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

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)

Parameter	Status
Closest approach	(2012 HM) at 0.079303 AU
Largest object	374038 (2004 HW) — ~1.56 km
PHA count	2 of 5 objects (YE6, 2004 HW)
Highest ARI score	49 — 374038 (2004 HW)
Hazard level	No immediate threats; all passes are distant

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

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.

• Full scientific data analysis by Astrophyzix can be found here https://www.astrophyzix.com/2026/04/apophis-2029-approach-offical-data.html
• You can use the Astrophyzix Asteroid Lookup tool to view the live NASA data profile of Apophis. 
• See live detailed data, orbital dynamics, flyby countdown and comprehensive data sets using the Astrophyzix Live Apophis Tracker

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.

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.

Near Earth Object NEO Close Approach Report: Asteroid (2026 GD) Updated Solution JPL 2

Astrophyzix Near-Earth Object (NEO) Close Approach Report: (2026 GD) — Updated Solution (JPL 2) - Real Time NEO News

Written by: Astrophyzix Digital Observatory

📌 Cited by DiscoverWildScience 📌 Cited by MSN News 📌 Cited by Bing Copilot News

Image Credit: NASA JPL SBDB

Introduction

Asteroid (2026 GD) is an Apollo-class near-Earth object (NEO) currently undergoing rapid orbital refinement following its recent discovery in April 2026. This report is a follow-up of our initial report and is based on the updated JPL solution (Solution 2), incorporating an expanded observational dataset and improved orbital constraints.

The object is notable for an exceptionally close Earth flyby occurring on April 9, 2026, within lunar distance. Although the orbit remains classified with moderate uncertainty, current data provides a consistent and stable close-approach solution with no indication of impact risk.

Key Takeaways

• Very close Earth approach on 2026-Apr-09 at 22:59 (TBD) at ~0.00168 AU.
• Equivalent to approximately 0.65 lunar distances (~251,000 km).
• Relative velocity: ~12.66 km/s.
• Small object (~20–30 meters estimated diameter).
• Earth MOID: 0.000525 AU (very low orbital intersection distance).
• Orbit refined using 117 observations over 2 days.
• Condition code remains 7 (moderate uncertainty).
• No impact threat identified. 

Scientific Consensus Snapshot

The updated orbital solution reflects improved constraint quality due to an increased number of observations and an extended data arc. While uncertainties have decreased across all orbital parameters, the orbit remains in an early refinement stage. 

Close approach predictions are now more precise, particularly in timing, but continued observation is required to fully stabilise the solution.

Newly Discovered NEO Asteroid (2026 GD) Exclusive Close Approach Report and Object Profile Astrophyzix Digital Observatory NASA Data

Astrophyzix Near-Earth Object (NEO) Close Approach Report: (2026 GD) Newly Discovered Asteroid Will Pass Closer than the Moon. 

Written by: Astrophyzix Digital Observatory

📌 Cited by DiscoverWildScience 📌 Cited by MSN News 📌 Cited by Bing Copilot News

Introduction

New updates found in our JPL Solution 2 Report

Asteroid (2026 GD) is a recently observed Apollo-class near-Earth object (NEO) identified in April 2026. With a short observational arc of just 1 day, its orbital solution remains preliminary and subject to refinement. Despite this, current data indicates an exceptionally close Earth approach occurring on 09 April 2026.

The object’s very low Earth Minimum Orbit Intersection Distance (MOID) and near-term encounter geometry place it within the category of close-approach monitoring priority objects, although no confirmed impact risk is currently established based on available solutions at this time. Astrophyzix will update you as new data comes in. 

Key Takeaways

• Apollo-class near-Earth asteroid with Earth-crossing orbit.
• Very close Earth approach on 2026-Apr-09 at ~0.00168 AU.
• Equivalent to approximately 0.65 lunar distances (~251,000 km).
• Estimated relative velocity: ~12.66 km/s.
• Small object (~20–30 meters estimated diameter range).
• Extremely low Earth MOID: 0.000525 AU.
• Orbit uncertainty remains high (condition code 7).
• No confirmed impact risk in current datasets at the time of this report. 

