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Thursday 27 October 2011

Charts-info Astrosite Groningen (October 24, 2011)

Dear comet observers,
 
We have prepared the following new chart for our homepage:
 *  45P/Honda-Mrkos-Pajdusakova: 
  • a 5.0x6.7 degrees chart for the period 25 October - 3 November 2011.
 This new chart can now be downloaded from the charts section of our mainpage:
Here you can also download charts from earlier updates....
Reinder Bouma/Edwin van Dijk.
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--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

Monday 24 October 2011

SPA ENB No. 319



                 ***********************************
                 The SOCIETY for POPULAR ASTRONOMY
                ***********************************
        ====================================================
         Electronic News Bulletin No. 319   2011 October 23
        ====================================================


Here is the latest round-up of news from the Society for Popular
Astronomy.  The SPA is one of Britain's liveliest astronomical
societies, 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 visiting  
http://www.popastro.com/


DRACONID METEOR OUTBURST

Observations by BAA members and others indicate that a short-lived
outburst of Draconid meteors occurred on 2011 October 8.  Observers in
the UK had to contend with cloud and rain on the evening of October 8,
but it is extremely encouraging that so many individuals and local
society groups battled the elements in the hope of getting a view of
the shower.

More observations of the Draconid outburst, by photographic, visual,
and radio techniques, from individuals and groups in the UK and
overseas, are urgently required to build up a full picture of the
shower's rapidly changing activity.  Even if you have only glimpsed a
few meteors during a short-lived break in the clouds, the BAA Meteor
Section would like to receive your report.  So if you did manage any
sort of observations, please submit them to the BAA Meteor Section,
either via email to:
meteor@britastro.org or by post to: Draconid
Meteor Project 2011, British Astronomical Association, Burlington
House, Piccadilly, London W1J 0DU.


WATER SIMILAR TO THAT IN EARTH'S OCEANS FOUND IN COMET
The Register

Ice found in a comet is consonant with a theory that the Earth's
oceans were delivered here by comets.  (Of course it would take an
awful LOT of comets to fill an ocean!)  Be that as it may, it has been
proposed that the oceans formed about 8 million years after the Earth
itself.  An instrument on the Herschel space observatory is able to
determine the isotopic composition of hydrogen, and has found that ice
in Comet Hartley 2 has the same isotopic composition, i.e. the same
proportion of deuterium to ordinary hydrogen, as the water found in
our oceans.  Herschel has observed six other comets, but only the ice
in Hartley 2 matches the Earth's water.  Hartley 2 comes from the
Kuiper belt, not too far beyond Pluto, whereas the other five come
from the hypothesised far-off Oort Cloud.  The Kuiper belt is about 30
times further from the Sun than the Earth is; the Oort Cloud is
supposed to be more than 5,000 times further out than the Earth.

Meanwhile, analysis of data from the Deep Impact spacecraft, which
passed close to Hartley 2 on 2010 November 4, shows that that comet
throws off much more material in relation to its own size than Tempel
1, which was encountered by Deep Impact in 2005, or Wild 2, which was
observed by the Stardust mission.  Halley, which was observed by the
Giotto mission, lies somewhere in the middle of the spectrum of
activity.  Hartley 2 also shows surprising diversity -- ice on the
comet's sunlit surface is found in patches that are isolated from
areas of dust.  In addition, one lobe of the dog-bone-shaped comet
may have lost much more of its primordial material than the other,
suggesting that Hartley 2 may originally have been two comets that
came together in a gentle collision.


THE CAUSE OF ASTEROID SCHEILA'S OUTBURST
RAS

On 2010 December 12 a 110-km asteroid named Scheila changed its
appearance and looked more like a comet, with a bright tail.  Comets
tend to have highly elliptical orbits that keep them most of the time
in the cold outer parts of the Solar System, and it is when they come
briefly close to the Sun that the heat causes icy material in the
comet to vaporize and stream out, forming the characteristic tails.
Asteroids, however, are supposed to be just rocky bodies that
primarily circle the Sun between the orbits of Mars and Jupiter.
That an asteroid acquired a comet-like tail took some explaining.
Astronomers measured the brightness of Scheila's tail, noting how it
declined over the course of several weeks.  They think that the tail
was caused by another object colliding with Scheila and causing debris
to be thrown off.  The best estimates are that the collision occurred
within three days either side of 2010 November 27, and that the
impactor had a diameter in the range 60--180 m.


