Europe's mission

Europe is launching two space missions on a big scale over the next two decades. One is an X-ray telescope to study the origin of black holes, and the other is a gravitational wave observatory, writes Jonathan Amos.

Europe has fixed a broad plan for the big space science missions it will launch over the next two decades. It will likely lead to a large X-ray telescope being launched in 2028, and to an orbiting observatory to detect gravitational waves going up in 2034.

Together, these two ventures will cost in excess of  € 2 billion. They join a mission already approved known as Juice, which will see a big satellite sent to observe Jupiter and its icy moons in 2022.
The path ahead was set by the Science Policy Committee (SPC) of the European Space Agency (ESA), which is meeting in Paris. The committee’s decision should now give clear direction and certainty to Europe’s research and industrial base.

“These big missions take a long time to put together — of the order of 20 years,” said Fabio Favata, head of ESA’s Science Planning and Community Coordination Office. “Of course, when you fix things you trade flexibility for stability, but this gives the community the opportunity to plan. They now understand what will be the ‘pillars,’ what will be the ‘cornerstones,’ ” he told BBC News.

The SPC gathering was asked to approve a set of scientific ‘themes’ that will guide the selection of ESA’s next Large Class mission opportunities. The agency tries to launch one of these flagship endeavours every six years.

The themes are titled the “hot and energetic universe,” and the “gravitational universe.” And although these themes do not endorse a specific X-ray telescope or gravitational wave detection concept, their prescription is so tight that only two candidates can have real confidence of making it through the forthcoming selection process. These are the two consortia that narrowly lost out to the Juice team in the last L-Class competition in 2012. The X-ray telescope proposal currently goes by the name of Athena+. It would be roughly four tonnes in mass and have a 12-metre focal length. With a survey capability and sensitivity a hundred times better than today’s best space telescopes, Athena+ would be used to study the origin of the monstrous black holes that reside at the centres of galaxies, among other objectives.

The gravitational wave observatory goes by the name of LISA, which stands for Laser Interferometer Space Antenna.

It would fire lasers across millions of kilometres of space to try to measure the disturbance in the fabric of space-time resulting from exploding stars and merging black holes. It is a concept that has been studied for the better part of 20 years already. Indeed, ESA is about to fly a small satellite called LISA Pathfinder to demonstrate some of the key technologies.

The agency will call for proposals to take the 2028 launch opportunity early next year. There will then be a design phase with various technical reviews before a formal adoption of a mission in about 2018. “It’s very important that ESA takes a long-term perspective,” argued Dr Kirpal Nandra, the chairman of the Athena+ collaboration.

“If we don’t take such a long-term view then there’s a danger universities won’t hire people in high-energy astrophysics and black holes and galaxy clusters — because they won’t see a future in these areas. But now they can, and they can be pretty much guaranteed that some exciting times lie ahead, especially for the young people just starting out in their careers.”

International partners

A call for a gravitational wave detection mission will not go out to the community for about five years, and with a launch opportunity no earlier than 2034, it means many of those people who have worked on Lisa will be long retired by the time an observatory of its ilk is taken into orbit. The advantage is it provides more time to mature the complex technology and to find the international partners needed to fly the most capable architecture possible — something that was compromised back in 2012 when the Americans said they could not afford to participate.

This forced European mission designers to de-scope the proposed laser observatory. “We’ve been through a very lean period with the U.S., but I don’t think that will persist indefinitely,” says Henry Ward, a Glasgow University scientist in the LISA collaboration.

“And indeed, at a meeting in Paris recently, the Americans were talking about a contribution being realistic in the timeframes we’re now discussing. The amount of money we have on the table is going to make a difference to the architecture we are able to fly.” The L-Class missions of ESA are part of the agency’s mandatory programme. That is, all member states contribute to ESA’s costs according to the relative size of their economy.

This means Germany, the U.K., France and Italy contribute the most . There tend, however, to be additional contributions in the form of instruments, which member states will offer to the projects to secure leadership roles. The U.K. has traditionally been very strong in both X-ray astronomy and gravitational wave research, and so scientists in Britain will be looking to the U.K. Space Agency to play a strong hand when the 2028 and 2034 opportunities come up for adoption.

“The decision...is about themes, but we know pretty much what sort of missions will deliver those themes,” commented Chris Castelli, a UKSA delegate to ESA’s Science Policy Committee. “We need to take a careful look at the technologies we could fly, and only then work out what everyone’s participation should be.”

BBC News
The New York Times Syndicate