Lifson
Lifson
Modeling
Miles Lifson, Aniqua Baset, Grant Cates, Bill Chen, Angelo Connor, Carson Coursey,
Gregory Henning, Michael Miyamoto, Glenn E. Peterson, Brian Weeden, and Grant
Williams
The Aerospace Corporation
Indigo Brownhall
University College London
Matthew G. Burgess
University of Wyoming
Mark Moretto
North Carolina State University
Akhil Rao
Middlebury College
Abstract
Models are widely used to understand potential futures of the space environment and space sustainability risks. In
other domains, these models have often been combined with shared reference scenarios to support the development
of effective policy solutions. Evolutionary space environment modeling is sensitive to modeling assumptions and
inputs, but these inputs often rely on controlled information or are simply not disclosed. At the same time, a lack of
a set of common modeling assumptions complicates communication across organizations and interpretation of
detailed modeling results from different entities. This work describes preliminary efforts to develop a set of
indicative reference scenarios for evolutionary space environment modeling, supported by publicly-releasable input
sets. Community feedback is solicited on the proposed scenarios, parameter choices, and data formats. Dubbed, the
“Space Environment Pathways” (SEPs), a set of six scenarios are defined along three axes: market demand for space
services, non-market demand for space services, and level of space sustainability effort. Various modeling inputs are
provided including narrative descriptions of the scenarios, an initial population model, future traffic model, and solar
inputs for atmospheric density models. The process by which the scenarios and axes were defined is described. It is
argued that a set of shared scenarios would provide multiple benefits to the modeling community including making
it easier to develop, verify, and validate new models, supporting integrated assessment modeling, improving public
communication about space sustainability, and enabling future adaptive management and governance structures for
the space domain.
1. Introduction
As Bohr noted, prediction is very difficult, especially about the future. This paper describes a project to develop a
set of 6 potential futures “scenarios” for the space environment, dubbed “The Space Environment Pathways”
(SEPs). Scenarios can be thought of as ‘if-then’ statements. If we make a given set of assumptions about key
economic, technological, and policy parameters, scenarios explore the consequences of these assumptions. In this
way, scenarios serve as agenda-setting tools for research and policy (e.g., [1] describes how scenarios are used in
climate-change research). The SEPs do not attempt to predict the exact future we will experience; rather, they
attempt to identify key behaviors and potential outcomes that might influence the direction the space environment
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evolves and to provide an accessible, open set of data products to the community to model those potential futures.
This paper describes the preliminary phases of work to develop these scenarios with the objective of beginning what
we hope will be a community discussion on assumptions, methodologies, formats, and outputs for what we hope
will eventually become a set of community standard outputs for evolutionary modeling of the space environment.
The scenarios and inputs are intended for release in October 2024.
This paper focuses on articulating the value of having a set of standardized community reference scenarios for
evolutionary space environment modeling, describing the methodology used to develop the 6 chosen scenarios and
the scenarios themselves. While the various components that make up the inputs for each scenario are briefly
described in this paper, they will be described more fully with underlying technical methodologies in a paper by this
same team to be presented at the International Astronautical Congress [2] in a few weeks.
In wider literature and across research domains, developing scenarios to focus research community efforts is a
common exercise [3] [4] [5]. Most notable are the Representative Concentration Pathways (RCPs) [6] and the
Shared Socioeconomic Pathways (SSPs) [7] for climate change, which were central to the fifth and sixth assessment
reports, respectively, of the Intergovernmental Panel on Climate Change (IPCC). The RCPs and SSPs were
developed through community efforts to define ranges of socioeconomic, technological, and policy pathways that
would create different greenhouse-gas emissions trajectories throughout the twenty-first century. The ranges of
assumptions explored in the SSP and RCPs were chosen based partly on what relevant domain experts thought of as
plausible, but also based on specific needs of climate researchers and policymakers. For example, the SSPs include
scenarios consistent with limiting global warming to 1.5 degrees Celsius by 2100, as this is an aspirational goal of
the 2015 Paris Agreement [7], even though the sociotechnical assumptions required to achieve that goal may be
implausible (e.g., [8] [9]). Conversely, the scenarios with highest emissions—RCP8.5 and SS5-8.5—were originally
intended to explore extreme upper bounds (despite widespread subsequent misuse), which can be useful in
exploratory research and are also widely thought to be implausible [10] [9].
