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Moon Atlas in 20 Maps

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appreciation if you do. Author - John
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The Moon in the News
2009
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NEWS ARCHIVE

Moon Atlas
The Moon Atlas has been sent to interested parties around the
world: Australia, Belgium, Canada, Denmark, France, Germany,
Greece, Hawaii, Hong Kong, Iceland, Ireland, Isle of Man, Italy,
Netherlands, New Zealand, Poland, Portugal, South Africa, Spain,
Sweden, Switzerland, UK, United Arab Emirates and the USA.
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29 June 2009: Three space exploration
experts - Paul Spudis, Dennis Wingo and Gordon Woodcock - have
written a long missive on reasons for returning to the Moon over
Mars. The missive tackles nearly all the current problems facing
NASA's 'Vision For Space Exploration', and re-crafts suggestions
into it that will hopefully gain acceptance with the public as well
as those in the US Congress. Several areas of interest are covered
that include: (1) Construction and maintenance of a spaceport on the
lunar surface; (2) Using the moon's natural resources - minerals,
metals and potential water deposits - as means for energy and
survival requirements in human settlement there; (3) How these
resources may aid as cheaper options in getting to the Moon from
Earth in the future - using the existing infrastructure to create
reusable rockets, that in turn leads to a lesser need for heavy-lift
ones for launching large ground-integrated systems from Earth to the
Moon. (4) And how all this will lead to a cheaper but more efficient
way in the long run, which when set up finally will then be used for
further exploration of other planets, like Mars, and beyond. There's
a lot more in the missive that can't be written here, however, if
you'd like to read more, then please go
HERE. If you
need to contact me about this article, then please do
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24 June 2009: Astronaut, Buzz Adrin,
who walked on the Moon some forty years ago during the Apollo 11
mission, is suggesting some major changes in the current NASA
structure. First off, Buzz suggests scraping the current Ares I
rocket - currently having serious design problems - and instead
stretch out the six remaining shuttle flights to 2015 - one per
year. In place of the Ares I he suggests to use a more reliable
rocket like the Delta IV Heavy or the Atlas V satellite launchers
that would be upgraded to Orion status for getting man back
to the Moon. Second off, stop the current space race that has
developed (directly or indirectly) between China and America. A
go-it-alone path to the Moon isn't the way to go according to Buzz,
so
with US participating, let international partners like China,
Europe, Russia, India and Japan get involved more together in terms
of planning, technical development and funding. Third-off, if
the Moon doesn't turn out to be commercially viable with
potential resources of minerals deposits, Helium-3...etc., then
"kill the program", he suggests, and "aim higher than a place we've
already set foot on six times".
There's a
whole lot more to his plans for future and further exploration to
the Moon and beyond, so do check out his Popular Mechanics article
appearing online
here. By the way, Buzz isn't a man to be messed with, as he
seems to be a guy that has a
good punch
(YouTube vid). Image of Buzz above - Credit Platon. If you
need to contact me about this article, then please do
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23 June 2009: After initial launch on
the 18 June 2009 (see below), NASA's
Lunar Reconnaissance Orbiter (LRO) mission today entered orbit around the Moon.
Over the next few days further adjustments with rocket firings will eventually
put the craft into a commissioning-phase orbit - a 60-day-long
period used for calibrations and tests of instruments onboard. After
this period, it will then be manoeuvred into its final orbit around
the Moon bringing it's altitude close to some 50 kilometres above
the surface in preparation for its mapping objectives. Meanwhile,
the Lunar CRater Observation and Sensing Satellite (LCROSS) which
separated from LRO two hours after launch made its first swingby of
the Moon that brought it as close as 3200 kilometres from the
surface. This gravity-assist swingby puts LCROSS into its cruise
Lunar Gravity Assist Lunar Return Orbit (LGALRO), where sometime in
October 2009 it will then line up for two impacts onto the lunar
surface.
For more on orbital events see
here, and an introductory YouTube video
here (Part
1 is very good, Part 2 okay). If you
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23 June 2009: To mark the fortieth
anniversary of the first Lunar landing of Apollo 11 on the 20 July
1969, the science publication,
NATURE, have launched a free on-line special issue. Rather than
talk about it more, why not have a look for yourself - just
start
here. If you
need to contact me about this article, then please do
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18 June 2009: NASA's Lunar
Reconnaissance Orbiter (LRO) along with its companion spacecraft,
Lunar CRater Observation and Sensing Satellite (LCROSS),
successfully launched today from the
Kennedy Space Center in Cape Canaveral, Florida. The dual-based
mission is America's return to the Moon in forty years, which next
month marks the historic Apollo 11 mission that landed two men on
the lunar surface on 20 July 1969. LRO/LCROSS has a suite of
instruments onboard - each with several different objectives in mind.
For example: LOLA (Lunar Orbiter Laser Altimeter) will determine the
global topography of the Moon - investigating landing site slopes, surface
roughness, and possible polar surface ice in shadowed regions;
LROC
(Lunar Reconnaissance Orbiter Camera) will acquire targeted narrow
angle images of the surface, and resolve meter-scale features to
support future landing site selections (several cameras on the
mission will return unprecedented images of the lunar surface -
accurately mapping the Moon globally through high resolution imaging
down to 0.5 m per pixel and low resolution made at 100 m per pixel -
see LRO/LCROSS target sites
here); LEND (Lunar Exploration Neutron Detector)
will provide global mapping of hydrogen content on the lunar surface
(the IBEX mission recently
observed the stream of neutral hydrogen atoms caused by the solar
wind scattering off the moon's surface), as well as characterise
neutron components of the lunar radiation environment; DLRE or DIVINER (Diviner Lunar Radiometer
Experiment) will measure lunar surface temperature
profiles for habitability, map variants in
silicate mineralogy and chart the temperature of the entire lunar
surface to identify cold traps and potential ice deposits; LAMP
(Lyman-Alpha Mapping Project) will map the entire lunar surface in the far ultraviolet,
providing images of permanently shadowed regions illuminated only by
starlight (it will also search for surface ice and
frost in the polar regions); and CRaTER (Cosmic Ray Telescope for the
Effects of Radiation) will investigate the effects of galactic
cosmic rays and solar energetic particles on tissue-equivalent
plastics (measurements will characterize the deep space
radiation environment and provide a baseline to the amount of
radiation humans could be exposed to). One of the main highlights
in the mission will be to crash two probes onto the surface in
search of water deposits. These probes basically consist the makeup
of LCROSS itself -
the first being an upper stage rocket, called Centaur, and the
second a Shepherding Spacecraft, called the S-S/C. As both approach the moon's South Pole region, Centaur
will first decouple from the S-S/C for line-up of impact into a crater
(possibly, Shackleton), and then the S-S/C will
fly through the plume of disturbed material for analyses in
any signs of water and other compounds released. Approximately
fifteen minutes later the S-S/C itself will then line up for impact
also into another nearby crater (possibly, Cabaeus, Faustini or
Shoemaker) - releasing a second plume of material 2 million tonnes in
quantity. Telescopes on Earth - both professional and amateur - will try to observe the events, but the LRO
orbiting overhead and possibly other orbiting space telescopes like
Hubble will
have the best views. A
new topographic map released today by JPL revealing areas unseen
at the South Pole region may aid in the target water-points that LCROSS may strike. Such water-ice resources will
prove extremely important in the development of a lunar base. Colonists will need water to grow food, produce
rocket fuel (from the hydrogen in H2O), and build up oxygen reserves
for breathing. Two previous missions,
Clementine and
Lunar Prospector,
detected water ice signatures back in the 1990s but analyses of the
data has been a controversial issue since then. The Lunar Reconnaissance Orbiter is the
first of many robotic missions NASA will use to study the Moon
under its “Vision for Space Exploration”.
