• → European Space Agency

    • About Science & Technology

    • For Public

    • For Educators

    • ESA

    • Science & Technology

    • Educational Support

    • Educational Support
    • Overview
    • Contact us
    • Competition
    • Competition winners attend INTEGRAL anniversary event
    • Cassini Scientist for a Day 2012 Competition - Results
    • Starter Activities
    • Mindmap
    • Brainstorming
    • Themes
    • Wavelength
    • Solar System
    • Resources
    • Images
    • Video
    • Publications
    • Spacecraft Models
    • Spacecraft Orbits
    • Posters
    • Materials
    • Miscellaneous
    • Interactive
    • Little Books of Gaia
    • Cut-out & Build
    • Exercises in Astronomy
    • Teacher Notes
    • Bookmark and Share

    XMM-Newton: light path of X-rays

    Date: 16 May 2012
    Depicts: Light path of X-rays through XMM-Newton
    Copyright: ESA / AOES Medialab

    The light path of X-rays through XMM-Newton (upper section). The spacecraft carries three telescopes each consisting of 58 nested, gold-coated, tube-like mirrors. The combination of parabolic and hyperbolic mirrors used is shown in a  cross section through one of the telescopes (middle section). X-rays that graze the mirror surfaces are reflected twice and focused onto a detector. The X-rays must graze the mirror at angles of 1° or even less, or they are likely to be absorbed (lower section).

     


    Last Update: 23 May 2012

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=50381
    • Latest selection
    • Saturn
    • Saturn's F ring
    • Pan
    • Image Hi-Res Versions
    • Hi-Res [jpg]
      503.40 kb.

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Livestream
    • Subscribe
    • App Store
    • ESA Science Twitter

    Follow ESA science

    • Copyright 2000 - 2013 © European Space Agency. All rights reserved.

    • Terms and Conditions