Scott Tilley 🇺🇦 Profile picture
Jan 12, 2023 13 tweets 6 min read Read on X
I've recently renewed an observing campaign on #TIANWEN1. The orbit hasn't changed so an aerobrake test claimed for late 2022 has not occurred yet. In preparation for observing an aerobraking manoeuvre I thought it would be interesting to study past missions that did one. 🧵⬇️ By NASA/JPL/Corby Waste - https://solarsystem.nasa.gov/multi
First a bit a reference of why we believe #TIANWEN1 will conduct an aerobraking test. This all relates to the #TIANWEN3 Mars sample return mission.
spacenews.com/china-aims-to-…
Aerobraking is used to allow a spacecraft to lower its apopasis by using a planet's atmosphere to decelerate the spacecraft as it passes through the tenuous upper atmosphere of the planet at periapsis at just the right altitude as not to cook the spacecraft and max. drag. ⬇️
Aerobraking requires a spacecraft attitude to maximize drag and constant attention from ground controllers. Risks of over-heating its tenderbits, undesired attitude changes and the ever changing density of the planet's atmosphere require constant attention and human management.⬇️
Relatively low energy orbital insertions usually result in a spacecraft being in a highly elliptical orbit. When aerobraking you only have the very limited time at periapsis to impart deceleration, so you're not going to change an orbit significantly by completing one pass. ⬇️ MARS RECONNAISSANCE ORBITER AEROBRAKING DAILY OPERATIONS AND
To quantify what it takes in time to change an orbit lets consider a few past missions at Mars that used aerobraking. For comparison #TIANWEN1 is in a ~7hr period orbit presently. So any test will take time and continued focus to demonstrate an operational capability.⬇️
One of the reasons #TIANWEN1 needed such a large rocket is that it propulsively lowered it's orbit. This can use almost as much delta-V as the insertion burn. MRO used 1015m/s for MOI burn, and aerobraking to science orbit saved 1080m/s, double the mass would have been needed!⬇️
Further communications is complicated by the need to change the spacecraft attitude at periapsis to present maximum area to the planet's atmosphere. This in MRO's case resulted in a low gain antenna and a simply carrier being emitted for aerobraking portions of the orbit.⬇️ Mars Reconnaissance Orbiter Aerobraking Navigation Operation
Next consider as the orbit's period gets shorter and shorter mission control has less time to consider changes and react to issues. Recall, Mars is 3-22 minutes light time away... So the manoeuvre is complex and labour intensive.⬇️ Mars Reconnaissance Orbiter Aerobraking Navigation Operation
Most Aerobraking manoeuvres are broken into phases:
- Walk-in/testing
- Prime aerobraking manouver
- Walkout to restore long term stable orbit.⬇️
Aerobraking manoeuvrers we need human control so consider the worldwide coverage of the Chinese deep space network. China has ground stations in China and in Argentina. This leaves potential gaps in coverage at present. This could perhaps limit a sample return mission too. ⬇️
What orbit would #TIANWEN1 be targeting? I would expect something that a MAV could reach if they are doing a full up test and want to something that really tests their mission capabilities so something in the 300-400km near circular range similar to what #ESA is proposing.⬇️
If #TIANWEN1 begins an aerobrake test what could be see?
- Weak/no signals around periareion,
- Slow initial change in orbital period particularly at first as they dip their toes,
- Odd signal behaviour as the spacecraft attitude is constantly changed.🛑

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More from @coastal8049

Dec 22, 2023
Update on the Chinese 'spaceplane' monitoring effort. @plugger_lockett observed possible emissions from objects from the 2023-195 launch. Despite using the same modulations it turns out these emissions are from other secret Chinese military sats, raising more questions. 🧵⬇️
Upon fixing a minor timing issue with his ground station @plugger_lockett sent me data from a pass yesterday & I was able to determine that the object being tracked yesterday was in fact YAOGAN-30 X the track of which passed over one of 2023-195. ⬇️ Image
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A telegram post by @roscosmos provides limited information of the status of #Luna25. Apparently, the spacecraft failed to adjust its orbit as planned.⬇️ https://t.me/roscosmos_gk/10535
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I have been asked repeatedly about #Luna25.

Thus far I have no independent observations of the mission to share. That is not without extensive trying to observe it.

So why am I not detecting anything? 🧵⬇️ Image
#Luna25 was launched into a trajectory that is largely only visible on Earth in daylight. Secondly, that trajectory is not exactly known. I have calculated one based on the launch timing and the scant public info shared and used GMAT to find a good direct trajectory. ⬇️ Image
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A follower asked if #Chandrayaan3 could land on the Moon before #Luna25. The short answer is maybe.

As we'll see in this thread changing a plan as complex as landing on the Moon is not a great idea.🧵⬇️
#Chandrayaan3 is presently largely locked into an orbital plane above the Moon. What that means is that it needs to wait for the Moon to rotate under-neigh it to reach the primary landing site that @isro has painstakingly planned to land at. ⬇️
Therefore, if you want to rush to get to the landing site it's too late. Therefore, you need to pick a new landing site under up coming terrain that may be suitable and also change the mission plan. Recalculate, adjust and then execute. ⬇️
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Aug 3, 2023
#Chandrayaan3 trajectory update 2023-08-02 #2.

Despite my better judgement, I did a TLE update on the Doppler data. The problem with TLEs in these types of orbits is they degenerate fast as the model is not designed to deal with long periods et. al. 🧵⬇️
Image
Image
Small changes in the data or the fit has profound effects on the TLE and the orbital model. But they are convenient. So I offer a couple of TLEs to aid anyone wishing to hunt for #Chandrayaan3. NO WARRANTY offered 😉, look with WIDE field... ⬇️
Data fit to released orbital parameters:
1 57320U 23213.95526600 .00000000 00000-0 00000-0 0 04
2 57320 21.4000 180.4625 9648325 12.6358 39.3505 0.10345282 04
# 20230801.30-20230802.61, 53466 measurements, 0.005 kHz rms⬇️
Read 4 tweets
Jan 10, 2023
#TIANWEN1 orbit remains unchanged based on period measurements.
T=25482s,
a=8898km. So no aerobrake test yet.

Neuquén ground station apparently attempted to lock to the spacecraft last night and failed. News reports of orbiter having communications issues. 🧵⬇️ ImageImage
This zoomed in Doppler plot of #TIANWEN1's signal during the anomalous lock attempt from yesterday is depicted below. Neuquén ground station appears to be using uplink Doppler compensation but is out of sync with the actual orbit of the spacecraft. ⬇️ Neuquén ground station in A...
Uplink Doppler compensation (UDC) is used by a ground station to place the uplinked signal at the spacecraft at a constant signal. It does this by 'ramping' the signal it transmits to match the 1-way Doppler to the spacecraft. ⬇️
Read 5 tweets

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