Costing approximately $616m (2007 quote) in total for both LRO and LCROSS,
the mission is expected to last up to 14 months initially, however,
depending on the condition of the spacecraft and finances available,
its lifetime could be extended up to four years. If you
need to contact me about this article, then please do
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10 June 2009: Just about everyone on
the planet now knows that the Japanese spacecraft,
Kaguya (Selene),
launched two years ago to the Moon has crashed on the lunar
surface. The impact is reported to have occurred at 3.25 am JST
(Japan Standard Time -11 June) in
an area of the Moon's south-east (rough coordinates given are 80.4E, 65.5S). Some
observations of a flash are being reported, but these have as yet to be
confirmed. For more information see Chuck Wood's 'Kaguya Special'
here. If you
need to contact me about this article, then please do
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10 June 2009:
LOIRP (Lunar Orbiter Image
Recovery Project) in their quest to recover Lunar Orbiter images
taken during missions from 1966 to 1967 have released another series
of images. The first includes a
Lunar
Orbiter III oblique view of
Oceanus Procellarum - a huge mare region on the eastern side of the
Moon, the second relates to the
impact site of the
Ranger 8
spacecraft which struck the Moon on the 20 February 1965 in
Tranquillitatis - another mare region on the western side of the
Moon, and the third relates to the
landing site of Apollo 14. On June 15 2009, LOIRP also released
images of the
Apollo 12/Surveyor III landing site, and on the 14 June 2009 an
image of the
South Pole region was released. For an update on future images,
see Moon Views. The images are just some of those taken
amongst the ~1000 pairs of medium
(MR) and high resolution (HR) images produced during the Lunar
Orbiter Program. Back then, they were produced with two types of
70-mm black and white cameras onboard each orbiter - the MR camera
having a short focal length with a wide field of view, while the HR
camera had a long focal length with a narrow field of view. All
processing of the images were done onboard the crafts, that is,
negatives were developed, then scanned and transmitted to
photographic and magnetic tape recorders back on Earth through the
Deep Space Network operated by JPL (Jet Propulsion Laboratory). The
images were then transferred onto 35-mm film in the lab and turned
into film segments, called a framelet (about 60cm long), and from
these a full reconstruction of a single frame of each image was
produced. Some of the images taken were extremely difficult to see
any clear detail as scanning in between framelets produced a bright
line to run across each subframe. As a result, this produced images
with brightness variations and streaking defects. These defects,
however, were somewhat cleared up later as photographic techniques
developed in the intervening years, however, today more modern
techniques are tackling the problem. LOIRP is based at NASA's Ames
Research Centre, and is undertaking the task of translating original
Lunar Orbiter analog data from 1,500 tapes into digitalised format.
For more information see here. If you
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9 June 2009: Tomorrow is a big day for
Japan because that's the day when their current orbiting spacecraft,
Kaguya (SELENE), launched two years ago will end its life with a
bang. The crash is intentional, and will occur in a dark region on
the Moon northeast of Gill crater situated on its south-eastern edge as viewed by an observer on Earth. Official news
from the Japan Space Agency, JAXA, says impact will occur around
18.30 UT at coordinates 63S, 80E, however, this could change as the
orbiter gets closer and closer to the surface. Factors like gravity
anomalies (or gravity disturbances) produced from a difference in
rock density underneath the moon's surface could cause Kaguya
to veer slightly from its intended impact site, or, an unexpected
mountain peak could end the mission sooner than expected. Observers
situated more easterly and southerly from India to Japan (Australia,
New Zealand...etc.,) are the only ones who will have the opportunity
to record any plume of material ejected from the surface. Amateurs
with good-sized telescopes should be able to see the event if all
goes according to plan - giving them some kind of advantage over the
professional telescopes. Who will be the first to get in a good
shot? Could it be YOU? If you
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4 June 2009: The USA's House
Appropriations Subcommittee on Commerce, Justice, Science & Related
Agencies will see NASA's exploration budget in FY 2010 reduce by as
mush as $212.3 million. In FY 2009, NASA's exploration budget came in at
$3505.3 million, but for next year that now is going to be $3293.2
million. Congressman and Chairman of the Subcommittee, Alan
Mollohan, said: "It is a pause, a time-out, to allow the
President to establish his vision for human space exploration and to
commit to realistic future funding levels to realize this vision."
If the above budget cuts, and
potential future budget cuts, is anything to go by, the whole lunar
program could suffer a delay setback. Already, a blue ribbon panel
appointed some weeks ago is currently reviewing the vision for human
spaceflight, and the recommendations on this, when reported, could
have serious constraints for returning Man to the Moon by 2020. Is
this 'pause' and 'time out' a no-confidence vote in NASA's
exploration path, or is it really a vote in defining the role the
agency should go in the future? NASA has created
a
Web site
for the Review of U.S. Human Space Flight Plans Committee as a way
of inviting the public to submit their views, so YOU decide! See more on Mollohan's
statement
here
and on NASA's FY 2010 budget summary
here. If you
need to contact me about this article, then please do
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1 June 2009: As the NASA Lunar
Reconnaissance Orbiter (LRO)
prepares for launch within the next few weeks, India's Chandrayaan 1
lunar spacecraft currently orbiting the Moon may work alongside with
it in a near future research collaboration. The research will
involve the two orbiters looking for signs of water-ice
signatures at both poles of the Moon. It has long been suggested
that such deposits may lie closely under the surface at the pole
positions where portions of some craters remain forever in darkness.
Three instruments onboard LRO are capable of looking for water-ice signatures,
while on Chandrayaan 1 there already is a NASA-built instrument
called the Miniature Synthetic Aperture Radar (MSAR).
Each instrument can look at different aspects of
possible signatures at the pole regions, and all data will then be
collected and shared collaboratively. Two previous missions,
Clementine and
Lunar Prospector,
detected water ice signatures back in the 1990s but analyses of the
data have been a controversial issue since then. Talks between the
two space agencies are now undergoing, and expectation of the collaborative announcement
is due out soon. If you
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21 May 2009: The Japan Aerospace
Exploration Agency (JAXA)
has announced the expected date and impact point of the Kaguya
spacecraft currently orbiting the Moon. The date is 10 June 2009,
and the impact point will be on the nearside of the Moon close to a
south-eastern crater called Gill (Lat 63.9S, Long 75.9E). The Moon
will be some 16 to 18 days old at time of impact, showing a waning
gibbous Moon (looking up at the Moon in the sky one would see a
nearly full-ish Moon but a sliver of it's right-hand side would be
in darkness). At time of expected impact, Gill will lie in this dark
sliver region, so when impact occurs good-sized amateur and
professional telescopes observing the event may have opportunity to
observe a plume of lunar dust ejected off the surface. The time of
impact is given as 18:30 GMT, so observers at mid latitudes in
Eastern countries from India to Japan should be suitably placed to
take any recordings (unfortunately observers situated in the USA or
Europe will not see the event as daylight will interfere). Countries
such as Dubai to Karachi will see the Moon low on the horizon, while
others like Bangalore to Lhasa to Tokyo and Hong Kong will have the
best views. Of course, the date, time and location of impact is
subject to change over the coming weeks, so please do check into the
JAXA website for updates. If you
need to contact me about this article, then please do
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18 May 2009: Remember back in the 60s
and 70s when Moon rocks were all the rage - for geologists anyway,
well, they are about to be highlighted again because this time they
heading back into space. Not actual space, but the furthest reaches
of terrestrial space - this time to Chomolungma, or Mount
Everest to you and me. Climber,
Scott Parazynski, who
secured the samples from NASA several months ago and currently
attempting his first summit on Everest, is carrying 0.052 grams of
the rocks encapsulated within a clear acrylic "button". The samples
were initially collected by Neil Armstrong in July 1969 during the
Apollo 11 mission which landed on a lava mare known as the Sea of
tranquility. The samples came from some several metres away from the
main Lunar Module "Eagle", and Parazynski hopes to get them to the
top of Everest in time to celebrate and honour the upcoming 40th
Anniversary of the historic landing on the Moon. Parazynski himself
is a former astronaut who flew five times on the space shuttle and performed
seven spacewalks while helping out at the International Space
Station. He retired from the astronaut corps back in March and ever
since he set out on the Everest trip, his activities have been
reported and monitored using a special
SPOT device. The device enables Internet users to track his steps in real time. Two other
members in his team - Keith Cowing (located at Everest Base Camp),
and Miles O'Brien (located in New York City) - are all members of
the Board of Directors of the
Challenger Center - established by family members of the crew of
STS-51L shortly after the shuttle accident in 1986.
The centers were created
by the directors as an immersive, stimulating learning environment
for middle school students who role play simulated space missions.
This is
certainly one to watch as Parazynski makes his final attempt, so if
you'd like to follow his progress do check on him
HERE. UPDATE: Parazynski
successfully reached the summit of Mount Everest on 20 May 2009 at
3.55 am local time - a big congratulations to him. If you
need to contact me about this article, then please do
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15 May 2009: NASA has just announced
that launch of the LRO/LCROSS
mission to the Moon planned for 2 June will now launch within a
four-window close on 17 June. The delay isn't sue to any
un-necessary problems that have arisen but simply down to engineers
wanting to carry out final analysis between the Atlas 5 rocket's
upper stage and the impactor spacecraft payload. The extra time
allocated will also give the engineers a look into
potential thrust disturbances on the LCROSS impactor associated with
fill and drain valves on the rocket's Centaur upper stage. If you
need to contact me about this article, then please do
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14 May 2009: Both the European Space
Agency (ESA) and Alenia Space Italy
(TAS-I) have commissioned GMV to
build a prototype, all-terrain rover for use on the Moon and Mars.
