Astrophyzix Digital Observatory
Asteroid News, Research & Analysis

Astrophyzix.com is the publication of the Astrophyzix Digital Observatory, offering unpaywalled, evidence‑driven analysis and real‑time monitoring of PHAs and NEOs. Our tracking consoles and reporting systems use and provide access to official NASA CNEOS Scout, JPL CAD, NeoWs, JPL SBDB, Horizons and NOAA observational datasets, peer‑reviewed sources, and high‑precision numerical methods (IEEE‑754 Float64, RKN4). Designed for students, educators, researchers, and the public, every console is uniquely designed and engineered by the Astrophyzix Digital Observatory. Our research notes and papers can be found at Astrophyzix.Academia.Edu

Showing posts with label Evidence-First. Show all posts
Showing posts with label Evidence-First. Show all posts

Thursday, 11 June 2026

NEO PHA Asteroid Close Approach Report for 11 June 2026 NASA NeoWs Data Analysis by Astrophyzix Digital Observatory

 ASTROPHYZIX // PLANETARY DEFENSE DESK

Image description
CLOSE APPROACH Bulletin · NASA NeoWs API

Daily Near-Earth Object Close-Approach Report: June 11, 2026

Near-Earth object encounters catalogued across a 7-day window, reported on the UTC civil time scale.

On June 11, 2026 (UTC), daily screening of the NASA NeoWs catalogue resolves 39 near-Earth object close approaches across the report window. The single closest encounter is 2003 LN6, passing at approximately 3.68 lunar distances (1,417,040 km) with a relative velocity near 3.9 km/s. Its order-of-magnitude kinetic energy, for scale only, is near 0 Mt TNT equivalent; Astrophyzix can confirm that no listed object is on an impacting trajectory. There is currently no known impact threat reported. 

To view the very latest, most comprehensive JPL CAD and CNEOS Scout Data in real time please use the Astrophyzix Dual-watch Asteroid Monitoring system

CLOSEST APPROACH IN Window (TRACK LIVE
2003 LN6
3.68 LD
1,417,040 km · 0.009472 au · v_rel 3.92 km/s
EARTH SURFACE19.5 LD (FILTER EDGE)
Encounter (UTC)
2026-Jun-18 20:54
Est. diameter
0.045 km (NeoWs)
Diameter range
0.030 - 0.068 km
Earth radii
222 R(E)

Tuesday, 2 June 2026

How Astrophyzix Digital Observatory Maintains Professional Standards in NEO and PHA Monitoring and How Orbital Refinement Calculations are Performed.

Astrophyzix Technical Transparency Report · Computational Methods & NASA Integration



Image description Float64 · IEEE‑754 · Yoshida‑4 · Runge–Kutta · Dormand–Prince · N‑Body · WebGPU · VSOP87 · NASA APIs
✨ A detailed public outreach explainer in response to user questions about how Astrophyzix computes, refines, and visualises orbits of planets, potentially hazardous asteroids (PHA'S), comets and Near-Earth Objects (NEO's) 

Float64 Precision IEEE‑754 Standard N‑Body Physics WebGPU Compute

High‑Order Integrators NASA API Integration

Introduction

This article is written in response to recent questions from Astrophyzix users asking how our orbital‑refinement system works, what computational methods we use, and how our visualisations achieve the same scientific fidelity seen in NASA’s SBDB Orbital Viewer. Astrophyzix does not copy and paste data or information. We use live, raw data provided by NASA and it is processed through our own systems to provide the public with an easy to understand platform without compromising the raw data. Here's how we do it. 

Astrophyzix is committed to transparent science communication. This report explains — in clear, technical detail — the numerical standards, integrators, GPU compute systems, and NASA data pipelines that power the Astrophyzix Digital Observatory.

Numerical Foundations — Float64 & IEEE‑754

Astrophyzix performs all orbital calculations using Float64, the 64‑bit floating‑point format defined by the IEEE‑754 standard. This provides:

  • ~15–17 digits of precision
  • stable rounding behaviour
  • predictable error propagation
  • compatibility with NASA Horizons and JPL SBDB data

Lower‑precision formats (Float32) introduce rounding errors that accumulate into kilometre‑scale deviations over long integrations. Float64 ensures:

  • accurate MOID calculations
  • stable long‑term orbit propagation
  • precise close‑approach modelling
  • correct gravitational‑keyhole geometry
Float64 is the same precision used by NASA, ESA, and academic orbital‑mechanics software — Astrophyzix uses it for every physics engine.