Scientific Consensus Snapshot

The orbital parameters for (2026 GD) are based on a limited observational dataset spanning approximately one day. As a result, uncertainties remain significant, reflected in its condition code of 7. (Explanation of Code 7 below) 

Additional observations are required to refine its trajectory and reduce positional uncertainty. Close-approach predictions at this stage should be treated as provisional.

Near Earth Object NEO Close Approach Report April 07–13, 2026 Official Data

Astrophyzix Near-Earth Object (NEO) Close Approach Report: April 07–13, 2026. Real Time Asteroid News

Written by: Astrophyzix Digital Observatory

Introduction

This report summarises near-Earth object (NEO) activity during the monitoring window of April 07–13, 2026, based on live data from NASA’s CNEOS NeoWs API. A total of 66 objects are tracked within this interval, including 4 classified as Potentially Hazardous Asteroids (PHAs).

The dataset reflects real-time orbital solutions and close-approach predictions. While multiple objects pass within lunar-distance scales, all currently known trajectories indicate no impact threat. The Astrophyzix Risk Index® (ARI) is included as an internal comparative metric and does not represent official hazard classification.

Key Takeaways (Data correct at time of publication)

• Total monitored NEOs: 66
• Potentially Hazardous Asteroids (PHA): 4
• Objects passing within 10 lunar distances: 4
• Closest approach: (2011 FT9) at 3.437 LD
• Average relative velocity: 13.3 km/s
• Largest object: 302831 (2003 FH) at ~645 meters
• No confirmed impact risks identified

Scientific Consensus Snapshot

All orbital predictions are derived from NASA CNEOS datasets and are continuously refined through optical and radar tracking. Close approach distances are calculated using numerical integration models incorporating gravitational perturbations from major planetary bodies. 

Objects classified as PHAs meet defined thresholds for size and Earth MOID but do not imply imminent impact.

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

📌 Referenced by iAsk Student

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.

Near Earth Object (NEO) Close Approach Report: Asteroid 2026 FB6 Official Data Profile - Latest Asteroid News

Astrophyzix Near-Earth Object (NEO) Close Approach Report: 2026 FB6 - Real Time, Trusted Asteroid News 

Written by: Astrophyzix Digital Observatory 

📌 Referenced by iAsk Student

Introduction

This report presents an institutional summary of near-Earth asteroid 2026 FB6, an Apollo-class near-Earth object (NEO) with a trajectory that intersects Earth's orbital path. The analysis is based on orbital data derived from NASA’s JPL Small-Body Database and ephemerides generated using JPL dynamical models and planetary perturbation integrations.

Due to the limited observational arc and associated high condition code, orbital parameters remain uncertain and subject to refinement through continued astrometric tracking.

Key Takeaways (ADO) 

• 2026 FB6 is classified as an Apollo-type near-Earth asteroid.
• Semi-major axis: 1.658 AU, indicating an orbit extending well beyond Earth’s orbit.
• Eccentricity: 0.398, representing a moderately elongated orbit.
• Perihelion distance: 0.999 AU, near Earth’s orbital distance.
• Earth MOID: 0.0141 AU (~2.1 million km), indicating a relatively safe orbital separation.
• Absolute magnitude (H): 27.82, implying a small object (tens of meters in diameter, size dependent on albedo).
• Observational arc: 5 days with 17 observations; condition code: 9 (high uncertainty).
• Predicted close approach: 2026-Apr-04 03:48 TDB (±2 minutes).

Scientific Consensus Snapshot

Orbital solutions for 2026 FB6 are computed using heliocentric dynamics referenced to the JPL DE441 planetary ephemeris. The solution incorporates gravitational perturbations from major planetary bodies and is constrained by a limited observational dataset spanning five days. The high condition code indicates that additional observations are required to significantly reduce uncertainties in the orbital solution.

