<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"><channel><title>Space Digest</title><description>Space exploration and astronomy news aggregator — launches, missions, discoveries, and research, summarized and categorized by AI</description><link>https://space.pages.dev/</link><item><title>Stops Along the Path of Totality</title><link>https://space.pages.dev/item/622b8b758baacfa5/</link><guid isPermaLink="true">https://space.pages.dev/item/622b8b758baacfa5/</guid><description>NASA highlights the August 12, 2026 total solar eclipse, which will be visible from limited land areas in Iceland and Spain, with details on key viewing locations and cloud cover odds.</description><pubDate>Wed, 12 Aug 2026 04:01:00 GMT</pubDate><category>discovery_research</category><category>solar eclipse</category><category>Iceland</category><category>Spain</category><category>totality</category></item><item><title>Filling the Gap: Calibrating Gyrochronology at 1.3 Gyr with the Benchmark Cluster NGC-752</title><link>https://space.pages.dev/item/09e59690d52c2b6e/</link><guid isPermaLink="true">https://space.pages.dev/item/09e59690d52c2b6e/</guid><description>Researchers calibrate gyrochronology at the intermediate age of 1.3 Gyr using the cluster NGC-752, mapping its slow-rotator sequence for the first time. The new data show that existing gyrochronology models overestimate ages of many G and early-K dwarfs by 20–50%, providing a needed anchor for age estimates ahead of large-scale rotation surveys.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>gyrochronology</category><category>NGC-752</category><category>stellar rotation</category><category>benchmark clusters</category></item><item><title>A cosmic collision in the making: JWST/NIRISS reveals a merging and maturing protocluster core at z~3 around a red quasar</title><link>https://space.pages.dev/item/0c3f410b2de51998/</link><guid isPermaLink="true">https://space.pages.dev/item/0c3f410b2de51998/</guid><description>JWST/NIRISS has uncovered &apos;The Step&apos;, an extremely dense protocluster at z=3 surrounding a luminous quasar, with over 18 member galaxies and signs of an ongoing halo merger. Its exceptional density and mix of star-forming and quiescent galaxies make it a key system for studying how the most massive clusters form.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>JWST</category><category>protocluster</category><category>quasar</category><category>high redshift</category></item><item><title>Spiral Morphology and Radial Migration: Kinematically heating, cooling, and cold</title><link>https://space.pages.dev/item/0f9f5cc94c0cf31d/</link><guid isPermaLink="true">https://space.pages.dev/item/0f9f5cc94c0cf31d/</guid><description>A new study explores how the shape of spiral arms—their number, pitch angle, lifetime, and pattern speed—affects the radial migration of stars in disk galaxies. Using analytic models and tracer-particle simulations, it finds that the efficiency of &apos;cold torquing&apos; depends on spiral morphology in opposite ways for different spiral types, and that spirals also cause both kinematic heating and cooling.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>spiral arms</category><category>radial migration</category><category>galactic dynamics</category><category>corotation resonance</category></item><item><title>An Enriched Methane D/H Ratio in the Interstellar Object 3I/ATLAS</title><link>https://space.pages.dev/item/35517fcb6ee88356/</link><guid isPermaLink="true">https://space.pages.dev/item/35517fcb6ee88356/</guid><description>JWST observations of the interstellar object 3I/ATLAS reveal an unexpectedly high methane D/H ratio—the highest ever measured for methane in any object—providing a rare glimpse into volatile chemistry in another planetary system.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>interstellar object</category><category>James Webb Space Telescope</category><category>methane deuteration</category><category>3I/ATLAS</category></item><item><title>An X-ray Absorption-Line Survey of the Circumgalactic Medium of M31 with XMM-Newton</title><link>https://space.pages.dev/item/424f9ce8a2cfc396/</link><guid isPermaLink="true">https://space.pages.dev/item/424f9ce8a2cfc396/</guid><description>A new X-ray absorption-line survey of the hot circumgalactic medium around M31 finds a marginal excess absorption beyond the Milky Way foreground, hinting at hot gas associated with M31. The signal is only ~2.2–2.3σ and the inferred gas mass is highly model-dependent, so deeper observations are needed.