Science News

... from universities, journals, and other research organizations

Pre-Life Molecules Present In Comets

ScienceDaily (July 27, 2006) — Evidence of atomic nitrogen in interstellar gas clouds suggests that pre-life molecules may be present in comets, a discovery that gives a clue about the early conditions that gave rise to life, according to researchers from the University of Michigan and the Harvard-Smithsonian Center for Astrophysics.

The finding also substantially changes the understanding of chemistry in space.

The question of why molecular nitrogen hasn't been detected in comets and meteorites has puzzled scientists for years. Because comets are born in the cold, dark, outer reaches of the solar system they are believed to be the least chemically altered during the formation of the Sun and its planets.

Studies of comets are thought to provide a "fossil" record of the conditions that existed within the gas cloud that collapsed to form the solar system a little more than 4.6 billion years ago. In this cloud, since nitrogen was thought to be in molecular form, and it follows that comets should contain molecular nitrogen as well.

But the reason it isn't there is because it isn't present in the gas clouds whose microscopic solid particles eventually form comets, said Sébastien Maret, research fellow in astronomy at the University of Michigan, and Edwin Bergin, a professor of astronomy at the University of Michigan. Those clouds contain mostly atomic nitrogen, not molecular nitrogen, as previously thought.

Maret, Bergin, and collaborators from Harvard-Smithsonian Center for Astrophysics will publish their findings in the July 27 issue of the journal Nature.

The nitrogen bearing molecules in comets that crashed into Earth millions of years ago may have provided a sort of "pre-biotic jump start" to form the complex molecules that eventually led to life here, Bergin said.

"A lot of complex and simple biotic molecules have nitrogen and it's much easier to make complex molecules from atomic nitrogen," Bergin said. "All DNA bases have atomic nitrogen in them, amino acids also have atomic nitrogen in them. By that statement what we're saying is if you have nitrogen in its simplest form, the atomic form, it's much more reactive and can more easily form complex prebiotic organics in space". These complex organics were incorporated into comets and were provided to the Earth.

"What we're seeing in space is telling us something about how you make molecules that led to us," Bergin said.

Also of importance is the fact that odd anomalies in isotopic values in meteorites can also be explained if the nitrogen is not molecular, Bergin said.

Recommend this story on Facebook, Twitter,
and Google +1:

Other bookmarking and sharing tools:

| More

Story Source:

The above story is reprinted from materials provided by University of Michigan.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


APA

MLA

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.

Search ScienceDaily

Number of stories in archives: 114,804

Find with keyword(s):
 
Enter a keyword or phrase to search ScienceDaily's archives for related news topics,
the latest news stories, reference articles, science videos, images, and books.

 
  more breaking science news

Social Networks


Recommend this story on Facebook, Twitter,
and Google +1:
Other bookmarking and sharing tools:
| More

Breaking News

... from NewsDaily.com

In Other News ...

Copyright Reuters 2008. See Restrictions.

Free Subscriptions

... from ScienceDaily

Get the latest science news with our free email newsletters, updated daily and weekly. Or view hourly updated newsfeeds in your RSS reader:

Feedback

... we want to hear from you!

Tell us what you think of ScienceDaily -- we welcome both positive and negative comments. Have any problems using the site? Questions?

 
Post this page to your favorite social bookmarking site:
close
Include this item in your blog or web site:
close
Cite this article in your essay, paper, or report:
close
Email this page's link to a friend or colleague:
close