Astrophyzix Digital Observatory's
Evidence-First Asteroid Reporting

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 Latest News. Show all posts
Showing posts with label Latest News. Show all posts

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 the 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]

Wednesday, 13 May 2026

Asteroid Apophis 2029 Flyby Updated Frequently Asked Questions — Answered With Real Science by Astrophyzix Digital Observatory

Everything you need to know about Asteroid Apophis and it's 2029 Close Approach to Earth - Evidence-First Asteroid News Without Sensationalism or Hype


Published by: Astrophyzix Digital Observatory — Latest PHA Asteroid News (Data updated: 13 May 2026)



📌 Cited by Microsoft Bing AI 📌 Cited by MSN NEWS
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Introduction 


This FAQ uses verified scientific data from NASA, JPL, ESA, and peer‑reviewed research. It is designed to cut through misinformation and explain the 2029 Apophis flyby using real orbital mechanics, radar measurements, and planetary defence standards


Planetary Defence is a serious subject, it should be reported responsibly and with clarity. Never trust click-bait titles or sensational headlines you see online. Always consult official data from credible, trusted sources. Below are common questions people ask, answered with integrity. 

What is Apophis?

Asteroid (99942) Apophis is a near‑Earth asteroid discovered on 19 June 2004. It is an Aten‑class asteroid, meaning its orbit is smaller than Earth’s but crosses Earth’s orbital path. Apophis is classified as an S‑type stony asteroid with a diameter of roughly 340–370 metres. Radar imaging from NASA’s Goldstone facility shows Apophis has a bi‑lobed “peanut” shape, similar to other rubble‑pile asteroids.



The new V4 Astrophyzix Apophis Tracking and Monitoring tool is considered by Microsoft Bing to be the "best public Apophis tracker available online". It offers the most comprehensive tracking experience with real-time data, including the asteroid's position, speed, and potential encounters with Earth. The tool is integrated with the official NASA API and provides exclusive data sets, making it a valuable resource for both astronomers and the general public interested in the asteroid's trajectory and safety

Is Apophis going to hit Earth in 2029?

No. Astrophyzix can confirm that there is no risk in 2029. Ignore all of the click-bait and sensational headlines. Again, there is no impact risk in 2029 — you're safe. 

NASA’s orbital solutions, refined with radar data from 2020–2021, eliminated all impact trajectories for 2029, 2036, 2068, and the next 100 years. Apophis is now rated Torino Scale 0 and Condition Code 0, meaning its orbit is extremely well known. If NASA had even the slightest doubts the condition code would be higher than zero, and it isn't. 

How close will Apophis come to Earth in 2029?

On Friday 13 April 2029, Apophis will pass about 32,000 km above Earth’s surface — closer than geostationary satellites. This is roughly:

  • 1/10th the distance to the Moon
  • Closer than many communication satellites
  • Visible to the naked eye from parts of Europe, Africa, and Asia

Why was Apophis once considered dangerous?

In 2004, astronomers had only a short observation arc. With limited data, the uncertainty region for Apophis’s orbit was large, and some early solutions intersected Earth. As more data arrived, especially radar ranging, the uncertainty collapsed and all impact scenarios were ruled out.


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.


Asteroid (2001 MS3 / 2026 GF) — 2026 Scientific Close‑Approach Report and Asteroid Profile - Official NASA Data - Latest Potentially Hazardous Asteroid News by Astrophyzix Digital Observatory

Near Earth Asteroid (2001 MS3) — 2026 Scientific Close‑Approach Report and Asteroid Profile - Official NASA Data Sources


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Apollo [NEO] SPKID: 50092326 JPL Solution 16 Epoch 2461000.5 (2025‑Nov‑21.0 TDB)