Called the EGP (Eurobot Ground Prototype), the rover will be
capable of carrying upto 400 kg payloads at a time,
tackle obstacles 20cm high, and climb up slopes with angles
approaching 15 degrees. As it roves about on the lunar or martian
surface using rear-wheel steering with 120 degrees turning, the
rover can be controlled by instructions from Earth, or by voice
command of an astronaut working alongside. A
stereoscopic camera mounted on the rover will allow for 360-degree
imaging of the surface; building up successive digital maps of the
terrain it has covered over a period of time. The main task of the
rover, however, will be to assist astronauts in the
moving of equipment from location to location, and aid in the
construction of future bases planned for the Moon and Mars. If you
need to contact me about this article, then please do
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13 May 2009: The Lunar Reconnaissance
Orbiter (LRO), along with with
its companion Lunar
Crater Observation and Sensing Satellite (LCROSS), are both due for
launch in early June. As a precursor in build-up to the launch, NASA is putting the
integrated crafts on view this Friday for the
media to photograph at the Astrotech Space Operations facility in
Titusville, Fla. There will be an opportunity to interview
project and launch program officials at the facility, so if you are
interested in covering the event, participants should proceed
directly to Astrotech located in the Spaceport Florida Industrial
Park, 1515 Chaffee Drive, Titusville. The gates will open at around
7.00 am - photo-ID is
required and foreign journalists attending should have a
media accreditation badge - available from the Kennedy Space Center). If you
need to contact me about this article, then please do
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27 April 2009: Russia's next step onto
the international lunar stage is a mission known as
Luna Glob. The
spacecraft's objectives initially had three main objectives,
firstly, set a lander down near the South Pole Aitkin Basin
region to search for signs of water ice deposits, secondly and
thirdly, impact two slow-descending penetrator/landers in regions
near where Apollo's 11 and 12 spacecrafts landed in 1969, and 10 fast-descending
penetrators somewhere near Mare Fecunditatis (Sea of Fertility) to
collect data about surface seismic moonquakes. Launch of the mission
was all set for 2012, however, as budget constraints and recent
suggestions of changes to the spacecraft will come under intense
scrutiny by the Russian government this coming May and June, is Luna
Glob set for a delay? The changes mainly concern the penetrators, as
it now looks like only eight in total will be used. The first four
would initially be set for impact at the above Apollo sites,
however, as there are two additional penetrators in this
configuration, the objective may also take into account the Apollo
14 landing site at Fra Mauro. The lander would afterwards be
deployed to set down somewhere near the South Pole, but as to where
the other four remaining penetrators will impact eventually, the
above-mentioned Fecunditatis region may be changed. Russian
scientists involved with the mission say more than likely that the
2012 launch date will still go ahead despite the changes, however,
space experts in the Russian media keeping an eye on the whole
procedures suggest the new configurations will inevitably cause a
delay. If the delay goes ahead, it may also affect other planned
lunar missions that Russia has agreed to with other countries like
India who together planned a cooperative lunar rover mission planned
for 2012-13 launch, as well as the future Lunar Robotic Network it
talked about last year with the U.S., the European Space Agency and
several other countries. One to watch over the coming months. If you
need to contact me about this article, then please do
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22 April 2009: If you've ever wanted to
know where a particular feature on the nearside surface of the Moon
is, or instant information about it, then this 20-Maps's atlas might
be for you. Nearly 3000 features -- from craters to mountains,
rilles to domes, lacus to maria, and a whole lot more -- are
indexed. The end product has been professionally printed on very
high-quality paper, is wire-bound (recommended), and is available in
three viewable formats: natural, inverted-mirror and mirror --
suitable for nearly all telescopes. I have worked on this for a long
time, so if it's of interest please do have a
peek. Who knows, it might be just what you're looking for?
Thanks...John (author of this website).
Top
20 April 2009: Two new papers accepted by
Science publication, Geophysical Research Letters (GRL), will
soon hit the headlines. The first paper looks at
"Assessing Access of Galactic Cosmic Rays at Moon's Orbit",
while the second paper looks at "Direct active
measurements of movements of lunar dust: Rocket exhausts and
natural effects contaminating and cleansing Apollo hardware on
the Moon in 1969". (1) Cosmic rays, which
are considered harmful radiation for us humans, are generated
both from within our own solar system for example, by exploding
stars, or from outside our own solar system by
high-speed jets near black holes.
Made up of high-energy particles, billions strike earth each day, however, most are
deflected by our magnetic field and so we remain relatively
protected. However, as the Moon doesn't have a magnetic field to
speak of, the rays which strike the surface head on may present
a serious problem for future astronauts and colonists. As
concentration of these rays may vary throughout at distances
roughly in the region of the moon's orbit , the first paper will
be of utmost interest to understanding their potential risks.
(2) One of the most frustrating facets of lunar exploration for
astronauts during the Apollo programs was lunar dust. It
stuck to everything - to the astronauts' suits, clogged up their
sensitive sensors and electronics, and even got into their eyes
and lungs. Each dust particle is just a few microns wide and
very abrasive, and as there is no weathering process on the Moon
to wear each down, their potential to affect future lunar
missions and astronauts remains at very high risk. Detectors
onboard the then Apollo 11, 12 and 14 landers supplied data
about the dust, and these were beamed back to Earth and stored
on magnetic tapes. However, during the intervening years the
tapes subsequently became "misplaced" by NASA afterwards, and so
all the information about lunar dust seemed lost forever. But, a
new light has shone above the horizon. It now seems that the
tapes have been around all along, and were in a room in Perth,
Australia, for the last 40 years or so. Upto 173 tapes at the
time were recorded, and only recently have they been looked at
to see if the information enclosed can be retrieved. In the
second paper above, 75-year-old physicist, Brian O'Brien, who
had access to the tapes presents his findings. Self- funded, and
working for two years alone, O'Brien has come up with some
new data about the electrostatic problems with lunar dust, as
well as some practical solutions as to future avoidance. Access
to both papers, unfortunately, are through subscription only to
GRL. If you need to contact me
about this article, then please do
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11 April 2009: Origin of the Moon is currently theorised to be
the violent result of a giant asteroid, called 'Theia', that
impacted the early-forming Earth. Debris created from the impact
-- both of Earth and asteroid material -- coalesced together
eventually to give us the Moon we have today. Theia may have been just
one of billions of stray asteroids roaming around the early
solar system, and may have come from any direction in space. However, two observatories (Stereo
A and Stereo B) currently studying the Sun may throw light
on the subject as to where it originally came from. Each observatory
-- one ahead of Earth in its orbit, the other trailing behind --
are about to pass through points in space, known as Lagrangian
Points. Gravitational forces and orbital motions of objects
at these points usually balance out with each other, and so
many remain there relatively undisturbed for billions of years.