The RCPs focused mainly on providing emissions pathways specifically [6]. The SSPs focused on explicitly
defining socioeconomic scenarios—which affect energy demand and technological progress—as a framework for
exploring emissions scenarios. Figure 1, reproduced from O’Neill et al. [11] and Riahi et al. [7], illustrates this. The
SSPs defined five socioeconomic pathways (SSP1,... SSP5) (Figure 1A), within which different stringencies of
global climate policies could produce different emissions pathways, compared to ‘baselines’ with no climate policy
(Figure 1B). Given that socioeconomic conditions also affect society’s ability to adapt to climate change and cope
with its consequences, foregrounding the socioeconomic assumptions in the SSP scenario framework was useful to
research jointly exploring climate change pathways and their societal consequences (e.g., Moyer et al. [12]).
However, given that some climate change research only needs emissions as an input (e.g., physical climate
modeling), and many emissions pathways can be produced by multiple sets of socioeconomic assumptions (Figure
1B), the ongoing effort to develop scenarios for the upcoming seventh IPCC assessment report has reverted to
foregrounding emissions pathways [13].
Figure 1 A: Overview of Shared Socioeconomic Pathways (SSPs). B: Scenario Matrix specified by SSPs and forcing levels.
Scenarios populate individual cells providing information about mitigation benefits and costs [7].
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The RCPs and SSPs have been extremely successful in providing a common framework for climate change research.
For example, between 2014-2019, at least 1,378 analyses were published that used or continued to develop the
scenarios [1]. Retrospective reviews by the RCP and SSP architects (e.g., [11] [13]), and critical reviews by others
(e.g., [10]; [9]; [14]) make several recommendations, with clear analogs to other domains such as the space
environment—the focus of our work. These recommendations include: distinguishing key axes of scenario
assumptions that can vary separately (e.g., emissions and economic development) [13], distinguishing scenarios
intended to be considered plausible from those intended to be considered exploratory [10] [9], developing widely
accessible and user-friendly online repositories to catalyze collaboration and capacity building ( [1]; see also IIASA,
2022 [15], for an example), avoiding insularity in scenario development that limits the scope of models and futures
that can be explored [14], and having frameworks that allow scenarios to be regularly updated in light of new
information and sociotechnical developments [10] [16].
There are clear analogs between the needs for common scenarios in climate modeling and modeling of the future of
the space environment. It is well known that the outputs of evolutionary space environment models depend strongly
on the chosen inputs. Without agreement on inputs, it can be difficult to compare models and studies and understand
the potential consequences of choices or interventions. The presence of a common baseline of assumptions would be
invaluable for the evolutionary space environment modeling community as it grapples with numerous sources of
rapid change including a dramatic increase in the active space population and supporting launch rates, significant
concern about space sustainability and orbital capacity and proposals for new mitigation and remediation
requirements, and heightened geopolitical tensions as a backdrop for future space development. This idea is not new
in a space context. The Inter-agency Space Debris Coordinating Committee (IADC) has long used standardized
inputs for model cross-validation and prediction, such as the 2013 study by Liou et al. [17]. However, it does not
make those inputs public, the inputs are not intended to fully span a range of potential futures, and relatively little of
this work has been published. In this paper we take the idea of the SSPs and associated design recommendations as
an inspiration but adapt it for suitability to the space environment. It is hoped that these scenarios and the associated
inputs and methodology can help support improved modeling, and ultimately decision-making.
2. Methods
This section describes the process used by the SEP definition team to develop and validate the set of SEP scenarios,
as well as the associated scope and goals for the project: a set of a manageable number of exploratory scenarios for
potential space futures supported by publicly available model inputs.
One of the first tasks for the SEP definition team was to determine an appropriate process to develop our initial
proposal for the SEPs. While this project was partially inspired by the previously mentioned SSPs for the climate
research community, it quickly became evident that the SSPs would not provide an appropriate procedural example
to emulate. Defining the SSPs in the climate research community followed an elaborate formal process with multiple
preparatory conferences, papers, and participants and a considerable level of organizational infrastructure. The SSPs
progressed from a proposal for development that was submitted to the community and ultimately obtained formal
approval. The space environment modeling community is considerably smaller than the climate community, and we
determined that the level of organization infrastructure used for that process would be overly inhibitive and
unnecessary for a community of our size. We also determined that there is not yet a critical mass of support for
reference scenarios within our community, which would complicate efforts to build a truly community-wide process
from the start. Instead, we concluded that the best first step would be to gather a group of experts with experience in
astrodynamics, orbital capacity, debris modeling, policy, space and resource economics, as well as experience with
the development of and lessons learned from the SSP process. This group could then develop a preliminary proposal
that would be provided to the broader space community for iterative feedback.
