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Wednesday, 15 December 2010

[Baa-ebulletin 00546] GEMINID METEOR ACTIVITY INCREASING

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BAA electronic bulletin
======================================================================
BAA e-bulletin, 2010 Dec. 12
GEMINID METEOR ACTIVITY INCREASING

BAA observers have reported the first meteors of this year's Geminid meteor
shower, which is expected to peak around dawn on Tuesday, December 14.
The maximum is broad, however, and it is important to have a spread of
observers making observations on nights both before and after maximum.
During last year's very favourable display, peak Geminid Zenithal Hourly
Rates approached 140 m/h, and similar rates may be expected this year in the
pre-dawn hours.

The Geminid radiant (at RA 07h 32m  Dec +33o, just north of Castor) rises
early on and reaches a respectable altitude well before midnight, but
observers will achieve better results in the early morning hours this year
because the waxing gibbous Moon in Pisces will rather hamper observations
earlier in the night. The early morning hours of December 14, as dawn
approaches, are likely to yield the best observed rates this year, but
watches on the mornings of December 13 and 15 should also be worthwhile,
with the radiant still high in the sky.

Active through to Thursday, December 16, the Geminids are currently the most
active of the regular annual showers, with rates outstripping those of the
Perseids for a 24-hour interval centred on the peak - a real treat for
observers prepared to brave the winter cold and damp.

Additional information about the Geminid shower is given in the 'Notes and
News' section of the December BAA Journal.

For further details, or copies of report forms, observing notes, and
details of how to carry out group meteor watches, please visit the BAA
Meteor Section website at
http://britastro.org/meteor or contact the
undersigned:

John Mason
Acting Director, BAA Meteor Section
email:
docjohn@dircon.co.uk

51 Orchard Way, Barnham, West Sussex PO22 0HX
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Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
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Web:
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Geminid Meteors and a "Spiral Asteroid"

Space Weather News for Dec. 12, 2010
http://spaceweather.com

GEMINID METEOR SHOWER: The Geminid meteor shower peaks this year on Dec. 13th and 14th.  Forecasters say meteor rates could exceed 100 per hour for observers under dark rural skies.  For best results, start your meteor watch on Monday night, Dec. 13th, around midnight.  Keep an eye out for Geminids until sunrise on Tuesday, Dec. 14th. There's no special trick to seeing the Geminids.  Bundle up for maximum warmth, go outside, lie down and look up. Geminids can appear in any part of the sky, but all their tails will point back to the radiant in the constellation Gemini.  Check http://spaceweather.com for updates, images and a sky map.

SPIRAL ASTEROID:  Put this in the "weird" category.  Main belt  asteroid (596) Scheila has suddenly developed an apparently spiral-shaped tail.  The surprising structure might be a result of a recent asteroid-asteroid collision, or perhaps a sign that this asteroid is really a comet.  An image of Scheila is featured on today's edition of
http://spaceweather.com.

UNIQUE CHRISTMAS GIFT:  Would you like to put friends and family in closer touch with the night sky?  SpaceWeather PHONE makes a unique Christmas gift for the stargazer in your life.  
 
More information at http://spaceweatherphone.com ...

--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
--
Profile:
http://www.google.com/profiles/astrocomera
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra

[Baa-ebulletin 00545] Large main-belt asteroid (596) Scheila exhibits 'cometary' appearance

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BAA electronic bulletin
======================================================================
The first well-observed case has been reported of a large main-belt asteroid
apparently exhibiting 'comet-like' behaviour.

Steve Larson of the Lunar and Planetary Laboratory, University of Arizona,
has reported that images of the minor planet (596) taken on December
11.44-11.47 UT with the 0.68-m f/1.8 Schmidt telescope at Catalina show the
object to be in apparent outburst with a comet-like appearance, exhibiting a
total V magnitude of about 13.4 and an envelope that extends 2' north and 5'
west of the central condensation (CBET No.2583 issued December 12).  Note
that the predicted magnitude of this asteroid at the time of Steve's
observation is about 60% fainter than the observed value.

BAA member Peter Birtwhistle obtained images from Great Shefford Observatory
between December 12.178-12.204 showing the presence of a large arc to the
north and smaller arc to the south in a field 3'x3' in size - See:
http://www.birtwhistle.org/Gallery(596)Scheila.htm

(596) Scheila is a large asteroid (diameter ~113 km) situated in the outer
regions of the Main Belt, having a dark surface (albedo = 0.038). A rotation
period of 15.8 hours has been reported and from the amplitude of its
lightcurve(0.09 mag) it must be relatively spherical in shape.  In other
words it is a very ordinary, rather typical asteroid with no special
features.  Likewise its orbit is definitely asteroidal in nature and not
cometary.

