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DISTANT DISCOVERIES
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THE "EYEBALL"
NEBULA
Astronomers
using the Hubble Space Telescope recently released a striking new image
of a planetary nebula, or dying star, called NGC 6751 in the constellation
Aquila. See the AstroNews website for this spectacular photo.
Resembling a glowing eye, the nebula was found to be 6,500 light-years
away from Earth in a far region of the Milky Way galaxy. Its discovery
is helping astronomers map stars in our home galaxy and understand the
eventual fate of our own sun.
Planetary nebulas are big, bright clouds of gas and dust that puff out
from an exploding, dying sun. They are so named not because they have anything
to do with planets, but because of their round shape.
Astronomers are learning a great deal about planetary nebulas at the
edge of our galaxy and beyond. But interestingly, they lack some important
data about nebulas in our own Milky Way.
NGC 6751 is apparently an odd planetary nebula because it resembles
another type of solar explosion called a supernova. It looks like somebody
ripped it apart into little pieces. Experts aren’t sure why exactly this
particular planetary nebula looks so odd compared to other planetary nebulas.
Astronomers expect that our own sun will someday end up as a similar
planetary nebula after it dies. However, because our sun has large gaseous
planets like Jupiter and Saturn surrounding it, it might look more like
an elliptical egg than a circular eye when it does explode.
SPACECRAFT
BUMPS COMET TAIL
Sometimes in science, little surprises can have great impacts. Just ask
the astronomers who stumbled across a small blip in the data collected
from the European Space Agency/NASA ULYSSES spacecraft when it passed through
supposedly empty space. The blip, it turns out, was the signature from
an INVISIBLE COMET TAIL, a comet tail that was more than 310.7 million
miles (500 million kilometers) long -- almost double the longest comet
tail previously known to exist.
A comet passed through the exact position that Ulysses -- a probe orbiting
the sun that studies the solar wind -- occupied. The comet in question
was the HYAKUTAKE comet, which was visible to the naked eye from Earth
in 1996.
Comets are small icy objects that formed at the dawn of the solar system,
some 4.5 billion years ago. As a comet nears the sun, its icy core boils
off, forming a cloud of dust and gas called a head, or coma. Comets become
visible when sunlight reflects off this cloud. As the comet gets closer
to the sun, more gas is produced. The gas and dust is pushed away by charged
particles known as the solar wind, forming two tails. Dust particles form
a yellowish tail, and charged gas makes a bluish ion tail. A comet's tails
always point away from the sun.
Clues about Ulysses’ contact with Comet Hyakutake’s tail began to appear
when a team of scientists who were studying charged particles emanating
from the sun noticed something odd in their data.
The collision will help comet experts understand the life cycle and
fate of comets, which many think of as prehistoric relics from the earliest
days of the solar system. In particular, the discovery of such a long comet
tail invites astronomers to believe that they may find and study past comets
whose tails are still intact.
Today, Comet Hyakutake is far, far away from the Earth: 1.2 billion
miles (2 billion kilometers), to be exact. But astronomers speculate that
there will always be new comets flying in the vicinity of our home planet.
As a result, a cometary impact on Earth is always a possibility and concern.
However, scientists now say they may be able to use the results from the
Ulysses-Hyakutake finding to study the probability of comets hitting the
Earth.
[Source: space.com . 04.07.00]
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FAR OUT FACT
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ESREVER NI EMIT
In a distant galaxy, a star UNEXPLODES.
Just moments ago a shell of tortured matter was flying together at 30
000 kilometres a second. Now it has become a star, and the last shreds
of glowing debris are being sucked in. With the explosion undone, the star
begins the long journey back to the time when it will be UNBORN into the
gas and dust of an interstellar cloud.
Is someone running the film backwards for comic effect? Not necessarily.