This group, the SEP definition team, is composed of Miles Lifson, Indigo Brownhall, Matthew Burgess, Marcus
Holzinger, Daniel Kaffine, Mark Moretto, Akhil Rao, and Brian Weeden. It was responsible for defining the axes
for exploration across the various scenarios, the points where each scenario would be placed on each axis, the
narrative descriptions of each scenario, and overall direction of the project. A broader research team at The
Aerospace Corporation lent technical expertise and support and developed detailed methodologies and data products
in line with the direction from the SEP definition team. Miles Lifson coordinated the overall project and coordinated
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between the two teams. Having established the SEP project team, we make several early decisions concerning the
objective and course of the project:
First, the scenarios and inputs to the project need to be publicly released and available openly to the full community.
We felt this was important to achieve multiple objectives for the project even though it would impose limitations on
the types of data sources and methodologies that could be used to construct modeling inputs. The entire team felt
that associated losses in input fidelity were more than offset by the benefits of openness, and members noted that
modeling using closed inputs would invariably continue alongside modeling of the open reference cases.
Second, the purpose of the reference scenarios should be exploratory and clearly conveyed as such. When
conducting modeling and constructing scenarios, multiple objectives are possible. Exploratory modeling seeks to
understand how a system responds to certain inputs. Such modeling can be used in a variety of ways including
seeing how a system responds to possible environment inputs (which may be controlled or uncontrolled) and to
understand how the system will respond to certain behavior and policy choices. Exploratory modeling can be
distinguished from predictive modeling, which seeks to identify the actual future state of the modeled system, and
normative modeling, which seeks to specify what should happen [18]. While a single set of scenarios can be used in
multiple ways, we determined that the critical need for the community was a set of scenarios that would reasonably
explore the set of potential futures to help inform model-development and policy decision-making. We viewed
predictive modeling as impossible to achieve over the relevant time horizons, and normative modeling being too
actor-specific to support generalization in common reference scenarios.
Third, we should provide a manageable number of scenarios that are conceptually distinct, recognizing that this
handful of scenarios would be unable to sample all combinations of states on all axes of interest. In the case of the
SSPs, a set of primary and secondary scenarios were identified that combine the socioeconomic aspects of the SSPs
with various levels of radiative forcing from the RCPs [1].
Fourth, we identify several limits in scope to keep the project manageable for the first iteration. These limitations
include constraining our focus to Low Earth Orbit (LEO), excluding future governmental large constellations,
except where reported to the International Telecommunication Union (ITU) or Federal Communications
Commission (FCC), and excluding commercial space stations and/or crewed space vehicles except insofar as these
vehicles are captured in the replicated historical non-constellation launch traffic. We also decided not to include the
modeling of the outcomes of a significant space conflict and/or future debris-producing anti-satellite missile tests.
There are several reasons for this. First, we viewed the utility of such a scenario as limited. While the specific
consequences of a significant conflict in outer space are highly dependent on the specific technical dimensions of
that conflict, the result would be disastrous for other operators and the long-term space environment. This is widely
understood and does not require a community consensus model to understand. With regards to debris-producing
direct-ascent anti-satellite missile tests, the reprise of another FY-1C event appears remote due to emerging
international norms and the widespread condemnation of that event. Recent anti-satellite missile tests have occurred
at much lower altitudes and produced more limited and shorter-term environmental contexts. Additionally, the
United States has announced a voluntary moratorium on such tests that has been joined by more than 30 additional
countries [19].
Having defined the broad outlines of the task, we developed a process beginning with an open-ended discussion of
key themes that we believed would influence the potential evolution of the space environment. From this
discussion, we down-select a set of largely independent axes that corresponded to potential variation that we might
see in future behaviors. As part of this process, we collapse and merge axes that are correlated and eliminate axes
that we felt are of secondary importance. We then define points on each axis and identify combinations that
corresponded to the most important combinations of potential states. At this point we construct paragraph narratives
for each of the scenarios. These narratives describe the “what” that each scenario seeks to capture, emulating similar
narratives for the SSPs. In our case, these narratives also provide context to assist modelers who wish to include
factors not already specified in the scenario definition. In these cases, such individuals can use their judgment to
identify additional parameters as necessary that correspond to scenario narrative of interest.
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To assist with preliminary validation, an initial concept for the SEPs was presented in June 2024 for preliminary
feedback at the 7th International Workshop on Debris Modeling and Remediation. Feedback was positive and
generally noted the usefulness that such a dataset would provide to the community, and desirability of eventually
integrating such efforts into internationally coordinated work on space environment modeling through organizations
such as the IADC. To ensure that the scenarios covered were robust to future behaviors, The Aerospace
Corporation’s Strategic Foresight Team [20] was asked to examine the scenarios and provide feedback. They
determined that the scenarios were defined at an appropriate level of detail, responsive to major identified behaviors,
and were developed using a reasonable methodology.