It has been speculated that we have just witnessed the aftermath of a
high-speed collision between (596) and a small, non-descript object, perhaps
no more than a metre or two in size.  The two conjoined arcs visible in
Peter's stacked image are reminiscent of the arc-shaped material of 'Comet
P/2010 A2' imaged by the Hubble Space Telescope in January of this year -
See:
http://hubblesite.org/newscenter/archive/releases/2010/07/image/a/
For this latter case, it has now been shown that this phenomenon was not
cometary but was indeed the result of a collision between two small bodies
in the asteroid belt.

Further observations of the evolution of the 'debris', dust, etc. around
(596) Scheila should make it possible to discriminate between the collisonal
hypothesis and a cometary origin.  My money is on the former.  Indeed,
high-resolution spectroscopy of the emitted cloud of material could provide
a unique opportunity to probe the composition of an asteroid by analysing
the nature of the expelled material.  Let's hope that an 8-metre or 10-metre
class telescope will be put to work doing just this in the very near future.
Checks should also be made on images of (596) taken in the past to see
whether an associated coma can be found at some other epoch.  If such a coma
were to have occurred in the past then this would demonstrate recurrent
activity characteristic of a true comet.

Richard Miles
Director, Asteroids and remote Planets Section
BAA
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--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
--
Profile:
http://www.google.com/profiles/astrocomera
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
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[Baa-ebulletin 00544] Observing Alert: Spots on Saturn

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BAA electronic bulletin
======================================================================

Observing Alert: Spots on Saturn

On 8 Dec 2010 two spots were recorded on Saturn at the same latitude.

Firstly, a bright spot was recorded close to the central meridian in
an image taken at 02:12UT by Sadegh Ghomizadeh in Iran.
The provisional position for this spot masured from the image is:
latitude 37.5 degrees north (planetographic), longitude (System 3) 248 degrees.

Just over 5 hours later, David Gray in the UK visually recorded a
light spot approaching the p. limb.
The provisional position for this spot measured from David's drawing is:
latitude of 37.5 degrees north,  longitude (System 3) 29 degrees.

Saturn is well placed for observation before dawn and more
observations are urgently required to confirm these features.

Mike Foulkes
BAA Saturn Section director.
12 December 2010
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--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra

[Baa-ebulletin 00543] BRILLIANT FIREBALL OF 2010 DECEMBER 8

======================================================================
BAA electronic bulletin
======================================================================
BAA e-bulletin, 2010 Dec. 11

BRILLIANT FIREBALL OF 2010 DECEMBER 8

Reports are coming in of a brilliant fireball seen on the evening of
Wednesday, 8th December 2010 at around 17:40 UT.  A more precise time for
this event has still to be determined.

Sightings indicate that the fireball was visible over an extremely large
area of the country, with reports being received from locations as far apart
as Bath, Northampton, Leicester and the Isle of Man.

The peak brightness of the fireball was in excess of magnitude -8, and
eyewitnesses report that the object fragmented towards the end of its
trajectory.

Further reports of this event are urgently required. Did you see this
fireball yourself, or do you know of someone else who saw it?  Those
belonging to local astronomical societies are asked to enquire of other
society members whether they witnessed the event. Please take care not to
bias eyewitnesses beforehand by discussing with them what you or others saw.

Reports should contain some or all of the following information:

1) Name, address and contact details of the observer.

2) Date and time of the event in UT (GMT), as accurately as this can be
specified.

3) Location of the observer when witnessing the fireball.  If driving a car
please specify the road, location and the direction the observer was
driving.

4) The path of the fireball against the background stars, as accurately as
this can be described.  If this is not possible, then please try to answer
questions 5) and 6) below:

5) The compass direction and altitude (in degrees) of the fireball when it
was first seen.

6) The compass direction and altitude (in degrees) of the fireball when it
was last seen. Please state if something obscured the view of the end (e.g.
if it went behind a tree or a building).

7)  A general description of the colour and appearance of the fireball,
whether this changed during the trajectory and any terminal burst or
break-up at the end.

Please send in your completed reports as soon as possible.

