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
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Apollo NEO Condition Code 7 Short‑Arc Object  NO IMPACT RISK — See JPL Solution

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

Parameter	Status
Closest approach	2026‑05‑18 21:23 UTC at 0.000611 AU
Nominal miss distance	0.238 LD / 91,500 km
Largest uncertainty	Condition code 7 (47 obs, 5‑day arc)
PHA status	No (H > 22)
Hazard level	Non‑hazardous size; no impact geometry

Asteroid Apophis 2029 Flyby Scientific Report - What NASA JPL Data Says In 2026 - Asteroid News Without the Hype - Updated 14/05/26

Asteroid (99942) Apophis — 2026 NASA-Verified Scientific Status News Report
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 in 15 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]

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.

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.

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

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

Written by: Astrophyzix Digital Observatory

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

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 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

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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 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.

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

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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.

Mid-week Astrophyzix CNEOS Report 23-26 February Powered by NASA - No Impact Risks

Written By: Astrophyzix Science Communication 

 

Astrophyzix Midweek CNEOS Close-Approach Full Report for 23–26 February 2026 Powered by the Official NASA JPL CNEO API

This midweek Near-Earth Object monitoring report summarises confirmed close approaches recorded in NASA/JPL orbital databases for the period 23–26 February 2026. All orbital solutions referenced here are validated entries from the Small-Body Database and represent routine Solar System traffic with no impact risk.

A total of 25 catalogued near-Earth asteroids pass within 100 lunar distances during this reporting window. None are classified as hazardous.