In 1999, Lawrence SCHULMAN of Clarkson University in Potsdam, New York
dropped a bombshell. He showed that regions where TIME FLOWS in the NORMAL
direction can COEXIST with regions where it FLOWS BACKWARDS!! There could
be places, perhaps even within our Galaxy, where stars unexplode, eggs
unbreak and living things grow younger with every second.
To understand how time could run backwards, you need to understand why
it has a preferred direction at all. Physics say particles of matter don't
care what direction time runs in: any interaction between two particles
could happen just as easily in reverse. (Some nuclear interactions do show
a small bias, but no one has found a way to turn this into an arrow of
time.)
But when you have a lot of particles instead of just two, things change.
Messy, disordered states tend to develop from tidier ones. This tendency
is called the thermodynamic ARROW OF TIME. Physicists say that ENTROPY
- a measure of disorder - always increases. "It's easy to break an egg,
difficult or impossible to put the pieces back together," says Schulman.
Say the air in a large room is confined in a 1-metre cube in one corner,
then released. It is perfectly possible that, after five minutes, the air
molecules will all be back in the same 1-metre cube. Perfectly possible
but hugely IMPROBABLE, because there are far more ways to arrange the individual
molecules when they are spread out than when they are confined. In fact,
the most disordered state-in which the air molecules are spread more or
less evenly throughout the room-can be achieved in far more ways than any
other state. "This is the second law of thermodynamics," says Schulman,
"which seals the fate of Humpty Dumpty."
However, argues Schulman, a reverse arrow is perfectly possible: "It's
all down to the 'boundary conditions'-the external constraints imposed
on the system." In the room, the air has to be in the 1-metre cube only
at the start of the five-minute period. There is no constraint on it at
the end of the five minutes-the system can find its own final state.
But say a final condition is imposed. After five minutes, the air molecules
have to be back in the 1-metre cube. On Earth, this is clearly an artificial
situation. But for Schulman, it is perfectly legitimate to consider such
a state of affairs. "There is no reason in principle why the Universe might
not have a future boundary condition imposed on it," he says.
The future condition would constrain the molecules to follow only a
tiny subset of trajectories, ending up in the 1-metre cube. From our point
of view, time would be running backwards.
But there's an objection to having forward and backward time regions
in the same universe. Surely the arrow of a reverse-time region would be
wiped out by the slightest interaction with a normal-time region, leaving
a completely disordered system with no arrow at all?
Imagine a GAME OF POOL in which the triangle of balls is struck by the
cue ball and scattered around the table. Now imagine the reverse-time scenario.
For the balls to follow the precise trajectories necessary to finish in
a triangle will take a MONUMENTAL amount of coordination. The slightest
disturbance will spoil it. Any interaction with a region with normal time-for
instance, the smallest cry of amazement from someone watching-could vibrate
the air, nudge the balls and wreck everything. So the backward arrow of
a reverse-time region would be instantly destroyed by any interaction with
a normal-time region.
Schulman sees a flaw in this idea. The two systems are on an EQUAL FOOTING,
so the reverse-time region is AS LIKELY to destroy the arrow of the normal-time
region as vice versa. "All we can say is that if the two regions interact
their arrows will either both be destroyed or both survive."
Most physicists would have put good money on the former possibility.
But Schulman's startling conclusion is that as long as the interaction
between the two regions is weak, both arrows will survive. He bases this
claim on a simple computer model that allows him to set up weakly interacting
systems with opposite arrows of time and see what happens.
HERE'S HOW IT WORKS. Take a square 1 unit on each side, and add a particle
with coordinates x and y. Move the particle by repeatedly replacing x with
x + y and y with x + 2y, and discarding any integer parts of the results
(so x and y stay in the range from 0 to 1). The particle will flit about
the square chaotically. "This mimics the essential BEHAVIOR OF A GAS PARTICLE,
while being a lot simpler than reality," according to Schulman.
