Destination Mars
by John Bell
(Reported by Jim Walker)
By way
of introduction, John noted that the British now have an unmanned space
probe on its way to Mars. The probe is appropriately named the Beagle,
after the ship that carried Darwin’s expedition around the world.
John also
mentioned Project Orion, involving atomic scientists who had worked on
the a-bomb program during World War II. The Orion rocket was to be
nuclear powered. It would have weighed 4,000 tons and would
have carried a payload of 1,000 tons to Mars. But the project was
soon abandoned because of concerns about safety. However, NASA is
now interested in Orion as a possible means of diverting an asteroid headed
for the earth.
The video
Destination Mars considered a manned mission that would travel 250 million
miles over a period of 2 1/2 years. Mars is only about 1/3 the size
of Earth, but there are mountains 3 times the size of Everest. Mars
gravity is only 1/2 that of the Earth. We already know something
about the geology of Mars because meteorites blasted off its surface by
impacts have been found on the earth.
Mars has
caught the world’s imagination for many years, due in no small part to
Percival Lowell’s belief that the planet was criss-crossed by a network
of canals to bring water from the polar snowcaps to the desiccated equatorial
regions. But Lowell’s canals have long since failed to appear in
our many close-up pictures of the planet. There are, however, many
photographs of channels that give strong evidence of flowing water, perhaps
long in the past. Indeed, if all the ice on Mars melted, the planet
would be covered by 600 feet of water (the earth, however, would be under
6,000 feet if all our water melted).
Former
Astronauts Eugene Cernan and Buzz Aldrin discussed plans for a manned expedition
to Mars. One of the most difficult problems involves the huge weight
of the rocket fuel to be consumed on a trip to Mars and back. One
possible solution is to send rockets to Mars that would manufacture the
fuel needed for the return trip, producing methane and extracting oxygen
from the abundant carbon dioxide in the Martian atmosphere. Because
of safety concerns, nuclear rockets have been essentially ruled out.
(See Sky Watch for more on Mars.)
- End of Minutes -
Respectfully submitted,
Jim Walker, Secretary
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The Perseid Meteors
by C. L. Hall
(Edited by permission from North American Meteor Network.)
The Perseids
are perhaps the best known meteor shower to serious observers and the general
populace alike. Every year we await its arrival, its distinctive
meteors, and the nice warm nights of summer.
This famous
shower has been observed for about 2000 years, with the first known information
on these meteors coming from the far east. In early Europe, the Perseids
came to be known as the Tears of St. Lawrence. In an article by Mark
Littmann called 'The Discovery of the Perseid Meteors' on the Sky and Telescope
website, Littmann writes: "Saint Lawrence was tortured and killed in Rome
on August 10, 258 during the reign of the anti-Christian emperor Valerian.
. . Citing Quetelet, 'a superstition has 'for ages' existed among
the Catholics of some parts of England and Germany that the burning tears
of St. Lawrence are seen in the sky on the night of the 10th of August,
this day being the anniversary of his martyrdom.' "
Legends
abound about Perseus. In ancient Greek mythology, he was a hero -
the son of Zeus. On one quest, he took off to slay the famed Medusa,
a beautiful mortal lady who had been unceremoniously turned into a fearsome
Gorgon by the jealous goddess Athena. Medusa's beautiful hair became
a squirming mass of snakes - and her gaze deadly. Perseus travelled
with the help of winged sandals from Hermes, the messenger god; a sword
of diamond from Hephaestus, the god of fire and the forge; and a
magical helmet to make him invisible, from Hades, god of the underworld.
He slew Medusa without looking at her by using her reflection in his shield.
The blood of Medusa fell to earth and created the great winged horse Pegasus.
On his
way home, Perseus rescued the princess Andromeda, daughter of King Cepheus,
who was chained to a rock as a sacrifice to the sea monster Cetus because
of the vainful boasting of her mother, Queen Cassiopeia. Perseus
rescued the fair maiden and married her. And now, in our constellations,
we have all the players in the legend: Perseus, Pegasus, Andromeda, Cepheus,
Cassiopeia, and Cetus - and even the infamous Medusa, immortalized as the
'Demon Star' in the constellation of Perseus.