However, some objects are disturbed by external forces from the gravitational influence
of planets, and this can send
them hurdling outwards. Is this what happened with Theia when
planets Venus or Jupiter were forming? Did their influence exert
forces on it which sent the
asteroid spiralling towards Earth? There are five Lagrange Points between
the Earth-Moon system -- three are quasi-stable (that is, simple
nudging of an object here could send it out of the points known
as L1, L2 and L3), while the other two points, L4 and L5, are
more stable (a nudged object here could still remain within the
points). Stereo will pass through the latter two for several
months -- Stereo A making its closest approach this September of
L4, and Stereo B of L5 in October. The two together will look
for asteroids that have similar composition of the Earth and the
Moon, and if found, it could give substantial evidence to the impact theory between the Theia
and Earth. As a lot of data is likely to be produced
during the several months, the team of scientists involved with
Stereo are asking the public to get involved. For more on this,
see
here. If you need to contact me
about this article, then please do
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8 April 2009: Coming in at approximately 2500 km in diameter and
lying mostly hidden on the farside of the Moon (a portion can be
seen at the lunar south pole), the South Pole Aitken (SPA) basin
is the oldest documented 'crater' on the lunar surface. For such
a big-sized crater, one would naturally think the object that
produced the initial basin struck the crust first, and then dug
deep down into the moon's upper mantle -- allowing most of this
type of material to entirely fill the basin afterwards. However,
when one analyses the basin floor, roughly, half is made up of
mantle material, and the other half of lower crustal material
totally different to normal highland crustal rocks. So what is
going on? Why isn't there more mantle material than lower
crustal material inside the SPA? Does it have something to do
with the dynamics of the initial impact (e.g. was it a
high-velocity or low oblique low-velocity impact), does it have something to
do with alteration of the target rock by the impactor (e.g. high
concentrations of iron and magnesium-rich rocks in the SPA could
be produced by the huge temperatures involved), or is it that
volcanism is the cause (e.g. evidence of Potassium K, Rare Earth
Elements REE and Phosphorous P inside the SPA suggest a KREEP-type
volcanism event). In the April edition of
Nature Geoscience, Dr Paul Spudis of the
Lunar Planetary Institute
looks to going "Back
to the Moon" and poses some questions about the SPA. The
article is free, so do check it out. If you need to contact me
about this article, then please do
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1 April 2009: "This is an extraordinary discovery!" So says Dr. April
Foley of Lirpaloof Observatory in Farlipool who
discovered the crater yesterday in a region of the Moon known as Palus Epidemiarum. Foley, who has been observing the
lunar surface over the last two years for rare events known as TLPs
(Trans Lunar Phenomena), came across the new crater by mistake. "I
have been studying this particular region for awhile now and had taken several photographs, however,
when I was browsing through the images for the TLP signatures, I
noticed that
one
image looked unusually different. I
immediately thought that I had caught a TLP (a bright flash
believed to be produced by gas), however, on closer examination
I could see it was a small crater." The surface of the Moon is
hit every day by minute specs of interstellar dust that are too
small to produce anything of note, but occasionally when small
stray asteroids get through, the result of the impact produces a
crater that can be seen from Earth-based telescopes. Judging by
the direction of the ejecta driven off by the initial impact, it
looks like the strike came in from a north-westerly direction.
This is obvious in the image as lighter material underneath has
been flung outwards in a direction away from the impact, which is thought to have been low and highly oblique.
"Currently, there are two lunar space probes orbiting the Moon
and another is set to launch this June", says Foley. "I do hope
that they'll be able to take a closer look as events like this
are somewhat rare." If you need to contact me about this article, then please do
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26 March 2009: As part of the International Year of Astronomy
the Society for Popular Astronomy (SPA)
in the UK are organising a week long Moonwatch from Saturday 28
March to 5 April 2009. Observatories, science centres and
astronomical societies from around the country will open up
their resources to the public; the goal of which is to get as
many people as possible view the Moon through a telescope. SPA
chose the above period to run the event because as the
Moon will remain high above the horizon for UK viewers it will
allow for longer and clearer observations to be
made. This is just one of three Moonwatchs that SPA will run
during the year -- the other two occurring from 24 Oct to 1 Nov
(Autumn Moonwatch) and
19 Nov to 29 Nov (Schools Moonwatch) respectively. If you need to contact me about this article, then please do
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23 March 2009: Over the next five days international scientists
from around the world will meet in Texas USA to discuss the many
different aspects of science and research in planetary science.
Covering the latest research and results over a diverse range of
areas -- from petrology to geochemistry to geophysics -- the
Lunar & Planetary Science Conference (LPSC) represents
one of the main events in this Year of Astronomy for the lunar and planetary science community.
Representatives from the US Government, academia and private
industry will also attend, and the whole event is an opportunity
for publishers, educational institutions and scientific societies
to show off their there wares. For the lunar community
attending, the discussions and presentations cover a broad
spectrum of interests. On Monday, 23 March, upto thirteen
scientists working in separate areas of research will each
present the latest news and results under the heading "Origin
and Evolution of the Early Moon" (see all thirteen PDF abstracts
here). On Tuesday, results from missions like Kaguya,
Chang'e 1 and Chandrayaan 1 will be discussed (Part
1 and
Part 2), while on the following day participants can get to
hear about impact of the
South Pole Aitken (SPA) basin -- one of the largest impact
basins in the Solar System. On Thursday, 26 March, the
Diversity of Lunar Lithologies will be be discussed, and there's also a poster
session in the town centre exhibit area on
Meteoritic Samples of the Moon. Finishing off the conference
on the 27 March will be a session on
Planning for Future Exploration of the Moon where scientists
will present the latest developments in several areas of
interest, for example, there's a
Progress Report on the Lunar Exploration Roadmap, a
Seismic Exploration of the Moon, and a sesssion that will
cover the latest scientific opportunities
for
Human Exploration of the Schrodinger Basin . Note, all the
above-mentioned areas of research and results are just a tiny
sample of lunar-related science that will be looked at over the
next few days, however, if you want to see more of what's on --
see here -- the full program. If you need to contact me about this article, then please do
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17 March 2009: The ten space agencies from around the world that
met in Japan last week have
adopted for further study three scenarios for conducting
internationally coordinated robotic and human exploration
activities on the Moon. The three scenarios include: (1) short
duration missions and (2) extended stay missions -- both of
which will be able to go to any
location on the Moon, and (3) longer duration missions for up to six
months at polar sites like the North Pole or most favourably the
South Pole where the first lunar base may start construction by
2020. Development and
placement of infrastructure systems in space and on the surface
of the Moon are also included, and the space agencies also agreed on
increased cooperation between all with emphasis on the
exploration of locations in the Solar System where humans may
someday live and work in the spirit of the Global Exploration
Strategy (GES)2.
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15 March 2009: While most of us on St Patrick's Day will be
celebrating all that is Irish around our world, a team of
international experts will be discussing what it means for us as
we look towards two other worlds
-- the Moon and Mars. Hosted by
the National Institute of Aerospace and NASA's Langley Research Center's
Systems Analysis and Concepts Directorate, four scientists will
be given a platform to talk about the Visions for Space
Exploration set up by the George Bush administration a few years
ago. They will debate and ask
whether it is a good idea to go back to the Moon and then onto
Mars, and why we as humans need and want to explore. Questions like:
Is it necessary to send humans to the Moon prior to Mars?
Why? Why not? Are human Mars missions too risky and costly to
be considered in the near future? Could humans be sent to
explore other destinations in the solar system? What unique
advantages do humans provide over purely robotic missions? Why
are the Moon and Mars of scientific interest? These and other
questions will undoubtedly put the four scientists -- Scott
Pace, director of the Space Policy Institute; Paul D. Spudis,
senior staff scientist at the Lunar and Planetary Institute in
Houston; G. Scott Hubbard, a Stanford University professor; and
Joel S. Levine, senior research scientist in the Science
Directorate at NASA Langley Research Center -- on the spot. The
event will begin at around 7pm at
the Virginia Air and Space Center in Hampton, Virginia, and audience
members are invited to submit questions in advance to Dr
Douglas Stanley of the
National Institute of Aerospace who will be moderating the
forum.
The Forum is just one in a series of distinguished
lectures that started in 2006, featuring
presentations by experts from academia, industry, and government on
the conception, design, engineering, analysis, and operation of
vehicles and systems towards exploration of our Solar System.
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3 March 2009: By now, everyone on the planet will have heard of
Second Life (SL) -- an online 3D digital world where players are
able to walk, fly, and teleport to thousands of 3D locations.