Condition Code 0

Asteroid 2001 MS3 Key Takeaways

  • Precisely determined Apollo NEO: (2001 MS3) is an Apollo‑class Near‑Earth Object with semi‑major axis a = 2.139 au and perihelion q ≈ 0.997 au, crossing Earth’s orbital region on a ~3.13‑year cycle.
  • Epoch‑anchored orbit: All osculating elements are referenced to Epoch 2461000.5 (2025‑Nov‑21.0 TDB) in the heliocentric IAU76/J2000 ecliptic frame (JPL Solution 16).
  • 2026 flyby is distant and safe: On 2026‑May‑13, 2001 MS3 passes Earth at a nominal distance of 0.05306 au (~7.94 million km), with minimum and maximum distances identical at the quoted precision.
  • Elite orbit quality: A 24.82‑year data arc (39 observations) with DE441 and SB441‑N16 yields a Condition Code 0 solution and normalized RMS 0.60351.
  • Small, non‑hazardous body: With absolute magnitude H = 24.0, the diameter is of order tens of metres; Earth MOID is 0.0243864 au, and no impact solutions are known.

Scientific consensus snapshot (preliminary)

Parameter Status
Orbit determination quality Excellent — Condition Code 0, long data arc, low RMS
Impact risk No known impact trajectories; not on active risk lists
2026 Earth encounter Distant, dynamically routine, fully non‑hazardous
Long‑term dynamics Moderate secular evolution; weak Jovian perturbations (Tjup = 3.514)
Planetary‑defence relevance Benchmark small Apollo NEO for MOID‑based classification and tracking

Object overview and physical characteristics

Parameter Value
Primary designation (2001 MS3)
Alternate designation 2026 GF
Classification Apollo‑class Near‑Earth Object (NEO)
Absolute magnitude (H) 24.0 (reference: MPO74093)
Estimated diameter (typical NEO albedo) ~40–60 m (order‑of‑magnitude)
Rotation period Not determined
Albedo / spectral type Unknown; no published taxonomy at this solution


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

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.


Friday, 1 May 2026

Astrophyzix Launches SolarForm — A Real‑Time Solar System Formation Simulation Engine

A One of a Kind, Unique, Real‑Time Solar System Formation Simulation Engine


Written by: Astrophyzix Digital Observatory

Astrophyzix banner image
Platform Update Astrophysics Simulation Educational Module

Introduction

Astrophyzix is proud to announce the release of SolarForm, a scientifically rigorous, real‑time simulation engine that models the birth and evolution of a planetary system from the collapse of a protoplanetary nebula to the emergence of planetesimals, proto‑planets, and gas giants.

SolarForm is designed as an educational scientific module, providing the public, students, and astronomy enthusiasts with a clear, interactive way to explore the physics that shaped our Solar System. The module is powered by real astrophysical equations, peer‑reviewed models, and a direct N‑body gravitational integrator.

A Real‑Time Window Into Planetary Formation

SolarForm simulates the early stages of solar system formation using physically grounded models drawn from astrophysics, celestial mechanics, and planetary science. Users can watch a nebular disk evolve dynamically as bodies collide, merge, accrete, and migrate under gravity.

Key features include:

  • N‑body gravitational physics using a velocity‑Verlet symplectic integrator.
  • Planetesimal growth and accretion through inelastic collisions with gravitational focusing.
  • Protoplanetary disk density profiles based on the Minimum Mass Solar Nebula (MMSN).
  • Keplerian orbital initialization scaled by nebula mass and angular momentum.
  • Snowline physics determining where ice bodies and gas giant cores can form.
  • Real‑time classification of bodies into planetesimals, proto‑planets, rocky planets, and gas giants.

The simulation updates continuously, allowing users to observe the chaotic, emergent behaviour of early planetary systems as they stabilize over time.