ABOUT URANUS AND ITS SIDEWAYS SPIN
RAS

Uranus is unusual in that its spin axis is inclined by 98° to its
orbital plane around the Sun.  That is quite different from the axial
inclinations of the other planets (Mercury O°, Venus 177°, Jupiter
3°, or the Earth, Mars, Saturn and Neptune, all around 25°),
although Pluto, at 120°, is not so very different.  Uranus is, in
effect, spinning on its side.

It has been suggested that in the past a body a few times more massive
than the Earth collided with Uranus, knocking the planet on its side.
There is, however, a significant flaw in that notion: the moons of
Uranus should have been left orbiting in their original plane, but
they too lie at almost exactly 98 degrees.  Scientists at Observatoire
de la Cote d'Azur in Nice have now realised that if Uranus had been
hit when still surrounded by a protoplanetary disc (the material from
which the moons would form) then the disc would have re-formed in the
new, highly-tilted equatorial plane, and would then go onto form the
moons in the positions in which we see them today.  The computer
models, however, threw up an unexpected result: the moons displayed
retrograde motion -- they orbited in the opposite direction to that
which we observe. The researchers discovered that if Uranus were not
tilted all in one go, but rather was bumped in at least two smaller
collisions, then there is a much higher probability that the moons
would orbit in the direction we observe.  The received theory includes
an assumption that the outer planets formed by accreting only small
objects in their protoplanetary discs; the indication now that Uranus
may have suffered at least two major impacts may warrant a revision of
that assumption.


UNUSUAL MULTI-PLANET SYSTEM DISCOVERED
NASA

The Kepler spacecraft is constantly measuring, very accurately, the
magnitudes of a large number of stars in a field in Cygnus, looking
for small dips in brightness caused by planets transiting across the
faces of the stars.  It has recently discovered an unusual planetary
system containing a super-Earth and two Neptune-sized planets orbiting
in resonance with each other around Kepler-18, a star that is just 10%
larger than the Sun and contains 97% of the Sun's mass.  The planets
are designated b, c, and d; they all orbit much closer to Kepler-18
than Mercury does to the Sun.  The closest, b, has a 3.5-day period,
is about 6.9 times the Earth's mass, and twice Earth's size; it is
what has been dubbed a 'super-Earth'.  Planet c has a mass of about
17 Earths, is about 5.5 times the Earth's size, and orbits in 7.6
days.  Planet d has about 16 Earth masses, 7 times Earth's size, and
a 14.9-day orbit.  The masses and sizes of c and d qualify them as
low-density 'Neptune-class' planets.

Planet c orbits the star twice for every one orbit that d makes.  But
the times that each of the planets transit the face of Kepler-18 are
not keeping exactly on that orbital period.  One is slightly early
when the other one is slightly late, then both are on time at the same
time, and then vice-versa.  They are in what is called an orbital
resonance, in which they interact with one another and periodically
exchange energy.


SEVEN SUPERNOVAE IN ONE GALAXY
ScienceDaily

It is hardly surprising that galaxies that are prolifically forming
stars are also prolifically letting off supernovae.  Now seven
previously unknown supernovae have been detected in a galaxy called
Arp 220, 250 million light-years away.  Astronomers using a worldwide
network of radio telescopes obtained extremely sharp images of Arp
220. They observed about 40 radio sources in the centre of the galaxy;
the sources are invisible in ordinary telescopes, hidden behind thick
layers of dust and gas.  The variation of radio brightness with wave-
length and time convinced the astronomers that seven of the sources
are supernovae that appear to have exploded within the last 60 years.
In Arp 220, we see far more supernovae than in our own Galaxy, the
Milky Way, in which there is said to be only one supernova per
century.  (But the last one was seen in 1604!)  The radio measurements
have also offered some insight into how radio waves are generated in
supernovae and their remnants.


