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    Home»Space»Solar Eclipses on Demand: Proba-3’s Precision Satellites Enter Orbit
    Space

    Solar Eclipses on Demand: Proba-3’s Precision Satellites Enter Orbit

    By European Space Agency (ESA)December 14, 2024No Comments7 Mins Read
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    Proba-3 Occulter Eclipsing Sun for Coronagraph Spacecraft
    The two spacecraft of Proba-3 fly in precise formation about 150 m apart to form an external coronagraph in space, one spacecraft eclipsing the Sun to allow the second to study the otherwise invisible solar corona. Credit: ESA-P. Carril

    Proba-3, a collaboration among 14 ESA Member States and Canada, was launched to facilitate autonomous space operations and precision maneuvering. The mission focuses on the solar corona, aiming to fill critical observational gaps and advance the capability for precision formation flying in space.

    Two spacecraft launched on December 5 from India, marking a breakthrough in space mission technology. ESA’s twin Proba-3 satellites will fly in precise formation, maintaining accuracy within a single millimeter — functioning as if they were one giant spacecraft. This advanced coordination will allow them to create artificial solar eclipses in space, enabling extended observations of the Sun’s faint outer atmosphere, the corona.

    Proba-3 Mission Launch

    Fourteen ESA Member States including Canada collaborated on the Proba-3 mission to showcase cutting-edge European technology. The mission aims to advance autonomous space operations and precision satellite maneuvering while unlocking unprecedented scientific discoveries.

    Proba-3 launched aboard a four-stage PSLV-XL rocket from the Satish Dhawan Space Centre in Sriharikota, India, on December 5 at 11:34 CET (10:34 GMT, 16:04 local time). Approximately 18 minutes after liftoff, the mission’s two satellites separated from the rocket’s upper stage.

    Proba-3 PSLV-XL Liftoff
    Proba-3 lifted off on its PSLV-XL rocket from Satish Dhawan Space Center in Sriharikota, India, on Thursday, December 5, at 11:34 CET (10:34 GMT, 16:04 local time). Credit: ISRO

    The satellites will remain connected during the initial commissioning phase, which will be managed by mission control at the European Space Security and Education Centre (ESEC) in Redu, Belgium.

    Dietmar Pilz, ESA Director of Technology, Engineering and Quality notes, “Proba-3 has been many years in the making, supported through ESA’s General Support Technology Programme fostering novel technologies for space. It is an exciting feeling to see this challenging enterprise enter orbit.”

    Proba-3 Stack on Way to Orbit
    Artist’s view of Proba-3 on an ISRO PSLV-XL launch vehicle. Credit: ESA – P. Carril

    Partnerships and Technological Challenges

    Proba-3 mission manager Damien Galano adds, “Today’s liftoff has been something all of us in ESA’s Proba-3 team and our industrial and scientific partners have been looking forward to for a long time. I’m grateful to ISRO for this picture-perfect ascent to orbit. Now the hard work really begins, because to achieve Proba-3’s mission goals, the two satellites need to achieve positioning accuracy down to the thickness of the average fingernail while positioned one and a half football pitches apart.”

    Proba-3 Separation From PSLV-XL Upper Stage
    Artist’s view of Proba-3 separating from its ISRO PSLV-XL launch vehicle’s upper stage. Credit: ESA-P. Carril

    “We are honored that ESA entrusted NewSpace India Limited, NSIL, with its Proba-3 mission, and we are extremely satisfied to have delivered the satellites precisely into their designated orbit,” remarked Radhakrishnan Durairaj, Chairman and Managing Director of NSIL. “This is an extremely ambitious mission, with an ambitious orbit to go with it: the satellites have been placed into a highly elliptical orbit which extends more than 60 500 km from the surface of Earth. Reaching this orbit required the most powerful PSLV-XL variant of our launcher, equipped with additional propellant in its six solid rocket boosters.”

