The spooky image reveals part of a star-forming area called the Serpens Nebula, which stays in the tail of the Snake constellation. It’s house to a young star called HCD 672, which has a thick protoplanetary disk of gas and dust around it.
Now here’s where the Bat Shadow is available in. The star’s particles ring is too little and far-off to be seen by Hubble, however the disk casts beast shadows onto the nebula. The 2 cone-like shadows in the upper right of the image are referred to as the Bat Shadow thanks to the wing-like look. It’s as close as we’ll get to seeing a Bat-Signal amongst the stars.
” This is an analog of what the planetary system appeared like when it was just 1 or 2 million years of ages,” stated Klaus Pontoppidan, an Area Telescope Science Institute (STScI) astronomer. “For all we understand, the planetary system as soon as produced a shadow like this.”