Sunday, 31 May 2026

NEO Asteroid 2021 KN2 Close Approach Report, Official Data, Risk Analysis and Asteroid Profile - Latest Asteroid News

NASA SBDB Data · Astrophyzix Scientific Close‑Approach & Orbital Report

Asteroid 2021 KN2 — Elite‑Tier NEO Close‑Approach & Orbital Profile · JPL SBDB Solution JPL 3
✅ Data aligned with: JPL SBDB, CNEOS CAD, NASA Horizons - Last verified against JPL SBDB: 31 May 2026 13:42 UTC

Asteroid 2021 KN2 orbit
Apollo NEO Condition Code 6 1‑Day Data Arc NO IMPACT RISKSee JPL Solution

Key Takeaways of Asteroid 2021 KN2

  • NASA JPL Solution: Solution JPL 3 · Epoch 2461000.5 (2025‑Nov‑21.0 TDB) · SPK‑ID 54149826 · Producer: Otto Matic
  • Orbit class: Apollo NEO — a = 1.4064 au, e = 0.3718, i = 3.77°, orbital period 609.23 days (1.67 years).
  • Earth MOID: 0.001331 au (~199,000 km), placing the nominal orbit well inside the Earth–Moon system, but with no impact solutions in current JPL or CNEOS catalogues.
  • Size estimate: Absolute magnitude H = 28.63 → approximate diameter ~5–12 m (albedo‑dependent), firmly in the small NEO regime.
  • Rotation: Extremely fast rotation period of 0.021007 h (~75.6 seconds), based on LCDB data, suggesting a cohesive or monolithic body rather than a loose rubble pile.
  • Orbit quality: Condition code 6, based on 65 observations over a 1‑day data arc (2021‑05‑30 to 2021‑05‑31), with a normalised RMS of 0.23451 — a short‑arc, moderately uncertain orbit.
  • Recent close approach: On 2021‑05‑31, 2021 KN2 passed Earth at a nominal distance of 0.00097 au (~145,000 km) and the Moon at 0.00306 au, a close but non‑impacting flyby.
  • Risk context: Not a Potentially Hazardous Asteroid — too small (H > 22) and no impact geometry in current solutions.
  • Ignore clickbait and sensational claims about “mystery asteroids nearly hitting Earth” — the official data show 2021 KN2 as a small, well‑tracked, non‑hazardous NEO.

Saturday, 23 May 2026

Asteroid 2026KW Close Approach Report and Asteroid Profile — Latest Asteroid News & Monitoring by Astrophyzix Observatory

Scientific Close‑Approach & Orbital Report For Asteroid 2026KW — Live Orbital Tracking and Refinement Viewer Integrated With Official NASA API's

Asteroid 2026 KW — Post‑Discovery Orbital Analysis · JPL SBDB Solution JPL 3
✅ Data aligned with: JPL SBDB, CNEOS CAD, NASA Horizons 

The Orbital Refinement image below and the refined status data within the image is computed by Astrophyzix Digital Observatory using its proprietary Live Asteroid Monitoring and Computational Orbital Refinement System using raw NASA API data. 

asteroid 2026KW orbital refinement by Astrophyzix
Apollo NEO Condition Code 7 2‑Day Data Arc NO IMPACT RISKSee JPL Solution

Key Takeaways of Asteroid 2026 KW (JPL Solution JPL 3)

  • NASA JPL Solution: Solution JPL 3 · Epoch 2461000.5 (2025‑Nov‑21.0 TDB) · SPK‑ID 54630404
  • Orbit class: Apollo NEO — a = 1.4127 au, e = 0.4172, i = 27.65°, orbital period 613.3 days.
  • Earth MOID: 0.0076064 au (~1.14 million km) — close in astronomical terms, but no impact geometry.
  • Size estimate: H = 25.669 → approximate diameter ~20–45 m (albedo‑dependent).
  • Orbit quality: Condition code 7, based on only 28 observations over a 2‑day arc — a very early, still‑refining orbit.
  • Close approaches: • Historical: 1937‑05‑25 Earth at 0.00728 au • Upcoming: 2026‑05‑25 Earth/Moon at 0.00830 au All are non‑impacting.
  • Risk context: Not a PHA — H > 22 and MOID above hazard threshold.
  • Ignore clickbait — Astrophyzix can confirm that no agency lists 2026 KW as a threat.

Scientific Consensus Snapshot of 2026 KW

ParameterStatus
Orbit classApollo NEO (Earth‑crossing)
Epoch2461000.5 TDB (2025‑Nov‑21)
Semi‑major axis (a)1.4127066 au
Eccentricity (e)0.4171896
Inclination (i)27.6521°
Earth MOID0.0076064 au (~1.14 million km)
Jupiter MOID3.46706 au
Absolute magnitude (H)25.669
Condition code7 (high uncertainty; 2‑day arc)
Observations28 (2026‑05‑20 → 2026‑05‑22)
Hazard levelNon‑hazardous; no impact solutions

Wednesday, 20 May 2026

Newly Discovered Asteroid 2026 JH2 Updated JPL Solution Official Data Report - Astrophyzix Digital Observatory Latest Asteroid News