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>circumgalactic medium</category><category>X-ray absorption spectroscopy</category><category>M31</category><category>XMM-Newton</category></item><item><title>Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics</title><link>https://space.pages.dev/item/432481c625aebb8c/</link><guid isPermaLink="true">https://space.pages.dev/item/432481c625aebb8c/</guid><description>Astronomers used VLBI observations and relativistic magneto-hydrodynamic simulations to trace the highest recorded polarized optical flare from BL Lacertae to helical, kink-like instabilities in its jet, with baryon loading required to match the observed jet structure.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>BL Lacertae</category><category>MHD simulations</category><category>VLBI</category><category>blazar jet</category></item><item><title>A Sulfur-Rich Atmosphere for the Young Jupiter Analog AF Lep b Reveals Significant Solid Accretion</title><link>https://space.pages.dev/item/5914bd270b210fa2/</link><guid isPermaLink="true">https://space.pages.dev/item/5914bd270b210fa2/</guid><description>JWST spectroscopy of the young Jupiter analog AF Lep b reveals a sulfur-rich atmosphere with significant metal enrichment (C/H=2.9x, O/H=3.7x, S/H=4.7x solar). The high sulfur abundance implies ~56 Earth masses of accreted solids during formation, and the enrichment pattern suggests gas-giant metal accretion may be similar across different orbital distances and planet masses.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>AF Lep b</category><category>JWST</category><category>exoplanet atmosphere</category><category>metal enrichment</category></item><item><title>JWST Spectroscopy of Type Ia Supernova 2025rbs from Maximum Light to the Nebular Phase</title><link>https://space.pages.dev/item/6c8bd51870f4ea0e/</link><guid isPermaLink="true">https://space.pages.dev/item/6c8bd51870f4ea0e/</guid><description>New JWST mid-infrared spectra of Type Ia supernova 2025rbs, taken from peak light into the nebular phase, reveal stratified ejecta with stable nickel at the core, radioactive cobalt at intermediate velocities, and argon in an outer shell. The observations include the first maximum-light MIR spectrum of a Type Ia supernova and earliest MIR spectroscopic sequence.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>JWST</category><category>Type Ia supernova</category><category>mid-infrared spectroscopy</category><category>2025rbs</category></item><item><title>Technology and Science Advancing Observations with Roman Coronagraph Informed by Ground-Based High-Contrast Imaging</title><link>https://space.pages.dev/item/712114a9dd2dc2ad/</link><guid isPermaLink="true">https://space.pages.dev/item/712114a9dd2dc2ad/</guid><description>A new study identifies promising targets for NASA&apos;s Roman Coronagraph technology demonstration, using ground-based survey data to select stars where the instrument can best test its ability to image and characterize faint companions. The study recommends adding spectroscopic observations of the superjovian planet HIP 99770 b to the planned demonstration.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>Roman Coronagraph</category><category>OASIS</category><category>Subaru Telescope</category><category>high-contrast imaging</category></item><item><title>Discovery of four Narrow-line Type-1 Quasars at z = 2.54 -- 6.06 with Subaru &apos;Onohi&apos;ula PFS-SSP</title><link>https://space.pages.dev/item/84252d3b979ea8e0/</link><guid isPermaLink="true">https://space.pages.dev/item/84252d3b979ea8e0/</guid><description>Astronomers report the discovery of four narrow-line type-1 quasars at redshifts 2.54–6.06 using the Subaru Prime Focus Spectrograph, pushing studies of this rare quasar population into the distant universe.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>quasars</category><category>Subaru</category><category>PFS-SSP</category><category>black holes</category></item><item><title>Explaining the X-ray Precursor, Ultra-long Prompt Emission, and Week-long Decay of GRB250702B with a Jetted Micro-TDE</title><link>https://space.pages.dev/item/874315304e738b4b/</link><guid isPermaLink="true">https://space.pages.dev/item/874315304e738b4b/</guid><description>This paper proposes that the longest-known gamma-ray burst, GRB250702B, was powered by a jetted micro-tidal disruption event (TDE), in which a stellar-mass black hole shredded a Sun-like star and launched a relativistic jet. Using simulations and analytic models, the authors reproduce the burst&apos;s three-phase emission, establishing micro-TDEs as a plausible engine for ultra-long GRBs.