Re: ZQ-3 R/B near re-entry

From: Marco Langbroek via Seesat-l <seesat-l_at_lists.seesatmail.org>
Date: Sun, 1 Feb 2026 18:56:04 +0100
I used our TU Delft Astrodynamics Toolkit (Tudat) to explore this idea further,
mostly by trial-and-error with various assumed masses and break-up altitudes.

I so far have trouble getting results with breakup during or just before the
12:39 UTC first TIP. It requires significant masses separating well before the
TIP time, and then the modelled reentry of the R/B no longer fits well with the TIP.

However: I am able to reproduce the two TIP times and locations by having a
surprisingly small solid object separate at the *PREVIOUS* perigee pass, around
11:24 UTC (so 1h 15m before the first of the two TIP moments).

Assuming a solid steel sphere, a 7.9 kg (12.4 cm diameter) object separating
from the R/B at the previous perigee around 11:24 UTC at an altitude of about
109.5 km, does indeed survive the next perigee where the R/B reenters at 12:39
UTC (first TIP), and reenters around 13:43 UTC near 5 S, 62 E, values close to
the second TIP.

- Marco



Op 31-1-2026 om 19:25 schreef Marco Langbroek via Seesat-l:

>> The ZQ-3 RB reentry was from a somewhat eccentric orbit (more so than your
>> average reentry. The last available orbit was 211 x 102 km.
>>
>> The 12:39 UTC first "reentry" point could be where the R/B started to ablate
>> and fragment near perigee. One relatively massive fragment however might have
>> survived perigee and finally reentered half an orbital revolution later at
>> 13:43 UTC.
>>
>> I wonder whether that fragment was the dummy payload, still attached to the
>> upper stage, that might have come loose during the first "reentry" moment and
>> survived, for example because it was a massive dummy mass with relatively
>> large weight to size, while the rest of the R/B (the R/B proper) reentered at
>> the 12:30 first reentry point.
------
Dr Marco Langbroek
Lecturer in optical Space Situational Awareness (SSA)

TU Delft, Faculty of Aerospace Engineering
section Astrodynamics and Space Missions
------

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Received on Sun Feb 01 2026 - 09:56:17 UTC

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