© Lick ObservatoryHalley's Comet becomes visible to the unaided eye about every 76 years as it nears the sun.
The idea of nearby stars influencing comets goes back to 1950, when the astronomer Jan Hendrik Oort hypothesized an invisible repository of comets - the so-called Oort cloud - swarming around the solar system out to a distance of 100,000 AU (one AU is the distance between the sun and the Earth).
Oort assumed that stars passing through the cloud would cause a fresh batch of comets to fall in towards the sun, where they become visible to astronomers. Such a disturbance could have long term effects.
"The comets we see now could be from a stellar passage hundreds of millions of years ago," said Hans Rickman of the Uppsala Astronomical Observatory in Sweden.
However, Rickman and his colleagues have confirmed that star encounters alone cannot explain comet behavior. Using a computer model of the Oort cloud, they show that gravity effects from the galaxy are equally important. The results are reported in a recent article in the journal Celestial Mechanics and Dynamical Astronomy.
Two stars passing in the night
Although Earth has almost certainly been hit by comets throughout its history, it is not all that clear how often that has happened. Much of the crater history on Earth has been erased because of erosion or tectonic activity. The remaining craters could have come from asteroids instead of comets.
"It's quite difficult to tell a comet-induced crater from an asteroid one, since the impactor gets essentially vaporized," Rickman said.
© UnknownWhat our Milky Way Galaxy may look like from above, and the position of our star, the sun, within the galaxy. The gravitational influence of the galaxy may disrupt the Oort Cloud of comets that surrounds our solar system.
Comet impacts are, however, likely to be more energetic (and therefore more damaging), since comets are moving much faster than asteroids when they pass by Earth.
Comet orbits can be altered whenever another star comes within 10,000 AU of our sun. Such a close encounter - occurring every 100 million years or so - will not typically disturb asteroids or planets, but it definitely "shakes up the whole Oort cloud," Rickman said.
Most scientists have presumed that these star crossings will lead to a shower of comets raining down on the Earth and the rest of the inner solar system. Some have even claimed to find evidence of periodic mass extinctions that might be explained by a single (as-yet-unidentified) star in an elliptical orbit around the sun.
To study the effect of stellar perturbations, Rickman and his colleagues model the Oort cloud with a sample of one million comets (the true number of cloud comets is unknown, but certainly much higher). The simulations are allowed to run for a time period corresponding to the 5-billion-year age of the solar system.
The results show that stars can induce comet showers, but the contrast with non-shower periods is less than what people have thought before, Rickman said. This leveling out in comet activity is due to the influence of the gravitational field of the Milky Way.
Galactic tide
© Southwest Research InstituteDiagram showing the position of the Oort Cloud.
The simulations by Rickman and colleagues show how the galactic tide constantly gives a small nudge to the cloud's comets. Some of these comets are in rather unstable orbits to begin with, so the slight push can send them on a sun-bound trajectory. Eventually, however, all these unstable comets are ejected from the solar system.
And this is where stellar encounters become important. They scramble the Oort cloud, so that the galactic tide has a new crop of unstable comets to funnel into the inner solar system.
"The general picture spawned by our results is that injection of comets from the Oort Cloud is essentially to be seen as a team work involving both tides and stars," the scientists write in their paper.
This star-tide collaboration keeps a relatively steady supply of comets zooming nearby, so the threat from comet impacts probably does not change much over time.
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