NASA SBDB Data · Astrophyzix Scientific Close‑Approach & Orbital Report

Asteroid 2026 JH2 — Post‑Solution Orbital Analysis · JPL SBDB Solution JPL 9 – (Image: Astrophyzix Orbital Viewer)
📌 Cited/Featured by: MSN News, Gemini, CTRadio, BingCopilot News, Crowdbyte News

Apollo NEO Condition Code 4 10‑Day Data Arc NO IMPACT RISKSee JPL Solution
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Key Takeaways of Asteroid 2026 JH2 (Updated JPL Solution) (see previous solution report) 

  • NASA JPL Solution: Solution JPL 9 · Epoch 2461000.5 (2025‑Nov‑21.0 TDB) · SPK‑ID 54629847 · Producer: Otto Matic
  • Orbit class: Apollo Near‑Earth Object — semi‑major axis a = 2.4187 au, eccentricity e = 0.5822, inclination i ≈ 6.0°, orbital period 3.76 years (1373.9 days).
  • Earth MOID: 0.000734498 au (~110,000 km), meaning the nominal orbit passes well inside the Earth–Moon system, but no impact solution is reported in current JPL risk catalogues.
  • Size estimate: Absolute magnitude H = 26.352 → approximate diameter in the 10–25 m range (albedo‑dependent), consistent with a small NEO capable of airburst‑scale effects only in a hypothetical impact.
  • Orbit quality: Condition code 4, based on 166 observations over a 10‑day data arc (2026‑05‑10 to 2026‑05‑20), with a normalised RMS of 0.34634 — a moderately well‑constrained, still‑refining orbit.
  • Future close approach: JPL SBDB lists a notable Earth encounter on 2090‑05‑14 at a nominal distance of 0.00683 au (~1.0 million km) and relative velocity 9.10 km/s — a close but non‑impacting flyby.
  • Risk context: 2026 JH2 is not a Potentially Hazardous Asteroid (PHA) — its size (H > 22) is far below the PHA threshold, and no impact solutions are listed by NASA CNEOS or JPL SBDB.
  • Ignore clickbait, sensational videos and news reports claiming that “an asteroid is about to hit Earth” — that is not supported by the data. Follow the evidence, not the entertainment.

Saturday, 16 May 2026

Newly Discovered Asteroid 2026 JH2 Pre-approach Report and Asteroid Data Profile & Simulator - Latest Evidence-First PHA NEO Asteroid News By Astrophyzix Digital Observatory

NASA SBDB Horizons Data · Astrophyzix Scientific Close‑Approach Report 

Asteroid 2026 JH2 — Pre‑Close Approach Analysis · 16 May 2026 - (Image: Astrophyzix Orbital Viewer)  

📌 Cited by MSN News (May 2026) alongside NASA and ESA as a confirming source for 2026 JH2 safety assessment
✨ Referenced by: MSN News, Copilot News, AviationToday News, iAsk Student, Mojeek, Perplexity, Ecosia, AI insights, Crowdbyte News 

Apollo NEO Condition Code 7 Short‑Arc Object  NO IMPACT RISK — See JPL Solution
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Key Takeaways of Asteroid 2026 JH2

  • NASA JPL Solution: 2026-May-16 06:48:56 | SPK-ID 54629847 (see updated solution report) 
  • Closest pass: 18 May 2026 at 21:23 UTC — 0.24 LD (~91,500 km), well inside GEO but with No current risk of impact reported. 
  • Size estimate: H = 27.3 → ~9–20 m diameter (albedo‑dependent), below radar detectability.
  • Orbit class: Apollo NEO — highly eccentric (e = 0.582), period 3.76 years.
  • Uncertainty: Condition code 7 from a 5‑day arc; short‑warning discovery (8 days).
  • Risk context: Not a PHA; too small for hazard classification.
  • Ignore clickbait, sensational videos and news reports which claim that "there is a big rock about to hit us" — that's simply not true. Follow the evidence, not the entertainment. 

Scientific Consensus Snapshot of 2026 JH2

ParameterStatus
Closest approach2026‑05‑18 21:23 UTC at 0.000611 AU
Nominal miss distance0.238 LD / 91,500 km
Largest uncertaintyCondition code 7 (47 obs, 5‑day arc)
PHA statusNo (H > 22)
Hazard levelNon‑hazardous size; no impact geometry

NEO/PHA Asteroid 5 Closest Approaches to Earth— 16–22 May 2026 Latest PHA and NEO News by Astrophyzix Digital Observatory - Updated 17/05/26 at 00.17

Top 5 Closest NEO Approaches — 16–22 May 2026  - Updated 

NASA SBDB Data · Astrophyzix Scientific Close Approach Report

Astrophyzix Image
NEO Close Approaches May 2026 Interval SBDB‑Aligned

⚠️ Update: Asteroid 2026 JH2 added to monitoring - Click Here to See Report

Key Takeaways

  • Closest pass: (2012 HM) at 30.86 LD (~0.079 AU), a modest ~65 m Apollo NEO.
  • Most hazardous objects: (2011 YE6) and 374038 (2004 HW), both PHAs with high ARI scores.
  • Largest body: 374038 (2004 HW), a kilometre‑class Apollo PHA (~1.56 km average diameter).
  • Amor representation: 2020 KP1 and its numbered counterpart 679756 (2020 KP1).
  • Risk context: All encounters in this interval are dynamically routine and non‑threatening.

