A Space Debris Alert System for Aviation. US Patent pending Inventor: T. Sgobba - ESA Independent Safety Office

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A Space Debris Alert System for Aviation US Patent pending Inventor: T. Sgobba - ESA Independent Safety Office

Re-entry breakup basics Space systems in LEO reenter naturally at very shallow angle (<1 degree). Location of uncontrolled reentries is unpredictable Major breakup at ~78 km 10 to 40% of mass survives reentry and impacts the Earth s surface posing hazard to people and property (e.g. of the ATV-1 mass of 12.3 tons about 3.5 tons in 183 fragments survived re-entry, 28.4% of mass) Debris spread over long, thin ground footprint (e.g. for ATV ~ 817km by 30km) Texas, 1997 Saudi Arabia, 2001 30 kg Mongolia, 2010 Brazil, 2012 South Africa, 2000 250 kg 250 kg 250 kg

Space debris as re-entry risk 1. Over 20000 tracked objects (objects larger than 10 cm diameter) a. 1000 operating satellites b. Over 13000 tracked objects in Low Earth Orbit (LEO) 2. ~40 large debris objects (>800 kg) reenter randomly per year. 38 large debris objects have reentered since the beginning of 2012. a. Dead satellites (e.g., UARS, ROSAT, Phobos-Grunt) b. Launch upper-stages (the upper-stage of Zenit-2SB that launched Phobos- Grunt reentered 2 weeks later, mass > of UARS+ROSAT). 3. Reentry within 25 years is recommended end-of-mission disposal option for LEO objects a. Controlled reentry to safe oceanic area for objects with casualty expectation exceeding defined limit (1x10-4 for US, 2x10-5 for France ) b. Random reentry acceptable in US (exceptionally acceptable in France) for objects with risk lower than 1x10-4

Space debris as re-entry safety risk 1. Currently most large objects in LEO exceed the 1x10-4 risk limit but lack the capability to perform a controlled reentry (e.g. UARS estimated risk was 1 in 3200)

Estimating safety risk 1. Models predict number, size, mass of surviving debris 2. Debris will fall in latitude band defined by orbit inclination 3. Risk estimated for objects with enough kinetic energy to cause injury or death on ground (> 15 Joules in U.S.) 4. Risk estimated based on population density within latitude band 5. Currently no estimate is performed of risk for aviation

Like a skipping pebble 1. Precise location of space debris reentry point (defined altitude prior to breakup) impossible to predict for uncontrolled reentries 2. At very shallow angle of reentry a spacecraft behavior when approaching the upper layers of the atmosphere is similar to a pebble skipping across the surface of a pond. (in 1930s Eugen Sänger proposed using such skipping effect to increase the range of a suborbital bomber)

Current reentry predictions capability 1. Generally assume ±10-25% error in time of reentry due to atmospheric and drag uncertainties a. Example: Prediction made with tracking data 1 orbit revolution (90 minutes) from reentry has ±9 minute error Object travelling at 7.5 km/sec x ±9 minutes ±4050 km uncertainty in reentry location 2. The US official source of reentry predictions for uncontrolled reentry is USSTRATCOM s Joint Space Operations Center (JSpOC).TIP (Tracking and Impact Prediction) messages released at intervals (T-4 days, T-3 days, T- 2 days, T-1 day, T-12 hrs, T-6 hrs,t-2hours) 3. The IADC (Inter-Agency Space Debris Coordination Committee) performs annually reentry predictions exercises. Results are not released to the public

Where will fragments land? 1. Impact point for surviving fragments also impossible to predict a. Spread of fragments will depend on where fragments released, flight characteristics of each fragment b. Fragments impact many kilometers from each other c. Local wind can be significant factor 2. Uncertainties are addressed by footprint probability boxes (e.g. 1x10-5, and 1x10-2 ) 3. Footprint probability boxes are routinely used to determine re-entry maneuvers for controlled re-entries (e.g. ATV)

Risk for aviation (video clip not for public distribution)

Risk for aviation 1. Casualty expectations for people in commercial aircraft exposed to the risk of falling fragments after Shuttle Columbia disintegration was 0.3 2. On average >27 fragments from random re-entry exceeds specified limit for aircraft in hazard area 3. The core area of Europe has one of the highest air traffic density in the world 4. On Sunday 15 January 2012, in the middle of the Russian Phobos-Grunt uncontrolled re-entry window, the EUROCONTROL Network Management Operations Centre received an international NOTAM from Russian authorities, requesting European States to close their airspace for two hours 5. Closing the European airspace for 2 hours could cost up to 20 Mln of Euro

Risk for aviation 1. The US Federal Aviation Administration (FAA) Office of Commercial Space Transportation (AST) and the US Department of Defence co-sponsored the development of Aircraft Vulnerability Models (AVMs) to quantify the areas of aircraft susceptible to catastrophic or emergency outcome (e.g. fuselage penetration, fuel tank rupture) following impact with falling space debris. A fragment > 300gm is generally considered catastrophic.