CRAB PULSAR BEAMS UNEXPECTEDLY ENERGETIC GAMMA RAYS
University of California

The Crab pulsar is a rapidly spinning neutron star, the collapsed core
of a massive star that exploded in a spectacular supernova in the year
1054, leaving behind the brilliant Crab Nebula, with the pulsar at its
heart. It is one of the most intensively studied objects in the sky.
Rotating about 30 times a second, the pulsar has an intense,
co-rotating magnetic field from which it emits beams of radiation.
The beams sweep around like a lighthouse beacon because they are not
aligned along the star's rotation axis, so although the beams are
steady, they are detected on Earth as rapid pulses of radiation.
Scientists have long agreed on a general picture of what causes pulsar
emission -- electromagnetic forces created by the star's rapidly
rotating magnetic field accelerate charged particles to near the speed
of light, producing radiation over a broad spectrum -- but the details
remain obscure.  The picture led to an expectation of an exponential
decay of the emission spectrum above about 10*10 electron volts (10
GeV), so it has come as a surprise that the Whipple Observatory in
Arizona has now found pulsed gamma-ray emission at energies above 100
GeV -- far beyond what current theoretical models of pulsars can
explain.


THE TIME OF RE-IONISATION
ESO

It is thought that, early in the history of the Universe, there was a
time when the initial universal fog of neutral hydrogen gas was
clearing, allowing ultraviolet light to pass unhindered for the first
time.  It is called the 'epoch of re-ionisation', and occurred about
13 billion years ago.  ('Neutral' hydrogen atoms consist of a proton
and an electron; they can be 'ionised' -- the electron can be removed
-- by energetic (ultraviolet-light) photons.  Such photons trying to
pass through a lot of neutral hydrogen gas get absorbed and their
energy goes into ionising the  gas; when the gas is already ionised
there is nothing left for them to do, so then they can pass freely.)

Scientists have been using the Very Large Telescope to observe some
very distant galaxies, in an effort to establish a calendar for
re-ionisation.  It seems that that phase must have happened more
quickly than was previously thought.  One of the strongest ultraviolet
emission lines is the Lyman-alpha line of hydrogen, which is bright
and recognisable enough to be seen even in observations of very faint
galaxies.  Observations of the Lyman-alpha line in the spectra of five
very distant galaxies allowed the team to do two things.  First the
red-shift of the line enabled them to place them in chronological
order.  Secondly, they were able to see the extent to which the
Lyman-alpha emission from within the galaxies was absorbed by the
neutral-hydrogen fog in inter-galactic space at different points in
time.

The scientists saw a great difference in the amount of ultraviolet
light that was blocked between the earliest and latest galaxies in
their sample.  When the Universe was 780 million years old the neutral
hydrogen was quite abundant, filling from 10 to 50% of the Universe's
volume.  But 'only' 200 million years later the amount of neutral
hydrogen had dropped to a very low level, similar to its present one.
As well as indicating the rate at which the primordial fog cleared,
the observations also hint that the source of the ultraviolet light
which ionised the hydrogen was the first generation of stars, which
must have included many very massive stars which would burn up very
quickly and emit a great deal of ultraviolet.



Bulletin compiled by Clive Down


(c) 2011 the Society for Popular Astronomy



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Good Clear Skies
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Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

Orionid Meteor Shower

Space Weather News for Oct. 21, 2011
http://spaceweather.com

WEEKEND METEOR SHOWER: Today Earth is entering a stream of debris from Halley's comet, source of the annual Orionid meteor shower. Forecasters expect the shower to peak on Saturday morning, Oct. 22nd, with more than 15 meteors per hour.  Check
http://spaceweather.com for links to a live meteor radar, sky maps and observing tips.

MASSIVE SATELLITE NEARS RE-ENTRY: The massive ROSAT X-ray space telescope is making its final spiralling orbits around Earth. Most experts agree that re-entry will occur during the early hours of Oct. 23rd over a still-unknown region of our planet.  Sky watchers report that the descending satellite can be as bright as a first magnitude star and it occasionally "flares" to even greater intensity.  For last-chance sightings of ROSAT in your area, please check SpaceWeather's online satellite tracker (
http://spaceweather.com/flybys) or turn your smartphone into a ROSAT tracker: http://simpleflybys.com .