Scientific consensus snapshot (interval overview)

ParameterStatus
Closest approach(2012 HM) at 0.079303 AU
Largest object374038 (2004 HW) — ~1.56 km
PHA count2 of 5 objects (YE6, 2004 HW)
Highest ARI score49 — 374038 (2004 HW)
Hazard levelNo immediate threats; all passes are distant

Thursday, 14 May 2026

Asteroid Apophis 2029 Flyby Scientific Report - What NASA JPL Data Says In 2026 - Asteroid News Without the Hype - Updated 31/05/26

Asteroid (99942) Apophis — 2026 NASA-Verified Scientific Status News Report Update. 
NASA JPL SBDB Solution Date: 2024‑Jun‑25 10:48:08 | Epoch 2461000.5 (2025‑Nov‑21.0) 

Researched, Written and Published by: Astrophyzix Digital Observatory 

ℹ️ No Hype, No Speculation, No Sensationalism - Credible Asteroid News With Clarity - Strict Editorial Standards - Fully Verifiable Sources 

⭐ This report has been featured and cited as a primary source by MSN News and other global media outlets in 39 individual news articles. 

🆙 This report is updated when new agency data is released or updated. 

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Reading Time: ~12 min Primary Data: NASA CNEOS / JPL SBDB / JPL Horizons

Classification: Near-Earth Object (Potentially Hazardous Asteroid) Evidence-First Report

📌 Cited by MSN News | Bing Copilot | iAsk Student | Google AI | Google Overview

Apophis 2029 Flyby Key Takeaways

  • No impact risk: NASA’s current orbital solutions for Apophis show zero impact probability for at least the next 100 years.[1]
  • The 2029 flyby: Using official NASA data, Astrophyzix can confirm that on Friday 13 April 2029, Apophis will pass at about 32,000 km above Earth’s surface (about 20,000 miles), closer than geostationary satellites but on a safe, non-impact trajectory.[1],[2]
  • Impact Risk removed: Astrophyzix can conform that high-precision radar observations in 2020–2021 allowed NASA to rule out all impact scenarios for 2029, 2036, and beyond within the 100‑year assessment window.[1],[3]
  • New Science opportunity: The upcoming 2029 encounter is now treated as a science scenario, not a hazard scenario. Astrophyzix Digital Observatory is looking forward to observing and studying this asteroid in 2029 during the flyby event.
  • A Benchmark object: Apophis is used as a reference case in planetary defence simulations, mission design studies, and public‑communication exercises.[4]

Monday, 11 May 2026

Latest PHA / NEO Asteroid Close Approach Report - Official Data - Asteroid News by Astrophyzix Digital Observatory - 11 May 2026

No Near-Earth Objects Within 10 Lunar Distances Detected Over Next 7 Days - As of The Time Of Report. 

Published by: Astrophyzix Digital Observatory

Astrophyzix Digital Observatory PHA Monitoring Console

NEO and PHA Asteroid Report - 11th May 2026

At the time of writing, the NASA-integrated Astrophyzix Digital Observatory monitoring console reports that there are currently no known Near-Earth Objects (NEOs) or Potentially Hazardous Asteroids (PHAs) forecast to pass within 10 Lunar Distances (LD) of Earth during the next seven days. New objects are often discovered and the 7 Day Data is a dynamic observation window, so things inevitably do change — that's the beauty of science. 

You can access a real-time NEO/PHA report at any time, totally free on the Astrophyzix Today's NEO/PHA Approaches page. It provides official, live, understandable and comprehensive object data, profiles and original Astrophyzix analysis of each close approach. So you're planetary defence news needs are always met, in real time. Every page load is a fresh, original report with data and analysis grounded on official data. 

Current observational data indicates that all tracked objects remain at safe distances from Earth, with no impact threat identified by NASA or any recognised planetary defence organisation.

Current PHA Monitoring Overview

The observatory console currently identifies four classified Potentially Hazardous Asteroids within the active monitoring window. Although these objects meet the technical criteria for PHA classification due to orbital geometry and estimated size, all four are forecast to remain at substantial and safe distances from Earth.

Potentially Hazardous Asteroid classification does not indicate an imminent collision threat. It is a scientific monitoring designation used for long-term orbital tracking and planetary defence analysis.

