|Cosmic Vision Themes||The Hot and Energetic Universe|
|Primary goals||Mapping hot gas structures and determining their physical properties
Searching for supermassive black holes
|Orbit||Halo orbit around L2, the second Lagrange point of the Sun-Earth system|
|Lifetime||Four years, plus possible extensions|
Athena – Advanced Telescope for High-ENergy Astrophysics – will be an X-ray telescope designed to address the Cosmic Vision science theme 'The Hot and Energetic Universe'. The theme poses two key astrophysical questions:
- How does ordinary matter assemble into the large-scale structures we see today? and
- How do black holes grow and shape the Universe?
To address the first question, it will be necessary to map hot gas structures in the Universe – specifically the gas in clusters and groups of galaxies, and the intergalactic medium – determine their physical properties and track their evolution through cosmic time.
To answer the second question, supermassive black holes (SMBH) must be revealed, even in obscured environments, out into the early Universe, and both the inflows and outflows of matter and energy as the black holes grow must be understood.
Because most of the baryonic component of the Universe is locked up in hot gas at temperatures of millions of degrees, and because of the extreme energetics of the processes close to the event horizon of black holes, understanding the Hot and Energetic Universe requires space-based observations in the X-ray portion of the electromagnetic spectrum.
By combining a large X-ray telescope with state-of-the-art scientific instruments, Athena will be able to make an important contribution to answering these questions.
On 27 June 2014, Athena was selected as the second L-class mission in ESA's Cosmic Vision 2015–25 plan. The mission has now entered the study phase; once the mission design and costing have been completed, it will eventually be proposed for 'adoption' around 2023, before the start of the construction phase.