cepheus. These formations are situated beyond the plane of the Milky Way, at the boundary of the Cepheus Flare molecular cloud complex, which is approximately 1,200 light-years away, as of October 30, 2026. The Ghost Nebula, which has alternative names such as vdB 141 or Sh2-136, spans over 2 light-years and is noted for containing reddish indicators of dense cores undergoing early star formation. This nebula is positioned in the lower right of the visible star field. To the left of the center in the image, the Iris Nebula is visible, reflecting bluish light originating from the hot young stars of NGC 7023, which contrasts against the darkness. The wide telescopic view captures these fertile interstellar dust fields covering an area equivalent to almost six full moons across the sky.