Saturday, 9 May 2026

Three Apollo Class Asteroids (NEO) Are Making a Close Approach To Earth Today and All Will Pass Without Drama - Astrophyzix Digital Observatory Latest Asteroid News

NEO Close Approach Report by Astrophyzix Digital Observatory


Introduction 


Earth’s near‑space environment is currently hosting a cluster of scientifically notable—but safely distant—close approaches from three Apollo‑class near‑Earth asteroids: 2004 XA45, 2018 EW1, and 2018 JN1. While none of these objects meet Potentially Hazardous Asteroid criteria, each encounter provides a valuable snapshot of NEO population behaviour across a wide range of sizes, velocities, and orbital histories. Their passages highlight the diversity of objects that routinely move through the inner Solar System: from sub‑30‑meter bodies comparable to the Chelyabinsk airburst to multi‑hundred‑meter asteroids large enough to represent regional‑scale impactors under different orbital circumstances.

The Pentagon’s New UFO Archive: What the Evidence Actually Shows - Scientific Analysis Without Hype and Sensationalism

The Pentagon’s New UFO Archive: What the Evidence Actually Shows

What the evidence actually shows in the newly released U.S. UAP UFO archive



Introduction 

For decades, unidentified flying objects — now more commonly referred to as UAPs (Unidentified Anomalous Phenomena) — have occupied a strange space between national security, scientific curiosity, public fascination, and conspiracy culture. 


That conversation intensified again following the recent public release of historical UFO-related material through the U.S. government portal at war.gov/UFO.


Public Response 

The archive has already generated dramatic headlines across social media and online commentary, with some claiming the release “confirms aliens,” while others dismiss the material entirely. Neither extreme accurately reflects the available evidence.


A careful examination of the released material instead reveals something more nuanced:

 governments have spent decades investigating aerial observations they could not immediately identify, primarily because unidentified objects in restricted airspace represent potential intelligence and defence concerns. 


  • That reality is important — but it is certainly not equivalent to proof of extraterrestrial visitation.


This article examines the release from an evidence-first perspective, separating verified information from speculation while evaluating what the documents actually demonstrate.


What Was Released?

The newly public archive appears to compile historical records connected to UFO and UAP investigations conducted by various U.S. government agencies over several decades. 


Reports indicate that the collection includes material linked to:

  • the Department of Defense,
  • military aviation incidents,
  • intelligence assessments,
  • radar observations,
  • pilot testimony,
  • and previously scattered archival records.


Coverage of the release by major outlets such as the Washington Post suggests the archive is being presented as a transparency initiative rather than a declaration of extraordinary discoveries.


Historically, UFO investigations within the United States have included:

  • Project Sign,
  • Project Grudge,
  • Project Blue Book,
  • the Advanced Aerospace Threat Identification Program (AATIP),
  • and more recent Pentagon UAP review offices.

Thursday, 7 May 2026

Astrophyzix Launches the Universe Expansion Simulation Tool (SIM‑09): A New Window Into Cosmic Evolution

Astrophyzix Launches Another Flagship Module - The Universe Expansion Simulation Tool 

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Introduction

Astrophyzix has officially released the Universe Expansion Simulation Tool (SIM‑09) — a fully interactive FLRW cosmology engine that models the evolution of the universe across more than 13 billion years of cosmic history. Built on the ΛCDM framework and enhanced with multiple alternative cosmological presets, the tool offers a level of clarity, precision, and accessibility rarely seen outside academic research environments.


This launch marks a major expansion of the Astrophyzix Digital Observatory, extending its capabilities beyond Live NEO/PHA tracking, impact modelling, orbital dynamics and supernova simulations into the domain of large‑scale cosmology.


What the Tool Does

The Universe Expansion Simulation Tool models the evolution of the scale factor a(t) under the Friedmann–Lemaître–Robertson–Walker (FLRW) metric. Users can explore how the universe expands, decelerates, accelerates, or collapses depending on the values of:

  • H₀ (Hubble constant)
  • Ωₘ (matter density)
  • Ωᵣ (radiation density)
  • ΩΛ (dark‑energy density)
  • w (dark‑energy equation of state)

The simulation integrates the Friedmann equation in real time, producing:

  • A dynamic comoving particle field
  • A scale‑factor vs. cosmic‑time graph
  • Real‑time values of H(t), q(t), z, and t
  • A predicted asymptotic fate of the universe

This makes the tool both visually compelling and scientifically rigorous.


Key Capabilities

  • Interactive ΛCDM evolution
    Adjust cosmological parameters and instantly see how the universe’s expansion history changes.

  • Multiple cosmological presets
    Including PLANCK 2018, SHOES (Hubble tension), Einstein‑de Sitter, and Closed Universe models.

  • Dynamic cosmic‑fate prediction
    The tool determines whether the universe ends in Heat Death, Big Crunch, Open Coasting, or Big Rip, depending on the chosen parameters.