Near Earth Object (NEO) Close Approach Report Asteroid 2026 FF7 Official Data - Real Time NEO News

Astrophyzix Near-Earth Object (NEO) Close Approach Report: Asteroid 2026 FF7 - Credible Planetary Defence News

Written by: Astrophyzix Digital Observatory 

📌 Referenced by iAsk Student

Introduction

This report summarizes the orbital characteristics and Earth close-approach context for the near-Earth asteroid 2026 FF7, an Apollo-class object classified as a near-Earth object (NEO). The analysis is derived from publicly available data provided by the NASA JPL Small-Body Database and associated ephemerides generated through NASA and JPL orbital computation systems operated by the Jet Propulsion Laboratory.

The dataset reflects a short observational arc and therefore carries significant orbital uncertainty. As such, all derived predictions should be interpreted within the context of ongoing refinement through additional astrometric observations.

Key Takeaways (ADO) 

• 2026 FF7 is classified as an Apollo-type near-Earth asteroid with an Earth-crossing orbit.
• Estimated semi-major axis: 1.236 AU, indicating an orbit extending beyond Earth's orbital path.
• Orbital eccentricity of ~0.418 suggests a moderately elongated trajectory.
• Perihelion distance: 0.720 AU; aphelion distance: 1.753 AU.
• Earth MOID: 0.00494 AU (~739,000 km), indicating a potentially close orbital intersection.
• Absolute magnitude (H): 27.47, implying a small object on the order of tens of meters in diameter (size estimate dependent on albedo assumptions).
• Observational arc is limited to 2 days with 14 observations, resulting in a high condition code (9), indicating substantial orbital uncertainty.

Scientific Consensus Snapshot (ADO) 

Orbital parameters for 2026 FF7 are computed using heliocentric reference frames and the JPL DE441 planetary ephemeris. The solution is based on a limited observational dataset and therefore exhibits elevated uncertainty. Continuous follow-up observations are required to reduce uncertainties in orbital elements such as semi-major axis, eccentricity, and mean anomaly.

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.

EXCLUSIVE NEO REPORT: Newly Discovered NEO Asteroid 2026 FG6 and it's Current Close Approach March 2026

Exclusive Report: Asteroid 2026 FG6 (SPK-ID 54606975) Newly Discovered Near-Earth Object Which Was Discovered Just Two Days Before it's Close Approach

Written by: Astrophyzix Digital Observatory

Published on: 27 March 2026

📌 Cited by iAsk Student

Image Credit: NASA JPL SBD

Introduction (Latest update here) 

2026 FG6 (SPK-ID 54606975) is an Apollo-class Near-Earth Object (NEO) recently discovered on March 25, 2026 by automated surveys cataloged by JPL’s Solar System Dynamics team. This asteroid was identified following routine scanning of near-Earth space, and its extremely small Earth Minimum Orbit Intersection Distance (MOID) immediately marked it as noteworthy. Observations over just two days have provided preliminary orbital data, though with high uncertainty (Condition Code 7), emphasizing the need for continued tracking to refine its orbit and assess any potential hazard.

Despite its short observation arc, 2026 FG6’s Earth MOID of 0.00045 au (~67,000 km) makes it one of the closest-passing NEOs identified in recent weeks. Its absolute magnitude of H = 27.369 suggests a very small object, likely only a few meters in diameter, but its proximity highlights the importance of rapid follow-up for newly discovered NEOs. - It poses no impact risk.

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.

NEO Close Approach Report 24-27 March 2026: Astrophyzix Digital Observatory NEO Monitoring

25 Asteroids Are Flying Past Earth This Week  Here's What NASA's Data Actually Tells Us

NEO Close Approach Report | March 24–27, 2026

By Astrophyzix Digital Observatory | Published March 24, 2026

Introduction 

Twenty-five near-Earth objects will make close approaches to our planet between March 24 and March 27, according to live data from NASA's Center for Near Earth Object Studies. The vast majority pose no threat whatsoever — but three carry a formal hazard classification, and one will pass closer to Earth than almost anything we've tracked in recent memory.

