News story

Gaia: ‘Go’ for science

Following extensive in-orbit commissioning and several unexpected challenges, Europe’s billion-star surveyor is ready to begin its mission.

Inside Gaia’s billion-pixel camera

The satellite was launched on 19 December 2013, and is orbiting a virtual location in space 1.5 million kilometres from Earth.

Gaia’s goal is to create the most accurate map yet of the Milky Way. It will make extremely accurate measurements of the positions and motions of about 1% of the total population of roughly 100 billion stars in our home galaxy to help answer questions about its origin and evolution.

Professor Gerry Gilmore, from the University of Cambridge and UK Principal Investigator for Gaia, said:

Gaia will be a revolution in our knowledge of the local Universe. For the first time we will have a fair sample of what is out there, where it is, how it is moving, how unseen (dark) matter is distributed, where and when stars formed and where and when the chemical elements of which we are made were created. Gaia will make a huge step towards understanding how the Milky Way came to be formed, and evolved into what we see today. For the first time, we will be able to see the Milky Way in 3-D. In fact in 6-D – where stars are, and how they are moving.

UK participation in the mission is funded by the UK Space Agency and scientists and engineers from around the UK have played key roles in the design and build of Gaia. The UK Science and Technology Facilities Council (STFC) funded the early development of the project, including the set-up of the data applications centre. STFC’s current support involves the UK exploitation of the scientific data to be yielded from the mission.

The Cambridge Gaia Data Processing Centre will be the front line in processing Gaia’s images, which will play an important role in the discovery of many thousands of transient stars and supernovae: these will be made immediately available to schools and the public for their participation in the research.

Repeatedly scanning the sky, Gaia will observe each of its billion stars an average of 70 times each over five years. Small apparent motions in the positions of the stars will allow astronomers to determine their distances and movements through the Milky Way.

In addition, Gaia will also measure key physical properties of each star, including its brightness, temperature and chemical composition.

Gaia spins slowly once every six hours, sweeping its two telescopes across the sky and focusing the light from their separate fields simultaneously onto a single focal plane – the largest digital camera ever flown in space, with nearly a billion pixels.

As the stars drift across the camera, the relative positions of all detected stars are measured and downlinked to Earth. Over time, a complete network of positions of stars covering the whole sky is built up, before being analysed to yield a highly accurate 3D map.

The accuracy required is astonishing: Gaia must be able to measure positions to a level equivalent to the width of a human hair seen at 2,000 km. In turn, these measurements demand a very rigorous calibration of the satellite and its instruments, a painstaking procedure that has taken the first part of the year to complete.

Gaia is now ready to begin its five-year science phase, but the commissioning also uncovered some unexpected anomalies.

One problem detected early in the commissioning was associated with water freezing on some parts of the optics, causing a temporary reduction in transmission of the telescopes.

This water was likely trapped in the spacecraft before launch and emerged once it was in a vacuum. Heating the affected optics to remove the ice has now largely solved this problem, but it is likely that one or two more ‘decontamination’ cycles will be required during the mission to keep it in check.

Another problem is associated with ‘stray light’ reaching Gaia’s focal plane at a level higher than predicted before launch. This appears to be a mixture of light from the Sun finding its way past Gaia’s 10-m-diameter sunshield and light from other astronomical objects, both making their way to the focal plane as a diffuse background.

The effect on Gaia’s performance is negligible for brighter objects at magnitude 15 and above, and a slight degradation in the positional accuracy is seen for fainter stars, reaching 50% for stars at Gaia’s nominal faint limit of magnitude 20.

There is also some effect on the accuracy to which stellar brightnesses will be measured.

The impact of the stray light should, in principle, be more significant for faint stars seen by Gaia’s Radial Velocity Spectrometer (RVS). However, Gaia scientists are optimizing the on-board software to mitigate as much as possible the impact caused by these higher background levels of light, and are confident that they will not be far off their initial and somewhat conservative estimate of studying 150 million stars with RVS.

Further tests made during commissioning have shown that it may be possible to extend Gaia’s reach to stars even fainter than magnitude 20, while at the other end, software changes enable Gaia to measure almost all of the brightest stars in the sky, previously ruled out as being too bright for such a sensitive system. Both of these extensions will need further analysis before being implemented.

Finally, Gaia also contains a laser device called the ‘basic angle monitor,’ designed to measure the angle of separation between Gaia’s two telescopes to an extremely high level of accuracy. This is necessary in order to correct for expected periodic variations in the separation angle caused by thermal changes in the payload as Gaia spins.

Although this system is working, the detected variations in the basic angle are larger than expected. Further efforts are being made to measure and accurately calibrate the variations, with the aim of largely eliminating them during the overall data analysis.

The commissioning has not only focused on the spacecraft performance, but also on the flow of data on the ground, testing procedures that will be used to process and analyse the vast amount of data that will be transmitted to Earth on a daily basis for the next five years.

Thus, after extensive testing and analysis of systems both in space and on the ground, Gaia is now in a position to begin routine operations.