High-energy astronomy from the International Space Station

Authors
Citation
A. Parmar, High-energy astronomy from the International Space Station, EARTH MOON, 87(3), 2001, pp. 149-157
Categorie Soggetti
Space Sciences
Journal title
EARTH MOON AND PLANETS
ISSN journal
01679295 → ACNP
Volume
87
Issue
3
Year of publication
2001
Pages
149 - 157
Database
ISI
SICI code
0167-9295(2001)87:3<149:HAFTIS>2.0.ZU;2-W
Abstract
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.