To further assist with validation, a selected literature review of evolutionary space environment modeling work was
conducted. Evolutionary space environment modeling is a broad field with significant international work over the
course of multiple decades. In defining a set of shared scenarios that wrap in various assumptions made in the
modelling process, it was critical to understand what assumptions others have made in developing evolutionary
models of the space environment and to confirm the general perceptions of the SEP definition team. To reduce the
change that this analysis would be distorted by the pre-formed opinions of the SEP definition team, this literature
review process was conducted by an additional researcher who was not involved with the SEP definition team. The
intention of this literature review was not to be comprehensive, but to provide insight into the types of assumptions
and choices commonly made in high-quality modeling work and to identify the types of data products that would
need to be provided to support common modeling tasks. A number of papers ranging in publication year from 2002
to 2023 and origin were reviewed. A subset of these papers that included a robust outline of the assumptions adopted
were used to generate a matrix of assumptions and studies from which overarching conclusions were drawn.
Some assumptions endure across almost all studies, even those with different goals. Launch traffic was always based
on historical behaviors and was almost always a repeat of the last 8 years [21, 22, 23, 24, 25, 26, 27, 28, 29, 30].
Unless the effects of explosion rate were being evaluated, the explosion rate was commonly held to 0% [21, 22, 23,
17, 29]. This is similarly true for collision avoidance maneuvers; many earlier studies assume none [22, 17, 29, 31].
However, in the first 6 months of 2024 Starlink, a LEO constellation, reported over 50,000 [32]. Some efforts assumed
no collision avoidance maneuvers only after successful post-mission disposal [21], and several studies varied the rate
of collision avoidance maneuvers to evaluate its impact [28, 27]. 200 years is by far the dominant simulation timespan,
reflecting that 200 years is thought to be long enough for relevant behaviors and results to become clear [21, 22, 23,
25, 17, 28, 29, 30, 31, 33]. Minimum object size is often held at 10cm, in keeping with the current understanding of
what non-cooperative space situational awareness sensors are able to reliably detect and maintain [21, 25, 27, 26, 28,
29, 30, 31, 33]. This size may be decreased in years to come, particularly in parts of LEO, as the capabilities of the
US DOD’s Space Fence system are better understood. Spacecraft mission lifetime was most commonly 8 years [21,
22, 26, 29, 30, 34, 33]. Solar and geomagnetic effects were always rooted in past data, either by using a random
combination of datasets, the mean, highs, or varied across a study effort to detect sensitivity [22, 24, 26, 30, 34]. Initial
populations are often pulled from some standard catalog, such as DISCOS, MASTER, or the US DOD's catalog [21,
22, 26, 30, 33], and sometimes includes a freshness check to ensure only objects with recent states were ingested [24,
25]. When mentioned, crewed objects were excluded, as they are presumed to maneuver more often and operate with
a more conservative collision risk posture [24, 25]. When LEO is the primary study regime, this is commonly defined
as a perigee between 200km and 2000km [24, 26, 28, 29, 31, 34].
Post-mission disposal (PMD) timelines and rates are often set to 25 years with 90% success, reflecting longstanding
standards [23, 26, 28, 30, 33]. However, this is also frequently varied to predict the state of the space environment
given various levels of compliance for various types of spacecraft. For example, 0%, 50%, 60%, 75%, 99.5%, and
100% were all investigated [21, 25, 27], and rocket bodies were assumed to not be disposed in one case to demonstrate
this impact [31]. As the most recent study reviewed was from 2023, but many were from before this, a 5-year rule was
not often included as an assumption. Similarly, active debris removal (ADR) is typically not discussed, unless its
effect is being evaluated in the study [28].
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In some cases, where the effort is primarily interested in the relationship between a specific class of spacecraft (e.g.,
CubeSats or large LEO constellations) and the environment, assumptions are made about the attributes and behavior
of these spacecraft. This often include the profile and length of the orbit raising and lowering periods, spacecraft
shapes, sizes, masses, propulsion methods, and deployment/replenishment models [25, 27, 31, 33].
3. Results
To define the scenarios, axes were established to bound the dimensions on which the reference scenarios would be
built. These axes are categorized into two main groups: the future population model and sustainability efforts. The
future traffic model is further divided into Commercial and Non-Commercial demand. Non-Commercial launches
encompass satellites built to meet inherent consumer demands commonly driven by governments, such as Earth
Observation (EO), scientific, Position Navigation and Timing (PNT), and other Defense payloads. In contrast,
Commercial demand launches are driven by market users and include internet or communication constellations, as
well as private market PNT (LEO) and EO constellations. In both cases, demand is modeled exogenously, i.e.
satellites are pre-specified based on criteria rather than being the function of internal economic logic within the
model. The second category addresses the level of mitigation and sustainability efforts. This axis is crucial for
developing regulations, guidelines, and improvements in space operations. An example of an action along this axis
could be investing in ADR to remove high-risk rocket-bodies or inactive payloads. Finally, a proposed axis for
atmospheric density and solar activity/space weather was considered but ultimately rejected due to the project design
team’s opinion that atmospheric density variability was less important for exploration than the existing axes, would
additionally complicate interpretation of results, and that limited scientific understanding of the probabilities
associated with various solar activity excursion cases meant that it would be likely that a solar axes would have
modest effects or overly explore fairly unlikely cases.
