Mission Control/WAR.GOV/UFO PURSUE ARCHIVE & CNEOS CORRELATION ENGINE
GEMMA ENGINE: LOCAL SERVER BOX [ACTIVE]war.gov/ufoaaro.milarchives.gov/uaps
2026 DOD / AARO / NARA PURSUE TRANCHES 01–06200 NASA CNEOS BOLIDE & TLE SHELL CROSS-CORRELATIONDUAL IMPERIAL (FT / MI / MPH) & METRIC (M / KM / KM/S)

2026 war.gov/ufo PURSUE Releases 01–06 & AARO Multi-Sensor UAP Correlation Engine

Meteors.ai ingests all 6 official 2026 Department of Defense (war.gov/ufo), AARO (aaro.mil), and National Archives (archives.gov/research/topics/uaps) PURSUE releases and correlates every multi-sensor track against 200 NASA JPL CNEOS atmospheric fireballs and NORAD satellite TLE shells. Field investigators and skywatchers can verify orbital glints, stratospheric bolides, and low-altitude tracks using 15x70 astronomy binoculars[↗], a plate-solved smart telescope[↗], an all-sky meteor camera[↗], an ADS-B receiver[↗], and an RTK GPS module[↗].

PURSUE Tranches
6 Releases
May – Sep 2026 Archive
Multi-Sensor Cases
8 / 8 Tracks
Radar • IR • 70mm Film
CNEOS Reference
200 Bolides
JPL SSD Vector Catalog
Altitude Envelope
50 ft – 71,458 mi
15 m – 115,000 km

OFFICIAL 2026 DOD / AARO / NARA PURSUE RELEASE TRANCHES (RELEASE_01 – RELEASE_06)

Primary Repositories: war.gov/ufo • aaro.mil • archives.gov/research/topics/uaps
RELEASE_012026-05-08

PURSUE Release 01 — Historic Spaceflight & Orbital Anomaly Photography (Gemini VII & Apollo 17 Archive)

High-resolution 4K densitometric scans of original 70mm Hasselblad spaceflight magazines from Gemini VII (1965) at 301 km (187 mi / 987,500 ft) LEO and Apollo 17 (1972) at 115,000 km (71,458 mi) cislunar coast, cross-examined against NORAD space catalog TLEs and thruster plume photometry.

Record Group: NARA RG 255 & RG 615 (NASA & AARO Declassified Spaceflight Film)
RELEASE_022026-06-05

PURSUE Release 02 — CENTCOM MQ-9 Reaper EO/IR Metallic Orb & Multi-Sensor Tracks

Declassified USCENTCOM MQ-9 Reaper electro-optical and mid-wave infrared (MX-20 EO/IR) full-motion video telemetry documenting spherical metallic orbs operating at 4,572 m (15,000 ft / 4.57 km / 2.84 mi) and 380 mph (0.17 km/s) without thermal exhaust signatures.

Record Group: NARA RG 615 (AARO Declassified ISR Telemetry)
RELEASE_032026-07-02

PURSUE Release 03 — Maritime Carrier Strike Group Radar-IR Correlated Tracks (USS Nimitz & East Coast Range)

Consolidated Cooperative Engagement Capability (CEC) AN/SPY-1B phased-array radar plots and F/A-18F Super Hornet AN/ASQ-228 ATFLIR infrared tracks from Carrier Strike Group 11, including rapid non-ballistic descents from 24,384 m (80,000 ft / 15.15 mi) to 15 m (50 ft) at 18,000+ mph (8.05 km/s).

Record Group: NARA RG 38 & RG 615 (Naval Aviation & CEC Radar Logs)
RELEASE_042026-08-01

PURSUE Release 04 — DHS / CBP Thermal Transmedium & Coastal Airspace Telemetry (Aguadilla & Southern Border)

Calibrated L-3 WESCAM MX-15D 3–5 μm thermal imaging and maritime surveillance radar logs from DHS/CBP DHC-8 patrols capturing low-altitude 365 m (1,200 ft / 0.365 km / 0.23 mi) transmedium coastal trajectories at 95 mph (0.042 km/s).

