Sharp-tailed Grouse
A Lunar Corona with Jupiter and Saturn : Why does a cloudy moon sometimes appear colorful? The effect, called a lunar corona, is created by the quantum mechanical diffraction of light around individual, similarly-sized water droplets in an intervening but mostly-transparent cloud. Since light of different colors has different wavelengths, each color diffracts differently. Lunar Coronae are one of the few quantum mechanical color effects that can be easily seen with the unaided eye. Solar coronae are also sometimes evident. The featured composite image was captured a few days before the close Great Conjunction between Saturn and Jupiter last month. In the foreground, the Italian village of Pieve di Cadore is visible in front of the Sfornioi Mountains. via NASA
( <= green bean
Falsetober 29 - 31 (The end) Thanks so much for reading everyone! ❤️ You can preorder the whole story as a physical booklet here. There’s also prints and original artwork from the whole month available!
on graduation & parting ways
Night of the Woods: Chapter 3 / unknown / When We Were Young - Adele / We May Never Pass This Way (Again) - Seals and Crofts / Mikko Harvey, for M / John Berger, “Will it be a likeness?” from The Shape of a Pocket / forever - Charli XCX / Lemony Snicket, The Beatrice Letters / nice2KnoU - All Time Low / @alisonzai
the colors of winter
Two more weeks of gender!
imagine someone thinking of you and buying you flowers
Inktober 2021 by Gregory Fromenteau
Recycling Cassiopeia A : Massive stars in our Milky Way Galaxy live spectacular lives. Collapsing from vast cosmic clouds, their nuclear furnaces ignite and create heavy elements in their cores. After a few million years, the enriched material is blasted back into interstellar space where star formation can begin anew. The expanding debris cloud known as Cassiopeia A is an example of this final phase of the stellar life cycle. Light from the explosion which created this supernova remnant would have been first seen in planet Earth’s sky about 350 years ago, although it took that light about 11,000 years to reach us. This false-color image, composed of X-ray and optical image data from the Chandra X-ray Observatory and Hubble Space Telescope, shows the still hot filaments and knots in the remnant. It spans about 30 light-years at the estimated distance of Cassiopeia A. High-energy X-ray emission from specific elements has been color coded, silicon in red, sulfur in yellow, calcium in green and iron in purple, to help astronomers explore the recycling of our galaxy’s star stuff. Still expanding, the outer blast wave is seen in blue hues. The bright speck near the center is a neutron star, the incredibly dense, collapsed remains of the massive stellar core. via NASA