*Major military spending state is defined as the top 20 states by defense spending in 2023, as calculated by Stockholm
International Peace Research Institute’s Military Expenditure Database.
The project team quickly realized that the level of space traffic and its properties would be one of the most important
inputs to a set of reference scenarios. In recent years, the overwhelming majority of traffic in LEO has been
commercial, driven primarily by large commercial communications constellations. SpaceX and Eutelsat OneWeb
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have both deployed very large constellations, with future generations of their constellations already proposed.
Multiple other operators have also proposed ambitious constellations. The team generally agreed that there is
considerable uncertainty about the level of demand for space services that will emerge in the coming years, and the
number and distribution of satellite constellations and satellites that this demand will support. We accordingly
prioritized future commercial traffic as a key axis for our model.
Most space environment evolutionary modeling paradigms and implementations require specific information about
particular spacecraft orbits, engineering properties, and behaviors for the duration of the modeling span, which is
often 100-200 years. Naturally, this level of precision cannot feasibly be obtained with any level of fidelity based on
the information available today for points a decade from now, much less centuries into the future. When faced with
such uncertainty, M. Granger Morgan [35] describes a process first proposed in a paper by Casman, Morgan, and
Dowlatabadi [36] whereby models with different levels of fidelity are fused to provide an estimate over differing
timespans, with transitions between detailed modeling, order-of-magnitude estimation, and bounding analysis. For a
project that seeks to support a wide variety of modeling paradigms with common inputs, we cannot insist on such
capabilities in the models themselves. However, we can design the inputs to provide appropriate inputs to test
information over these timeframes, starting with more detailed information where it exists and extrapolating into the
future while recongizing that over intermediate and long-term time horizons, the specific outputs obtained are more
appropriate for order of magnitude and bounding analysis rather than detailed predictive outcomes. This objective
informs the approach we take to estimating the future launch population.
In predicting future space traffic, we wanted to provide a set of inputs based on defensible, objective criteria that
could be plausibly updated on a regular cadence while tracking shifts in the nature of the space environment. We
determined that the best way to do so would be approach rooted in regulatory filings for large constellations and a
repeated historical non-constellation model. FCC and ITU filings were downloaded and processed to produce a list
of unique physical satellites proposed in those filings. This list was categorized into a set of constellation
development tiers based on a quasi-objective rubric for constellation deployment status, financial resources/stability,
legal and regulatory status, and business history. The full methodology is described in Lifson et al. [2]. Ratings were
applied on a per-company rather than a per-constellation basis. These constellations were then assigned to
representative launch vehicles with a deployment schedule based on the required ITU deadlines for bringing their
spectrum into use, assuming continued replenishment for the duration of the scenario. This is accompanied by a non-
constellation traffic model that repeats launches from recent years with a multipler based on the level of demand
provided as an input, concentrating traffic over a shorter time period between repetitions for multipliers greater than
one. This is a coarse model of future demand but is designed as a leading indicator to roughly reflect the continued
behavior of near-future constellation proposals, recognizing that there is wide variance in the likelihood of various
filings and that a method based only on deployments to date would ignore significant future constellations, even
high likelihood systems. It produces fairly detailed information about near-term satellite deployments as a function
of estimated level of demand for satellite services, but transitions to a more approximate estimate of traffic on longer
time-scales that may underestimate traffic in the far future. Nonetheless, the chosen approach still provides useful
input on the question of how current levels of traffic demand and behaviors will influence the long-term
sustainability and space operational assurance of the space environment. This question is one of the most important
outcomes for long-term environmental modeling.
In addition to satellites and constellations driven by market demand, there will also be other satellites and
constellations that do not respond to market-driven economic logic. These are primarily government missions
developed for civil or national security purposes. Such missions are likely to be driven by different demand factors
than commercial economic demand (even if at least some services are provided by commercial satellites). At the
same time, non-market demand will be related to and benefit from economies of scale and technical innovation in
the commercial market. As a reminder and as described in the scope limitations for the project in Section 2, the
focus for this axis is describing the peaceful environmental consequences of non-commercial demand rather than
explicitly simulating the environment consequences of kinetic space conflict.