Record Group: NARA RG 563 & RG 615 (DHS Air and Marine Operations)
RELEASE_052026-08-28

PURSUE Release 05 — DoW PR-134 Declassified Multi-Sensor Cases & FBI FD-302 Linear Craft Witness/Radar Filings

Joint DoW PR-134 stratospheric fast-mover telemetry at 18,288 m (60,000 ft / 18.29 km / 11.36 mi) and 4,250 mph (1.90 km/s) alongside declassified FBI FD-302 commercial/military aircrew primary radar intercepts of 45.7 m (150 ft) linear craft at 10,972 m (36,000 ft).

Record Group: NARA RG 65 & RG 615 (FBI FD-302 Aviation Filings & DoW PR-134)
RELEASE_062026-09-18

PURSUE Release 06 — NARA RG 341 Project Blue Book Photogrammetry Re-Digitization (Tremonton Navy Film & High-Altitude Tracks)

Optical micro-densitometry and frame-by-frame 35mm photogrammetry re-digitizations from NARA Record Group 341, featuring Chief Photographer Delbert Newhouse’s 1952 Tremonton, Utah 16mm daylight formation film at 3,658 m (12,000 ft / 3.66 km / 2.27 mi).

Record Group: NARA Record Group 341 (Headquarters USAF / Project Blue Book)

MULTI-SENSOR UAP TRACK DOSSIERS & NASA CNEOS CORRELATION (8 DISPLAYED)

All Telemetry Readouts Shown in Dual Imperial (ft / mi / mph) & Metric (m / km / km/s)
RELEASE_01CASE ID: pursue-r1-gemini-vii-1965DATE: 1965-12-04COORDS: (28.5°, -80.6°)

Gemini VII Orbital Cylindrical Object & Thruster Plume Correlation

Low Earth Orbit over Cape Canaveral / Western Atlantic Sector • NARA RG 255 / NASA Magazine 29-B Frames S65-63722 & S65-63723

Altitude (Imperial & Metric)
301 km / 187 mi (301,000 m / 987,500 ft)
987,500 ft (187 mi) / 301,000 m (301 km)
Estimated Speed (mph & km/s)
17,023 mph / 7.61 km/s (Mach 22.2 Orbital)
17,023 mph / 7.61 km/s (Mach 22.2)
Target Size (ft & m)
25 ft / 7.6 m
Primary Sensor: Hasselblad 70mm Orbital Film
Nearest CNEOS Bolide Distance (mi & km)
624 km / 387.7 mi
Sensor Modalities:Hasselblad 70mm Orbital Film35mm PhotogrammetryNORAD Space Surveillance Radar

During Revolution 3 of the Gemini VII mission on December 4, 1965, Command Pilot Frank Borman and Pilot Jim Lovell photographed a cylindrical metallic-albedo object accompanied by a luminous multi-lobed plume at 301 km (187 mi / 987,500 ft) altitude and 17,023 mph (7.61 km/s). PURSUE Release 01 provides 4K micro-densitometric scans of the original Hasselblad 70mm Orbital Film paired with NORAD Space Surveillance Radar two-line element (TLE) reconstructions. Observers tracking low-Earth orbital cylinders, upper-stage boosters, and bright LEO passes can resolve magnitude +2.5 to +6.0 targets using 15x70 astronomy binoculars[↗] or a plate-solved smart telescope[↗] with satellite ephemeris tracking.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Titan II GLV-4 Upper Stage Booster Shell (295–305 km / 183–190 mi LEO, 28.87° inc.)
CNEOS Bolide Match Probability4%
TLE Satellite Flare Likelihood78%
Kinematic Anomaly Score34 / 100

Local Gemma (tier1-local-server-gemma) cross-correlation against 200 NASA CNEOS fireballs rules out atmospheric bolide ablation (4% match) because the 301 km (187 mi / 987,500 ft) track lies 260+ km above the stratospheric airburst zone. TLE orbital propagation shows a 78% match to specular solar reflection off the venting Titan II GLV-4 second stage (7.6 m / 25 ft at 17,023 mph / 7.61 km/s), with a 34/100 kinematic anomaly residual from asymmetric plume photometry. Nearest cataloged NASA CNEOS bolide is cneos-fb-07 (624 km / 387.7 mi great-circle separation).