The game allows individuals to build up virtual businesses, own
real-estate properties for sale or rent, and create virtual
worlds limited only by the imagination. Now, a team of
scientists working at the Center
for Educational Technologies in West Virginia USA are going
to create a virtual piece of land - an island in the
SL sky -- that will simulate the surface of the Moon. Called
MoonWorld, the
virtual island will resemble an actual area of the Moon (a 34km-wide
crater called Timocharis) where players can explore the
surrounding lunarscape and environment. Future visitors will first
be
teleported into a lunar base at the island where they will be outfitted with a spacesuit,
which will allow them to go on a series of missions to investigate how the impact crater formed
and how identifying geologic features like scarps and melt can help their overall understanding. There'll also be volcanic features
like lava flow-fronts, domes and rilles (~ collapsed lava tubes)
to investigate, where the visitor can learn about each of their
morphologies as they walk and climb around inside them. While
the spacesuit will give players the experience of the reduced gravity
of the Moon (~ 1/6 that of Earth's), it will also be capable of accepting
numerous instrument packages from magnetometers to gravimeters
to interact with the environment. There'll even be a cool jetpack that
one can strap on for
flying around the whole Timocharis area -- letting the viewer
get a
better perspective of what they are actually investigating. The whole reason behind MoonWorld, however, is to give visitors a meaningful experience
of what it would be like to live and work on the Moon, and
provide an educational but fun environment in which to
learn about an extraordinary world. MoonWorld is expected to be
up and running sometime near the end of this Summer, with no
paid subscription to SL necessary. For more
about MoonWorld see
here (PDF file ~ 480kb), and for an image of the Timocharis
region see Chuck Wood's
Lunar Picture
of the Day website. The above title was taken from the song
written by English rock band, The Police. If you need to contact me about this article,
then please do
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2 March 2009: UNESCO has marked this International Year of
Astronomy by asking six international astronomers to write in
Physics World about the challenges ahead in
different areas of astronomy. Well-known lunar geologist and
author, Paul Spudis, from the Lunar Planetary Institute (LPI)
in Houston, has written an extensive article about his own
particular area of expertise on the future
exploration of the Moon, and what will happen over the next few
decades. Rather than give a brief synopsis of the contents Dr Spudis covers, I think a reading of the
full
article would be more suitable. If you need to contact me about this article,
then please do
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1 March 2009: China's Chang'e 1 mission that launched to the
Moon nearly two years ago has crashed on the Moon. The
spacecraft, which carried an array of scientific instruments
designed to take three-dimensional images of the lunar surface,
is said to have crashed somewhere in Mare
Faecunditatis (see image of crash site on Chuck Wood's
Lunar Photo
Of the Day). The craft hit the surface at approximately 16:13pm
Beijing time (08:13GMT)
today in an oblique angle, and was navigated down onto the
surface by remote control stations situated in China's Qingdao and northwest China's Kashi regions.
The craft marked the first
stage in the country's intentions to explore the Moon -- leaving
engineers prepare for the the next stage, Chang'e 2. This craft
is expected to be launched sometime in 2011/12 into an orbit of 100 km above
the moon's surface, later followed in 2013/14 by Chang'e 3
that may involve soft landings and inspection of the lunar surface. This
mission will be an exciting one as it may also include a rover
whose main objective will be to transmit video footage and
analyse soil samples in preparation for a sample return
mission, Chang'e 4, in 2017 (returned to Earth orbit
several months later). Chang'e 1
initially was designed to last a year in orbit around the Moon,
however, good conditions onboard allowed it survive for an
additional three months. In all, it transmitted upto 1.4
terabytes (1 terabyte = 1000 gigabytes) of data back to stations on Earth. No reports, as yet,
suggest that the craft's descent was videoed, however, only
computer graphics of the crash are being released. If you need to contact me about this article,
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27 February 2009: If you are someone that is interested
in producing a piece of art about the Moon, then why not enter the
latest competition organised by NASA. Under the theme: 'Life and Work on
the Moon', the agency is asking all full-time college students from around the world
to submit digitally-created images that reflect the harsh
environment of the Moon as they see it. Images can be of serious
realistic content, for instance, like depiction of a future colony as
astronauts work and live on the Moon, however, comical and surrealistic images
will also be accepted, too -- just once they come under the above
context and theme. And it doesn't only have to be of two-dimensional
images like sketches, drawings or paintings, because three-dimensional
representations like sculptures or models will also be eligible to
enter. All the agency requires is that you create an original piece of
art,
take a digital photograph (e.g. a jpeg image) of the work, and then submit
it online. If you're interested in entering the competition
and think you have a chance, then firstly see the contest rules
here, secondly,
see how to enter
here, and when you think you've got all the relevant details, go
here
to register. Deadline for the competition
has been extended to April 15, 2009. If you need to contact me about this article,
then please do
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20 February 2009: Another set of images taken during the
Lunar Orbiter missions NASA sent to the Moon
between 1966 and 1967 have been restored. This is the second set of
images NASA retrieved since it set up the restoration
project known as
LOIRP (Lunar Orbiter Image Recovery Project);
whose principle aim is to translate
original Lunar Orbiter analog data from 1500 tapes into digitised
format. Images of the moon's surface taken during the Lunar Orbiter
Program were produced and
processed onboard the orbiters back in the 60s, which were then scanned
and transmitted back to photographic and magnetic tape recorders on
Earth. Some of the images, however, were very bad -- resulting in
streaking and brightness variations in between individual framelets.
Modern-day photographic reconstruction techniques are now being used to
restore these bad images, and in a year's time are expected to be
available to the public. But it's not all modern equipment that the team
of scientists and engineers are using to restore the images, as they
found out that some of the tapes will only be accepted through machines
that were used back then. The images so far have not been recognised as
to the area taken, however, they are from LO I and LO II data (see
here a stitched image taken by LO I -- 102). For more news and
information about the project see also this
News story. If you need to contact me about this article,
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14 February 2009: The following interview took place in
celebration of the International Year of Astronomy 2009, and in
recognition of Galileo Galilei who first used the telescope 400 years
ago to observe the Universe and Moon. The interview also marks the
birthday of this extraordinary man...born in Pisa on the 15 February
1564.
INTERVIEW BEGINS
J:
First, thank you for taking the time in your busy schedule for this
interview.
Gal: Prego.
J:
This must be a momentous occasion for you -- tell me how you feel.
Gal: Well, I feel deeply touched and honoured to see so much
interest being generated in this International Year of Astronomy
which, I think, if I'm correct, marks the 400th anniversary of me
using my little telescope.
J:
Yes, you are correct! Could you tell us about how all that happened,
how you came about using the telescope, what you observed...etc?
Gal: Sì. Well, as you know, it was Dutch lens maker, Hans
Lippershey, who on the
25
September 1608
produced the first effective telescope. Lipp., had attempted to
patent the scope by means of the States-General in
The
Hague,
however, he was not successful, as you know, and this led to
(unashamed) duplication of the device by others at the time. News of
the instrument's magnification performance spread amongst the
various foreign delegations in
The
Hague
at the time, and as these were trying to negotiate a peace
settlement, fame of the telescope spread like wildfire throughout
Europe.
The secret was out, so one could attain a copy of the instrument in
Paris
by April in 1609, in
Milan
by May, and in various cities across
Italy
by July, and that's when I came across it.
J:
Your first view of the telescope then?
Gal: Sì..sì..it was a funny-looking thing and I wanted
to...!
J:
Sorry to interrupt you, but why do you say it was funny-looking?
Gal: Ah, mi scusi. It had this long type of tube and at each end
two pieces of curved glass was inserted. These, apparently, were
being used to make distant objects appear closer.
Well,
I was amused by the use of the curved glass as anyone knows that
such objects, for example, like curved mirrors produce great
distortion effects in any viewed images. So, if one piece of glass
produced distortion, then two in combination would not simply work.
That was my initial presumption, however, it was wrong, and, in
fact, I later discovered that the two pieces used effectively
in correct alignment and spacing could indeed produce some magnification of clarity.
J:
And so that's when you built your own telescope?
Gal: Sì! Initially, these Lipp., telescopes had just a
magnification of about two or three, however, I was able to grind
and polish my own lenses, and so in August of that year I had made a
telescope with 8 X magnification. Eccellento!
J:
Don't you mean...magnifique [smiling at Galileo]?
Gal: Haha...you Irish [shaking his finger at me]...sì sono cosi
affascinante (you are so charming). Anyway, I demonstrated this
telescope to the authorities in
Venice
who were simply amazed and, as a result, I received a big increase
in my Paduan salary, which led me to produce an even better
telescope of 20 X magnification by year's end.
J:
Wow!
Gal: Sì…but that's not all! Later in 1610, the Grand Duke of
Tuscany made me a life-time appointment in Florence as mathematician
and philosopher to him, however, upto this, I was able to experiment
around with the telescope -- making objectives with longer focal
lengths, include aperture stops between the lenses, and eventually
producing a telescope with 30 X magnification.
J:
Excellento!
Gal: Don't you mean...magnifique [we both laugh].
J:
So, what did you observe with this wonderful telescope?
Gal: Oh my God...where do I start? The stars in the sky…cosi
bella (so beautiful). I could see stars that weren't visible to the
naked eye, and I could resolve myriads of them in the Milky Way --
confirming the speculation reported by Aristotle two millennia
before. I saw how the planet Jupiter had stars that moved back and
forth on either side of it. These observations later led me to
believe that they
weren't actual stars at all, but were, in fact, little
moons circling
around the planet itself [small but nice video
here]. I could see also weird-looking appendages
around the planet Saturn that one day were there and later
had disappeared -- so puzzling to me. Looking at Venus I could
discern how it went through a complete sequence of phases appearing
with a full disc in one instant and then a crescent disc
afterwards...just like our Moon. I was so excited!