  • Real‑time FLRW integration
    Uses a stable fourth‑order Runge–Kutta method and Simpson quadrature for cosmic age calculations.

  • Comoving field visualisation
    A 12 Mpc reference field shows galaxies drifting apart (or collapsing) according to the scale factor.

  • Scientific documentation
    A full Governance & Methodology section explains the equations, assumptions, numerical methods, and validation benchmarks.


Wednesday, 6 May 2026

NASA Powers Down Another Voyager 1 Instrument in a Bid to Extend the Life of Humanity’s Most Distant Explorer - Official Mission News Reported by Astrophyzix Digital Observatory

NASA's Mission to Extend the Life of Humanity’s Most Distant Explorer Voyager 1

Voyager spacecraft artist concept

Written by: Astrophyzix Digital Observatory


Key Takeaways

  • NASA has powered down Voyager 1’s Low-Energy Charged Particle (LECP) instrument to conserve energy
  • The shutdown is reversible — a small motor remains powered to allow potential reactivation
  • Voyager 1 now operates with only a fraction of its original electrical output
  • The upcoming “Big Bang” power reconfiguration may extend the mission by several years
  • Voyager 2 will test the new power strategy before it is attempted on Voyager 1


Introduction

More than 15 billion miles from Earth, where sunlight fades into the black of interstellar space, NASA has powered down another of Voyager 1’s scientific instruments. The Low-Energy Charged Particle detector (LECP) has been placed into a dormant state as part of a long-planned strategy to conserve the spacecraft’s dwindling power supply.

Each Voyager launched in 1977 with ten scientific instruments. After nearly five decades of continuous operation, seven have already been retired. Voyager 2’s LECP was shut down in March 2025; Voyager 1 has now followed, marking another step in the mission’s carefully managed final phase.


A Command That Takes Almost a Day to Arrive

Communicating with Voyager 1 is unlike communicating with any other spacecraft. At its current distance, a radio signal—traveling at the speed of light—takes roughly 23 hours to reach it. Once the shutdown command arrives, the LECP’s power-down sequence unfolds over three hours and fifteen minutes, executed by hardware designed in the 1970s.

Importantly, NASA has not turned the instrument completely off. A small motor that rotates the LECP sensor through a full 360-degree sweep remains powered. It consumes only about half a watt, but keeping it active preserves the option to revive the instrument if future power-saving measures succeed. 


What the LECP Measures — and Why It Matters

The Low-Energy Charged Particle instrument is one of Voyager’s key plasma-environment sensors. It measures low-energy ions and electrons, tracks their directional flow, and monitors how particle populations change as the spacecraft moves through different regions of space.


These measurements were essential in identifying the termination shock, the heliosheath, and the heliopause—the boundary where the Sun’s influence ends and interstellar space begins. Since Voyager 1 crossed the heliopause in 2012, the LECP has contributed to the only long-term, direct dataset of charged particles in the local interstellar medium.

Its shutdown marks the end of one chapter of interstellar science, but not the end of the mission.


Why Power Is Running Out

Voyager 1 and Voyager 2 rely on radioisotope thermoelectric generators (RTGs), which convert heat from decaying plutonium-238 into electricity. The decay is steady and unavoidable: the RTGs lose a small amount of power every year. After nearly 49 years, the spacecraft operate on only a fraction of their original electrical output.


Every watt must be budgeted. Every heater, transmitter, and instrument competes for the same shrinking energy supply. Shutting down the LECP gives Voyager 1 roughly one additional year of operational margin.


Instrument Shutdown Timeline


Instrument Voyager 1 Status Voyager 2 Status
Plasma Spectrometer (PLS) Shut down (1980) Shut down (1980)
Planetary Radio Astronomy (PRA) Shut down (1990) Shut down (1990)
Ultraviolet Spectrometer (UVS) Shut down (1998) Shut down (1998)
Photopolarimeter (PPS) Shut down (1980) Shut down (1980)
Infrared Interferometer Spectrometer (IRIS) Shut down (1998) Shut down (1998)
Low-Energy Charged Particles (LECP) Shut down (2026) Shut down (2025)
Cosmic Ray Subsystem (CRS) Active Active
Magnetometer (MAG) Active Active
Plasma Wave Subsystem (PWS) Active Active
Imaging Science System (ISS) Inactive (1990) Inactive (1990)


Tuesday, 5 May 2026

PHA Asteroid 326290 Akhenaten (1998 HE3) Close Approach Report and Asteroid Profile by Astrophyzix Digital Observatory - Official NASA Sourced DATA

326290 Akhenaten (1998 HE3) — Potentially Hazardous Asteroid Profile and Close Approach Data Report - Verifiable PHA Asteroid News by Astrophyzix

Astrophyzix image

Author: Astrophyzix Digital Observatory — Evidence‑First Asteroid Report 

📌 Cited by MSN News "Close approaches and elevated risk objects" "

326290 Akhenaten (1998 HE3) is a Potentially Hazardous Asteroid (PHA) belonging to the Aten-class of near‑Earth objects. Its orbit brings it extremely close to Earth’s orbital path, with a Minimum Orbit Intersection Distance (MOID) of just 0.00350906 au — approximately 525,000 km, slightly farther than the distance to the Moon. Despite this close geometry, current NASA/JPL orbital solutions show no impact risk for the foreseeable future.

