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Wednesday, 22 April 2026

Weekly Potentially Hazardous Asteroid and NEO Close Approach Report 22 April to 28 April Official 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

Closest Approach Analysis — (2026 HL2)

ParameterValue
Approach Date2026-04-22
Miss Distance2.956 LD
Estimated Diameter7 m
Velocity5.47 km/s
ARI Score34
ClassificationNEO
Hazard StatusNot Hazardous



(2026 HL2 represents the minimum-distance encounter within the current monitoring window. At a separation of 2.956 lunar distances, the object remains well outside Earth's gravitational capture threshold for impact scenarios under nominal orbital conditions.


Its estimated diameter of 7 metres places it within the lower end of the size-frequency distribution of near-Earth objects.


No impact solution or Earth-intersecting trajectory is indicated in the source dataset.


Potentially Hazardous Asteroids (PHA)

Object Date Miss Distance (LD) Velocity (km/s) Size (m) ARI
(2026 BK2)2026-04-229.9998.1326550
(2004 PJ2)2026-04-2226.2576.2920937
612786 (2004 PJ2)2026-04-2226.2576.2922038
(2026 FH12)2026-04-2854.15514.3318739
434196 (2003 HG2)2026-04-2259.51410.1921039
(2004 KB)2026-04-2470.36112.1324941

All PHAs listed meet standard classification thresholds (absolute magnitude and minimum orbit intersection distance).


However, none of the objects listed exhibit Earth-impact solutions within this monitoring window based strictly on the provided data.

Sub-10 Lunar Distance Objects

Object Date Distance (LD) Velocity (km/s) Size (m) ARI
(2026 HL2)2026-04-222.9565.47734
(2026 HY1)2026-04-223.9029.292734
(2026 GL2)2026-04-227.08010.403927
(2022 UU8)2026-04-258.6974.041119
(2026 HW)2026-04-289.53411.784324
(2026 BK2)2026-04-229.9998.1326550

High-Mass / Large Diameter Objects

Object Date Size (m) Distance (LD) Velocity (km/s)
54071 (2000 GQ146)2026-04-22141861.39513.36
88710 (2001 SL9)2026-04-26129377.63714.79

Orbital Behaviour & Distribution

All listed objects fall under the Near-Earth Object classification. No additional orbital subclass (Apollo, Aten, Amor) is explicitly provided within the supplied dataset and therefore is not inferred.


Velocity distribution across the dataset ranges from 4.04 km/s to 19.84 km/s. No anomalous velocity outliers beyond expected heliocentric encounter ranges are identified.

Planetary Defence Context

The presence of eight PHAs within the monitoring window reflects classification thresholds rather than immediate risk.


PHA designation does not imply collision probability; it indicates objects that warrant continued tracking due to size and orbit.


No deviation from predicted orbital paths is present in the dataset. All trajectories remain consistent with established solutions derived from current observational arcs.

Scientific Notes

Sources

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