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We note that the satellites and constellations providing such services are likely to be subject to increased sensitivity
about the nationalities of object ownership and operation and that, particularly in a national security context,
political leaders may be willing to relax space sustainability requirements for missions with national security
imperatives, particularly if such requirements are perceived as delaying or diminishing important mission’s
capabilities. We also determined that we did not wish to try to model potential future purely government owned and
operated constellations. There are not, to our knowledge, great open data sources to characterize such constellations
and attempts to guess their properties are likely quite fraught, particularly if our guesses were to closely resemble the
eventual design of actual classified government satellites.
As a result, we opted for the approach seen in Table 1, where the level of non-market demand acts as a modifier that
increases the likelihood status of commercial constellations associated with nations with substantial defense
spending as identified by a respected third-party methodology. This approach captures the recognition that the
primary driver for non-market demand for large constellation traffic will be national security rather than civil, even
though new civil large constellations may also emerge.
In addition to the level of traffic, the behavior of that traffic strongly influences the evolution of the space
environment. The extent to which space traffic fails to dispose promptly and successfully at end of mission, fails
during operational lifetime, and/or experiences spontaneous explosions all provide strong influences on the future
for the debris environment. We sought to create an axis that reflects levels of effort in this domain, ranging from
current behavior to strongly improved behavior at the levels posited to be necessary to ensure long-term
sustainability. Along this axis, we included two additional levels: one corresponding to an extrapolation of today’s
trends to reflect weak but incremental improvement over current practices, and another corresponding to
considerable but not aspirational levels of improvements aligned largely to industry recommendations about
improvements. While a variety of sources were consulted, the values in Table 3 drawn primarily on current practices
and best practices as documented in the ESA Space Environment Report [33] and IADC Space Debris Mitigation
Guidelines [37], the Space Safety Coalition’s Best Practices for the Sustainability of Space Operations, and the
newly revised ESA Zero Debris Charter [38]. These values were selected by the Aerospace technical team without
Office of Space Commerce consultation and do not constitute an official statement of endorsement or preference by
the Office of Space Commerce for the Traffic Coordination for Space System, policy, or more generally. While
these sources were consulted, they are not encoded literally. Certain aspects of the requirements in these documents,
for instance conditioning mitigation requirements on levels of estimated orbit-specific cumulative collision risk as
calculated with third-party tools would be too onerous to impose as a requirement intended to be broadly compatible
with multiple modeling tools that operate are widely varying levels of fidelity. For the same reason, we opted to
make the values on level of the axis constant rather than time-varying. In practice, slow improvements are likely to
occur over time, with factors like PMD rates increasing as engineering improves and older missions are replaced by
newer satellites with greater sustainability focus. Nonetheless, it is likely that only a subset of models will be able to
support time-varying behaviors for mitigation actions (which in at least some models are set by a single global
parameter). Because of the importance of broad compatibility, we opt for the easier to implement, but lower-fidelity
alternative. The use of constant values also simplifies interpretation of outcomes versus a time-varying outcome, in
alignment with this project’s focus on exploratory rather than predictive scenario design.
Perhaps controversially, our methodology combines both mitigation and remediation into a combined single axis.
One of the design principles for this project was to minimize the number of axes while covering the most important
and truly distinct axes. We reasoned that a world that seeks to commit effort to address space sustainability
concerns is also one that will likely begin operational remediation to some degree. Most contemporary analysis
argues that mitigation is a necessary but insufficient condition for long-term sustainability and that remediation will
also be necessary. At the same time, remediation concepts continue to mature technically while continuing to face
significant economic and policy questions. Remediation, particularly ADR, will likely continue to be a more
expensive way to remove risk than mitigation. Values were set based on the group’s informal judgment concerning
levels of ADR that were potentially plausible but also environmentally significant. While most high-risk objects
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currently on-orbit are high-altitude derelicts from the Soviet space program, we do not currently impose any
limitations on the nationality of objects that are removed. Over the timeframes countenanced in these scenarios,
accounting for contemporary space capabilities, economic scale, and political alignment is overly precise relative to
the scale of other assumptions. Similar to the description of mitigation actions, we impose a constant rate of
removal at each level of the axis. This is again less realistic than an increasing slope but simplifies analysis and is in
line with the options explored in [39, 40]. Nevertheless, variable rates of ADR activity are likely more easily
implementable across the broad scope of evolutionary space debris models than PMD and this is a factor that could
be revisited based on community feedback.
3.2 Scenarios
Ultimately, at least 6 scenarios are necessary to cover key potential futures. These scenarios and narrative
descriptions are present in Table 2. The position of each scenario along the three axes is described in Table 3. The
scenarios range from a highly synthetic to plausible extrapolations of current behaviors. All scenarios feature the
same shared initial population model and time-varying solar activity indices, described in more detail in Lifson et al.