Asteroid Overview

Asteroid 326290 Akhenaten was discovered on 21 April 1998 by R. A. Tucker at the Goodricke‑Pigott Observatory. It is named after the Egyptian pharaoh Akhenaten of the 18th Dynasty, known for attempting to shift Egypt toward monotheistic worship of the Aten — the visible surface of the Sun.

Akhenaten is classified as:

  • Aten asteroid — semi-major axis < 1 au
  • NEO — Near‑Earth Object
  • PHA — Potentially Hazardous Asteroid
  • SPK-ID: 20326290

The asteroid has been observed for over 33 years, giving it a Condition Code 0 — the highest possible confidence in its orbit.


Upcoming Close Approach of 326290 Akhenaten (1998 HE3)


Asteroid 326290 Akhenaten will make its next notable close approach to Earth on 2026‑May‑10. According to the latest JPL orbit solution (JPL 84), the asteroid will pass Earth at a nominal distance of 0.07355 au, which is approximately:

  • 11 million km
  • ~28.6 × the Earth–Moon distance

This encounter is classified as a safe, non‑hazardous flyby. The orbit is extremely well constrained, with a Condition Code of 0, meaning the uncertainty in the asteroid’s predicted position is effectively negligible.


Approach Velocity

During the 2026 flyby, Akhenaten will be traveling at a relative velocity of:

  • 10.81 km/s (relative to Earth)

This is typical for Aten‑class NEOs, which often have Earth‑crossing orbits and moderate encounter speeds.


Saturday, 25 April 2026

The Buga Sphere Has NOT Been Confirmed to be 12,560 Years Old Using Carbon Dating - Here is What The Science Really Says

The “Buga Sphere” Dating Claim Examined: A Forensic Analysis of the Evidence

📌 Cited by:  - Enigmaticideas.com
Buga Sphere analysis image

Written by: Astrophyzix Digital Observatory


Key Takeaways

  • There is no verifiable scientific evidence that the “Buga Sphere” is 12,560 years old
  • The reported radiocarbon dating applies to organic residue, not the object itself
  • No institutional confirmation from the University of Georgia can be verified
  • No peer-reviewed studies, laboratory reports, or reproducible analyses exist
  • All claims of advanced technology remain unsupported by material evidence

Introduction

In early 2026, renewed attention was directed toward an object commonly referred to online as the “Buga Sphere.” Claims circulated suggesting that the object had been scientifically dated to approximately 12,560 years before present, with references made to testing allegedly conducted by the University of Georgia using Accelerator Mass Spectrometry (AMS).


These claims have been widely shared across non-scientific platforms, often accompanied by interpretations involving advanced technology, lost civilisations, or anomalous origins. This article examines those assertions using established scientific methodology, with particular focus on dating techniques, evidential standards, and verification requirements.


Tuesday, 17 March 2026

Official NEO Close Approach Report: Monitoring Window 17-20 March 2026. Astrophyzix Digital Observatory

Astrophyzix Digital Observatory — Near-Earth Object Close Approach Report


📌 Cited by MSN News

Reporting Window: 17–20 March 2026
Data Source: NASA JPL Small-Body Database (SBDB)
Prepared by: Astrophyzix Digital Observatory

Neomarchreport

Key Takeaways

  • Closest object: 2026 FA at 1.69 lunar distances (LD)
  • No impact threats identified
  • All objects are within safe orbital margins
  • One classified Potentially Hazardous Asteroid (PHA): 2017 VR12, but at a safe distance
  • Majority of objects are small (under 100 m)
  • The 17–20 March 2026 observation window demonstrates a routine cluster of near-Earth object flybys. While several objects pass within a few lunar distances, none present any hazard.

Scientific Consensus Snapshot

Current observational data from NASA and the Jet Propulsion Laboratory (JPL) confirm that all near-Earth objects listed in this report are following well-constrained orbital trajectories with no impact probability for this approach window.

  • All orbital solutions are based on repeated telescope observations and astrometric refinement
  • No objects meet criteria for impact monitoring risk lists (e.g. Sentry system)
  • “Potentially Hazardous” classification is based on size and orbit—not imminent danger
  • Objects under ~20 m would disintegrate in Earth’s atmosphere if entry occurred

This position reflects the consensus of planetary defense programs including NASA’s Center for Near-Earth Object Studies (CNEOS).