RELEASE_01CASE ID: pursue-r1-apollo-17-1972DATE: 1972-12-12COORDS: (0.7°, 23.5°)

Apollo 17 Cislunar Trans-Earth Frame AS17-147-22470 Photometric Anomaly

Cislunar Trans-Earth Injection Corridor (Sub-Satellite 0.7°N, 23.5°E) • NARA RG 255 / NASA Apollo 17 Magazine 147-JJ Frame AS17-147-22470

Altitude (Imperial & Metric)
115,000 km / 71,458 mi (115,000,000 m / 377,296,588 ft)
377,296,588 ft (71458 mi) / 115,000,000 m (115000 km)
Estimated Speed (mph & km/s)
4,877 mph / 2.18 km/s (Cislunar Trans-Earth Coast)
4,877 mph / 2.18 km/s (Mach 6.36)
Target Size (ft & m)
40 ft / 12.2 m
Primary Sensor: Hasselblad 70mm Orbital Film
Nearest CNEOS Bolide Distance (mi & km)
1,800.1 km / 1,118.5 mi
Sensor Modalities:Hasselblad 70mm Orbital Film35mm PhotogrammetryDeep-Space S-Band Doppler Telemetry

Captured during Apollo 17 trans-Earth coast on December 12, 1972 at a cislunar altitude of 115,000 km (71,458 mi / 377,296,588 ft), frame AS17-147-22470 records a structured high-contrast specular anomaly against the blackness of deep space. PURSUE Release 01 pairs 35mm Photogrammetry and Hasselblad 70mm Orbital Film grain analysis to separate hardware reflections from emulsion artifacts. Deep-sky cislunar hardware and high-altitude NEOs between magnitude +11 and +15 require a plate-solved smart telescope[↗] with live-stacking CMOS photometry and a light pollution filter[↗].

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Saturn IVB-512 / Spacecraft-LM Adapter (SLA) Cislunar Drift Corridor (110,000–120,000 km / 68,350–74,565 mi)
CNEOS Bolide Match Probability2%
TLE Satellite Flare Likelihood68%
Kinematic Anomaly Score41 / 100

Local Gemma (tier1-local-server-gemma) confirms near-zero CNEOS atmospheric bolide probability (2%) at 115,000 km (71,458 mi) cislunar altitude. Photometric phase-angle modeling yields a 68% match to a tumbling Spacecraft-LM Adapter (SLA) panel or Saturn IVB stage reflection at 4,877 mph (2.18 km/s), with a 41/100 anomaly score due to off-plane ejection geometry. Nearest cataloged NASA CNEOS bolide is cneos-fb-174 (1,800.1 km / 1,118.5 mi great-circle separation).

RELEASE_05CASE ID: pursue-r5-dow-uap-pr134-2025DATE: 2025-11-14COORDS: (32.9°, -117.4°)

DoW PR-134 High-Altitude Multi-Sensor Fast-Mover Track

Southern California Offshore Warning Area W-291 (San Diego Range) • NARA RG 615 / DoW PR-134 Multi-Sensor Case File

Altitude (Imperial & Metric)
18,288 m / 60,000 ft (18.29 km / 11.36 mi)
60,000 ft (11.36 mi) / 18,288 m (18.29 km)
Estimated Speed (mph & km/s)
4,250 mph / 1.90 km/s (Mach 5.54 Hypersonic)
4,250 mph / 1.9 km/s (Mach 5.54)
Target Size (ft & m)
30 ft / 9.1 m
Primary Sensor: AN/SPY-1B Radar
Nearest CNEOS Bolide Distance (mi & km)
407.8 km / 253.4 mi
Sensor Modalities:AN/SPY-1B RadarATFLIR IRMX-20 EO/IR

