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RXTE Guest Observer Faciliity

The Rossi X-ray Timing Explorer Mission
(1995-present)

The Rossi X-ray Timing Explorer (RXTE) is a satellite that observes the fast-moving, high-energy worlds of black holes, neutron stars, X-ray pulsars and bursts of X-rays that light up the sky and then disappear forever.

How fast and how energetic are they? Well, some pulsars spin faster than a thousand times a second. And a neutron star produces a gravitational pull so powerful that a marshmallow striking the star's surface would hit with the force of a thousand hydrogen bombs. Astronomers study changes that happen from microseconds to months in cosmic objects to learn about how gravity works near black holes, how pulsars in binary systems are affected by mass transferring from one star to the other, and how the giant engines in distant galaxies are powered. RXTE was launched into low-Earth orbit on December 30, 1995, and is still going strong, making unique contributions to our understanding of these extreme objects.

For RXTE, the trick to observing these kinds of objects is all in the timing -- an ability to observe changes in X-ray brightness that occur in a mere thousandths of a second, or over several years. Learn more about how this one-of-a-kind satellite has reshaped our understanding of what goes on in the most violent and bizarre regions of the Universe.

Enter here for images, videos and tales from the world of extremes.

Latest News
  • RXTE Workshop to follow Fermi Symposium (12 Oct 2009)
    RXTE Workshop to be held Thursday, Nov. 5 in Washington, D.C.
  • RXTE Returns to Normal Operations (02 Oct 2009)
    RXTE has resumed a normal observation schedule
  • RXTE in Inertial Hold on IGR J17511-3057 due to Spacecraft Anomaly (23 Sep 2009)
    RXTE slews are disabled while team investigates a spacecraft anomaly
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    Other News

    RXTE-related Astronomical Notices
    Latest RXTE-related ATELs, IAUCs, and GCN notices

    TOO News
    TOO News

    Latest Target of Opportunity Information


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    This page is maintained by the RXTE GOF and was last modified on Wednesday, 15-Apr-2009 17:10:40 EDT.

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