A Poem to Music. The arrow of time, both ruthless and kind, I stroll through the park, a peaceful mind. As raindrops fall and thunderstorms break, Life's beauty unfolds, a sweet, gentle ache. Every breath is a gift, each step, a tale, Time's arrow propelling, a relentless trail. The past stands behind, yet resides in our core, The future unknown, forever more. With each step, chase your dreams and delight, March on with courage, even in the night. Let rain wash away all your darkest doubts, The arrow of time cares not what life's about. Peace and love in each stride do dwell, Share your hope, let compassion swell. Take heed of my words, both cruel and nice, The arrow of time, in its ceaseless device. ... https://www.youtube.com/watch?v=PkfiWmgtG8M

In this mosaic image stretching 340 light-years across, Webb’s Near-Infrared Camera (NIRCam) displays the Tarantula Nebula star-forming region in a new light, including tens of thousands of never-before-seen young stars that were previously shrouded in cosmic dust. The most active region appears to sparkle with massive young stars, appearing pale blue. Scattered among them are still-embedded stars, appearing red, yet to emerge from the dusty cocoon of the nebula. NIRCam is able to detect these dust-enshrouded stars thanks to its unprecedented resolution at near-infrared wavelengths. To the upper left of the cluster of young stars, and the top of the nebula’s cavity, an older star prominently displays NIRCam’s distinctive eight diffraction spikes, an artifact of the telescope’s structure. Following the top central spike of this star upward, it almost points to a distinctive bubble in the cloud. Young stars still surrounded by dusty material are blowing this bubble, beginning to carve out their own cavity. Astronomers used two of Webb’s spectrographs to take a closer look at this region and determine the chemical makeup of the star and its surrounding gas. This spectral information will tell astronomers about the age of the nebula and how many generations of star birth it has seen. Farther from the core region of hot young stars, cooler gas takes on a rust color, telling astronomers that the nebula is rich with complex hydrocarbons. This dense gas is the material that will form future stars. As winds from the massive stars sweep away gas and dust, some of it will pile up and, with gravity’s help, form new stars. Credit: NASA, ESA, CSA, STScI, Webb ERO Production Team Processed by STYX AI #science #nature #ai #machinelearning #nasa #photography #4k ... https://www.youtube.com/watch?v=iW9a3K6idOo