Kessler Syndrome: System Dynamics Model
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F18%3A10392051" target="_blank" >RIV/00216208:11320/18:10392051 - isvavai.cz</a>
Nalezeny alternativní kódy
RIV/00216224:14230/18:00104837
Výsledek na webu
<a href="https://doi.org/10.1016/j.spacepol.2018.03.003" target="_blank" >https://doi.org/10.1016/j.spacepol.2018.03.003</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.spacepol.2018.03.003" target="_blank" >10.1016/j.spacepol.2018.03.003</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Kessler Syndrome: System Dynamics Model
Popis výsledku v původním jazyce
The present article explores the Kessler syndrome (the potentially catastrophic accumulation of debris in the low-earth orbit) through system dynamics methodology. It models satellites and three classes of debris, their fragmentation, interactions, and gradual decay over 50 years. It presents 5 scenarios: (a) a "business as usual" approach, which leads to exponential accumulation and growing rate of satellite losses, but no catastrophic chain reaction; (b) a conflict with a large-scale deployment of antisatellite weapons, leading to an accelerated accumulation and losses, but still no chain reaction; (c) electromagnetic pulse scenario modeling loss of control over satellites en masse; (d) cessation of all low earth orbit (LEO) satellite launches, illustrating high inertia of the system, which continues to produce more debris; and (e) scenario representing an attempt to mitigate the situation via direct removal of some portion of inactive satellites from the LEO. All scenarios take place in 2040. The article demonstrates the gravity of the situation and the necessity for a sustainable long-term solution, as orbital debris poses a threat to our future space operation even without triggering a catastrophic chain reaction.
Název v anglickém jazyce
Kessler Syndrome: System Dynamics Model
Popis výsledku anglicky
The present article explores the Kessler syndrome (the potentially catastrophic accumulation of debris in the low-earth orbit) through system dynamics methodology. It models satellites and three classes of debris, their fragmentation, interactions, and gradual decay over 50 years. It presents 5 scenarios: (a) a "business as usual" approach, which leads to exponential accumulation and growing rate of satellite losses, but no catastrophic chain reaction; (b) a conflict with a large-scale deployment of antisatellite weapons, leading to an accelerated accumulation and losses, but still no chain reaction; (c) electromagnetic pulse scenario modeling loss of control over satellites en masse; (d) cessation of all low earth orbit (LEO) satellite launches, illustrating high inertia of the system, which continues to produce more debris; and (e) scenario representing an attempt to mitigate the situation via direct removal of some portion of inactive satellites from the LEO. All scenarios take place in 2040. The article demonstrates the gravity of the situation and the necessity for a sustainable long-term solution, as orbital debris poses a threat to our future space operation even without triggering a catastrophic chain reaction.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10201 - Computer sciences, information science, bioinformathics (hardware development to be 2.2, social aspect to be 5.8)
Návaznosti výsledku
Projekt
—
Návaznosti
S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2018
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Space Policy
ISSN
0265-9646
e-ISSN
—
Svazek periodika
44-45
Číslo periodika v rámci svazku
AUG
Stát vydavatele periodika
GB - Spojené království Velké Británie a Severního Irska
Počet stran výsledku
11
Strana od-do
29-39
Kód UT WoS článku
000454381000003
EID výsledku v databázi Scopus
2-s2.0-85043989302