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>GRB250702B</category><category>tidal disruption event</category><category>ultra-long GRB</category><category>relativistic jet</category></item><item><title>Reconstructing Dark Matter Mass and Discriminating Standard and Non-Standard WIMP-Nucleus Interactions with Paleo-Detectors</title><link>https://space.pages.dev/item/869b589b8545d6a5/</link><guid isPermaLink="true">https://space.pages.dev/item/869b589b8545d6a5/</guid><description>A new modeling study shows that paleo-detectors—ancient minerals that record dark matter recoils over geological timescales—could reconstruct WIMP dark matter masses and distinguish between different dark matter-nucleus interaction types, with particular strength for low-mass WIMPs below 10 GeV.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>paleo-detectors</category><category>WIMP dark matter</category><category>NREFT</category><category>direct detection</category></item><item><title>Flat Galactic Rotation Curves Interpreted as Evidence for the Mach&apos;s Principle</title><link>https://space.pages.dev/item/939d08d566f8f406/</link><guid isPermaLink="true">https://space.pages.dev/item/939d08d566f8f406/</guid><description>A new arXiv paper proposes that flat galactic rotation curves—traditionally explained by dark matter or modified gravity—may instead be evidence for Mach&apos;s Principle. The authors recast the MOND acceleration scale and the Baryonic Tully-Fisher Relation in cosmological terms, and they argue that high-redshift observations favor a baryon-only, Λ-dominated universe over standard ΛCDM or MOND.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>Mach&apos;s Principle</category><category>galactic rotation curves</category><category>Tully-Fisher relation</category><category>MOND</category></item><item><title>Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy</title><link>https://space.pages.dev/item/96c2c7b8f1a7aa57/</link><guid isPermaLink="true">https://space.pages.dev/item/96c2c7b8f1a7aa57/</guid><description>A JWST/NIRSpec stacking analysis of 135 galaxies at redshifts 6–10 finds that nitrogen enhancement is a generic feature of early galaxies, not limited to extreme systems. The study yields supersolar N/O ratios while C/O remains subsolar, indicating significant nitrogen enhancement within the first billion years and pointing to standard enrichment processes.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>JWST</category><category>NIRSpec</category><category>high-redshift galaxies</category><category>chemical enrichment</category></item><item><title>SMA Observations Reveal Abundant HNC Chemistry in Transition Disks</title><link>https://space.pages.dev/item/a747d507b0ae0717/</link><guid isPermaLink="true">https://space.pages.dev/item/a747d507b0ae0717/</guid><description>New Submillimeter Array observations of five transition disks reveal unexpectedly bright HNC emission, with HNC-to-HCN ratios 3–10 times higher than model predictions for normal disks, suggesting cavities drive efficient HNC production and offering a new tracer of disk gas conditions.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>transition disks</category><category>HNC</category><category>Submillimeter Array</category><category>disk chemistry</category></item><item><title>From Cluster Core to Splashback: Linking Dynamical Structure to Multidimensional Galaxy Evolution in the Coma Cluster</title><link>https://space.pages.dev/item/d35a2fc5be54ce3e/</link><guid isPermaLink="true">https://space.pages.dev/item/d35a2fc5be54ce3e/</guid><description>A new study links galaxy evolution in the Coma cluster to its dynamical structure, finding that the splashback radius marks a critical transition where quiescent, bulge-dominated galaxies give way to star-forming, disk-dominated populations. Using a multidimensional classification, the authors show that galaxy transformation proceeds through continuous pathways rather than a simple binary process.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>Coma cluster</category><category>galaxy evolution</category><category>splashback radius</category><category>SDSS</category></item><item><title>Lyman Break Galaxy selection and redshift measurement with supervised contrastive learning</title><link>https://space.pages.dev/item/d86bc3cfd833408e/</link><guid isPermaLink="true">https://space.pages.dev/item/d86bc3cfd833408e/</guid><description>A new machine-learning method using supervised contrastive learning improves Lyman Break Galaxy selection and redshift measurement for DESI Run 2, outperforming the previous network on outlier classification while matching redshift accuracy.