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. 

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

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

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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]

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

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.

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

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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.

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

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.

Potentially Hazardous Asteroid 2026GU Close Approach Report and Asteroid Profile Latest Near Earth Object News

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

Written by: Astrophyzix Digital Observatory

📌 Cited by iAsk Student

Image Credit: NASA JPL SBDB

Introduction

A Potentially Hazardous Asteroid (PHA)  is a near-Earth object with an absolute magnitude of 22.0 or brighter (typically larger than ~140 metres) and a minimum orbit intersection distance (MOID) of 0.05 AU or less. This classification does not indicate an impact threat, but identifies objects that require precise orbital monitoring.

Asteroid (2026 GU) is an Amor-class near-Earth object (NEO) classified as a Potentially Hazardous Asteroid (PHA) based on its size and orbital proximity to Earth. The object was observed over a short 5-day arc in this week and its orbit is currently defined by the initial JPL solution (Solution 1 on 09 April 2026.) 

Despite its PHA classification, current orbital solutions indicate a relatively distant Earth flyby on 14 April 2026. Continued observations are required to refine its trajectory due to the limited observational baseline and elevated uncertainty level.

Key Takeaways

• Close approach on 2026-Apr-14 at ~0.09884 AU.
• Equivalent to approximately 38.4 lunar distances (~14.8 million km).
• Classified as a Potentially Hazardous Asteroid (PHA).
• Estimated diameter: ~150–300 meters (based on H magnitude).
• Orbit currently constrained using 90 observations over 5 days.
• Condition code 8 indicates high orbital uncertainty.
• No impact threat identified.

Scientific Consensus Snapshot

The current orbital solution for (2026 GU) is based on a short observational arc and remains subject to refinement. While the object's classification as a PHA reflects its long-term orbital geometry, the 14 April 2026 encounter is well outside any hazardous threshold. Future observations will reduce uncertainties and improve long-term trajectory modelling.

Potentially Hazardous Asteroid PHA 363599 (2004 FG11) Close Approach Report and PHA NEO Profile Official Data - Real Time Asteroid News

Astrophyzix Near-Earth Object (NEO) Close Approach Report: 363599 (2004 FG11)  Official Data, Real Time Reporting

Written by: Astrophyzix Digital Observatory

Image Credit: NASA JPL SBDB

2026 Relevance: Illustrates orbital geometry and Earth-approach context for monitored near-Earth objects during the 2026 observation window.

Introduction

A Potentially Hazardous Asteroid (PHA)  is a near-Earth object with an absolute magnitude of 22.0 or brighter (typically larger than ~140 metres) and a minimum orbit intersection distance (MOID) of 0.05 AU or less. This classification does not indicate an impact threat, but identifies objects that require precise orbital monitoring.

Asteroid 363599 (2004 FG11) is a well-studied Apollo-class near-Earth object (NEO) and is formally classified as a Potentially Hazardous Asteroid (PHA). This classification arises from its size and orbital proximity to Earth, specifically its Minimum Orbit Intersection Distance (MOID). The object has been extensively observed since its discovery in 2004, resulting in a highly refined orbital solution with exceptionally low uncertainty.

Notably, (2004 FG11) is a binary system with a confirmed satellite, making it scientifically significant for studies of asteroid mass, density, and internal structure. Its repeated close approaches to Earth make it a key object in long-term planetary defence monitoring.

Key Takeaways

• Binary Apollo-class NEO and Potentially Hazardous Asteroid (PHA).
• Highly reliable orbit (condition code 0) based on 22+ years of observations.
• Estimated diameter: ~152 meters with relatively high albedo (0.306).
• Rotation period: ~7.02 hours.
• Earth MOID: 0.0203 AU (~3.04 million km).
• Regular Earth close approaches approximately every 2 years.
• Next significant Earth approach: 2026-Apr-11 at 0.05652 AU (~8.46 million km).
• No impact risk identified in current orbital solutions.

Scientific Consensus Snapshot

The orbital solution for (2004 FG11) is based on 507 optical observations and radar astrometry spanning over 22 years. The inclusion of radar delay and Doppler measurements significantly enhances orbital precision, resulting in a condition code of 0. This allows for highly accurate forward propagation of the orbit and reliable close-approach predictions.

Asteroid 2006 GC1 Potentially Hazardous Asteroid (PHA) Close Approach 2026 and Asteroid Profile - Astrophyzix Digital Observatory - Official Data Set

Astrophyzix Near-Earth Object (NEO) (PHA) Close Approach Report and Object Profile: Asteroid 2006 GC1 

Written by: Astrophyzix Digital Observatory

Image Credit: NASA JPL SBDB

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Introduction

A Potentially Hazardous Asteroid (PHA)  is a near-Earth object with an absolute magnitude of 22.0 or brighter (typically larger than ~140 metres) and a minimum orbit intersection distance (MOID) of 0.05 AU or less. This classification does not indicate an impact threat, but identifies objects that require precise orbital monitoring.

Asteroid (2006 GC1) is a well-characterised Apollo-class near-Earth object (NEO) and is formally classified as a Potentially Hazardous Asteroid (PHA). This designation is based on its size and its Minimum Orbit Intersection Distance (MOID) with Earth. Unlike recently discovered objects with short observational arcs, (2006 GC1) benefits from a long-term observational dataset spanning over 15 years, resulting in a highly constrained and reliable orbital solution.

This report provides a detailed orbital, physical, and close-approach analysis using data derived from the NASA JPL Small-Body Database and associated dynamical models. All values presented reflect current best-fit solutions and should be interpreted within the context of continuous observational refinement.