John Mason
email:
docjohn@dircon.co.uk


51 Orchard Way, Barnham, West Sussex PO22 0HX

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--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra

Thursday, 9 December 2010

[Baa-ebulletin 00542] Venus

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BAA electronic bulletin
======================================================================
 
VENUS

Venus is now quite well placed for observation in the morning sky, but
she seems to be being ignored telescopically by the vast majority of
our members. Perhaps conditions in the UK are too extreme at present?
The Director would like to have a far greater number of observations
to hand for analysis, and he would urge members to make the effort to
observe.

At or before 7 am the sky is still dark enough (and the phase ideal)
to make a search for the Ashen Light either visually or by imaging.
Negative observations will be of value, but not once the sky has
become too bright. If the phenomenon is seen or suspected, try hiding
the bright crescent with an occulting bar or even placing Venus at the
edge of the field, to see whether it still remains visible (and so to
avoid the possibility of illusion).

The bright crescent has shown the usual fugitive markings to Mario
Frassati, David Gray and the Director. To Gray on November 28, and to
the Director on December 3 and 7 the region of the south cusp was
considerably brighter than the north. A good series of images has been
received from Sadegh Ghomizadeh (Tehran).

Where are all the other observers? A quick visual inspection will not
take you very long, and you may be able to make a valuable
contribution. Please give all the usual data with your observation.

With Season's greetings,


Richard McKim, Director

2010 December 8
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======================================================================
--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Profile:
http://www.google.com/profiles/astrocomera
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra

BRIGHT FIREBALL SEEN OVER BRITAIN

        **********************************
         The SOCIETY for POPULAR ASTRONOMY
          ***********************************
       =====================================================
        Special Electronic News Bulletin    2010 December 9
       =====================================================
 
 
BRIGHT FIREBALL SEEN OVER BRITAIN
 
Many people saw a spectacular fireball at around 17.40 GMT last
night.  The unusually bright object, witnessed by observers in
Scotland, England and Wales, was seen to explode, leaving a green
trail in its wake.  There is speculation that the fireball may be a
precursor to the annual Geminid meteor shower which peaks on December
13 -- 14.  The Geminids are unusual in that the parent body is not a
comet but an asteroid, 3200 Phaethon.
 
The BBC has asked the Society for Popular Astronomy to appeal for
any photos that ENB readers may have obtained of last night's event.
Please forward them to me at    SPAstronomy@aol.com
 
 
Bulletin compiled by Clive Down
 
 
(c) 2010 the Society for Popular Astronomy
 
 
--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
--
 

Wednesday, 8 December 2010

SPA ENB No. 300

                ***********************************
                 The SOCIETY for POPULAR ASTRONOMY
                ***********************************
        ====================================================
         Electronic News Bulletin No. 300   2010 December 5
        ====================================================
 
 
Here is the latest round-up of news from the Society for Popular
Astronomy.  The SPA is Britain's liveliest astronomical society, with
members all over the world.  We accept subscription payments online
at our secure site and can take credit and debit cards. You can join
or renew via a secure server or just see how much we have to offer by
 
 
RHEA HAS AN 'ATMOSPHERE', BUT IT IS AN INCREDIBLY THIN ONE
BBC News
 
Scientists using the Cassini probe say that Rhea, the second-biggest
of Saturn's moons, has an excessively thin atmosphere of oxygen and
carbon dioxide.  Oxygen exospheres have previously been found on
Jupiter's moons Europa and Ganymede.  The tenuous envelope around Rhea
is maintained by high-energy particles that constantly bombard the
moon's icy surface.  As Saturn's magnetic field rotates with the
planet, particles carried in the field impinge on the hemisphere of
Rhea that faces their flow and break water molecules on the surface.
The atoms then rearrange themselves to make O2 molecules, which are
sputtered from the surface by other impacting particles.  It is an
ongoing process -- as fast as the oxygen is created, it is being lost
into space.  The researchers say that the mechanism driving the
production of carbon dioxide is less obvious.  Like the O2, it could
be being produced as a result of high-energy particle impacts, if
carbon- containing compounds are present in the surface ice.  It is
possible also that the carbon dioxide was made in deep sub-surface
processes and the CO2 is slowly escaping the moon's body.  Cassini's
mass spectrometer measured peak densities of oxygen and carbon dioxide
of about 50 and 20 molecules per cubic millimetre, respectively.  Such
a density of oxygen is about 10*(-14) of that at sea-level on the
Earth, so it is hardly likely to support life as we know it.
 