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>Lyman Break Galaxies</category><category>contrastive learning</category><category>DESI</category><category>redshift measurement</category></item><item><title>3D Binary Neutron Star Merger Ejecta Evolution up to Seconds Timescale: Dynamics, Element Distribution, and Light Curves</title><link>https://space.pages.dev/item/bffa67cf674d3656/</link><guid isPermaLink="true">https://space.pages.dev/item/bffa67cf674d3656/</guid><description>Long-term 3D simulations of binary neutron star merger ejecta show that nuclear heating delays homologous expansion and reshapes heavy-element distribution, and that 2D kilonova light curves are broadly robust but only upper limits, with increased dimensionality unlikely to reconcile models with AT2017gfo.</description><pubDate>Wed, 12 Aug 2026 04:00:00 GMT</pubDate><category>discovery_research</category><category>binary neutron star mergers</category><category>kilonova</category><category>nucleosynthesis</category><category>numerical relativity</category></item><item><title>What Is the Nancy Grace Roman Space Telescope? (Grades 5-8)</title><link>https://space.pages.dev/item/6755a9c9607b3906/</link><guid isPermaLink="true">https://space.pages.dev/item/6755a9c9607b3906/</guid><description>This educational article from NASA explains the upcoming Nancy Grace Roman Space Telescope, a new astrophysics observatory designed to study dark energy, dark matter, and exoplanets. It covers the mission&apos;s launch details, orbit at Lagrange Point 2, and its two science instruments.</description><pubDate>Tue, 11 Aug 2026 21:04:39 GMT</pubDate><category>launch_mission</category><category>Nancy Grace Roman Space Telescope</category><category>dark energy</category><category>exoplanets</category><category>infrared astronomy</category></item><item><title>NASA Completes Astronaut-Deployed Science Instrument for Lunar Surface</title><link>https://space.pages.dev/item/d55fb0d9684a7184/</link><guid isPermaLink="true">https://space.pages.dev/item/d55fb0d9684a7184/</guid><description>NASA has completed the Lunar Environment Monitoring Station (LEMS), the first science payload designed for Artemis astronauts to deploy on the Moon. The instrument uses highly sensitive seismometers to study moonquakes and lunar interior structure, supporting sustained lunar exploration and future astronaut safety.</description><pubDate>Tue, 11 Aug 2026 19:41:34 GMT</pubDate><category>exploration_program</category><category>LEMS</category><category>Artemis</category><category>lunar seismology</category><category>NASA Goddard</category></item><item><title>Lion Nebula Roars in Webb’s Sights</title><link>https://space.pages.dev/item/1338e455948d7408/</link><guid isPermaLink="true">https://space.pages.dev/item/1338e455948d7408/</guid><description>NASA&apos;s James Webb Space Telescope captured new high-resolution images of the Lion Nebula (NGC 2392), revealing its &apos;mane&apos; of ionized gas and dust in striking detail. The observations showcase Webb&apos;s powerful infrared imaging capabilities for studying planetary nebulae.</description><pubDate>Tue, 11 Aug 2026 17:02:49 GMT</pubDate><category>discovery_research</category><category>James Webb Space Telescope</category><category>Lion Nebula</category><category>NGC 2392</category><category>planetary nebula</category></item><item><title>NASA Telescopes Create Colorful ‘Craft’ From Nearby Nebula</title><link>https://space.pages.dev/item/0c51e2835359480d/</link><guid isPermaLink="true">https://space.pages.dev/item/0c51e2835359480d/</guid><description>NASA telescopes combined X-ray, infrared, and optical observations to create a new composite view of the Tarantula Nebula, revealing that the star-forming region emits far less X-ray gas than expected. The finding suggests much of the energy from massive star winds may be leaking away or dissipating through mixing.</description><pubDate>Tue, 11 Aug 2026 15:19:15 GMT</pubDate><category>discovery_research</category><category>Tarantula Nebula</category><category>Chandra X-ray Observatory</category><category>James Webb Space Telescope</category><category>star formation</category></item><item><title>Building the Moon Base: NASA Stories at the Ion</title><link>https://space.pages.dev/item/40ee85b32c4451c4/</link><guid isPermaLink="true">https://space.pages.dev/item/40ee85b32c4451c4/</guid><description>NASA&apos;s Moon Base Program principal systems engineer Shatel Bhakta discussed the challenges and opportunities of building a sustainable lunar base at the South Pole during a NASA Stories at the Ion event. The talk covered the step-by-step development approach, including robotic missions, and key challenges like terrain, lighting, communications, and Moon dust.