J:
Yes, I can imagine. What about our own Moon as you mention
it...did you look at that?
Gal: Oh sì...certamente! During late November 1609 and well into
December I did thorough examinations of it though my telescope. I
could easily see that its surface was very irregular with mountains
and valleys like those on Earth. I noticed small dark spots on the
illuminated part of the Moon, with similar lighter spots in the dark
areas. These spots were a puzzle to me because at times
they changed, for example, some spots had a dark part on the same
side toward the Sun, while the opposite side showed up as very
bright. It's as if they resembled some kind of ridge or similar
structure like that. I later thought that these changes were
possibly due to shadows cast as the Sun falls on them.
J:
That was certainly a discovery! So
the telescope was of great benefit when observing the Moon?
Gal: Sì...sì...it opened up a whole new world to me, however,
that said, it was hard at times to use as the small field of view
restricted what I could see fully and clearly of the
Moon as a
whole. This meant I had to move it around several times to get just
one view of an area, and also, the fact that the Moon
appeared moving all the time, it got frustrating to make any decent
drawings. However, I struggled though and learned a lot, and when I
had enough information, I decided to go to print.
J: Ah
yes, your
Sidereus Nuncius
[in Italian] of March 1610.
Gal: Sì...my little book of findings was such a success that
they had to run a second edition in
Frankfurt
before the year was out...molto apprezzato (much appreciated).
J: Did you observe anything else about the Moon afterwards?
Gal: Well, I did want to produce a series of drawings showing
the phases of the Moon and to demonstrate the uneven surface to my
objectors, however, in the end I decided not to, as some feedback
later showed that those in a higher power were convinced the Moon
was so. I did, however, later look more into the libration aspect of
the Moon.
J: Oh...do tell us about that.
Gal: Ah
sì.
Well, during past observations I noticed that on some nights in the
months the face of the Moon did a kind of a...hmmm...how do you say
'rocking'?
J: Oh, you mean 'nod'.
Gal: Esatemente (exactly). This nod effect suggested to me
that parts of the moon's face was visible at certain times in its
orbit, and so I set about in trying to figure it out. I first
measured the changing distance of the large darkish patch on the
right side of the Moon [here, he means Mare Crisium on the East side
-- the name wasn't known back then until Riccioli in 1651 put it
down in print in his Almagestum Novum publication] with the limb,
and then I measured the same on the other side of the Moon at
Grimaldi. I could immediately see that some foreshortening effect
was occurring -- some more so at different times of the moon's path
through my sky, and so I came to the conclusion that the moon's face
was showing me more at these equatorial regions.
J: So if it was
nodding equatorially, then was it also nodding pole-wise as well?
Gal: This I later discovered to be the case, with some of the bottom part
of the Moon [the South Pole region] coming into view more than
expected.
J: Wonderful discoveries indeed.
Gal: Scoperte sono il cibo della vita (discoveries are the
food of life)...[he chuckles a loud laugh].
J: Whatever happened to your telescopes in the end?
Gal: As I improved upon them, I threw away the old ones, or,
misled them...I'm not sure, however, my good ones I gave to others
-- Pierre Gassendi for one, who, as you know, went on to produce
some wonderful images of the Moon in collaboration with Claude
Mellan and Nicolas-Claude Fabri de Peiresc. I did, however, continue
to make better lenses and these, too, I gave away to friends.
J: Who continued the research, no doubt, working on the shoulders of
giants like yourself.
Gal: Ah...modestia vieta (modesty forbids)....[he slightly
shrugs his shoulders and turns his hands palm-wards to heaven].
J: In all this time you were constantly reviewing and updating your
observations and research, which finally led to your publication
'Dialogue on the Two Worlds' published in 1632.
Gal:
Sì...sì!
For a long time I had plans to do some kind of major publication
concerning cosmology. I had originally intended to entitle it 'On
the Ebbing and Flowing of the Sea' on the conviction that the tides
(due to the Moon) provided clear proof of the earth's rotation,
however, in the end I went with the title you see today. You
see...[becoming slightly anxious here] from my findings and from
subsequent encounters with authority, I knew I was on delicate
grounds when it came to expressing a not-so popular belief of a
system other than Aristotle's. So, rather than just let it lie there
in that unpopular state and keep these findings to myself and a
select few friends, I decided that more people should have the right
to read about the changes happening in their universe, which I hoped
would open up new discussions. The possibilities of
what that might lead to was enormous, so I thought, these findings
should be 'out there' for
the betterment of man's progress and his life.
J: If I'm correct, you presented the publication in a manner showing
the advantages of the Copernican cosmology, and of the telescopic
evidence in its favour?
Gal:
Sì!
The 'Dialogue' is a discussion between three friends -- there is Salviati who speaks for me, there is Simplicio who speaks for
Aristotle, and there is Sagredo who is a kind of a middle man who
looks at both our versions. However, I went a bit overboard in
certain aspects with the dialogue in relation to Simplicio through views
of a certain person [he means here the Pope], and this led to
displeasure in certain quarters that led to my house arrest. I had
to abjure my Copernicanism views for the time-being to 'literally' save my life, I
believed. However, looking back at it now, I think I could have
presented those viewpoints in a better manner and, perhaps, things
wouldn't have worked out the way they did...magari?...magari?
(perhaps?...perhaps?).
J: Of
course, I understand that you were already having problems with the
church about certain beliefs on proofs, but this was the final push,
was it not, that really got you into a whole lot of serious trouble
with them? Would you like to add anything there?
Gal: Oh cara (oh dear)...[he sighs]...cosa posso dire (what can
I say)? I think…I had better leave that one for another day, if you
don't mind. Scusa Giovanni...mi scusi.
J:
Not at all...not at all...I well understand!
Gal: [sighs again…vacant look in his eyes].
J:
Okay...well [awkward moment passes...and rather than prolong it any further about this
controversial whole area, I decided it was time to end
the interview], Well...[cough], I think that's it Galileo...is
there anything else you'd like to add or perhaps give advice to our
readers?
Gal: Hmmm...tante, tante cose (so many, many things). I would
suggest to look more into science, learn about the heavens and the
universe...and most important of all, observe the Moon...it's such a
wonderful presence in our lives!
J: On
that note, thank you Galileo...it was such a pleasure to finally
meet you...I've been such a fan for these many years.
Gal: Ah... voi mi pianeggianti (you flatter me). Arrivederci Giovanni....e ringrazio anche voi
(goodbye...and thank you too).
[Author's note: During the interview several other discussions did
take place later...mainly concerning the Church...etc. It was felt
un-necessary, however, to include these comments afterwards as they, unfairly,
may cause undue stress to the maestro -- a nice man...it has to be said.]]
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13 February 2009: Four new research papers reporting on
the latest developments about our Moon have hit print in the latest
issue of Science magazine. The
results and data come from investigations carried out by scientists
working with the Japanese Kaguya spacecraft that launched on the 14
September 2007 last, and which now is orbiting the Moon. The
papers report on various aspects about the moon's crust, gravity
anomalies, with some interesting results from surface maps suggesting
water may not exist on or below the lunar surface because of crustal
rigidity. Access to the papers is through AAAS subscribed membership,
however, for $15 you can
purchase it online. If you need to contact me about this article,
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6 February 2009: The Moon is believed to have formed
from consolidated debris left over from a collision of Earth by a
Mars-sized object. Most of this debris may have developed
globally into an outer, molten magma ocean around denser solid debris,
and this then solidified over a period of time -- giving us the solid
Moon and
surface-crust we see today. The rate of this solidification, which
can be found from examining minerals, like zircon (aka: Apollo samples),
gives an approximate age for the impact and formation of the Moon at
about ~ 4,520 million years ago. However,
new
research, as reported in the latest issue of Nature Geoscience,
suggest that the rate of solidification may have been a lot quicker than
previously believed, and that the above events may have occurred upto
a 100 million years earlier. The researchers involved base their
findings around dating of the oldest zircon found in breccia samples at
an age of 4,417
million years. Their findings suggest that the proposed magma ocean existed for
about the first 100 million years of the moon's history, it solidified a
lot faster, and the crust later formed on top of about 80 to 85% of this
original melt. Existence of the magma ocean is still a controversial
area, and was initially estimated to have solidified over a 215
million-year period. However, if the above research is to be followed,
then evolution of the Earth-Moon system -- from formation to impact
history to present-day -- may have been very different than once thought.
