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Office of the Secretary of Defense: 027_Satellite_Flaring_Paper

Department of Defense. Office of the Secretary of Defense. · 2023 · 18 pages · text from the file's own layer

This information paper from the Department of Defense's All-domain Anomaly Resolution Office (AARO) is dated December 2024 and was released in full in February 2025. It explains how sunlight reflecting off Starlink and other low Earth orbit satellites produces bright flares and satellite trains that observers can mistake for UAP. It gives step-by-step methods for predicting flare windows from the ground and from aircraft. It concludes that lights reported by an airline pilot near Gallup, New Mexico, in October 2022 were very likely satellite flares.

  • p. 1 …2 Altitude for Low Earth Orbit (LEO) ranges from 300km to 2,000km.027Page determined to…
  • p. 5 …During this phase, the satellites navigate from their initial low orbit to their final orbital altitude…
  • p. 17 …Acronyms Acronym Definition AARO All-domain Anomaly Resolution Office LEO Low Earth Orbit LOS Line of…
  • p. 18 …Boley, "Satellite mega-constellations create risks in Low Earth Orbit, the atmosphere and on Earth," Scientific…
All-domain Anomaly Resolution Office (AARO)
14
Unlike the ground-based observation case discussed above, an airborne observer does not have the
ability to “park themselves” at a given location and wait for the Starlink flaring window to come
into view. Consequently, the process described below is more likely useful to determine whether
a previous sighting phenomenon may have been the result of Starlink flares.
Below is the process for determining the elevation and azimuth look angles for an airborne
observer to determine whether their sighting may potentially have been due to Starlink flares. Table
3 is an example template that may be useful.
1. Choose the observation location (latitude and longitude, O1), altitude and aircraft bearing
for the airborne observer (or azimuth look angle as noted in Footnote 3).
2. Use Figure 15 and online resources or Google Earth to calculate the effective observation
location, O2, for the airborne observer. Note the effective latitude and longitude in Table 3.
3. Select the year of the observation.
4. Select the calendar day of the observation.
5. Select the local time of the observation.
6. Determine the Sun's azimuth for the given time, date, and year at the effective observation
position O2. If O1 and O2 are not in the same time zone, use the time zone for O1 when
converting from local time to UTC.
7. Go to the online Sun altitude and azimuth calculator of your choice, e.g.,
https://www.suncalc.org/ or https://www.timeanddate.com/sun, and enter the information
from steps (2) through (5).
8. Use the slider bar at the top of the page for suncalc.org or the expandable tables on
timeanddate.com to find the Sun’s azimuth for the given local time of the observation and
record this into the appropriate blocks in the table.
9. Use Figure 10 above to estimate the elevation look angle at which Starlink flares should
have been visible and record this information into the table.
10. Compare the Sun’s azimuth and elevation look angle for the estimated flare window to the
sighting’s azimuth and elevation to determine if Starlink flares may be a likely explanation
for the observed phenomena.
Case
AARO received a Federal Aviation Administration UAP report from an airline pilot describing
multiple unidentified lights moving in different directions. The report states that the pilot was
traveling eastbound near Gallup, NM (35.5224°N, 108.7235°W) on October 9, 2022, at
approximately 3:50AM local time. The aircraft was at an altitude of 35,000 feet and had a bearing
(heading) of approx. 70° from true North. The pilot noted that the UAP were “multiple lights
moving in different directions, left of the constellation Leo.” No further data was provided.
The following procedure will determine if the reported lights could be Starlink flares.027Page determined to be Unclassified
Reviewed by Chief of Staff, AARO
IAW FY24 NDAA, Section 1841(a)(1)(C)
Date: 2/14/2025

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Official release, from the nara collection. The PDF is mirrored here; the original link is above. 18 pages are in the text index: search them above, or from the library's search.