Key Takeaways

• (2006 GC1) is classified as both an Apollo NEO and a Potentially Hazardous Asteroid (PHA).

• Extremely well-constrained orbit (condition code 0) based on 92 observations over 15.3 years.

• Highly eccentric orbit (e = 0.817) with a perihelion deep inside Mercury’s orbital region.

• Estimated size range: ~200–400 meters (based on H = 20.5).

• Earth MOID: 0.00914 AU (~1.37 million km), within the PHA threshold.

• Next notable Earth close approach: 2026-Apr-05 at 0.08876 AU (~13.3 million km).

• Relative velocity during Earth encounter: ~30.66 km/s.

• No impact risk indicated for any known approach in current orbital solutions.

Scientific Consensus Snapshot

The orbital solution for (2006 GC1) is derived using high-precision numerical integrations incorporating the DE441 planetary ephemeris and perturbations from major solar system bodies. With a condition code of 0 and a multi-decade observation arc, the orbit is considered highly reliable. Uncertainty margins in orbital elements are extremely low, allowing for precise long-term trajectory propagation and close-approach prediction.

CNEO NEO PHA Asteroid Close Approach Report: 29 March 2026 - 4 April 2026 Official Data

Astrophyzix Near-Earth Object (NEO) Close Approach Report

Written by: Astrophyzix Digital Observatory

Monitoring Window: 29 March – 4 April 2026 (UTC)

Official NEO Data Reporting

This report presents a comprehensive analysis of Near-Earth Object (NEO) activity detected within a 7-day monitoring window using live orbital data from the NASA Center for Near-Earth Object Studies (CNEOS) NeoWs API, integrated via the Astrophyzix Digital Observatory. All objects listed have been evaluated using standard orbital mechanics and observational datasets, alongside the Astrophyzix Risk Index (ARI v2) for comparative educational context.

Potentially Hazardous Asteroid 837253 (2013 FW13) Close Approach 27 March 2026 - Astrophyzix Digital Observatory

Astrophyzix PHA NEO Close Approach Report and Profile: 837253 (2013 FW13)

Written by: Astrophyzix Digital Observatory for Planetary Defence and NEO Reporting

Image Credit: NASA JPL Small Body Database 

What is a Potentially Hazardous Asteroid? 

A Potentially Hazardous Asteroid (PHA)  is a near-Earth object with an absolute magnitude of 22.0 or brighter (typically larger than ~140 metres) and a minimum orbit intersection distance (MOID) of 0.05 AU or less. This classification does not indicate an impact threat, but identifies objects that require precise orbital monitoring.

Close Approach Event — 27 March 2026

Asteroid 837253 (2013 FW13) undergoes a monitored Earth flyby on 27 March 2026 at approximately 02:27 UTC. This event represents a routine, non-hazardous close approach within the broader Near-Earth Object tracking catalogue, with a miss distance that remains comfortably beyond the Earth–Moon system.

Parameter	Value
Close Approach Date	27 March 2026
Time (UTC)	02:27
Nominal Distance	0.17170 au
Distance (km)	~25,685,800 km
Distance (Lunar Distances)	~66.8 LD
Relative Velocity	~19.8 km/s (~71,100 km/h)

Dynamical Interpretation

At a nominal separation of 0.17170 astronomical units, this flyby occurs at approximately 66.8 times the average Earth–Moon distance, placing it far outside the regime typically considered a “close” encounter in planetary defence terms.

Despite its classification as a Potentially Hazardous Asteroid, this designation is based on long-term orbital geometry (MOID and size) rather than immediate encounter conditions. The March 2026 passage represents a distant orbital crossing alignment rather than a near-Earth interaction.

Context Within NEO Monitoring Framework

For comparison, objects typically flagged for heightened observational campaigns during close approaches pass within <10 lunar distances, and in some cases within 1–2 LD. In contrast, 2013 FW13 remains well beyond even the outer boundary of the Earth–Moon system during this event.

The significance of this flyby is therefore observational rather than hazardous. Events at this scale are routinely used to refine orbital solutions, validate dynamical models, and maintain continuity in long-arc tracking datasets.

Asteroid (PHA/NEO) 879537 (2014 AF51) 19 March 2026 Close Approach and Profile by Astrophyzix Digital Observatory

Close Approach Data and Official NEO Profile 
Written by: Astrophyzix Digital Observatory 

📌 Cited by NewsBreak

2026 Close Approach to Earth

Asteroid 879537 (2014 AF51) will make a notable close approach to Earth on 19 March 2026 at 21:10 TDB. This object is classified as an Amor-type Near-Earth Object (NEO) and a Potentially Hazardous Asteroid (PHA), although its orbit remains safely exterior to Earth's path at perihelion, and no impact risk is associated with this encounter.

Parameter	Value	Units
Close Approach Date (TDB)	2026-03-19 21:10	UTC / TDB
Nominal Distance from Earth	0.11658	AU (~17.4 million km)
Relative Velocity	8.94	km/s
Minimum Orbit Intersection Distance (MOID)	0.0222536	AU
Classification	Amor, NEO, PHA	—

Although classified as potentially hazardous due to its size and orbital proximity thresholds, this March 2026 approach occurs at a distance more than 45 times the average Earth–Moon separation, placing it well outside any collision scenario. Its Amor-type orbit ensures that it does not currently cross Earth's orbital path, instead approaching from just beyond 1 AU at perihelion.