The European Space Agency, ESA, is currently studying 3 high-energy astrono
my missions that use the International Space Station (ISS). These are Lobst
er-ISS, an all-sky imaging X-ray monitor, the Extreme Universe Space Observ
atory (EUSO) which will study the highest energy cosmic rays by using the E
arth's atmosphere as a giant detector and XEUS - the X-ray Evolving Univers
e Spectroscopy Mission, a potential successor to ESA's XMM-Newton X-ray obs
ervatory. These first 2 missions will he attached to the external platforms
on the Columbus module, while XEUS will visit the ISS to attach additional
X-ray mirrors to enlarge the original 4.5 m diameter mirrors to the 10 m d
iameter required to observed redshifted iron lines from massive black holes
in the early Universe.