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Dr.
David Latham of the Harvard-Smithsonian Center for Astrophysics
in Cambridge, MA writes:
"I
am an observational astronomer. I like telescopes and
tall mountains and staying up all night and seeing the
sun rise just before I go to bed. When I was younger
I built instruments, but now I am happy to let others
do that job. I have worked on observational cosmology,
mapping out the distances to nearby galaxies, and I
have studied the structure and evolution of our own
Milky Way galaxy. Most of my recent work has focussed
on stars and their companions, especially low-mass companions
such as planets and brown dwarfs. I have participated
in some of the exciting discoveries involving extrasolar
planets: the first planet candidate (orbiting HD 114762)
found with Doppler shifts in 1988, and the first planet
to transit its parent star (orbiting HD 209458) found
in 2000. Astronomy has been very, very good to me."
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For
links to this scientist's home page and other related infomation
please see our resources
page.
Latham
responds :
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1.03.01
Miguel asked:
I have a very simple question. Aren't we thinking like
people thought in the past? After all, we used to think
that Europe was the only place in the Galaxy, then we
found America. So now we think that there is life in
this world only. Aren't we making the same mistake?
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Latham's
response:
We
do not yet have any convincing scientific evidence that
there is (or was) life elsewhere in the universe. But,
like you, I would be amazed if it turns out that we
are alone. This is one of the really big questions,
and we are now in an era where we are beginning to have
the technological capability to look for some answers.
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1.03.01
Juwon Kwon asked:
I wanted to know if do you think that the planets and
their civilizations are far more advanced than we are?
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Latham's
response:
We
have no evidence that there is life in any of the planetary
systems found so far. If intelligent life has arisen
often, then inevitably one of two things must be true:
there are many technical civilizations out there now,
and the vast majority must have attained our level of
technology a long time ago, or else there are very few
out there now because technical civilizations destroy
themselves before or soon after they reach our level.
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1.03.01
Bob Cicalo asked:
Can black holes be detected with the same wobble measurement
techniques mentioned in the show? If so, is there a
mathematical formula for this?
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Latham's
response:
Yes,
black holes may not radiate any light that we can detect,
but they still have gravitational pull. In fact, this
is one of the main ways for detecting black holes, by
seeing how hard they pull on nearby stars or gas. Newton's
theory of gravitation is good enough for describing
the motions that result. One formula that is especially
useful is Newton's revised version of Kepler's third
law, which gives the relationship between the period
of the orbit, the size of the orbit, and the masses
involved. You should be able to find this formula in
an astronomy text book.
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1.03.01
Russell M Mott asked:
Could the Earth's magnetic field be generated from salt
water -a conductor in motion. Could that be why Earth
has a magnetic field and Mars does not?
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Latham's
response:
I'm
not a geologist, but my understanding is that convective
motions in the molten inner regions of the earth generate
the magnetic field. Mars does not have a molten interior,
and thus can not generate a significant magnetic field.
The oceans may seem deep, but compared to the radius
of the earth they are a very thin layer. I bet it would
be hard to generate a large-scale magnetic field with
such a thin surface layer.
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1.03.01
Fred Metterhausen asked:
On the show they said that the planet found orbiting
HD 209458 was much larger, therefore less dense then
what was originally calculated. I was just wondering
if it was considered that the gravitational field of
the planet might make the planet divert more of HD 209458
light then the planet alone, therefor making the planet
much smaller?
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Latham's
response:
The
giant planet orbiting HD 209458 is indeed larger and
less dense than Jupiter. Astronomers who make theoretical
models for giant planets say they have an explanation
for this. The planet is so much closer to its parent
star that it has not had a chance to cool off, so it
has stayed puffed up. In fact, if the planet formed
out in the distant icy regions around its star, like
Jupiter, and then migrated into its present orbit, it
had to do so in the first few million year after it
formed, otherwise it would have cooled off too much.
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