Declassified under PURSUE Release 05 (DoW PR-134), this November 14, 2025 multi-sensor intercept off San Diego, California correlated shipboard AN/SPY-1B Radar tracks with airborne ATFLIR IR and MX-20 EO/IR locks on a 9.1 m (30 ft) fast-mover maintaining level stratospheric flight at 18,288 m (60,000 ft / 18.29 km / 11.36 mi) and 4,250 mph (1.90 km/s / Mach 5.54). High-altitude stratospheric fast-movers and grazing bolides along coastal ranges are monitored using an all-sky meteor camera[↗] paired with an ADS-B receiver[↗] and SDR receiver[↗] for transponder exclusion.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Below Orbital LEO Perigee (18.29 km / 11.36 mi / 60,000 ft Stratospheric Corridor — Non-Satellite)
CNEOS Bolide Match Probability12%
TLE Satellite Flare Likelihood6%
Kinematic Anomaly Score91 / 100

Local Gemma (tier1-local-server-gemma) evaluates a 12% CNEOS bolide match and 6% TLE satellite flare likelihood. Although 18,288 m (60,000 ft / 18.29 km) intersects the lower CNEOS airburst stratum, the object’s level flight path and 4,250 mph (1.90 km/s / Mach 5.54) velocity—well below Earth escape speed (11.2 km/s / 25,054 mph) yet lacking thermal plume on ATFLIR IR and MX-20 EO/IR—yields a 91/100 kinematic anomaly score. Nearest cataloged NASA CNEOS bolide is cneos-fb-124 (407.8 km / 253.4 mi great-circle separation).

RELEASE_05CASE ID: pursue-r5-fbi-302-linear-craftDATE: 2025-04-19COORDS: (35°, -106.6°)

FBI FD-302 Declassified Linear Craft / Aircrew Primary Radar Intercept

Albuquerque ARTCC High-Altitude Corridor, New Mexico • NARA RG 65 & RG 615 / FBI FD-302 Aviation Witness & Radar Dossier

Altitude (Imperial & Metric)
10,972 m / 36,000 ft (10.97 km / 6.82 mi)
36,000 ft (6.82 mi) / 10,972 m (10.97 km)
Estimated Speed (mph & km/s)
1,840 mph / 0.82 km/s (Mach 2.40 Supersonic)
1,840 mph / 0.82 km/s (Mach 2.4)
Target Size (ft & m)
150 ft / 45.7 m
Primary Sensor: AN/SPY-1B Radar
Nearest CNEOS Bolide Distance (mi & km)
312.4 km / 194.1 mi
Sensor Modalities:AN/SPY-1B RadarATFLIR IRFAA ARSR-4 Long-Range Primary Radar

Released in PURSUE Tranche 05, this declassified FBI FD-302 aviation investigation documents a April 19, 2025 commercial and military aircrew visual encounter corroborated by FAA ARSR-4 primary radar and defensive AN/SPY-1B Radar / ATFLIR IR telemetry over New Mexico (35.0°N, -106.6°W). Multiple flight crews reported a 45.7 m (150 ft) matte-gray linear craft crossing at 10,972 m (36,000 ft / 10.97 km / 6.82 mi) and 1,840 mph (0.82 km/s / Mach 2.40). Flight crews and ground skywatchers cross-verifying high-altitude linear tracks against civil traffic should pair 15x70 astronomy binoculars[↗] with a dual-band ADS-B receiver[↗] and RTK GPS module[↗].

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Starlink V2 Mini 53° Shell Specular Flare Ruled Out by Primary Radar Range Lock at 10.97 km (6.82 mi / 36,000 ft)
CNEOS Bolide Match Probability5%
TLE Satellite Flare Likelihood9%
Kinematic Anomaly Score86 / 100

Local Gemma (tier1-local-server-gemma) rules out Starlink V2 Mini satellite train flares (9% likelihood) and CNEOS meteoroid fireballs (5% probability) because primary ARSR-4 and AN/SPY-1B Radar locked trueslant range at 10,972 m (36,000 ft / 10.97 km / 6.82 mi). The 45.7 m (150 ft) linear airframe moving at 1,840 mph (0.82 km/s / Mach 2.40) registers an 86/100 kinematic anomaly score. Nearest cataloged NASA CNEOS bolide is cneos-fb-125 (312.4 km / 194.1 mi great-circle separation).