To set up two gases with opposite arrows of time, Schulman imposes appropriate
boundary conditions. In one model gas, the particles start in one corner
of the square and spread out until they are completely disordered. They
have a "normal" arrow of time (that is, the same arrow as us). In the other,
Schulman imposes the final condition that after, say 20 moves, corresponding
to 20 time steps, the particles are all in the corner of the square. This
system has a backward arrow of time. Call the normal-time region ALICE
and the reverse-time region BOB.
The next step is to LET ALICE AND BOB INTERACT. Schulman tweaks the
coordinates of each normal-time particle according to the coordinates of
the reverse-time test particle, and vice versa.
When Schulman lets both systems run, he finds that neither arrow of
time is destroyed by the other. "All that happens is that Bob adds a bit
of noise to Alice and Alice adds a bit of noise to Bob," says Schulman.
The two arrows of time are remarkably robust.
"I had no idea when I started my work that this would be the outcome,"
he says. "The result surprised me as much anyone else." But this surprise,
he adds, comes from a prejudice against future boundary conditions. Once
you are used to the idea of matter having some MEMORY of what we call its
future, it ceases to surprise. From our point of view, the memory of future
organisation drags any reverse time region in the direction of increasing
order, despite any small disturbances from our own "normal" region.
The paper has created quite a stir. "This is very cool stuff indeed,"
says Max Tegmark of the University of Pennsylvania. At the Technion-Israel
Institute of Technology, where Sculman began this work, Amos Ori agrees.
"Schulman has shown that the consistency of a model with two simultaneous
time arrows can be explored by relatively simple means. This is a very
important observation."
And he has some equivocal support from David Pegg of Griffith University
in Brisbane. "I see no obvious flaw in the calculations Schulman has done.
He makes his case quite well and I am willing to accept it, at least until
convinced otherwise."
Other physicists don't believe that Schulman's computer model is relevant
to the real world. According to Paul Davies of the University of Adelaide,
a real physical system with a backward arrow would be so fantastically
SENSITIVE to an outside influence that it would be easily destroyed. "Imagine
a box of gas with molecular velocities reversed to bring about an ordered
state," he says. "The gravity of a single electron at the edge of the observable
Universe is enough to throw out the motion of a given molecule by 90 degrees
after only 20 or so intermolecular collisions. That's pretty sensitive."
CROSSING THE DIVIDE
Surprisingly, Schulman does not dispute Davies' point. "He's absolutely
right. But the very set-up of his thought experiment, with initial conditions
only, precludes an opposite-directed arrow," he says. "My result applies
when boundary conditions are imposed at two separate times."
Some might attack the realism of Schulman's interaction, which he admits
is an abstract mathematical one and not related to a real physical force
such as gravity. "Nevertheless, I maintain that the interaction is adequate
for treating the conceptual issue of the effects of future-conditioning,"
he says.
So could we actually see reverse-time beings if they exist, and maybe
even wave to them? Remarkably, Schulman says yes. Using a theory originally
developed by Richard FEYNMAN and John WHEELER, which treats light waves
travelling in both time directions on an equal footing, he shows that forward
and reverse regions could communicate by light signals.
But COMMUNICATING with the other side has its DANGERS. If normal-time
Alice were to see rain pouring out through reverse-time Bob's window, she
could wait until before the rain started and shout to Bob to close his
window. "So did Bob's floor get wet or not?" says Schulman.
Perhaps something intermediate happens which smears out the paradox.
"Alice sees the window open, shouts to Bob but the message gets blurred
and Bob doesn't close the window," says Schulman.
And there's another, more disturbing possibility. "If you impose initial
and final boundary conditions, it may turn out that the events described
simply can't happen," he says. "In mathematical terms, they are simply
not a solution." In other words, we might just be fated not to cause any
paradoxes.