The above research is available through subscription from Nature
Geoscience, or as a once-off purchase for $18.00. If you need to contact
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5 February 2009: Remember that cool-looking NASA moon
rover (SPR -- Small Pressurised Rover) that did a display and dance down
the inaugural route for President Obama (see My News
here)? Well, have a closer look at the
SPR in this ~ 9-minute-long
YouTube video
created by NASA Edge. It includes a spin in the rover across rough
terrain, how the astronauts get in and out of the rover in their suits,
and, there's a bit of fun, too. If you need to contact
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3 February 2009: Right now four radio telescopes across
China are tracking its country's first spacecraft,
Chang'e 1 to the Moon. Precise tracking of the craft is necessary because
instruments onboard taking data of the lunar surface will have to know
exactly where it is in its orbit around the Moon. The data covers a
range of various aspects about the Moon as a whole -- both externally
and internally -- so researchers are always reaching out for anything
that will help them understand that data better. The quality of that
data, however, is about to get an additional boost as a new array of 19
radio telescopes, called the East Asia Very Long Baseline
Interferometer, begin full-scale operations in 2010.
The array will join an already existing
network of radio telescopes spread across China, Japan and Korea; that
together will produce a single radio dish some 6000 kilometres in
diameter -- making it one of the largest radio telescope networks in the
world. Radio interferometry began back in the 1960s which subsequently
developed into Very Long Baseline Interferometry, however, since then
Asia has been home to the largest amount of radio telescopes in the
world (over 20 in Japan, 5 in East Asia including those under
construction in Korea, and 5 in China, as well as several others being
constructed). When operations finally get going, Chang'e 1's state of
health could degrade further over time (it launched in 2007 and
initially was designed for a one-year mission lifetime), so any data
coming from instruments onboard now, and well into 2010, will depend
very much on monitoring precisely its orbit. The craft has
advanced cameras and x-ray spectrometers onboard to obtain
three-dimensional images of the Moon's surface, analyze content and
distribution of useful chemical elements, an map the thickness of the
lunar regolith (the moon’s soil). If you need to contact
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30 January 2009: It has long been understood that the
gravitational influence of the Moon in its orbit around the Earth is
responsible for the bulge in the oceans and subsequent tides (see more on these tides
here). But what about the Moon's influence on
the crust of the Earth -- does it, too, bulge as parts of its surface
comes nearer the Moon? The answer, of course, is yes! The rise is very
imperceptible, however, when the Sun, Earth and the Moon are in the same
alignment -- especially at New Moon and Full Moon times, the combined forces between all three can
cause the earth's crust to rise and fall by upto 20 to 30 centimetres.
This effect is now being looked at by a
Professor at
Harvard University who is investigating how the 'combined influence' and 'crust
tide' can help better understand earthquakes. Earthquakes and their sources are usually worked out from
timings of when they arrived at particular instruments and, particularly, by back-projection of seismic waves (ripples
through the earth's crust) produced. If it is possible to use this
back-projection method to find out more about earthquakes, then
shouldn't it also be of use in finding a correlation between moon
alignments when these quakes occur? By back-projecting the crust
tides and alignments records of the past, and then correlating them to
hundreds of earthquakes that Earth has experienced over time, the
research could lead to a more effective detection and warning system for
future potential threats. But, there is, however, some controversy amongst
scientists that the alignment/earthquake correlation may not be all that
relevant. The two main bodies
concerned -- the Earth and the Moon -- are totally different in size and
mass (the moon's diameter is roughly a quarter that of earth's and has a
mass of ~ 0.012). While it has been shown that the Earth can
cause moonquakes (aka: seismometers left on the Moon during the Apollo
missions), the moon's size and mass may just be too weak to have the
opposite
effect on the Earth. The back-projection method the Harvard
professor is using, however, is relatively new and some say "ground-breaking", and
while it may be a year or so before any completion is finalised,
researchers will have a another tool to better understand the occurrence
of earthquakes around the world. If you need to contact
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29 January 2009: The moon's surface is set to receive
two man-made impactors over the coming months sometime before 2009 ends.
The two impactors -- an upper stage rocket, called Centaur, and a
Shepherding Spacecraft, called the S-S/C -- make up the LCROSS (Lunar CRater
Observation and Sensing Satellite) spacecraft; which is a companion
spacecraft onboard NASA's Lunar
Reconnaissance Orbiter to map the Moon. As part of the 'smashing'
occasion, the
Universities Space Research Association (USRA)
in Alabama, USA, has announced funding of four proposals that will be carried out
to compliment NASA's observing campaign of the Moon as a whole. The
four chosen include: (1) "Accessing LCROSS Ejecta: Water Vapor and Particle Size and
Composition from Keck, Gemini, and the IRFT Telescopes," Southwest
Research Institute, Dr. Eliot Young (Principle Investigator); (2) "LCROSS Lunar Plume Observations with the Apache Point
Observatory," New Mexico State University, Dr. Nancy Chanover
(Principle Investigator); (3) "Multi-spectral Imaging of the LCROSS Impact," Southwest
Research Institute, Dr. Marc Buie (Principle Investigator); and (4) "Searching for Polar Water Ice During the LCROSS Impact Using
the MMT Observatory," University of Arizona, Dr. Faith Vilas
(Principle Investigator). All four were chosen by USRA's call for
proposals back in 2008, which were then rigorously reviewed based around
their scientific contribution towards understanding the moon's surface
and sub-surface. Observations of the event as Centaur impacts first will
be recorded by both the Earth-based observatories and
by LRO itself orbiting overhead, as well as the S/SC which will fly through
the initial plume. Fifteen minutes later, the S/SC will then impact --
probably in a different part of the Moon -- so that the scientists will
get a broader aspect of analyses about the surrounding region and
environment. The most likely areas on the Moon that will
receive the impactors are the pole regions -- the South Pole in
particular -- because water-ice deposits may lie several metres down
underneath the surface in permanently-shadowed craters. Water will play
an important role for a future lunar base (expected to begin around
2020), as colonists will need 'free' resources to grow food, produce
rocket fuel (from the hydrogen in H2O), and build up oxygen reserves for
breathing. If you need to contact
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23 January 2009: As the old saying goes -- "tides wait
for no man". But in Strangford Lough in Northern Ireland, the opposite
will apply when man will wait for tides as a newly-build tidal generator is turned on for the first
time. The generator was installed in the Lough last year by
SeaGen, and is
the world's first commercial-scale turbine capable of producing upto 1.2
megawatts of power -- enough to supply upto a thousand houses with
electricity. The Strangford site is a relatively sheltered location above the waterline, however,
below, its a very different matter as the tides are extremely strong.
Two propellers fixed on either side of a central column on the generator
when submerged will harness the power of these tides -- both
in-tide and out-tide -- and the electricity generated will be sent
off-shore into the general grid. The one big influencing
factor on production of this power is of course due to the tides and the Moon. As the Moon orbits around the Earth once every ~
28 days, its gravitational influence causes oceans on the earth's side
that faces the Moon
to bulge outwards in its direction. As a result, we experience one tide. However, as the Earth, too, is being
pulled in a direction towards the Moon at the same, another bulge of water occurs on
the opposite far side of the Earth, and so another tide follows some 12
hours later as the Earth rotates around on its axis. But the Moon
is not the only body responsible for the tides, as the sun's
gravitational influence on the Earth and the Moon also plays a part. For
example, when the
three are in different alignments in their orbits, the strengths of high
and low tides on the Earth are very much dependant upon the combined gravitational influence
between them. So, when the Sun and the Moon are aligned with
each other in one direction, 'Spring' tides occur that produce very high tides and very
low tides (usually at New or Full moon times). However, when the alignment
doesn't occur (particularly during Quarter moon times), the smaller
gravitational influence between them produces the 'Neap' tides, and
these are neither too high nor too low, but, generally, more
weaker. There is, however, another tide that occurs once every 1.5 years
or so -- called the Proxigean tide. This tide is very rare and only
occurs when the Moon is at its closest to the Earth during time of a New
moon. The advantage in the arrangement between all three bodies, however, is
that we on Earth can use this periodicity to turn tides into
electricity. The occurrence, or strengths, of tides in the
Strangford Lough, therefore, is highly advantages for the community, and
a resource for the island as a whole towards becoming more greener. This
will be the first major test of one of ten
turbines envisioned for the area over time, so all eyes worldwide will
be keeping tabs on the results.
Ireland is currently a leader in this technology, and has one of the best wave-energy
and tidal energy
resources in the world. If you need to contact
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19 January 2009: Sounds like the beginning to a
fairytale, however, as president elect, Barack Obama, tomorrow enters
the annals of history as the USA's 44th President, a lunar rover that
one day may roam around on the moon's surface will also get a look in.
