In article , Don Pearce
wrote:
The variables are part of the problem, but it is also quite an
ill-conditioned equation.
As for the variables themselves, it looks like planets are far more
ubiquitous than it allowed for. It seems that every star that can be
imaged has planets. I suspect that is going to be the case generally -
if there is enough "stuff" to make a star, there will be enough left
over to form planets as well.
Yes, now we've started to be able to detect them, that particular factor
can be assumed to approach unity. But in the past - although some argued
planets would be the norm (in single-star systems) - it was just as easy to
argue that the startup of the star would tend to remove and/or eat the
remaining material.
What has been more unexpected is planets in binary+ systems.
FWIW I used to work on instrumentations for 'Far Infra Red' (say 100 micron
to 3 mm wavelength) astronomers many years ago. Back then no-one had
detected anything in the FIR sky beyond the Sun, Moon, main solar planets
and *barely* the crab nebula. At the time it was hard go get support or
telescope time because other astronomers said there was no reason to expect
the FIR would reveal anything.
How wrong they were. A decade or so later the FIR/mm-wave people were block
booking time on the larger telescopes and publishing a stream of reports on
detecting new things. Interesting time... :-)
Jim
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