[2].For each scenario, the goal was to find a possible outcome that develops from changing hypothetical positions
along the axes:
SEP 1 is a synthetic scenario that, although extremely unrealistic, is highly useful for model comparison and
troubleshooting. “No future launch” scenarios have been used for model comparison in an IADC context as they
limit the number of additional variables and degrees of freedom that need to be coordinated across models and make
it easier to identify problematic discrepancies or modeling errors before additional complexity is added [17].
Furthermore, evolutionary studies have shown that there is currently enough debris in LEO that the number of
inactive objects will rise even in a baseline scenario – providing an outcome to model policy and potential
mitigations for future studies [25].
SEP 2 follows another common idea in evolutionary studies, which is the extrapolation of the current behavior: what
would happen if we continued to operate as we are today. Note that this scenario reflects current behavior, rather
than current trends, so that factors such as gradually increasing compliance with post-mission disposal guidelines
will not be reflected. Rather, today’s compliance rates are continued for the duration of the scenario, along with
current rates of explosions for rocket bodies and satellites and no ADR.
SEP 3 describes a scenario in which commercial and governmental interest in using space declines substantially.
Some combination of easing political tensions, the development of cheaper substitutes (e.g., proliferated high-
altitude balloons), and rising economic uncertainty reduces the importance of space development on national and
international agendas. Though national security demand from large nations with developed space programs
continues, the influx of new space actors and investments diminishes considerably. The significant reduction in
space activity in this scenario is accompanied by medium (primary) or high (secondary) space-related environmental
policies in the two sub-scenarios, with a heavier focus on maintaining existing operations than on ensuring future
growth in space environment usage is sustainable.
SEP 4 and 5 consider two large variations in the sources of demand for space activity in LEO. SEP 4 is a scenario
where there is a new space race or cold war and interest in LEO comes primarily from governments, military and
defense organizations and market demand (i.e., for satellites serving non-governmental customers) is weaker.
Strategic imperatives lead to low sustainability effort, as outcompeting rivals attains more national importance than
long-term sustainability. SEP 5 is the opposite: a scenario in which commercially-driven development of LEO
increases while government-driven investment decreases. In SEP 5, there is a steady increase in constellations and
satellites, without a corresponding build-up in non-commercial demand. Here, two cases are considered with
medium or high sustainability effort, with medium effort being considered the primary scenario.
Finally, SEP 6 was included as possible outcome where both market and non-market demand drive an extremely
busy and operationally complex space environment. This interest drives increased sustainability behavior, with high
sustainability effort being the primary case, and medium effort as the secondary case.
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Table 2 Narrative Descriptions of the Space Environment Pathways
SEP 2: Continuing The world follows a path that maintains current behaviors, with existing partially-
Current Behaviors deployed large constellations finishing their deployments and then replenishing
over time, along with a continuation of recent historical launch traffic. Commercial
interest in internet connectivity and lower launch costs drive the growth of
satellites, with a few constellations satisfying market demand. There are no
advancements to sustainability guidelines or practices beyond today’s behaviors.
SEP 3: Space Winter The space bubble pops - after a period of rapid growth, the demand for commercial
and governmental space activities crashes. Easing political tensions and rising
economic uncertainty diminishes the importance of space development on national
and international agendas, resulting in limited future investments in the sector and
new space launch.
3H: Despite the low level of traffic, sustainability practices continue to increase
with global and national institutions as well as operators working to improve
sustainability practices to achieve long-term outcomes. Significant ADR begins to
occur.
SEP 4: Strategic Rivalry A rise in tensions between major space nations leads to significant government-
backed demand, while predicted future commercial market demand for space
services fails to materialize. Some LEO Earth observing, communications and
Position, Navigation and Timing (PNT) constellations are deployed and
maintained, but through government funding rather than commercial demand, with
a focus on nationally-affiliated satellites. Urgent perceived self-interest among
nations results in a low level of effort being applied towards space sustainability.
SEP 5: Commercially Non-market demand for space services declines, but the demand for commercial
Driven Development space-based activities such as internet, earth-observation imagery, and PNT steadily
increases, leading to the expansion of multiple existing and new large LEO
constellations.
5H: The complex operating environment spurs strong sustainability effort including
greatly improved PMD, reduced explosions, and significant ADR
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SEP 6: Intensive Space Driven by both rising international tensions and robust commercial market
Demand demands for satellite services, innovative technologies and reduced launch costs
lead to growth in market and non-market demand for satellites. The space economy
rapidly becomes the next trillion-dollar industry. LEO becomes an even busier
environment, with a significant increase in both maneuverable and non-
maneuverable objects, creating challenges for space traffic management and
sustainability.