</description><pubDate>Tue, 11 Aug 2026 14:16:45 GMT</pubDate><category>exploration_program</category><category>Moon Base</category><category>lunar South Pole</category><category>NASA</category><category>Ion</category></item><item><title>A total solar eclipse is coming to Europe</title><link>https://space.pages.dev/item/180d8326e7fa0722/</link><guid isPermaLink="true">https://space.pages.dev/item/180d8326e7fa0722/</guid><description>A total solar eclipse will cross parts of Greenland, Iceland, Portugal, and Spain on August 12, marking the first such eclipse visible from mainland Spain since 1905. The European Space Agency will host a live broadcast and free in-person events to let people worldwide experience the rare phenomenon.</description><pubDate>Tue, 11 Aug 2026 12:30:00 GMT</pubDate><category>other</category><category>solar eclipse</category><category>ESA</category><category>Spain</category><category>live broadcast</category></item><item><title>Sophie Adenot’s first spacewalk</title><link>https://space.pages.dev/item/64e2221ef2307182/</link><guid isPermaLink="true">https://space.pages.dev/item/64e2221ef2307182/</guid><description>ESA astronaut Sophie Adenot will perform her first-ever spacewalk during U.S. Spacewalk 97, joined by NASA astronaut Anil Menon to replace a critical Space-to-Ground antenna on the ISS. Live coverage starts at 13:00 CEST on ESA WebTV and YouTube, with the EVA scheduled to begin around 14:35 CEST.</description><pubDate>Tue, 11 Aug 2026 08:00:00 GMT</pubDate><category>exploration_program</category><category>spacewalk</category><category>ISS</category><category>ESA</category><category>Sophie Adenot</category></item><item><title>Dust and water spotted close to giant black hole</title><link>https://space.pages.dev/item/cbf5fed7cbf69492/</link><guid isPermaLink="true">https://space.pages.dev/item/cbf5fed7cbf69492/</guid><description>Using the James Webb Space Telescope, astronomers discovered that dust and water can form and survive surprisingly close to the supermassive black hole at the Milky Way&apos;s center, thanks to observations of the evolved star IRS 3.</description><pubDate>Tue, 11 Aug 2026 08:00:00 GMT</pubDate><category>discovery_research</category><category>James Webb Space Telescope</category><category>supermassive black hole</category><category>IRS 3</category><category>dust formation</category></item><item><title>Curiosity Blog, Sols 4968-4974: Rock Climbing Towards the Discontinuity</title><link>https://space.pages.dev/item/644309c0cec8c986/</link><guid isPermaLink="true">https://space.pages.dev/item/644309c0cec8c986/</guid><description>NASA&apos;s Curiosity rover spent Sols 4968-4974 investigating a suspected &apos;erosional supersurface&apos; in Gale Crater, climbing onto the Cerro Paine Grande outcrop to image and analyze rock layers above and below the discontinuity. The rover reached a 24-degree tilt—near its contact-science record—and gathered data with Mastcam, MAHLI, APXS, and ChemCam.</description><pubDate>Tue, 11 Aug 2026 06:50:07 GMT</pubDate><category>exploration_program</category><category>Curiosity</category><category>Mars Science Laboratory</category><category>Gale Crater</category><category>erosional supersurface</category></item><item><title>APOD: 2026 August 11 – Six Moons of Saturn</title><link>https://space.pages.dev/item/89bd74943186ef9d/</link><guid isPermaLink="true">https://space.pages.dev/item/89bd74943186ef9d/</guid><description>The August 11, 2026 Astronomy Picture of the Day shows six of Saturn&apos;s largest moons in a single telescopic portrait, highlighting Titan&apos;s size and the planet&apos;s record 293 confirmed moons.</description><pubDate>Tue, 11 Aug 2026 04:05:00 GMT</pubDate><category>discovery_research</category><category>Saturn</category><category>moons</category><category>Titan</category><category>solar system</category></item><item><title>Bountiful Roebuck Bay</title><link>https://space.pages.dev/item/c78797e793d42c46/</link><guid isPermaLink="true">https://space.pages.dev/item/c78797e793d42c46/</guid><description>NASA&apos;s Earth Observatory spotlights Roebuck Bay in Western Australia, where tides of up to 9 meters shape vast mudflats, mangroves, and tidal creeks. The bay teems with marine life and attracts birds, while Landsat data reveal mangroves expanding westward as sediment accumulates.</description><pubDate>Tue, 11 Aug 2026 04:01:00 GMT</pubDate><category>other</category><category>Roebuck Bay</category><category>tides</category><category>mangroves</category><category>NASA Earth Observatory</category></item><item><title>Lion Nebula roars to life for Webb</title><link>https://space.pages.dev/item/8dd8712f7deec915/</link><guid isPermaLink="true">https://space.pages.dev/item/8dd8712f7deec915/</guid><description>The James Webb Space Telescope has captured new infrared images of the planetary nebula NGC 2392, the Lion Nebula, revealing details sharper than Hubble&apos;s earlier visible-light view. The images highlight dust clumps and ionized gas structures powered by a central white dwarf, offering a clearer look at this evolving nebula.