--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

Friday 21 October 2011

Whatever goes up must come down

Ready for Rosat's Reentry?

The old saying "Whatever goes up must come down" doesn't always apply to spacecraft, but it does most of the time. And, to be honest, old satellites, rocket parts, and big chunks of orbiting debris come crashing back to Earth almost weekly without much notice.

Only several dozen space scraps have ever been found after reentry despite thousands of launchings. The two credible reports I could find of someone being hit by falling space debris involve five Japanese sailors injured by a Russian reentry in 1969, and the tiny piece of a Delta II's fuel tank that glanced off Lottie Williams in Tulsa, Oklahoma, in 1997.

Germany's Röntgensatellit (known as Rosat) started its mission in an orbit 360 miles (580 km) high. But it's predicted to reenter Earth's atmosphere in late October 2011.

DLR

That's why you didn't see anything here about the over-dramatized reentry of NASA's Upper Atmosphere Research Satellite last month — and nary a word about a 6-ton Chinese rocket booster that fell to Earth a week ago.

But the situation with Röntgensatellit (usually called Rosat) is worth mentioning, because this time the doomed craft is a German-built X-ray observatory launched by NASA in 1990. Its total mass is nothing special, just 2½ tons (less than half that of UARS). But much of that is concentrated in the telescope itself, which consists of two sets of nested mirrors made of gold-plated Zerodur bonded to a carbon-fiber structure.

Rosat employed gold-plated ceramic glass mirrors, four hyperboloids and four hyperboloids, nested in two sets. Such a grazing-incidence arrangement, known as a Wolter type I configuration, is necessary to bring X-rays to a focus.

Bernd Aschenbach / Zeiss

Zerodur is an ultralow-expansion ceramic glass, much like the shiny-smooth surface found on modern stovetops. With a melting point of 1,100°F (600°C), it's unlikely to bubble into oblivion during reentry.

An analysis by the European Space Agency's Space Debris Office suggests that the spacecraft could begin to break apart at an altitude of about 65 miles (105 km). But the entire mirror assembly — 1.6 metric tons in all — should hit the ground intact at hundreds of miles per hour. Up to 29 other fragments, totaling another 200 pounds (100 kg), might survive the white-hot descent as well.

As was the case with UARS, Rosat has no propulsion system on board and so there's no way to control where and when it falls to Earth. Rosat's orbit is inclined 53° to the equator, putting virtually all inhabited areas at some risk. According to ESA's Heiner Klinkrad, the odds of anything striking somewhere in Germany (or in a comparable target area, say, Montana) are about one in 580.

With an orbital inclination of 53°, Rosat could fall anywhere in latitude between southern Canada and the tip of South America. Three representative orbits are shown.

DLR

"One day before Rosat reenters, we will be able to predict its landing with an accuracy of within one orbit," Klinkrad says. That's still an hours-long window covering a wide swath of land and ocean. As of this morning, the oddsmakers had pegged Sunday morning, October 23rd, as the most likely reentry time. But that prediction is still considered uncertain by ± 72 hours.

In a way, it's sad that hard-working satellites like UARS and Rosat only make the news when they fall from the sky in pieces. They deserve better. Measurements from UARS helped unlock the secrets of how chlorine-based gases create the atmosphere's ozone holes and allowed scientists to track the spread of sulfurous gases from Mount Pinatubo's titanic 1991 eruption.

This is a High-Resolution Imager (HRI) observation of the expanding bubble of a supernova observed by Danish astronomer Tycho Brahe in 1572.

S. L. Snowden

Likewise, during its eight years of service, Rosat gave astronomers an important window on the X-ray universe (Röntgen is the German word for X-ray). Its wide-field camera, supplied by British researchers at the University of Leicester, surveyed the entire sky. More importantly, a high-resolution imager, built by a NASA-funded team at the Harvard-Smithsonian Center for Astrophysics, zeroed in on thousands of million-degree-hot cosmic phenomena such as active galactic nuclei, neutron stars, and supernovae remnants. It even discovered, astoundingly, that some comets emit X-rays.

Operations came to an abrupt, premature end in September 1998, when Rosat's orientation system malfunctioned and caused the telescope to point directly at the Sun, which damaged the high-resolution imager beyond repair. Ground controllers shut down the craft for good the following February.