RELEASE_02CASE ID: pursue-r2-mq9-persian-gulfDATE: 2022-07-12COORDS: (26.2°, 51.5°)

AARO Middle East MQ-9 Reaper Spherical Metallic Orb EO/IR Track

Persian Gulf / USCENTCOM Maritime Overwatch Corridor • NARA RG 615 / AARO USCENTCOM Declassified Case 2022-ME-01

Altitude (Imperial & Metric)
4,572 m / 15,000 ft (4.57 km / 2.84 mi)
15,000 ft (2.84 mi) / 4,572 m (4.57 km)
Estimated Speed (mph & km/s)
380 mph / 0.17 km/s (Mach 0.50 Subsonic)
380 mph / 0.17 km/s (Mach 0.5)
Target Size (ft & m)
4 ft / 1.2 m
Primary Sensor: MX-20 EO/IR
Nearest CNEOS Bolide Distance (mi & km)
1,118 km / 694.7 mi
Sensor Modalities:MX-20 EO/IRWESCAM MX-15D ThermalMulti-Spectral Laser Rangefinder

Formally cataloged in PURSUE Release 02 by DoD AARO and USCENTCOM, an MQ-9 Reaper ISR platform tracked a 1.2 m (4 ft) specular metallic sphere across the Persian Gulf (26.2°N, 51.5°E) at 4,572 m (15,000 ft / 4.57 km / 2.84 mi) and 380 mph (0.17 km/s / Mach 0.50) using a gimbaled MX-20 EO/IR turret and WESCAM MX-15D Thermal sensor. Low-altitude daytime metallic spheres and anomalous UAV targets are best resolved with high-contrast 10x50 binoculars[↗], an ADS-B receiver[↗], and an RTK GPS module[↗] for azimuth-elevation logging.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Tropospheric 4.57 km (2.84 mi / 15,000 ft) Look-Down Geometry — Zero Orbital TLE Conjunction
CNEOS Bolide Match Probability1%
TLE Satellite Flare Likelihood2%
Kinematic Anomaly Score84 / 100

Local Gemma (tier1-local-server-gemma) assigns a 1% CNEOS bolide probability and 2% TLE flare likelihood because the MQ-9 Reaper MX-20 EO/IR turret tracked the 1.2 m (4 ft) sphere in a nadir look-down orientation against the Earth’s surface at 4,572 m (15,000 ft / 4.57 km / 2.84 mi) and 380 mph (0.17 km/s), yielding an 84/100 kinematic anomaly score. Nearest cataloged NASA CNEOS bolide is cneos-fb-035 (1,118 km / 694.7 mi great-circle separation).

RELEASE_06CASE ID: pursue-r6-tremonton-navy-filmDATE: 1952-07-02COORDS: (41.71°, -112.16°)

Tremonton, Utah Navy Photographer Delbert Newhouse 16mm Formation Track

Tremonton / Great Salt Lake Basin, Box Elder County, Utah • NARA Record Group 341 (Project Blue Book Case #1699 Photogrammetry)

Altitude (Imperial & Metric)
3,658 m / 12,000 ft (3.66 km / 2.27 mi)
12,000 ft (2.27 mi) / 3,658 m (3.66 km)
Estimated Speed (mph & km/s)
760 mph / 0.34 km/s (Mach 1.00 Transonic)
760 mph / 0.34 km/s (Mach 1)
Target Size (ft & m)
10 ft / 3 m
Primary Sensor: 35mm Photogrammetry
Nearest CNEOS Bolide Distance (mi & km)
746.1 km / 463.6 mi
Sensor Modalities:35mm PhotogrammetryBell & Howell 16mm Telephoto FilmNARA RG 341 Densitometry

