"In early October, 1977, Luis W. Alvarez and his son Walter dropped into my office at the Lawrence Berkeley Laboratory (LBL)... There was no funding for these measurements, so we had to squeeze them in with our other work."Scientists are forced to do this all the time. Their ideas develop more rapidly than their funding sources. At the time of this meeting, their quest was in the realm of "normal science." They intended to measure the time it took to deposit the clay layer by measuring the concentration of the element, iridium. Iridium is not a major component of Earth's crust, but the Earth does obtain iridium at a steady rate from the infall of micrometeorites from space. The estimated rate is considerable, about ten million kilograms of iridium per year, but it's distributed uniformly on Earth's surface, so the concentration in any one place is very small. The Alvarez duo approached Asaro, since his lab could do a very sensitive trace element analysis called neutron activation. By measuring the iridium, they would be measuring the duration of time.
Luiz Alvarez (left) and his son, Walter. (Lawrence Berkeley Laboratory photograph, via Wikipedia). |
"By virtue of the fact that we know these objects, and we know their orbits, we can predict that they are no longer hazardous to Earth in the sense that we can follow them, and we know that there are none that pose any imminent risk of an impact."[4]The orbital data indicate that none of the large asteroids would collide with Earth in the next few centuries.[3-8] After the population of large asteroids, there exists about 20,000 100 meter near-Earth asteroids that could destroy a city. NASA is tracking more than 5,000 of these, but it expects that it needs to discover an additional 15,000 to have their full complement (see figure).[4] NASA has the additional mandate from the US Congress to find ninety percent of asteroids larger than about 450 feet in size by 2020.[5] Asteroid census data from the NASA WISE mission. Each image represents 100 objects in the population of near-Earth asteroids. The blue outlines show the estimated numbers before the NEOWISE survey. The shaded objects show NASA's revised, lower estimate.(Image: NASA/JPL-Caltech). Lurking in the background are more than a million smaller near-Earth asteroids that would still survive their plunge through Earth's atmosphere and inflict ground damage, although on a smaller scale.[3] WISE data also falsified a theory of the origin of the dinosaur-annihilating asteroid. This theory was proposed in 2007 on the basis of ground-based telescope data of the remnant of the large asteroid, Baptistina. The theory proposed that Baptistina crashed into another asteroid about 160 million years ago, and a large fragment from the impact found its way to Earth.[9]. WISE measured 1,056 members of the Baptistina family and determined that the break-up occurred just 80 million years ago, only half as far back as the original estimate. This estimate was based on the time it would take for the fragments to reach their present positions. This would give a Baptistina fragment just 15 million years to reach Earth, which is not possible considering that the mechanism would need to have been the gravitational influences of Jupiter and Saturn.[9]
"As one of my colleagues at the Jet Propulsion Laboratory likes to say, the best three ways of dealing with the potential of an asteroid impact are to find them early, find them early and find them early."[5]