Officials at DLR might not be able to pinpoint the time and location of forthcoming Rosat's demise, but I'll give them credit for putting together an informative website (much of it in English) about the reentry and the observatory's accomplishments.

One last thought: Given all the hubbub regarding these two modest scientific satellites, I can't wait to hear how NASA plans to bring down the International Space Station when its time comes a decade or so from now. At the moment, there's no specific plan, though the project's partners are "committed to a controlled deorbit when the time comes," notes Nicholas Johnson, chief scientist for NASA's orbital-debris team.

 

Posted by Kelly Beatty, October 18, 2011

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Good Clear Skies
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Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

Sunday 16 October 2011

German satellite to fall from orbit / Delta 4 rolls out

 NEWSALERT: Thursday, October 13, 2011 @ 1403 GMT
--------------------------------------------------
  The latest news from Spaceflight Now


+++
NEW INTERNATIONAL SPACE STATION PATCHES!
Crew patches for Expeditions 31, 32 and 36 are now available from our
store.
http://www.spaceflightnowstore.com/
+++


ALL OVER AGAIN: GERMAN SATELLITE POISED FOR PLUNGE
--------------------------------------------------
Less than a month after NASA's falling UARS satellite grabbed the
headlines, the German space agency says one of its abandoned satellites
will dive back to Earth later this month, but no one knows where it will
land.

http://spaceflightnow.com/news/n1110/12rosat/


TROPICAL CLIMATE SATELLITE SOARS FOR INDIA, FRANCE
--------------------------------------------------
An Indo-French satellite launched on an international climate research
mission Wednesday, ascending into space to track tropical cyclones,
monsoons and storm systems for at least three years. The one-ton
spacecraft was put in orbit by an Indian rocket.

http://spaceflightnow.com/news/n1110/12meghatropiques/

LAUNCH PHOTO GALLERY:
http://spaceflightnow.com/news/n1110/12pslvphotos/


NEXT DELTA 4 ROCKET TO BOOST MILITARY COMMUNICATIONS
----------------------------------------------------
The United Launch Alliance Delta 4 rocket that will deploy a vital
communications satellite for U.S. military forces overseas was placed atop
its Cape Canaveral pad this week.

http://spaceflightnow.com/delta/d358/rollout.html

ROLLOUT PHOTO GALLERY:
http://spaceflightnow.com/delta/d358/rollout/


NASA HANDS ENDEAVOUR TO LOS ANGELES MUSEUM
------------------------------------------
Astronauts, celebrities and local officials held a ceremonial transfer of
ownership for the space shuttle orbiter Endeavour from NASA to the
California Science Center in Los Angeles on Tuesday.

PHOTO GALLERY:
http://spaceflightnow.com/shuttle/sts134/111011/

OUR STS-134 ARCHIVE:
http://spaceflightnow.com/shuttle/sts134/


+++
NEW IN OUR STORE: SPACE MODELS
Spaceships scaled to fit on your desk
http://spaceflightnowstore.com/us/catalog/
+++

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Good Clear Skies
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Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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)
--
Information -- More Info -- And More Info

Saturday 15 October 2011

Massive X-ray Satellite Set to De-orbit

ALL OVER AGAIN: GERMAN SATELLITE POISED FOR PLUNGE
--------------------------------------------------
Less than a month after NASA's falling UARS satellite grabbed the
headlines, the German space agency says one of its abandoned satellites
will dive back to Earth later this month, but no one knows where it will
land.
 
 
Space Weather News for Oct. 14, 2011
http://spaceweather.com

ROSAT RE-ENTRY: The ROSAT X-ray observatory, launched in 1990 by NASA and managed for years by the German Aerospace Center (DLR), will return to Earth within the next two weeks. Current best estimates place the re-entry between Oct. 22nd and 24th over an unknown part of Earth. ROSAT will produce a spectacular fireball when it re-enters, but not all of the satellite will disintegrate.  According to the DLR, heat-resistant fragments as massive as 1.7 tons could reach Earth's surface.  Check
http://spaceweather.com for more information.

