[meteorite-list] Contact!

From: mark ford <markf_at_meteoritecentral.com>
Date: Wed Feb 1 09:18:41 2006
Message-ID: <6CE3EEEFE92F4B4085B0E086B2941B3145BAA7_at_s-southern01.s-southern.com>

Indeed, but if you alter the number of planet forming stars by a factor
of two of three (which this research would suggest) you still only end
up with a couple extra possible alien worlds and the chances of them
being within comms range = really not a lot!

Drat

Best,

Mark Ford


-----Original Message-----
From: meteorite-list-bounces_at_meteoritecentral.com
[mailto:meteorite-list-bounces_at_meteoritecentral.com] On Behalf Of Pete
Pete
Sent: Wednesday, February 01, 2006 10:45 AM
To: meteorite-list_at_meteoritecentral.com
Subject: [meteorite-list] Contact!

This will surely change the Drake Equation!

Cheers,
Pete



http://www.cfa.harvard.edu/press/pr0611.html

Most Milky Way Stars Are Single


Release No.: 06-11
For Release: Monday, January 30, 2006
Note to editors: An image to accompany this release is online at
http://www.cfa.harvard.edu/press/pr0611image.html.



Cambridge, MA - Common wisdom among astronomers holds that most star
systems
in the Milky Way are multiple, consisting of two or more stars in orbit
around each other. Common wisdom is wrong. A new study by Charles Lada
of
the Harvard-Smithsonian Center for Astrophysics (CfA) demonstrates that
most
star systems are made up of single stars. Since planets probably are
easier
to form around single stars, planets also may be more common than
previously
suspected.

Astronomers have long known that massive, bright stars, including stars
like
the sun, are most often found to be in multiple star systems. This fact
led
to the notion that most stars in the universe are multiples. However,
more
recent studies targeted at low-mass stars have found that these fainter
objects rarely occur in multiple systems. Astronomers have known for
some
time that such low-mass stars, also known as red dwarfs or M stars, are
considerably more abundant in space than high-mass stars.

By combining these two facts, Lada came to the realization that most
star
systems in the Galaxy are composed of solitary red dwarfs.

"By assembling these pieces of the puzzle, the picture that emerged was
the
complete opposite of what most astronomers have believed," said Lada.

Among very massive stars, known as O- and B-type stars, 80 percent of
the
systems are thought to be multiple, but these very bright stars are
exceedingly rare. Slightly more than half of all the fainter, sun-like
stars
are multiples. However, only about 25 percent of red dwarf stars have
companions. Combined with the fact that about 85 percent of all stars
that
exist in the Milky Way are red dwarfs, the inescapable conclusion is
that
upwards of two-thirds of all star systems in the Galaxy consist of
single,
red dwarf stars.

The high frequency of lone stars suggests that most stars are single
from
the moment of their birth. If supported by further investigation, this
finding may increase the overall applicability of theories that explain
the
formation of single, sun-like stars. Correspondingly, other
star-formation
theories that call for most or all stars to begin their lives in
multiple-star systems may be less relevant than previously thought.

"It's certainly possible for binary star systems to 'dissolve' into two
single stars through stellar encounters," said astronomer Frank Shu of
National Tsing Hua University in Taiwan, who was not involved with this
discovery. "However, suggesting that mechanism as the dominant method of

single-star formation is unlikely to explain Lada's results."

Lada's finding implies that planets also may be more abundant than
astronomers realized. Planet formation is difficult in binary star
systems
where gravitational forces disrupt protoplanetary disks. Although a few
planets have been found in binaries, they must orbit far from a close
binary
pair, or hug one member of a wide binary system, in order to survive.
Disks
around single stars avoid gravitational disruption and therefore are
more
likely to form planets.

Interestingly, astronomers recently announced the discovery of a rocky
planet only five times more massive than Earth. This is the closest to
an
Earth-size world yet found, and it is in orbit around a single red dwarf

star.

"This new planet may just be the tip of the iceberg," said Lada. "Red
dwarfs
may be a fertile new hunting ground for finding planets, including ones
similar in mass to the earth."

"There could be many planets around red dwarf stars," stated astronomer
Dimitar Sasselov of CfA. "It's all in the numbers, and single red dwarfs

clearly exist in great numbers."

"This discovery is particularly exciting because the habitable zone for
these stars - the region where a planet would be the right temperature
for
liquid water - is close to the star. Planets that are close to their
stars
are easier to find. The first truly Earth-like planet we discover might
be a
world orbiting a red dwarf," added Sasselov.

This research has been submitted to The Astrophysical Journal Letters
for
publication and is available online at
http://arxiv.org/abs/astro-ph/0601375

Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for
Astrophysics (CfA) is a joint collaboration between the Smithsonian
Astrophysical Observatory and the Harvard College Observatory. CfA
scientists, organized into six research divisions, study the origin,
evolution and ultimate fate of the universe.

For more information, contact:

David A. Aguilar
Director of Public Affairs
Harvard-Smithsonian Center for Astrophysics
617-495-7462
daguilar_at_cfa.harvard.edu

Christine Pulliam
Public Affairs Specialist
Harvard-Smithsonian Center for Astrophysics
Phone: 617-495-7463, Fax: 617-495-7016
cpulliam_at_cfa.harvard.edu


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Received on Wed 01 Feb 2006 09:21:58 AM PST