Gaia space telescope measures our Solar System’s acceleration



Credit: ESA/Gaia/DPAC / CC BY-SA 3.0 IGO

What is Gaia? The aim of the ESA mission, launched on December 19, 2013, is nothing less than to produce a three-dimensional map of all astronomical objects that can be detected by the satellite’s 1000 megapixel camera – an impressive average of three million stars per hour. The observations are so accurate that Gaia could trace a motion of only a few centimeters for objects that are as far away as the Moon. An international team of scientists generates scientifically usable results from this enormous amount of observational data. This calculation, the iterative solution of a huge system of equations with 10 billion unknowns, has kept supercomputers in several European research institutions busy since 2015. Among those, TU Dresden’s high performance computers were heavily demanded by Prof. Klioner’s team to produce the numerous interim solutions which finally resulted in decisive improvements of the new Gaia products.

The excellent quality of these results enabled the scientists in Dresden to detect a highly interesting phenomenon: The acceleration of our Solar System. In astronomy, it has been known for a while that such an acceleration causes a slow, apparent displacement of all astronomical objects, which should become noticeable as a global pattern in the measured motions. However, for nearby stars, this effect is completely superposed by the complex structure and dynamics of our Galaxy.

Only a precise measurement of extremely distant astronomical objects, so-called quasars, could reveal this acceleration effect. These extremely luminous nuclei of distant galaxies are considered to be almost fixed on the sky, which is why they are used in astronomy as reference points.

The Dresden team identified about 1.6 million Gaia objects to be quasars, which will now be published as a Gaia own celestial reference system. These quasars clearly show the expected motion pattern of the extremely small acceleration, which, according to the results produced in Dresden, is 0.23 nanometers per second squared. It is the first time that this detection is obtained using optical observations. Professor Klioner explains:

“Measuring the acceleration of the Solar System with a relative precision of 7 percent is a very important scientific result, and at the same time, it is a convincing demonstration of the quality of the new data. The acceleration measured by Gaia shows a close agreement with theoretical expectations and provides important information on the motion of the Solar System in the gravitational field of our Galaxy.”

The next publication of the Gaia catalog is scheduled for the first half of 2022. Given the data published up until now, we can certainly expect considerable top-level research in the future. Since its release in April 2018, the second version of the Gaia catalog has generated an average of five publications per day!

In Dresden, preparations have already commenced for the fourth Gaia catalog, which will be published in 2025. The observation data for this catalog will be awaiting the Dresden Gaia team from January 2021 at the latest, including both its very special challenges that have to be mastered, and its scientific treasures that are to be retrieved.


Details on the German event

  • Organized by DLR, Germany’s research center for aeronautics and space, in cooperation with AIP Potsdam, ARI Heidelberg, MPIA Heidelberg and TU Dresden
  • Time: December 3, 11:00 am until around 12:30 pm CET
  • YouTube live stream
  • The ESA overview page for the EDR3 release and the programs of the individual events
  • Gaia archive
  • DLR live stream (on December 3)
  • All publications related to the EDR3 release

Media Contact
Prof. Sergei A. Klioner
[email protected]

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