RBS 77 Extended Range Aerospace Defense System
System Overview:
The RBS 77 ERADS is a rapidly deployable, highly mobile upper-tier ballistic missile defense (BMD) system designed to protect corps to field army units, military facilities, and civilian infrastructure from medium to intercontinental range ballistic missiles by intercepting them in their terminal phase with hit-to-kill interceptors. A full RBS 77 ERADS Battery consists of eight truck mounted launchers with six interceptors each, a trailer mounted X band extended long range acquisition and tracking radar which can track and discriminate incoming missiles and update tracking information for launched interceptors, and a fire control and communications vehicle which controls battery operation and which can communicate with other air defense sensors and systems to allow the RBS 77 ERADS system to be seamlessly integrated into a larger integrated air-defense network. The entire RBS 77 ERADS is system is road mobile and can be transported by either ship, rail, or strategics airlifter aircraft in order to allow the entire system to be rapidly deployed around the globe where needed.
Rb 77 interceptor
- Weight: 2,000 kg
- Length: 6.6 m
- Diameter: 0.56 m
- Propulsion: Two-stage solid fuel rocket
- Operational Range: 1,000 km
- Intercept Altitude: 20-500 km
- Speed: 5.5 km/s (Mach 18)
- Warhead: none- KE hit to kill
- Guidance: dual-band infrared FPA
- Steering: Thrust-vectoring, solid DACS
- Launcher: Trailer based launcher with six canisters
The Rb 77is a anti-ballistic missile interceptor designed to provide hit-to-kill terminal phase intercept of intercontinental ballistic missile (ICBM) and submarine-launched ballistic missile (SLBM) reentry vehicles, maneuvering reentry vehicles (MaRVs), and hypersonic glide vehicles (HGVs). The Rb 77 interceptor consists of a two-stage solid-fuel rocket booster and an endo/exo-atmospheric kill vehicle. The two booster stages employ graphite filament wound epoxy casings with 3-D carbon-carbon nozzles and employs a high performance HNF/AL/GAP composite propellant consisting of 60% HNF (Hydrazinium nitroformate) oxidizer, 20% Aluminum fuel, and 20% GAP (Glycidyl azide polymer) energetic binder. The first stage weighs 1,300 kilograms, has a specific impulse of 270 seconds, and burns for six seconds, accelerating the interceptor to a first stage burnout velocity of 2.4 km/s where the second stage separates and ignites. The first stage employs an electromechanical actuator (EMA) based gimballed nozzle with +/- 7.5° gimbal angle which is used for first-stage thrust vector control. The second stage weighs 450 kilograms, has a specific impulse of 290 seconds, and features a dual-pulse motor with two 4.5 second burns and provides additional acceleration and divert capability for the kill vehicle. The second stage features a thrust vectoring nozzle with a +/- 7.5° gimbal angle and features an integral warm-gas/cold-gas attitude control system (ACS) built into the aft end of the second stage motor which combines a cold-gas system (CGS) using compressed nitrogen thrusters and and warm-gas system (WGS) using solid-propellant gas generators and nozzles which provide roll, pitch, and yaw control while the second stage motor is firing or while the stage is coasting in between motor pulses. The interceptor's endo/exo-atmospheric kill vehicle weighs approximately 75 kg and employs a solid-propellant divert and attitude control system (DACS) for maneuvering. The kill vehicle DACS employs a total of 10 thrusters with variable-area pintle nozzles which allow each thruster to be throttled from 0-100% of maximum thrust for precise in-flight control. The 10 DACs thrusters provide roll, pitch, and yaw control during the terminal phase of intercepts and provide the kill vehicle with over 2.0 kilometers per second of divert delta-V with the ability to maneuver at up to 100 g.