Tuesday, 28 April 2026

Newly discovered NEO Asteroid 2026 HZ3 Close Approach Report and NEO Profile by Astrophyzix Digital Observatory

Asteroid (2026 HZ3) — 2026 NASA-Linked Preliminary Scientific Status Report
NASA JPL SBDB Solution 5 (2026-Apr-28 06:20:37)


Researched, Written and Published by: Astrophyzix Digital Observatory

Original, Timely, Verifiable Asteroid News and Planetary Defence Monitoring by Astrophyzix.com & Astrophyzix.org


📌 Cited by MSN News | Bing Copilot News Image
Reading Time: ~8 min Primary Data: NASA JPL SBDB / CNEOS

Classification: Apollo Near-Earth Object (NEO) SPK-ID: 54613601

Asteroid 2026 HZ3 Key Takeaways

  • Newly discovered NEO: (2026 HZ3) is a recently observed Apollo-class near-Earth asteroid with a short data-arc (4 days) and a relatively high orbital uncertainty (condition code 7).
  • Small object: With an absolute magnitude H ≈ 25.3, (2026 HZ3) is likely a small asteroid, on the order of a few tens of metres in diameter, depending on its surface reflectivity.
  • Close approach in 2026: A nominal close approach to Earth occurs on 1 May 2026 at a distance of about 0.010 au (around 1.5 million km), well outside any impact scenario under current solutions.
  • Earth MOID: The current Minimum Orbit Intersection Distance (MOID) with Earth is about 0.00497 au (~745,000 km), indicating close-approach potential but not an imminent threat.
  • Preliminary orbit: Because the orbit is based on only 38 observations over 4 days, all risk and trajectory assessments are considered preliminary and will be refined as more data are collected.

Scientific consensus snapshot (preliminary)

ParameterStatus (NASA JPL SBDB Solution 5 | 2026-Apr-28 06:20:37)
Impact risk (100-year context)No confirmed impact solution; orbit still under refinement (condition code 7).
Orbital uncertaintyModerate–high (short 4-day data-arc, condition code 7).
2026 close approachNominal miss distance ~0.010 au (~1.5 million km) — a safe flyby under current solutions.
Hazard classificationNEO (Apollo). Not formally classified as a Potentially Hazardous Asteroid (PHA) at this time.
Scientific priorityMonitoring and orbit refinement; representative of small NEOs that frequently pass near Earth.

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.


Wednesday, 22 April 2026

Weekly Potentially Hazardous Asteroid and NEO Close Approach Report 22 April to 28 April Official NASA Planetary Defence Data

Astrophyzix Dynamic 7 Day NEO and PHA Close Approach Report and Forecast

Astrophyzix Weekly Near-Earth Object (NEO) & Potentially Hazardous Asteroid (PHA) Close Approach Report

Written by: Astrophyzix Digital Observatory
Astrophyzix Planetary Defence Systems NEO Monitoring Visual
Credit: Astrophyzix Planetary Defence Systems

Observatory Status & Data Integrity

Astrophyzix Planetary Defence reports are written using a fully dynamic, on-demand data retrieval pipeline linked directly to NASA's CNEOS NeoWs API infrastructure.

The monitoring interval is calculated at runtime and spans seven days forward from the exact timestamp of system access.

No caching layers, pre-processing, or static datasets are used. Every value presented is sourced from the most recent orbital solutions available within NASA systems at the time of query execution by the Astrophyzix Planetary Defence System.



Certain data is computed through the Astrophyzix Risk Index and presented alongside the raw data to give readers an easy to visualise scale of how notable an object is an a clear interpretation of the data.