LAST-CHANCE SIGHTINGS:  As ROSAT slowly descends it is growing brighter. During favorable passes, the satellite can now be seen shining as brightly as a first magnitude star in the night sky.  Local flyby times may be found using SpaceWeather's Satellite Tracker:
http://spaceweather.com/flybys .   Or turn your smartphone into a ROSAT tracker using our Simple Flybys app: http://simpleflybys.com .

Check
http://spaceweather.com for more information


--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
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)
--

Wednesday 12 October 2011

[BAA-ebulletin 00620] DRACONID METEOR OUTBURST OBSERVED

============================================================
BAA electronic bulletin
============================================================
DRACONID METEOR OUTBURST OBSERVED

Observations by BAA members and by non-members who have so far communicated
with the Director of the Meteor Section confirm that a short-lived outburst
of Draconid meteors occurred on 2011 October 8.

Draconid rates were generally low until around 1900 UT on October 8 when a
rapid increase in activity occurred, peaking between 2005 and 2015 UT.
Thereafter there was a rapid decline, with Draconid meteor rates returning
to a low level by 2130 UT.  A very preliminary analysis of visual
observations made by a group of observers led by the Director, observing
from near Goreme in central Turkey, indicates that the peak equivalent ZHR
was about 350 m/h between 2005 and 2015 UT, although correction factors are
high due to the effect of bright moonlight.  It is possible that lesser,
short-lived secondary bursts in Draconid activity were also noted around
1915 and 1938 UT.

Observers in the UK had to contend with cloud and rain on the evening of
October 8, but it is extremely encouraging that so many individuals and
local society groups battled the elements in the hope of getting a view of
the shower.  Some were rewarded for their persistence.  A short period of
partially clear weather enabled observers in Dorset, Wiltshire, Oxfordshire,
Gloucestershire and Berkshire (and hopefully other areas as well) to glimpse
the shower between 1955 and 2030 UT.  By a fortunate circumstance this was
coincident with the main peak in Draconid activity.

The Director is extremely grateful to all those observers in the UK who have
so far communicated with him by email, including: Len Entwisle, Peter Gill
(Eastbourne AS), Gerard Gilligan (Liverpool AS), Tim Haymes (Maidenhead AS),
Brian Heath (Nottingham AS), Nick James, Gordon MacLeod, Bob Mizon, Alex
Pratt, George Spalding and David Swain.

More observations of the Draconid outburst, using photographic, visual, and
radio techniques, from individuals and groups in the UK and overseas, are
urgently required to build up a full picture of the shower's rapidly
changing activity.  Even if you have only glimpsed a few meteors during a
short-lived break in the clouds, the Section would like to receive your
report. Simple counts of meteors seen within given time periods will also be
welcome. It is intended that a summary of all the observations received,
crediting all of the individual observers and society groups, will be
published in the BAA Journal as soon as all observations have been received
and the analysis completed.

There must be many observers - including many non BAA members - who
witnessed the peak of the shower, and we would like to encourage all these
people to submit their observations to the Section, either via email to:
meteor@britastro.org

or by post to:

Draconid Meteor Project 2011
British Astronomical Association
Burlington House
Piccadilly
London W1J 0DU


This e-bulletin issued by:
John W. Mason, Director, BAA Meteor Section
2011 October 11
============================================================
BAA-ebulletin mailing list visit:
http://lists.britastro.org/mailman/listinfo/baa-ebulletin
(c) 2011 British Astronomical Association    http://www.britastro.org/
============================================================

--
Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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)
--
Information -- More Info -- And More Info

Tuesday 11 October 2011

[BAA-ebulletin 00618] 2011 Deep Sky Section Newsletter on BAA Web Site

============================================================
BAA electronic bulletin
============================================================
The latest Deep Sky Section Newsletter (2011 September) is now on the Members' Only section of the BAA web site:

A few people have told me they have had problems navigating to this area of the web site.  So, if this applies to you, please follow the instructions below:

1)  Go to BAA web site
2)  Login (top RHS of screen) - enter username and password
3)  Go to Members
4)  Then to Downloads
5)  Scroll down to Sections
6)  Then scroll to Deep Sky Section

And there you will find it, along with previous Newsletters.