Re-digitized at 8K resolution in PURSUE Release 06 from NARA Record Group 341, U.S. Navy Warrant Officer and Chief Photographer Delbert C. Newhouse filmed 12–14 bright self-luminous or specular discoid objects maneuvering in formation over Tremonton, Utah (41.71°N, -112.16°W) on July 2, 1952 using a Bell & Howell 16mm camera with a 3-inch telephoto lens. Daylight and twilight high-albedo formation targets at 3,658 m (12,000 ft) can be tracked with tripod-mounted 15x70 astronomy binoculars[↗] or a smart telescope[↗] operating in solar-safe / high-shutter tracking mode.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Pre-Sputnik Historical Epoch (1952-07-02) — Zero Artificial Earth Satellites in Orbit
CNEOS Bolide Match Probability3%
TLE Satellite Flare Likelihood0%
Kinematic Anomaly Score79 / 100

Local Gemma (tier1-local-server-gemma) assigns 0% satellite flare likelihood (filmed July 2, 1952—over five years before Sputnik 1) and 3% CNEOS bolide match probability due to 70+ seconds of non-linear multi-object reversals. NARA RG 341 35mm Photogrammetry at 3,658 m (12,000 ft / 3.66 km / 2.27 mi) and 760 mph (0.34 km/s) yields a 79/100 kinematic anomaly score. Nearest cataloged NASA CNEOS bolide is cneos-fb-04 (746.1 km / 463.6 mi great-circle separation).

RELEASE_03CASE ID: uss-nimitz-tic-tac-2004DATE: 2004-11-14COORDS: (31.2°, -118.4°)

USS Nimitz Carrier Strike Group 11 "Tic-Tac" AN/SPY-1B + F/A-18F ATFLIR Intercept

SOCAL Offshore Operating Area (60–100 mi SW of San Diego / Catalina) • NARA RG 38 & RG 615 / DoD AARO CSG-11 Nimitz-Princeton Case File

Altitude (Imperial & Metric)
24,384 m -> 15 m / 80,000 ft -> 50 ft (24.38 km -> 0.015 km / 15.15 mi -> 0.009 mi)
80,000 ft (15.15 mi) / 24,384 m (24.38 km)
Estimated Speed (mph & km/s)
18,000+ mph / 8.05 km/s (Mach 23.47 Rapid Vertical Descent)
18,000 mph / 8.05 km/s (Mach 23.47)
Target Size (ft & m)
46 ft / 14 m
Primary Sensor: AN/SPY-1B Radar
Nearest CNEOS Bolide Distance (mi & km)
486.9 km / 302.5 mi
Sensor Modalities:AN/SPY-1B RadarATFLIR IRE-2C Hawkeye APS-145 Radar

Benchmark multi-sensor case in PURSUE Release 03: on November 14, 2004, USS Princeton (CG-59) AN/SPY-1B phased-array radar, E-2C Hawkeye radar, F/A-18F visual aircrews (CDR David Fravor & LCDR Alex Dietrich), and AN/ASQ-228 ATFLIR IR pods tracked a 14 m (46 ft) white oblong "Tic-Tac" craft dropping from 24,384 m (80,000 ft / 24.38 km / 15.15 mi) to 15 m (50 ft) above the Pacific Ocean in 0.78 seconds (18,000+ mph / 8.05 km/s / Mach 23.47). Maritime horizon and high-altitude aerospace tracking benefits from stabilized 15x70 astronomy binoculars[↗], an all-sky meteor camera[↗], and an SDR receiver[↗] for S-band / ADS-B correlation.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Iridium Classic 780 km (485 mi) Polar Shell Cross-Checked — Non-Ballistic Hover at 15 m (50 ft) ASL Rules Out Orbital Re-Entry
CNEOS Bolide Match Probability3%
TLE Satellite Flare Likelihood1%
Kinematic Anomaly Score98 / 100

Local Gemma (tier1-local-server-gemma) computes a 98/100 kinematic anomaly score—the highest in the PURSUE archive. Although peak vertical speed (8.05 km/s / 18,000+ mph / Mach 23.47) approaches lower CNEOS meteoroid entry speeds, the 14 m (46 ft) object arrested its descent at 15 m (50 ft) above the ocean, hovered over a roiling subsurface disturbance, and re-ascended to CAP point on AN/SPY-1B Radar and ATFLIR IR (3% bolide match, 1% satellite flare likelihood). Nearest cataloged NASA CNEOS bolide is cneos-fb-124 (486.9 km / 302.5 mi great-circle separation).