So, how would a reverse-time region arise? Schulman says such regions
may exist for the same inexplicable reason that regions of normal time
exist. But there is one more concrete possibility: perhaps we live in a
Universe whose expansion from a BIG BANG will one day be reversed into
a contraction down to a "BIG CRUNCH", a sort of mirror-image of the big
bang in which the Universe was born 13 billion years ago. Although the
latest cosmological evidence is AGAINST this, the question isn't settled.
In 1958, Thomas Gold of Cornell University argued that the thermodynamic
arrow of time would reverse during the contraction phase, creating order
out of chaos. Gold's reasoning turned out to be flawed, but in the 1970s,
Schulman used his own model to show that the conclusions were right. As
the big bang and big crunch are both highly ordered (all the matter is
in a small volume), thermodynamic arrows of time should point away from
both ends. The arrow of time depends on the expansion or contraction of
the Universe. "Coffee cools because the quasar 3C 273 grows ever more distant,"
says Schulman.
Of course, if you were alive during a cosmic contraction phase you would
see nothing untoward-you'd have the same arrow as most of the matter in
the Universe, and it would look like expansion (see Diagram). Stepping
outside the Universe, the situation appears perfectly symmetrical; it makes
just as much sense to call either end the big bang or the big crunch.
A bizarre consequence of Schulman's theory is that some reverse-time
regions from a future contracting phase of the Universe could have survived
until today-and could be only a few tens of light years away. "Some bits
of the Universe might have reverse arrows while other bits with forward
arrows might survive well into the contraction phase."
As the "turnaround" time when the Universe's expansion turns into contraction
could be many hundreds of billions of years away, any stars would have
burnt out. Unfortunately, there would be little prospect of seeing stellar
unexplosions or backwards people among such cold stuff. "We would still
feel their gravity, though," says Schulman. "Such reverse-time matter would
have all the attributes of the invisible, or 'dark', matter thought to
make up most of the mass of our Universe."
COLLIDING MATTER
Another possibility is that in the 13 billion years since the big bang
most of the Universe's matter has collided with reverse-time matter from
the future. The result of such collisions would be matter in "equilibrium"
with no time direction. "Once again, it would appear exactly like dark
matter," says Schulman. Other physicists are sceptical. "I doubt that this
has anything to do with the dark matter problem," says Tegmark.
So what would it be like in a region that is changing its time direction?
Would exploding things suddenly start unexploding? And what would happen
to the minds of beings around at the time? Sadly, it would be rather undramatic.
For a particular area to change its arrow, it would first have to go through
a period of maximum disorder where there could be no stars or explosions
or structured, working minds. But if you survived for long enough, you
might be able to watch the Universe around you starting to contract, and
most of its matter going into reverse.
If all this is getting a bit difficult to stomach, there is A WAY TO
TEST IT-even if we can't spy on a nearby backwards planet. "Things happening
today could be influenced by boundary conditions at the end of the Universe,"
says Schulman. What he has in mind are ultra-slow processes.
In the 1970s, John Wheeler of Princeton University suggested observing
the decays of atomic nuclei with ultra-long half-lives, perhaps many tens
of billions of years. The suggestion was that the normal exponential decay
would be modified by exponential "undecay" and that this might actually
be observable in a sample of a few kilograms in the laboratory. Possible
candidates are rhenium-187 and samarium-147, which have half-lives of about
100 billion years.
Unfortunately, Wheeler was too optimistic. For an experiment of a sensible
duration, a few years, say, you'd need roughly the total supply of these
isotopes in the Universe to see deviations from exponential decay.
"A far better bet is galaxy clustering," says Schulman. He believes
that the way galaxies cluster together could be affected by a future contraction
phase. Unfortunately, he has not yet worked out what form this effect might
take.
But over the past few years, a small group of of physicists have been
claiming that the Universe has an inexplicable FRACTAL structure. Most
cosmologists disagree, partly because they have no way to explain such
a bizarre pattern. But say there is something in it. Could it perhaps be
a MEMORY OF THE FUTURE?
LAST PLUG
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