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Many famous comets originally formed in other solar systems

Date:
June 11, 2010
Source:
Southwest Research Institute
Summary:
Many of the most well known comets, including Halley, Hale-Bopp and, most recently, McNaught, may have been born in orbit around other stars, according to a new theory by an international team of astronomers.

Comet Hale-Bopp photographed on April 9, 1997.
Credit: iStockphoto/Scott Orr

Many of the most well known comets, including Halley, Hale-Bopp and, most recently, McNaught, may have been born in orbit around other stars, according to a new theory by an international team of astronomers led by a scientist from the Southwest Research Institute (SwRI) in Boulder, Colo.

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Dr. Hal Levison (SwRI), Dr. Martin Duncan (Queen's University, Kingston, Canada), Dr. Ramon Brasser (Observatoire de la Cτte d'Azur, France) and Dr. David Kaufmann (SwRI) used computer simulations to show that the Sun may have captured small icy bodies from its sibling stars while it was in its birth star cluster, thereby creating a reservoir for observed comets.

While the Sun currently has no companion stars, it is believed to have formed in a cluster containing hundreds of closely packed stars that were embedded in a dense cloud of gas. During this time, each star formed a large number of small icy bodies (comets) in a disk from which planets formed. Most of these comets were gravitationally slung out of these prenatal planetary systems by the newly forming giant planets, becoming tiny, free-floating members of the cluster.

The Sun's cluster came to a violent end, however, when its gas was blown out by the hottest young stars. These new models show that the Sun then gravitationally captured a large cloud of comets as the cluster dispersed.

"When it was young, the Sun shared a lot of spit with its siblings, and we can see that stuff today," says lead author Levison.

"The process of capture is surprisingly efficient and leads to the exciting possibility that the cloud contains a potpourri that samples material from a large number of stellar siblings of the Sun," says co-author Duncan.

Evidence for the team's scenario comes from the roughly spherical cloud of comets, known as the Oort cloud, that surrounds the Sun, extending halfway to the nearest star. It has been commonly assumed this cloud formed from the Sun's proto-planetary disk. However, because detailed models show that comets from the solar system produce a much more anemic cloud than observed, another source is required.

Levison says, "If we assume that the Sun's observed proto-planetary disk can be used to estimate the indigenous population of the Oort cloud, we can conclude that more than 90 percent of the observed Oort cloud comets have an extra-solar origin."

"The formation of the Oort cloud has been a mystery for over 60 years and our work likely solves this long-standing problem," says Brasser.

The article by Levison, Duncan, Brasser and Kaufmann, was published in the June 10 issue of Science Express.

Funding for this research was provided by NASA's Astrobiology Institute, Outer Planets Research and Origins of Solar Systems programs, the Natural Science and Engineering Research Council of Canada, and Germany's Helmholtz Alliance.


Story Source:

The above story is based on materials provided by Southwest Research Institute. Note: Materials may be edited for content and length.


Journal Reference:

  1. Harold F. Levison, Martin J. Duncan, Ramon Brasser, and David E. Kaufmann. Capture of the Sun's Oort Cloud from Stars in its Birth Cluster. Science, 2010; DOI: 10.1126/science.1187535

Cite This Page:

Southwest Research Institute. "Many famous comets originally formed in other solar systems." ScienceDaily. ScienceDaily, 11 June 2010. <www.sciencedaily.com/releases/2010/06/100610141038.htm>.
Southwest Research Institute. (2010, June 11). Many famous comets originally formed in other solar systems. ScienceDaily. Retrieved March 28, 2015 from www.sciencedaily.com/releases/2010/06/100610141038.htm
Southwest Research Institute. "Many famous comets originally formed in other solar systems." ScienceDaily. www.sciencedaily.com/releases/2010/06/100610141038.htm (accessed March 28, 2015).

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