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FIGURE 2‐2 <strong>The</strong> source 3C 75, shown here in x‐rays (blue) and radio waves (pink), is a rare example where<br />

two galaxies have been caught in the act <strong>of</strong> merging. Not only do their stars merge, but their central black<br />

holes ‐ each producing a pair <strong>of</strong> jets containing gas moving outward with speed close to that <strong>of</strong> light ‐ will<br />

do likewise in perhaps a few hundred million years. Many similar mergers involving smaller black holes in<br />

the nuclei <strong>of</strong> younger galaxies are thought to have taken place. When black holes coalesce, they create<br />

intense bursts <strong>of</strong> gravitational radiation. (Credit: X‐ray: NASA/CXC/AIfA/D.Hudson & T.Reiprich et al.;<br />

Radio: NRAO/VLA/NRL.)<br />

galaxies form and evolve will be possible. We are on the verge <strong>of</strong> a new era <strong>of</strong> discovery in gravitational<br />

wave astronomy.<br />

In addition, gravitational waves could be created by exotic processes occurring in the young<br />

universe and would have been propagating freely to us ever since. Several speculative sources such as<br />

cosmic strings and abrupt changes in the form that the contents <strong>of</strong> the universe assumed—“phase<br />

changes,” like the change from water to ice—have been suggested but the truth is that we do not quite<br />

know what to expect. A possible way to see if there are any measurable signals with wavelengths <strong>of</strong><br />

roughly light years employs very precise radio measurements <strong>of</strong> naturally occurring cosmic “clocks”<br />

called pulsars. 2 Spread across the sky, the separations between these cosmic clocks will change as a long<br />

wavelength gravitational wave passes by, potentially measurably changing the arrival times <strong>of</strong> their radio<br />

pulses.<br />

Opening the Time Domain: Making Cosmic Movies<br />

By eye, the universe appears static apart from the twinkling <strong>of</strong> starlight caused by Earth’s<br />

atmosphere. In fact, it is a place where dramatic things happen on timescales we can observe—from a<br />

tiny fraction <strong>of</strong> a second to days to centuries. Stars in all stages <strong>of</strong> life rotate, pulsate, and undergo<br />

activity cycles while many flare, accrete, lose mass, and erupt, and some die in violent explosions. Binary<br />

neutron stars and black holes merge, emitting, in addition to bursts <strong>of</strong> radiation, gravity waves.<br />

Supermassive black holes in the centers <strong>of</strong> galaxies swallow mass episodically and erupt in energetic<br />

outbursts. Some objects travel rapidly enough for us to measure their motion across the sky.<br />

2 <strong>The</strong> 1993 Nobel Prize in Physics was awarded to two American astronomers for their work on binary pulsars.<br />

PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />

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