[meteorite-list] SOHO Prepares For Comet McNaught

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu, 11 Jan 2007 09:51:25 -0800 (PST)
Message-ID: <200701111751.JAA19302_at_zagami.jpl.nasa.gov>

ESA News
http://www.esa.int

11 January 2007

SOHO prepares for comet McNaught

Recently, sky watchers in the Northern Hemisphere have been enjoying the
sight of Comet McNaught in the twilight sky. Now, solar physicists using the
ESA-NASA SOHO spacecraft are getting ready for their view. For four days in
January, the comet will pass through SOHO's line of sight and could be the
brightest comet SOHO has ever seen.

As Comet McNaught heads towards its closest approach to the Sun on 12
January 2007, it will disappear from view for earthbound observers, becoming
lost in the Sun's glare. That's where SOHO comes in. Poised in space between
the Earth and Sun, SOHO ceaselessly watches the Sun and objects that pass
nearby.

Comet McNaught will pass within a fifth of the distance between the Earth
and the Sun. As the comet approaches the Sun, the amount of dust and gas it
releases will increase dramatically, causing the comet to become extremely
bright. "This might become the brightest comet SOHO has ever seen," says
Bernhard Fleck, SOHO Project Scientist.

The material ejected from the comet forms the tails. There are two tails,
the dust tail and the gas -- or ion -- tail. The dust tail is the brighter
and is formed by the intense sunlight forcing dust particles away from the
comet. The solar wind, a constant stream of material flowing from the Sun,
drags ionized gas from the comet to create the ion-tail.

Researchers Karl Battams and Jeff Morrill at the Naval Research Laboratory
in Washington, DC are planning colour filter observations of these two comet
tails. "Close to the Sun the ion and dust tails move apart, a phenomenon
that is often difficult to observe from the Earth. By measuring the ion-tail
angle we can get information about the solar wind speed very close to the
Sun," says Morrill.

Comet McNaught is moving through space on an inclined orbit. This will carry
it above the Sun's north pole and across the Sun's equator, a place where
there is a reversal of the magnetic properties of the solar wind. Crossing
this boundary could cause the comet's ion-tail to fragment. Observations of
such events are generally very rare, so SOHO's images of comet McNaught
constitute an exciting opportunity for scientists.

After SOHO's work is finished, the comet will emerge from the Sun's glare
and become visible again to earthbound sky watchers in the Southern
Hemisphere. "It could become a really bright object in the twilight sky,"
says Fleck. The ghostly veils of a bright comet are amongst the most
spectacular of sights that can be seen in the night sky.

Between 12 and 15 January, Comet McNaught will not be visible from Earth but
everyone can still track the comet's passage near the Sun by looking at the
SOHO images at
     http://soho.esac.esa.int/hotshots/

For more information
 
Bernhard Fleck, ESA SOHO Project Scientist
Email: bfleck _at_ esa.nascom.nasa.gov

Daniel Mler, ESA SOHO Deputy Project Scientist
Email: dmueller _at_ esa.nascom.nasa.gov

Karl Battams, Naval Research Laboratory, Washington DC, USA
Email: karl.battams _at_ nrl.navy.mil

Jeff Murrill, Naval Research Laboratory, Washington DC, USA
Email: morrill _at_ shogun.nrl.navy.mil

[NOTE: Images supporting this release are available at
http://www.esa.int/esaSC/SEMMCRSVYVE_index_1.html ]
Received on Thu 11 Jan 2007 12:51:25 PM PST