</description><pubDate>Mon, 10 Aug 2026 14:00:00 GMT</pubDate><category>discovery_research</category><category>James Webb Space Telescope</category><category>NGC 2392</category><category>planetary nebula</category><category>infrared astronomy</category></item><item><title>Wildfires, drought and extreme heat, 2026</title><link>https://space.pages.dev/item/8b8551232d063c1d/</link><guid isPermaLink="true">https://space.pages.dev/item/8b8551232d063c1d/</guid><description>ESA highlights how Earth observation satellites are tracking wildfires, drought, and extreme heat in 2026, reporting exceptional June temperatures and over 30 Copernicus Emergency Management Service activations for fires across Europe and beyond.</description><pubDate>Mon, 10 Aug 2026 13:00:00 GMT</pubDate><category>discovery_research</category><category>Earth observation</category><category>wildfires</category><category>Copernicus</category><category>climate change</category></item><item><title>NASA figured out how to keep its Voyager 2 probe running for another year</title><link>https://space.pages.dev/item/3aa7e99d23550e64/</link><guid isPermaLink="true">https://space.pages.dev/item/3aa7e99d23550e64/</guid><description>NASA has adjusted Voyager 2&apos;s power usage to keep its three remaining science instruments running for at least another year. The move, prompted by dwindling nuclear battery power, involves shutting off non-essential systems and using lower-power alternatives.</description><pubDate>Sat, 08 Aug 2026 01:49:11 GMT</pubDate><category>launch_mission</category><category>Voyager 2</category><category>NASA</category><category>interstellar probe</category><category>power management</category></item><item><title>Water system controllers don&apos;t belong on the internet, says ex-NSA chief</title><link>https://space.pages.dev/item/276c8ef8fa869440/</link><guid isPermaLink="true">https://space.pages.dev/item/276c8ef8fa869440/</guid><description>Retired Gen. Paul Nakasone says US water system controllers should not be internet-connected, citing recent attacks on water facilities across 12 states likely by Iran. He calls for higher security standards and public-private partnerships, including volunteer efforts like DEF CON Franklin.</description><pubDate>Fri, 07 Aug 2026 21:19:57 GMT</pubDate><category>other</category><category>cybersecurity</category><category>water infrastructure</category><category>PLC</category><category>Paul Nakasone</category></item><item><title>Danube’s waters fall to record lows</title><link>https://space.pages.dev/item/a6f36a487375131b/</link><guid isPermaLink="true">https://space.pages.dev/item/a6f36a487375131b/</guid><description>New Copernicus Sentinel-2 images show the Danube River at a record low near Budapest, Hungary, after a severe drought in central Europe. The shrinking river has caused energy and water shortages, disrupted river traffic, and threatened wildlife.</description><pubDate>Fri, 07 Aug 2026 11:40:00 GMT</pubDate><category>other</category><category>Copernicus</category><category>Sentinel-2</category><category>drought</category><category>Danube</category></item><item><title>Nashville uses eminent domain to block data center near zoo</title><link>https://space.pages.dev/item/759f183f7f216e02/</link><guid isPermaLink="true">https://space.pages.dev/item/759f183f7f216e02/</guid><description>Nashville&apos;s Metro Council voted 27-5 to use eminent domain to potentially acquire land near the zoo where DC Blox plans a data center, citing office space shortages. The move faces zoning appeals, potential legal fights, and cost concerns, with the property valued at $37M but recently sold for $23M.</description><pubDate>Thu, 06 Aug 2026 16:12:24 GMT</pubDate><category>other</category><category>eminent domain</category><category>Nashville</category><category>data center</category><category>DC Blox</category></item><item><title>Total solar eclipse: how to watch live from home</title><link>https://space.pages.dev/item/7d92603cf2986fc0/</link><guid isPermaLink="true">https://space.pages.dev/item/7d92603cf2986fc0/</guid><description>ESA will livestream the 12 August 2026 total solar eclipse as it crosses Europe, featuring expert commentary, telescope views, and a rare glimpse of the Sun&apos;s corona. The broadcast makes the event accessible to viewers worldwide, even those outside the path of totality.</description><pubDate>Wed, 05 Aug 2026 08:00:00 GMT</pubDate><category>other</category><category>total solar eclipse</category><category>ESA</category><category>livestream</category><category>Javalambre</category></item></channel></rss>