prepublication copy - The Department of Astronomy & Astrophysics ...
prepublication copy - The Department of Astronomy & Astrophysics ...
prepublication copy - The Department of Astronomy & Astrophysics ...
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
ubiquitous high-energy charged-particle cosmic rays, including those that crash into Earth’s atmosphere<br />
producing telltale radioactive isotopes. X-ray, gamma-ray, and radio observations <strong>of</strong> these stellar<br />
remnants will test this hypothesis and reveal the accelerator dynamics <strong>of</strong> the stellar ghosts (Figure 2-10).<br />
Planetary Systems<br />
Our Sun is just one <strong>of</strong> the several hundred billion stars in the Milky Way, and its well-ordered<br />
configuration <strong>of</strong> eight planets just one <strong>of</strong> the many diverse planetary systems. While we have studied our<br />
Solar System with telescopes for four hundred years, we have only, in the last two decades, been able to<br />
detect planets orbiting other stars and begun to appreciate their astonishing diversity. We have uncovered<br />
surprises ranging from Earth-sized planets orbiting the compact corpses <strong>of</strong> burned-out stars to planets<br />
termed “hot Jupiters” that are more than one hundred times the mass <strong>of</strong> Earth but which are so close to<br />
their stars that they orbit them in just a few days. Models <strong>of</strong> the formation <strong>of</strong> planetary systems predict<br />
that planets this massive should form at much greater distances; these bodies have forced us to consider<br />
processes <strong>of</strong> “migration” that bring large planets closer to their stars early in their histories.<br />
<strong>The</strong> details <strong>of</strong> how planets form within disks are still being revealed by current astronomical<br />
techniques including imaging from Hubble, Spitzer, and the largest ground-based telescopes, plus<br />
theoretical studies including computer modeling. Disks start out being dominated by gas—the hydrogen<br />
and helium <strong>of</strong> the primordial cosmos salted with the heavy elements out <strong>of</strong> which planets and life are<br />
composed—and evolve with time into dusty disks or rings between the newborn planets themselves.<br />
While most if not all stars like our Sun may possess disks early in their histories, what fraction <strong>of</strong> these<br />
turn into planetary systems is not known.<br />
FIGURE 2‐10 Image <strong>of</strong> the supernova remnant RX J1713.7‐3946 observed in the highest energy (TeV) gamma<br />
rays. Recent observations using atmospheric Čerenkov telescopes have demonstrated that cosmic rays are<br />
accelerated to energies in excess <strong>of</strong> 100 TeV and that magnetic field is amplified to high strength. Contours<br />
are x‐ray emission. Supernova explosions like those that left behind this source created and dispersed heavy<br />
elements as well as accelerated cosmic rays. Source: “A detailed spectral and morphological study <strong>of</strong> the<br />
gamma‐ray supernova remnant RX J1713.7‐3946 with H.E.S.S,” <strong>The</strong> HESS Collaboration: F. Aharonian et al.<br />
PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION<br />
2-24