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. 🧵⬇️
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. ⬇️
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.⬇️
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.⬇️
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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#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. 🧵⬇️
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. ⬇️
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. ⬇️
The R/B of the Yunhai 1-03 mission appears to have suffered a breakup event. The plane of the orbit is nicely visible in the evening in the Northern hemisphere. Observers could look for debris by observing along the R/B plane and looking early.
OBJECT B [54236, 2022-151B] 🧵
The irony is the satellite Yunhai 1-03 is replacing was itself hit by another satellite. Goes to show you that space junk at these orbital altitudes is not a good thing. space.com/china-yunhai-1…
Look as soon as possible if you plan too before it disperses too much.
#CAPSTONE appears to be garnering the DSN's attention over the last day or so. Continuous uplinks with no downlink like the anomaly observed after the spacecraft was released post TLI.
She was scheduled for TCM-3 in early September based on statements after TCM-2.
I'm presently tracking #CAPSTONE on X-band and noting no emissions from it over the last few hours.
DSN NOW just updated and most of Goldstone's DSS antennas are now tasked with #CAPSTONE. Even DSS 14.
Overall visibility of the spacecraft from my ground station location. Elevation above the horizon will be a key factor. As you can see during the early and late stages of the mission Artemis will be low in my sky.
Next lets consider the range to #ARTEMIS1 so a model of the expected signal level can be obtained using Free Space Path Loss (FSPL) assumptions. Data is only plotted when Artemis is above my horizon.
The following are estimates of the SNR of #ARTEMIS1's signal in my 1.8m dish using an Equivalent Noise Bandwidth (ENBW) of ~2Hz for my usual SDR setup during the course of the mission. Assumed spacecraft High Gain Antenna (HGA) and the known sensitivity of my system used here.
As you can see here there's legit Russian military traffic here.
Aircraft spotters I make a call for you to pay attention to this 🧵.
MERIDIAN 9, 990MHz transponder narrow data. This type of traffic has been observed for decades on the Molniya-T1 spacecraft too. It is thought to be part of the Russian Strategic Rocket Force's communication system.
A call for #OSINT air traffic gurus to see if any Russian aircraft with strange humps on their back are orbiting somewhere over Russia right now. Like RSD79 in this post.