Billions of Habitable Planets?
cbv writes: "MSNBC has an interesting article about new calculations by Charly Lineweaver and Daniel Grether, both of the University of New South Wales in Australia, which provides an interesting answer to the question on how many potentially habitable planets exist in our galaxy."
Because by the time we can find another one that is, this one won't be.
--Blair
"Keeping up with the Gbrtlrxzes."
N = R* × fp × ne × fl × fi × fc × L
Where,
N = The number of communicative civilizations
The number of civilizations in the Milky Way Galaxy whose radio emissions are detectable.
R* = The rate of formation of suitable stars
The rate of formation of stars with a large enough "habitable zone" and long enough lifetime to be suitable for the development of intelligent life.
fp = The fraction of those stars with planets
The fraction of Sun-like stars with planets is currently unknown, but evidence indicates that planetary systems may be common for stars like the Sun. more info
ne = The number of "earths" per planetary system
All stars have a habitable zone where a planet would be able to maintain a temperature that would allow liquid water. A planet in the habitable zone could have the basic conditions for life as we know it. more info
fl = The fraction of those planets where life develops
Although a planet orbits in the habitable zone of a suitable star, other factors are necessary for life to arise. Thus, only a fraction of suitable planets will actually develop life.
fi = The fraction life sites where intelligence develops
Life on Earth began over 3.5 billion years ago. Intelligence took a long time to develop. On other life-bearing planets it may happen faster, it may take longer, or it may not develop at all. For more information, please visit Dr. William Calvin's "The Drake Equation's fi"
fc = The fraction of planets where technology develops
The fraction of planets with intelligent life that develop technological civilizations, i.e., technology that releases detectable signs of their existence into space.
L = The "Lifetime" of communicating civilizations
The length of time such civilizations release detectable signals into space.
I think only telelphone sanitizers, hairdressers and middle management will get to go, if I remember correctly.
As the article says, Jupiter-like planets can act like a debris-magnet to protect Earth-like planets from comets, asteroids, and the various other junk floating around solar systems. Their immense gravity can either force and object out of the solar system entirely or force it to collide with the large gas giant. (An impact which would leave Earth near-barran for centuries is barely felt on Jupiter gas giant.)
The moons of the Jupiter-like planet offer another possibility for life. Like Europa, gravitational stresses from orbiting such a large planet can cause heat to warm up a normally frozen world. This heat might help melt ice into water (as is thought to be on Europa under the ice shell). And where there's water, life might not be far behind.
Now this isn't to say that life=intelligence. We might be talking about the ET equivalent of bacteria, here. Still, the discovery of ET-bacteria would be a huge matter.
My sci-fi novel, Ghost Thief, is now available from Amazon.com.
Manned interstellar spaceflight would require:
Some have observed that the level of committment this would require of humanity would be like nothing ever seen before, and which would require devotion that has historically only been commanded by religious quests.
Toronto-area transit rider? Rate your ride.
I don't care how many worlds there are in the Galaxy. I'm NOT going to wear a red shirt when I beam down to one of them.
"Giving money and power to governments is like giving whiskey and car keys to teenage boys." - P.J. O'Rourke
No matter how badly we mistreat this world, it won't be worse than anything we find out there, unless one happens to have extremely Earth-like life on it already, the kind of place they find all the time on Star Trek, with lumpy-foreheaded humans and grass and spruce trees (foam boulders optional).
By "habitable" they mean planets like Mars and Venus. Places you can live on in extremely well made air-tight shelters, and maybe eventually terraform.
We could have a sustained nuclear war (presumably sustained from off-planet), stripping the planet of sophisticated lifeforms and blowing off half of its atmosphere, and it would still be a nicer place to live than anywhere else in our solar system or anything we're likely to find orbiting another star.
In terms of human habitability, we're taking pretty good care of this one. Wiping out the wilds is sad, but a choice of farms or forests is easy for hungry people. Where it appears unnecessary, done too casually for convenience rather than survival, that is just staying ahead of what the population growth will demand in a generation or two. The pollution looks bad, but it's a feature of short-lived transitional technology, and will tail off before intolerable damage is done.
On the whole, human effort is greatly increasing human habitability of Earth, not decreasing it. The pristine, wild world of a hundred centuries ago couldn't support half a billion humans, while today it supports well over 6 billion, and the way is being made for 10. Even one century ago, it probably couldn't have sustained half our current population. Things probably won't get tight here on Earth's surface until at least 100 billion, by which time we'll be seriously working on these other places to live. As it is, we haven't seriously dented the resources of our planet, just dug around a little at the choice bits on the surface.
Can anyone tell me the difference between a 'metric buttload' and an 'Imperial buttload'? Thanks.
I believe the imperial buttload is based on the size of Hing Henry V's rear end. Quite large, it was.
While the metric buttload is smaller, it scales nicely. For example, there are 10 metric buttloads in a metric shitload.
QED
Anybody want a peanut?
3. Such civilizations do not last a long time, and blow themselves up or otherwise fall apart pretty quickly
Or alternatively, civilizations progress at a geometric rate, transcending themselves in a few short generations, so that by the time intersteller travel becomes feasable they have lost interest and moved on to more compelling possibilities (perhaps departing this frame of reference entirely).
Once one hypothesizes a civilization significantly more advanced than our own it becomes difficult to even imagine the technologies they may have, much less what interests they would find compelling, or what goals they might set for themselves. For all we know they are all around us, unrecognized because they operate at levels as far beyond us as we are beyond the simple microbe.
The Future of Human Evolution: Autonomy