RELEASE_04CASE ID: aguadilla-cbp-dhs-2013DATE: 2013-04-25COORDS: (18.49°, -67.13°)

Aguadilla, Puerto Rico DHS/CBP DHC-8 WESCAM MX-15D Thermal Track

Rafael Hernández Airport / Aguadilla Coastal Waters, Puerto Rico • NARA RG 563 & RG 615 / DHS CBP Air and Marine Operations Thermal Tape

Altitude (Imperial & Metric)
365 m / 1,200 ft (0.365 km / 0.23 mi)
1,200 ft (0.23 mi) / 365 m (0.365 km)
Estimated Speed (mph & km/s)
95 mph / 0.042 km/s (Mach 0.12 Coastal Transmedium)
95 mph / 0.042 km/s (Mach 0.12)
Target Size (ft & m)
5 ft / 1.5 m
Primary Sensor: WESCAM MX-15D Thermal
Nearest CNEOS Bolide Distance (mi & km)
1,093.7 km / 679.6 mi
Sensor Modalities:WESCAM MX-15D ThermalAN/APS-143B(V)3 OceanEye Maritime Radar

Archived in PURSUE Release 04 from DHS / U.S. Customs and Border Protection Air and Marine Operations, a Bombardier DHC-8 maritime patrol aircraft recorded 3 minutes and 54 seconds of calibrated L-3 WESCAM MX-15D 3–5 μm thermal video over Aguadilla, Puerto Rico (18.49°N, -67.13°W) on April 25, 2013. The 1.5 m (5 ft) object maneuvered at 365 m (1,200 ft / 0.365 km / 0.23 mi) and 95 mph (0.042 km/s) before entering the Atlantic Ocean without splash signature or deceleration. Coastal low-altitude airspace monitoring combines 10x50 binoculars[↗] with an ADS-B receiver[↗], digital anemometer[↗], and RTK GPS module[↗] to distinguish wind-borne thermal lanterns from powered transmedium tracks.

LOCAL GEMMA (TIER1-LOCAL-SERVER-GEMMA) MULTI-CATALOG CORRELATION METRICSTLE Assessment: Marine Boundary Layer 365 m (1,200 ft / 0.23 mi) — Zero Orbital TLE or Atmospheric Re-Entry Match
CNEOS Bolide Match Probability1%
TLE Satellite Flare Likelihood1%
Kinematic Anomaly Score88 / 100

Local Gemma (tier1-local-server-gemma) records a 1% CNEOS bolide match and 1% satellite flare likelihood for this marine boundary layer track at 365 m (1,200 ft / 0.365 km / 0.23 mi) and 95 mph (0.042 km/s). WESCAM MX-15D Thermal pixel radiometry showing air-to-sea transmedium entry and dual-target bifurcation yields an 88/100 kinematic anomaly score. Nearest cataloged NASA CNEOS bolide is cneos-fb-093 (1,093.7 km / 679.6 mi great-circle separation).

OPTICAL TRACKING REQUIREMENTS // PHOTOMETRIC LINK
TIER A: NAKED-EYE / BINOCULAR
Calculated Apparent Magnitude (Vmag)
Vmag -5.48
Abs. Magnitude H = 8.50
Required Aperture (mm)
70 mm Optical Aperture
Wide-Field Sweeping / Tripod-Stabilized 15x70 Visual Track
Best Viewing Window
Local Astronomical Twilight to Pre-Dawn Zenith (Bortle 1–5)
Target: PURSUE Multi-Sensor UAP & Atmospheric Bolide Corridor

PURSUE Multi-Sensor UAP & Atmospheric Bolide Corridor produces luminous atmospheric bolide ion trails visible to the unaided eye and wide-field 15x70 astronomy binoculars[↗].

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2026 war.gov/ufo PURSUE Releases 01–06 & AARO Multi-Sensor UAP Correlation Engine | Meteors.ai | Meteors.ai Space Network