07.06.2015 Views

The Astrology of Space - Matrix Software

The Astrology of Space - Matrix Software

The Astrology of Space - Matrix Software

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

<strong>The</strong> <strong>Astrology</strong> <strong>of</strong> <strong>Space</strong><br />

star, adding matter to the white dwarf and pushing the<br />

mass beyond the critical limit <strong>of</strong> 1.44 solar masses. At<br />

that point the core <strong>of</strong> the white-dwarf collapses<br />

violently, releasing energy as a supernova, leaving<br />

behind a binary system <strong>of</strong> an ordinary giant star and<br />

an x-ray source.<br />

For a star much more massive than the Sun, the<br />

supernova evolution is different. <strong>The</strong> star also fuses<br />

hydrogen into helium in its core for a few hundred<br />

million years and, when the hydrogen is almost<br />

exhausted, the core contracts, the outer layers <strong>of</strong> the<br />

star expand, and the star becomes a red giant.<br />

Hydrogen continues to be burned in a shell around<br />

the core, as the core itself contracts until it heats up<br />

enough to fuse helium into carbon. When the helium<br />

is nearly exhausted, the core begins to burn the<br />

carbon.<br />

At that point, one <strong>of</strong> two conditions can occur. <strong>The</strong><br />

ignition <strong>of</strong> the carbon could induce instabilities that<br />

would detonate the star as a SN II, leaving behind<br />

nothing but an expanding gaseous remnant. Or, if the<br />

carbon is safely ignited, the extraordinarily high<br />

temperatures in the core could generate neutrinos at<br />

an ever-increasing rate sapping the stars energy,<br />

causing the core to plunge to a total collapse. In this<br />

event, a final burst <strong>of</strong> neutrinos might carry away so<br />

much <strong>of</strong> the red giant's rotational momentum, that it<br />

would blow <strong>of</strong>f the entire outer envelope <strong>of</strong> the star.<br />

An explosion <strong>of</strong> this kind would leave behind a<br />

gaseous remnant, in the center <strong>of</strong> which would be a<br />

pulsating pulsar a rapidly rotating neutron star) or a<br />

black hole.<br />

183

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!