R&D to reduce re-entry hazards 1. ESA TEC-QI is promoting operational testing and use of new instruments recording what happens during breakup and providing precise information on debris impact locations Reentry Breakup Recorder assembly (recorder is inside heat shield) a. Reentry Breakup Recorder (REBR) developed by The Aerospace Corporation collected data on re-entry breakup of JAXA s HTV-2 and -3 and on ESA s ATV-3 cargo vehicles b. REBR provided data on its trajectory and impact location 2. REBR data are meant to help improve breakup and hazard prediction models Reentry Breakup Recorder during pre-flight testing

R&D to reduce re-entry hazards 1. Currently REBR includes: a. Two three-axis accelerometers, one with a 2-g maximum level and a second with 200-g maximum level (the low-level is part of the re-entry detection system; the high-g accelerometer captures higher accelerations expected during re-entry and breakup) b. Rate gyro, which captures angular rates about the three REBR axes c. GPS receiver d. Heat shield temperature sensors 2. Data from sensors is collected and recorded for several minutes during re-entry, then an Iridium modem is activated which makes a call and downloads recorded data

ESA re-entry observation campaigns 1. The destructive re-entry of ATV-1 Jules Verne occurred on the 29th September 2008. ESA organized with NASA the first ever multi-aircraft reentry observation campaign aiming at: a) characterizing fragmentation and explosive events, including altitude of explosion, identification of likely cause (e.g. fuel tank rupture) and resulting fragments; c) characterizing ablation products and demise; d) reconstructing fragments trajectories and impact points 2. A second observation campaign is being proposed for ATV-4 as part of a multi-year ISS reentry vehicles observation program

Localizing the footprint

Localizing the footprint 1. Length of predicted impact zone depends on observation altitude 2. Most accurate prediction for observation at primary breakup altitude 3. On average, first fragment reaches the airspace (i.e. 18km) ~10 minutes after breakup 4. Last fragment reaches ground ~26 minutes after breakup

Re-entry Direct Broadcasting Alert System 1. The Re-entry Direct Broadcasting Alert System (R-DBAS) works as a smart fragment which can autonomously determine its own position during re-entry, and which knows its relative location in the projected hazard area (footprint probability box), which has been pre-computed on ground. 2. The R-DBAS allows to directly broadcast related alerts to potential users within the time falling fragments take to reach altitudes used by aviation or to reach Earth surface.

R-DBAS description 1. The Re-entry Direct Broadcasting Alert System (R-DBAS) consists of two units: an On-board Unit and a Receiver-Display Unit: a. The On-Board Unit consists essentially of a Global Positioning System (GPS) tracking device, a central processing unit (CPU), memories and software, transmitter, and antennas. The On-board Unit includes also an aerodynamically shaped housing and related heat shield, power storage/distribution unit, and switching device. b. The Receiver-Display Unit consists of receiver device, antenna, and display system.

R-DBAS: On-board Unit 1. The housing that attaches the R-DBAS On-board Unit to the host vehicle is designed to protect the unit from debris impacts during breakup, but to release the unit when exposed to significant aerodynamic heating. In addition the breaking or melting of one or more electrical wires connecting the R-DBAS Core Unit to the space system will close the power circuit thus switching on the unit. The R-DBAS On-board Unit housing is aerodynamically shaped to stabilize during the descent. The overall mass and drag of the R-DBAS Core Unit is optimized such to achieve a ballistic coefficient that allows direct alert broadcasting coverage of the entire hazard area and of vicinity. 2. After activation the On-board unit acquires the GPS signal and determines its own state vector, then it computes longitudes/latitudes of the hazard area (box corners) by using stored algorithm/data on size and shape of hazard area, and finally broadcasts the hazard areas geographical coordinates to any Receiver-Display Unit in the hazard areas and in their vicinity.

R-DBAS: Receiver-display unit 1. The Receiver-Display unit will receive in real-time the hazard area geographical coordinates and display them as a simple alphanumeric message on a computer screen or digital mobile phone, or against a map backdrop. The Receiver-Display unit may be integrated or adapted to existing computer and display systems, and include user s GPS location to track user s relative position with reference to hazard area. 2. The Receiver-Display unit can be carried or installed on airplanes, ships, boats, offshore platforms, ground vehicles, on personal and mobile communication devices, and on centralized computer systems. By receiving the alert notification, collision avoidance or escape maneuvers may be performed or the user may need to take shelter.