Stewart Moore
Deep Sky Section Director

============================================================
BAA-ebulletin:
visit:
http://lists.britastro.org/mailman/listinfo/baa-ebulletin
(c) 2011 British Astronomical Association    http://www.britastro.org/
============================================================

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Good Clear Skies
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Astrocomet
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Colin James Watling
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Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
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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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Information -- More Info -- And More Info

Wednesday 5 October 2011

Sputnik 1

Sputnik 1
Mon, 03 Oct 2011 23:00:00 -0500

On Oct. 4, 1957, Sputnik 1 successfully launched and entered Earth's orbit. Thus, began the space age. The successful launch shocked the world, giving the former Soviet Union the distinction of putting the first human-made object into space. The word 'Sputnik' originally meant 'fellow traveler,' but has become synonymous with 'satellite' in modern Russian. This historic image shows a technician putting the finishing touches on Sputnik 1, humanity's first artificial satellite. The pressurized sphere made of aluminum alloy had five primary scientific objectives: Test the method of placing an artificial satellite into Earth orbit; provide information on the density of the atmosphere by calculating its lifetime in orbit; test radio and optical methods of orbital tracking; determine the effects of radio wave propagation though the atmosphere; and, check principles of pressurization used on the satellites. Image Credit: NASA/Asif A. Siddiqi


 


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Good Clear Skies
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Astrocomet
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Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

 

October...

What's Up for October? Moons and meteor showers.
 
Hello and welcome. I'm Jane Houston Jones at NASA's Jet Propulsion Laboratory in Pasadena, California.
 
How many moons can you see this month?
 
Our moon is easy to see, but the others will take a little magnification. Jupiter's four Galilean moons can be spotted with a pair of steady binoculars but really shine through a telescope.
 
You might be able to see the different sizes of the four moons like what Galileo saw and sketched over 400 years ago.
 
And this is a great month to view Jupiter. It reaches opposition on October 28 when the king of the planets is closest to Earth in its orbit around the sun and best-placed for viewing.
 
If you haven't seen Jupiter through a telescope, join your nearest amateur astronomy club or observatory on their monthly public nights and have a look!
 
Last fall Jupiter's south equatorial belt dramatically disappeared.
 
This year the clouds that obscured it are gone, and the familiar reddish belt and the famous Great Red Spot are prominent once again.
 
What other planetary moons are on display? Both Neptune and Uranus are low in the southern sky this month, just after sunset. You'll need a big and powerful telescope to spot their moons, though.
 
It might be easier to look at photos of these moons taken by astrophotographers or sketches of objects seen through the eyepiece of a telescope.
 
Mark Oct. 8 on your calendars. That special night is both International Observe the Moon night and the peak of the Draconid meteor shower.
 
Unfortunately, you can't have your cake -- or your green cheese -- and eat it, too.
 
Moonlight interferes with both the Draconids on the 8th and the Orionids later in the month.
 
Europe gets the best view of the Draconids.
 
But maybe you'll see a few Orionids closer to the end of the month. They peak on the 21st.
 
You can read about moons of the solar system at http://solarsystem.nasa.gov/yss for Year of the Solar System.
 
And you can learn about all of NASA's missions at www.nasa.gov.
 
That's all for this month. I'm Jane Houston Jones.
 

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Good Clear Skies
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Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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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Information -- More Info -- And More Info

 

Monday 3 October 2011

View of Mission Operations Control Room During the Apollo 13 Mission

View of Mission Operations Control Room During the Apollo 13 Mission


View of Mission Operations Control Room During the Apollo 13 Mission
Thu, 29 Sep 2011 23:00:00 -0500

Gene Kranz (foreground, back to camera), an Apollo 13 Flight Director, watches Apollo 13 astronaut and lunar module pilot Fred Haise onscreen in the Mission Operations Control Room, during the mission's fourth television transmission on the evening of April 13, 1970. Shortly after the transmission, an explosion occurred that ended any hope of a lunar landing and jeopardized the lives of the crew. Image Credit: NASA



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--

Good Clear Skies
--
Astrocomet
--
Colin James Watling
--
Various Voluntary work-Litter Picking for Parish Council (Daytime) and also a friend of Kessingland Beach (Watchman)
--
--
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)
--
Information -- More Info -- And More Info