The parent
comet of the Perseid meteors, 109/P Swift-Tuttle, was discovered in July
of 1862 by both Lewis Swift of Marathon, New York, and Horace Tuttle of
Harvard Observatory, Massachusetts. It was about magnitude 7.5 at
discovery and brightened to about magnitude 2 by early September, which
is about the same brightness as the stars in the Big Dipper. It sported
a tail of between 25 and 30 degrees long, and was quite impressive.
By length comparison, the pointer stars of the Big Dipper are about 5 degrees
apart. The comet comes around to our part of the solar system about every
120 years and was seen most recently in the mid 1990's. In November of
1992, it brightened to about magnitude 5.0.
Because
the orbit of the Perseid meteoroid particles is tilted so much in relation
to the plane of our own solar system, the Perseids have stayed fairly similar
in characteristics since ancient times, and have not been changed much
by the influence of our large planets such as Jupiter. It was Schiaparelli,
the astronomer most noted for observing the so-called 'canali' on Mars,
who discovered that the Perseid meteors were related to Comet 1862 III,
also known as 109/P Swift-Tuttle. This was the first proven association
between a comet and a meteor shower.
The magnitude
or brightness of the meteors themselves is interesting as well. Studies
by Hruska and Ceplecha in the 1950's indicated that the Perseids generally
seem to be brighter before the date of maximum activity than afterwards,
but that some periods of brighter or fainter meteors do occur. This tends
to indicate some filamentary structure in the Perseid meteoroid stream.
In other words, we encounter clumps of brighter or fainter meteors
as the earth passes through different layers of debris shed long-ago by
Comet Swift-Tuttle. These are fast meteors, at about 59 km per second.
The Perseids
(PER) can be seen from about July 17th until about August 24th, with the
main peak time occurring on the 13th of August at 4h 40m UT (Universal
Time). ZHR rates at maximum reach about 110 meteors per hour.
ZHR stands for Zenithal Hourly Rate, and is the average number of meteors
that observers would expect to see if they were out under a dark country
sky, and if the radiant, the area in the sky where the meteors seem to
come from, were directly overhead.
Will we
see this many meteors for this Perseid display? Looking at the calendar,
the full moon in August occurs on the 12th, at 4h 48m UT. This will
wash out the fainter meteors. However, the good news is that the
Perseids are noted for lots of bright meteors, and these will still be
visible.
How can
you see more meteors, in spite of the full moon this year? It is
still worthwhile getting away from city lights. Face away from the
moon when observing - put it behind you, or at the very least, to your
side. Do not stare at it, or it will destroy whatever dark adaptation
you have. Or try blocking the moon with a tree, or even a dark umbrella
that you reposition during the night. Every little bit of decreased
light or glare will increase your meteor perception.
The Perseids
are probably the best shower of the year to try photographing. It's
warm, and the number of bright meteors is high. Use a camera with
a time exposure, and a normal lens (not a telephoto). Set the lens
wide open (or perhaps 1 stop down), and set the focus on infinity.
Put the camera on a tripod, and use a cable release to keep the lens open.
You won't want fast film - or it will 'fog' over quickly with the bright
moon. Use a slower film, and keep your exposures fairly short - you
might try 5 minute shots, for example. It is always wise to take
a variety of exposures, as some will turn out better than others.
A map
showing the radiant of the Perseid shower, and its movement across the
sky throughout the month, can be found on the website of the IMO, the International
Meteor Organization, at http://www.imo.net/calendar/cal02.html#Perseids
Is there
just one peak time? In fact, there are several. The predicted
times of high Perseid activity are as follows, according to the IMO's 2003
Meteor Shower Calendar: Aug 13, 4h 40m UT - the main peak;
Aug 13, about 2h 40m UT - possible maxima; Aug 13, about 14h 40m
UT - possible maxima. For Central Daylight Times, subtract 5 hours
from the above. Good hunting! |