The kill vehicle employs a dual-band imaging infrared (IIR) seeker which is used to provide endo and exo-atmopsheric target discrimination and tracking capability. The seeker uses a radiation hardened 512 x 512 pixel dual-band (MWIR and LWIR) digital-pixel focal plane array (FPA) with a 48 by 48° overall field of view mounted to a 2-axis stabilized AlBeMet alloy optical telescope assembly with selectable wide and narrow field-of view (WFOV and NFOV) modes which are selected in-flight based on whether the intercept is endo or exo-atmospheric. The optical assembly employs active line-of-sight (LOS) stabilization using the 2-axis stabilized telescope and a 6-axis laser-ring gyro IMU to provide sub-pixel image stabilization capability while the kill vehicle maneuvers at up to 100 g. Seeker acquisition range against a typical ICBM RV varies from 40 kilometers for endo-atmopsheric intercepts to over 300 kilometers for exo-atmospheric intercepts. The measurements from the seeker are combined with body orientation measurements from the 6-axis laser-ring gyro IMU based altitude reference system (ARS) built into the kill vehicle which when combined with the DACS thruster system steers the kill vehicle onto the correct interception trajectory after it has detected its target. The seeker window is mounted off-axis to the kill vehicle line of sight and employs a diamond/silicon optical window actively cooled with cold nitrogen gas pumped through internal micro-cooling channels for endo-atmospheric intercepts. The cooling system is designed to allow the infrared window to survive exposure to extreme hypersonic heating and also to provide minimal flow interference so that the infrared seeker can effectively acquire its target. For exo-atmospheric intercepts the seeker window is ejected with non-explosive actuators in order to remove residual heating effects and improve seeker sensitivity. The kill vehicle and interceptor have three selectable guidance modes depending on whether launch commit and target intercept happen in the endo or exo-atmospheric phases of flight including exo-commit/endo-intercept, endo-commit/endo-intercept, and exo-commit/exo-intercept:
Exo-commit/endo-intercept: In this mode a mid-course sensor tracks the target vehicle or target cluster in its midcourse phase while it is still travelling through the exoatmosphere and queues the interceptor to launch where the interceptor then launches and intercepts the target as it enters the upper endoatmosphere. After launch the first stage burns and is discarded where depending on the intercept range the second stage is either immediately ignited (for shorter range intercepts) or the interceptor coasts before igniting the second stage (for longer ranged intercepts). After the first pulse of the second stage burns out the interceptor coasts towards the target where the second stage warm-gas/cold-gas attitude control system is used to steer the vehicle towards the desired intercept point. When the interceptor closes to within seeker range the shroud over the kill vehicle seeker is jettisoned and the kill vehicle's dual-band infrared seeker begins a wide field-of-view (WFOV) sweep of the target area. The dual-band seeker is used to discriminate the warhead from decoys in the target cluster. When the seeker has locked onto the desired target the second pulse of the second stage is ignited and the kill vehicle's solid-propellant DACS thrusters are used to steer and accelerate the kill vehicle towards the target. After second pulse burnout the kill vehicle separates from the second stage and uses its DACS thrusters to perform the final steering and corrective maneuvers before hitting the target.
Endo-commit/endo-intercept: This mode is similar to exo-commit/endo-intercept except the interceptor is launched while the target is being tracked as it re-enters the atmosphere by a terminal sensor with the target intercept happening in the lower atmosphere. In this mode there is no coast between first and second stage motor burns or between the second stage pulses with kill-vehicle shroud jettison and kill-vehicle seeker target acquisition happening during first and second stage motor burn. After second stage burn the kill vehicle separates and the kill vehicle DACS for endgame maneuvering before impact with the target.
Exo-commit/exo-intercept: In this mode target tracking, discrimination, and commit and intercept happen while the target is travelling through the exo-atmosphere in its midcourse phase. Flyout and intercept are similar to exo-commit/endo-intercept mode except the coast between first stage burnout and second stage ignition is typically much longer. In this mode target discrimination is performed by the midcourse sensor with the interceptor correlating its seeker scene in NFOV mode with that of the midcourse sensor for terminal target acquisition and homing. This mode also lets the interceptor act as an ASAT (anti-satellite) missile with the capability to intercept satellite targets in low-earth orbit.
FMG 330 Extended Range Acquisition and Tracking Radar
- Weight: 30,000 kg
- Length: 13.0 m
- Height: 3.6 m
- Frequency: 8-12 GHz (X-band)
- Peak Power: 1.1 MW
- Average Power: 80 kW
- Instrumented Range: 3,000 km
- Tracking Range (1m2 RCS ballistic missile): 1,500 km
- Detection sector: 120 deg
- Engagement sector: 90 deg
- Target Capacity: 100 simultaneous