IXV mission recap

ESA's IXV
02 JUL. 2014 publication date 21507 Views

The IXV project developed and tested in flight the technologies and critical systems for Europe’s future autonomous controlled reentry for return missions from low Earth orbit.

The experimental vehicle is 5 m long, 1.5 m high, and 2.2 m wide – about the size of a car – and weighs almost 2 t.


Launch and recovery

IXV was injected into a suborbital path by a Vega rocket launched from Europe’s Spaceport in French Guiana on 11 February 2015. IXV separated from Vega at an altitude of 340 km. It attained an altitude of around 412 km, allowing it to reach a speed of 7.5 km/s when reentering the atmosphere at an altitude of 120 km – fully representative of any return mission from low orbit. It collected a large amount of data during its hypersonic and supersonic flight, while being controlled by thrusters and aerodynamic flaps.

The craft then deployed a parachute to slow its descent for a safe splashdown in the Pacific Ocean to await recovery and analysis.

The complete mission lasted for approximately 1 hour and 40 minutes.


IXV mission overview

Mission operations

The Mission Control Centre at the Advanced Logistics Technology Engineering Centre (ALTEC) in Turin, Italy, closely monitored IXV during its mission. This facility was also in charge of coordinating the activities of the entire ground segment, including the fixed ground stations in Libreville, Gabon and Malindi, Kenya, and the naval station on the recovery ship in the Pacific Ocean.


Space and ground segment activities

2014

May

IXV integration & qualification (Turin, Italy)

Jun–Aug

IXV environmental tests (Noordwijk, The Netherlands)

Aug–Sep

IXV flight & ground segments deployment (worldwide)

2015

Jan–Feb

IXV ground segment launch campaign (worldwide)

Jan–Feb

IXV flight segment launch campaign (Kourou)

Feb

Launch, mission & recovery (Kourou)


Applications for controlled atmospheric reentry vehicles

  • Reusable launchers stages (lower and upper),

  • Robotic exploration (for example, sample return from Mars or asteroid),

  • Servicing of orbital infrastructures (for example, International Space Station),

  • Servicing of future generation satellites (for example, in-orbit refuelling or disposal),

  • Microgravity experiments (for example, optimum time/cost ratio),

  • Earth sciences (for example, high-altitude atmospheric research),

  • Earth observation (for example, crisis monitoring).


PRIDE mission

Looking to the future

The knowledge gained from the IXV mission will be key in ESA’s future plans involving applications requiring controlled atmospheric reentry.


Related links

fallback image 2


stay updated

Subscribe to our newsletter to receive the latest news, mission updates, and exclusive insights directly in your inbox. Be the first to know about our upcoming projects and breakthroughs.