    Proba-3 Orbit
    The paired Proba-3 satellites will have a highly elliptical orbit with an apogee (or top of orbit) of around 60,000 km and a perigee of 600 km. Coronagraph observation is based on forming an artificial eclipse between the two satellites as well as active formation flying experiments taking place towards apogee, with passive formation flying taking place as the satellites circle closer to Earth. Credit: ESA – P. Carril, 2013

    Advanced Solar Observations and Scientific Goals

    Up around the top of their orbits the Proba-3 Occulter spacecraft will cast a precisely controlled shadow onto the Coronagraph spacecraft around 150 m away, to produce solar eclipses on demand for six hours at a time.

    “There was simply no other way of reaching the optical performance Proba-3 requires than by having its occulting disc fly on a separate, carefully controlled spacecraft,” explains ESA’s Proba-3 mission scientist Joe Zender. “Any closer and unwanted stray light would spill over the edges of the disc, limiting our close-up views of the Sun’s surrounding corona.”

    Proba-3 Occulter and Coronagraph Spacecraft
    The Proba-3 Occulter (forward) and Coronagraph (background) spacecraft in a cleanroom for testing at Redwire Space in September 2024. Credit: Redwire Space

    “Despite its faintness, the solar corona is an important element of our Solar System, larger in expanse than the Sun itself, and the source of space weather and the solar wind,” explains Andrei Zhukov of the Royal Observatory of Belgium, Principal Investigator for Proba-3’s ASPIICS (Association of Spacecraft for Polarimetry and Imaging Investigation of the Corona of the Sun) coronagraph.

    “At the moment we can image the Sun in extreme ultraviolet to image the solar disc and the low corona, while using Earth- and space-based coronagraphs to monitor the high corona. That leaves a significant observing gap, from about three solar radii down to 1.1 solar radii, that Proba-3 will be able to fill. This will make it possible, for example, to follow the evolution of the colossal solar explosions called Coronal Mass Ejections as they rise from the solar surface and the outward acceleration of the solar wind.”

    Proba-3 Mission Control at ESEC
    Proba-3’s mission control center at ESEC in Redu, Belgium. Credit: ESA-S. Blair

    Impact and Future Potential of the Mission

    ESA Director General Josef Aschbacher commented, “Proba-3’s coronal observations will take place as part of a larger in-orbit demonstration of precise formation flying. The best way to prove this new European technology works as intended is to produce novel science data that nobody has ever seen before.

    “It is not practical today to fly a single 150-m long spacecraft in orbit, but if Proba-3 can indeed achieve an equivalent performance using two small spacecraft, the mission will open up new ways of working in space for the future. Imagine multiple small platforms working together as one to form far-seeing virtual telescopes or arrays.”

    Proba-3 Spacecraft Infographic
    Lined up with the Sun, Proba-3’s Occulter spacecraft uses its occulting disc to cast a precisely-controlled shadow onto the Coronagraph spacecraft. The pair host multiple positioning technologies to achieve millimeter level precision: GNSS receivers, radio links, optical cameras tracking flashing LEDs, a reflected laser, and shadow-detecting sensors. Credit: ESA-F. Zonno

    If Proba-3’s initial commissioning phase goes to plan then the spacecraft pair will be separated early in the new year to begin their individual check-outs. The operational phase of the mission, including the first observations of the corona through active formation flying, should begin in about four months.

    The Proba-3 mission was led by Sener in Spain on behalf of ESA, coordinating contributions from 14 ESA Member States and Canada. Airbus Defence and Space in Spain built the spacecraft, while Redwire Space in Belgium handled the spacecraft’s avionics, assembly, and operations. CSL in Belgium developed Proba-3’s ASPIICS coronagraph, and Spacebel, also based in Belgium, created the onboard and ground segment software. GMV was responsible for the formation flying system and flight dynamics.

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    Astronomy Astrophysics European Space Agency Popular Proba-3 Sun
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