UTC Timestamp Wed, 22 Apr 2026 20:10:55
Monitoring Window 2026-04-22 → 2026-04-28
Data Source NASA CNEOS NeoWs API (Live Stream)

Monitoring Overview

  • Total NEOs tracked: 87
  • Potentially Hazardous Asteroids: 8
  • Objects within 10 Lunar Distances: 6
  • Closest recorded approach: 2.956 LD
  • Mean relative velocity: 13.7 km/s
  • Largest object: 54071 (2000 GQ146) — 1418 m

Thursday, 16 April 2026

Potentially Hazardous Asteroid and Near-Earth Object (NEO) Close Approach Report & Asteroid Profile for Asteroid 2026 BK2

Astrophyzix Near-Earth Object (NEO) Close Approach Report & Asteroid Profile: (2026 BK2)

Written by: Astrophyzix Digital Observatory

📌 Cited by MSN News 📌 Referencd by Copilot News
Astrophyzix NEO Image
Image Credit: NASA JPL SBDB

Introduction


Asteroid (2026 BK2) is an Apollo-class near-Earth object (NEO) classified as a Potentially Hazardous Asteroid (PHA). Its orbit intersects Earth's orbital region, and its size exceeds the threshold used in hazard classification frameworks.


The close approach on 2026-Apr-22 12:36 (TDB) represents a relatively close but well-understood encounter. Despite its classification, no impact risk is identified based on current orbital solutions.


Potentially Hazardous Asteroid (PHA) news refers to verified reports of near-Earth asteroids that meet specific size and orbital proximity thresholds. Despite the classification, the vast majority of PHAs pose no impact threat during observed close approaches.

Key Takeaways


  • Close approach on 2026-Apr-22 12:36 (TDB).
  • Miss distance: 0.02569 AU (~10.0 LD / ~3.84 million km).
  • Relative velocity: 8.13 km/s.
  • Estimated diameter: ~160–350 meters (derived from H=21.05).
  • Condition code 0 (extremely well constrained orbit).
  • No impact threat identified.
  • ARI Score: 50/100 - Notable Approach 


Scientific Consensus Snapshot


The orbital solution for (2026 BK2) is based on 125 observations spanning 2096 days (2020-07-18 to 2026-04-14). The condition code of 0 indicates a highly reliable trajectory solution. The timing uncertainty for the 2026-Apr-22 12:36 (TDB) close approach is less than one minute, confirming extremely high positional certainty.


Saturday, 11 April 2026

Potentially Hazardous Asteroid Close Approach Report For Asteroid 192559 (1998 VO) April 2026 Official NASA Data

Astrophyzix Near-Earth Object (NEO) Close Approach Report & Asteroid Profile: 192559 (1998 VO)

Written by: Astrophyzix Digital Observatory

📌 Cited by iAsk Student

Astrophyzix Image

Image Credit: NASA JPL SBDB

Introduction


Asteroid 192559 (1998 VO) is a well-characterised Apollo-class near-Earth object (NEO) classified as a Potentially Hazardous Asteroid (PHA). With a data arc spanning over two decades and hundreds of observations, its orbit is extremely well constrained, allowing for precise modelling of its trajectory across both past and future epochs.

The close approach on 2026-Apr-14 10:04 (TDB) represents a routine, distant flyby with no impact risk. Its PHA classification reflects orbital geometry (Earth-crossing potential) and size thresholds, not an immediate threat.


Potentially Hazardous Asteroid (PHA) news refers to verified reports of near-Earth asteroids that meet specific size and orbital proximity thresholds. Despite the classification, the vast majority of PHAs pose no impact threat during observed close approaches.

Key Takeaways


  • Close approach on 2026-Apr-14 10:04 (TDB).
  • Miss distance: 0.32726 AU (~127.3 LD / ~48.9 million km).
  • Relative velocity: 17.60 km/s.
  • Estimated diameter: ~300–700 meters.
  • Condition code 0 (orbit extremely well constrained).
  • No impact threat identified.
  • Astrophyzix Risk Index® Notibility score: 48 (Elevated).


Scientific Consensus Snapshot


The orbit of 192559 (1998 VO) is derived from 575 observations spanning 1998-11-10 to 2018-11-13, producing a condition code of 0—the highest confidence level in orbit determination. The timing uncertainty for the 2026-Apr-14 10:04 (TDB) encounter is less than one minute, indicating negligible positional uncertainty.


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