"Not to be: Universe too short for Shakespeare's typing monkeys." Views expressed in this science and technology update are those of the reporters and correspondents. Accessed on 30 October 2024, 1953 UTC. Content and Source: https://scienceblog.com/newsletter. Please check link or scroll down to read your selections. Thanks for joining us today. Russ Roberts (https://hawaiisciencejournal.blogspot.com). Forwarded this email? Subscribe here for more Not to be: Universe too short for Shakespeare's typing monkeys Oct 30 READ IN APP Read: Universe too short for Shakespeare typing monkeys The surprising reason a classical computer beat a quantum computer at its own game Boozing animals may not be as rare as we thought New Screening System Fast-Tracks Treatments for Alzheimer’s, Parkinson’s AI might scare us, but can we scare it? Giant rats sniff out illegal ivory trade Researchers Get Leg Up on Bone Repair with 3D-Printed Femur New app...
![Hubble and Webb Observations of Vega Circumstellar Debris Disk. [left]-A Hubble Space Telescope false-color view of a 100-billion-mile-wide disk of dust around the summer star Vega. Hubble detects reflected light from dust that is the size of smoke particles largely in a halo on the periphery of the disk. The disk is very smooth, with no evidence of embedded large planets. The black spot at the center blocks out the bright glow of the hot young star. [right]-The James Webb Space Telescope resolves the glow of warm dust in a disk halo, at 23 billion miles out. The outer disk (analogous to the solar system’s Kuiper Belt) extends from 7 billion miles to 15 billion miles. The inner disk extends from the inner edge of the outer disk down to close proximity to the star. There is a notable dip in surface brightness of the inner disk from approximately 3.7 to 7.2 billion miles. The black spot at the center is due to lack of data from saturation.](https://blogger.googleusercontent.com/img/proxy/AVvXsEhEDUvNPSq-KIYknX0wwZRbdIaAGfWIOvtT7-zlqH2R29Mn_s0wmCgrjIc03o_CJG_usAeRYIxYbmHmmFHCmUD4eZPQmw5ErlVwC15EE32HeJMIAsC4ZpHVR88rHv65gf-jLm_gvpyp4XgehJI6PL0V0uC6V6D06KwEg4u4tMv958irVjt4KJ_BLmH-VMH4-nSCY7pmdtYjJ9Q7kUGi5zMRBMx3OZMi4FDhBXHnXtcOg7AavRrI7C8yGAqQ77de1Bae2978k6QK0Ncu-sfw2Mf8O7HnshdJq-wT0Ut5FfdhK9bBeW7jY0WQP4iPzCcM8pBiKXy5QpOFfZFCHKcFssuFS5ZUECx1kmJxC_N3gN2G527-TA=s0-d-e1-ft,c_limit,f_auto,q_auto:good,fl_progressive:steep/https%3A%2F%2Fsubstack-post-media.s3.amazonaws.com%2Fpublic%2Fimages%2Fd378982a-92f6-4002-88cc-f4fb9805febe_300x200.jpeg "Hubble and Webb Observations of Vega Circumstellar Debris Disk. [left]-A Hubble Space Telescope false-color view of a 100-billion-mile-wide disk of dust around the summer star Vega. Hubble detects reflected light from dust that is the size of smoke particles largely in a halo on the periphery of the disk. The disk is very smooth, with no evidence of embedded large planets. The black spot at the center blocks out the bright glow of the hot young star. [right]-The James Webb Space Telescope resolves the glow of warm dust in a disk halo, at 23 billion miles out. The outer disk (analogous to the solar system’s Kuiper Belt) extends from 7 billion miles to 15 billion miles. The inner disk extends from the inner edge of the outer disk down to close proximity to the star. There is a notable dip in surface brightness of the inner disk from approximately 3.7 to 7.2 billion miles. The black spot at the center is due to lack of data from saturation.")
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