Here is what the numbers actually mean. 

The Closest One: A Six-Metre Pebble

The object arriving first and nearest is (2026 FM3), due to pass on March 25 at a distance of just 0.62 lunar distances — roughly 238,000 kilometres, barely farther than the Moon itself. 

• It is travelling at 5.44 km/s and is estimated to be around six metres across: roughly the size of a large van. It carries no hazard classification. At that size, even if it were somehow on an impact trajectory, it would almost certainly burn up in the atmosphere before reaching the ground.

Close behind it, (2026 FB4) passes on March 26 at 1.69 LD, followed by (2026 FX3) and (2026 FT2) on the 24th at 2.99 and 4.13 LD respectively. All are small, all are fast, and none are considered dangerous.

Asteroids Approaching Earth This Week: NEO PHA Close Approach Report 20-23 March 2026

Astrophyzix Digital Observatory

Near-Earth Object (NEO) Close Approach Report

Observation Window: 20–23 March 2026

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Executive Summary

During the monitoring period spanning 20–23 March 2026, a total of 25 Near-Earth Objects (NEOs) are recorded making close approaches to Earth within a range of 1.54 to 59.76 Lunar Distances (LD).

• Closest approach: 2026 FU at 1.54 LD
• Largest object: (2018 YU) at ~444 m diameter
• Highest velocity: 2022 SR2 at 24.33 km/s
• Potentially Hazardous Objects (PHAs): 2 identified
• Impact risk: None detected

All objects remain well within safe margins with no impact probabilities identified by current orbital solutions.

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.

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

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).

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Astrophyzix Digital Observatory NEO Asteroid Close Approach Report 13-16 March 2026 - Official Data

Written by: Astrophyzix Digital Observatory

Near-Earth Object Close Approach Report — 13–16 March 2026

📌 Cited by Innovatopia News

Your Reliable Weekly NEO Report 

The following Near-Earth Object (NEO) monitoring report summarises asteroid flybys occurring between 13 March and 16 March 2026. Data is compiled from the NASA Jet Propulsion Laboratory Small-Body Database and associated planetary defence monitoring systems.

Distances are expressed in Lunar Distances (LD), where 1 LD = 384,400 km. This unit provides an intuitive scale for evaluating asteroid flybys relative to the Earth–Moon system.

During this monitoring interval 25 catalogued Near-Earth Objects make relatively close approaches to Earth. None of the objects present any impact risk. Several larger asteroids are formally classified as Potentially Hazardous Asteroids (PHAs), however all remain safely tens of lunar distances from Earth.

Close Approach Series. 04 March 2026 CNEO REPORT - Official NASA Data

MONITORING ACTIVE

Written By Astrophyzix Digital Observatory and Planetary Defence Research 

Near‑Earth Object Report – Week of March 4, 2026

Near‑Earth objects (NEOs) — asteroids and comets whose orbits bring them into the Earth’s orbital neighborhood — remain a central focus of planetary science and defense. This report synthesizes the latest state of the NEO population, recent close approaches, tracking and discovery statistics, risk assessment frameworks, observational campaigns, and planetary defense strategies as of early March 2026. All figures and operational descriptions derive from official NASA science and NASA Jet Propulsion Laboratory (JPL) data streams.

Potentially Hazardous Asteroid 2011 WV134 (500080) Close Approach Planetary Defence Profile

MONITORING ACTIVE

Written by: Astrophyzix Digital Observatory and Planetary Defence Research centre
Image: Copyright © Astrophyzix Science Network

Discovery & Designation

(500080) 2011 WV134 is a numbered near-Earth asteroid (NEA) first detected on 30 November 2011 by the Catalina Sky Survey, a NASA-funded asteroid detection program based in Arizona. Following confirmation and orbital refinement, the object received its permanent minor planet number 500080 from the International Astronomical Union Minor Planet Center (MPC).

The asteroid’s provisional designation “2011 WV134” follows the standard MPC naming convention, indicating discovery in the second half of November 2011.