NASA announced the news last Friday saying that the rover will role down
the same inaugural route -- Washington's
Pennsylvania Avenue -- as President Obama in honour of the
momentous occasion. The rover, or, given its official name, the
Lunar Electric
Rover (LER), is just one of many designs the agency came up with
last October as it prepares for return to the Moon in 2020, when astronauts (not Presidents :-)) will
again walk on its surface. The rover can house
upto two astronauts at a time, is equipped with beds and a toilet, and
has space for any equipment or provisions that will be required as they
explore the Moon for upto two weeks at a time. With a 12 wheel
undercarriage, the rover can manoeuvre up and down any serious inclines,
drive forward, sideways, or a combination of both, and can travel upto
500 miles before its Lithium-ion batteries need to be recharged. The
whole cab itself is pressurised inside, so astronauts will be able to
travel along in their shirtsleeves, and when it comes to the exploring
side of things, all they need do is enter into suitports
which allows them step into their spacesuits for easy access. While the
rover is still undergoing tests and is a serious contender
for the future exploration of the Moon, development of its technologies
will have serious kickbacks for
designs of electric motors here on Earth. As the newly-elected
President's keen eye will, undoubtedly, be on the inauguration process
tomorrow, lets hope he gives a small sideways glance to the rover that
is, in all seriousness, a project in the advancement of his country (and
the world). See a
YouTube vid of the rover on the inaugural route. If you need to contact
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13 January 2009: Following hot on the heels of already
receiving $5m for construction of a Lunar Dust Experiment (see 12
January News item below), the University of Colorado at Boulder is set
to receive an
additional $6m for
conducting a variety of astronomical observations from the lunar
surface. Called LUNAR (Lunar University Node for Astrophysical
Research), scientists at the University will develop instruments that
will be sited on the farside of the Moon (the side that we from Earth
cannot observe directly due to orbital mechanics between the Moon and
us), which will look at areas, such as, the early Universe,
the Sun and Einstein's' General Theory of Relativity. The research will
encompass some of the top scientists from around the US, collaboratively
working with institutions like NASA, Harvard, MIT and the University of
California at San Diego. The $11m in total is being funded by NASA's
Lunar Science Institute,
which was created last March
2008 to further the agency's research agenda regarding its future space
exploration goals. The Institute made a total of seven grants nationwide
recently to interdisciplinary science teams all based in the US, and is
being managed
by the NASA Ames Research Center in California. If you need to contact
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12 January 2009: Construction of a high-tech lunar dust
detector that will launch onboard the
LADEE (Lunar Atmosphere and Dust
Environment Explorer) moon mission in 2011/12 got the go-ahead today, as
upto $5m has been granted to build it. The instrument, called LDEX
(Lunar Dust Experiment), will be used to study the tenuous atmosphere of
the Moon; measuring its environment for dust and other elements before
it is perturbed by future human activity. Construction of the instrument
will be done at the Laboratory for
Atmospheric and Space Physics in the University of Colorado at Boulder, and will
later be tested and calibrated for flight by the Colorado Center for
Lunar Dust and Atmospheric Studies; one of seven initial members of
NASA's Lunar Science Institute announced on 9 January (see 9 January News item
below). LADEE is a small cooperative mission
between NASA's Ames Research Center at
Moffett Field, Calif., Goddard Space Flight Center in Greenbelt, Md.,
and Marshall Space Flight Center in Huntsville, Ala. Currently
two instruments -- a neutral mass spectrometer and lunar dust experiment
(LDEX) -- are
envisioned, however, NASA may put on an additional atmospheric
instrument as the mission develops -- depending on the orbital
elements that are now designed to go on it versus the payload mass (the
total must not exceed 20 kg) and mission length. LADEE is expected to
piggyback onboard NASA's
GRAIL (Gravity Recovery And Interior
Laboratory) mission that will use two separate satellites to monitor
gravity anomalies on the lunar surface, and will be placed into a 50 km low orbit
around the Moon for upto four months. After that period, the satellite's
lifetime could be extended depending on its state of health, however,
like all other satellites that have gone to the Moon for brief
lifetimes, NASA could gain additional information by intentionally
crashing it onto the surface. If you need
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9 January 2009: As we prepare to return to the Moon in
the next few decades, good heads with good brains inside them will be
required. In preparation for that daunting road ahead NASA, today, took
a major step today in choosing seven academic and research
teams as initial members of the
Lunar Science Institute.
The institute is responsible for supporting research toward science
programs in exploration of our Solar System, and has for the last decade
been a cornerstone for communications between the top lunar scientists
around the world. Out of the 33 proposals initially entered, the seven,
so far, chosen are: Carle Pieters of Brown University in Providence (The
Moon as Cornerstone to the Terrestrial Planets: The Formative Years);
Ben Bussey, Johns Hopkins University Applied Physics Laboratory in
Laurel (Scientific and Exploration Potential of the Lunar Poles); David
Kring, Lunar and Planetary Institute in Houston (Impact Processes in the
Origin and Evolution of the Moon: New Sample-driven Perspectives);
William Farrell, NASA Goddard Space Flight Center in Greenbelt (Dynamic
Response of the Environment at the Moon); William Bottke, Southwest
Research Institute in Boulder, Colo. (Understanding the Formation and
Bombardment History of the Moon); Jack Burns, University of Colorado in
Boulder (Lunar University Node for Astrophysics Research: Exploring the
Cosmos from the Moon); and Mihaly Horanyi, University of Colorado in
Boulder (NASA Lunar Science Institute: Colorado Center for Lunar Dust
and Atmospheric Studies). The seven were chosen based around a
competitive evaluation process last June, and the members will remain in
their seats on the Institute for the next two years.
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9 January 2009: Okay, you've build, on your own, that
extension you've always wanted, you've cemented bricks together like
there was no tomorrow, and later you've stood back in amazement at your
finished piece of art. Next project, let's build an igloo of bricks!
WHERE? -- on the Moon, of course. That's what a group of students from
the College of Engineering at Virginia
Tech., USA did recently; which won them
the In-Situ Lunar Resource Utilization
materials and construction category award from the Pacific International
Space Center for Exploration Systems (PISCES). While they didn't
actually get to go to the Moon to build it there, they did, however, manage
to create the same foundation for a structure that one day could be used to
construct a future lunar base. They used a composite material of
ceramics and powered aluminium to simulate the lunar soil (the
regolith), and formed solid bricks -- 5.0 inches x 2.5 inches x 1.0 inch
-- after heating them to 2,700 degrees Fahrenheit. The reaction
triggered a self-propagating high-temperature synthesis (SHS) which, in
the end, left them with a brick strong enough
to withstand the harsh environment
of the Moon where gravity is 1/5 that of Earth's and harmful solar
radiation hits the surface head on. The research by the students could someday
have serious applicability on the Moon, where the regolith soil could
substitute for the mixture they created. All that is required are
some enthusiastic brickies looking to build that next big project. To
apply for the positions, please upload your experience with construction
of extensions, sheds, dog houses etc., to.....?
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5 January 2009:
Chandrayaan-1 - India's
first spacecraft that launched to the Moon last October - is working
so well its space agency may extend operations beyond its
expected two-year lifetime. Accuracy in putting the craft into a
precise 100km altitude orbit around the Moon in November has
saved so much fuel, engineers now see the mission work well into
2011. Every now and then the craft has to expend fuel to keep
its orbital manoeuvre correct around the Moon, however, as very
little is used during this process, the 183 kg of fuel currently
onboard is set to last for a fair few many of these adjustments. Chandrayaan-1's overall objective is to carry out high
resolution mapping of the lunar surface and take distribution
readings of various chemical elements and minerals in its rockmass. Already, unprecedented amounts of data about the
surface has been returned to ISRO through its deep space network
(two dish antennas 32 metres and 18 metres in diameter
respectively) installed at Byalu. Over the coming months,
engineers will prepare for launch of an impactor payload onboard that
will crash on to the lunar surface, and, if it survives, it will carry
out analyses of surface materials and rocks. Chandrayaan-1 is just the
first step in India's plans to go to the Moon. Its success could lead to
future ambitious plans of launching Chandryaan-2 in 2012 (not later than
2016) that will put a rover down on the lunar surface, and
Chandrayaaan-3 which will put a man into orbit around the Moon by 2020.
In two weeks time, several of the leading international scientists who
have instruments onboard Chandrayan-1 will meet in Bangalore to discuss
the data they have gathered already, and from this meeting more should
be revealed about the craft's ambitious plans and lifetime.
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