 
ASTRONOMERS FIND 'ROSETTA STONE' FOR T-DWARF STARS
RAS
 
An international team of astronomers has discovered a star system with
a very cool methane-rich (or T-) dwarf star and a white-dwarf stellar
remnant in orbit around one another.  The system is the first of its
kind to be found, and gives scientists a means to estimate the mass
of a T dwarf.  The two stars are low in mass and have a weak mutual
gravitational attraction, as they are separated by about a quarter of a
light-year.  Despite the frailty of the system it has stayed together
for billions of years, but its stars are cooling down to a dark
demise.
 
Methane dwarfs are on the star/planet boundary and are about the size
of Jupiter.  They have temperatures of less than 1000°C.  Methane is a
fragile molecule destroyed at higher temperatures, so it is seen only
in very cool stars and objects like Jupiter.  Neither giant planets
nor T-dwarf stars are hot enough for the hydrogen fusion that powers
the Sun to take place, so they simply cool and fade over time.  White
dwarfs are the end state of stars similar to and including the Sun.
Once such stars have exhausted the available nuclear fuel in their
cores, they expel most of their outer layers into space, forming a
remnant planetary nebula, and leave behind a hot, but cooling, core
or white dwarf about the size of the Earth.  In the newly-discovered
binary, the remnant nebula has long since dissipated, and all that is
left is the steadily cooling white dwarf and its methane-dwarf
companion.  The present temperature of the white dwarf provides an
estimate of the age of both objects, and calibrates properties of the
methane dwarf such as its mass.
 
The methane dwarf was identified by UKIRT as part of a project to
identify the coolest objects in the Galaxy.  Its temperature and
spectrum were measured by the Gemini North telescope in Hawaii.  The
team then found that the methane dwarf shares its proper motion with a
nearby blue object catalogued as LSPM 1459+0857, which they studied
with the VLT, finding it to be a cool white dwarf.  The objects were
then re-named LSPM 1459+0857 A and B.
 
 
MASS OF ONE CEPHEID VARIABLE STAR DETERMINED
European Southern Observatory
 
Astronomers have used the 3.6-m NTT telescope in Chile to observe the
first double star to be discovered in which a pulsating Cepheid
variable and another star eclipse one another, and have determined
accurately the mass of the Cepheid.  Up to now astronomers had two
incompatible theoretical predictions of Cepheid masses; the new result
shows that the prediction from stellar-pulsation theory is correct,
while the prediction from stellar-evolution theory is not.  Classical
Cepheid variables, usually just called Cepheids, are unstable stars
that are much larger and brighter than the Sun.  They expand and
contract in a regular way, taking anything from a few days to a month
or so to complete the cycle.  There is a relationship between the
stars' luminosities and the periods of their variability, making the
study of Cepheids a way to estimate the distances to 'nearby' galaxies
and from there to extrapolate the distance scale to the whole Universe.
 
Unfortunately, Cepheid masses derived from the theory of pulsating
stars are 20-30% less than predictions from the theory of the
evolution of stars.  That embarrassing discrepancy has been known
since the 1960s.  The discovery of an eclipsing binary that includes a
Cepheid has now allowed the mass of one such star to be determined
accurately from the orbital parameters derived from radial-velocity
measurements.  The system is in the Large Magellanic Cloud and
contains a Cepheid pulsating every 3.8 days.  The other star is
slightly bigger and cooler, and the two stars orbit one another in 310
days.  The mass of the Cepheid was found to be 4.14 ± 0.05 solar
masses, in excellent agreement with expectations from the theory of
stellar pulsation.
 
 
PLANET FROM ANOTHER GALAXY
ESO
 
In the last 15 years, astronomers have detected nearly 500 planets
orbiting stars in our cosmic neighbourhood, but none outside our Milky
Way.  Now, a planet with a minimum mass 1.25 times that of Jupiter has
been discovered orbiting a star that is thought to be of extragalactic
origin, although it is now in our own Galaxy.  It is part of the
'Helmi stream' -- a group of stars that may have belonged originally
to a dwarf galaxy that merged with the Milky Way billions of years ago.
 
The star, known as HIP 13044, is about 2000 light-years away in the
southern constellation Fornax.  The astronomers detected the planet
from radial-velocity measurements made with the 2.2-m telescope at La
Silla in Chile.  The planet is one of the few such objects known to
have survived the period when its host star passed through the
red-giant phase of stellar evolution and became very much bigger after
exhausting the hydrogen fuel supply in its core.  The star has now
contracted again and become a so-called horizontal-branch star,
burning helium in its core.  Even so, the planet is less than one
stellar diameter from the surface of the star at periastron (the
closest point in its elliptical orbit).  Its 'year' -- the time taken
to complete an orbit -- is only 16.2 days.
 
