Spaceports Guiana Space Centre Esrange. A thin, heat resistant shell made of CMC Ceramic Matrix Composite is designed to withstand mechanical loads due to extreme heat fluxes while maintaining the outer aerodynamic line of the vehicle. It was recognised that, in order for significant progress to be made, FLPP would require the production and testing of a prototype reentry vehicle that drew on their existing research, technologies, and designs. The Navigation function is based on linear acceleration and attitude measurements improved with GPS position and velocity updates and Drag Derived Altitude pseudo-measurements during the GPS blackout phase. The entire experiment telemetry was flawlessly transmitted to the naval station during the descent phase managing realtime storage and five complete delayed TM playbacks during the visibility window. The thruster uses the catalytic decomposition of hydrazine monopropellant over a heated catalyst bed with redundant heater units. The system also uses a store and playback mechanism that downlinks data in real time when a ground station is visible and plays back stored data from periods of LOS Loss of Signal.

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IXV was delivered to the launch site in September to be loaded with propellants and installed on the Vega launcher for liftoff. Four N thrusters and two aerodynamic flaps, located at the base of the vehicle.

IXV first results

The planning for the second spaceflight was originally to begin during Marchwhile design work on the modified vehicle was to commence during mid The first results of the IXV mission telemetry analyses are reported for the three avionics subsystems. Signals from the spacecraft were tracked by two ground stations in Africa and by an antenna on the recovery ship, Nos Aries, in the Pacific.

In the event of high flap deflection, the shock forming upstream the flap hinge will induce a separation and reattachment shock — a phenomenon that is hoped to be characterized with this experiment since it has a significant effect on the efficiency of the flap system. They are used to measure the forces on the ixg stand-offs on the nose cone and the windward thermal protection system.


The acquired data is encapsulated into data packets and delivered to the Network Gateway via the Network Switch.

Europe’s Newly Tested Space Plane Aims for Next Launch in 2019

It was designed and developed to support data, voice and video transmission. The attitude is also driven by the requirement to ensure proper zenith-pointing of the GPS antenna which idv done by having the craft follow a pre-determined attitude profile stored in the flight computer — consisting of desired attitude as a function of vehicle longitude.

The RTC subsystem provides the transmission capabilities to downlink, in a redundant scheme with respect to on-board recorders, the telemetry data and to receive GPS signal for navigation purposes.

The experimental vehicle is 5 m long, 1. The IMU delivers data at a speed of Hz through the data bus. The Data Handling Subsystem of the IXV spacecraft consists of two elements — one handling spacecraft telemetry and commands, and one collecting data from the experimental flight sensors. The main elements that are demonstrated by IXV include the development of a system capable of returning from Low Earth Orbit with a lifting system that is capable of reaching ixf large down range distance with significant cross-range capability using a combination of rockets and aerosurfaces.

Z9 operates at a nominal thrust of 22, Kilogram-force. A metallic dome is fastened to the ring, and provides support to the insulating layers. It was developed to serve as a prototype spaceplane to validate the ESA’s work in the field of reusable launchers.

IXV / Space Transportation / Our Activities / ESA

The IXV technology demonstration spaceplane was launched on Feb. The Base Flow Field Experiment uses a series of sensors on the base of the vehicle to deliver data on the separated base flow in the various lxv environments which is hard to model and often leads to large errors in the estimation of the drag coefficient and other parameters when only using computational data.

The focus of activity on flight day will be the MCC, housed at the Advanced Logistics Technology Engineering Center, in Turin, Italy, which will coordinate the entire ground segment, including the 10 m diameter dishes in Libreville Gabon and Malindi Kenyaand the tracking antenna on the recovery ship, Nos Aries. The Flush Air Data System aims to derive precise vehicle attitude in the form of angle of attack, angle of sideslip and atmospheric properties from pressure and temperature measurements taken at the nose of the vehicle.


Note that the white color is due to the accumulation of salt resulting from the immersion in sea water after splashdown. CMC skins, insulation material and attachment system. It is also in charge of encoding the Vital Layer Kxv and storing it onboard as well as downlinking it to the ground. As an experimental vehicle primarily intended to gather data, various assorted sensors and monitoring equipment are present and operational throughout the full length of the flight in order to gather data to support the evaluation effort, including the verification of the vehicle’s critical reentry technologies.

The EPS primary aim is to provide and distribute electrical power to the vehicle throughout the entire mission: The IVX is supported on-orbit by a separate manoeuvring and support module, which iixv largely similar to the Resource Module that had been intended for use by the cancelled Hermes shuttle.

Intermediate eXperimental Vehicle – Wikipedia

The nose assembly is derived from the windward technology to maximize synergies. IXV, still packed inside its container, will then travel to Turin for inspection and further analysis. Atmospheric re-entry vehicle by the European Space Agency. In a world first, Europe will launch and land an unmanned spaceplane that has no wings but instead features an aerodynamic shape that produces the lift to fly through the atmosphere.

Given their installation location, the strain gauges have to be able to withstand high temperatures. The RF links, with receiving stations located in Libreville and Malindi, was stable and continuous with no intermediate transition gap.

The system has been designed to keep the spacecraft afloat for 48 hours in order to allow an extended recovery operation. The S-band downlinks, guaranteed by the RTC subsystem, allowed for complete telemetry download to the ground.

Its end-to-end European mission on the Vega launcher is planned for February