There's a strong focus on the collision avoidance capabilities of the #Starlink satellites rather than on the services that inform those capabilities. Ryan Hiles and co-authors presented a hugely valuable insight on this aspect at @amoscon last year amostech.com/TechnicalPaper…
The impact of #Starlink on the work of @SpaceForceDoD is explained clearly, as are the steps taken to manage the screening burden that has emerged with growing numbers of #Starlink satellites. That burden is continuing to grow (exponentially by my estimates)
It's also revealing that @SpaceX present the thousands of manoeuvres as successes rather than a signal of a stressed environment. In many respects, the avoidance of collisions should be seen as a success but it's hard to find anything to celebrate in it.
And, as others are starting to point out, it's great that the #Starlink plan A is working, and much of this update from @SpaceX is about things that are working, but what happens when things go wrong? TBH, you can argue a lot has gone wrong already
There's also a concern that even the 1-in-100,000 collision probability threshold for manoeuvres is not sufficient (even though it is far better than the NASA standard). David Hand talks about rare events (like 1-in-a-million) in his book 'The Improbability Principle'...
...and how the law of very large numbers reveals why rare and seemingly improbable events can and do happen. Given sufficient opportunity (i.e. lots of close approaches) even the conjunctions falling below the manoeuvre threshold can become concerning.
And this is for all the objects we can detect and track. There's a very important and substantial population of lethal non-trackable objects that pose very real risks to #Starlink. Aaron Boley & Michael Byers explored this in their insightful paper nature.com/articles/s4159…
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Elon Musk told the Financial Times that "Tens of billions" of satellites can be accommodated in orbits close to Earth. Here's a thread looking at whether this is correct... bbc.co.uk/news/business-…
1/ To investigate, I used the stability model developed by Don Kessler & Phillip Anz-Meador, which Phillip presented at the 3rd European Conference on Space Debris in 2001
2/ I will skip over the derivation of the model to go straight to the key result, the
critical number of intact objects above a specified altitude producing a
runaway environment:
Maybe I am overthinking this, but it appears to me that all the reporting of the conjunctions involving Starlink satellites & the Chinese Space Station is forgetting that close approaches & avoidance manoeuvres are a normal part of space traffic management.
Even in environments with little to no debris (e.g. in Mars orbit) collision avoidance manoeuvres are performed. Perhaps not routinely, but they do occur.
Even with great surveillance and tracking in the future, and the most robust space traffic regulations, collision avoidance manoeuvres will be part of space operations. Avoidance manoeuvres are unavoidable.
Here's a thread containing the slides and thoughts I shared at today's @seradata space conference. I wasn't able to invest much time to prepare the talk, so some of the slides will look familiar to those attending April's ESA #SpaceDebris conference. Some are new [1/n]
[alt text: talk title "The Space Debris Environment - Current Status and Evolution of the Risk"]
I put this slide together using data from celestrak.com. It shows the historical evolution of the orbital object population (as recorded in the public catalogue). The highlight statistic is that active spacecraft make up 20% of the current catalogue population [2/n]
I think the #KesslerSyndrome is too often presented as a tipping point or a threshold we have yet to cross, so I wanted to use some aspects of my paper at the 8th European Conference on #SpaceDebris to explain why I think that is wrong [1/n]
The starting point of my thinking was to look at how natural populations grow. The simple exponential model is a standard model that describes the growth of a single population [2/n]
If we know the initial number of individuals in the population N(0) then this model allows us to estimate the number of individuals at any future time t. Here, r is the intrinsic rate of natural increase, which depends on the birth rate, b, and death rate, d [3/n]
I am seeing some ill-informed takes on today's near-miss in orbit so would like to offer some trajectory corrections if I may. Firstly, the chance that a single collision would trigger a catastrophic 'chain reaction' that would sweep through LEO is tiny.
For every close pass involving catalogued objects in orbit we can estimate a collision probability, or Pc. The Pc is between 0 and 1. If it is 1 we can say that a collision is certain. If it is 0 then we can say that a miss is certain.
The event today may have had a Pc between 0.02 & 0.2. In any case, the Pc was relatively small (compared to a Pc of 1) so a miss was the most likely outcome. For a chain reaction to occur a long & sustained sequence of collisions would need to take place.
All of my work interactions are virtual at the moment, as I am sure many of yours are too. In this format I think it is even more difficult to be aware of an #InvisibleIllness or #InvisibleDisability so for #MEAwarenessHour I'd like to ask you to keep this in mind.
It will be harder for you to see if someone is facing challenges so it's perhaps even more important than ever to be kind & considerate in all of your online work interactions.
It's easy to be dismissive, to compare someone else's situation to your own, or to persuade yourself that perhaps your colleague's slow progess is because of a lack of effort. It's important to have empathy & not to judge.