 
POSSIBLE COLLISION IN LOCAL GROUP AGES AGO
Paris Observatory
 
Numerical simulations suggest that a major collision between two
massive galaxies occurred in the Local Group 6 billion years ago.
It seems that the Andromeda Galaxy (M31), as well as the Magellanic
Clouds, may have formed as a result of such a collision between
two galaxies.  The Local Group includes nearly 40 galaxies and is
dominated by two giant spiral ones -- Andromeda and our own Galaxy,
the Milky Way.  Some astronomers believe that Andromeda may have
formed through a collision and merger event between two galaxies, one
slightly more massive than the Milky Way, the other about 3 times less
massive.  The epoch suggested for the event is that the first passage
and the final fusion occurred about 9 and 5.5 billion years ago,
respectively.  Such a collision would be the most important event that
has ever occurred in the Local Group, because the Andromeda galaxy and
its satellites gather the largest fraction of the mass of the Group.
The collision must have been violent enough to generate the large
amount of angular momentum (rotation) needed to form the great
galactic disc of Andromeda.
 
The researchers also considered the possible consequences of such a
major event in the neighbourhood of our Galaxy, and proposed
that the Magellanic Clouds could have formed within one of the tidal
tails produced during the interaction 9 billion years ago.  The Clouds
might have been ejected towards the Milky Way, at a velocity that has
recently been re-evaluated at about 300 km/s.  That might explain why
the Magellanic Clouds are the only gas-rich and irregular companions
of the Milky Way.
 
 
MASSIVE GALAXIES MAY HAVE BEEN FORMED WHEN THE UNIVERSE WAS YOUNG
ScienceDaily
 
Astronomers have identified a large number of galaxies five to ten
times more massive than our own Milky Way among a sample studied at
red-shifts 3 to 4, when the Universe was between 1.5 and 2 billion
years old.  More than 80% of the massive galaxies show very high
infrared luminosities, indicating that they were extremely active,
probably in a phase of intense growth.  Current ideas about the
physical processes responsible for forming such massive galaxies has
difficulty in producing them so quickly.  Before too much excitement
is generated by that difficulty, however, the caveat is made that the
red-shifts were estimated only from spectral energy distributions and
not by actual spectroscopy, and may be mistaken.
 
 
Bulletin compiled by Clive Down
 
 
(c) 2010 the Society for Popular Astronomy
 
 
--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
--

[Baa-ebulletin 00540] Reminder for Next meeting of the BAA

========================================================
BAA electronic bulletin
========================================================
I would like to remind you that the next meeting of the BAA will be on
Saturday 11th December 2010 in the new lecture room, Burlington House.

14:30 Dr David Boyd BAA President - Welcome OM, notices etc
14:40 Stewart Moore - Sky Notes
15:00 Dr Martin Dominik - Theory of photometric and astrometric microlensing
16:00 Tea
16:25 Dr David Arditti - Christmas Lecture - Andrew Anslie Common:
the First Modern Astronomer
17:30 Close

Doors open at 14.00 and the meeting will start at 14.30 and is due to
finish by 17:30. Tea will be served in the library at 16:00. Please
not there will be no tea before the meeting.

Hope to see you there

Hazel

Hazel Collett
Meeting Secretary
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========================================================
--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Profile:
http://www.google.com/profiles/astrocomera
--
Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
--
Web:
http://lyra.freewebsites.com/
--
Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra

Demonstration Flight Of Falcon 9 Rocket Set For Wednesday

Demonstration Flight Of Falcon 9 Rocket Set For Wednesday
Mon, 06 Dec 2010 23:00:00 -0600

The first demonstration flight of SpaceX's Falcon 9 rocket and Dragon capsule for NASA's Commercial Orbital Transportation Services program has been scheduled for Wednesday, Dec. 8, from Cape Canaveral Air Force Station in Florida.


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Good Clear Skies
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Astrocomet
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Colin James Watling
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Profile:
http://www.google.com/profiles/astrocomera
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Real Astronomer and head of the Comet section for LYRA (Lowestoft and Great Yarmouth Regional Astronomers) also head of K.A.G (Kessingland Astronomy Group) and Navigator (Astrogator) of the Stars (Fieldwork)
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Web:
http://lyra.freewebsites.com/
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Information:
http://www.clubbz.com/club/2895/LOWESTOFT---3054/Lowestoft%20And%20Great%20Yarmouth%20Regional%20Astronomers%20(Lyra