Med
SEP 5 M/H: (primary) Significant commercial demands drives
Commercial-
Low High expansion of space traffic
driven High
Development (secondary)
Med
SEP 6 M/H: (secondary) A combination of international tensions and
Intensive Space High High validation of commercial business cases leads to
High
Demand doubly intensive space demand
(primary)
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4. Conclusions and Future Work
As seen in other environmental modeling disciplines, community-agreed reference scenarios have the potential to
provide multiple benefits. They reduce barriers to entry for the development, verification, and validation of new
modeling approaches and improve comparability between modeling methods and tools. They also help promote
better integrated modeling across issue areas and disciplines—for instance, unifying assumptions (and potentially
models) for assessing multiple types of negative externalities or integrating economic decision-making and
environmental modeling. Reference scenarios can additionally facilitate improved public communication about
likely future behaviors subject to different societal choices and support the development of necessary workflows for
adaptive, or other model-informed, space environment management strategies.
This paper presents a preliminary set of six proposed reference scenarios for community feedback and discussion.
The scenarios are intended to be distinct while broadly spanning the range of plausible futures for the space
environment. Each proposed reference scenario is framed with a narrative context and supported by associated
modeling inputs which will be released alongside the scenarios. The process used to develop these scenario concepts
was validated with a conference presentation to experts, literature review, and review by strategic foresight experts.
Key inputs include the initial population model, future launch model, atmospheric model and inputs, and operator
behavioral assumptions. The focus of this paper is on the reference scenarios themselves and the high-level choices
that feed into them. The chosen methods are intended to support a wide variety of potential approaches to space
environment modeling, be transparent and defensible in their assumptions and choices, and avoid a reliance on
controlled information. The workflow to develop these inputs is being designed to sustainably support a periodic
update cadence.
The project team hopes to continue to improve the scenario methodology over future iterations, including
transitioning the non-constellation satellite model to an endogenous function of economic and environmental factors
(building on the approach by Rao et al. [41]), rather than relying purely on recent historical launch traffic. In many
cases we have had to apply coarse assumptions for object properties, particular satellite mass and cross-sectional
area for future systems. We also hope to improve the quality of this data and reduce the importance of assumptions
by gathering additional inputs as they become available, including from the designs of such satellites and
constellations.
Initial development of the SEPs proceeded as a shared project team but outside the aegis of a formal governance
organization. We believe that this choice was prudent to allow us to develop a preliminary proposal for community
feedback. That being said, we recognize that broader community feedback, contributions, and ultimate adoption,
particularly at an international level, would benefit from and may require a more formalized process and institutional
home. One putative organizational home would be the Inter-Agency Space Debris Coordination Committee (IADC),
which is composed of representatives from a select set of national space agencies, with access to high quality data
and considerable experience and expertise. Particularly if there was an IADC structure that could support broader
community involvement beyond national space agencies, it could be an ideal institutional home for the continued
development and stewardship of the SEPs.
Future work will simulate each reference scenarios using the provided modeling inputs and different evolutionary
space environment models to help validate the project concept and design choices. After the scenario designs are
finalized, a set of modeling outputs for each scenario will be generated to support secondary modeling and
derivative analysis.
Acknowledgements
This work was funded by the Department of Commerce, NOAA, Office of Space Commerce. The content of this
presentation does not necessarily reflect the position or the policy of the United States Government. No official
endorsement should be inferred.
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Appendix A.
Trackable 10 cm 10 cm 5 cm 5 cm
Object Size All sats trackable All sats trackable
(char. length)
Post-Mission Compliance Time Limit: Compliance Time Compliance Time LLCs use check-out
Disposal 25 years Limit: 25 years for Limit: 5 years* [42, pp.altitudes, checkout alt.
(PMD) non-constellation 15, sec. 7.i] lifetime <= 5 years [43, p.
Defence/Civil: 65% [33, traffic 5.4.2.4a]
p. 93] General PMD: 90%
5 years for [43, p. 5.4.1.1a] LLC LEO PMD: 99% w/in 5
Commercial/Amateur/ constellations* years*
Cubesat: 95% [33, p. Large LEO
102] Defence/Civil: 70% Constellations (LLCs) LEO PMD w/in 5 years:
use check-out altitudes 95% [42, pp. 12, sec. 5.a]
R/B: 90% [33, pp. 98- Commercial/Amateur/ [43, p. 5.4.2.4]
100] Cubesat: 98% [33, p. LEO PMD w/in 25 years:
102] 99% [42, pp. 12, sec. 5.a]
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R/B: 90% [33, pp. 98- Commercial/Amateur/ R/B: 98% [43, p. 5.4.1.1a]
100] Cubesat: 98% [33, p.
102]
ADR (2030 None 5 large objects per year 10 large objects per 15 large objects per year
onwards) year
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