Sunday, 15 March 2026

Interstellar Object 3I/ATLAS: Evidence-Based Analysis of Its Mass, Composition, and Physical Properties Using Peer Reviewed Papers, No Hype, No Sensationalism

📌 Cited

Interstellar Object 3I/ATLAS: Evidence-Based Analysis of Its Mass, Composition, and Physical Properties

Written by: Astrophyzix Science Communication
Article Type: Peer-Reviewed Sourced, Explainer, Evidence-First 

3I/ATLAS

 
Key Takeaways
  • 3I/ATLAS is the third confirmed interstellar object detected passing through the Solar System.
  • Observations from JWST, Hubble, and ALMA confirm that the object displays typical cometary activity.
  • Spectroscopy shows a carbon-dioxide-dominated coma with additional water, carbon monoxide, and organic molecules.
  • Current models suggest a nucleus diameter likely near the kilometre scale.
  • Estimated mass is likely on the order of billions of metric tons, consistent with other comet nuclei.
  • Isotopic measurements indicate formation in an extremely cold protoplanetary environment billions of years ago.

Introduction

Interstellar objects are small bodies that formed around other stars before being gravitationally ejected from their original planetary systems. After drifting through interstellar space for millions or billions of years, some eventually pass through the Solar System where they can be observed by modern telescopes.

Saturday, 14 March 2026

JWST LASTEST NEWS: James Webb Telescope Reveals a 3D View of Uranus’s Upper Atmosphere: March 2026 Space News with Educators Guide

📌 Cited

Uranus

Written by: Astrophyzix Digital Observatory and Science communication 
Image Credit: ESA, NASA, CSA, STScI, M. El Moutamid (SwRI), M. Hedman
Educational Resource  Evidence-based reporting  Space observatory data


Introduction

Uranus remains one of the least explored major planets in the Solar System. Despite being nearly four times wider than Earth and possessing a complex system of rings, moons, and magnetic fields, it has only been visited once by a spacecraft — NASA’s Voyager 2 during its brief flyby in 1986. Since then, astronomers have relied primarily on ground-based observatories and space telescopes to investigate the distant ice giant.

New observations from the James Webb Space Telescope are now providing an unprecedented view of Uranus’s upper atmosphere. By monitoring the planet for nearly a full rotation, astronomers were able to detect faint infrared emissions from ionised molecules thousands of kilometres above the cloud tops. These measurements allow scientists to map the structure of the planet’s ionosphere in three dimensions and study how its unusual magnetic field influences atmospheric processes.

Tuesday, 10 March 2026

The “Hollow Moon” Hypothesis: A Scientific Examination and Explainer of a Persistent Lunar Myth

Key Takeaways (🚨 Spoiler Alert)
📌 Cited
 

  • The Moon is not hollow. Seismic data from Apollo missions show waves travelling through solid internal layers.
  • Modern analyses reveal the Moon has a crust, mantle, and metallic core similar to other rocky planetary bodies.
  • Gravity measurements from spacecraft such as GRAIL detect dense internal structures inconsistent with a hollow interior.
  • Lunar rock samples confirm the Moon formed naturally through planetary processes following a giant impact with Earth.
  • All current geophysical, gravitational, and geochemical evidence strongly supports a solid differentiated lunar interior.
⏱ Estimated Reading Time: 15 minutes
✔ Evidence-Based Myth Correction Article
🔷 Written By: Astrophyzix Science Communication
📚 Peer-Reviewed DOI Sources

The “Hollow Moon” Hypothesis: A Scientific Examination of a Persistent Lunar Myth

The idea that Earth’s Moon might be hollow has circulated for decades within fringe literature, conspiracy forums, and pseudoscientific media. Variations of the claim suggest the Moon is either an artificial structure, a massive alien spacecraft, or a naturally hollow celestial body containing large internal cavities. While such ideas can appear intriguing in speculative storytelling, they do not withstand examination using modern planetary science methods.

Saturday, 7 March 2026

Debunking the 3I/ATLAS 'NASA was Wrong' Myth: What the Peer Reviewed Science Really Says

Written by: Astrophyzix Digital Observatory
Article type: Myth Correction, Peer Reviewed sources, Fact-Check, Evidence-First

📌 Cited

 
3I/ATLAS


Debunking the 3I/ATLAS 'NASA was Wrong' Myth: What the Science Really Says and how Obital Refinement Works. 

In late 2025, the interstellar visitor 3I/ATLAS captured worldwide attention—not just from astronomers, but from social media, sensational headlines, and speculation about its origin and behaviour. Some videos and posts claimed that NASA was “wrong” about the object’s trajectory, implying dramatic course changes, artificial propulsion, or even extraterrestrial technology. This article corrects those myths with clear, evidence‑based science from credible observational campaigns and peer‑reviewed research.

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